From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #27
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
Errors-To: owner-wien-digest@theochem.tuwien.ac.at
Precedence: bulk


wien-digest         Thursday, July 18 2002         Volume 2002 : Number 027




----------------------------------------------------------------------

Date: Thu, 11 Jul 2002 12:19:24 +0800
From: "wan liu" <wien97wan@hotmail.com>
Subject: Re: [WIEN]: About Total Energy

====
"wan liu" <wien97wan@hotmail.com>
submitted the following contribution:
====

Dear Prof. Blaha

Thank you.

Best Wish

Liu


>From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: <wien@zeus.theochem.tuwien.ac.at>
>Subject: Re: [WIEN]: About Total Energy
>Date: Mon, 8 Jul 2002 11:55:45 +0200 (MEST)
>
>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
> > I want to know whether or not I can find the values of BAND ENERGY, 
CORE
> > ENERGY, KINETIC ENERGY, and COULOMB ENERGY in WIEN.
>
>Kinetic and coulomb energy is not seperated in WIEN:
>
>:DEN  : DENSITY INTEGRALS =            -690.575068   (Ry)
>Contains the contribution of all integrals rho * (V + E_xc)
>
>:SUM  : SUM OF EIGENVALUES =             -9.384373
>(contains sum of band energies)
>
>         1.ATOM      Ti                    4 CORE STATES
>:1S 01: 1S                   -363.121745 Ry
>:2S 01: 2S                    -42.906536 Ry
>Core energies for all atoms and core states seperately
>
> >
> > The reason why I want to see it is that
> >
> > I find difference between the two crystal structure is very small, but 
the
> > difference of :ENE is very large about 2Ry. I want know if the result 
is
> > reasonable? Where the difference comin from?
>
>If the two structures are really similar, 2 Ry is a really large number.
>
>In order to compare you must have:
>Same atomic sphere sizes for both cases
>same RKMAX value (also effective)
>same GMAX
>compatible (or converged) k-mesh (But this should account only for some 
mRy)
>
>For more help you must provide more info (struct files, last iteration 
scf-file)
>
>Regards
>
>                                       P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: 
http://www.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
>====
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>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====




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------------------------------

Date: Thu, 11 Jul 2002 02:43:29 +0100
From: Ian Morrison <i.morrison@salford.ac.uk>
Subject: [WIEN]: ice cmc2_1

====
Ian Morrison <i.morrison@salford.ac.uk>
submitted the following contribution:
====


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Carl,

   could you use cerius to make a picture of the cmc2_1 unit cell  -
both eps and
jpeg (alex knows how to do eps -> jpeg).

   If you could also insert some arrows showing the movement of
molecules in
the phono we mapped would be useful.

  Ian

Xiangyuan Cui wrote:

> Dear Professor Blaha and other Wien2k users, We are trying to analysis
> the phonon frequency of hydrogen bond in ICE crystal by comparing the
> GGA and meta-GGA. We use R_O=1.2, R_H=0.6, R*K=5. For GGA, Gmax=22
> gives reasonable answer.For meta-GGA, when we used Gmax=24, the
> results is not as good as we expected. Then we tried Gmax=25 and
> continue running the job, all the calculations (5 single-point
> calculations) finished with one or two extra iterations.But something
> happens here: For 2 cases, the total energy remains nearly unchanged.
> But for the other 3 cases, the energy got higher (typically 0.025 Ry,
> which is too large for our purpose). I noticed your warning in
> January: Warning: Use GMAX as large as possible (24), even though it
> might be
> numerically unstable.
> Note: The meta-GGA uses the GGA potential, only the total Energy is
> changed!
> It seems it is necessary to use Gmax=25 here.My question is: how to
> overcome this instability? any remedy? Many Thanks!
> ---
> Outgoing mail is certified Virus Free.
> Checked by AVG anti-virus system (http://www.grisoft.com).
> Version: 6.0.365 / Virus Database: 202 - Release Date: 24/05/2002

- --
Dr Ian Morrison
Joule Physics Laboratory and Institute for Materials Research
University of Salford, M5 4WT, UK
email: i.morrison@salford.ac.uk  tel: +44 161 2955303


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<html>
<body bgcolor="#FFFFFF">
Carl,
<p>&nbsp;&nbsp; could you use cerius to make a picture of the cmc2_1 unit
cell&nbsp; - both eps and
<br>jpeg (alex knows how to do eps -> jpeg).
<p>&nbsp;&nbsp; If you could also insert some arrows showing the movement
of molecules in
<br>the phono we mapped would be useful.
<p>&nbsp; Ian
<p>Xiangyuan Cui wrote:
<blockquote TYPE=CITE><style></style>
<font face="Arial"><font size=-1>Dear
Professor Blaha and other Wien2k users,</font></font>&nbsp;<font face="Arial"><font size=-1>We
are trying to analysis the phonon frequency of hydrogen bond in ICE crystal
by comparing the GGA and meta-GGA. We use R_O=1.2, R_H=0.6, R*K=5.</font></font>&nbsp;<font face="Arial"><font size=-1>For
GGA, Gmax=22 gives reasonable answer.</font></font><font face="Arial"><font size=-1>For
meta-GGA, when we used Gmax=24, the results is not as good as we expected.
Then we tried Gmax=25 and continue running the job, all the calculations
(5 single-point calculations) finished with one or two extra iterations.</font></font><font face="Arial"><font size=-1>But
something happens here: For 2 cases, the total energy remains nearly unchanged.
But for the other 3 cases, the energy got higher (typically 0.025 Ry, which
is too large for our purpose).</font></font>&nbsp;<font face="Arial"><font size=-1>I
noticed your warning in January:</font></font>&nbsp;<b>Warning: Use GMAX
as large as possible (24), even though it might be</b>
<br><b>numerically unstable.</b>
<br><b>Note: The meta-GGA uses the GGA potential, only the total Energy
is changed!</b>&nbsp;
<br><font face="Arial"><font size=-1>It seems it is necessary to use Gmax=25
here.</font></font><font face="Arial"><font size=-1>My question is: how
to overcome this instability? any remedy?</font></font>&nbsp;<font face="Arial"><font size=-1>Many
Thanks!</font></font>&nbsp;&nbsp;
<br><font face="Arial"><font size=-1>---</font></font>
<br><font face="Arial"><font size=-1>Outgoing mail is certified Virus Free.</font></font>
<br><font face="Arial"><font size=-1>Checked by AVG anti-virus system (<a href="http://www.grisoft.com">http://www.grisoft.com</a>).</font></font>
<br><font face="Arial"><font size=-1>Version: 6.0.365 / Virus Database:
202 - Release Date: 24/05/2002</font></font></blockquote>

<p>--
<br>Dr Ian Morrison
<br>Joule Physics Laboratory and Institute for Materials Research
<br>University of Salford, M5 4WT, UK
<br>email: i.morrison@salford.ac.uk&nbsp; tel: +44 161 2955303
<br>&nbsp;
</body>
</html>

- --------------42AA47A1600B2A8ACB9FB027--

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------------------------------

Date: Thu, 11 Jul 2002 02:45:00 +0100
From: Ian Morrison <i.morrison@salford.ac.uk>
Subject: Re: [WIEN]: Meta-GGA (unstability)

====
Ian Morrison <i.morrison@salford.ac.uk>
submitted the following contribution:
====


- --------------0E9BC3018782EA13382112D7
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Ignore my last message - I replied to the wrong email !!

sorry

Xiangyuan Cui wrote:

> Dear Professor Blaha and other Wien2k users, We are trying to analysis
> the phonon frequency of hydrogen bond in ICE crystal by comparing the
> GGA and meta-GGA. We use R_O=1.2, R_H=0.6, R*K=5. For GGA, Gmax=22
> gives reasonable answer.For meta-GGA, when we used Gmax=24, the
> results is not as good as we expected. Then we tried Gmax=25 and
> continue running the job, all the calculations (5 single-point
> calculations) finished with one or two extra iterations.But something
> happens here: For 2 cases, the total energy remains nearly unchanged.
> But for the other 3 cases, the energy got higher (typically 0.025 Ry,
> which is too large for our purpose). I noticed your warning in
> January: Warning: Use GMAX as large as possible (24), even though it
> might be
> numerically unstable.
> Note: The meta-GGA uses the GGA potential, only the total Energy is
> changed!
> It seems it is necessary to use Gmax=25 here.My question is: how to
> overcome this instability? any remedy? Many Thanks!
> ---
> Outgoing mail is certified Virus Free.
> Checked by AVG anti-virus system (http://www.grisoft.com).
> Version: 6.0.365 / Virus Database: 202 - Release Date: 24/05/2002

- --
Dr Ian Morrison
Joule Physics Laboratory and Institute for Materials Research
University of Salford, M5 4WT, UK
email: i.morrison@salford.ac.uk  tel: +44 161 2955303


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<body bgcolor="#FFFFFF">
Ignore my last message - I replied to the wrong email !!
<p>sorry
<p>Xiangyuan Cui wrote:
<blockquote TYPE=CITE><style></style>
<font face="Arial"><font size=-1>Dear
Professor Blaha and other Wien2k users,</font></font>&nbsp;<font face="Arial"><font size=-1>We
are trying to analysis the phonon frequency of hydrogen bond in ICE crystal
by comparing the GGA and meta-GGA. We use R_O=1.2, R_H=0.6, R*K=5.</font></font>&nbsp;<font face="Arial"><font size=-1>For
GGA, Gmax=22 gives reasonable answer.</font></font><font face="Arial"><font size=-1>For
meta-GGA, when we used Gmax=24, the results is not as good as we expected.
Then we tried Gmax=25 and continue running the job, all the calculations
(5 single-point calculations) finished with one or two extra iterations.</font></font><font face="Arial"><font size=-1>But
something happens here: For 2 cases, the total energy remains nearly unchanged.
But for the other 3 cases, the energy got higher (typically 0.025 Ry, which
is too large for our purpose).</font></font>&nbsp;<font face="Arial"><font size=-1>I
noticed your warning in January:</font></font>&nbsp;<b>Warning: Use GMAX
as large as possible (24), even though it might be</b>
<br><b>numerically unstable.</b>
<br><b>Note: The meta-GGA uses the GGA potential, only the total Energy
is changed!</b>&nbsp;
<br><font face="Arial"><font size=-1>It seems it is necessary to use Gmax=25
here.</font></font><font face="Arial"><font size=-1>My question is: how
to overcome this instability? any remedy?</font></font>&nbsp;<font face="Arial"><font size=-1>Many
Thanks!</font></font>&nbsp;&nbsp;
<br><font face="Arial"><font size=-1>---</font></font>
<br><font face="Arial"><font size=-1>Outgoing mail is certified Virus Free.</font></font>
<br><font face="Arial"><font size=-1>Checked by AVG anti-virus system (<a href="http://www.grisoft.com">http://www.grisoft.com</a>).</font></font>
<br><font face="Arial"><font size=-1>Version: 6.0.365 / Virus Database:
202 - Release Date: 24/05/2002</font></font></blockquote>

<p>--
<br>Dr Ian Morrison
<br>Joule Physics Laboratory and Institute for Materials Research
<br>University of Salford, M5 4WT, UK
<br>email: i.morrison@salford.ac.uk&nbsp; tel: +44 161 2955303
<br>&nbsp;
</body>
</html>

- --------------0E9BC3018782EA13382112D7--

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------------------------------

Date: Thu, 11 Jul 2002 15:52:39 -0500 (GMT)
From: "Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
Subject: [WIEN]: about contour plotting

====
"Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
submitted the following contribution:
====

Dear WIEN users

I want to know that whether any body has developed any program for viewing
the contour plots in detail and willing to share the program with the
users of WIEN? Also, if some one will be able to tell me how to use the
XCRYSDEN for plottting utilities, I will be very grateful (as no user
manual is available for the functions and so far I have been able to
generate only a single straight line in XCRYSDEN while trying to plot the
contours). I am calculating the electron density for CuV2O5 which is
monoclinic system and I want to plot the electron density in the local
axis and not in cartesian axis which is required for using rhoplot and
gnuplot. 



Dr. Sharat Chandra %%%%%%%% _ %%%%%%%%%%%% ___ %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
Materials Science Division (_) ___   ___  / _ \  ___
Indira Gandhi Centre for   | |/ _ \ / __\| |_| |' _ \ 183, Central Avenue
Atomic Research            | | (_) | |__,|  _  | | \| DAE Township, Kalpakkam
Kalpakkam 603102 TN INDIA  |_|\__/ |\___/|_| |_|_|    603102 TN INDIA
Ph. & FAX: 91 4114 480081     / /| | %%%%%%%%%%%%%%%% 91 4114 481521
email: sharat@igcar.ernet.in | |_| | %%%%%%%%%%%%%%%% sharat_c@yahoo.com
%%%%%%%%%%%%%%%%%%%%%%%%%%%%% \___/ %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%



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------------------------------

Date: Fri, 12 Jul 2002 08:27:32 +0800 (CST)
From: =?gb2312?q?Weidong=20zou?= <zouwd@yahoo.com.cn>
Subject: [WIEN]: fmt:read unexpected character

====
=?gb2312?q?Weidong=20zou?= <zouwd@yahoo.com.cn>
submitted the following contribution:
====

Dear wien users,
  When I implement SCF cycle, I have obtained the
error message in cycle 5 : 
        "fmt: read unexpected character
        apparent state:unit 45 named ./CuCl.help45up" 

and the error file write:"Error in LAPW2". 
   In the file CuCl.help45up, I find:
   BAND#  1 E= -6.9918 WEIGHT=0.40000
   L=0 23.42762 ********17895.491***********-1779.157 

   L=1 0.0004   0.000   0.000    0.000  0.000  0.000

   BAND#  2 E= -6.9946 WEIGHT=0.40000
   L=0 23.37931 ********178525.491**********-1779.157 

   L=1 0.0007   0.000   0.000    0.000  0.000  0.0000

  I don't know how to adjust this error .could anyone
help me? I am desperate. I would very heartily
appreciate any help.

Best regardes!
                                   W.D.Zou

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------------------------------

Date: Sun, 14 Jul 2002 12:00:25 +0800
From: "wan liu" <wien97wan@hotmail.com>
Subject: [WIEN]: about mini

====
"wan liu" <wien97wan@hotmail.com>
submitted the following contribution:
====

Dear Wien users and developers

Now I try to use min_lapw to optimize the internal parameter of crystal. I 
have two questions.

(1) According the space-group symmetry, the position is (0.5, 0.25, x), so 
I write the case.inM as 
(0.0 0.0 1.0 0.5). It is right?

(2) The min_lapw is working. But first the total energy decrease, after 
about four iteration the total energy will increase(now the force is still 
large), on the other hand, the force will decrease. My question is I can 
take which structure as the ground state? The structure has minimal total 
ernergy and large force; or the structure has minimal force but not minimal 
total ernergy?

Best wish!

Liu


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------------------------------

Date: Sun, 14 Jul 2002 10:29:08 -0500 (GMT)
From: "Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
Subject: [WIEN]: about monoclinic brillouin zone

====
"Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
submitted the following contribution:
====


  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

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Hi wien users

I am doing calculations for the CuV2O5 in base centered monoclinic phase. 
My problem concerns the band structure calculations. When I try to
generate the case.klist file with XCrysden, it shows a B.Z. similar to
base centered Orthorhombic, rather than base centered monoclinic. So, I
have just taken the B.Z. for base centered monoclinic and generated my own
klist, which does the integration along the V->Z->Gamma->A->M->L path
(Bradley & Cracknell). I want to know is it OK to do so?

Dear Prof. Holzwarth: thanks for the information and the 3D program. I am
trying to learn the open DX these days. 

Regards
Sharat Chandra

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- ---559023410-851401618-1026660194=:506--

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------------------------------

Date: Sun, 14 Jul 2002 10:17:55 +0200 (CEST)
From: =?iso-8859-1?q?fafa=20chiker?= <chiker_fafa@yahoo.fr>
Subject: [WIEN]: thank's Msr Blaha

====
=?iso-8859-1?q?fafa=20chiker?= <chiker_fafa@yahoo.fr>
submitted the following contribution:
====

Dear Prof.Blaha i am very happy to your answer, so i
have found the solution to my problem and I am very
grateful, sir,to your help, also to my chairman
B.Abbar.
the solution is to make the -c in x dstart command in
the three jobs: eos.job, rhomb.job and tetra.job.
thank you very much,
yours

___________________________________________________________
Do You Yahoo!? -- Une adresse @yahoo.fr gratuite et en français !
Yahoo! Mail : http://fr.mail.yahoo.com
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------------------------------

Date: Mon, 15 Jul 2002 09:54:23 -0500 (GMT)
From: "Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
Subject: [WIEN]: about monoclinic brillouin zone

====
"Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
submitted the following contribution:
====


  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---559023410-851401618-1026660194=:506
Content-Type: TEXT/PLAIN; CHARSET=US-ASCII
Content-ID: <Pine.SV4.3.93.1020714102336.506C@msd>

Hi all

This is in continuation of the previous mail. I have calculated the band
structure without the band character plotting and I get a band structure
with gaps in between with the attached klist. This can only mean that this
klist is incorrect. Can anybody please tell me what can be the problem? Or
should I calculate the band structure with the base centered Orthorhombic
klist? In which case will it be the correct one anyway?

Regards
Sharat Chandra

- ---------- Forwarded message ----------

I am doing calculations for the CuV2O5 in base centered monoclinic phase. 
My problem concerns the band structure calculations. When I try to
generate the case.klist file with XCrysden, it shows a B.Z. similar to
base centered Orthorhombic, rather than base centered monoclinic. So, I
have just taken the B.Z. for base centered monoclinic and generated my own
klist, which does the integration along the V->Z->Gamma->A->M->L path
(Bradley & Cracknell). I want to know is it OK to do so?

Regards
Sharat Chandra

- ---559023410-851401618-1026660194=:506
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Content-Description: case structure file

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IC0yNiAgIDM4ICAgNzYgIDEuMA0KICAgICAgICAgICAgLTM4ICAtMjQgICAz
OCAgIDc2ICAxLjANCiAgICAgICAgICAgIC0zOCAgLTIyICAgMzggICA3NiAg
MS4wDQogICAgICAgICAgICAtMzggIC0yMCAgIDM4ICAgNzYgIDEuMA0KICAg
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IDc2ICAxLjANCiAgICAgICAgICAgIC0zOCAgLTEwICAgMzggICA3NiAgMS4w
DQogICAgICAgICAgICAtMzggICAtOCAgIDM4ICAgNzYgIDEuMA0KICAgICAg
ICAgICAgLTM4ICAgLTYgICAzOCAgIDc2ICAxLjANCiAgICAgICAgICAgIC0z
OCAgIC00ICAgMzggICA3NiAgMS4wDQogICAgICAgICAgICAtMzggICAtMiAg
IDM4ICAgNzYgIDEuMA0KTCAgICAgICAgICAgLTM4ICAgIDAgICAzOCAgIDc2
ICAxLjANCkVORA0K
- ---559023410-851401618-1026660194=:506--

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------------------------------

Date: Mon, 15 Jul 2002 15:12:52 +1000
From: chen0130@flinders.edu.au
Subject: [WIEN]: k-list

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Dear Wien users,

I am a beginner with Wien97.10, and I have 2 questions,

1) Where can I find some resources for generating a k-list for a slab of Li2O
(antifluorite unit cells separated by a vacuum region) with XCrysDen, as I seek
a band structure calculation.

2) What are the maximum Dimensional Parameters, or what stops me from enlarging
the parameters so that I have plenty of room for my slab calculation... is it a
bad idea to increase the parameters so they are much larger than the minimum
requirements of  a calc.?

Thanks for your time, sorry to ask such basic questions!

Cheng Chen
Nonours student
Flinders University of South Australia 


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------------------------------

Date: Mon, 15 Jul 2002 10:37:13 +0100
From: "Xiangyuan Cui" <x.cui@pgr.salford.ac.uk>
Subject: Re: [WIEN]: about mini

====
"Xiangyuan Cui" <x.cui@pgr.salford.ac.uk>
submitted the following contribution:
====

Hi, Liu


> Dear Wien users and developers
>
> Now I try to use min_lapw to optimize the internal parameter of crystal. I
> have two questions.
>
> (1) According the space-group symmetry, the position is (0.5, 0.25, x), so
> I write the case.inM as
> (0.0 0.0 1.0 0.5). It is right?

Right!

> (2) The min_lapw is working. But first the total energy decrease, after
> about four iteration the total energy will increase(now the force is still
> large), on the other hand, the force will decrease. My question is I can
> take which structure as the ground state? The structure has minimal total
> ernergy and large force; or the structure has minimal force but not
minimal

A coorect mini process will creat several or quite a lot converged *.scf
files (case_1.scf, case_2.scf, etc). I wonder the energies you compared have
not converged yet (since you just compare four ITERATION). Of course, the
optimal geometry corresponds minimum total energy on ground state.
Otherwise, you may need to refine other parameters.

regards,

xiangyuan Cui

>


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------------------------------

Date: Mon, 15 Jul 2002 15:48:22 +0300
From: "B. Yanchitsky" <yan@im.imag.kiev.ua>
Subject: Re: [WIEN]: about monoclinic brillouin zone

====
"B. Yanchitsky" <yan@im.imag.kiev.ua>
submitted the following contribution:
====

"Dr. Sharat Chandra" wrote:
> 
> Hi all
> 
> This is in continuation of the previous mail. I have calculated the band
> structure without the band character plotting and I get a band structure
> with gaps in between with the attached klist. This can only mean that this
> klist is incorrect. Can anybody please tell me what can be the problem? Or
> should I calculate the band structure with the base centered Orthorhombic
> klist? In which case will it be the correct one anyway?
> 

Probably the problem is due to wrong struct file.
The following portion

ATOM=-22: X=0.52690000 Y=0.36500000 Z=0.10200000
          MULT= 1          ISPLIT= 8

ATOM=-23: X=0.46320000 Y=0.65500000 Z=0.91800000
          MULT= 1          ISPLIT= 8

is not consistent with any monoclinic space group.

Regards,

Bogdan
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Date: Mon, 15 Jul 2002 10:55:56 -0400
From: Jeff Spirko <spirko@lehigh.edu>
Subject: [WIEN]: Re: about mini

====
Jeff Spirko <spirko@lehigh.edu>
submitted the following contribution:
====

On Mon, Jul 15, 2002 at 10:37:13AM +0100, Xiangyuan Cui wrote:
> Hi, Liu
> > (2) The min_lapw is working. But first the total energy decrease, after
> > about four iteration the total energy will increase(now the force is still
> > large), on the other hand, the force will decrease. My question is I can
> > take which structure as the ground state? The structure has minimal total
> > ernergy and large force; or the structure has minimal force but not
> > minimal
> A coorect mini process will creat several or quite a lot converged *.scf
> files (case_1.scf, case_2.scf, etc). I wonder the energies you compared have
> not converged yet (since you just compare four ITERATION). Of course, the
> optimal geometry corresponds minimum total energy on ground state.
> Otherwise, you may need to refine other parameters.

Also, on the last iteration at any geometry, FOR should be set in
the *.in2[c] file.  This can be done by using the force convergence
criterion (-fc 0.5, for example) or manually.

As a question to the experts, is it okay to do something like the
following:

  $ run_lapw -ec 0.001 -it -I         # -I sets TOT in *.in2c file
  $ emacs *.in2c                      # Manually change to FOR
  $ run_lapw -i 1 -s lapw2c

I'm hoping this will converge the calculation, then re-calculate the
total forces on the last iteration without having to run lapw1c again.

- -- 
Jeff Spirko   spirko@lehigh.edu   spirko@yahoo.com   WD3V   |=>

The study of non-linear physics is like the study of non-elephant biology.

All theoretical chemistry is really physics;
and all theoretical chemists know it. -- Richard P. Feynman 
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------------------------------

Date: Mon, 15 Jul 2002 18:55:57 +0200 (CEST)
From: =?iso-8859-1?q?Houda=20Imene?= <houda_imene@yahoo.fr>
Subject: [WIEN]: boron space group

====
=?iso-8859-1?q?Houda=20Imene?= <houda_imene@yahoo.fr>
submitted the following contribution:
====

- --0-1560328206-1026752157=:26338
Content-Type: text/plain; charset=iso-8859-1
Content-Transfer-Encoding: 8bit


Dear wien user;

I'm interested in structural properties of Boron, and it has the space group 166 (R-3m) with alpha=beta=gama different from 90°, with tow internal parmeters that I want to optimize.

The problem is that when I choose 166 as space group, I'm asked if I want hexagonal or rhombohedral structure, and both answers lead to floating point error displayed on the window and the lines of atomic positions on the case.struct are simply deleeted! I don't know if it is a bug corresponding to this special space group or I done some mistake, since I started with an ad-hoc internal parameters.

Any suggestion will be appreciated!

Regards

Houda Imane



- ---------------------------------
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- --0-1560328206-1026752157=:26338
Content-Type: text/html; charset=iso-8859-1
Content-Transfer-Encoding: 8bit

<P>Dear wien user;</P>
<P>I'm interested in structural properties of Boron, and it has the space group 166 (R-3m) with alpha=beta=gama different from 90°, with tow internal parmeters that I want to optimize.</P>
<P>The problem is that when I choose 166 as space group, I'm asked if I want hexagonal or rhombohedral structure, and both answers lead to floating point error displayed on the window and the lines of atomic positions on the case.struct are simply deleeted! I don't know if it is a bug corresponding to this special space group or I done some mistake, since I started with an ad-hoc internal parameters.</P>
<P>Any suggestion will be appreciated!</P>
<P>Regards</P>
<P>Houda Imane</P><p><br><hr size=1><a href="http://fr.mail.yahoo.com">Yahoo! Mail</a> -- Une adresse @yahoo.fr gratuite et en français !<br>
- --0-1560328206-1026752157=:26338--
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------------------------------

Date: Tue, 16 Jul 2002 10:27:32 -0500 (GMT)
From: "Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
Subject: Re: [WIEN]: about monoclinic brillouin zone

====
"Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
submitted the following contribution:
====

Dear Dr. Yanchitsky

These two atom positions correspond to the 4b Wyckoff positions (x,y,z and
x,-y,z) and all the other atoms correspond to the 2a positions (x,0,z). 
The problem is that If I give both x,y,z and x,-y,z positions for the Cu
atoms, it puts them very very close to each other, so I have given only
one of the two positions. I know that in this material only one of the
positions is supposed to be occupied. Also, I have checked the BZ problem
with a simple monoclinic structure and there also I get a BZ which
corresponds to the base centered Orthorhombic structure.

Regards
Shara Chandra

On Mon, 15 Jul 2002, B. Yanchitsky wrote:
> Probably the problem is due to wrong struct file.
> The following portion
> 
> ATOM=-22: X=0.52690000 Y=0.36500000 Z=0.10200000
>           MULT= 1          ISPLIT= 8
> 
> ATOM=-23: X=0.46320000 Y=0.65500000 Z=0.91800000
>           MULT= 1          ISPLIT= 8
> 
> is not consistent with any monoclinic space group.



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------------------------------

Date: Tue, 16 Jul 2002 07:18:50 +0000
From: "tayeb Meftah" <motay@hotmail.com>
Subject: Re: [WIEN]: boron space group

====
"tayeb Meftah" <motay@hotmail.com>
submitted the following contribution:
====

<html><div style='background-color:'><DIV>
<P>Bonjour Imene;</P>
<P>J'ai recu de votre part un grand nombre de mail concernant votre sujet de recherche.</P>
<P>C'est un domaine qui interesse notre equipe de recherche installée en Algerie. Je transmetterai</P>
<P>vos mails aux membres du laboratoires. Vous etes en quel Laboratoire actuellement?</P>
<P>Merci et a la prochaine<BR><BR></P></DIV>
<DIV></DIV>
<DIV></DIV>&gt;From: Houda Imene <HOUDA_IMENE@YAHOO.FR>
<DIV></DIV>&gt;Reply-To: wien@zeus.theochem.tuwien.ac.at 
<DIV></DIV>&gt;To: wien@zeus.theochem.tuwien.ac.at 
<DIV></DIV>&gt;Subject: [WIEN]: boron space group 
<DIV></DIV>&gt;Date: Mon, 15 Jul 2002 18:55:57 +0200 (CEST) 
<DIV></DIV>&gt; 
<DIV></DIV>&gt; 
<DIV></DIV>&gt;Dear wien user; 
<DIV></DIV>&gt; 
<DIV></DIV>&gt;I'm interested in structural properties of Boron, and it has the space group 166 (R-3m) with alpha=beta=gama different from 90°, with tow internal parmeters that I want to optimize. 
<DIV></DIV>&gt; 
<DIV></DIV>&gt;The problem is that when I choose 166 as space group, I'm asked if I want hexagonal or rhombohedral structure, and both answers lead to floating point error displayed on the window and the lines of atomic positions on the case.struct are simply deleeted! I don't know if it is a bug corresponding to this special space group or I done some mistake, since I started with an ad-hoc internal parameters. 
<DIV></DIV>&gt; 
<DIV></DIV>&gt;Any suggestion will be appreciated! 
<DIV></DIV>&gt; 
<DIV></DIV>&gt;Regards 
<DIV></DIV>&gt; 
<DIV></DIV>&gt;Houda Imane 
<DIV></DIV>&gt; 
<DIV></DIV>&gt; 
<DIV></DIV>&gt; 
<DIV></DIV>&gt;--------------------------------- 
<DIV></DIV>&gt;Yahoo! Mail -- Une adresse @yahoo.fr gratuite et en français ! 
<DIV></DIV></div><br clear=all><hr>MSN Photos is the easiest way to share and print your photos: <a href='http://g.msn.com/1HM1ENFR/c156??PI=44338'>Click Here</a><br></html>
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------------------------------

Date: Tue, 16 Jul 2002 15:30:28 +0800
From: "wan liu" <wien97wan@hotmail.com>
Subject: Re: [WIEN]: Re: about mini

====
"wan liu" <wien97wan@hotmail.com>
submitted the following contribution:
====




>From: Jeff Spirko <spirko@lehigh.edu>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: wien@zeus.theochem.tuwien.ac.at
>Subject: [WIEN]: Re: about mini
>Date: Mon, 15 Jul 2002 10:55:56 -0400
>
>====
>Jeff Spirko <spirko@lehigh.edu>
>submitted the following contribution:
>====
>
>On Mon, Jul 15, 2002 at 10:37:13AM +0100, Xiangyuan Cui wrote:
> > Hi, Liu
> > > (2) The min_lapw is working. But first the total energy decrease, 
after
> > > about four iteration the total energy will increase(now the force is 
still
> > > large), on the other hand, the force will decrease. My question is I 
can
> > > take which structure as the ground state? The structure has minimal 
total
> > > ernergy and large force; or the structure has minimal force but not
> > > minimal
> > A coorect mini process will creat several or quite a lot converged 
*.scf
> > files (case_1.scf, case_2.scf, etc). I wonder the energies you compared 
have
> > not converged yet (since you just compare four ITERATION). Of course, 
the
> > optimal geometry corresponds minimum total energy on ground state.
> > Otherwise, you may need to refine other parameters.
>
>Also, on the last iteration at any geometry, FOR should be set in
>the *.in2[c] file.  This can be done by using the force convergence
>criterion (-fc 0.5, for example) or manually.
>
>As a question to the experts, is it okay to do something like the
>following:
>
>   $ run_lapw -ec 0.001 -it -I         # -I sets TOT in *.in2c file
>   $ emacs *.in2c                      # Manually change to FOR
>   $ run_lapw -i 1 -s lapw2c
>
>I'm hoping this will converge the calculation, then re-calculate the
>total forces on the last iteration without having to run lapw1c again.

Thank you very much!

First I run init_lapw, then run min_lapw. From case.scf_mini, I find the 
total energy isn't decrease, on the other hand the force will decrease.

Your suggestion is to set FOR in the case.in2c to improve the calculated 
force. The default term in min_lapw is "run_lapw -I -fc 1." As you said 
that the I-option in run_lapw sets TOT in case.in2c file. So, I want to 
delete the -I-option in min_lapw, and set FOR in case.in2c, and run the 
min_lapw directly. I don't know if it is right?

Best wish!

Liu
>
>--
>Jeff Spirko   spirko@lehigh.edu   spirko@yahoo.com   WD3V   |=>
>
>The study of non-linear physics is like the study of non-elephant biology.
>
>All theoretical chemistry is really physics;
>and all theoretical chemists know it. -- Richard P. Feynman
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====




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------------------------------

Date: Tue, 16 Jul 2002 00:42:43 -0700 (PDT)
From: sayede adlane <dft22000@yahoo.fr>
Subject: Re: [WIEN]: boron space group

====
sayede adlane <dft22000@yahoo.fr>
submitted the following contribution:
====

Hi houda, send me your struct file
Adlane.
- --- Houda Imene <houda_imene@yahoo.fr> wrote:
> 
> Dear wien user;
> 
> I'm interested in structural properties of Boron,
> and it has the space group 166 (R-3m) with
> alpha=beta=gama different from 90°, with tow
> internal parmeters that I want to optimize.
> 
> The problem is that when I choose 166 as space
> group, I'm asked if I want hexagonal or rhombohedral
> structure, and both answers lead to floating point
> error displayed on the window and the lines of
> atomic positions on the case.struct are simply
> deleeted! I don't know if it is a bug corresponding
> to this special space group or I done some mistake,
> since I started with an ad-hoc internal parameters.
> 
> Any suggestion will be appreciated!
> 
> Regards
> 
> Houda Imane
> 
> 
> 
> ---------------------------------
> Yahoo! Mail -- Une adresse @yahoo.fr gratuite et en
> français !
> 


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------------------------------

Date: Tue, 16 Jul 2002 10:32:15 +0200 (CEST)
From: =?iso-8859-1?q?Houda=20Imene?= <houda_imene@yahoo.fr>
Subject: Re: [WIEN]: boron space group

====
=?iso-8859-1?q?Houda=20Imene?= <houda_imene@yahoo.fr>
submitted the following contribution:
====

- --0-1445261461-1026808335=:67074
Content-Type: text/plain; charset=iso-8859-1
Content-Transfer-Encoding: 8bit


 Hi Adlane;
In fact the mane problem is the struct file generation. Since i have no idea about the values of internal parameters, I usually start with any random values (close to physical tolerance) and optimize... In this case, the wien utility to generate the space group 166 do not help! It only display an error message (floatin point error)
to learn more about Boron structure go to http://cst-www.nrl.navy.mil/lattice/struk/alphaB.html
Thanks
  sayede adlane <dft22000@yahoo.fr> a écrit : ====
sayede adlane 
submitted the following contribution:
====

Hi houda, send me your struct file
Adlane.
- --- Houda Imene wrote:
> 
> Dear wien user;
> 
> I'm interested in structural properties of Boron,
> and it has the space group 166 (R-3m) with
> alpha=beta=gama different from 90°, with tow
> internal parmeters that I want to optimize.
> 
> The problem is that when I choose 166 as space
> group, I'm asked if I want hexagonal or rhombohedral
> structure, and both answers lead to floating point
> error displayed on the window and the lines of
> atomic positions on the case.struct are simply
> deleeted! I don't know if it is a bug corresponding
> to this special space group or I done some mistake,
> since I started with an ad-hoc internal parameters.
> 
> Any suggestion will be appreciated!
> 
> Regards
> 
> Houda Imane
> 
> 
> 
> ---------------------------------
> Yahoo! Mail -- Une adresse @yahoo.fr gratuite et en
> français !
> 


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- --0-1445261461-1026808335=:67074
Content-Type: text/html; charset=iso-8859-1
Content-Transfer-Encoding: 8bit

<P> Hi Adlane;
<P>In fact the mane problem is the struct file generation. Since i have no idea about the values of internal parameters, I usually start with any random values (close to physical tolerance) and optimize... In this case, the wien utility to generate the space group 166 do not help! It only display an error message (floatin point error)
<P>to learn more about Boron structure go to <A href="http://cst-www.nrl.navy.mil/lattice/struk/alphaB.html">http://cst-www.nrl.navy.mil/lattice/struk/alphaB.html</A>
<P>Thanks
<P>&nbsp; <B><I>sayede adlane &lt;dft22000@yahoo.fr&gt;</I></B> a écrit&nbsp;: 
<BLOCKQUOTE style="BORDER-LEFT: #1010ff 2px solid; MARGIN-LEFT: 5px; PADDING-LEFT: 5px">====<BR>sayede adlane <DFT22000@YAHOO.FR><BR>submitted the following contribution:<BR>====<BR><BR>Hi houda, send me your struct file<BR>Adlane.<BR>--- Houda Imene <HOUDA_IMENE@YAHOO.FR>wrote:<BR>&gt; <BR>&gt; Dear wien user;<BR>&gt; <BR>&gt; I'm interested in structural properties of Boron,<BR>&gt; and it has the space group 166 (R-3m) with<BR>&gt; alpha=beta=gama different from 90°, with tow<BR>&gt; internal parmeters that I want to optimize.<BR>&gt; <BR>&gt; The problem is that when I choose 166 as space<BR>&gt; group, I'm asked if I want hexagonal or rhombohedral<BR>&gt; structure, and both answers lead to floating point<BR>&gt; error displayed on the window and the lines of<BR>&gt; atomic positions on the case.struct are simply<BR>&gt; deleeted! I don't know if it is a bug corresponding<BR>&gt; to this special space group or I done some mistake,<BR>&gt; since I started with an ad-hoc !
internal parameters.<BR>&gt; <BR>&gt; Any suggestion will be appreciated!<BR>&gt; <BR>&gt; Regards<BR>&gt; <BR>&gt; Houda Imane<BR>&gt; <BR>&gt; <BR>&gt; <BR>&gt; ---------------------------------<BR>&gt; Yahoo! Mail -- Une adresse @yahoo.fr gratuite et en<BR>&gt; français !<BR>&gt; <BR><BR><BR>__________________________________________________<BR>Do You Yahoo!?<BR>Yahoo! Autos - Get free new car price quotes<BR>http://autos.yahoo.com<BR>====<BR>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at<BR>To (un)subscribe send mail to<BR>majordomo@zeus.theochem.tuwien.ac.at<BR>====</BLOCKQUOTE><p><br><hr size=1><a href="http://fr.mail.yahoo.com">Yahoo! Mail</a> -- Une adresse @yahoo.fr gratuite et en français !<br>
- --0-1445261461-1026808335=:67074--
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------------------------------

Date: Tue, 16 Jul 2002 20:50:28 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: about mini

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Now I try to use min_lapw to optimize the internal parameter of crystal. I
> have two questions.
>
> (1) According the space-group symmetry, the position is (0.5, 0.25, x), so
> I write the case.inM as
> (0.0 0.0 1.0 0.5). It is right?

Most likely (local rotations?), but it is not necessary to restrict the
other positions to zero (since they have no forces anyway)

> (2) The min_lapw is working. But first the total energy decrease, after
> about four iteration the total energy will increase(now the force is still
> large), on the other hand, the force will decrease. My question is I can
> take which structure as the ground state? The structure has minimal total
> ernergy and large force; or the structure has minimal force but not minimal
> total ernergy?

If your calculations are done properly, zero force and lowest E-tot must
coincide. If this does not happen, something is wrong. Either the symmetry
or too small RKmax, GMAX, k-mesh ?

Send:

grep :ENE *mini
grep :FORxx *mini     (where xx is the atom in question)
grep :POSxx *mini

In a regular nonmagnetic case it is not necessary to change anything
and just jun    min_lapw
The default switches -fc 1.0 and -I should be ok. Make sure your case
converges within the default 20 iterations.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 16 Jul 2002 20:56:27 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Re: about mini

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> As a question to the experts, is it okay to do something like the
> following:
>
>   $ run_lapw -ec 0.001 -it -I         # -I sets TOT in *.in2c file
>   $ emacs *.in2c                      # Manually change to FOR
>   $ run_lapw -i 1 -s lapw2c
>
> I'm hoping this will converge the calculation, then re-calculate the
> total forces on the last iteration without having to run lapw1c again.

No. Two reasons:
mixer will be totally confused, since it gets twice the same density for
mixing and also the scf file will be strange, since you the iteration
number is twice the same (wrong e-tot, forces).

Secondly: There"s no guarantee that your forces are converged. A total
energy convergence of 1 mRy only may give absolute nonsense for the
forces.

You can first converge the energy (-ec 0.0001( and then the forces (-fc
1.0). With this you are sure that both quantities are converged, since
there are (few) strange cases, where the forces may be converged before
E-tot is.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 16 Jul 2002 20:59:24 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: about monoclinic brillouin zone

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> These two atom positions correspond to the 4b Wyckoff positions (x,y,z and
> x,-y,z) and all the other atoms correspond to the 2a positions (x,0,z).
> The problem is that If I give both x,y,z and x,-y,z positions for the Cu
> atoms, it puts them very very close to each other, so I have given only
> one of the two positions. I know that in this material only one of the
> positions is supposed to be occupied. Also, I have checked the BZ problem
> with a simple monoclinic structure and there also I get a BZ which
> corresponds to the base centered Orthorhombic structure.

You cannot do partial occupations in WIEN2k. You must reduce symmetry and
then occupy only one of those two positions, but this cannot be done in
this spacegroup.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 16 Jul 2002 21:03:46 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: boron space group

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I'm interested in structural properties of Boron, and it has the space group 166 (R-3m) with alpha=beta=gama different from 90°, with tow internal parmeters that I want to optimize.
>
> The problem is that when I choose 166 as space group, I'm asked if I want hexagonal or rhombohedral structure, and both answers lead to floating point error displayed on the window and the lines of atomic positions on the case.struct are simply deleeted! I don't know if it is a bug corresponding to this special space group or I done some mistake, since I started with an ad-hoc internal parameters.

A rhombohedral space group requires the hexagonal lattice parameters !!!!
(There is a rhombohedral and a hexagonal setting  please check a good book
on crystallography). The UG tells you how to convert rhombohedral lattice
parameters into hexagonal ones.

Strangly enough, WIEN requires rhombohedral positions, but a program can
automatically convert this for you, but you must tell the program if you
entered R or hex coordinates.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 16 Jul 2002 21:08:20 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: k-list

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I am a beginner with Wien97.10, and I have 2 questions,
>
> 1) Where can I find some resources for generating a k-list for a slab of Li2O
> (antifluorite unit cells separated by a vacuum region) with XCrysDen, as I seek
> a band structure calculation.

You just need to plot them in 2 dimensions. Xcrysden shows you a very flat
cell. Just ignore the dispersion in the z-direction.

> 2) What are the maximum Dimensional Parameters, or what stops me from enlarging
> the parameters so that I have plenty of room for my slab calculation... is it a
> bad idea to increase the parameters so they are much larger than the minimum
> requirements of  a calc.?

The memory of your computer! Larger parameters means large memory
requirements. If your computer is large enough, you can of course use
large Parameters even for a small case.  (WIEN2k with dynamic allocation
does this automatically).

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 17 Jul 2002 11:33:51 +1000
From: chen0130@flinders.edu.au
Subject: Re: [WIEN]: k-list

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Dear Peter,

Thanks for your response, but I am not sure what you mean by plotting them in 2 
dimensions... I actually have very little idea how to generate a k list, sorry 
to be so vague, could you give me some 'idiots' advice?

Thanks,

Cheng

Quoting Peter Blaha <pblaha@theochem.tuwien.ac.at>:

> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> > I am a beginner with Wien97.10, and I have 2 questions,
> >
> > 1) Where can I find some resources for generating a k-list for a slab of
> Li2O
> > (antifluorite unit cells separated by a vacuum region) with XCrysDen, as I
> seek
> > a band structure calculation.
> 
> You just need to plot them in 2 dimensions. Xcrysden shows you a very flat
> cell. Just ignore the dispersion in the z-direction.
> 
> > 2) What are the maximum Dimensional Parameters, or what stops me from
> enlarging
> > the parameters so that I have plenty of room for my slab calculation... is
> it a
> > bad idea to increase the parameters so they are much larger than the
> minimum
> > requirements of  a calc.?
> 
> The memory of your computer! Larger parameters means large memory
> requirements. If your computer is large enough, you can of course use
> large Parameters even for a small case.  (WIEN2k with dynamic allocation
> does this automatically).
> 
> Regards
> 
> 
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
> http://www.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 
> 



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------------------------------

Date: Wed, 17 Jul 2002 14:04:59 +0800
From: "wan liu" <wien97wan@hotmail.com>
Subject: Re: [WIEN]: about mini

====
"wan liu" <wien97wan@hotmail.com>
submitted the following contribution:
====




>From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: <wien@zeus.theochem.tuwien.ac.at>
>Subject: Re: [WIEN]: about mini
>Date: Tue, 16 Jul 2002 20:50:28 +0200 (MEST)
>
>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
> > Now I try to use min_lapw to optimize the internal parameter of 
crystal. I
> > have two questions.
> >
> > (1) According the space-group symmetry, the position is (0.5, 0.25, x), 
so
> > I write the case.inM as
> > (0.0 0.0 1.0 0.5). It is right?
>
>Most likely (local rotations?), but it is not necessary to restrict the
>other positions to zero (since they have no forces anyway)

If they have forces, it means the structure file is wrong?

>
> > (2) The min_lapw is working. But first the total energy decrease, after
> > about four iteration the total energy will increase(now the force is 
still
> > large), on the other hand, the force will decrease. My question is I 
can
> > take which structure as the ground state? The structure has minimal 
total
> > ernergy and large force; or the structure has minimal force but not 
minimal
> > total ernergy?
>
>If your calculations are done properly, zero force and lowest E-tot must
>coincide. If this does not happen, something is wrong. Either the symmetry
>or too small RKmax, GMAX, k-mesh ?
>
>Send:
>
>grep :ENE *mini
>grep :FORxx *mini     (where xx is the atom in question)
>grep :POSxx *mini
>
>In a regular nonmagnetic case it is not necessary to change anything
>and just jun    min_lapw
>The default switches -fc 1.0 and -I should be ok. Make sure your case
>converges within the default 20 iterations.
>
>Regards
>                                       P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: 
http://www.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====




_________________________________________________________________
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------------------------------

Date: Wed, 17 Jul 2002 15:39:38 -0500 (GMT)
From: "Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
Subject: Re: [WIEN]: about monoclinic brillouin zone

====
"Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
submitted the following contribution:
====

Dear Prof. Blaha

What you say is true. I can not reduce the symmetry for this spacegroup. 
But to be able to calculate the band structure, I want to know, whether it
is all right to shift the Cu atoms a little apart manually to satisfy the
occupancy conditions (to positions which are different from those I get
from the Rietveldt refinement of the structure) and what effect is it
expected have on the ultimate band structure? I am asking this as it takes
almost a month to complete the SCF iteration on my 2 processor server.

Regards
Sharat Chandra

> You cannot do partial occupations in WIEN2k. You must reduce symmetry and
> then occupy only one of those two positions, but this cannot be done in
> this spacegroup.


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------------------------------

Date: Wed, 17 Jul 2002 16:44:08 -0500 (GMT)
From: "Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
Subject: Re: [WIEN]: about monoclinic brillouin zone

====
"Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
submitted the following contribution:
====


  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---559023410-851401618-1026942248=:8621
Content-Type: TEXT/PLAIN; charset=US-ASCII

Dear Prof. Blaha

I have tried the CuV2O5 structure with the Cu atoms shifted a little from
their actual positions but with Cu atoms having multiplicity 2. Even now I
find that the XCrysden shows the BZ to be base centered Orthorhombic type
rather than base centered monoclinic. I have also found that the struct
file now has zero number of symmetry operations instead of the usual one.
If you have any ideas about how to prepare the correct input file for this
compound, I will be very grateful. 

Regards

Sharat Chandra

> 
> > These two atom positions correspond to the 4b Wyckoff positions (x,y,z and
> > x,-y,z) and all the other atoms correspond to the 2a positions (x,0,z).
> > The problem is that If I give both x,y,z and x,-y,z positions for the Cu
> > atoms, it puts them very very close to each other, so I have given only
> > one of the two positions. I know that in this material only one of the
> > positions is supposed to be occupied. Also, I have checked the BZ problem
> > with a simple monoclinic structure and there also I get a BZ which
> > corresponds to the base centered Orthorhombic structure.


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- ---559023410-851401618-1026942248=:8621--

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------------------------------

Date: Wed, 17 Jul 2002 04:45:50 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: band structure

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started Band structure and in Xspaghetti-C, got
this message "case.insp.1st line should started with
### what it the mean? and not derived band structure
figure.
Thank you for the guide.
H-Salehi 


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------------------------------

Date: Wed, 17 Jul 2002 06:10:10 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [none]

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien2k users;


with best wishes for all you .When the  "run  Scf"in
wien2k,the  " Stop error"  in Lapw1   displayed.What
does it mean?Thank  or what is its reason?
What should be done for eliminating it?
best wishes
H-Salehi
dept of physics
Ferdowsi university
Mashhad  IRAN
post boxs 1436
postcode 91775



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------------------------------

Date: Wed, 17 Jul 2002 15:56:05 +0200 (CEST)
From: =?iso-8859-1?q?Houda=20Imene?= <houda_imene@yahoo.fr>
Subject: [WIEN]: Re: 

====
=?iso-8859-1?q?Houda=20Imene?= <houda_imene@yahoo.fr>
submitted the following contribution:
====

- --0-830740164-1026914165=:11453
Content-Type: text/plain; charset=iso-8859-1
Content-Transfer-Encoding: 8bit


 May be you must give more details... the lapw1.error for example!
Regards
  hamid salehi <salehihamid@yahoo.com> a écrit : ====
hamid salehi 
submitted the following contribution:
====

Dear wien2k users;


with best wishes for all you .When the "run Scf"in
wien2k,the " Stop error" in Lapw1 displayed.What
does it mean?Thank or what is its reason?
What should be done for eliminating it?
best wishes
H-Salehi
dept of physics
Ferdowsi university
Mashhad IRAN
post boxs 1436
postcode 91775



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- ---------------------------------
Yahoo! Mail -- Une adresse @yahoo.fr gratuite et en français !

- --0-830740164-1026914165=:11453
Content-Type: text/html; charset=iso-8859-1
Content-Transfer-Encoding: 8bit

<P> May be you must give more details... the lapw1.error for example!
<P>Regards
<P>&nbsp; <B><I>hamid salehi &lt;salehihamid@yahoo.com&gt;</I></B> a écrit&nbsp;: 
<BLOCKQUOTE style="BORDER-LEFT: #1010ff 2px solid; MARGIN-LEFT: 5px; PADDING-LEFT: 5px">====<BR>hamid salehi <SALEHIHAMID@YAHOO.COM><BR>submitted the following contribution:<BR>====<BR><BR>Dear wien2k users;<BR><BR><BR>with best wishes for all you .When the "run Scf"in<BR>wien2k,the " Stop error" in Lapw1 displayed.What<BR>does it mean?Thank or what is its reason?<BR>What should be done for eliminating it?<BR>best wishes<BR>H-Salehi<BR>dept of physics<BR>Ferdowsi university<BR>Mashhad IRAN<BR>post boxs 1436<BR>postcode 91775<BR><BR><BR><BR>__________________________________________________<BR>Do You Yahoo!?<BR>Yahoo! Autos - Get free new car price quotes<BR>http://autos.yahoo.com<BR>====<BR>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at<BR>To (un)subscribe send mail to<BR>majordomo@zeus.theochem.tuwien.ac.at<BR>====</BLOCKQUOTE><p><br><hr size=1><a href="http://fr.mail.yahoo.com">Yahoo! Mail</a> -- Une adresse @yahoo.fr gratuite et en français !<br>
- --0-830740164-1026914165=:11453--
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------------------------------

Date: Wed, 17 Jul 2002 22:12:01 +0300
From: "B. Yanchitsky" <yan@im.imag.kiev.ua>
Subject: Re: [WIEN]: about monoclinic brillouin zone

====
"B. Yanchitsky" <yan@im.imag.kiev.ua>
submitted the following contribution:
====

"Dr. Sharat Chandra" wrote:
> 
> Dear Prof. Blaha
> 
> I have tried the CuV2O5 structure with the Cu atoms shifted a little from
> their actual positions but with Cu atoms having multiplicity 2. Even now I
> find that the XCrysden shows the BZ to be base centered Orthorhombic type
> rather than base centered monoclinic. I have also found that the struct
> file now has zero number of symmetry operations instead of the usual one.
> If you have any ideas about how to prepare the correct input file for this
> compound, I will be very grateful.
> 

Dear Sharat,

lapw.struct is correct (after x symmetry, *.struct_st file contains
2 operations as it should be.)
It is still being unclear for me what is your problem. If z is very small
(Z=0.10200000) and the cell has monoclinic symmetry,
then it would be a reasonable guess that z=0. with z=0
4b is transformed to 2a with mult=1 and no problem
with extremely small distance between atoms.

Regards,

Bogdan
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------------------------------

Date: Wed, 17 Jul 2002 23:57:07 +0200 (CEST)
From: Stefaan.Cottenier@fys.kuleuven.ac.be
Subject: Re: [WIEN]: band structure

====
Stefaan.Cottenier@fys.kuleuven.ac.be
submitted the following contribution:
====

> ====
> hamid salehi <salehihamid@yahoo.com>
> submitted the following contribution:
> ====
> 
> Dear wien users.
> Ihave started Band structure and in Xspaghetti-C, got
> this message "case.insp.1st line should started with
> ### what it the mean? and not derived band structure
> figure.

In wien2k, the format of the input file for spaghetti has changed compared to
wien97. You are using a wien97-file. Look for a template of the new case.insp in
SRC_templates.

Stefaan

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------------------------------

Date: Thu, 18 Jul 2002 10:17:58 -0500 (GMT)
From: "Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
Subject: Re: [WIEN]: about monoclinic brillouin zone

====
"Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
submitted the following contribution:
====


Dear Prof. Bogdan

My problem is that I am not able to get the correct base centered
monoclinic BZ with this file. Instead I get a BZ which looks like that of
base centered Orthorhombic. Base centered Monoclinic has a parallopiped BZ
whereas base centered Orthorhombic has one which looks like a hexagonal
traversed along the z direction (Bradley and Kracknell). I want to know
how this problem can be solved, because if I do the band structure
calculations with the base centered monoclinic klist, after running
spaghetti I get a band structure with gaps in between different
directions. If I just use the klist generated by XCrysden, will it be
correct band structure?

Regards
Sharat Chandra

> lapw.struct is correct (after x symmetry, *.struct_st file contains
> 2 operations as it should be.)
> It is still being unclear for me what is your problem. If z is very small
> (Z=0.10200000) and the cell has monoclinic symmetry,
> then it would be a reasonable guess that z=0. with z=0
> 4b is transformed to 2a with mult=1 and no problem
> with extremely small distance between atoms.


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------------------------------

End of wien-digest V2002 #27
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #28
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
Errors-To: owner-wien-digest@theochem.tuwien.ac.at
Precedence: bulk


wien-digest         Thursday, July 25 2002         Volume 2002 : Number 028




----------------------------------------------------------------------

Date: Thu, 18 Jul 2002 16:28:08 +1000
From: chen0130@flinders.edu.au
Subject: [WIEN]: Generating a k-list

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Dear Wien users,

I have a very elementary question, I have no idea how to generate a k-list
through xcrysden,

I was wondering if someone could point me i some direction as to resources, I
have a Li2O slab, and the BZ is a rectangular prism, I am not sure what process
is required to select points in this 3D zone,

Thanks!

Cheng Chen
honours student
Flinders University of South Australia  


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------------------------------

Date: Fri, 19 Jul 2002 12:13:56 +0100 (BST)
From: pauhar@chem.gla.ac.uk
Subject: [WIEN]: Unoccupied DOS

====
pauhar@chem.gla.ac.uk
submitted the following contribution:
====

Dear Wien Users,

I am using wien97 to calculate a supercell with a core-hole. When l look at the 
unoccupied DOS it is calculated up to 18eV, whereas l am able to investigate up 
to 40 or 50 eV beyond the fermi level if the calculation is done using a normal 
unit cell in the .struct file. I have increased the value of Emax set in .in1 
and .klist but this makes no difference. Also the value of Emax in .int is set 
to the lowest energy of the highest band in .outputt to make sure that there is 
no problem with the range being plotted. Is there some other parameter that l 
could alter which is limiting the calculation?

Thanks in advance for your help,
Paula
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------------------------------

Date: Fri, 19 Jul 2002 15:08:18 +0200
From: Florent Boucher <Florent.Boucher@cnrs-imn.fr>
Subject: Re: [WIEN]: Unoccupied DOS

====
Florent Boucher <Florent.Boucher@cnrs-imn.fr>
submitted the following contribution:
====

Dear Paula,
it seems that your problem is directly corralated to the value of NUME. 
This a parameter for the compilation and by default the value is 300 
(for WIEN97). It defines the maximum number of eigen velues that can be 
computed.
Using siteconfig your can increase it and then recompile  WIEN97.
Regards
Florent

pauhar@chem.gla.ac.uk wrote:

>====
>pauhar@chem.gla.ac.uk
>submitted the following contribution:
>====
>
>Dear Wien Users,
>
>I am using wien97 to calculate a supercell with a core-hole. When l look at the 
>unoccupied DOS it is calculated up to 18eV, whereas l am able to investigate up 
>to 40 or 50 eV beyond the fermi level if the calculation is done using a normal 
>unit cell in the .struct file. I have increased the value of Emax set in .in1 
>and .klist but this makes no difference. Also the value of Emax in .int is set 
>to the lowest energy of the highest band in .outputt to make sure that there is 
>no problem with the range being plotted. Is there some other parameter that l 
>could alter which is limiting the calculation?
>
>Thanks in advance for your help,
>Paula
>====
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>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
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>

- -- 
 --------------------------------------------------------------------------
| Florent BOUCHER                    |                                     |
| Institut des Matériaux Jean Rouxel | Mailto:Florent.Boucher@cnrs-imn.fr  |
| 2, rue de la Houssinière           | Phone: (33) 2 40 37 39 24           |
| BP 32229                           | Fax:   (33) 2 40 37 39 95           |
| 44322 NANTES CEDEX 3 (FRANCE)      | http://www.cnrs-imn.fr              |
 --------------------------------------------------------------------------



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------------------------------

Date: Sat, 20 Jul 2002 00:02:36 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Generating a k-list

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I have a very elementary question, I have no idea how to generate a k-list
> through xcrysden,
>
> I was wondering if someone could point me i some direction as to resources, I
> have a Li2O slab, and the BZ is a rectangular prism, I am not sure what process
> is required to select points in this 3D zone,

If you do a slab, usually this means you want to simulate a surface.
A surface has only 2D periodicity and thus a 2D BZ.

In xcrysden your BZ should be very small along the z direction (when a
cell is large in direct space, it is very small in reciprocal space.)
First click on "display reciprocal lattice vectors".
Just click at the red dot (this is the center of the BZ, i.e. Gamma) and
then at some other points at the border of the BZ. This will define lines
along which the bands are calculated.
There is no "rule" which directions to go. Either you want to compare with
a destinct experiment and thus choose the experimental directions, or just
go in 100 and  110 direction. It also depends on symmetry,....

Regards

                                     P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Sat, 20 Jul 2002 00:11:33 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: about mini

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> > > Now I try to use min_lapw to optimize the internal parameter of
> crystal. I
> > > have two questions.
> > >
> > > (1) According the space-group symmetry, the position is (0.5, 0.25, x),
> >Most likely (local rotations?), but it is not necessary to restrict the
> >other positions to zero (since they have no forces anyway)
>
> If they have forces, it means the structure file is wrong?

Usually 0.5 or 0.25 means  a special position in a spacegroup and these
positions must not change. (Of course x could still be a free parameter
and x=0.5 is just an experimental estimate or so. You must check your
specific spacegroup.).

If you have a local rotation matrix different from the unit matrix (see
your struct file), than it is posible to have forces in other directions.
But normally I would say: Yes if you have forces in x or y direction,
something is wrong in your struct file....

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 22 Jul 2002 16:37:24 +1000
From: chen0130@flinders.edu.au
Subject: Re: [WIEN]: Generating a k-list

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Dear Prof Blaha,

Thanks so much for your valuable advice. I am now comfortable to work with
generating a k -list!

My conventional BZ is the same as the primitive BZ, I was seeking some advice
about how many k-paths (points) is 'reasonable'...

Thanks for the starting point!

Cheng  

Quoting Peter Blaha <pblaha@theochem.tuwien.ac.at>:

> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> > I have a very elementary question, I have no idea how to generate a
> k-list
> > through xcrysden,
> >
> > I was wondering if someone could point me i some direction as to resources,
> I
> > have a Li2O slab, and the BZ is a rectangular prism, I am not sure what
> process
> > is required to select points in this 3D zone,
> 
> If you do a slab, usually this means you want to simulate a surface.
> A surface has only 2D periodicity and thus a 2D BZ.
> 
> In xcrysden your BZ should be very small along the z direction (when a
> cell is large in direct space, it is very small in reciprocal space.)
> First click on "display reciprocal lattice vectors".
> Just click at the red dot (this is the center of the BZ, i.e. Gamma) and
> then at some other points at the border of the BZ. This will define lines
> along which the bands are calculated.
> There is no "rule" which directions to go. Either you want to compare with
> a destinct experiment and thus choose the experimental directions, or just
> go in 100 and  110 direction. It also depends on symmetry,....
> 
> Regards
> 
>                                      P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
> http://www.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
> 
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 
> 



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------------------------------

Date: Mon, 22 Jul 2002 16:51:48 +0200 (MEST)
From: Pio =?ISO-8859-1?Q?B=E4ttig?= <baettigp@gmx.net>
Subject: [WIEN]: Problems compiling Wien2k with IFC

====
Pio =?ISO-8859-1?Q?B=E4ttig?= <baettigp@gmx.net>
submitted the following contribution:
====

Dear Wien-users

I encountered a small problem while trying to compile wien2k_02 with IFC 6.0
on a PIII/800. I obtain the following errors. I retried to compile on
another machine (AMD Duron 1200), with the same effects.
I managed to compile it without errors on a DEC Alpha with Tru64 and the
Compaq compilers.
Thank you very much for any hints
Pio Bättig



done.

Compile messages for each SRC_* directory can be found in the
file "compile.msg".

Compile time errors (if any) were:
SRC_lapw3/compile.msg:Error FCE22 : Module KGRID USEd by subroutine RECPR in
work.pc not found
SRC_lapw3/compile.msg:Error 24 at (25:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 24 at (25:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 24 at (25:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 24 at (41:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 24 at (41:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 395 at (113:recpr.f) : This entity is not an
array and must not be subscripted
SRC_lapw3/compile.msg:Error 43 at (115:recpr.f) : Label 6 refers to a
non-executable statement at (114:recpr.f)
SRC_lapw3/compile.msg:Error 43 at (115:recpr.f) : Label 6 refers to a
non-executable statement at (111:recpr.f)
SRC_lapw3/compile.msg:Error 65 at (115:recpr.f) : This statement cannot
terminate a DO loop
SRC_lapw3/compile.msg:Error 24 at (115:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 24 at (115:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 24 at (115:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 43 at (116:recpr.f) : Label 7 refers to a
non-executable statement at (99:recpr.f)
SRC_lapw3/compile.msg:Error 43 at (116:recpr.f) : Label 7 refers to a
non-executable statement at (83:recpr.f)
SRC_lapw3/compile.msg:Error 24 at (116:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 24 at (116:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 43 at (119:recpr.f) : Label 8 refers to a
non-executable statement at (118:recpr.f)
SRC_lapw3/compile.msg:Error 65 at (119:recpr.f) : This statement cannot
terminate a DO loop
SRC_lapw3/compile.msg:Error 24 at (119:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 24 at (119:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 24 at (119:recpr.f) : syntax error
SRC_lapw3/compile.msg:Error 395 at (137:recpr.f) : This entity is not an
array and must not be subscripted
SRC_lapw3/compile.msg:Error 395 at (149:recpr.f) : This entity is not an
array and must not be subscripted
SRC_lapw3/compile.msg:Error 395 at (151:recpr.f) : This entity is not an
array and must not be subscripted
SRC_lapw3/compile.msg:25 Errors
SRC_lapw3/compile.msg:make[1]: *** [recpr.o] Error 1
SRC_lapw3/compile.msg:make: *** [complex] Error 2

Here the full messages from SRC_lapw3/compile.msg:
   external subroutine RECPR
Error FCE22 : Module KGRID USEd by subroutine RECPR in work.pc not found

      allocate (absk(nkd+1), kzz(3,nkd+1),inst(nkd))
                ^
Error 24 at (25:recpr.f) : syntax error

      allocate (absk(nkd+1), kzz(3,nkd+1),inst(nkd))
                        ^
Error 24 at (25:recpr.f) : syntax error

      allocate (absk(nkd+1), kzz(3,nkd+1),inst(nkd))
                           ^
Error 24 at (25:recpr.f) : syntax error

      allocate ( TAUK(NFK),KREC(3,NFK))                            
                 ^
Error 24 at (41:recpr.f) : syntax error

      allocate ( TAUK(NFK),KREC(3,NFK))                            
                          ^
Error 24 at (41:recpr.f) : syntax error
   entry RECPR2

      ABSK(NJJ+1)=ABSK(NJJ)                                             
      ^
Error 395 at (113:recpr.f) : This entity is not an array and must not be
subscripted

  6   KZZ(N,NJJ+1)=KZZ(N,NJJ)                                           
  ^
Error 43 at (115:recpr.f) : Label 6 refers to a non-executable statement at
(114:recpr.f)
  ^
Error 43 at (115:recpr.f) : Label 6 refers to a non-executable statement at
(111:recpr.f)
      ^
Error 65 at (115:recpr.f) : This statement cannot terminate a DO loop
      ^
Error 24 at (115:recpr.f) : syntax error

  6   KZZ(N,NJJ+1)=KZZ(N,NJJ)                                           
           ^
Error 24 at (115:recpr.f) : syntax error

  6   KZZ(N,NJJ+1)=KZZ(N,NJJ)                                           
               ^
Error 24 at (115:recpr.f) : syntax error

   7  ABSK(J)=ABSM                                                      
   ^
Error 43 at (116:recpr.f) : Label 7 refers to a non-executable statement at
(99:recpr.f)
   ^
Error 43 at (116:recpr.f) : Label 7 refers to a non-executable statement at
(83:recpr.f)
      ^
Error 24 at (116:recpr.f) : syntax error

   7  ABSK(J)=ABSM                                                      
            ^
Error 24 at (116:recpr.f) : syntax error

   8  KZZ(N,J)=IM(N)                                                    
   ^
Error 43 at (119:recpr.f) : Label 8 refers to a non-executable statement at
(118:recpr.f)
      ^
Error 65 at (119:recpr.f) : This statement cannot terminate a DO loop
      ^
Error 24 at (119:recpr.f) : syntax error

   8  KZZ(N,J)=IM(N)                                                    
           ^
Error 24 at (119:recpr.f) : syntax error

   8  KZZ(N,J)=IM(N)                                                    
             ^
Error 24 at (119:recpr.f) : syntax error

      INST(I)=NST                                                       
      ^
Error 395 at (137:recpr.f) : This entity is not an array and must not be
subscripted

      TAUK(IND)=TAUP(JJ)
      ^
Error 395 at (149:recpr.f) : This entity is not an array and must not be
subscripted

        KREC(JJJ,IND)=ISTM(JJJ,JJ)  
        ^
Error 395 at (151:recpr.f) : This entity is not an array and must not be
subscripted

25 Errors
compilation aborted for recpr.f (code 1)
make[1]: *** [recpr.o] Error 1
make[1]: Leaving directory `/mnt/1/home/baettigp/wien2k_02/SRC_lapw3'
make: *** [complex] Error 2

- -- 
GMX - Die Kommunikationsplattform im Internet.
http://www.gmx.net

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------------------------------

Date: Mon, 22 Jul 2002 17:12:52 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: [WIEN]: Re: 

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Mr. Salehi,

this error usually comes when lapw1 has exited with an error... - then 
the error message is in [up|dn]lapw1.error . Alternatively, there is a 
problem with the compilation. Insert "status='replace'" in "errclr.f", 
i.e., replace

OPEN (99,FILE=FNAME)

by

OPEN (99,FILE=FNAME,STATUS='REPLACE')

and recompile. This removes that error on some sun machines.

Best regards,
Torsten Andersen.

hamid salehi wrote:

>====
>hamid salehi <salehihamid@yahoo.com>
>submitted the following contribution:
>====
>
>Dear wien2k users;
>
>
>with best wishes for all you .When the  "run  Scf"in
>wien2k,the  " Stop error"  in Lapw1   displayed.What
>does it mean?Thank  or what is its reason?
>What should be done for eliminating it?
>best wishes
>H-Salehi
>dept of physics
>Ferdowsi university
>Mashhad  IRAN
>post boxs 1436
>postcode 91775
>
>
>
>__________________________________________________
>Do You Yahoo!?
>Yahoo! Autos - Get free new car price quotes
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>====
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>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Tue, 23 Jul 2002 13:25:45 +0800 (CST)
From: music@theory.issp.ac.cn
Subject: [WIEN]: Stoner parameter

====
music@theory.issp.ac.cn
submitted the following contribution:
====


Dear wien users,
   I want to calculate stoner parameter in wien2k program ?
   How can I do it ?
   Could anyone help me ?  many thanks !!!!!
    

- -- 





sincerely yours 

Ying.X


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------------------------------

Date: Tue, 23 Jul 2002 10:10:30 -0400
From: Igor Mazin <mazin@dave.nrl.navy.mil>
Subject: Re: [WIEN]: Stoner parameter

====
Igor Mazin <mazin@dave.nrl.navy.mil>
submitted the following contribution:
====

The only way is to make fixed-spin-moment calculations and then fit them
with the stoner formula,
Delta E=(M^2/4)(1/N-I), where N is the nonmagnetic DOS per spin,
M is the fixed spin moment. I found that for small M's, M \lessim 0.1,
the Energy calculated by WIEN2k is noisy (as opposed to my earlier 
experience with WIEN-97,
but I have not done systematic tests), so I either use the field,
that is, EF_up-EF_dn, which is the derivative of E, namely
(M/2)(1/N-I), or use Andersen's extended Stoner formula (see Krasko,
Phys. Rev. B, around 1985, and refs therein), which allows
to use M's up to 1 uB.

Good luck,
Igor

P.S. Note I always speak about the TOTAL Stoner factor, which for compounds
is defined as (I_A N_A^2+I_B N_B^2+...)/N^2

At 13:25 7/23/2002 +0800, you wrote:
>====
>music@theory.issp.ac.cn
>submitted the following contribution:
>====
>
>
>Dear wien users,
>    I want to calculate stoner parameter in wien2k program ?
>    How can I do it ?
>    Could anyone help me ?  many thanks !!!!!
>
>
>--
>
>
>
>
>
>sincerely yours
>
>Ying.X
>
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====

*****************************************************************************
Igor Mazin, NRL, code 6391, 4555 Overlook Ave, Was., DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; e-mail mazin@nrl.navy.mil
Home Page (under construction) http://cst-www.nrl.navy.mil/~mazin
*****************************************************************************


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------------------------------

Date: Tue, 23 Jul 2002 16:56:57 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Problems compiling Wien2k with IFC

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I encountered a small problem while trying to compile wien2k_02 with IFC 6.0
> on a PIII/800. I obtain the following errors. I retried to compile on
> another machine (AMD Duron 1200), with the same effects.

> Compile time errors (if any) were:
> SRC_lapw3/compile.msg:Error FCE22 : Module KGRID USEd by subroutine RECPR in
> work.pc not found
> SRC_lapw3/compile.msg:Error 24 at (25:recpr.f) : syntax error

Change into SR_lapw3, type
make clean
make
make clean
make complex

It should do the job.

Regards

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------------------------------

Date: Tue, 23 Jul 2002 21:03:01 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: [WIEN]: Intel fortran compiler on a cluster

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====

Dear Wien2k Experts,

I am about to obtain a new linux cluster and was wondering if someone
could comment on the quality of the Intel compiler. I have only been
running simple cases on a single cpu using the Portland compiler until
now. Do the perfomance gains from parallelization depend on the compiler
(I know next to nothing about practical parallel computing except what was
taught in my comp. sci. theory class).  If the Portland compiler is still
the better option, do we need to purchase one of their "cluster" versions?

Thank you for any responses,  Fred

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------------------------------

Date: Wed, 24 Jul 2002 10:09:03 -0500 (GMT)
From: "Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
Subject: Re: [WIEN]: Problems compiling Wien2k with IFC

====
"Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
submitted the following contribution:
====

Hi

In addition to make clean, you will need to delete the work.pc, work.pcl
and *.d files too before running make complex command.

regards
Sharat Chandra

> > I encountered a small problem while trying to compile wien2k_02 with IFC 6.0
> > on a PIII/800. I obtain the following errors. I retried to compile on
> > another machine (AMD Duron 1200), with the same effects.
> 
> > Compile time errors (if any) were:
> > SRC_lapw3/compile.msg:Error FCE22 : Module KGRID USEd by subroutine RECPR in
> > work.pc not found
> > SRC_lapw3/compile.msg:Error 24 at (25:recpr.f) : syntax error
> 
> Change into SR_lapw3, type
> make clean
> make
> make clean
> make complex
> 
> It should do the job.
> 
> Regards
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 
> 


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------------------------------

Date: Wed, 24 Jul 2002 09:31:26 +0200 (CEST)
From: Stefaan.Cottenier@fys.kuleuven.ac.be
Subject: Re: [WIEN]: Intel fortran compiler on a cluster

====
Stefaan.Cottenier@fys.kuleuven.ac.be
submitted the following contribution:
====

> ====
> Fred Nastos <nastos@physics.utoronto.ca>
> submitted the following contribution:
> ====
> 
> I am about to obtain a new linux cluster and was wondering if someone
> could comment on the quality of the Intel compiler. I have only been
> running simple cases on a single cpu using the Portland compiler until
> now. Do the perfomance gains from parallelization depend on the
> compiler (I know next to nothing about practical parallel computing except 
> what was taught in my comp. sci. theory class).  If the Portland compiler 
> is still the better option, do we need to purchase one of their "cluster"
> versions?

Dear Fred,

For this problem, you can even forget what has been taught in your computer 
classes. It's easier than that. In order to use k-point parallelization with 
wien2k, you can use any serial (f90) compiler. Wien2k itself takes care of 
the "parallelization": it distributes the k-points over the different machines, 
where they are all treated by *serial* code (this can be done as in order to do 
the diagonalization for 1 k-point, no information about the others is needed). 
Afterwards, all individual results are pasted together. This scheme works as 
long as you have a reasonably large number of k-points (at least as many as the 
number of computers you have). If you have very large unit cells that need only 
a few k-points, than it becomes useful to consider true parallelization (where 
the diagonalization of 1 matrix is distributed over different machines, which 
cannot operate independently any more). This is possible in wien2k, but you 
need MPI installed (and have fast communication). Most likely, you will not 
need this. In any case, the regular (serial) Portland compiler will do the job 
(although I hear rumours that the free Intel f90 is currently faster).

Stefaan
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------------------------------

Date: Wed, 24 Jul 2002 10:50:44 +0200 (CEST)
From: =?iso-8859-1?q?jonny=20sham?= <sham_jonny@yahoo.fr>
Subject: [WIEN]: problem in struct of alloy

====
=?iso-8859-1?q?jonny=20sham?= <sham_jonny@yahoo.fr>
submitted the following contribution:
====

please help me to understand why to generate the
case.struct for the alloy materials.

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------------------------------

Date: Thu, 25 Jul 2002 03:41:15 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: [none]

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====

Dear wien users:
    I want to calcualte system like AB, where A is a f-element and B is 
p-element,
 because A has localized f orbit, so I want to add ORB to the system. But 
there are some
 questions I cann't solve
  
   My procedure is list below:
      
       1:  run init_lapw.
       2:  run initso_lapw
       3:  copy case.indm and case.inorb to my case directory, and modified 
them 
       4:  run runsp_lapw -orb -so

 there is error after the lapw2
        
         ............
        >>:lapw2 -c -dn -so
        >>: stop error

but there are no error can be find in my error files. It is obvious that 
the lapwdm
 can't been executed. I have also execute the fourth step like these two:
         runsp_lapw -orb
         runsp_lapw -so
they are all ok. So it is not the problem of input file. I don't know how 
to solve this
problem.


now I give som input files, I hope someone  can help me.

   (My system has a spacegroup Fm3m, 48 kinds of operation)

after the normal init_lapw:
   
 case.in2:
         
           ToT
              -9.0  17.0 0.50 0.05
           TETRA   0.000
           0 0 4 0 4 4 6 0 6 4----------------------------- line 4
           0 0 4 0 4 4 6 0 6 4----------------------------- line5
         FILE    FILE/NOFILE  Write recrplist

case.klist:
   
           1  0  0  0  4 1.0 -7.0 1.5---->
           2  1  1 -1  4 8.0
           3  2  2 -2  4 4.0
           4  2  0  0  4 6.0
           5  3  1 -1  4 24.0
           6  4  2 -2  4 12.0
           7  4  0  0  4 3.0
           8  4  2  0  4 6.0

after initso_lapw ,
  
 case.in1 : I change emax from 1.5 to 8.5(I believe the SO is strong) 

 case.in2c(case.in2 doesn't change,in SO it will no use) :
           Line 4--------------> 0 0 2 0 4 0 4 4 6 0 6 4
           Line 5--------------> 0 0 2 0 4 0 4 4 6 0 6 4

case.inso:

          WFFIL
              4  1  0
             -10.000  1.5000---->if this energy also change according to 
case.in1?
              0. 0. 1------------>magnetization direction(001)
              1
              2  -4.97 0.005---->according to userguide ,these energy 
parameter 
                                  should agree with the energy parameter of 
p-orbit 
                                 in case.in1,but what : just El for P or 
E_LO for P? 
 
              1  1----------->p-element is my first atom and I don't want 
to add SO on it

case.indm:
          
        -9
         1
         2  1  3-------------------> f-element is my second atom, I want to 
add ORB on its f electron 
         0 0 

case.inorb is empty, then I change case.inorb like this:
      
         1  1  0
        PRATT  1.0
         2  1  3------------>f-element f orbit
         0
           0.59  0.07

case.klist is the same as above.(but if I run initso_lapw again , I found 
the case.klist 
will change to follow, is this a bug?)
        1  0  0  0  4 1.0 -7.0 1.5   100k div(4x4x4)-->Does this also 
should be 8.5 like case.in1?
        2  1  1 -1  4 8.0
        3  2  2 -2  4 4.0
        4  2  0  0  4 4.0
        5  3  1 -1  4 16.0
        6  4  2 -2  4 8.0
        7  4  0  0  4 2.0
        8  0  0  2  4 2.0
        9  2  2  0  4 4.0
       10  3  3 -1  4 8.0
       11  4  2  0  4 4.0
       12  4  0  2  4 2.0
       13  0  0  4  4 1.0

case.struct file is still Cubic ,but the kinds of operation reduce from
 48 to 16(accoring to the userguide, the Cubic system with magnetization 
direction (001) should change to tetragonal, why in my case still Cubic 
system? In my structure a=b=c)

and another question: because my system has inversion symmetry , after 
initso_lapw , 
it also preserve inversion, so in my case , the input file should be 
case.in1 and case.in2c,
but when during initso_lapw , at rerun kgen, it always show the messages:

   cp: can not stat "case.in1c_so", no such file or directory
   cp: can not stat "case.in2c_so", no such file or directory

but the case.in1 and case.in2c can stil be created

So I hope some one can help me, I was confused by these all

    
           
    
       

          
    


















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------------------------------

Date: Thu, 25 Jul 2002 14:07:15 +0200 (CEST)
From: Stefaan.Cottenier@fys.kuleuven.ac.be
Subject: [WIEN]: textbook: correction

====
Stefaan.Cottenier@fys.kuleuven.ac.be
submitted the following contribution:
====

Dear Wien-users,

Something got mixed up in section 6.1 of "DFT and the family of (L)APW 
methods" (*). In this section, some output lines where referring to a different 
example, used in a trial version of the text. It has been corrected now. The 
new version carries number 1.03 in the header of the odd pages.

Thanks to Michel Jaouen for indicating the problem, and sorry to the people 
that have been searching in vain for what they where doing wrong...

Stefaan

(*) http://www.wien2k.at/reg_user/textbooks
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------------------------------

End of wien-digest V2002 #28
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #29
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
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Precedence: bulk


wien-digest         Thursday, August 1 2002         Volume 2002 : Number 029




----------------------------------------------------------------------

Date: Thu, 25 Jul 2002 14:07:49 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: [WIEN]: Re: your mail

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>     I want to calcualte system like AB, where A is a f-element and B is
> p-element,
>  because A has localized f orbit, so I want to add ORB to the system. But
> there are some
>  questions I cann't solve
>
>    My procedure is list below:
>
>        1:  run init_lapw.
>        2:  run initso_lapw
>        3:  copy case.indm and case.inorb to my case directory, and modified
> them
>        4:  run runsp_lapw -orb -so
>
>  there is error after the lapw2
>
>          ............
>         >>:lapw2 -c -dn -so
>         >>: stop error
>
> but there are no error can be find in my error files. It is obvious that
> the lapwdm
>  can't been executed. I have also execute the fourth step like these two:
>          runsp_lapw -orb
>          runsp_lapw -so
> they are all ok. So it is not the problem of input file. I don't know how

The reason is quite simply: SO calculation require complex lapw2 and
lapwdm, so you are missing a case.indmc file. Just copy your indm file to
indmc.

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Thu, 25 Jul 2002 09:36:50 -0400
From: Igor Mazin <mazin@dave.nrl.navy.mil>
Subject: [WIEN]: Re: 

====
Igor Mazin <mazin@dave.nrl.navy.mil>
submitted the following contribution:
====

A few comments to this point:

1) With magnetism and SO, your symmetry has to be broken. Just make c.ne.a,b
slightly, it will do the job. Correspondingly, if you want to get the right
orbital moment, you have to use the complex version of lapw1 (in Wien2k.
Apparently Wien2k_02 is organized differently)
2) I have a neat script to create indm and inorb. See
http://cst-www.nrl.navy.mil/~mazin/, scroll down to
CCMS WIEN LAPW tips.
3) There can be different opinions, but I am very confident that for
f-electrons you want to use the localized version of LDA+U, nicknamed
SIC in WIEN2k.
4) U for f-electrons is large, at least 0.4 Ry, therefore different
valence state of the rare earth may be stabilized in LDA+U. Be careful
to find the right ground state. The -orbc option is great for
steering the calculations into a given valence state.
5) I can send you input files for SmZn (a well behaving calculation), if you
want to compare with yours.

Good luck,
Igor


====


*****************************************************************************
Igor Mazin, NRL, code 6391, 4555 Overlook Ave, Was., DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; e-mail mazin@nrl.navy.mil
Home Page (under construction) http://cst-www.nrl.navy.mil/~mazin
*****************************************************************************


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Date: Thu, 25 Jul 2002 18:24:48 +0200 (MEST)
From: Pio =?ISO-8859-1?Q?B=E4ttig?= <baettigp@gmx.net>
Subject: [WIEN]: Calculation crashes with LAPW2

====
Pio =?ISO-8859-1?Q?B=E4ttig?= <baettigp@gmx.net>
submitted the following contribution:
====

Dear Wien users

I am trying to calculate a ferromagnetically coupled system,
a perovskite in which the small cations are alternatingly
Fe and Cr (resulting in (111)planes) with Wien2k_02
For the atomic calculations I chose the PBE96 XC and -6.0 eV to separate
core
and valence states. 
I chose RKmax=8.0, 256 kpoints, spinpolarized, everything else was standard.
The .struct file looks as follows:

Title                                                                       
  
F   LATTICE,NONEQUIV. ATOMS: 4 225 Fm-3m                                    
  
MODE OF CALC=RELA unit=bohr                                                 
  
 14.739900 14.739900 14.739900 90.000000 90.000000 90.000000                
  
ATOM=  1: X=0.75000000 Y=0.25000000 Z=0.25000000
          MULT= 2          ISPLIT= 2
       1: X=0.25000000 Y=0.75000000 Z=0.75000000
Bi1        NPT=  781  R0=0.00000500 RMT=    1.8000   Z: 83.0                
  
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=  2: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT= 2
Fe1        NPT=  781  R0=0.00005000 RMT=    1.8000   Z: 26.0                
  
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=  3: X=0.50000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT= 2
Cr1        NPT=  781  R0=0.00005000 RMT=    1.8000   Z: 24.0                
  
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -4: X=0.50000000 Y=0.25000000 Z=0.00000000
          MULT= 6          ISPLIT=-2
      -4: X=0.50000000 Y=0.75000000 Z=0.00000000
      -4: X=0.00000000 Y=0.50000000 Z=0.25000000
      -4: X=0.00000000 Y=0.50000000 Z=0.75000000
      -4: X=0.25000000 Y=0.00000000 Z=0.50000000
      -4: X=0.75000000 Y=0.00000000 Z=0.50000000
O 1        NPT=  781  R0=0.00010000 RMT=    1.8000   Z:  8.0                
  
LOCAL ROT MATRIX:    0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
                     1.0000000 0.0000000 0.0000000
  48      NUMBER OF SYMMETRY OPERATIONS
.
.
.

I checked the geometry in xcrysdens and everything should be correct.
The .inst looks as follows:

Bi
Xe 7 5
4, 3,3.0  N
4, 3,3.0  N
4,-4,4.0  N
4,-4,4.0  N
5, 2,2.0  N
5, 2,2.0  N
5,-3,3.0  N
5,-3,3.0  N
6,-1,1.0  N
6,-1,1.0  N
6, 1,1.0  N
6, 1,1.0  N
6,-2,1.0  N
6,-2,0.0  N
Fe
Ar 3 5
3, 2,2.0  N
3, 2,2.0  N
3,-3,3.0  N
3,-3,0.0  N
4,-1,1.0  N
4,-1,0.0  N
Cr
Ar 3 5
3, 2,2.0  N
3, 2,1.0  N
3,-3,2.0  N
3,-3,0.0  N
4,-1,1.0  N
4,-1,0.0  N
O
He 3 5
2,-1,1.0  N
2,-1,1.0  N
2, 1,1.0  N
2, 1,1.0  N
2,-2,2.0  N
2,-2,0.0  N
****
****         END of input (instgen_lapw)

The SCF breaks down in LAPW2 with the following error message:

forrtl: severe (64): input conversion error, unit 1001, file
/usr/tmp/baettigp/b2.helpup031
   0: __FINI_00_remove_gp_range [0x3ff81a6c374]
   1: __FINI_00_remove_gp_range [0x3ff81a6c8f4]
   2: __FINI_00_remove_gp_range [0x3ff81a93b84]
   3: outp_ [outp.f: 179, 0x120068b30]
   4: l2main_ [l2main_tmp_.F: 1230, 0x12005f7a8]
   5: lapw2_ [lapw2_tmp_.F: 465, 0x120064c18]
   6: main [for_main.c: 203, 0x12007e32c]
   7: __start [0x1200084c8]

In b2.helpup031 are some lines as the following:

 BAND#   8  E= -1.47073  WEIGHT= 0.0046296
  L= 0   50.00000  ********** 18741.993********************-18658.372
  L= 1    0.00000       0.000     0.000     0.000     0.000     0.000
  L= 2    0.00000       0.000     0.000     0.000     0.000     0.000
  D-EG:   0.00000       0.000     0.000     0.000     0.000     0.000
 D-T2G:   0.00000       0.000     0.000     0.000     0.000     0.000
  L= 3    0.00000       0.000     0.000     0.000     0.000     0.000
  L= 4    0.00000       0.000     0.000     0.000     0.000     0.000
  L= 5    0.00000       0.000     0.000     0.000     0.000     0.000
  L= 6    0.00000       0.000     0.000     0.000     0.000     0.000
  BAND#   9  E= -1.47073  WEIGHT= 0.0046296
  L= 0   50.00000  ********** 18741.993********************-18658.371

I can run the testcase (eg TiO2), and it converges:
    cycle 3 	(18/18 to go)
...
>   mixer	(15:19:19) 0.82u 0.28s 0:01 99% 0+50k 0+183io 0pf+0w
:ENERGY convergence:  1 0.0001 .0000040000000000


I would be grateful for any hint.

Thank you very much

Kind regards

Pio Bättig

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GMX - Die Kommunikationsplattform im Internet.
http://www.gmx.net

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Date: Fri, 26 Jul 2002 15:27:16 +0200 (CEST)
From: Georg Madsen <gmadsen@zeus.theochem.tuwien.ac.at>
Subject: [WIEN]: Re: your mail (Yue Hai)

====
Georg Madsen <gmadsen@zeus.theochem.tuwien.ac.at>
submitted the following contribution:
====

>        1:  run init_lapw.
>        2:  run initso_lapw
>        3:  copy case.indm and case.inorb to my case directory, and modified 
> them 
>        4:  run runsp_lapw -orb -so
> 
>  there is error after the lapw2
>         
>          ............
>         >>:lapw2 -c -dn -so
>         >>: stop error
Have you copied your in2 file to in2c?

 Georg

> 
> but there are no error can be find in my error files. It is obvious that 
> the lapwdm
>  can't been executed. I have also execute the fourth step like these two:
>          runsp_lapw -orb
>          runsp_lapw -so
> they are all ok. So it is not the problem of input file. I don't know how 
> to solve this
> problem.
> 
> 
> now I give som input files, I hope someone  can help me.
> 
>    (My system has a spacegroup Fm3m, 48 kinds of operation)
> 
> after the normal init_lapw:
>    
>  case.in2:
>          
>            ToT
>               -9.0  17.0 0.50 0.05
>            TETRA   0.000
>            0 0 4 0 4 4 6 0 6 4----------------------------- line 4
>            0 0 4 0 4 4 6 0 6 4----------------------------- line5
>          FILE    FILE/NOFILE  Write recrplist
> 
> case.klist:
>    
>            1  0  0  0  4 1.0 -7.0 1.5---->
>            2  1  1 -1  4 8.0
>            3  2  2 -2  4 4.0
>            4  2  0  0  4 6.0
>            5  3  1 -1  4 24.0
>            6  4  2 -2  4 12.0
>            7  4  0  0  4 3.0
>            8  4  2  0  4 6.0
> 
> after initso_lapw ,
>   
>  case.in1 : I change emax from 1.5 to 8.5(I believe the SO is strong) 
> 
>  case.in2c(case.in2 doesn't change,in SO it will no use) :
>            Line 4--------------> 0 0 2 0 4 0 4 4 6 0 6 4
>            Line 5--------------> 0 0 2 0 4 0 4 4 6 0 6 4
> 
> case.inso:
> 
>           WFFIL
>               4  1  0
>              -10.000  1.5000---->if this energy also change according to 
> case.in1?
>               0. 0. 1------------>magnetization direction(001)
>               1
>               2  -4.97 0.005---->according to userguide ,these energy 
> parameter 
>                                   should agree with the energy parameter of 
> p-orbit 
>                                  in case.in1,but what : just El for P or 
> E_LO for P? 
>  
>               1  1----------->p-element is my first atom and I don't want 
> to add SO on it
> 
> case.indm:
>           
>         -9
>          1
>          2  1  3-------------------> f-element is my second atom, I want to 
> add ORB on its f electron 
>          0 0 
> 
> case.inorb is empty, then I change case.inorb like this:
>       
>          1  1  0
>         PRATT  1.0
>          2  1  3------------>f-element f orbit
>          0
>            0.59  0.07
> 
> case.klist is the same as above.(but if I run initso_lapw again , I found 
> the case.klist 
> will change to follow, is this a bug?)
>         1  0  0  0  4 1.0 -7.0 1.5   100k div(4x4x4)-->Does this also 
> should be 8.5 like case.in1?
>         2  1  1 -1  4 8.0
>         3  2  2 -2  4 4.0
>         4  2  0  0  4 4.0
>         5  3  1 -1  4 16.0
>         6  4  2 -2  4 8.0
>         7  4  0  0  4 2.0
>         8  0  0  2  4 2.0
>         9  2  2  0  4 4.0
>        10  3  3 -1  4 8.0
>        11  4  2  0  4 4.0
>        12  4  0  2  4 2.0
>        13  0  0  4  4 1.0
> 
> case.struct file is still Cubic ,but the kinds of operation reduce from
>  48 to 16(accoring to the userguide, the Cubic system with magnetization 
> direction (001) should change to tetragonal, why in my case still Cubic 
> system? In my structure a=b=c)
> 
> and another question: because my system has inversion symmetry , after 
> initso_lapw , 
> it also preserve inversion, so in my case , the input file should be 
> case.in1 and case.in2c,
> but when during initso_lapw , at rerun kgen, it always show the messages:
> 
>    cp: can not stat "case.in1c_so", no such file or directory
>    cp: can not stat "case.in2c_so", no such file or directory
> 
> but the case.in1 and case.in2c can stil be created
> 
> So I hope some one can help me, I was confused by these all
> 
>     
>            
>     
>        
> 
>           
>     
> 
> 
> 
> 
> 
> 
> 
> 
> 
> 
> 
> 
> 
> 
> 
> 
> 
> 
> _________________________________________________________________
> ÓëÁª»úµÄÅóÓÑ½øÐÐ½»Á÷£¬ÇëÊ¹ÓÃ MSN Messenger: 
> http://messenger.microsoft.com/cn/
> 
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Date: Fri, 26 Jul 2002 15:51:25 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Calculation crashes with LAPW2

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I am trying to calculate a ferromagnetically coupled system,
> a perovskite in which the small cations are alternatingly
> Fe and Cr (resulting in (111)planes) with Wien2k_02
>
> The SCF breaks down in LAPW2 with the following error message:
>
> forrtl: severe (64): input conversion error, unit 1001, file
> /usr/tmp/baettigp/b2.helpup031
>    0: __FINI_00_remove_gp_range [0x3ff81a6c374]
>    1: __FINI_00_remove_gp_range [0x3ff81a6c8f4]
>    2: __FINI_00_remove_gp_range [0x3ff81a93b84]
>    3: outp_ [outp.f: 179, 0x120068b30]
>    4: l2main_ [l2main_tmp_.F: 1230, 0x12005f7a8]
>    5: lapw2_ [lapw2_tmp_.F: 465, 0x120064c18]
>    6: main [for_main.c: 203, 0x12007e32c]
>    7: __start [0x1200084c8]
>
> In b2.helpup031 are some lines as the following:
>
>  BAND#   8  E= -1.47073  WEIGHT= 0.0046296
>   L= 0   50.00000  ********** 18741.993********************-18658.372
>   L= 1    0.00000       0.000     0.000     0.000     0.000     0.000

Most likely the energy parameters are not ok and you got ghostbands.

Check the scf cycle. In what iteration did it happen ? Was :DIS decreasing
or diverging ? Check the energy parameters (case.scf1) and the respective
eigenvalues. I suppose for the first atom the l=0 (s) LO and APW energies
are too close to each other.

Most likely you will have to clean, run dstart (up/dn) again, reduce
the mixing and change energy parameters in case.in1

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Fri, 26 Jul 2002 09:28:50 -0700
From: David Clatterbuck <clatterb@uclink4.berkeley.edu>
Subject: [WIEN]: stress in WIEN2k?

====
David Clatterbuck <clatterb@uclink4.berkeley.edu>
submitted the following contribution:
====


Is WIEN2k able to compute stresses (not forces) on the unit cell
directly as is possible with most planewave codes? One can get the
stress by computing the energy of a unit cell before and after a small
strain and using sigma~(delta energy)/(delta strain), but I'm wondering
if one can get the entire stress tensor from a single computation. I
don't think this was possible with WIEN97 but am wondering if WIEN2K has
this feature.


Thanks,
David Clatterbuck
Lawrence Berkeley National Lab
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Date: Sat, 27 Jul 2002 01:48:26 +0000
From: "zhang YS Zhang" <zhangysthinker@hotmail.com>
Subject: Re: [WIEN]: Re:

====
"zhang YS Zhang" <zhangysthinker@hotmail.com>
submitted the following contribution:
====

Dear Igor Mazin:
   Thanks for your help. Now I use Wine2k_02, According to the useguide ,it 
maybe also to use the real version lapw1 if a system has inversion, but I 
am not sure. I just use the real lapw1

>
   >====
  >Igor Mazin <mazin@dave.nrl.navy.mil>
  >submitted the following contribution:
   >====
  >
  >A few comments to this point:
  >
   >1) With magnetism and SO, your symmetry has to be broken. Just make 
  >c.ne.a,b
  >slightly, it will do the job.

 my origin system Fm3m(a=b=c=5.932), you mean I make c.ne.a,b 
slightly(a=b=5.932, c=5.940),can this correct when my system cubic Fm3m? 

   > Correspondingly, if you want to get 
  >the right
  >orbital moment, you have to use the complex version of lapw1 (in 
  >Wien2k.
  >Apparently Wien2k_02 is organized differently)

 Now I use Wine2k_02, According to the useguide ,it maybe also useful to 
use the real version lapw1 if a system has inversion and I just use the 
real lapw1.
 but I am not sure if this is true?. According to the situation of my case, 
the orbit moment can also be obtained in my recent calculation.(but there 
has osciallation unfortunately). And I also want to know if the real lapw1 
in LDA+U calculation can be used, is it still necessary to make the lattice 
parameter c.ne.a and b? 

  >2) I have a neat script to create indm and inorb. See
  >http://cst-www.nrl.navy.mil/~mazin/, scroll down to
  >CCMS WIEN LAPW tips.

   >3) There can be different opinions, but I am very confident that for
  >f-electrons you want to use the localized version of LDA+U, 
  >nicknamed SIC in WIEN2k.

Oh this may be a stupid question , but I really want to know the difference 
between the  three kinds of LDA+U: SIC, AMF,HMF?  And I want to know the 
difference between LDA+U and OP?  How can I choose them in different case?

  >4) U for f-electrons is large, at least 0.4 Ry, therefore different
  >valence state of the rare earth may be stabilized in LDA+U. Be 
  >careful
  >to find the right ground state. The -orbc option is great for
  >steering the calculations into a given valence state.
 >5) I can send you input files for SmZn (a well behaving 
  >calculation), if you want to compare with yours.

If you can send it to me , I will great thankful!
>
>====
>
>
>*****************************************************************************

>Igor Mazin, NRL, code 6391, 4555 Overlook Ave, Was., DC 20375
>Ph.: 202 767-6990; Fax: 202 404-7546; e-mail mazin@nrl.navy.mil
>Home Page (under construction) http://cst-www.nrl.navy.mil/~mazin
>*****************************************************************************

>
>
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Date: Sat, 27 Jul 2002 02:37:13 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: Re: [WIEN]: Re: your mail

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====




>====
   >Peter Blaha <pblaha@theochem.tuwien.ac.at>
   >submitted the following contribution:
   >====
   >
   > >     I want to calcualte system like AB, where A is a f-element and B 
is
   > > p-element,
   > >  because A has localized f orbit, so I want to add ORB to the 
system. But
   > > there are some
   > >  questions I cann't solve
   >The reason is quite simply: SO calculation require complex lapw2 and
   >lapwdm, so you are missing a case.indmc file. Just copy your indm file 
to
   >indmc.
   >
Dear Peter and Georg Madsen:

    Thanks for your help , yes I cp case.indm to case.indmc .It is ok now.

but there are still qeustions  I  want to know:
  
    1 .Now I use wien2k_02, why my system with a cubic Fm3m 
(a=b=c=5.932)did't change to tetragonal system when the initso_lapw has 
been executed(still  a=b=c=5.932)? According to the userguide this change 
will occur. But just the number of symmetry operation reduce from 48 to 16. 
 Is this correct? If this is not correct, it mean that I must change 
parameter c slightly not equal to a and b just as Mr Igor Mazin has 
suggested to ?
  
    2. In Wien2k_02, we use real lapw1 also can obtain orbit moment, is 
this right?   If it is not correct, and I want to obtain the orbit moment 
of a system with  inversion ,how can I handle it?  Just cp case.in1 to 
case.in1c or broke the system by hand?(for example add extra atom or change 
slightly the parameter of system)

    3. when I use initso_lapw first ,when it ask if rerun kgen,  I select 
yes but the file case.klist did't change , it is the same as the case.klist 
during the init_lapw.  But when I run initso_lapw again ,after kgen ,the 
file changed. If I run initso_lapw for the third time , the file din't 
change again. If this means that we must run initso_lapw two times to 
obtain the correct case.klist file? Is this a bug in wien2k_02?


>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: 
http://www.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
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------------------------------

Date: Sat, 27 Jul 2002 10:56:58 -0400 (EDT)
From: Igor Mazin <mazin@dave.nrl.navy.mil>
Subject: Re: [WIEN]: Re:

====
Igor Mazin <mazin@dave.nrl.navy.mil>
submitted the following contribution:
====

Hi, I'm leaving for vacations, will be away from my mail for a week.
> 
>  my origin system Fm3m(a=b=c=5.932), you mean I make c.ne.a,b 
> slightly(a=b=5.932, c=5.940),can this correct when my system cubic Fm3m? 

Peter should know better, but my understanding is, what really matters,
is that the Number of operations reduces from 48 to 16. This should jhappen.

> Oh this may be a stupid question , but I really want to know the difference 
> between the  three kinds of LDA+U: SIC, AMF,HMF?  And I want to know the 
> difference between LDA+U and OP?  How can I choose them in different case?

There are many opinions. Mine is expressed in a recent cond-mat,
cond-mat/0206548. Briefly, for localized systems I believe SIC is in place,
(although I say this name is a misnomer), for weakly localized systems
no LDA+U is good, but if anything, AMF is better, and HMF should never be used.
Re OP my personal opinion is it is not physically justifiable,
there is a good deal of discussion of that in an older PRL by Soloviev and
Lichtenstein, and a little bit in an even older PRB by Anisimov and myself.
> 
> If you can send it to me , I will great thankful!

I did.

- -- 
*****************************************************************************
Igor Mazin, NRL, code 6391, 4555 Overlook Ave SW, Washington, DC 20375-5320
Phone: (202) 767-6990; Fax: (202) 404-7546; e-mail mazin@dave.nrl.navy.mil
Home Page (under construction) http://cst-www.nrl.navy.mil/~mazin
*****************************************************************************

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Date: Sat, 27 Jul 2002 18:21:41 -0400 (EDT)
From: Neme Nnolim <non6886@alizarin.njit.edu>
Subject: [WIEN]: Calculated DOS consists of single spike and nothing else?

====
Neme Nnolim <non6886@alizarin.njit.edu>
submitted the following contribution:
====


Dear WIEN users,

I am trying to calculate density of states for compressed unit cells of
tantalum. However,the calculated total DOS consists of a single
narrow pike going up to 200 states/eV.cell and nothing else.

I have changed the EMIN parameter in case.in2, tried using TEMP and GAUSS
instead of TETRA with EVAL = 0.002, tried using 100,000 k-points ( ~ 6500
irreducible k-points), tried changing energy limits in case.in1, all to no
avail.

I have also tried using GMAX of 10 and 14 with GGA option of 13.

There doesn't seem to be anything about this in the digest of previous
questions.

Below is a truncated version of my struct file (4th to 16th symmetry
operations are not shown).

- ---struct file begin-----------------------------------------
Ta-10_9
B   LATTICE,NONEQUIV. ATOMS: 1
MODE OF CALC=RELA
  6.280500  6.280500  6.155520 90.000000 90.000000 90.000000
ATOM= -1: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT=-2
Ta         NPT=  781  R0=0.00000500 RMT=    1.9000   Z: 73.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
  16      NUMBER OF SYMMETRY OPERATIONS
 1 0 0 0.0000000
 0-1 0 0.0000000
 0 0-1 0.0000000
       1
 0-1 0 0.0000000
 1 0 0 0.0000000
 0 0-1 0.0000000
       2
- -1 0 0 0.0000000
 0-1 0 0.0000000
 0 0-1 0.0000000
       3
 0 1 0 0.0000000
 1 0 0 0.0000000
 0 0-1 0.0000000
- --struct file end---------------------------------------------

- --begin case.in1 ---------------------------------------------

WFFIL        (WFPRI, SUPWF)
  10.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  0.30    7      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
 0    0.30      0.000 CONT
 0   -5.03      0.005 STOP
 1   -2.41      0.010 CONT
 1    0.30      0.000 CONT
 3    0.30      0.000 CONT
 3   -1.42      0.010 CONT
 2    0.30      0.010 CONT
K-VECTORS FROM UNIT:4    -9.0      2.5      emin/emax window

- ---end case.in1 -----------------------------------------------

Any ideas?

Thanks and regards,

Neme

- ------------------------------------------------------------------------------
Neme Okechukwu Nnolim
Department of Materials Science, New Jersey Institute of Technology
Room 302, Tiernan Hall, 161 Warren Street, University Heights
Newark, New Jersey 07102-1982
Tel: (973) 596-8283, FAX: (973) 596-5794
- -------------------------------------------------------------------------------


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Date: Sat, 27 Jul 2002 23:07:12 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: Calculated DOS consists of single spike and nothing else?

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====

> I am trying to calculate density of states for compressed unit cells of
> tantalum. However,the calculated total DOS consists of a single
> narrow pike going up to 200 states/eV.cell and nothing else.

Since you kindly provided a structure file, I tried the same calculation and 
also got a single spike, except that mine went up to 2000!  Mine may be
higher because I used a very coarse k-mesh.  Anyway, I tried the calculation 
again, but I used a larger RMT (2.5) and got something that looks reasonable, 
with the same k-mesh that I used for the RMT=1.9 run.  I'm not sure if it 
makes sense that the RMT value could do that, but that's what I found.  I am 
emailing you the DOS and the Bandstructure.

Fred Nastos
Department of Physics
University of Toronto

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Date: Sun, 28 Jul 2002 01:07:52 -0400 (EDT)
From: Neme Nnolim <non6886@alizarin.njit.edu>
Subject: Re: [WIEN]: Calculated DOS consists of single spike and nothing else?

====
Neme Nnolim <non6886@alizarin.njit.edu>
submitted the following contribution:
====


Fred,

Thanks for the insight. I will try to play around with the RMT values.
I should have tried doing that first. Thanks.


Regards,

Neme

On Sat, 27 Jul 2002, Fred Nastos wrote:

> Date: Sat, 27 Jul 2002 23:07:12 -0400
> From: Fred Nastos <nastos@physics.utoronto.ca>
> Reply-To: wien@zeus.theochem.tuwien.ac.at
> To: wien@zeus.theochem.tuwien.ac.at
> Subject: Re: [WIEN]: Calculated DOS consists of single spike and nothing
>     else?
> Since you kindly provided a structure file, I tried the same calculation and 
> also got a single spike, except that mine went up to 2000!  Mine may be
> higher because I used a very coarse k-mesh.  Anyway, I tried the calculation 
> again, but I used a larger RMT (2.5) and got something that looks reasonable, 
> with the same k-mesh that I used for the RMT=1.9 run.  I'm not sure if it 
> makes sense that the RMT value could do that, but that's what I found.  I am 
> emailing you the DOS and the Bandstructure.
> 
> Fred Nastos
> Department of Physics
> University of Toronto

- -- 

- ------------------------------------------------------------------------------
Neme Okechukwu Nnolim
Department of Materials Science, New Jersey Institute of Technology
Room 302, Tiernan Hall, 161 Warren Street, University Heights
Newark, New Jersey 07102-1982
Tel: (973) 596-8283, FAX: (973) 596-5794
- -------------------------------------------------------------------------------



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Date: Sat, 27 Jul 2002 22:47:25 -0700 (PDT)
From: Rose makine <r_makine@yahoo.com>
Subject: [WIEN]: problem on DOS

====
Rose makine <r_makine@yahoo.com>
submitted the following contribution:
====

Dear WIEN Users
when I calculate DOS,lapw2 is not run.This error is
appear: 
PGFIO-F-252/list-directed read/unit=29/operation
attempted after end of file.
     File name = LDA.energydn    formatted, sequential
access   record = 5000
     In source file fermi.f, at line number 63
    0.040u 0.000s 0:00.10 40.0%     0+0k 0+0io
214pf+0w

Why?How I solve it?
Thanks.
       R. Makine.

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------------------------------

Date: Mon, 29 Jul 2002 08:48:37 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Re: your mail

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>     1 .Now I use wien2k_02, why my system with a cubic Fm3m
> (a=b=c=5.932)did't change to tetragonal system when the initso_lapw has
> been executed(still  a=b=c=5.932)? According to the userguide this change
> will occur. But just the number of symmetry operation reduce from 48 to 16.
>  Is this correct? If this is not correct, it mean that I must change
> parameter c slightly not equal to a and b just as Mr Igor Mazin has
> suggested to ?

No, you don't need to change the c parameter. symmetso can now reduce the
symmetry without further tricks.

>     2. In Wien2k_02, we use real lapw1 also can obtain orbit moment, is
> this right?   If it is not correct, and I want to obtain the orbit moment
> of a system with  inversion ,how can I handle it?  Just cp case.in1 to
> case.in1c or broke the system by hand?(for example add extra atom or change
> slightly the parameter of system)

If you have inversion, you can always keep lapw1, but after lapwso even in
this case the complex  lapw2c and lapwdmc must be used.

>     3. when I use initso_lapw first ,when it ask if rerun kgen,  I select
> yes but the file case.klist did't change , it is the same as the case.klist
> during the init_lapw.  But when I run initso_lapw again ,after kgen ,the
> file changed. If I run initso_lapw for the third time , the file din't
> change again. If this means that we must run initso_lapw two times to
> obtain the correct case.klist file? Is this a bug in wien2k_02?

This is a bug in initso_lapw. It runs first kgen and oly then will update the
struct file. Thus one should rerun kgen later on as you did. I'll fix this
very soon.

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 29 Jul 2002 09:00:53 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: problem on DOS

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> when I calculate DOS,lapw2 is not run.This error is
> appear:
> PGFIO-F-252/list-directed read/unit=29/operation
> attempted after end of file.
>      File name = LDA.energydn    formatted, sequential
> access   record = 5000
>      In source file fermi.f, at line number 63
>     0.040u 0.000s 0:00.10 40.0%     0+0k 0+0io

When running a spinpolarized case, you must have both, spin-up AND dn vectors.
I.e.:

x lapw1 -up
x lapw1 -dn
x lapw2 -up -qtl
x lapw2 -dn -qtl

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 29 Jul 2002 09:02:21 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: stress in WIEN2k?

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Is WIEN2k able to compute stresses (not forces) on the unit cell
> directly as is possible with most planewave codes? One can get the
> stress by computing the energy of a unit cell before and after a small
> strain and using sigma~(delta energy)/(delta strain), but I'm wondering
> if one can get the entire stress tensor from a single computation. I
> don't think this was possible with WIEN97 but am wondering if WIEN2K has
> this feature.

No, the stress tensor is not part of WIEN2k.
C.Ambrosch-Draxl is working on that.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Mon, 29 Jul 2002 02:43:55 -0700 (PDT)
From: Rose makine <r_makine@yahoo.com>
Subject: Re: [WIEN]: problem on DOS

====
Rose makine <r_makine@yahoo.com>
submitted the following contribution:
====

- --0-886712059-1027935835=:41827
Content-Type: text/plain; charset=us-ascii
Content-Disposition: inline

Dear Prof.Blaha
Thanks for your answer,but I have both, spin-up AND
spin-dn vectors.My DAYSFILE is attachment.
Sincerely.
         R_Makine.
- --- Peter Blaha <pblaha@theochem.tuwien.ac.at> wrote:
> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> > when I calculate DOS,lapw2 is not run.This error
> is
> > appear:
> > PGFIO-F-252/list-directed read/unit=29/operation
> > attempted after end of file.
> >      File name = LDA.energydn    formatted,
> sequential
> > access   record = 5000
> >      In source file fermi.f, at line number 63
> >     0.040u 0.000s 0:00.10 40.0%     0+0k 0+0io
> 
> When running a spinpolarized case, you must have
> both, spin-up AND dn vectors.
> I.e.:
> 
> x lapw1 -up
> x lapw1 -dn
> x lapw2 -up -qtl
> x lapw2 -dn -qtl
> 
> Regards
> 
>                                       P.Blaha
>
- --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna,
> A-1060 Vienna
> Phone: +43-1-58801-15671             FAX:
> +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
> http://www.tuwien.ac.at/theochem/
>
- --------------------------------------------------------------------------
> 
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====


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- --0-886712059-1027935835=:41827
Content-Type: text/plain; name=20
Content-Description: 20
Content-Disposition: inline; filename=20


   Calculating LDA in /home/makine/LDA
   on CondMat6

       start       (Tue Mar 19 14:33:08 IRT 2002) with lapw0 (200/20 to go)
   >   lapw0       (14:33:08) 8.570u 0.040s 0:08.77 98.1%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (14:33:17) 441.270u 11.690s 7:42.36 97.9%       0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (14:40:59) 438.200u 11.720s 7:40.63 97.6%       0+0k 0+0io 401pf+0w
   >   lapw2 -up   (14:48:40) 147.570u 0.810s 2:33.20 96.8%        0+0k 0+0io 331pf+0w
   >   lapw2 -dn   (14:51:13) 127.520u 0.550s 2:21.32 90.6%        0+0k 0+0io 329pf+0w
   >   lcore -up   (14:53:35) 0.240u 0.010s 0:00.24 104.1% 0+0k 0+0io 191pf+0w
   >   lcore -dn   (14:53:35) 0.240u 0.000s 0:00.24 100.0% 0+0k 0+0io 191pf+0w
   >   mixer       (14:53:35) 1.790u 0.020s 0:01.90 95.2%  0+0k 0+0io 214pf+0w
   :ENERGY convergence:  0 0.00001 0
   :CHARGE convergence:  0 0 0
   199/19 to go

   >   lapw0       (14:53:37) 8.510u 0.050s 0:08.93 95.8%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (14:53:46) 439.180u 11.380s 14:25.15 52.0%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (15:08:11) 439.660u 11.370s 17:49.40 42.1%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (15:26:01) 152.930u 0.580s 7:46.78 32.8%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (15:33:48) 126.490u 0.580s 5:15.99 40.2%        0+0k 0+0io 329pf+0w
   >   lcore -up   (15:39:04) 0.230u 0.010s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (15:39:04) 0.240u 0.010s 0:00.45 55.5%  0+0k 0+0io 191pf+0w
   >   mixer       (15:39:05) 1.780u 0.050s 0:03.92 46.6%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 0
   :CHARGE convergence:  0 0 0
   198/18 to go

   >   lapw0       (15:39:09) 8.770u 0.060s 0:18.04 48.9%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (15:39:27) 444.280u 12.160s 15:37.55 48.6%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (15:55:05) 444.650u 11.790s 15:20.68 49.5%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (16:10:25) 150.680u 0.540s 5:02.35 50.0%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (16:15:28) 125.640u 0.510s 4:12.23 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (16:19:40) 0.230u 0.010s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (16:19:41) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   mixer       (16:19:41) 1.810u 0.000s 0:03.61 50.1%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .1699260000000000
   :CHARGE convergence:  0 0 .5900908
   197/17 to go

   >   lapw0       (16:19:45) 8.980u 0.060s 0:18.10 49.9%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (16:20:03) 436.510u 12.000s 14:57.11 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (16:35:01) 439.780u 11.350s 15:02.23 50.0%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (16:50:03) 154.850u 0.500s 5:10.76 49.9%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (16:55:14) 121.900u 0.500s 4:04.80 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (16:59:18) 0.220u 0.020s 0:00.44 54.5%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (16:59:19) 0.230u 0.010s 0:00.43 55.8%  0+0k 0+0io 191pf+0w
   >   mixer       (16:59:20) 1.790u 0.020s 0:03.61 50.1%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0409075000000000
   :CHARGE convergence:  0 0 .8151462
   196/16 to go

   >   lapw0       (16:59:24) 8.510u 0.050s 0:17.09 50.0%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (16:59:41) 436.710u 11.910s 14:57.37 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (17:14:38) 436.580u 11.510s 14:56.29 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (17:29:34) 150.240u 0.550s 5:01.51 50.0%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (17:34:36) 125.140u 0.500s 4:11.21 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (17:38:47) 0.250u 0.000s 0:00.42 59.5%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (17:38:48) 0.250u 0.000s 0:00.48 52.0%  0+0k 0+0io 191pf+0w
   >   mixer       (17:38:48) 1.780u 0.030s 0:03.55 50.9%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0554370000000000
   :CHARGE convergence:  0 0 .3410092
   195/15 to go

   >   lapw0       (17:38:52) 8.940u 0.030s 0:17.97 49.9%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (17:39:10) 436.820u 11.260s 14:56.21 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (17:54:07) 441.570u 11.620s 15:06.38 50.0%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (18:09:13) 148.760u 0.380s 4:58.29 49.9%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (18:14:11) 127.980u 0.520s 4:17.06 49.9%        0+0k 0+0io 329pf+0w
   >   lcore -up   (18:18:29) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (18:18:29) 0.240u 0.010s 0:00.48 52.0%  0+0k 0+0io 191pf+0w
   >   mixer       (18:18:30) 1.800u 0.020s 0:03.62 50.2%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0388500000000000
   :CHARGE convergence:  0 0 .4987429
   194/14 to go

   >   lapw0       (18:18:34) 8.430u 0.050s 0:16.93 50.0%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (18:18:51) 436.960u 11.470s 14:56.94 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (18:33:48) 436.650u 11.650s 14:56.66 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (18:48:44) 148.820u 0.400s 4:58.50 49.9%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (18:53:43) 127.740u 0.510s 4:16.40 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (18:57:59) 0.230u 0.020s 0:00.42 59.5%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (18:58:00) 0.250u 0.000s 0:00.42 59.5%  0+0k 0+0io 191pf+0w
   >   mixer       (18:58:00) 1.790u 0.040s 0:03.68 49.7%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0380310000000000
   :CHARGE convergence:  0 0 .4860822
   193/13 to go

   >   lapw0       (18:58:04) 8.920u 0.040s 0:17.83 50.2%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (18:58:22) 436.670u 11.620s 14:56.63 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (19:13:19) 436.630u 11.500s 14:56.43 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (19:28:16) 149.290u 0.470s 4:59.53 49.9%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (19:33:15) 127.160u 0.640s 4:15.54 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (19:37:31) 0.250u 0.000s 0:00.48 52.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (19:37:31) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   mixer       (19:37:32) 1.810u 0.020s 0:03.68 49.7%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0217865000000000
   :CHARGE convergence:  0 0 .5817786
   192/12 to go

   >   lapw0       (19:37:36) 8.930u 0.050s 0:17.98 49.9%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (19:37:54) 436.670u 11.460s 14:56.45 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (19:52:50) 436.850u 11.550s 14:56.83 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (20:07:47) 147.560u 0.450s 4:56.05 49.9%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (20:12:43) 129.580u 0.490s 4:20.26 49.9%        0+0k 0+0io 329pf+0w
   >   lcore -up   (20:17:04) 0.230u 0.020s 0:00.48 52.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (20:17:04) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   mixer       (20:17:05) 1.810u 0.030s 0:03.69 49.8%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0272660000000000
   :CHARGE convergence:  0 0 .3020233
   191/11 to go

   >   lapw0       (20:17:09) 8.890u 0.040s 0:17.87 49.9%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (20:17:27) 436.040u 12.210s 14:56.50 50.0%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (20:32:23) 440.320u 11.830s 15:04.43 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (20:47:28) 145.090u 0.590s 4:51.30 50.0%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (20:52:19) 130.680u 0.440s 4:22.12 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (20:56:41) 0.250u 0.000s 0:00.48 52.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (20:56:42) 0.240u 0.000s 0:00.42 57.1%  0+0k 0+0io 191pf+0w
   >   mixer       (20:56:42) 1.800u 0.040s 0:03.69 49.8%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0194925000000000
   :CHARGE convergence:  0 0 .2735661
   190/10 to go

   >   lapw0       (20:56:46) 8.800u 0.060s 0:17.68 50.1%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (20:57:04) 436.020u 11.940s 14:56.13 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (21:12:00) 436.370u 11.400s 14:55.49 50.0%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (21:26:56) 144.400u 0.570s 4:49.92 50.0%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (21:31:46) 131.130u 0.470s 4:23.10 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (21:36:09) 0.250u 0.000s 0:00.48 52.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (21:36:10) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   mixer       (21:36:10) 1.820u 0.030s 0:03.71 49.8%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0273845000000000
   :CHARGE convergence:  0 0 .3820988
   189/9 to go

   >   lapw0       (21:36:14) 8.710u 0.040s 0:17.50 50.0%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (21:36:32) 436.510u 11.760s 14:56.55 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (21:51:28) 436.780u 11.470s 14:56.67 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (22:06:25) 145.370u 0.470s 4:51.70 49.9%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (22:11:17) 130.850u 0.520s 4:22.66 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (22:15:40) 0.240u 0.000s 0:00.42 57.1%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (22:15:40) 0.240u 0.010s 0:00.48 52.0%  0+0k 0+0io 191pf+0w
   >   mixer       (22:15:41) 1.820u 0.030s 0:03.65 50.6%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0205370000000000
   :CHARGE convergence:  0 0 .1625775
   188/8 to go

   >   lapw0       (22:15:45) 8.780u 0.090s 0:17.74 50.0%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (22:16:03) 437.060u 11.240s 14:56.75 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (22:30:59) 437.750u 11.490s 14:58.52 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (22:45:58) 145.090u 0.590s 4:51.25 50.0%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (22:50:49) 130.740u 0.580s 4:22.64 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (22:55:12) 0.240u 0.000s 0:00.44 54.5%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (22:55:12) 0.240u 0.010s 0:00.42 59.5%  0+0k 0+0io 191pf+0w
   >   mixer       (22:55:13) 1.800u 0.050s 0:03.66 50.5%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0166900000000000
   :CHARGE convergence:  0 0 .1073723
   187/7 to go

   >   lapw0       (22:55:17) 8.430u 0.070s 0:16.95 50.1%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (22:55:34) 438.560u 11.300s 14:59.81 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (23:10:34) 437.060u 11.070s 14:56.23 50.0%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (23:25:30) 145.100u 0.470s 4:51.12 50.0%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (23:30:22) 130.760u 0.490s 4:22.43 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (23:34:44) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (23:34:45) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   mixer       (23:34:45) 1.820u 0.040s 0:03.70 50.2%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0048560000000000
   :CHARGE convergence:  0 0 .0964901
   186/6 to go

   >   lapw0       (23:34:49) 8.990u 0.050s 0:18.04 50.1%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (23:35:07) 438.530u 11.940s 15:00.95 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (23:50:08) 436.720u 11.430s 14:56.39 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (00:05:05) 145.210u 0.490s 4:51.31 50.0%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (00:09:56) 130.690u 0.480s 4:22.32 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (00:14:19) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (00:14:19) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   mixer       (00:14:20) 1.840u 0.020s 0:03.65 50.9%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0031690000000000
   :CHARGE convergence:  0 0 .0540543
   185/5 to go

   >   lapw0       (00:14:24) 8.900u 0.050s 0:17.84 50.1%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (00:14:42) 436.630u 12.050s 14:57.43 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (00:29:39) 436.930u 11.140s 14:56.15 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (00:44:35) 145.260u 0.590s 4:51.80 49.9%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (00:49:27) 130.890u 0.510s 4:22.78 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (00:53:50) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (00:53:51) 0.240u 0.000s 0:00.44 54.5%  0+0k 0+0io 191pf+0w
   >   mixer       (00:53:51) 1.830u 0.040s 0:03.67 50.9%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0006150000000000
   :CHARGE convergence:  0 0 .0345955
   184/4 to go

   >   lapw0       (00:53:55) 9.070u 0.030s 0:18.22 49.9%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (00:54:13) 436.600u 11.350s 14:55.96 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (01:09:09) 437.220u 11.430s 14:57.58 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (01:24:07) 145.200u 0.400s 4:51.21 49.9%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (01:28:58) 131.100u 0.500s 4:23.22 49.9%        0+0k 0+0io 329pf+0w
   >   lcore -up   (01:33:21) 0.230u 0.010s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (01:33:22) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   mixer       (01:33:23) 1.810u 0.060s 0:03.72 50.2%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0003090000000000
   :CHARGE convergence:  0 0 .0285507
   183/3 to go

   >   lapw0       (01:33:27) 8.870u 0.030s 0:17.84 49.8%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (01:33:44) 436.100u 11.870s 14:56.01 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (01:48:40) 436.460u 11.300s 14:55.51 50.0%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (02:03:36) 145.180u 0.420s 4:51.15 50.0%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (02:08:27) 130.790u 0.450s 4:22.43 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (02:12:50) 0.230u 0.020s 0:00.42 59.5%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (02:12:50) 0.240u 0.010s 0:00.48 52.0%  0+0k 0+0io 191pf+0w
   >   mixer       (02:12:51) 1.840u 0.020s 0:03.66 50.8%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0003735000000000
   :CHARGE convergence:  0 0 .0197750
   182/2 to go

   >   lapw0       (02:12:55) 8.670u 0.040s 0:17.34 50.2%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (02:13:12) 437.020u 11.230s 14:56.57 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (02:28:09) 436.940u 11.410s 14:56.88 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (02:43:06) 145.190u 0.450s 4:51.19 50.0%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (02:47:57) 130.500u 0.480s 4:21.90 50.0%        0+0k 0+0io 329pf+0w
   >   lcore -up   (02:52:19) 0.240u 0.010s 0:00.48 52.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (02:52:20) 0.240u 0.000s 0:00.42 57.1%  0+0k 0+0io 191pf+0w
   >   mixer       (02:52:20) 1.830u 0.040s 0:03.73 50.1%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0003920000000000
   :CHARGE convergence:  0 0 .0080772
   181/1 to go

   >   lapw0       (02:52:24) 9.000u 0.060s 0:18.11 50.0%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (02:52:43) 437.860u 11.290s 14:58.42 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (03:07:41) 437.100u 11.230s 14:56.71 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (03:22:38) 145.690u 0.530s 4:52.43 50.0%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (03:27:30) 130.700u 0.410s 4:22.24 49.9%        0+0k 0+0io 329pf+0w
   >   lcore -up   (03:31:53) 0.240u 0.010s 0:00.48 52.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (03:31:53) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   mixer       (03:31:54) 1.870u 0.020s 0:03.80 49.7%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  0 0.00001 .0003285000000000
   :CHARGE convergence:  0 0 .0065214
       restart
   180/20 to go

   >   lapw0       (03:31:58) 8.460u 0.050s 0:16.97 50.1%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (03:32:15) 436.650u 11.280s 14:55.99 49.9%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (03:47:11) 437.040u 11.700s 14:59.27 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (04:02:10) 145.860u 0.490s 4:52.87 49.9%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (04:07:03) 131.350u 0.570s 4:24.31 49.9%        0+0k 0+0io 329pf+0w
   >   lcore -up   (04:11:27) 0.240u 0.010s 0:00.48 52.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (04:11:28) 0.240u 0.000s 0:00.42 57.1%  0+0k 0+0io 191pf+0w
   >   mixer       (04:11:28) 1.820u 0.030s 0:03.65 50.6%  0+0k 0+0io 214pf+0w
   :ENERGY convergence:  0 0.00001 .0000385000000000
   :CHARGE convergence:  0 0 .0042511
   179/19 to go

   >   lapw0       (04:11:33) 8.500u 0.090s 0:17.10 50.2%  0+0k 0+0io 279pf+0w
   >   lapw1  -up          (04:11:50) 437.140u 12.020s 14:58.27 50.0%      0+0k 0+0io 401pf+0w
   >   lapw1  -dn          (04:26:48) 437.500u 11.510s 14:58.06 49.9%      0+0k 0+0io 401pf+0w
   >   lapw2 -up   (04:41:46) 145.200u 0.480s 4:51.98 49.8%        0+0k 0+0io 329pf+0w
   >   lapw2 -dn   (04:46:38) 130.260u 0.480s 4:22.14 49.8%        0+0k 0+0io 329pf+0w
   >   lcore -up   (04:51:00) 0.240u 0.010s 0:00.48 52.0%  0+0k 0+0io 191pf+0w
   >   lcore -dn   (04:51:01) 0.240u 0.000s 0:00.48 50.0%  0+0k 0+0io 191pf+0w
   >   mixer       (04:51:02) 1.840u 0.010s 0:03.82 48.4%  0+0k 0+0io 215pf+0w
   :ENERGY convergence:  1 0.00001 .0000055000000000
   :CHARGE convergence:  0 0 .0045833
   0/18 to go


   >   stop


- --0-886712059-1027935835=:41827--
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------------------------------

Date: Mon, 29 Jul 2002 04:11:00 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: [WIEN]: Does P1/2 basis also improve EFG?

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

Dear all,

Band structure calculation of fcc Th has shown that additional p1/2 local
orbitals improve the description of actinide. This improvement is
demonstrated by a reduction of second variation cutoff energy or E_max from
8 Ry within GGA+SO to 3 Ry within GGA+SO+P1/2 to calculate ENE. It is also
shown that p1/2 modification does not change the distribution of valence
bands, and hence any quantities related to the valence band. This means that
p1/2 modification just a bit increases the separation between the pick of
p1/2 DOS and the pick p3/2 DOS (~1eV), but does not change the total DOS in
vicinity the Fermi energy. As a result of this fact, one does not expect to
see a significant difference between two calculated equilibrium volumes
within GGA+SO and GGA+SO+P1/2.

Even though our calculated total energies of some actinide compounds for
various second variation cutoff energies confirm such an reduction and thus
the improvement of p1/2 basis, our calculated electric field gradient (EFG)
does not follow the story at all. The later one means that EFG is in
contrast with the reported improvement of P1/2 modification. We know that
EFG mainly originates from valence band and a bit from semi core states.
Therefore, one expects to observe a comparable behavior of EFG with other
quantity relative to valence bands, say equilibrium volume. So, the question
is the subject of this mail: Does P1/2 local orbitals improve the calculated
EFG of actinide compounds or Does one just calculating EFG say that
additional p1/2 local orbitals improve the description of actinide?

Thank you for your attention to this matter.

Your,

S. Jalali.


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------------------------------

Date: Mon, 29 Jul 2002 08:54:12 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Re: (Igor)

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

Dear Igor,

I know you are on vocation and away from your mail for a week. I followed
your recent discussion with Yue, and Peter in the mailing list during last
week, and heard about your nice presented poster on SmZn.



> 5) I can send you input files for SmZn (a well behaving calculation), if
you
> want to compare with yours.

It will be appreciated not only sending the input files, but also a copy of
your results (if possible).

I am looking forward for your coming back to work.

Your,

S. Jalali.


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------------------------------

Date: Mon, 29 Jul 2002 18:59:12 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [none]

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

My lapws crashed for my crystal calcultion for many times, I was told

"STOP: SELECT - Error"

even I changed the mixing factor from 0.5 to 0.01 and BROYD to PRATT,
could you please let me know the possible reasons for it and how to remedy
it?

Thank you in adavance!


Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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Date: Tue, 30 Jul 2002 08:48:42 +0800
From: caij@ihpc.a-star.edu.sg
Subject: [WIEN]: sorry just for test

====
caij@ihpc.a-star.edu.sg
submitted the following contribution:
====

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------------------------------

Date: Tue, 30 Jul 2002 08:33:58 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Does P1/2 basis also improve EFG?

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====


> quantity relative to valence bands, say equilibrium volume. So, the question
> is the subject of this mail: Does P1/2 local orbitals improve the calculated
> EFG of actinide compounds or Does one just calculating EFG say that
> additional p1/2 local orbitals improve the description of actinide?

NO!!! We are working on that.

The p1/2 basis should only contribute to the spherical part of the electron
density, but so far we do not force this. Thus very small nonspherical
contributions can occur and since the p1/2 function is non-zero at the
nucleus, it leads to a diverging contribution to the EFG.

So far, you MUST NOT use p1/2 LOs  when you are interested in EFGs on that
nucleus.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Tue, 30 Jul 2002 01:33:04 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Does P1/2 basis also improve EFG?

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

I am thankful to Peter for his accurate contribution to the matter of added
p1/2 function.

> So far, you MUST NOT use p1/2 LOs  when you are interested in EFGs on that
> nucleus.

We are calculating EFG at a tin nucleus, where even SO can be switched off.

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Date: Tue, 30 Jul 2002 13:24:01 +0430
From: "Mahmoud Payami" <mpayami@aeoi.org.ir>
Subject: [WIEN]: GETARG

====
"Mahmoud Payami" <mpayami@aeoi.org.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_000D_01C237CC.5E4A2A10
Content-Type: text/plain;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

Dear Wien users and developers,
When running "x nn", "x symmetry", "x lstart", "x kgen", "x dstart", I =
encounter the message:

GETARG: argument index (2) out of range.

This message is continued in each cycle of the scf calculation.
The file "lapw0.error" contains the message: error in lapw0.

Any suggestions is highly welcome.

Kind regards,

M. Payami


- ------=_NextPart_000_000D_01C237CC.5E4A2A10
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META content=3D"text/html; charset=3Diso-8859-1" =
http-equiv=3DContent-Type>
<META content=3D"MSHTML 5.00.2920.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT face=3DArial size=3D2>Dear Wien users and =
developers,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>When running "x nn", "x symmetry", "x =
lstart", "x=20
kgen", "x dstart", I encounter the message:</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>GETARG: argument index (2) out of=20
range.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>This message is continued in each cycle =
of the scf=20
calculation.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>The file "lapw0.error" contains the =
message: error=20
in lapw0.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Any suggestions is highly =
welcome.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Kind regards,</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>M. Payami</FONT></DIV>
<DIV>&nbsp;</DIV></BODY></HTML>

- ------=_NextPart_000_000D_01C237CC.5E4A2A10--


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Date: Tue, 30 Jul 2002 10:17:00 -0400
From: "Dadi Dai" <dai@unity.ncsu.edu>
Subject: [WIEN]: How to determine the space-group in AFM calculations?

====
"Dadi Dai" <dai@unity.ncsu.edu>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0040_01C237B2.3DFAFB00
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	charset="iso-8859-1"
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Dear WIEN authors and users,

I wish to carry antiferrimagnetic (AFM) calculation of CdVO3, which is =
orthorhombic Pnma (group #62) with a=3D14.301, b=3D3.598, c=3D5.204.  =
The fractional coordinates are:

Cd    0.3184    1/4    0.1383
V     0.0806    1/4    0.0826
O-1    0.1096    1/4    0.3930
O-2    -0.0579    1/4    0.0421
O-3    0.1941    1/4    -0.1064

In my calculations, the AFM chain is along c direction.  Therefore, I =
have to double the unit cell along c direction, namely, to make a =
super-unit-cell 1*1*2.  In this case, I can have two sets of V atoms, =
and I can put up-spin in one set of V while putting down-spin in another =
set of V.

My question is, what space-group should I specify in struct-generation =
for the AFM super-cell?

(It seems to me that the new super-cell does not satisfy #62 any more, =
after there are two sets of V.)

Thank you very much.

Dadi Dai

- ------=_NextPart_000_0040_01C237B2.3DFAFB00
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2713.1100" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD><FONT face=3DArial><FONT size=3D2>
<BODY>
<DIV>Dear WIEN authors and users,</DIV>
<DIV>&nbsp;</DIV>
<DIV>I wish to carry antiferrimagnetic (AFM)&nbsp;calculation of CdVO3, =
which is=20
orthorhombic Pnma (group #62) with a=3D14.301, b=3D3.598, =
c=3D5.204.&nbsp; The=20
fractional coordinates are:</DIV>
<DIV>&nbsp;</DIV>
<DIV>Cd&nbsp;&nbsp;&nbsp; 0.3184&nbsp;&nbsp;&nbsp; 1/4&nbsp;&nbsp;&nbsp; =

0.1383</DIV>
<DIV>V&nbsp;&nbsp;&nbsp;&nbsp; 0.0806&nbsp;&nbsp;&nbsp; =
1/4&nbsp;&nbsp;&nbsp;=20
0.0826</DIV>
<DIV>O-1&nbsp;&nbsp;&nbsp; 0.1096&nbsp;&nbsp;&nbsp; =
1/4&nbsp;&nbsp;&nbsp;=20
0.3930</DIV>
<DIV>O-2&nbsp;&nbsp;&nbsp; -0.0579&nbsp;&nbsp;&nbsp; =
1/4&nbsp;&nbsp;&nbsp;=20
0.0421</DIV>
<DIV>O-3&nbsp;&nbsp;&nbsp; 0.1941&nbsp;&nbsp;&nbsp; =
1/4&nbsp;&nbsp;&nbsp;=20
- -0.1064</DIV>
<DIV>&nbsp;</DIV>
<DIV>In my calculations, the AFM chain is along c direction.&nbsp;=20
Therefore,&nbsp;I have to double the unit cell along c direction, =
namely, to=20
make a super-unit-cell 1*1*2.&nbsp; In this case, I can have two sets of =
V=20
atoms, and I can put up-spin in one set of V while putting down-spin in =
another=20
set of V.</DIV>
<DIV>&nbsp;</DIV>
<DIV>My question is, what space-group should I specify in =
struct-generation for=20
the AFM super-cell?</DIV>
<DIV>&nbsp;</DIV>
<DIV>(It seems to me that the new super-cell does not satisfy #62 any =
more,=20
after there are two sets of V.)</DIV>
<DIV>&nbsp;</DIV>
<DIV>Thank you very much.</DIV>
<DIV>&nbsp;</DIV>
<DIV>Dadi Dai</DIV></BODY></HTML></FONT></FONT>

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Date: Tue, 30 Jul 2002 20:14:42 +0300
From: "B. Yanchitsky" <yan@im.imag.kiev.ua>
Subject: Re: [WIEN]: How to determine the space-group in AFM calculations?

====
"B. Yanchitsky" <yan@im.imag.kiev.ua>
submitted the following contribution:
====

This is a multi-part message in MIME format.
- --------------C785FA1BCAA842715597B471
Content-Type: text/plain; charset=koi8-r
Content-Transfer-Encoding: 7bit

>Cd    0.3184    1/4    0.1383
>V     0.0806    1/4    0.0826
>O-1    0.1096    1/4    0.3930
>O-2    -0.0579    1/4    0.0421
>O-3    0.1941    1/4    -0.1064

>In my calculations, the AFM chain is along c direction.  Therefore, I have to 
>double the unit cell along c direction, namely, to make a super-unit-cell 1*1*2.  
>In this case, I can have two sets of V atoms, and I can put up-spin in one set of 
>V while putting down-spin in another set of V.

>My question is, what space-group should I specify in struct-generation for the 
>AFM super-cell?

>(It seems to me that the new super-cell does not satisfy #62 any more, after 
>there are two sets of V.)

It's quite simple, but with a lot of typing.
The main idea - construct 1x1x2 supercell and introduce manually 
split for V atoms only, and find new cupercell with "x sgroup".
Below is attached 1x1x2 cupercell (with sgroup output), 
(if no split for V) then sgroup finds reduced supercell with #62 Pnma as it should be. With split for V atoms, new cell is
monoclinic and space group is #11,
but note that new 001 direction is 010 old one.

ps
it appears a small problem. Actually sgroup treats only 1-2 literal
positions for an atom name and appends digits to it if any.
But with such treatment it is not clear where are up and dn atoms
in output file. So to split V atoms 
i changed V -> Vu for up, and V -> Vd for down.
Make a check for initial CdVO3 file of course :)

Regards,

Bogdan Yanchitsky
- --------------C785FA1BCAA842715597B471
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Date: Tue, 30 Jul 2002 11:27:06 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: [WIEN]: Does -so split automatically p to its partial relativistic states?

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

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Dear all,

Is not it assumed that p-orbital of an actinide metal, e.g. fcc-Th, =
should automatically split to p1/2 and p3/2 after turning on the =
spin-orbit coupling or one needs to do something special? We have =
accidentally looking for something else found that p of fcc-Th is not =
splitted to its partial relativistic orbitals within GGA+SO or =
GGA+SO+p1/2 with and without spin polarization. Thus, we at this stage =
conclude that one needs to do something special. Are we in a right =
stage?! Spin intrinsically introduces itself solving fully relativistic =
Dirac equation, and so one thinks SO also cannot be independent of spin =
as it is. Indeed SO as an approximation to take into acount relativistic =
effect is a term proportional to a dot product of spin and orbit =
vectors. It looks all these are telling us one does not need to do such =
an special job to split p-orbital to p1/2 and p3/2 provided that SO does =
its job correctly. So, my questions are as follows: Why is not p-orbital =
of fcc-Th in the energy interval (-25eV, -13eV) within GGA+SO splitted =
to p1/2 and p3/2, and how can it be done?  Why is not the command of =
"run_lapw -so" meaningless, although imposing magnetic moment also has =
not shown an effect on splitting?

Thank you for your attention to this problem.

Your,

S. Jalali.

=20

=20




- ------=_NextPart_000_002E_01C237BC.0956FBB0
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT face=3DArial size=3D2><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial"><FONT size=3D2>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">Dear =
all,</SPAN><?xml:namespace=20
prefix =3D o ns =3D "urn:schemas-microsoft-com:office:office" =
/><o:p></o:p></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">Is not it assumed that =
p-orbital of=20
an actinide metal, e.g.&nbsp;fcc-Th, should automatically split to p1/2 =
and p3/2=20
after turning on the spin-orbit coupling or one needs to =
do&nbsp;something=20
special? We have accidentally looking for something else found that p of =
fcc-Th=20
is not splitted to its partial relativistic orbitals within GGA+SO or=20
GGA+SO+p1/2 with and without spin polarization. Thus, we at this stage =
conclude=20
that one needs to do something special. Are we in a right =
stage?!&nbsp;Spin=20
intrinsically introduces itself solving fully relativistic Dirac =
equation, and=20
so one thinks SO also cannot be independent of spin as it is. Indeed =
SO&nbsp;as=20
an approximation&nbsp;to&nbsp;take into acount&nbsp;relativistic effect =
is a=20
term proportional to a dot product of spin and orbit vectors. It looks =
all these=20
are&nbsp;telling us one does not need to do such an special job to split =

p-orbital to p1/2 and p3/2&nbsp;provided that&nbsp;SO does its job =
correctly.=20
So, my questions&nbsp;are as follows: Why is not p-orbital&nbsp;of =
fcc-Th in the=20
energy interval (-25eV, -13eV) within GGA+SO&nbsp;splitted to p1/2 and =
p3/2, and=20
how can it be done?&nbsp; Why is not the command of "run_lapw -so"=20
meaningless,&nbsp;although imposing magnetic moment also has not shown =
an effect=20
on splitting?</SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">Thank you for your =
attention to this=20
problem.</SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: =
Arial">Your,</SPAN><o:p></o:p></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">S. =
Jalali.</SPAN><o:p></o:p></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><o:p><FONT =
face=3D"Times New Roman"=20
size=3D3>&nbsp;</FONT></o:p></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><o:p><FONT =
face=3D"Times New Roman"=20
size=3D3>&nbsp;</FONT></o:p></P>
<P><FONT face=3D"Times New Roman" =
size=3D3></FONT></FONT></SPAN><o:p><FONT=20
face=3D"Times New Roman" =
size=3D3></FONT></o:p>&nbsp;</P></FONT></DIV></BODY></HTML>

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------------------------------

Date: Wed, 31 Jul 2002 20:35:05 +0900
From: =?ks_c_5601-1987?B?wMy9wsO2?= <leesc@kist.re.kr>
Subject: [WIEN]: lattice parameter and bulk modulus of hcp & fcc WC

====
=?ks_c_5601-1987?B?wMy9wsO2?= <leesc@kist.re.kr>
submitted the following contribution:
====

Dear WIEN2k users,

I am novice in ab initio calculation.

Now, I'm trying tocalculate energetics of hexagonal and fcc(NaCl) WC system. 

After lattice parameter optimization, I compared the equilibrium lattice parameter of both cases to experimental results.

1) hcp WC: lattice parameter a=5.49 au(Exp.)  5.43 (This Calculation)
                                           c=5.30
                  bulk modulus         329GPa (Exp.)  382 (This Calculation)

2) fcc WC: lattice paramter a =  8.00 au (Exp.)  8.28 au (This Calculation)
                 bulk modulus          319 GPa (LMTO) 378 GPa (This Calculation)

I think this discrepancy with the experimetal result is somehow large.

To check the reliability of my calculation, I calculated hexagonal and fcc TiC that is the same strucure with the WC.

In the TiC case, experiments and calculation results showed 0.1 % or less discrepancy.

Is there another additional parameter should be included in WC case?

As a reference, my initial condition is as follows,

W RMT=2.0, C RMT= 1.7

700 kpoints

RKmax=7

Energy window Emin= -7.0 Emax=3.5 in case.in1

Other parameters are the same as a standard input.

In my personal experiences, W is a difficult material to treat. It convergence properties were poor.

Thank you in advance.

Seung-Cheol Lee, Ph. D.
Research Scientist
Supercomputational Materials Simulation Lab.
Future Technology Research Division 
Korea Institute of Science and Technology
PO Box 131, Cheongryang, Seoul 130-650, KOREA
Tel) 82-2-958-6759 Fax) 82-2-958-5509
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------------------------------

Date: Thu, 01 Aug 2002 15:17:48 +0800
From: Kulkova <kulkova@ms.tsc.ru>
Subject: Re: [WIEN]: lattice parameter and bulk modulus of hcp & fcc WC

====
Kulkova <kulkova@ms.tsc.ru>
submitted the following contribution:
====

<HTML>
Dear Dr.Lee,

<P>In order to get good bulk modulus for hcp system the additional c/a
optimization for every volume must be also performed. I checked this procedure
for hcp BN.

<P>Regards

<P>Svetlana Kulkova

<P>&nbsp;
<BR><B>Prof. Dr. Svetlana E. Kulkova</B>
<BR><B>Russian Academy of Science</B>
<BR><B>Institute of Strength Physics and Material Science</B>
<BR><B>Russia, 634021 Tomsk</B>
<BR><B><FONT COLOR="#000000">pr.Akademichesky 2/1</FONT></B>
<BR><B><FONT COLOR="#000000">E-mail : kulkova@ispms.tsc.ru, kulkova@ms.tsc.ru</FONT></B>
<BR><B><FONT COLOR="#000000">My website:</FONT></B>
<BR><B><A HREF="http://www.ispms.tsc.ru/eng/kulkova.shtml">http://www.ispms.tsc.ru/eng/kulkova.shtml</A></B>
<BR>_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/_/ _/_/_/
<BR>&nbsp;</HTML>

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------------------------------

Date: Thu, 1 Aug 2002 16:03:28 +0200 (CEST)
From: =?iso-8859-1?q?youcef=20cherchab?= <cherchab@yahoo.fr>
Subject: [WIEN]: helpfull

====
=?iso-8859-1?q?youcef=20cherchab?= <cherchab@yahoo.fr>
submitted the following contribution:
====

Hello ,
  I had a question about the ZnO -DOS 
 I've had some problems with input data
for getting a best result  Idon't know what I can do
for this 
my list input:RMT(Zn)=2.1
              RMT(o)=1.5
               R*Kmax=8
               Lmax=10
for wurzite and zinc blend structure
 is wonder if anyone had somesuggestions/input.
  
  Any suggestions or help?

Thanks in advance,

Cherchab



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------------------------------

End of wien-digest V2002 #29
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #30
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
Errors-To: owner-wien-digest@theochem.tuwien.ac.at
Precedence: bulk


wien-digest        Saturday, August 10 2002        Volume 2002 : Number 030




----------------------------------------------------------------------

Date: Thu, 1 Aug 2002 20:50:38 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: Electron density plotting

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

When I used w2web to plot the electron density for my crystal
tugtupite after the SCF was done using parallization mode (11 cycles),
I found that there was no the file "tugtupite.in2" although there exists
the following files:

tugtupite.in2_ls   tugtupite.in2_st   tugtupite.in2_sy  tugtupite.in2c

Then, I copied tugtupite.in2_st as "tugtupite.in2" file and run other
steps such as lapw2, lapw5. Finally I run rhoplot, however, I was told there was
no "tugtupite.vector" file although there exist the following files:

tugtupite.vector     tugtupite.vector_2   tugtupite.vector_4
tugtupite.vector_6
tugtupite.vector_1   tugtupite.vector_3   tugtupite.vector_5
tugtupite.vector_7

After I checked the file "tugtupite.vector", I found it was a empty file,
nothing there.

So my questions are:

1. why are there no files tugtupite.in2 and tugtupite.vector?
2. How can I get the electron density plot for tugtupite?

Thanks!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Fri, 2 Aug 2002 13:21:56 +0900
From: ARAI Masao <arai.masao@nims.go.jp>
Subject: [WIEN]: sumpara (Intel Fortran on Linux/x86)

====
ARAI Masao <arai.masao@nims.go.jp>
submitted the following contribution:
====

Dear Wien users and developers,

The sumpara fails to execute on my environment(Intel Fortran on Linux/x86). 
On other enviroments(Compaq Fortran/Alpha), it works without problems.

If I understand correctly, It occurs due to undefined strings in sumpara.f
and/or bug in the Intel Fortran Compiler.

From lapw2para, sumpara is executed twice.
First time as 
    % sumpara sumpara.def 2
and second time as
    % sumpara sumpara_vresp.def 2
(Here, I assume parallel execution on two machines.)

In second execution, the content of sumara_vresp.def is as follows.

 6,'case.outputsum',   'unknown','formatted',0
17,'case.vrespval',    'unknown','formatted',0
20,'case.struct',    'old',    'formatted',0
21,'case.scf2',      'unknown','formatted',0
22,'case.scf2p',       'unknown','formatted',0

In sumpara,f line 98 to 113,

     98       idu=0
     99  783  CONTINUE
    100          READ (1,*,END=784,ERR=960) IUNIT,FNAME,STATUS,FORM,IRECL
    101          OPEN (IUNIT,FILE=FNAME,STATUS=STATUS,FORM=FORM,ERR=920)
    102          IF(IUNIT.EQ.8)  scfdmatFN=FNAME
    103          IF(IUNIT.EQ.17) CLMFN=FNAME
    104          IF(IUNIT.EQ.21) SCFFN=FNAME
    105          IF(IUNIT.EQ.22) SCFALL=FNAME
    106 
    107          IF(IUNIT.EQ.10) dmatFN10=FNAME
    108          IF(IUNIT.EQ.11) dmatFN11=FNAME
    109          IF(IUNIT.EQ.12) dmatFN12=FNAME
    110          IF(IUNIT.EQ.11) idu=2
    111       GOTO 783
    112  784  CONTINUE
    113       CLOSE (1)

the statements from line 107 to 110 are not executed because file numbers 10,11,12
are not defined. Therefore, dmatFN10, dmatFN11, dmatFN12 are undefined.

From line 313 to 321, 

    313       DO II=1,IPROC
    314          write(6,*)'DMAT summation of file ',II
    315          DO ifile=0,idu
    316             close(10+ifile)
    317             IF(ifile==0) dmatfn=dmatfn10
    318             IF(ifile==1) dmatfn=dmatfn11
    319             IF(ifile==2) dmatfn=dmatfn12
    320             call mknam(FNAME,dmatFN,II)
    321             OPEN(10+ifile,FILE=FNAME,STATUS='unknown',FORM='formatted',err=200)
    322             write(6,*)FNAME

The undefined dmatfn10 is used here, which seems to cause trouble on my enviroment
(Intel Fortran Compiler onf Linux/x86). On other enviroments, I think that undefined
FNAME causes I/O error on 321 and execution moves to "200". But it is not the case for
Intel Fortran and the execution continues to next lines.

If I insert initialization of dmatFN10 before line 99, sumpara executes without errors.

     98       idu=0
     99       dmatFN10 = "This_file_should_not_exist"
    100  783  CONTINUE

- -- 
Masao ARAI
National Institute for Materials Science (NIMS)
 Tel: 0298-51-3354 ext.504 (+81-298-51-3354 ext.504)
 Fax: 0298-52-7449 (+81-298-52-7449)
mail: arai.masao@nims.go.jp
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------------------------------

Date: Fri, 02 Aug 2002 12:41:39 -0500
From: Pablo de la Mora <delamora@servidor.unam.mx>
Subject: [WIEN]: Total energy

====
Pablo de la Mora <delamora@servidor.unam.mx>
submitted the following contribution:
====

Dear Wien Users,
    Many timies that I am running a case the total energy jumps to a 
crazy value, for example
:ENE  : ********** TOTAL ENERGY IN Ry =       -85889.063569
:ENE  : ********** TOTAL ENERGY IN Ry =       -85888.376196
...
:ENE  : ********** TOTAL ENERGY IN Ry =       -85914.716059
:ENE  : ********** TOTAL ENERGY IN Ry =       -85899.505409
:ENE  : ********** TOTAL ENERGY IN Ry =     -1129079.435723
:ENE  : ********** TOTAL ENERGY IN Ry =     -1129079.071157
...
:ENE  : ********** TOTAL ENERGY IN Ry =     -1129163.301102
:ENE  : ********** TOTAL ENERGY IN Ry =     -1129103.852864

    The jump happened when after noticing that the run was not 
converging, then I cleaned the directory (clean_lapw) and did a 'restore 
- -f -d conv init' (I had done a 'save_lapw' of the initial files). I 
changed the Broyden mixing factor and restarted the run, then the energy 
value had jumped. after this the energy stayed around this arbitrary 
large value.
    This has happened in many other cases.
    Yours

        Pablo de la Mora

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------------------------------

Date: Fri, 2 Aug 2002 16:33:21 -0400
From: Pierre Carrier <carriepi@MAGELLAN.UMontreal.CA>
Subject: [WIEN]: Physical units of <case>.m1 and <case>.m2

====
Pierre Carrier <carriepi@MAGELLAN.UMontreal.CA>
submitted the following contribution:
====

Dear Wien users,

The two files <case>.m1 and <case>.m2 give (the square of) the l+1 and l-1
energy dependent dipole matrix elements, as explained in the manual. What
are the physical units of these files ? I don't find it in the manual. The
first column is very likely in eV, but the second ?

Thanks in advance,

Best regards,
Pierre

- ---------------------------------------------------------------------
Pierre Carrier                                Tel: 514-343-6111 #4226
Bureau A-407                                  Fax: 514-343-2071
Département de physique              Boite vocale: 514-409-2238
Université de Montréal
C.P. 6128, succursale Centre-ville
Montréal, QC, H3C 3J7
Canada                                    Pierre.Carrier@UMontreal.CA
                                http://www.esi.umontreal.ca/~carriepi
- ---------------------------------------------------------------------


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Date: Fri, 02 Aug 2002 18:06:48 -0500
From: Pablo de la Mora <pm@fciencias.unam.mx>
Subject: Re: [WIEN]: Total energy

====
Pablo de la Mora <pm@fciencias.unam.mx>
submitted the following contribution:
====

Dear Wien Users,
    I updated the WIEN version from  WIEN2k_01 WIEN2k_02 and rerun a 
cycle and the normal energy returned. So it seems that it was a problem 
of older versions.
    If this problem returns I will bother you again.

        Pablo de la Mora

Pablo de la Mora wrote:

> ====
> Pablo de la Mora <delamora@servidor.unam.mx>
> submitted the following contribution:
> ====
>
> Dear Wien Users,
>    Many timies that I am running a case the total energy jumps to a 
> crazy value, for example
> :ENE  : ********** TOTAL ENERGY IN Ry =       -85889.063569
> :ENE  : ********** TOTAL ENERGY IN Ry =       -85888.376196
> ...
> :ENE  : ********** TOTAL ENERGY IN Ry =       -85914.716059
> :ENE  : ********** TOTAL ENERGY IN Ry =       -85899.505409
> :ENE  : ********** TOTAL ENERGY IN Ry =     -1129079.435723
> :ENE  : ********** TOTAL ENERGY IN Ry =     -1129079.071157
> ...
> :ENE  : ********** TOTAL ENERGY IN Ry =     -1129163.301102
> :ENE  : ********** TOTAL ENERGY IN Ry =     -1129103.852864
>
>    The jump happened when after noticing that the run was not 
> converging, then I cleaned the directory (clean_lapw) and did a 
> 'restore -f -d conv init' (I had done a 'save_lapw' of the initial 
> files). I changed the Broyden mixing factor and restarted the run, 
> then the energy value had jumped. after this the energy stayed around 
> this arbitrary large value.
>    This has happened in many other cases.
>    Yours
>
>        Pablo de la Mora
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>


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------------------------------

Date: Fri, 2 Aug 2002 22:39:10 -0400 (EDT)
From: Igor Mazin <mazin@dave.nrl.navy.mil>
Subject: Re: [WIEN]:Spam alert

====
Igor Mazin <mazin@dave.nrl.navy.mil>
submitted the following contribution:
====

For many years I was careful not to have my e-mail address accessible
for spammers' harvesting robots. Last month I signed up for the WIEN
list, having forgotten that thetraffic is being posted on the web.
Sure enough, as of today my mailbox receives up to 12 spam messages
which makes my life miserable. I travel a lot, often have bad connection
to the Internet, and now I cannot get to my mail because ofthe flood spam.

SOMETHING HAS TO BE DONE! I do not know what, I'll think,
let's think together, but our mails SHOULD NOT APPEAR on the web!

For the moment being, I will really, really appreciate, if Peter
or Georg would  make %s/dave.nrl.navy.mil/dave\.nrl\.navy\.ml,
or something similar. Then at least I have a chance that this 
spam flood will dry out in few months. Please, please!i

Sorry, sorry for an offtopic,

Igor
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------------------------------

Date: Fri, 2 Aug 2002 08:54:16 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Does -so split automatically p to its partial relativistic states?

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0012_01C23A02.2ED76990
Content-Type: text/plain;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

Dear wien users,
This is to answer the following dirty question of mine!
>Why is not p-orbital of fcc-Th in the energy interval (-25eV, -13eV) =
within GGA+SO splitted to p1/2 and p3/2, and how can it be >done?
It is if one does not FORGET to add -so switch to lapw2 -qtl command: x =
lapw2 -qtl -so!!!
Your,
S. Jalali.

- ------=_NextPart_000_0012_01C23A02.2ED76990
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML xmlns:o =3D "urn:schemas-microsoft-com:office:office"><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV>Dear wien users,<BR>This is to answer the following dirty question =
of=20
mine!</DIV>
<DIV><SPAN style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">&gt;Why is not =
p-orbital&nbsp;of=20
fcc-Th in the energy interval (-25eV, -13eV) within GGA+SO&nbsp;splitted =
to p1/2=20
and p3/2, and how can it be &gt;done?</SPAN></SPAN></DIV>
<DIV><SPAN style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">It is if one does not =
FORGET to add=20
- -so switch to lapw2 -qtl command: x lapw2 -qtl =
- -so!!!</SPAN></SPAN></DIV>
<DIV><SPAN style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">Your,</SPAN></SPAN></DIV>
<DIV><SPAN style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">S.=20
Jalali.</SPAN></SPAN></DIV></BODY></HTML>

- ------=_NextPart_000_0012_01C23A02.2ED76990--

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------------------------------

Date: Fri, 2 Aug 2002 23:22:34 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: STDOUT

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started "Electron density" and got this message
in "X Lapw2-up"  LAPW2-Error. what dose it mean?
Thank you for the guide.
H-Salehi 


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Date: Sun, 4 Aug 2002 04:29:11 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: Re: [WIEN]: STDOUT

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====


- --- hamid salehi <salehihamid@yahoo.com> wrote:
> ====
> hamid salehi <salehihamid@yahoo.com>
> submitted the following contribution:
> ====
> 
> Dear wien users.
> Ihave started "Electron density" and got this
> message
> in "X Lapw2-up"  LAPW2-Error. what dose it mean?
> Thank you for the guide.
> H-Salehi 
> 
> 
> __________________________________________________
> Do You Yahoo!?
> Yahoo! Health - Feel better, live better
> http://health.yahoo.com
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Date: Sun, 4 Aug 2002 14:15:42 +0200
From: "Dr. Alexander Hofmann" <ah@chemie.hu-berlin.de>
Subject: Re: [WIEN]:Spam alert

====
"Dr. Alexander Hofmann" <ah@chemie.hu-berlin.de>
submitted the following contribution:
====

Dear Igor,

I'm also subscribed to WIEN list (since ~3 months with my new email adress)
and I'm receiving NO spam.
Perhaps for two reasons (additions are welcome):
- - My top level domain is another (.de). So robots are 'intelligent'
- - The source of your email address is another than WIEN.

With best regards

Alex
- -- 

Dr. Alexander Hofmann

Humboldt-Universitaet zu Berlin
Institut fuer Chemie
Arbeitsgruppe Quantenchemie

Brook-Taylor-Strasse 2

12489 Berlin

ah@chemie.hu-berlin.de

Tel.: +49-30-2093-7138
Fax.: +49-30-2093-7136

http://www.chemie.hu-berlin.de/ag_sauer/index.html

PGP-Key: wwwkeys.de.pgp.net ID: D9D62D35
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Date: Sun, 4 Aug 2002 06:12:22 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: DOs

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started DOs and got this message in LAPW2-qtl
Error. what dose it mean?
Thank you for the guide.
H-Salehi 


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Date: Sun, 4 Aug 2002 15:16:49 +0200 (MEST)
From: Ravindran Ponniah <ravindran.ponniah@kjemi.uio.no>
Subject: Re: [WIEN]:Spam alert

====
Ravindran Ponniah <ravindran.ponniah@kjemi.uio.no>
submitted the following contribution:
====

On Fri, 2 Aug 2002, Igor Mazin wrote:

> ====
> Igor Mazin <mazin@dave.nrl.navy.mil>
> submitted the following contribution:
> ====
>
> For many years I was careful not to have my e-mail address accessible
> for spammers' harvesting robots. Last month I signed up for the WIEN
> list, having forgotten that thetraffic is being posted on the web.
> Sure enough, as of today my mailbox receives up to 12 spam messages
> which makes my life miserable. I travel a lot, often have bad connection
> to the Internet, and now I cannot get to my mail because ofthe flood spam.
>
> SOMETHING HAS TO BE DONE! I do not know what, I'll think,
> let's think together, but our mails SHOULD NOT APPEAR on the web!
>
> For the moment being, I will really, really appreciate, if Peter
> or Georg would  make %s/dave.nrl.navy.mil/dave\.nrl\.navy\.ml,
> or something similar. Then at least I have a chance that this
> spam flood will dry out in few months. Please, please!i
>
> Sorry, sorry for an offtopic,

Dear Igor,

	I am also having the problem of receiving almost 10 spam
mails per day. Using exim filter I am able to solve the problem
(i.e. morethan 90% of the spam mails are filtered out). If you
are interested to filter out your spam mails, I can send to you the
necessary instructions in a seperate email.

	I feel that one of the possibility of getting the email
address by the spammers from the papers we publish with our email address.

Best regards
Ravi

***********************************************************
Dr.P.Ravindran, Department of Chemistry|Tel: +47 22 85 56 06
University of Oslo, PO Box 1033        |Fax: +47 22 85 54 41/55 65
Blindern, N-0315 OSLO, NORWAY          |
Email: ravindran.ponniah@kjemi.uio.no  |
URL : http://folk.uio.no/~ravi/        |
************************************************************

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------------------------------

Date: Sun, 4 Aug 2002 12:01:47 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: lapw1 problem

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

After the first SCF calculation, it always crashed in running lapw1 in
second cycle no matter how hard I tried using WIEN2k_02.

I tried the parallization and single mode, the results are same, both
crashed at the same place, and I was told "STOP SELECT Error". I changed
the mixer vaule to 0.001 and switched BROYD to PRATT, but the calculation
was still crashed with the same problem.

So my questions are:
1. what might be the reasons caused the crashing in lapw1 with the message
"STOP SELECT Error"?
2. How can I remede the problem?

Thanks in advance!

Best wishes!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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Date: Mon,  5 Aug 2002 11:55:11 +1000
From: chen0130@flinders.edu.au
Subject: [WIEN]: Some questions

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Dear Wien,

I have some general simple questions,

1) I haven't been able to have SCF run more than 20 iterations, can I extend
this by some parameter, or is this the max that Wien will do. I haven't been
able to find any clues on this yet.

2) In my slab calculation, the total energy has :WARNING: befor announcing the
value. Can anyone tell me what this means,

eg :ENE  : *WARNING** TOTAL ENERGY IN Ry =        -1745.650010

Thanks,

Cheng Chen
	


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Date: Sun, 4 Aug 2002 23:12:53 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: Some questions -- answer to 1)

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====

> 1) I haven't been able to have SCF run more than 20 iterations, can I
> extend this by some parameter, or is this the max that Wien will do. I
> haven't been able to find any clues on this yet.

Yes. This is in the userguide in Chapter 5: Shell scripts for running 
programs. More specifically, it is page 50-51 in my version of the
userguide. You control the maximum number of iterations with the flag -i for 
run_lapw. So, if you wanted a maximum of 100 iterations you would run
run_lapw -i 100 and all the other options you would add.

In w2web I believe you can pass these through the "expert options" in
the run SCF menu.

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Date: Mon, 05 Aug 2002 14:36:23 +0430
From: Payami Mahmoud <mpayami@aeoi.org.ir>
Subject: [WIEN]: PGFIO error

====
Payami Mahmoud <mpayami@aeoi.org.ir>
submitted the following contribution:
====

Dear Wieners,

In execution of "xdstart" for Al_2 O_3 struct-file contained in exaples, 
I encountered the message:
 " PGFIO-F-231 /formatted read /unit=15 /error on data conversion"

Any suggestion is highly appreciated.

M. Payami


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Date: Mon, 5 Aug 2002 11:20:29 +0100
From: Andrew Scott <a.j.scott@leeds.ac.uk>
Subject: Re: [WIEN]: PGFIO error

====
Andrew Scott <a.j.scott@leeds.ac.uk>
submitted the following contribution:
====

I believe this may be a problem with the compiler.  See Dave Pankhurst's
contribution to the FAQ on the WIEN2K web-site.

Andrew.

 ________________________________________________
 Dr. Andrew Scott,
 Department of Materials,
 School of Process, Environmental and Materials Engineering,
 University of Leeds,
 Leeds LS2 9JT, U.K. 
 
 E-mail: a.j.scott@leeds.ac.uk
 Tel:  44 + (0)113 233 2573
 
 http://www.lemas.co.uk
 http://www.materials.leeds.ac.uk/lemas
 ________________________________________________


On Mon, 5 Aug 2002, Payami Mahmoud wrote:

> ====
> Payami Mahmoud <mpayami@aeoi.org.ir>
> submitted the following contribution:
> ====
> 
> Dear Wieners,
> 
> In execution of "xdstart" for Al_2 O_3 struct-file contained in exaples, 
> I encountered the message:
>  " PGFIO-F-231 /formatted read /unit=15 /error on data conversion"
> 
> Any suggestion is highly appreciated.
> 
> M. Payami
> 
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 

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------------------------------

Date: Mon, 05 Aug 2002 17:30:39 +0430
From: Payami Mahmoud <mpayami@aeoi.org.ir>
Subject: Re: [WIEN]: PGFIO error

====
Payami Mahmoud <mpayami@aeoi.org.ir>
submitted the following contribution:
====

Dear Andrew,

Thank you very much for your suggestion. I checked the ftp-site 
mentioned in FAQ and downloaded the patch files. I try to manage fixing 
this problem.

Kind regards,

M. Payami


Andrew Scott wrote:

>====
>Andrew Scott <a.j.scott@leeds.ac.uk>
>submitted the following contribution:
>====
>
>I believe this may be a problem with the compiler.  See Dave Pankhurst's
>contribution to the FAQ on the WIEN2K web-site.
>
>Andrew.
>
> ________________________________________________
> Dr. Andrew Scott,
> Department of Materials,
> School of Process, Environmental and Materials Engineering,
> University of Leeds,
> Leeds LS2 9JT, U.K. 
> 
> E-mail: a.j.scott@leeds.ac.uk
> Tel:  44 + (0)113 233 2573
> 
> http://www.lemas.co.uk
> http://www.materials.leeds.ac.uk/lemas
> ________________________________________________
>
>
>On Mon, 5 Aug 2002, Payami Mahmoud wrote:
>
>>====
>>Payami Mahmoud <mpayami@aeoi.org.ir>
>>submitted the following contribution:
>>====
>>
>>Dear Wieners,
>>
>>In execution of "xdstart" for Al_2 O_3 struct-file contained in exaples, 
>>I encountered the message:
>> " PGFIO-F-231 /formatted read /unit=15 /error on data conversion"
>>
>>Any suggestion is highly appreciated.
>>
>>M. Payami
>>
>>
>>====
>>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>>To (un)subscribe send mail to
>>majordomo@zeus.theochem.tuwien.ac.at
>>====
>>
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>


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------------------------------

Date: Tue, 06 Aug 2002 08:05:36 +0430
From: Payami Mahmoud <mpayami@aeoi.org.ir>
Subject: Re: [WIEN]: PGFIO error

====
Payami Mahmoud <mpayami@aeoi.org.ir>
submitted the following contribution:
====

Dear Andrew,

There was a small error in the symbol used for oxygen in the 
"case.struct". It was similar to
a prolate one. The "case.inst" was:
Al
Ne 2 5
3, -1, 1.0 N
3, -1, 1.0 N
3,  1, 1.0 N
3,  1, 0.0 N
Warning: Specified Element not in database!
**** End of input
**** End of input

But after retyping the symbol "O", the information of the oxygen atom 
was added to this file and the "PGFIO-error" was disappeared.

Thank you again!

Mahmoud

Andrew Scott wrote:

>====
>Andrew Scott <a.j.scott@leeds.ac.uk>
>submitted the following contribution:
>====
>
>I believe this may be a problem with the compiler.  See Dave Pankhurst's
>contribution to the FAQ on the WIEN2K web-site.
>
>Andrew.
>
> ________________________________________________
> Dr. Andrew Scott,
> Department of Materials,
> School of Process, Environmental and Materials Engineering,
> University of Leeds,
> Leeds LS2 9JT, U.K. 
> 
> E-mail: a.j.scott@leeds.ac.uk
> Tel:  44 + (0)113 233 2573
> 
> http://www.lemas.co.uk
> http://www.materials.leeds.ac.uk/lemas
> ________________________________________________
>
>
>On Mon, 5 Aug 2002, Payami Mahmoud wrote:
>
>>====
>>Payami Mahmoud <mpayami@aeoi.org.ir>
>>submitted the following contribution:
>>====
>>
>>Dear Wieners,
>>
>>In execution of "xdstart" for Al_2 O_3 struct-file contained in exaples, 
>>I encountered the message:
>> " PGFIO-F-231 /formatted read /unit=15 /error on data conversion"
>>
>>Any suggestion is highly appreciated.
>>
>>M. Payami
>>
>>
>>====
>>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>>To (un)subscribe send mail to
>>majordomo@zeus.theochem.tuwien.ac.at
>>====
>>
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>


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------------------------------

Date: Tue, 6 Aug 2002 01:05:08 -0700
From: "saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Some questions -- answer to 2

====
"saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> 2) In my slab calculation, the total energy has :WARNING: befor announcing
the
> value. Can anyone tell me what this means,
>
> eg :ENE  : *WARNING** TOTAL ENERGY IN Ry =        -1745.650010

You would try to look for in the mailing-list an e-mail from Stefaan with
the subject of Jumps, and the responses to him from Torsten and Pavel.
I paste below a related part of them:

">I don't know it that is a hint, but the warning in the :ENE line I had
>the other day. Increasing NMATMAX removed it. Don't you have a warning
>that rkmax is reduced somewhere in your scf file?
No. There are two reasons why there can be printed a **WARNING** in the :ENE
line: Rkmax which is reduced, and a bad integration which produces a :WAR
line. My :RKM line stays the same everywhere, and I have the **WARNING**
only
in that iteration where there is also a :WAR present. Obviously this is due
to
the second reason, bad integration."

Your,
S. Jalali.




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Date: Tue, 06 Aug 2002 16:04:30 +0430
From: Payami Mahmoud <mpayami@aeoi.org.ir>
Subject: [WIEN]: Problem with plot

====
Payami Mahmoud <mpayami@aeoi.org.ir>
submitted the following contribution:
====

Dear Wieners,

Using Wien2k-02, I have never succeeded in "Click & Plot" of the density 
or DOS and always I receive the message:
"Error- File not found or temporary file does not exist anymore".
But it is possible to call from a command shell the gnuplot and plot them.
Should I configure my W2WEB or something else? How?
Suggestions are highly appreciated.

Best regards,

M. Payami


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------------------------------

Date: Tue, 6 Aug 2002 14:35:26 +0200 (MEST)
From: buero@luitz.at
Subject: Re: [WIEN]: Problem with plot

====
buero@luitz.at
submitted the following contribution:
====

On Tue, 6 Aug 2002, Payami Mahmoud wrote:

> "Error- File not found or temporary file does not exist anymore".
> But it is possible to call from a command shell the gnuplot and plot them.
> Should I configure my W2WEB or something else? How?


Can your gnuplot version produce PNG graphics? If not, it is clear it
cannot find the appropriate file. Running gnuplot from the commandline
produces graphics on your X11 device.

In gnuplot try
help set terminal png

If you get an answer like "Sorry, no help for 'set terminal png', you
should upgrade your gnuplot.

Regards
  Joachim

 /---------------------------------------------------------\
(  luitz.at - Interfacing Art, Science and Technology       )
 )---------------------------------------------------------(
(  Büro für Informationstechnologie                         \
 ) und Technisches Büro für Technische Chemie                )
(  Dipl.-Ing. Joachim Luitz KEG         Tel: 022  31 61254  (
 ) Wohlmuthgasse 18                          0676 31 61254   )
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------------------------------

Date: Tue, 6 Aug 2002 15:05:53 -0400 (EDT)
From: Igor Mazin <mazin@dave.nrl.navy.mil>
Subject: Re: [WIEN]:Spam alert

====
Igor Mazin <mazin@dave.nrl.navy.mil>
submitted the following contribution:
====

Hi,

I never publish my e-mail with my papers, but I do not
think the papers are normally accessible by robots. These are
mostly primitive and do not serach the pdf files.

I do use procmail, but I found it rather annoying
to tune to all possible spam patterns.

Igor

> 
> ====
> Ravindran Ponniah <ravindran.ponniah@kjemi.uio.no>
> submitted the following contribution:
> ====
> 
> On Fri, 2 Aug 2002, Igor Mazin wrote:
> 
> > ====
> > Igor Mazin <mazin@dave.nrl.navy.mil>
> > submitted the following contribution:
> > ====
> >
> > For many years I was careful not to have my e-mail address accessible
> > for spammers' harvesting robots. Last month I signed up for the WIEN
> > list, having forgotten that thetraffic is being posted on the web.
> > Sure enough, as of today my mailbox receives up to 12 spam messages
> > which makes my life miserable. I travel a lot, often have bad connection
> > to the Internet, and now I cannot get to my mail because ofthe flood spam.
> >
> > SOMETHING HAS TO BE DONE! I do not know what, I'll think,
> > let's think together, but our mails SHOULD NOT APPEAR on the web!
> >
> > For the moment being, I will really, really appreciate, if Peter
> > or Georg would  make %s/dave.nrl.navy.mil/dave\.nrl\.navy\.ml,
> > or something similar. Then at least I have a chance that this
> > spam flood will dry out in few months. Please, please!i
> >
> > Sorry, sorry for an offtopic,
> 
> Dear Igor,
> 
> 	I am also having the problem of receiving almost 10 spam
> mails per day. Using exim filter I am able to solve the problem
> (i.e. morethan 90% of the spam mails are filtered out). If you
> are interested to filter out your spam mails, I can send to you the
> necessary instructions in a seperate email.
> 
> 	I feel that one of the possibility of getting the email
> address by the spammers from the papers we publish with our email address.
> 
> Best regards
> Ravi
> 
> ***********************************************************
> Dr.P.Ravindran, Department of Chemistry|Tel: +47 22 85 56 06
> University of Oslo, PO Box 1033        |Fax: +47 22 85 54 41/55 65
> Blindern, N-0315 OSLO, NORWAY          |
> Email: ravindran.ponniah@kjemi.uio.no  |
> URL : http://folk.uio.no/~ravi/        |
> ************************************************************
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 


- -- 
*****************************************************************************
Igor Mazin, NRL, code 6391, 4555 Overlook Ave SW, Washington, DC 20375-5320
Phone: (202) 767-6990; Fax: (202) 404-7546; e-mail mazin@dave.nrl.navy.mil
Home Page (under construction) http://cst-www.nrl.navy.mil/~mazin
*****************************************************************************

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------------------------------

Date: Tue, 6 Aug 2002 18:46:46 -0300 (ARST)
From: Fabian Dominguez <fabian@iflysib.unlp.edu.ar>
Subject: [WIEN]: Ndfeb - convergence 

====
Fabian Dominguez <fabian@iflysib.unlp.edu.ar>
submitted the following contribution:
====


Dear  Dr. Blaha:

Trying to run ndfeb, with 68 atoms per unit cell I found that I can't do
:DIS lower than 0.0055 or 0.0056 but energies values are like this, this
the las cycle done where 3 iterations are done and then It stops
:ENE  : ********** TOTAL ENERGY IN Ry =      -296439.449779
:ENE  : ********** TOTAL ENERGY IN Ry =      -296439.449790
:ENE  : ********** TOTAL ENERGY IN Ry =      -296439.449775

Dr Blaha: I use rkmax =5 and 6 point in IBZ, corrisponding 40 points in
total BZ.
I know this is not the best choice but greater values of these
parameters makes lapw1 rather longer or if I try with rkmax =7 u 8 even 6.
or more k-points.
I comment this in a previous mail before starting calculation and you
sugest me to do this , I mean get lower rkmax and get higher the number of
k-points.

Is is possible that the best convergence degree reached with these
parameters is this order...

best regards,
Fabian

============================***=================================

Lic. Fabian Alfredo Dominguez Avenalle.
Instituto de Fisica de Liquidos y Sistemas Biologicos (IFLYSIB).
Universidad Nacional de La Plata (UNLP).
Calle 59 N 789 La Plata CP.  1900  BUENOS AIRES  ARGENTINA
CC. 565
TE: 0221-4233283
TELEFAX: 0221-4257317
E-MAIL: fabian@iflysib.unlp.edu.ar
============================***=================================

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------------------------------

Date: Wed,  7 Aug 2002 10:39:00 +1000
From: chen0130@flinders.edu.au
Subject: Re: [WIEN]: Some questions -- thankyou

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Thanks saeid Jalali so much for you help, and also to Fred Nastos for answer to
my first question!

Gratefully yours

Cheng Chen

Quoting saeid Jalali <sjalali@cc.iut.ac.ir>:

> ====
> "saeid Jalali" <sjalali@cc.iut.ac.ir>
> submitted the following contribution:
> ====
> 
> > 2) In my slab calculation, the total energy has :WARNING: befor
> announcing
> the
> > value. Can anyone tell me what this means,
> >
> > eg :ENE  : *WARNING** TOTAL ENERGY IN Ry =        -1745.650010
> 
> You would try to look for in the mailing-list an e-mail from Stefaan with
> the subject of Jumps, and the responses to him from Torsten and Pavel.
> I paste below a related part of them:
> 
> ">I don't know it that is a hint, but the warning in the :ENE line I had
> >the other day. Increasing NMATMAX removed it. Don't you have a warning
> >that rkmax is reduced somewhere in your scf file?
> No. There are two reasons why there can be printed a **WARNING** in the
> :ENE
> line: Rkmax which is reduced, and a bad integration which produces a :WAR
> line. My :RKM line stays the same everywhere, and I have the **WARNING**
> only
> in that iteration where there is also a :WAR present. Obviously this is due
> to
> the second reason, bad integration."
> 
> Your,
> S. Jalali.
> 
> 
> 
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 
> 



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------------------------------

Date: Tue, 6 Aug 2002 21:28:41 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: Electron Density

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

After the running the SCF cycles using parallization mode, I tried to
draw the electronic density map. However, I found that there is no
case.in2 file in the directory although there are files such as:

tugtupite.in2_ls, tugtupite.in2_st, tugtupite.in2_sy, tugtupite.in2c

Then I found nothing in the file case.vector, i.e., it is empty, but the
following files are not empty:

tugtupite.vector     tugtupite.vector_2   tugtupite.vector_4
tugtupite.vector_6 tugtupite.vector_1   tugtupite.vector_3
tugtupite.vector_5   tugtupite.vector_7


So my question is: how can I get my electronic density map for my crystal?

Thanks in advance!


Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Tue, 6 Aug 2002 23:48:17 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: Electron Density

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====

> However, I found that there is no case.in2 file in the directory
> although there are files such as:
> 		tugtupite.in2c

Having a .in2c ending usually means that the crystal class does
not have inversion symmetry. The 'c' stands for complex and "reminds"
you that the caclulation is using complex wavefunctions.

> Then I found nothing in the file case.vector, i.e., it is empty, but the
> following files are not empty:
> 		tugtupite.vector

From what I gather from the furts part of your post, tugtupite.vector
is your case.vector file. I think if you actually have a file called 
'case.vector' there is something wrong... unless you purposely named
a calculation 'case'. The term case is used as a generic label throughout the 
manual.

> So my question is: how can I get my electronic density map for my crystal?

Use w2web, and page 22-24 of the manual. The interface knows to use the
correct files (tugtupite.in2c and tugtupite.vector in your case). At least it 
does for me.
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Date: Wed, 07 Aug 2002 08:27:32 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]:Spam alert

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Hi,

I find this discussion rather bizarre, as all mailing lists and most 
e-mails are transferred through several servers/routers/switches on 
their way from sender to recipient. Each of these places, a sniffer 
program can take out e-mail addresses, and I have not noticed any 
increase in junk mail because of the wien mailing list. Furthermore, I 
have set up a filter that takes about 9 out of 10 junk mails, since they 
usually fit a very simple pattern. Most of them are not adressed to me, 
so the first rule of the filter is that everything not addressed to me 
goes directly to trash. Next rules are exceptions from that... it also 
has the advantage that all wien mailing list postings come to a separate 
inbox.

I think using e-mail has it's risks of spamming, mostly due to people 
that could be taken out via US legislation, which they don't want to 
do... so you being in the US should contact your congressman. 
Unsolicited e-mail is already forbidden in most European countries, but 
we can't enforce it since most of that comes from the US where it is 
"free speech" although without any content. Don't blame the mailing list 
maintainers!

Sincerely,
Torsten Andersen.

Igor Mazin wrote:

>====
>Igor Mazin <mazin@dave.nrl.navy.mil>
>submitted the following contribution:
>====
>
>Hi,
>
>I never publish my e-mail with my papers, but I do not
>think the papers are normally accessible by robots. These are
>mostly primitive and do not serach the pdf files.
>
>I do use procmail, but I found it rather annoying
>to tune to all possible spam patterns.
>
>Igor
>
>>====
>>Ravindran Ponniah <ravindran.ponniah@kjemi.uio.no>
>>submitted the following contribution:
>>====
>>
>>On Fri, 2 Aug 2002, Igor Mazin wrote:
>>
>>>====
>>>Igor Mazin <mazin@dave.nrl.navy.mil>
>>>submitted the following contribution:
>>>====
>>>
>>>For many years I was careful not to have my e-mail address accessible
>>>for spammers' harvesting robots. Last month I signed up for the WIEN
>>>list, having forgotten that thetraffic is being posted on the web.
>>>Sure enough, as of today my mailbox receives up to 12 spam messages
>>>which makes my life miserable. I travel a lot, often have bad connection
>>>to the Internet, and now I cannot get to my mail because ofthe flood spam.
>>>
>>>SOMETHING HAS TO BE DONE! I do not know what, I'll think,
>>>let's think together, but our mails SHOULD NOT APPEAR on the web!
>>>
>>>For the moment being, I will really, really appreciate, if Peter
>>>or Georg would  make %s/dave.nrl.navy.mil/dave\.nrl\.navy\.ml,
>>>or something similar. Then at least I have a chance that this
>>>spam flood will dry out in few months. Please, please!i
>>>
>>>Sorry, sorry for an offtopic,
>>>
>>Dear Igor,
>>
>>	I am also having the problem of receiving almost 10 spam
>>mails per day. Using exim filter I am able to solve the problem
>>(i.e. morethan 90% of the spam mails are filtered out). If you
>>are interested to filter out your spam mails, I can send to you the
>>necessary instructions in a seperate email.
>>
>>	I feel that one of the possibility of getting the email
>>address by the spammers from the papers we publish with our email address.
>>
>>Best regards
>>Ravi
>>
>>***********************************************************
>>Dr.P.Ravindran, Department of Chemistry|Tel: +47 22 85 56 06
>>University of Oslo, PO Box 1033        |Fax: +47 22 85 54 41/55 65
>>Blindern, N-0315 OSLO, NORWAY          |
>>Email: ravindran.ponniah@kjemi.uio.no  |
>>URL : http://folk.uio.no/~ravi/        |
>>************************************************************
>>
>>====
>>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>>To (un)subscribe send mail to
>>majordomo@zeus.theochem.tuwien.ac.at
>>====
>>
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Wed, 07 Aug 2002 15:46:08 +0430
From: Payami Mahmoud <mpayami@aeoi.org.ir>
Subject: Re: [WIEN]: Problem with plot

====
Payami Mahmoud <mpayami@aeoi.org.ir>
submitted the following contribution:
====

Dear Joachim,

Thank you very much for your suggestion. I checked if my "gnuplot"  
supports "png" and     the answer is yes. I can set the terminal to png 
when I call the gnuplot in a command shell. The "libpng" and "zlib" had 
been installed. It should be mentioned that I had no "click & plot" 
problems when using the previous version, W2k_01.
The steps that I follow are:
x lapw2 -qtl
x tetra
DOSplot
The outcome is:
We are in Dosplotmode column 1 selected
Plot from atom: total DOS (file case.dos1ev)
....and no plot!
When I click "Download hardcopy in PS format",  then the mentioned error 
appears.

Should I check further for other requirements?

With best regards,

Mahmoud Payami

buero@luitz.at wrote:

>====
>buero@luitz.at
>submitted the following contribution:
>====
>
>On Tue, 6 Aug 2002, Payami Mahmoud wrote:
>
>>"Error- File not found or temporary file does not exist anymore".
>>But it is possible to call from a command shell the gnuplot and plot them.
>>Should I configure my W2WEB or something else? How?
>>
>
>
>Can your gnuplot version produce PNG graphics? If not, it is clear it
>cannot find the appropriate file. Running gnuplot from the commandline
>produces graphics on your X11 device.
>
>In gnuplot try
>help set terminal png
>
>If you get an answer like "Sorry, no help for 'set terminal png', you
>should upgrade your gnuplot.
>
>Regards
>  Joachim
>
> /---------------------------------------------------------\
>(  luitz.at - Interfacing Art, Science and Technology       )
> )---------------------------------------------------------(
>(  Büro für Informationstechnologie                         \
> ) und Technisches Büro für Technische Chemie                )
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>
>
>====
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>====
>
>


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------------------------------

Date: Wed, 7 Aug 2002 20:38:55 +0800
From: Wenhui Xie <xiewh@sun20.iphy.ac.cn>
Subject: [WIEN]: The problem in band character plot

====
Wenhui Xie <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear Sir,
     I download the new version of WIEN2K, and everything is good.
However, I do not plot the band and charater band like before.
I found that the figures of band are color figure,  which is not similar 
with the fig3.15 and 3.16 shown in User's Guide. Also, I do not plot 
the Ti t2g-like character bands. 
     Unfortunely, I have deleted the old version, now I do not know 
what's wrong happened in TiC case.  
     Thanks for any advise.
     Best Regards.
                                          Wenhui Xie


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------------------------------

Date: Wed, 7 Aug 2002 20:48:40 +0800
From: Wenhui Xie <xiewh@sun20.iphy.ac.cn>
Subject: [WIEN]: How to get the hyperfine field 

====
Wenhui Xie <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear Sir,

From the web site of WIEN2K, I know that the properties of 
electric field gradients, isomer shifts, hyperfine fields can be 
obtined from WIEN2K package. However, I do not know how to 
do.  Please tell me more detals. 
Thanks very much!

 yours sincerely
  Wenhui Xie
   
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------------------------------

Date: Wed, 7 Aug 2002 08:09:58 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: [none]

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

 
 

__________________________________________________
Do You Yahoo!?
Yahoo! Health - Feel better, live better
http://health.yahoo.com
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------------------------------

Date: Wed, 7 Aug 2002 08:53:33 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]:Spam alert

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

Hi,

I also find this discussion quite bizzare, and
particularly your reaction. If you are inetersted in
discussion of American and European political systems,
I suggest the proper avenue is via private e-mail.

To wrap it up, let me make a few points.

1) You both over- and underestimate the level of
sophistication of a typical spammer. They do not use
sniffers and similar devices reqiring hacking. They
use relatively primitive robots (crawlers) which
simply harvest e-mails from publicly availabel html
pages. While most, but not all spammers reside in the
US (and so does the overwhelming majority of
legitimate Internet businesses) they usually do not
use traceable American providers, since many states
have laws agains unsolicited e-mails, some at the
opt-out and some at the opt-in level. The main
anti-spam organisation in Europe is BTW EuroCAUCE, a
European branch of CAUCE, an antispam organization
originated in the US, more at
http://www.euro.cauce.org/en/index.html and
http://www.cauce.org/index.phtml. Unfortunately the
absolute majority of spam messages is coming with
faked headers (this is why you think they are send
from American providers) and are relayed via proxies
in China, Russia and other counries. This makes it
extremely difficult to fight scam by legal means, as
you suggest.

2)So far with the spam basic. Now, I do NOT blame the
list maintainers. There is nothing they can do. I
asked for a personal favor of having my address
cleaned out from the website. However, I do believe
that a newsgroup/discussion-club format is better, for
(i) you can follow messages by thread and (ii) you can
always give your address in a form understandable by
humans, but not robots. I know Peter is of different
opinion, and he has his own reasons.

3) You use Netscape 6.1 mailer agent, which does
indeed have a very nice filtering engine. For reasons
that are not interesting for the readeres, I use elm,
with the only option of procmailing. 

4) I just set up two test accounts, one subscribed to
the list, and one not. I will post (only once, don't
be afraid!) a message regarding the junk traffic in
both after a week or two.

Igor 

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Hi,

I find this discussion rather bizarre, as all mailing
lists and most e-mails are transferred through several
servers/routers/switches on their way from sender to
recipient. Each of these places, a sniffer program can
take out e-mail addresses, and I have not noticed any
increase in junk mail because of the wien mailing
list. Furthermore, I have set up a filter that takes
about 9 out of 10 junk mails, since they usually fit a
very simple pattern. Most of them are not adressed to
me, so the first rule of the filter is that everything
not addressed to me goes directly to trash. Next rules
are exceptions from that... it also has the advantage
that all wien mailing list postings come to a separate
inbox.

I think using e-mail has it's risks of spamming,
mostly due to people that could be taken out via US
legislation, which they don't want to do... so you
being in the US should contact your congressman.
Unsolicited e-mail is already forbidden in most
European countries, but we can't enforce it since most
of that comes from the US where it is "free speech"
although without any content. Don't blame the mailing
list maintainers!

Sincerely,
Torsten Andersen.


__________________________________________________
Do You Yahoo!?
Yahoo! Health - Feel better, live better
http://health.yahoo.com
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------------------------------

Date: Wed, 7 Aug 2002 13:20:44 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: Re: [WIEN]: Electron Density

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear Fred:

Thank you for your help!

1. During the process of init_lapw, I already set "center version" for my
crystal tugtupite, so I don't know why the tugtupite.in2 file was
still not created.

2. Yes, my case.vector is tugtupite.vector, and there also exists the file
with name "tugtupite.vector", however, it is an empty file! i.e.,

- -rw-------   1 umbingz  student        0 Jun 22 02:42 tugtupite.vector

3. I did use w2web for the electron density calculation and plotting, I
met the following problems:
(1) no file of tugtupite.in2;
(2) after I copied tugtupite.in2_st as my tugtupite.in2 file and run
"x lapw2", the following information was shown:

******  FORTRAN RUN-TIME SYSTEM  ******
 End-of-file:  -1 Location:  the READ statement at line 40 of "fermi.f"
  Unit:  30
 File:  tugtupite.energy
Abort
0.0u 0.0s 0:03 0% 0+0k 0+0io 0pf+0w

(3) Then I run the following steps, after "x -lapw5", the following
information was shown on the webpage:

39.0u 0.0s 0:39 98% 0+0k 0+0io 0pf+0w

(5) Finally I run "rhoplot", it keeps running and nothing came out on the
webpage, I am still waiting for any message from the program.


So I don't know why lapw2 is aborted, and is my EMIN=-1.0 in
tugtupite.in2 too high for my tugtupite? I will try lower EMIN to see what happens.


Thank you again!


Have a nice day!






On Tue, 6 Aug 2002, Fred Nastos wrote:
<nastos@physics.utoronto.ca> submitted the following contribution:
> > However, I found that there is no case.in2 file in the directory
> > although there are files such as:
> > 		tugtupite.in2c
>
> Having a .in2c ending usually means that the crystal class does
> not have inversion symmetry. The 'c' stands for complex and "reminds"
> you that the caclulation is using complex wavefunctions.
>
> > Then I found nothing in the file case.vector, i.e., it is empty, but the
> > following files are not empty:
> > 		tugtupite.vector
>
> From what I gather from the furts part of your post, tugtupite.vector
> is your case.vector file. I think if you actually have a file called
> 'case.vector' there is something wrong... unless you purposely named
> a calculation 'case'. The term case is used as a generic label throughout the
> manual.
>
> > So my question is: how can I get my electronic density map for my crystal?
>
> Use w2web, and page 22-24 of the manual. The interface knows to use the
> correct files (tugtupite.in2c and tugtupite.vector in your case). At least it
> does for me.
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Wed, 7 Aug 2002 15:57:59 -0400
From: Jeff Spirko <spirko@lehigh.edu>
Subject: [WIEN]: Bug in restore_lapw

====
Jeff Spirko <spirko@lehigh.edu>
submitted the following contribution:
====

restore_lapw will sometimes fail saying, "arg list too long".
It is related to a limitation in tcsh.  The line:

  set count = `ls $savedir/$savefile*|wc -l`

will fail if savedir is long and there are many files in the job.
A better way of counting the files might be:

  set count = `echo $savedir/$savefile* | wc -w`

This uses the shell builtin command echo (and wc -w), so it doesn't
encounter the same limitations.

- -- 
Jeff Spirko   spirko@lehigh.edu   spirko@yahoo.com   WD3V   |=>

The study of non-linear physics is like the study of non-elephant biology.

All theoretical chemistry is really physics;
and all theoretical chemists know it. -- Richard P. Feynman 
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------------------------------

Date: Wed, 7 Aug 2002 16:13:42 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: Electron Density

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====

> 1. During the process of init_lapw, I already set "center version" for my
> crystal tugtupite, so I don't know why the tugtupite.in2 file was
> still not created.

I'm not sure what you mean by 'I already set "center version" for my
crystal'. I believe the WIEN2k package will determine if your crystal
has inversion symmetry or not.

Could you type the following at the command prompt:

grep INVERSION tugtupite.output.s

A typical output from this is:

 PGBSYM: SPACE GROUP DOES NOT CONTAIN INVERSION

or

 PGBSYM: SPACE GROUP CONTAINS INVERSION

Could you indicate more precisely, where/how you 'set "center version"'?

> 2. Yes, my case.vector is tugtupite.vector, and there also exists the file
> with name "tugtupite.vector", however, it is an empty file! i.e.,
>
> -rw-------   1 umbingz  student        0 Jun 22 02:42 tugtupite.vector

I'm not sure why that would be empty, unless it was accidentally written
over. I'm not an expert (and barely a beginner) on the internals of 
lapw1/lapw2, but it could be that since lapw2 was abnormally aborted
(as you say below) your .vector file was left in an empty state.

> 3. I did use w2web for the electron density calculation and plotting, I
> met the following problems:
> (1) no file of tugtupite.in2;
> (2) after I copied tugtupite.in2_st as my tugtupite.in2 file and run
> "x lapw2"

I don't think that it is a good idea to create, by hand, files that WIEN2k 
provides just so that you can continue the calculation.  There is an old
saying from mine workers "figure out what killed the canary before you
continue mining."

> the following information was shown:
>
> ******  FORTRAN RUN-TIME SYSTEM  ******
>  End-of-file:  -1 Location:  the READ statement at line 40 of "fermi.f"
>   Unit:  30
>  File:  tugtupite.energy
> Abort
> 0.0u 0.0s 0:03 0% 0+0k 0+0io 0pf+0w
>
> (3) Then I run the following steps, after "x -lapw5", the following
> information was shown on the webpage:
>
> 39.0u 0.0s 0:39 98% 0+0k 0+0io 0pf+0w

Which just means the program exectued, and no abnormal exit
statement was picked up by the w2web perl script.

> (5) Finally I run "rhoplot", it keeps running and nothing came out on the
> webpage, I am still waiting for any message from the program.

You will probably not get anything, since lapw2 aborted.

> So I don't know why lapw2 is aborted, and is my EMIN=-1.0 in
> tugtupite.in2 too high for my tugtupite?

That just depends on what range of bands you want to include in
the plots. The density is, of course, Tr(rho), and Emin just allows you
to truncate the the tracing sum.

> I will try lower EMIN to see what happens.

I suggest, that instead, you find out what "killed the canary".

Fred

> Thank you again!
>
>
> Have a nice day!
>
> On Tue, 6 Aug 2002, Fred Nastos wrote:
>
> <nastos@physics.utoronto.ca> submitted the following contribution:
> > > However, I found that there is no case.in2 file in the directory
> > > although there are files such as:
> > > 		tugtupite.in2c
> >
> > Having a .in2c ending usually means that the crystal class does
> > not have inversion symmetry. The 'c' stands for complex and "reminds"
> > you that the caclulation is using complex wavefunctions.
> >
> > > Then I found nothing in the file case.vector, i.e., it is empty, but
> > > the following files are not empty:
> > > 		tugtupite.vector
> >
> > From what I gather from the furts part of your post, tugtupite.vector
> > is your case.vector file. I think if you actually have a file called
> > 'case.vector' there is something wrong... unless you purposely named
> > a calculation 'case'. The term case is used as a generic label throughout
> > the manual.
> >
> > > So my question is: how can I get my electronic density map for my
> > > crystal?
> >
> > Use w2web, and page 22-24 of the manual. The interface knows to use the
> > correct files (tugtupite.in2c and tugtupite.vector in your case). At
> > least it does for me.
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
> > majordomo@zeus.theochem.tuwien.ac.at
> > ====
>
> Bing Zhou
> Dept. of Geological Sc.
> The Univ. of Manitoba
> Canada R3T 2N2
> Tel: (204)474-8395
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====


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------------------------------

Date: Wed, 7 Aug 2002 21:25:49 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: Re: [WIEN]: Electron Density

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====



Dear Fred:

Thanks! I write my answer after your email, could you pleae take a look?
thank you for your help and patience.


> ====
> Fred Nastos <nastos@physics.utoronto.ca>
> submitted the following contribution:
> ====
>
> > 1. During the process of init_lapw, I already set "center version" for my
> > crystal tugtupite, so I don't know why the tugtupite.in2 file was
> > still not created.
>
> I'm not sure what you mean by 'I already set "center version" for my
> crystal'. I believe the WIEN2k package will determine if your crystal
> has inversion symmetry or not.

During init_lapw0, after "x kgen", there occurred the following
information on the screen:

>   inputfiles prepared (21:07:33)
>   inputfiles for lapw1c/2c prepared, no inversion present     (21:07:34)
>   kgen        (21:07:34)  4  symmetry operations without inversion
 Do you want to add inversion: No=0, Yes=1 (0/1)


Then I chose 1 for "yes", i.e., add the inversion.


>
> Could you type the following at the command prompt:
>
> grep INVERSION tugtupite.output.s
>
> A typical output from this is:
>
>  PGBSYM: SPACE GROUP DOES NOT CONTAIN INVERSION
>
> or
>
>  PGBSYM: SPACE GROUP CONTAINS INVERSION
>
> Could you indicate more precisely, where/how you 'set "center version"'?

As mentioned above, I chose 1 for adding inversion.

After the command "grep INVERSION tugtupite.output.s", I got the following
informaiton:

	polaris:10>grep INVERSION tugtupite.output.s
	grep: can't open tugtupite.output.s
so what does it mean?


>
> > 2. Yes, my case.vector is tugtupite.vector, and there also exists the file
> > with name "tugtupite.vector", however, it is an empty file! i.e.,
> >
> > -rw-------   1 umbingz  student        0 Jun 22 02:42 tugtupite.vector
>
> I'm not sure why that would be empty, unless it was accidentally written
> over. I'm not an expert (and barely a beginner) on the internals of
> lapw1/lapw2, but it could be that since lapw2 was abnormally aborted
> (as you say below) your .vector file was left in an empty state.

I plan to run one more SCF to see if I can get a tugtupite.vector file.


>
> > 3. I did use w2web for the electron density calculation and plotting, I
> > met the following problems:
> > (1) no file of tugtupite.in2;
> > (2) after I copied tugtupite.in2_st as my tugtupite.in2 file and run
> > "x lapw2"
>
> I don't think that it is a good idea to create, by hand, files that WIEN2k
> provides just so that you can continue the calculation.  There is an old
> saying from mine workers "figure out what killed the canary before you
> continue mining."
>
> > the following information was shown:
> >
> > ******  FORTRAN RUN-TIME SYSTEM  ******
> >  End-of-file:  -1 Location:  the READ statement at line 40 of "fermi.f"
> >   Unit:  30
> >  File:  tugtupite.energy
> > Abort
> > 0.0u 0.0s 0:03 0% 0+0k 0+0io 0pf+0w
> >
> > (3) Then I run the following steps, after "x -lapw5", the following
> > information was shown on the webpage:
> >
> > 39.0u 0.0s 0:39 98% 0+0k 0+0io 0pf+0w
>
> Which just means the program exectued, and no abnormal exit
> statement was picked up by the w2web perl script.
>
> > (5) Finally I run "rhoplot", it keeps running and nothing came out on the
> > webpage, I am still waiting for any message from the program.
>
> You will probably not get anything, since lapw2 aborted.
>
> > So I don't know why lapw2 is aborted, and is my EMIN=-1.0 in
> > tugtupite.in2 too high for my tugtupite?
>
> That just depends on what range of bands you want to include in
> the plots. The density is, of course, Tr(rho), and Emin just allows you
> to truncate the the tracing sum.
>
> > I will try lower EMIN to see what happens.
>
> I suggest, that instead, you find out what "killed the canary".

Thank you for your help, I try my best to the reason to kill the canary. I
hope you can give me more help.

Thanks!




>
> Fred
>
> > Thank you again!
> >
> >
> > Have a nice day!
> >
> > On Tue, 6 Aug 2002, Fred Nastos wrote:
> >
> > <nastos@physics.utoronto.ca> submitted the following contribution:
> > > > However, I found that there is no case.in2 file in the directory
> > > > although there are files such as:
> > > > 		tugtupite.in2c
> > >
> > > Having a .in2c ending usually means that the crystal class does
> > > not have inversion symmetry. The 'c' stands for complex and "reminds"
> > > you that the caclulation is using complex wavefunctions.
> > >
> > > > Then I found nothing in the file case.vector, i.e., it is empty, but
> > > > the following files are not empty:
> > > > 		tugtupite.vector
> > >
> > > From what I gather from the furts part of your post, tugtupite.vector
> > > is your case.vector file. I think if you actually have a file called
> > > 'case.vector' there is something wrong... unless you purposely named
> > > a calculation 'case'. The term case is used as a generic label throughout
> > > the manual.
> > >
> > > > So my question is: how can I get my electronic density map for my
> > > > crystal?
> > >
> > > Use w2web, and page 22-24 of the manual. The interface knows to use the
> > > correct files (tugtupite.in2c and tugtupite.vector in your case). At
> > > least it does for me.
> > > ====
> > > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > > To (un)subscribe send mail to
> > > majordomo@zeus.theochem.tuwien.ac.at
> > > ====
> >
> > Bing Zhou
> > Dept. of Geological Sc.
> > The Univ. of Manitoba
> > Canada R3T 2N2
> > Tel: (204)474-8395
> >
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
> > majordomo@zeus.theochem.tuwien.ac.at
> > ====
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Thu, 8 Aug 2002 00:18:22 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: Electron Density

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====


>  Do you want to add inversion: No=0, Yes=1 (0/1)
>
> Then I chose 1 for "yes", i.e., add the inversion.

O.K. You have told the WIEN2k package that you want it to use
the inversion of the k-space.  Explanation:

Your crystal has certain symmetry relations (4 of them).  These relations
transform the crystal strutcure and electron density to itself. I won't write
out the details here, but essentially there is a matrix R[i, j] for each for 
each symmetry operation that takes r[ i ] to some new r'[ i ], by

r' [ i ] = R[ i, j ] * r[ j ].

 These operations, applied to lattice coordinates, leave the crystal unchanged
(though there are small details not worth going into now).

Now, the cool thing is, that in k-space the energy e_n(k) of the block state 
|nk> satisfies the same symmetry properties, in the sense that

e_n(k') = e_n(k)

where k' is R[i, j]*k[j] (i.e. the transformed k-vector). The wavefunctions 
also have nice symmetry relations

<r|nk'>  = <r''|nk>

which help reduce computation time. Here r'' = transpose(R[ i, j ])*r[ j ].

Unless you are interested in spin-orbit effects and magnetic fields, there is 
an additional bonus! In k-space you also have inversion symmetry which
means that

e_n(-k) = e_n(k).

This is just a consequence of the single-particle Schroedinger equation. End 
of sloppy explanation.

Now, the reason I went through that is, when kgen asks you if you want to
add inversion symmetry it is only asking if you want to use inversion in the 
BZ.  Another way it could ask you (which would probably be suitable for all
low-end users like me) is: "Are going to do a spin-orbit and spin-polarized 
calculation?" If your answer is no, then you probably want to add inversion
symmetry. This is in the manual though.

> > Could you type the following at the command prompt:
> >
> > grep INVERSION tugtupite.output.s
>
> After the command "grep INVERSION tugtupite.output.s", I got the following
> informaiton:
>
> 	polaris:10>grep INVERSION tugtupite.output.s
> 	grep: can't open tugtupite.output.s
> so what does it mean?

It means I made a typo. Try this instead:

grep INVERSION tugtupite.outputs

In any case, you sent me your struct file and the answer is:

 PGBSYM: SPACE GROUP DOES NOT CONTAIN INVERSION

Which means that your crystal does not have inversion symmetry.

> I plan to run one more SCF to see if I can get a tugtupite.vector file.

Yes. Run the scf. Include inversion symmetry in the BZ. Do the calculation
only for a few kpts and make sure you are producing a tugtupite.vector file.

Fred
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------------------------------

Date: Wed, 7 Aug 2002 23:00:24 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: XSPES

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started  XSPEs and Not  plot XSpes.what is it
mean?
Thank you for the guide.
H-Salehi 


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------------------------------

Date: Thu, 08 Aug 2002 08:06:55 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: [WIEN]: Spam alert and protection against other abuse of the mailing list

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Igor,

I am not afraid, just puzzled about the two facts (i) that I post many 
messages on the mailing list, yet do not get any more spam than I have 
always gotten, and (ii) we don't get spam on the mailing list itself.

Regarding politics, I have tried the "opt-out" on my hotmail account 
once. It floods the inbox with spam... plus I get a lot of spam that 
claim to be "opt-in" although I never "opt-in"... most of the spam I get 
actually comes from U.S. adresses.

Of course, since the code is only obtainable by license and password, 
they could put the mailing list postings on the web behind that 
password, too. Actually, maybe for privacy among licensed users of the 
Wien code they should, since research topics are discussed and revealed 
before they are concluded.

So, although I disagree with your spam conclusion, I agree that our 
postings should be protected from the general public on the web.

Best regards,
Torsten.

Igor Mazin wrote:

>====
>Igor Mazin <wienuser1@yahoo.com>
>submitted the following contribution:
>====
>
>Hi,
>
>I also find this discussion quite bizzare, and
>particularly your reaction. If you are inetersted in
>discussion of American and European political systems,
>I suggest the proper avenue is via private e-mail.
>
>To wrap it up, let me make a few points.
>
>1) You both over- and underestimate the level of
>sophistication of a typical spammer. They do not use
>sniffers and similar devices reqiring hacking. They
>use relatively primitive robots (crawlers) which
>simply harvest e-mails from publicly availabel html
>pages. While most, but not all spammers reside in the
>US (and so does the overwhelming majority of
>legitimate Internet businesses) they usually do not
>use traceable American providers, since many states
>have laws agains unsolicited e-mails, some at the
>opt-out and some at the opt-in level. The main
>anti-spam organisation in Europe is BTW EuroCAUCE, a
>European branch of CAUCE, an antispam organization
>originated in the US, more at
>http://www.euro.cauce.org/en/index.html and
>http://www.cauce.org/index.phtml. Unfortunately the
>absolute majority of spam messages is coming with
>faked headers (this is why you think they are send
>from American providers) and are relayed via proxies
>in China, Russia and other counries. This makes it
>extremely difficult to fight scam by legal means, as
>you suggest.
>
>2)So far with the spam basic. Now, I do NOT blame the
>list maintainers. There is nothing they can do. I
>asked for a personal favor of having my address
>cleaned out from the website. However, I do believe
>that a newsgroup/discussion-club format is better, for
>(i) you can follow messages by thread and (ii) you can
>always give your address in a form understandable by
>humans, but not robots. I know Peter is of different
>opinion, and he has his own reasons.
>
>3) You use Netscape 6.1 mailer agent, which does
>indeed have a very nice filtering engine. For reasons
>that are not interesting for the readeres, I use elm,
>with the only option of procmailing. 
>
>4) I just set up two test accounts, one subscribed to
>the list, and one not. I will post (only once, don't
>be afraid!) a message regarding the junk traffic in
>both after a week or two.
>
>Igor 
>
>====
>Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
>submitted the following contribution:
>====
>
>Hi,
>
>I find this discussion rather bizarre, as all mailing
>lists and most e-mails are transferred through several
>servers/routers/switches on their way from sender to
>recipient. Each of these places, a sniffer program can
>take out e-mail addresses, and I have not noticed any
>increase in junk mail because of the wien mailing
>list. Furthermore, I have set up a filter that takes
>about 9 out of 10 junk mails, since they usually fit a
>very simple pattern. Most of them are not adressed to
>me, so the first rule of the filter is that everything
>not addressed to me goes directly to trash. Next rules
>are exceptions from that... it also has the advantage
>that all wien mailing list postings come to a separate
>inbox.
>
>I think using e-mail has it's risks of spamming,
>mostly due to people that could be taken out via US
>legislation, which they don't want to do... so you
>being in the US should contact your congressman.
>Unsolicited e-mail is already forbidden in most
>European countries, but we can't enforce it since most
>of that comes from the US where it is "free speech"
>although without any content. Don't blame the mailing
>list maintainers!
>
>Sincerely,
>Torsten Andersen.
>
>
>__________________________________________________
>Do You Yahoo!?
>Yahoo! Health - Feel better, live better
>http://health.yahoo.com
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Wed, 7 Aug 2002 23:30:04 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: Xlape2-up

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started  XSPES  and got this
message(PGFIO-F-231/formated read /unit=1001/error on
data conversion) in "Xlapw2-qtl-up". what dose it
mean?
Thank you for the guide.
H-Salehi 



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------------------------------

Date: Thu, 08 Aug 2002 11:21:28 +0200
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: NiO bandstructure

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

  Dear Wien users and developers!

I am doing bandstructure calculations on AFM NiO. This is the struct 
file I am using:

NiO
R LATTICE,NONEQUIV. ATOMS: 3
MODE OF CALC=RELA
5.605236 5.605236 27.459934 90.000000 90.000000 90.000000
ATOM= -1: X=0.00000000 Y=0.00000000 Z=0.00000000
MULT= 1 ISPLIT= 4
Ni1 NPT= 781 R0=0.00050000 RMT= 2.0000 Z: 28.0
LOCAL ROT MATRIX: 1.0000000 0.0000000 0.0000000
0.0000000 1.0000000 0.0000000
0.0000000 0.0000000 1.0000000
ATOM= -2: X=0.50000000 Y=0.50000000 Z=0.50000000
MULT= 1 ISPLIT= 4
Ni2 NPT= 781 R0=0.00050000 RMT= 2.0000 Z: 28.0
LOCAL ROT MATRIX: 1.0000000 0.0000000 0.0000000
0.0000000 1.0000000 0.0000000
0.0000000 0.0000000 1.0000000
ATOM= -3: X=0.25000000 Y=0.25000000 Z=0.25000000
MULT= 2 ISPLIT= 4
- -3: X=0.75000000 Y=0.75000000 Z=0.75000000
O NPT= 781 R0=0.00050000 RMT= 1.7500 Z: 8.0

My problem is that when I calculate the band strucutre along the GAMMA-X 
direction I get something which not at all looks like results from 
calculations done by others, see for instance S. Massidda et al., Phys. 
Rev. B 55, 13494 (1997). At the GAMMA-point and close to it it looks 
fairly OK, but then it looks strange. I have followed the instructions 
in section 4.5.4 of the userguide for treatment of AFM compounds and 
tried to run with both runafm_lapw and runsp_lapw, but the result is the 
same. Does anyone know what the reason could be? Perhaps I am doing some 
silly mistake.

Thanks for your replies!

Best regards,
Thomas Claesson.


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------------------------------

Date: Thu, 8 Aug 2002 13:55:55 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: NiO bandstructure

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

> ====
> Thomas Claesson <tcl@kth.se>
> submitted the following contribution:
> ====
> 
>   Dear Wien users and developers!
> 
> I am doing bandstructure calculations on AFM NiO.
> This is the struct 
> file I am using:
> 
> NiO
> R LATTICE,NONEQUIV. ATOMS: 3
> MODE OF CALC=RELA
> 5.605236 5.605236 27.459934 90.000000 90.000000
> 90.000000

There is something fishy here. AFM NiO is
rhombohedral, not tetragonal. The usual choice og the
unit cell is

1 .5 .5
.5 1 .5
.5 .5 1
in units of the cubic lattice parameter.

Experimental structure has a small rhombohedral
distortion, around %. Check a paper by Isaak, Cohen
and Singh on FeO in PRB around 1990. They have a nice
description of the crystallography of FeO (NiO is the
same, but not CoO).


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------------------------------

Date: Sat, 10 Aug 2002 00:23:40 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: Xlape2-

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started  XSPES  and got this
message(PGFIO-F-231/formated read /unit=1001/error on
data conversion or PGFIO-F-217/list-directed read
/unit=30/attempt to read past end of file:
filename=home.energyup  formatted,sequential access
record=285) in "Xlapw2-qtl-up". what dose it mean?
Thank you for the guide.
H-Salehi 




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------------------------------

End of wien-digest V2002 #30
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #31
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
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Precedence: bulk


wien-digest         Friday, August 16 2002         Volume 2002 : Number 031




----------------------------------------------------------------------

Date: Mon, 12 Aug 2002 07:02:01 -0700 (PDT)
From: yanming Ma <ymma66@yahoo.com>
Subject: [WIEN]: About AIM 

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-388034923-1029160921=:52419
Content-Type: text/plain; charset=us-ascii


Dear wien2k users,

I am interested in the function of AIM (atoms in molecules) in WIEN2k.

Can someone provide me the useful references for the basic Bader's theory of  AIM.

I will appreciate your helps.

Yanming

 



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- --0-388034923-1029160921=:52419
Content-Type: text/html; charset=us-ascii

<P>Dear wien2k users,</P>
<P>I am interested in the function of AIM (atoms in molecules) in WIEN2k.</P>
<P>Can someone provide me the useful references for the basic Bader's theory of&nbsp; AIM.</P>
<P>I will appreciate your helps.</P>
<P>Yanming</P>
<P>&nbsp;</P><p><br><hr size=1><b>Do You Yahoo!?</b><br>
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------------------------------

Date: Mon, 12 Aug 2002 15:53:19 +0100 (BST)
From: Dave Pankhurst <david.pankhurst@materials.oxford.ac.uk>
Subject: [WIEN]: bug in lapwdm Makefile

====
Dave Pankhurst <david.pankhurst@materials.oxford.ac.uk>
submitted the following contribution:
====

Dear wien users,

There is a bug in the SRC_lapwdm/Makefile which causes lapwdm to fail to
compile.  On line 134 changing the leading 8 spaces to a tab corrects
this.

best regards,

	Dave Pankhurst

+---------------------------------+------------------------------------+
| Dr David Pankhurst,             | Tel : +44 1865 283325/283326       |
| Department of Materials,        | Fax : +44 1865 273789              |    
| University of Oxford,           |                                    |
| Parks Road, Oxford OX1 3PH, UK  | david.pankhurst@materials.ox.ac.uk |
+---------------------------------+------------------------------------+

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Date: Mon, 12 Aug 2002 23:01:49 +0800
From: Wenhui Xie <xiewh@sun20.iphy.ac.cn>
Subject: [WIEN]: help, Fe3O4.struct

====
Wenhui Xie <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear WIEN Users,

I want to calculate Fe3O4, which have a spinel crystal structure. 
But I always do not generate the right structure file. 
Who can help me, or tell me the struct file of Fe3O4.
Thank you very much.

Looking forwards in here.

Wenhui Xie
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Date: Mon, 12 Aug 2002 11:10:42 -0400
From: "Jorge O. Sofo" <sofo@psu.edu>
Subject: RE: [WIEN]: About AIM 

====
"Jorge O. Sofo" <sofo@psu.edu>
submitted the following contribution:
====

You can find more information in R. Bader's page:

http://www.chemistry.mcmaster.ca/faculty/bader/aim/

Regards,
Jorge

- -----Original Message-----
From: owner-wien@zeus.theochem.tuwien.ac.at
[mailto:owner-wien@zeus.theochem.tuwien.ac.at] On Behalf Of yanming Ma
Sent: Monday, August 12, 2002 10:02 AM
To: wien@zeus.theochem.tuwien.ac.at
Subject: [WIEN]: About AIM 


Dear wien2k users,
I am interested in the function of AIM (atoms in molecules) in WIEN2k.
Can someone provide me the useful references for the basic Bader's
theory of  AIM.
I will appreciate your helps.
Yanming





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Date: Mon, 12 Aug 2002 17:48:49 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: About AIM

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Ms. Ma,

you can follow the link below:

http://www.chemistry.mcmaster.ca/faculty/bader/aim/

which is also proviuded ion the users guide.

Best regards,
Torsten Andersen.

yanming Ma wrote:

> Dear wien2k users,
>
> I am interested in the function of AIM (atoms in molecules) in WIEN2k.
>
> Can someone provide me the useful references for the basic Bader's 
> theory of  AIM.
>
> I will appreciate your helps.
>
> Yanming
>
>  
>
>
> ------------------------------------------------------------------------
> Do You Yahoo!?
> HotJobs, a Yahoo! service 
> <http://rd.yahoo.com/careers/mailsig/new/*http://www.hotjobs.com> - 
> Search Thousands of New Jobs 


- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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Date: Mon, 12 Aug 2002 17:50:59 +0200
From: "Dr. Alexander Hofmann" <ah@chemie.hu-berlin.de>
Subject: Re: [WIEN]: About AIM

====
"Dr. Alexander Hofmann" <ah@chemie.hu-berlin.de>
submitted the following contribution:
====


- --UlVJffcvxoiEqYs2
Content-Type: text/plain; charset=us-ascii
Content-Disposition: inline

Dear Yanming,

The basic articles are attached below.

For some reasons I made in my molecular life tests with Baders program (PROAIMV) on the water molecule with different basis sets. I did the same with the Mulliken analysis (very common in molecular chemistry) and the Gaussian98 NPA (=Natural Population Analysis). And it turned out that the NPA is the most stable analysis with respect to varying basis sets. 
We can learn at least a couple of things from this (comments welcome):
- - Even the conceptually best analysis (Bader) gives widely spreaded _absolute_ numbers. 
- - charge difference are quite reliable
- - NPA is best for water, but it seems this due to some error cancellation.

My take home message is: Carefully with absolute charges, trends are surely ok.


with best regards

Alex

PS: attached the mentioned table (TeX-Format)

@article{bader81,
TITLE={Quantum Theory of Atoms in Molecules - Dalton Revisited},
AUTHOR={R. F. W. Bader
and T. T. Nguyen-Dang},
JOURNAL={Adv. Quantum Chem.},
YEAR={1981},
VOLUME={14},
PAGES={63}
}

@book{bader90,
TITLE={Atoms in Molecules - A Quantum Theory},
AUTHOR={R. F. W. Bader},
PUBLISHER={Oxford University Press},
YEAR={1990},
address={Oxford},
}

@article{bader91,
TITLE={A Quantum Theory of Molecular Structure and Its Applications},
AUTHOR={R. F. W. Bader},
JOURNAL={Chem. Rev.},
YEAR={1991},
VOLUME={91},
PAGES={893}
}

- -- 

Dr. Alexander Hofmann

Humboldt-Universitaet zu Berlin
Institut fuer Chemie
Arbeitsgruppe Quantenchemie

Brook-Taylor-Strasse 2

12489 Berlin

ah@chemie.hu-berlin.de

Tel.: +49-30-2093-7138
Fax.: +49-30-2093-7136

http://www.chemie.hu-berlin.de/ag_sauer/index.html

PGP-Key: wwwkeys.de.pgp.net ID: D9D62D35

- --UlVJffcvxoiEqYs2
Content-Type: application/x-tex
Content-Disposition: attachment; filename="topologische.Ladungsdichteanalyse.tex"

\begin{center}\begin{tabular}{lqqq}
\hline
&\multicolumn{1}{c}{Mulliken}&\multicolumn{1}{c}{NPA}&\multicolumn{1}{c}{PROAIMV}\\
\hline
H$_2$O (lanl2dz)          & -0.792 & -0.975 & -1.048 \\   %  O  
%                         &  0.396 &  0.488 &  0.524 \\   %  H  
H$_2$O (6-31G)            & -0.811 & -0.966 & -1.043 \\   %  O  
%                         &  0.406 &  0.483 &  0.521 \\   %  H  
H$_2$O (6-31G*)           & -0.869 & -0.955 & -1.181 \\   %  O  
%                         &  0.434 &  0.477 &  0.590 \\   %  H  
H$_2$O (6-31G**)          & -0.673 & -0.974 & -1.242 \\   %  O  
%                         &  0.336 &  0.487 &  0.621 \\   %  H  
H$_2$O (6-31$^{++}$G**)   & -0.717 & -0.983 & -1.259 \\   %  O  
%                         &  0.358 &  0.491 &  0.630 \\   %  H  
H$_2$O (6-311$^{++}$G**)  & -0.515 & -0.916 & -1.225 \\   %  O  
%                         &  0.258 &  0.458 &  0.613 \\   %  H  
\hline			  	 	           	      
H$_2$O (lanl2dz B3LYP)    & -0.711 & -0.963 & -0.987 \\   %  O  
%                         &  0.356 &  0.481 &  0.493 \\   %  H  
H$_2$O (lanl2dz MP2)      & -0.745 & -0.965 & -0.989 \\   %  O  
%                         &  0.373 &  0.483 &  0.494 \\   %  H  
H$_2$O (lanl2dz MP4SDQ)   & -0.733 & -0.948 & -0.960 \\   %  O  
%                         &  0.366 &  0.474 &  0.480 \\   %  H  
\hline
H$_2$O (6-311$^{++}$G** B3LYP)    & -0.502 & -0.916 & -1.097 \\   %  O  
%                                 &  0.251 &  0.458 &  0.548 \\   %  H  
H$_2$O (6-311$^{++}$G** MP2)      & -0.496 & -0.898 & -1.133 \\   %  O  
%                                 &  0.248 &  0.448 &  0.566 \\   %  H  
H$_2$O (6-311$^{++}$G** MP4SDQ)   & -0.483 & -0.880 & -1.109 \\   %  O  
%                                 &  0.242 &  0.440 &  0.554 \\   %  H  
\hline
\hline
H$_3$O$^+$ (lanl2dz)      &   -0.745  &    -0.865 &    -1.117  \\   %  O  
%                         &    0.582  &     0.622 &     0.706  \\   %  H  
\hline			  	                		        
\hline			  	                		        
OH$^-$  (lanl2dz)         &   -1.184  &    -1.325 &    -1.280  \\   %  O  
%                         &    0.184  &     0.325 &     0.280  \\   %  H  
\hline
\end{tabular}\end{center}

- --UlVJffcvxoiEqYs2--
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Date: Mon, 12 Aug 2002 17:09:13 +0100
From: "Xiangyuan Cui" <x.cui@pgr.salford.ac.uk>
Subject: Re: [WIEN]: About AIM 

====
"Xiangyuan Cui" <x.cui@pgr.salford.ac.uk>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0008_01C24222.FBB09450
Content-Type: text/plain;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

Hi, Dear Yanming,

you can visit the webpage on:

http://www.chemistry.mcmaster.ca/faculty/bader/aim/

or for the full reference, see the book:

"Atom in molecules" by R.F.W. Bader. (the book name may be not very =
accurate)

regards,
Xiangyuan

  ----- Original Message -----=20
  From: yanming Ma=20
  To: wien@zeus.theochem.tuwien.ac.at=20
  Sent: Monday, August 12, 2002 3:02 PM
  Subject: [WIEN]: About AIM=20


  Dear wien2k users,

  I am interested in the function of AIM (atoms in molecules) in WIEN2k.

  Can someone provide me the useful references for the basic Bader's =
theory of  AIM.

  I will appreciate your helps.

  Yanming







- -------------------------------------------------------------------------=
- -----
  Do You Yahoo!?
  HotJobs, a Yahoo! service - Search Thousands of New Jobs
  Hi, Dear Yanming,

  you can visit the webpage on:

  http://www.chemistry.mcmaster.ca/faculty/bader/aim/

  or for the full reference, see the book:

  "Atom in molecules" by R.F.W. Bader. (the book name may be not very =
accurate)

  regards,
  Xiangyuan

    ----- Original Message -----=20
    From: yanming Ma=20
    To: wien@zeus.theochem.tuwien.ac.at=20
    Sent: Monday, August 12, 2002 3:02 PM
    Subject: [WIEN]: About AIM=20


    Dear wien2k users,

    I am interested in the function of AIM (atoms in molecules) in =
WIEN2k.

    Can someone provide me the useful references for the basic Bader's =
theory of  AIM.

    I will appreciate your helps.

    Yanming







- -------------------------------------------------------------------------=
- ---
    Do You Yahoo!?
    HotJobs, a Yahoo! service - Search Thousands of New Jobs

- ------=_NextPart_000_0008_01C24222.FBB09450
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2715.400" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT face=3DArial size=3D2>Hi, Dear Yanming,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>you can visit the webpage =
on:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2><A=20
href=3D"http://www.chemistry.mcmaster.ca/faculty/bader/aim/">http://www.c=
hemistry.mcmaster.ca/faculty/bader/aim/</A></FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>or&nbsp;for&nbsp;the full reference, =
see the=20
book:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>"Atom in molecules" by R.F.W. Bader. =
(the book name=20
may be not very accurate)</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>regards,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Xiangyuan</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<BLOCKQUOTE=20
style=3D"PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; =
BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
  <DIV style=3D"FONT: 10pt arial">----- Original Message ----- </DIV>
  <DIV=20
  style=3D"BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: =
black"><B>From:</B>=20
  <A title=3Dymma66@yahoo.com href=3D"mailto:ymma66@yahoo.com">yanming =
Ma</A> </DIV>
  <DIV style=3D"FONT: 10pt arial"><B>To:</B> <A=20
  title=3Dwien@zeus.theochem.tuwien.ac.at=20
  =
href=3D"mailto:wien@zeus.theochem.tuwien.ac.at">wien@zeus.theochem.tuwien=
.ac.at</A>=20
  </DIV>
  <DIV style=3D"FONT: 10pt arial"><B>Sent:</B> Monday, August 12, 2002 =
3:02=20
  PM</DIV>
  <DIV style=3D"FONT: 10pt arial"><B>Subject:</B> [WIEN]: About AIM =
</DIV>
  <DIV><BR></DIV>
  <P>Dear wien2k users,</P>
  <P>I am interested in the function of AIM (atoms in molecules) in =
WIEN2k.</P>
  <P>Can someone provide me the useful references for the basic Bader's =
theory=20
  of&nbsp; AIM.</P>
  <P>I will appreciate your helps.</P>
  <P>Yanming</P>
  <P>&nbsp;</P>
  <P><BR>
  <HR SIZE=3D1>
  <B>Do You Yahoo!?</B><BR><A=20
  =
href=3D"http://rd.yahoo.com/careers/mailsig/new/*http://www.hotjobs.com">=
HotJobs,=20
  a Yahoo! service</A> - Search Thousands of New Jobs
  <DIV><FONT face=3DArial size=3D2>Hi, Dear Yanming,</FONT></DIV>
  <DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
  <DIV><FONT face=3DArial size=3D2>you can visit the webpage =
on:</FONT></DIV>
  <DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
  <DIV><FONT face=3DArial size=3D2><A=20
  =
href=3D"http://www.chemistry.mcmaster.ca/faculty/bader/aim/">http://www.c=
hemistry.mcmaster.ca/faculty/bader/aim/</A></FONT></DIV>
  <DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
  <DIV><FONT face=3DArial size=3D2>or&nbsp;for&nbsp;the full reference, =
see the=20
  book:</FONT></DIV>
  <DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
  <DIV><FONT face=3DArial size=3D2>"Atom in molecules" by R.F.W. Bader. =
(the book=20
  name may be not very accurate)</FONT></DIV>
  <DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
  <DIV><FONT face=3DArial size=3D2>regards,</FONT></DIV>
  <DIV><FONT face=3DArial size=3D2>Xiangyuan</FONT></DIV>
  <DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
  <BLOCKQUOTE=20
  style=3D"PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; =
BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
    <DIV style=3D"FONT: 10pt arial">----- Original Message ----- </DIV>
    <DIV=20
    style=3D"BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: =
black"><B>From:</B>=20
    <A title=3Dymma66@yahoo.com href=3D"mailto:ymma66@yahoo.com">yanming =
Ma</A>=20
    </DIV>
    <DIV style=3D"FONT: 10pt arial"><B>To:</B> <A=20
    title=3Dwien@zeus.theochem.tuwien.ac.at=20
    =
href=3D"mailto:wien@zeus.theochem.tuwien.ac.at">wien@zeus.theochem.tuwien=
.ac.at</A>=20
    </DIV>
    <DIV style=3D"FONT: 10pt arial"><B>Sent:</B> Monday, August 12, 2002 =
3:02=20
    PM</DIV>
    <DIV style=3D"FONT: 10pt arial"><B>Subject:</B> [WIEN]: About AIM =
</DIV>
    <DIV><BR></DIV>
    <P>Dear wien2k users,</P>
    <P>I am interested in the function of AIM (atoms in molecules) in=20
WIEN2k.</P>
    <P>Can someone provide me the useful references for the basic =
Bader's theory=20
    of&nbsp; AIM.</P>
    <P>I will appreciate your helps.</P>
    <P>Yanming</P>
    <P>&nbsp;</P>
    <P><BR>
    <HR SIZE=3D1>
    <B>Do You Yahoo!?</B><BR><A=20
    =
href=3D"http://rd.yahoo.com/careers/mailsig/new/*http://www.hotjobs.com">=
HotJobs,=20
    a Yahoo! service</A> - Search Thousands of New=20
Jobs</BLOCKQUOTE></BLOCKQUOTE></BODY></HTML>

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Date: Mon, 12 Aug 2002 10:24:24 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: help, Fe3O4.struct

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

Here is a struct file for a spinel:

Title
F   LATTICE,NONEQUIV. ATOMS: 3
MODE OF CALC=RELA
 19.111531 19.111531 19.111531 90.000000 90.000000
90.000000
ATOM=  1: X=0.12500000 Y=0.12500000 Z=0.12500000
          MULT= 2          ISPLIT= 2
       1: X=0.87500000 Y=0.87500000 Z=0.87500000
Mn         NPT=  781  R0=0.00005000 RMT=    2.0000  
Z: 25.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -2: X=0.50000000 Y=0.75000000 Z=0.75000000
          MULT= 4          ISPLIT= 4
      -2: X=0.75000000 Y=0.50000000 Z=0.75000000
      -2: X=0.75000000 Y=0.75000000 Z=0.50000000
      -2: X=0.50000000 Y=0.50000000 Z=0.50000000
Cr         NPT=  781  R0=0.00005000 RMT=    2.0000  
Z: 24.0
LOCAL ROT MATRIX:    0.4082483 0.7071068 0.5773503
                    -0.4082483 0.7071068-0.5773503
                    -0.8164966 0.0000000 0.5773503
ATOM= -3: X=0.01130000 Y=0.01130000 Z=0.73870000
          MULT= 8          ISPLIT= 4
      -3: X=0.01130000 Y=0.73870000 Z=0.01130000
serene<211>%cat /scratch/mazin/SPINEL/SPINEL.struct
Title
F   LATTICE,NONEQUIV. ATOMS: 3
MODE OF CALC=RELA
 19.111531 19.111531 19.111531 90.000000 90.000000
90.000000
ATOM=  1: X=0.12500000 Y=0.12500000 Z=0.12500000
          MULT= 2          ISPLIT= 2
       1: X=0.87500000 Y=0.87500000 Z=0.87500000
Mn         NPT=  781  R0=0.00005000 RMT=    2.0000  
Z: 25.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -2: X=0.50000000 Y=0.75000000 Z=0.75000000
          MULT= 4          ISPLIT= 4
      -2: X=0.75000000 Y=0.50000000 Z=0.75000000
      -2: X=0.75000000 Y=0.75000000 Z=0.50000000
      -2: X=0.50000000 Y=0.50000000 Z=0.50000000
Cr         NPT=  781  R0=0.00005000 RMT=    2.0000  
Z: 24.0
LOCAL ROT MATRIX:    0.4082483 0.7071068 0.5773503
                    -0.4082483 0.7071068-0.5773503
                    -0.8164966 0.0000000 0.5773503
ATOM= -3: X=0.01130000 Y=0.01130000 Z=0.73870000
          MULT= 8          ISPLIT= 4
      -3: X=0.01130000 Y=0.73870000 Z=0.01130000
      -3: X=0.73870000 Y=0.01130000 Z=0.01130000
      -3: X=0.26130000 Y=0.98870000 Z=0.98870000
      -3: X=0.98870000 Y=0.26130000 Z=0.98870000
      -3: X=0.98870000 Y=0.98870000 Z=0.26130000
      -3: X=0.73870000 Y=0.73870000 Z=0.73870000
      -3: X=0.26130000 Y=0.26130000 Z=0.26130000
S          NPT=  781  R0=0.00010000 RMT=    2.0000  
Z: 16.0
LOCAL ROT MATRIX:   -0.4082483-0.7071068 0.5773503
                    -0.4082483 0.7071068 0.5773503
                    -0.8164966 0.0000000-0.5773503
  48      NUMBER OF SYMMETRY OPERATIONS



- --- Wenhui Xie <xiewh@sun20.iphy.ac.cn> wrote:
> ====
> Wenhui Xie <xiewh@sun20.iphy.ac.cn>
> submitted the following contribution:
> ====
> 
> Dear WIEN Users,
> 
> I want to calculate Fe3O4, which have a spinel
> crystal structure. 
> But I always do not generate the right structure
> file. 
> Who can help me, or tell me the struct file of
> Fe3O4.
> Thank you very much.
> 
> Looking forwards in here.
> 
> Wenhui Xie
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====


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Date: Mon, 12 Aug 2002 13:54:22 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: min_lapw

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear all:

I was aked "max. number of structure change---" when I run min_lapw with
w2web, so could you please let me know what the max. number is in general?

Thanks!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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====

------------------------------

Date: Mon, 12 Aug 2002 13:57:59 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: min_lapw

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====



Dear all:

I was aked "max. number of structure change---" when I run min_lapw with
w2web, so could you please let me know what the max. number is in general?

I also asked the "save every ___ iterations", so what should I put in the
blank box?


Thanks!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395


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------------------------------

Date: Mon, 12 Aug 2002 13:41:53 -0700 (PDT)
From: Michelle Johannes <johannes@maugre.ucdavis.edu>
Subject: [WIEN]: single vs. double cells

====
Michelle Johannes <johannes@maugre.ucdavis.edu>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---307652566-192031902-1029184913=:22883
Content-Type: TEXT/PLAIN; charset=US-ASCII

Dear Wien users:

	I am investigating a AFM compound and therefore have to double my
unit cell.  In the compound I am looking at the single cell is the cubic
space group #221 (Pm-3m).  This is a peroskite structure and the afm order
is along the (111) axis and therefore I end up with a rhombohedral cell
which is space group #166 (R-3m).  The problem is that if I calculate the
ferromagnetic solution in the doubled cell, my energy doesn't look
anything like that of double the single cell energy.  In fact, there is an
approximately 30 Ryd difference!!  
	I compared my energies with another full-potential program (FPLO
from IFW Dresden) and my single cell energy differs from the FPLO energy
by only 1 or 2 mHartree per atom, which is acceptable.  The doubled cell
energy is not even comparable.  Wien and FPLO are usually quite comparable
in terms of total energy.  So I wonder what makes this huge energy
difference.  
	I am concerned that something about the rhombohedral cell is not
being handled right, either in the way that I set it up or the way that it
is calculated.  Since the sgroup finds the right space group and xcrysden
gives me the picture I want, it seems like I have the right .struct file,
but I would be happy if someone could point out a mistake.  I am including
both the single and doubled cell .struct files in case someone would be
kind enough to look them over.  Any other explanations of energy
difference would also be most welcome.

	Thank you for your help,
			Michelle


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------------------------------

Date: Mon, 12 Aug 2002 19:26:32 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: EFG tensors direction 

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear all:

After the SCF cycles, how can I correlate the calculated EFG tensor
directions in PAS with the crystal directions (a, b, c)? can I find it in
the case.scf file or other files?



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Tue, 13 Aug 2002 03:18:58 +0200
From: Victor Lua~na Cabal <victor@fluor.quimica.uniovi.es>
Subject: Re: [WIEN]: About AIM

====
Victor Lua~na Cabal <victor@fluor.quimica.uniovi.es>
submitted the following contribution:
====

> Date: Mon, 12 Aug 2002 17:50:59 +0200
> From: "Dr. Alexander Hofmann" <ah@chemie.hu-berlin.de>
> Subject: Re: [WIEN]: About AIM
>
> ====
> "Dr. Alexander Hofmann" <ah@chemie.hu-berlin.de>
> submitted the following contribution:
> ====
> For some reasons I made in my molecular life tests with Baders program
> (PROAIMV) on the water molecule with different basis sets. I did the same
> with the Mulliken analysis (very common in molecular chemistry) and the
> Gaussian98 NPA (=Natural Population Analysis). And it turned out that
> the NPA is the most stable analysis with respect to varying basis sets.
> We can learn at least a couple of things from this (comments welcome):
> - Even the conceptually best analysis (Bader) gives widely spreaded
>   _absolute_ numbers.

I'm affraid that some of the calculations that you do compare can be
misleading with respect to the topological (Bader's) charges:

(1) Bader's charges do, in fact, converge quite well with respect to the
    basis set quality and theory level. To ensure a reasonable quality
    on your wavefunction you need to include polarization functions and,
    in the case of very electronegative atoms (O, F, etc), diffuse
    functions as well. Poor bases produce a poor wavefunction and,
    consequently, poor topological properties.

(2) Bader's techniques do work on all electron wavefunctions. The use
    of ECP's, like in your LANL2DZ calculations, excludes, in principle,
    the topological analysis. There have been some attempts to recover
    the complete electron density from the pseudodensity obtained
    in a pseudopotential calculation (see the references below). PROAIMV
    results for a valence electron pseudodensity are, in principle,
    a numerical freak.

          Best regards,
                        Victor Lua~na
                        victor@carbono.quimica.uniovi.es

@Article{AIM-VS97,
  author        = { S. F. Vyboishchikov and A. Sierraalta and G. Frenking },
  title         = { Topological Analysis of Electron-Density Distribution
                  Taken from a Pseudopotential Calculation },
  journal       = { J. Comput. Chem. },
  year          = { 1997 },
  volume        = { 18 },
  pages         = { 416-429 },
  address       = { UNIV-MARBURG, FACHBEREICH CHEM, D-35032 MARBURG, GERMANY }
}

@Article{AIM-CP96,
  author        = { J. Cioslowski and P. Piskorz },
  title         = { Properties of Atoms in Molecules from Valence-Electron
                  Densities Augmented with Core-Electron Contributions },
  journal       = { Chem. Phys. Lett. },
  year          = { 1996 },
  volume        = { 255 },
  pages         = { 315-319 },
  address       = { FLORIDA-STATE-UNIV, DEPT COMP, TALLAHASSEE, FL 32306,
                  USA; FLORIDA-STATE-UNIV, SUPERCOMP COMPUTAT RES INST,
                  TALLAHASSEE, FL 32306, USA; }
}
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------------------------------

Date: Mon, 12 Aug 2002 20:50:43 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: EFG tensors direction 

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> After the SCF cycles, how can I correlate the calculated EFG tensor
> directions in PAS with the crystal directions (a, b, c)? can I find it in
> the case.scf file or other files?

One interested to analyze EFG needs after a well converged SCF to first
change TOT to EFG in case.in2 file, and then run lapw2 program: x lapw2
(with the appropriate switch, e.g. -up/dn -so ..., if necessary). After the
step outlined above, the EFG component before transformation in general axis
system and after transformation in principal axis system (PAS), where the
tensor is diagonal, can be found in case.output2 (up/dn). Bing, I am sure
you will enjoy reading the nice written description manuscript by Stefaan:
http://www.wien2k.at/reg_user/faq/efg.html/efg.pdf
Your,
S. Jalali.



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------------------------------

Date: Tue, 13 Aug 2002 14:39:40 +0900
From: "Ichiro Nagano" <nagano@atrc.mhi.co.jp>
Subject: Re: [WIEN]: The problem in band character plot

====
"Ichiro Nagano" <nagano@atrc.mhi.co.jp>
submitted the following contribution:
====

Dear Dr. Wenhui Xie and WIEN2k users,

I have a same problem.

I tried TiC Bandstructure (with band character) as routine manner.
(Generate k-list, edit tic.in1, lapw1 -up, edit tic.in2, and
lapw2 -up -qtl.)

When I start lapw2 with -up spin option, the program seems to search
opposite down spin (tic.energydn) file. (see below)

executing: x lapw2 -up -qtl
PGFIO-F-252/list-directed read/unit=29/operation attempted after end of
file.
 File name = tic.energydn    formatted, sequential access   record = 698
 In source file fermi.f, at line number 63
0.040u 0.020s 0:00.15 40.0%     0+0k 0+0io 443pf+0w
RETURN key to continue ...

In case of with -dn spin option, lapw2 program seems to search
opposite upper spin (tic.energyup) file. (see below)

executing: x lapw2 -dn -qtl
PGFIO-F-252/list-directed read/unit=29/operation attempted after end of
file.
 File name = tic.energyup    formatted, sequential access   record = 697
 In source file fermi.f, at line number 63
0.030u 0.020s 0:00.19 26.3%     0+0k 0+0io 192pf+0w
RETURN key to continue ...

I recompiled with HP-Fortran90, it seemed no problem.
Though I recompiled with PGI, Intel, Absoft and Lahey, they caused same
error.

Thanks for any help.

Ichiro Nagano

Advanced Technology Research Center, Mitsubishi Heavy Industries, Ltd.
1-8-1, Sachiura, Kanazawa-ku, Yokohama, 236-8515, Japan
Ichiro Nagano
e-mail: <nagano@atrc.mhi.co.jp>
TEL: + 81 (45) 771-1222
FAX: + 81 (45) 771-3879

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------------------------------

Date: Tue, 13 Aug 2002 15:01:47 +0800
From: Wenhui Xie <xiewh@sun20.iphy.ac.cn>
Subject: Re: [WIEN]: help, Fe3O4.struct

====
Wenhui Xie <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear Mazin,

Thank you very much.
How to understant the u parameter in Spinel, which is not shown in your 
structure file?

Best Regard.

Wenhui Xie

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------------------------------

Date: Tue, 13 Aug 2002 06:33:31 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: help, Fe3O4.struct

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

Hi,

You need to change the line 
ATOM= -3: X=0.01130000 Y=0.01130000 Z=0.73870000
and the other "-3" lines according to your parameter
u.
X=a Y=a Z=0.75-a, where a is the internal structural 
parameter (your u may be defined differently,
but it is easy to figure out the correspondence).

Good luck.

- --- Wenhui Xie <xiewh@sun20.iphy.ac.cn> wrote:
> ====
> Wenhui Xie <xiewh@sun20.iphy.ac.cn>
> submitted the following contribution:
> ====
> 
> Dear Mazin,
> 
> Thank you very much.
> How to understant the u parameter in Spinel, which
> is not shown in your 
> structure file?
> 
> Best Regard.
> 
> Wenhui Xie
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
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------------------------------

Date: Tue, 13 Aug 2002 07:27:35 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: Xlape2-

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started  XSPES  and got this
message(PGFIO-F-231/formated read /unit=1001/error on
data conversion or PGFIO-F-217/list-directed read
/unit=30/attempt to read past end of file:
filename=home.energyup  formatted,sequential access
record=285) in "Xlapw2-qtl-up". what dose it mean?
Thank you for the guide.
H-Salehi 




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------------------------------

Date: Tue, 13 Aug 2002 07:28:07 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: Xlape2

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started  XSPES  and got this
message(PGFIO-F-231/formated read /unit=1001/error on
data conversion) in "Xlapw2-qtl-up". what dose it
mean?
Thank you for the guide.
H-Salehi 



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------------------------------

Date: Tue, 13 Aug 2002 07:43:10 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: XLstart

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started Initializ cale and got this
message(Xlstart:ERROR In OPENING UNIT:5
 FILE Name:
home inst
STATUS:Old         FORM:Formated
0.000u,0.000s....   0+0k     167pf+0w
and in "view outputstin" disappear System Error). what
dose it mean?or What is its reason?
What should be done for eliminating it?
Thank you for the guide.
H-Salehi 
Dept of physics
Ferdowsi University
MASHHAD IRAN


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------------------------------

Date: Tue, 13 Aug 2002 12:32:49 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: Xlape2-

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====

Hamid,

Please supply more information.  It is rarely enough that
anyone can figure out your mistake if you only give the
runtime error message.


On August 13, 2002 10:27 am, hamid salehi wrote:
> ====
> hamid salehi <salehihamid@yahoo.com>
> submitted the following contribution:
> ====
>
> Dear wien users.
> Ihave started  XSPES  and got this
> message(PGFIO-F-231/formated read /unit=1001/error on
> data conversion or PGFIO-F-217/list-directed read
> /unit=30/attempt to read past end of file:
> filename=home.energyup  formatted,sequential access
> record=285) in "Xlapw2-qtl-up". what dose it mean?
> Thank you for the guide.
> H-Salehi
>
>
>
>
> __________________________________________________
> Do You Yahoo!?
> HotJobs - Search Thousands of New Jobs
> http://www.hotjobs.com
> ====
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> majordomo@zeus.theochem.tuwien.ac.at
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------------------------------

Date: Tue, 13 Aug 2002 16:53:04 -0400 (EDT)
From: Neme Nnolim <non6886@alizarin.njit.edu>
Subject: [WIEN]: Struct file for Ta_2O_5?

====
Neme Nnolim <non6886@alizarin.njit.edu>
submitted the following contribution:
====


Dear Wien users,

I have been trying to build a struct file for Tantalum (V) oxide. Of
course this would require a knowledge of all atomic positions. I have so
far not come across a reference from which I can obtain this
information. 

Does anyone have a struct file for this material already
built, or can they point me to a good reference? I have ordered the relevant 
Landolt-Bornstein  series through our library but it will be a while
before I receive it. 


Regards,

Neme
- ------------------------------------------------------------------------------
Neme Okechukwu Nnolim
Department of Materials Science, New Jersey Institute of Technology
Room 302, Tiernan Hall, 161 Warren Street, University Heights
Newark, New Jersey 07102-1982
Tel: (973) 596-8283, FAX: (973) 596-5794
- -------------------------------------------------------------------------------



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------------------------------

Date: Tue, 13 Aug 2002 18:17:49 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: Struct file for Ta_2O_5?

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====


My understanding is that Tantalum (V) Oxide  has the chemical
formula Ta_{2}O_{5}, so I'd start with PRB 55, 11155 (1997).

On August 13, 2002 04:53 pm, Neme Nnolim wrote:
> ====
> Neme Nnolim <non6886@alizarin.njit.edu>
> submitted the following contribution:
> ====
>
> Dear Wien users,
>
> I have been trying to build a struct file for Tantalum (V) oxide. Of
> course this would require a knowledge of all atomic positions. I have so
> far not come across a reference from which I can obtain this
> information.
>
> Does anyone have a struct file for this material already
> built, or can they point me to a good reference? I have ordered the
> relevant Landolt-Bornstein  series through our library but it will be a
> while before I receive it.
>
>
> Regards,
>
> Neme
> ---------------------------------------------------------------------------
>--- Neme Okechukwu Nnolim
> Department of Materials Science, New Jersey Institute of Technology
> Room 302, Tiernan Hall, 161 Warren Street, University Heights
> Newark, New Jersey 07102-1982
> Tel: (973) 596-8283, FAX: (973) 596-5794
> ---------------------------------------------------------------------------
>----
>
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
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------------------------------

Date: Tue, 13 Aug 2002 19:50:41 -0400 (EDT)
From: Neme Nnolim <non6886@alizarin.njit.edu>
Subject: Re: [WIEN]: Struct file for Ta_2O_5?

====
Neme Nnolim <non6886@alizarin.njit.edu>
submitted the following contribution:
====


Actually, I have seen that paper before, and the structure given there is
a highly hypothetical structure of one type of Ta_2O_5, thought to
be present in thin films. I was looking for a recent structure
determination more based on experimental methods. Thanks for your trouble
anyway.

On Tue, 13 Aug 2002, Fred Nastos wrote:

> Date: Tue, 13 Aug 2002 18:17:49 -0400
> From: Fred Nastos <nastos@physics.utoronto.ca>
> Reply-To: wien@zeus.theochem.tuwien.ac.at
> To: wien@zeus.theochem.tuwien.ac.at
> Subject: Re: [WIEN]: Struct file for Ta_2O_5?
> 
> ====
> Fred Nastos <nastos@physics.utoronto.ca>
> submitted the following contribution:
> ====
> 
> 
> My understanding is that Tantalum (V) Oxide  has the chemical
> formula Ta_{2}O_{5}, so I'd start with PRB 55, 11155 (1997).
> 
> On August 13, 2002 04:53 pm, Neme Nnolim wrote:
> > ====
> > Neme Nnolim <non6886@alizarin.njit.edu>
> > submitted the following contribution:
> > ====
> >
> > Dear Wien users,
> >
> > I have been trying to build a struct file for Tantalum (V) oxide. Of
> > course this would require a knowledge of all atomic positions. I have so
> > far not come across a reference from which I can obtain this
> > information.
> >
> > Does anyone have a struct file for this material already
> > built, or can they point me to a good reference? I have ordered the
> > relevant Landolt-Bornstein  series through our library but it will be a
> > while before I receive it.
> >
> >
> > Regards,
> >
> > Neme
> > ---------------------------------------------------------------------------
> >--- Neme Okechukwu Nnolim
> > Department of Materials Science, New Jersey Institute of Technology
> > Room 302, Tiernan Hall, 161 Warren Street, University Heights
> > Newark, New Jersey 07102-1982
> > Tel: (973) 596-8283, FAX: (973) 596-5794
> > ---------------------------------------------------------------------------
> >----
> >
> >
> >
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
> > majordomo@zeus.theochem.tuwien.ac.at
> > ====
> 
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> 

- -- 

- ------------------------------------------------------------------------------
Neme Okechukwu Nnolim
Department of Materials Science, New Jersey Institute of Technology
Room 302, Tiernan Hall, 161 Warren Street, University Heights
Newark, New Jersey 07102-1982
Tel: (973) 596-8283, FAX: (973) 596-5794
- -------------------------------------------------------------------------------


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------------------------------

Date: Wed, 14 Aug 2002 10:23:48 +0800
From: Wenhui Xie <xiewh@sun20.iphy.ac.cn>
Subject: Re: [WIEN]: The problem in band character plot

====
Wenhui Xie <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear Naqano,

I just run lapw1 again to produce the case.energy.

Best Regards

Wenhui Xie


On Tuesday 13 August 2002 01:39 pm, Ichiro Nagano wrote:
> ====
> "Ichiro Nagano" <nagano@atrc.mhi.co.jp>
> submitted the following contribution:
> ====
>
> Dear Dr. Wenhui Xie and WIEN2k users,
>
> I have a same problem.
>
> I tried TiC Bandstructure (with band character) as routine manner.
> (Generate k-list, edit tic.in1, lapw1 -up, edit tic.in2, and
> lapw2 -up -qtl.)
>
> When I start lapw2 with -up spin option, the program seems to search
> opposite down spin (tic.energydn) file. (see below)
>
> executing: x lapw2 -up -qtl
> PGFIO-F-252/list-directed read/unit=29/operation attempted after end of
> file.
>  File name = tic.energydn    formatted, sequential access   record = 698
>  In source file fermi.f, at line number 63
> 0.040u 0.020s 0:00.15 40.0%     0+0k 0+0io 443pf+0w
> RETURN key to continue ...
.............................
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------------------------------

Date: Wed, 14 Aug 2002 15:03:23 +0200
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: Two questions

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

I have two different questions that I would appreciate your help with:

1. I am working on a case where I add LDA+U to the calculation. When 
comparing the bandstructures calculated with and without LDA+U, I can 
see that the Fermi energy has changed drastically. Without ordinary LDA 
(no U) there is a lot bands below the Fermi energy, but when LDA+U is 
added about half of the number of bands that were below E_f are instead 
above it. This seems strange! I am loosing electrons here or what happens?

2. When I reach self-consistency I always save my case in a separate 
directory (save_lapw -d) before calculating properties. I suppose I 
should not change (cd) to this new directory before starting to 
calculate properties like bandstructure and DOS. I always calculate 
properties from the original case directory where I started the SCF 
cycle. It this the correct approach?

Best regards,
Thomas Claesson



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------------------------------

Date: Wed, 14 Aug 2002 15:29:40 +0200
From: Thomas Claesson <thomas@matphys.kth.se>
Subject: [WIEN]: kgen crashes with segmentation fault

====
Thomas Claesson <thomas@matphys.kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

I am running Wien2k on an AIX multiprocessor system. Some days ago I 
found out that every time I try to run kgen (with x kgen) it crashes 
with an error message like

Segmentation fault (core dumped)
0.0u 0.0s 0:00 0% 0+0k 0+0io 0pf+0w

I tried downloading kgen again and it compiles just fine without any 
errors. I have used the xlf90 compiler. All the other programs seem to 
run fine. What could this mean and what can I do to avoid it? Any 
suggestions are welcome!

Thanks for your replies!

Best regards,
Thomas Claesson




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------------------------------

Date: Wed, 14 Aug 2002 16:16:37 +0200
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: A question and a comment

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

First a comment:

I really liked the new introductory text about DFT and LAPW-methods 
written by S. Cottenier and available at 
http://www.wien2k.at/reg_user/textbooks/. I downloaded the ps file 
version of the text, which was OK, but pdf-file is obviously not 
working. It would be usefull to have it pdf format as well, so I would 
appreciate it if Stefaan and/or the Wien people could fix that.

Then my question:

I wonder about the Fermi energy calculated in the SCF cycle. Suppose my 
case.scf file says that the Fermi energy is 0.52 Ry, where is the zero 
of that energy scale? In the above mentioned text it says that: 
"whenever an energy is expressed in Ry it is relative to a scale where 
the zero corresponds to the average potential in the interstitial 
region". Is this really true also for the Fermi energy itself?


Thanks for your replies!

Best regards,
Thomas Claesson



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------------------------------

Date: Wed, 14 Aug 2002 16:29:02 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Two questions - answer to the second one

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Thomas,

I have no real clue to the first question... I would guess it has 
something to do with how you select the U.

But to the second question... it is probably correct. You can always 
restore from your saved calculation if something fails. However, I 
usually save everything before doing properties, just to be sure I can 
reproduce them and that I will not get results related to the next (or 
next-next) cycle in stead. In the ideal case it should not matter. 
However, I don't do ideal cases.

Best regards,
Torsten.

Thomas Claesson wrote:

> ====
> Thomas Claesson <tcl@kth.se>
> submitted the following contribution:
> ====
>
> Dear Wien users and developers!
>
> I have two different questions that I would appreciate your help with:
>
> 1. I am working on a case where I add LDA+U to the calculation. When 
> comparing the bandstructures calculated with and without LDA+U, I can 
> see that the Fermi energy has changed drastically. Without ordinary 
> LDA (no U) there is a lot bands below the Fermi energy, but when LDA+U 
> is added about half of the number of bands that were below E_f are 
> instead above it. This seems strange! I am loosing electrons here or 
> what happens?
>
> 2. When I reach self-consistency I always save my case in a separate 
> directory (save_lapw -d) before calculating properties. I suppose I 
> should not change (cd) to this new directory before starting to 
> calculate properties like bandstructure and DOS. I always calculate 
> properties from the original case directory where I started the SCF 
> cycle. It this the correct approach?
>
> Best regards,
> Thomas Claesson
>
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Wed, 14 Aug 2002 07:32:01 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: XLstart

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started Initializ cale and got this
message(Xlstart:ERROR In OPENING UNIT:5
 FILE Name:
home inst
STATUS:Old         FORM:Formated
0.000u,0.000s....   0+0k     167pf+0w
and in "view outputstin" disappear System Error). what
dose it mean?or What is its reason?
What should be done for eliminating it?
Thank you for the guide.
H-Salehi 
Dept of physics
Ferdowsi University
MASHHAD IRAN


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------------------------------

Date: Wed, 14 Aug 2002 07:34:13 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: Xlape2-

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started  XSPES  and got this
message(PGFIO-F-231/formated read /unit=1001/error on
data conversion or PGFIO-F-217/list-directed read
/unit=30/attempt to read past end of file:
filename=home.energyup  formatted,sequential access
record=285) in "Xlapw2-qtl-up". what dose it mean?
Thank you for the guide.
H-Salehi 




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------------------------------

Date: Wed, 14 Aug 2002 07:35:31 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: Xlape2

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started  XSPES  and got this
message(PGFIO-F-231/formated read /unit=1001/error on
data conversion) in "Xlapw2-qtl-up". what dose it
mean?
Thank you for the guide.
H-Salehi 



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------------------------------

Date: Wed, 14 Aug 2002 07:39:53 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Two questions

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> 1. I am working on a case where I add LDA+U to the calculation. When
> comparing the bandstructures calculated with and without LDA+U, I can
> see that the Fermi energy has changed drastically. Without ordinary LDA
> (no U) there is a lot bands below the Fermi energy, but when LDA+U is
> added about half of the number of bands that were below E_f are instead
> above it. This seems strange! I am loosing electrons here or what happens?


Although it is beloved that LDA+U is not a pure ab initio calculation, it is
still an all electronic calculation. It is not as we add an extra potential
and so mix the initial DFT Hamiltonian with a given term of a model
Hamiltonian. It is still as the system under LDA+U study should not be
charged or inversely discharged by electrons. Thus, the total number of
electrons must within LDA+U remains constant changing the U value from zero
to any other positive value. Therefore, one would first check this role
integrating from the total DOS in the valence bands and semicore bands,
analyze total :QTL value, or look at in2 file. After this, one would look at
inc file to find the number of core electrons, and then plus it to total
number of valence electrons (semi core + valence). I am sure it will rich a
same value both for U=0 and U<>0, as number of electrons is independent of U
value. But Tomas, please consider this fact that U may change the bands
drastically depending on how the system is strongly correlated, as it is its
task to rich what DOS's or physics one is looking for.

Your,
S. Jalali.

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------------------------------

Date: Wed, 14 Aug 2002 10:48:57 -0400
From: Jeff Spirko <spirko@lehigh.edu>
Subject: Re: [WIEN]: kgen crashes with segmentation fault

====
Jeff Spirko <spirko@lehigh.edu>
submitted the following contribution:
====

On Wed, Aug 14, 2002 at 03:29:40PM +0200, Thomas Claesson wrote:
> I am running Wien2k on an AIX multiprocessor system. Some days ago I 
> found out that every time I try to run kgen (with x kgen) it crashes 
> with an error message like
> 
> Segmentation fault (core dumped)
> 0.0u 0.0s 0:00 0% 0+0k 0+0io 0pf+0w
> 
> I tried downloading kgen again and it compiles just fine without any 
> errors. I have used the xlf90 compiler. All the other programs seem to 
> run fine. What could this mean and what can I do to avoid it? Any 
> suggestions are welcome!

Try increasing your stack size before running kgen.  128MB seems to
be enough for kgen.  Choose from the following:
  bash>    ulimit -s unlimited       # automatically chooses hard limit
  ksh>     ulimit -s 131072
  csh>     limit stacksize 131072


- -- 
Jeff Spirko   spirko@lehigh.edu   spirko@yahoo.com   WD3V   |=>

The study of non-linear physics is like the study of non-elephant biology.

All theoretical chemistry is really physics;
and all theoretical chemists know it. -- Richard P. Feynman 
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Date: Wed, 14 Aug 2002 08:08:27 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: Two questions

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====


- --- Thomas Claesson <tcl@kth.se> wrote:
> ====
> Thomas Claesson <tcl@kth.se>
> submitted the following contribution:
> ====
>"whenever an energy is expressed in Ry it is relative
>to a scale where 
>the zero corresponds to the average potential in the
>interstitial 
>region". Is this really true also for the Fermi
>energy itself?

Yes
> 2. When I reach self-consistency I always save my
> case in a separate 
> directory (save_lapw -d) before calculating
> properties. I suppose I 
> should not change (cd) to this new directory before
> starting to 
> calculate properties like bandstructure and DOS. I
> always calculate 
> properties from the original case directory where I
> started the SCF 
> cycle. It this the correct approach?

Yes

> 1. I am working on a case where I add LDA+U to the
> calculation. When 
> comparing the bandstructures calculated with and
> without LDA+U, I can 
> see that the Fermi energy has changed drastically.
> Without ordinary LDA 
> (no U) there is a lot bands below the Fermi energy,
> but when LDA+U is 
> added about half of the number of bands that were
> below E_f are instead 
> above it. This seems strange! I am loosing electrons
> here or what happens?

The short answer is no, you are probably splitting
a correlated band into a lower Hubbard band and an
upper Hubbard band.

A long answer is: ideologically, LDA+U is very much
not the same as DFT. DFT is a well defined
approximation, which (with many reservations) can be
used by a knowledgeble solid state physicist without
previous experience in the field. LDA+U is NOT a well
defined approximation. First, it includes something
missing in LDA and misses something included in LDA.
It may be substantially inferior to straight LDA.
Second, it is not unique. It involves poorly defined
parameters U and J and a selection of different double
counting terms, all reflecting diferent physics.
Third, unlike LDA, it has much more often metastable
solutions which are not the ground state, but can be
easily mistaken for one. For these reasons, before
indulging in LDA+U calculations even a highly
qualified theorist, in my opininon, should thoroughly
study the literature and the theory of correlated
systems, to have a clear idea what kind of physics he
or she expects to describe using LDA+U, and WHY this
physics requires specifically LDA+U approach.

Good luck.
Igor

=====


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------------------------------

Date: Wed, 14 Aug 2002 10:58:40 -0700 (PDT)
From: Javad Hashemifar <s_javad@yahoo.com>
Subject: Re: [WIEN]: Xlape2-

====
Javad Hashemifar <s_javad@yahoo.com>
submitted the following contribution:
====


- --- hamid salehi <salehihamid@yahoo.com> wrote:
> ====
> hamid salehi <salehihamid@yahoo.com>
> submitted the following contribution:
> ====
> 
> Dear wien users.
> Ihave started  XSPES  and got this
> message(PGFIO-F-231/formated read /unit=1001/error
> on
> data conversion or PGFIO-F-217/list-directed read
> /unit=30/attempt to read past end of file:
> filename=home.energyup  formatted,sequential access
> record=285) in "Xlapw2-qtl-up". what dose it mean?
> Thank you for the guide.
> H-Salehi 
> 

I think that you have a spin polarized system but you
are trying to plot a non spin polarized band
structure.
May be the up and down switches aren't active in your
w2web interface. May be your problem solved if you run

"x lapw2 -up(dn) -qtl" in command box or terminal.
Bests.
J. Hashemifar
Isfahan univ. of Tech., Isfahan, Iran


> 
> 
> 
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------------------------------

Date: Wed, 14 Aug 2002 11:07:52 -0700 (PDT)
From: Javad Hashemifar <s_javad@yahoo.com>
Subject: Re: [WIEN]: XLstart

====
Javad Hashemifar <s_javad@yahoo.com>
submitted the following contribution:
====


- --- hamid salehi <salehihamid@yahoo.com> wrote:
> ====
> hamid salehi <salehihamid@yahoo.com>
> submitted the following contribution:
> ====
> 
> Dear wien users.
> Ihave started Initializ cale and got this
> message(Xlstart:ERROR In OPENING UNIT:5
>  FILE Name:
> home inst
> STATUS:Old         FORM:Formated
> 0.000u,0.000s....   0+0k     167pf+0w
> and in "view outputstin" disappear System Error).
> what
> dose it mean?or What is its reason?
> What should be done for eliminating it?
> Thank you for the guide.
> H-Salehi 
> Dept of physics
> Ferdowsi University
> MASHHAD IRAN
> 

dear Hamid,
Are you sure that you have a case.inst file.
A problem that may be occured is thta after struct
generelization and saving it you didn't click on 
"save file and clean up".
After clicking it, the case.inst file will produced.
Bests.
J. Hashemifar
Isfahan Univ. of Tech.
Isfahan. Iran



> 
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------------------------------

Date: Wed, 14 Aug 102 19:39:31 -0300 (EST)
From: Luiz Alberto Terrazo <lterrazo@macbeth.if.usp.br>
Subject: [WIEN]: intel IFC compiler

====
Luiz Alberto Terrazo <lterrazo@macbeth.if.usp.br>
submitted the following contribution:
====

Dear Wien users
I installed the wien2k code in a cluster machine (PIII) with Linux . I would like to know where I can download the IFC intel compiler.
best regards
luis
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------------------------------

Date: Thu, 15 Aug 2002 11:01:51 +0900
From: Hiroshi Tanaka <tanakah@riko.shimane-u.ac.jp>
Subject: Re: [WIEN]: intel IFC compiler

====
Hiroshi Tanaka <tanakah@riko.shimane-u.ac.jp>
submitted the following contribution:
====

Dear Luis,

At 19:39 02/08/14 -0300, you wrote:
>I would like to know where I can download the IFC intel compiler.
>best regards

You can download it from,
http://www.intel.com/software/products/global/eval.htm

Regards,
Hiroshi


Hiroshi Tanaka
Dept. of Material Science, Faculty of Sci. & Eng.
Shimane Univ.
E-mail:tanakah@riko.shimane-u.ac.jp
Phone :+81-852-32-6386
$BEg:,Bg3XAm9gM}9)3XItJ*<A2J3X2J(B
$BEDCf(B $B9(;V(B
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------------------------------

Date: Wed, 14 Aug 2002 13:16:49 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: [WIEN]: can antiferromagnetic be mimicked by U?

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

Dear all,

It is shown that TOTMM of FeAl within LDA+(U=5eV) calculation drops to zero
from the value obtained, 0.73mB, within LDA+(U=0)  calculation. It is an
indication of LDA+U capability to predict paramagnetic behavior which is in
excellent agreement with experiment and in contrast to predicted
ferromagnetic behavior by pure LDA. Consider a highly correlated
paramagnetic compound at room temperature. However, suppose it is an
antiferromagnetic system at low temperature with a small moment around
0.2mB. So to calculate low temperature properties, one would first make a
super cell with a known oriented spin directions classifying/indexing
equivalent atoms to non equivalent atoms to reproduce the experimental
values changing the external U parameter. This is one natural way, but I am
not sure if the following way also is a reasonable physical way or not:
Instead of making antiferromagnetic super cell, going through the problem
ferromagnetically within the primitive cell without assuming any initial
spin directions just changing the U value to regenerate the small
experimental moment. Then, keeping the obtained U value, try to find another
physical quantity taking still the ferromagnetic treatment into account.
Please notice that the obtained U values within antiferromagnetic and
ferromagnetic treatments can be different.

Now my two questions are as follows:

Can the obtained U value of a natural antiferromagnetic system within a
ferromagneticaly magnetic moment calculation mimic the antiferromagnetic
situation?

Can the obtained U value of a natural antiferromagnetic system within a
ferromagneticaly magnetic moment calculation mimic the paramagnetic
situation considering the small moment 0.2mB? This means that can the
calculation be extended to the room temperature?


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------------------------------

Date: Thu, 15 Aug 2002 17:13:02 +0200
From: Thomas Claesson <tcl@kth.se>
Subject: Re: [WIEN]: Two questions

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

Many thanks for your replies, Igor and Saeid. However I am still a bit 
confused about the results I get. I have compared running LDA+U where U 
is very small U (0.0001 Ry) and ordinary LDA (no U). The strange thing 
is that the bands look almost the same in these two cases but the Fermi 
energy shifts drastically. This surprises me, how can the Fermi energy 
shift so much with U so close to zero? The case I am workning on is NiO 
in the AF II configuration. Any suggestions are welcome!

Thanks for yuor replies!

Best regards,
Thomas Claesson

>====
>Igor Mazin <wienuser1@yahoo.com>
>submitted the following contribution:
>====
>
>
>--- Thomas Claesson <tcl@kth.se> wrote:
>
>>====
>>Thomas Claesson <tcl@kth.se>
>>submitted the following contribution:
>>====
>>"whenever an energy is expressed in Ry it is relative
>>to a scale where 
>>the zero corresponds to the average potential in the
>>interstitial 
>>region". Is this really true also for the Fermi
>>energy itself?
>>
>
>Yes
>
>>2. When I reach self-consistency I always save my
>>case in a separate 
>>directory (save_lapw -d) before calculating
>>properties. I suppose I 
>>should not change (cd) to this new directory before
>>starting to 
>>calculate properties like bandstructure and DOS. I
>>always calculate 
>>properties from the original case directory where I
>>started the SCF 
>>cycle. It this the correct approach?
>>
>
>Yes
>
>>1. I am working on a case where I add LDA+U to the
>>calculation. When 
>>comparing the bandstructures calculated with and
>>without LDA+U, I can 
>>see that the Fermi energy has changed drastically.
>>Without ordinary LDA 
>>(no U) there is a lot bands below the Fermi energy,
>>but when LDA+U is 
>>added about half of the number of bands that were
>>below E_f are instead 
>>above it. This seems strange! I am loosing electrons
>>here or what happens?
>>
>
>The short answer is no, you are probably splitting
>a correlated band into a lower Hubbard band and an
>upper Hubbard band.
>
>A long answer is: ideologically, LDA+U is very much
>not the same as DFT. DFT is a well defined
>approximation, which (with many reservations) can be
>used by a knowledgeble solid state physicist without
>previous experience in the field. LDA+U is NOT a well
>defined approximation. First, it includes something
>missing in LDA and misses something included in LDA.
>It may be substantially inferior to straight LDA.
>Second, it is not unique. It involves poorly defined
>parameters U and J and a selection of different double
>counting terms, all reflecting diferent physics.
>Third, unlike LDA, it has much more often metastable
>solutions which are not the ground state, but can be
>easily mistaken for one. For these reasons, before
>indulging in LDA+U calculations even a highly
>qualified theorist, in my opininon, should thoroughly
>study the literature and the theory of correlated
>systems, to have a clear idea what kind of physics he
>or she expects to describe using LDA+U, and WHY this
>physics requires specifically LDA+U approach.
>
>Good luck.
>Igor
>
>=====
>
>
>__________________________________________________
>Do You Yahoo!?
>HotJobs - Search Thousands of New Jobs
>http://www.hotjobs.com
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>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>


Although it is beloved that LDA+U is not a pure ab initio calculation, it is
still an all electronic calculation. It is not as we add an extra potential
and so mix the initial DFT Hamiltonian with a given term of a model
Hamiltonian. It is still as the system under LDA+U study should not be
charged or inversely discharged by electrons. Thus, the total number of
electrons must within LDA+U remains constant changing the U value from zero
to any other positive value. Therefore, one would first check this role
integrating from the total DOS in the valence bands and semicore bands,
analyze total :QTL value, or look at in2 file. After this, one would look at
inc file to find the number of core electrons, and then plus it to total
number of valence electrons (semi core + valence). I am sure it will rich a
same value both for U=0 and U<>0, as number of electrons is independent of U
value. But Tomas, please consider this fact that U may change the bands
drastically depending on how the system is strongly correlated, as it is its
task to rich what DOS's or physics one is looking for.

Your,
S. Jalali.




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------------------------------

Date: Thu, 15 Aug 2002 13:37:36 -0300 (ARST)
From: Fabian Dominguez <fabian@iflysib.unlp.edu.ar>
Subject: [WIEN]: TEMP-TETRA option / question for IGOR MAZIN

====
Fabian Dominguez <fabian@iflysib.unlp.edu.ar>
submitted the following contribution:
====


Dear Wien users,

I'm trying to run Fe-Nd and as if the case  in previous Fe-Nd-B runnings I
have problems of oscilations, and I get :DIS not lower than 0.02, getting
this value doing oscilations.
Questions are two:

I did these running using TETRA and after TEMP option, last one with eval
in 0.002, question is:

In a previous WIEN mails I saw thar somebody was told to use TEMP option,
BUT finally convergence MUST be got using TETRA, Is this true? or I can do
convergence till the end using TEMP or GAUSS option...?

Question 2:

How could I do to use TETRA option which I think is the best and get
through these problemas of converging?

IGOR...I need to say that in big cell NdFeB I use TEMP option and after I
didn't turn to TETRA option to get final convergence
It's necessary to say now I'm doing a running of NdFeB but with TETRA, and
apparently nothing strange happens, I mean oscilations..

Regards,
Fabian




============================***=================================

Lic. Fabian Alfredo Dominguez Avenalle.
Instituto de Fisica de Liquidos y Sistemas Biologicos (IFLYSIB).
Universidad Nacional de La Plata (UNLP).
Calle 59 N 789 La Plata CP.  1900  BUENOS AIRES  ARGENTINA
CC. 565
TE: 0221-4233283
TELEFAX: 0221-4257317
E-MAIL: fabian@iflysib.unlp.edu.ar
============================***=================================


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------------------------------

Date: Wed, 14 Aug 2002 22:46:40 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Two questions

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> energy shifts drastically. This surprises me, how can the Fermi energy
> shift so much with U so close to zero?
As far as I remember, it is recommended by the authors to use LDA for LDA+U
calculation and not any more advanced extended approximations for the
exchange correlation potential. This says that one should not compare GGA+U
with GGA or LDA+U with GGA and so on. I suggest to first check your LDA+U
calculation for a rather simple example, for instance fcc-Sm. Perhaps it is
better to wait to see if Igor would give us some insights in this respect.
Your,
S. Jalali.

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------------------------------

Date: Thu, 15 Aug 2002 11:30:35 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: Two questions

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

When you plot bands, do you not forget to add -orb to
lapw?

- --- Thomas Claesson <tcl@kth.se> wrote:
> ====
> Thomas Claesson <tcl@kth.se>
> submitted the following contribution:
> ====
> 
> Dear Wien users and developers!
> 
> Many thanks for your replies, Igor and Saeid.
> However I am still a bit 
> confused about the results I get. I have compared
> running LDA+U where U 
> is very small U (0.0001 Ry) and ordinary LDA (no U).
> The strange thing 
> is that the bands look almost the same in these two
> cases but the Fermi 
> energy shifts drastically. This surprises me, how
> can the Fermi energy 
> shift so much with U so close to zero? The case I am
> workning on is NiO 
> in the AF II configuration. Any suggestions are
> welcome!
> 
> Thanks for yuor replies!
> 
> Best regards,
> Thomas Claesson
> 
> >====
> >Igor Mazin <wienuser1@yahoo.com>
> >submitted the following contribution:
> >====
> >
> >
> >--- Thomas Claesson <tcl@kth.se> wrote:
> >
> >>====
> >>Thomas Claesson <tcl@kth.se>
> >>submitted the following contribution:
> >>====
> >>"whenever an energy is expressed in Ry it is
> relative
> >>to a scale where 
> >>the zero corresponds to the average potential in
> the
> >>interstitial 
> >>region". Is this really true also for the Fermi
> >>energy itself?
> >>
> >
> >Yes
> >
> >>2. When I reach self-consistency I always save my
> >>case in a separate 
> >>directory (save_lapw -d) before calculating
> >>properties. I suppose I 
> >>should not change (cd) to this new directory
> before
> >>starting to 
> >>calculate properties like bandstructure and DOS. I
> >>always calculate 
> >>properties from the original case directory where
> I
> >>started the SCF 
> >>cycle. It this the correct approach?
> >>
> >
> >Yes
> >
> >>1. I am working on a case where I add LDA+U to the
> >>calculation. When 
> >>comparing the bandstructures calculated with and
> >>without LDA+U, I can 
> >>see that the Fermi energy has changed drastically.
> >>Without ordinary LDA 
> >>(no U) there is a lot bands below the Fermi
> energy,
> >>but when LDA+U is 
> >>added about half of the number of bands that were
> >>below E_f are instead 
> >>above it. This seems strange! I am loosing
> electrons
> >>here or what happens?
> >>
> >
> >The short answer is no, you are probably splitting
> >a correlated band into a lower Hubbard band and an
> >upper Hubbard band.
> >
> >A long answer is: ideologically, LDA+U is very much
> >not the same as DFT. DFT is a well defined
> >approximation, which (with many reservations) can
> be
> >used by a knowledgeble solid state physicist
> without
> >previous experience in the field. LDA+U is NOT a
> well
> >defined approximation. First, it includes something
> >missing in LDA and misses something included in
> LDA.
> >It may be substantially inferior to straight LDA.
> >Second, it is not unique. It involves poorly
> defined
> >parameters U and J and a selection of different
> double
> >counting terms, all reflecting diferent physics.
> >Third, unlike LDA, it has much more often
> metastable
> >solutions which are not the ground state, but can
> be
> >easily mistaken for one. For these reasons, before
> >indulging in LDA+U calculations even a highly
> >qualified theorist, in my opininon, should
> thoroughly
> >study the literature and the theory of correlated
> >systems, to have a clear idea what kind of physics
> he
> >or she expects to describe using LDA+U, and WHY
> this
> >physics requires specifically LDA+U approach.
> >
> >Good luck.
> >Igor
> >
> >=====
> >
> >
> >__________________________________________________
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> >To (un)subscribe send mail to
> >majordomo@zeus.theochem.tuwien.ac.at
> >====
> >
> 
> 
> Although it is beloved that LDA+U is not a pure ab
> initio calculation, it is
> still an all electronic calculation. It is not as we
> add an extra potential
> and so mix the initial DFT Hamiltonian with a given
> term of a model
> Hamiltonian. It is still as the system under LDA+U
> study should not be
> charged or inversely discharged by electrons. Thus,
> the total number of
> electrons must within LDA+U remains constant
> changing the U value from zero
> to any other positive value. Therefore, one would
> first check this role
> integrating from the total DOS in the valence bands
> and semicore bands,
> analyze total :QTL value, or look at in2 file. After
> this, one would look at
> inc file to find the number of core electrons, and
> then plus it to total
> number of valence electrons (semi core + valence). I
> am sure it will rich a
> same value both for U=0 and U<>0, as number of
> electrons is independent of U
> value. But Tomas, please consider this fact that U
> may change the bands
> drastically depending on how the system is strongly
> correlated, as it is its
> task to rich what DOS's or physics one is looking
> for.
> 
> Your,
> S. Jalali.
> 
> 
> 
> 
> ====
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> ====


=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

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------------------------------

Date: Thu, 15 Aug 2002 11:34:30 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: TEMP-TETRA option / question for IGOR MAZIN

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====


- --- Fabian Dominguez <fabian@iflysib.unlp.edu.ar>
wrote:
> ====
> Fabian Dominguez <fabian@iflysib.unlp.edu.ar>
> submitted the following contribution:
> ====
> 
> > In a previous WIEN mails I saw thar somebody was
> told to use TEMP option,
> BUT finally convergence MUST be got using TETRA, Is
> this true? or I can do

Yes.

> It's necessary to say now I'm doing a running of
> NdFeB but with TETRA, and
> apparently nothing strange happens, I mean
> oscilations..

Sure. If you use temp smearing, you converge faster
and smoother, but to a wrong result. The more wrong
the larger T, and the better convergence the larger T.
Fermi or Gauss, does not matter. There were many
papers on this, for instance Paxton and Methfessel
around 1990.


=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

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------------------------------

Date: Thu, 15 Aug 2002 13:08:25 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: Two questions

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====


- --- Saeid Jalali <sjalali@cc.iut.ac.ir> wrote:
> ====
> "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> submitted the following contribution:
> ====
> 
> As far as I remember, it is recommended by the
> authors to use LDA for LDA+U
> calculation and not any more advanced extended
> approximations for the
> exchange correlation potential. This says that one
> should not compare GGA+U
> with GGA 

I do not see any reason why not.

> better to wait to see if Igor would give us some
> insights in this respect.

Thanks, but I have none. My earlier question was
irrelevant. With U that small it should not matter
whatsoever whether you put -orb in or not.

Case.scf has Fermi energy in it, from iteration to
iteration. Make several iterations with U=0.0001 and
J=0.0001 and then one without -orb. If you are
converged, nothing should change, including Fermi.

If this is so, but your bands are plotted with an
incorrect Ef, you will know were to look then.

Igor
> Your,
> S. Jalali.
> 
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====


=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

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------------------------------

Date: Thu, 15 Aug 2002 11:38:08 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Two questions

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> > As far as I remember, it is recommended by the
> > authors to use LDA for LDA+U
> > calculation and not any more advanced extended
> > approximations for the
> > exchange correlation potential. This says that one
> > should not compare GGA+U
> > with GGA

> I do not see any reason why not.
Let's below give it a try:
Basically, taking the LDA+U into account, (T+Vei+VH+VXC+VLDA+U) ji = ei ji ,
and comparing obtained total energy with the regular DFT equation, where the
later LDA+U potential is not there, allows to utilize any versions of
exchange correlation approximations. This means that in general comparing
GGA+U and GGA is also permitted. Why it is recommended to only use LDA
turning on the light of U, maybe is to not take into account further
correction in correlation potential. This means that any correlation
corrections have been entrusted to U and J parameters. Using GGA+U leads to
a U which may differ from the U value obtained via LDA+U. Thus maybe to find
a U and a J for a case at least employing wien code it is recommended to use
one version of exchange correlation potential which is selected to be LDA by
the wien author. Although U and J are considered as external parameters,
they are not so far from experiment within LDA.

> Case.scf has Fermi energy in it, from iteration to
> iteration. Make several iterations with U=0.0001 and
> J=0.0001 and then one without -orb. If you are
> converged, nothing should change, including Fermi.
>
> If this is so, but your bands are plotted with an
> incorrect Ef, you will know were to look then.

Here you touch a good point, and Thomas would pay attention to put manually
the correct Ef from the last iteration: grepline :FER *.scf 1.

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------------------------------

End of wien-digest V2002 #31
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #32
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
Errors-To: owner-wien-digest@theochem.tuwien.ac.at
Precedence: bulk


wien-digest         Friday, August 23 2002         Volume 2002 : Number 032




----------------------------------------------------------------------

Date: Thu, 15 Aug 2002 08:20:12 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: can antiferromagnetic be mimicked by U?

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

> "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> submitted the following contribution:
> ====
> It is shown that TOTMM of FeAl within LDA+(U=5eV)
> calculation drops to zero
> from the value obtained, 0.73mB, within LDA+(U=0) 
> calculation. 

Correct.

> It is an indication of LDA+U capability to predict
> paramagnetic behavior which is in
> excellent agreement with experiment

Not really. This is an indication that a particular
implementation of LDA+U accidentally has a regime (for
an unphysically large U) where the nonmagnetic
solution is lower in energy. In LDA-ASA+U, which is
likely better than LAPW+U for FeAl, due to close
packing and only moderate localization of Fe d's, the
region of nonmagnetic ground state disappears (Andre
Petukhov, unpublished). DMFT calculations stabilize
the nonmagnetic state for FeAl at reasonable U's,
independent of implementation, and without DOS
reduction (Lichtenstein and Chioncel, unpublished,
partially included in the cond-mat below).

More in http://www.arxiv.org/abs/cond-mat/0206548.

"There is infinite number of incorrect theories,
correctly describing a finite number of correct
experiments" - Bohr.

> suppose it is an
> antiferromagnetic system at low temperature with a
> small moment around
> 0.2mB. So to calculate low temperature properties,
> one would first make a
> super cell with a known oriented spin directions
> classifying/indexing
> equivalent atoms to non equivalent atoms to
> reproduce the experimental
> values changing the external U parameter. This is
> one natural way, but I am

This the right way, except U should not, generally
speaking, be used as an adjustable parameter (there
are exceptions, though). At least not outside a
reasonable range given, say, by constrained DFT
calculations of Anisimov-Gunnarsson type, or similar.

> not sure if the following way also is a reasonable
> physical way or not:

Not. First, all physics associated with the
superexchange, usually of utmost importance, is lost
this way. Second, U is not an adjustable parameter. It
is a prameter which is difficult to calculate, but it
does not mean one is permitted to use it as a knob
disregarding its physical meaning.

> Instead of making antiferromagnetic super cell,
> going through the problem
> ferromagnetically within the primitive cell without
> assuming any initial
> spin directions just changing the U value to
> regenerate the small
> experimental moment. Then, keeping the obtained U
> value, try to find another
> physical quantity taking still the ferromagnetic
> treatment into account.
> Please notice that the obtained U values within
> antiferromagnetic and
> ferromagnetic treatments can be different.

I do not understand either of these following
questions.
> 
> Now my two questions are as follows:
> 
> Can the obtained U value of a natural
> antiferromagnetic system within a
> ferromagneticaly magnetic moment calculation mimic
> the antiferromagnetic
> situation?
> 
> Can the obtained U value of a natural
> antiferromagnetic system within a
> ferromagneticaly magnetic moment calculation mimic
> the paramagnetic
> situation considering the small moment 0.2mB? This
> means that can the
> calculation be extended to the room temperature?
> 
> 
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====


=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

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------------------------------

Date: Fri, 16 Aug 2002 07:23:10 -0700 (PDT)
From: Ivan Oleynik <ivanolen@yahoo.com>
Subject: Re: [WIEN]: intel IFC compiler

====
Ivan Oleynik <ivanolen@yahoo.com>
submitted the following contribution:
====

Go to http://www.intel.com/software/products/compilers/

They provide free unsupported licenses for C++ and Fortran
compilers for academics.

- --- Luiz Alberto Terrazo <lterrazo@macbeth.if.usp.br> wrote:
> ====
> Luiz Alberto Terrazo <lterrazo@macbeth.if.usp.br>
> submitted the following contribution:
> ====
> 
> Dear Wien users
> I installed the wien2k code in a cluster machine (PIII) with
> Linux . I would like to know where I can download the IFC
> intel compiler.
> best regards
> luis
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
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------------------------------

Date: Fri, 16 Aug 2002 07:43:04 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: Two questions

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

1. I did not find anywhere any recommendation from the
authors of WIEN2k not to use GGA with U.
2. I would be surprised to find one, for Vienna people
just started with LDA+U and if from anywhere, I'd
expect practical recommendation of this sort from
Ekaterinburg group etc.
3. I am not aware of any statistics showing GGA+U to
be more inferior/superior to LDA+U than GGA to LDA.
4. If such statistics existed, it'd be strange, for
GGA and +U strive to correct entirely different and
unrelated deficiencies in LDA. It does not mean I say
it is impossible, just it'd be unexpected, and I never
heard about such situation being systematically
observed. I myself did GGA+U with WIEN2k and did not
not notice any problem. 

- --- Saeid Jalali <sjalali@cc.iut.ac.ir> wrote:
> ====
> "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> submitted the following contribution:
> ====
> 
> > > As far as I remember, it is recommended by the
> > > authors to use LDA for LDA+U
> > > calculation and not any more advanced extended
> > > approximations for the
> > > exchange correlation potential. This says that
> one
> > > should not compare GGA+U
> > > with GGA
> 
> > I do not see any reason why not.
> Let's below give it a try:
> Basically, taking the LDA+U into account,
> (T+Vei+VH+VXC+VLDA+U) ji = ei ji ,
> and comparing obtained total energy with the regular
> DFT equation, where the
> later LDA+U potential is not there, allows to
> utilize any versions of
> exchange correlation approximations. This means that
> in general comparing
> GGA+U and GGA is also permitted. Why it is
> recommended to only use LDA
> turning on the light of U, maybe is to not take into
> account further
> correction in correlation potential. This means that
> any correlation
> corrections have been entrusted to U and J
> parameters. Using GGA+U leads to
> a U which may differ from the U value obtained via
> LDA+U. Thus maybe to find
> a U and a J for a case at least employing wien code
> it is recommended to use
> one version of exchange correlation potential which
> is selected to be LDA by
> the wien author. Although U and J are considered as
> external parameters,
> they are not so far from experiment within LDA.
> 
> > Case.scf has Fermi energy in it, from iteration to
> > iteration. Make several iterations with U=0.0001
> and
> > J=0.0001 and then one without -orb. If you are
> > converged, nothing should change, including Fermi.
> >
> > If this is so, but your bands are plotted with an
> > incorrect Ef, you will know were to look then.
> 
> Here you touch a good point, and Thomas would pay
> attention to put manually
> the correct Ef from the last iteration: grepline
> :FER *.scf 1.
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====


=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

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------------------------------

Date: Fri, 16 Aug 2002 02:12:26 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Two questions

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> 3. I am not aware of any statistics showing GGA+U to
> be more inferior/superior to LDA+U than GGA to LDA.
> 4. If such statistics existed, it'd be strange, for
> GGA and +U strive to correct entirely different and
> unrelated deficiencies in LDA.

It'd be strange for striving of neither GGA nor +U, as GGA calculation is an
ab initio calculation but +U calculation. For more realization, one would
consider an ideal case and suppose that there is an exact analytical
expression for the exchange correlation potential, say Vxc, but still would
keep the +U potential, say Vexact+u. Now in this ideal case with exact Vxc
keeping V_(exact+u), one may ask what the U and J values are and would know
what the difference between V_(lda+u) and V_(exact+u) is. It'd be surprised
too if one says that after a self consistent calculation within such a
Vxc+V_(exact+u) calculation the values of U and J can remain those used
values in Vlda+V_(lda+u) calculation with one expression for V(+u)
potential. It is obvious that U and J are two physical quantities referring
to splitting of lower and upper bands: U+6J, but they depend on our
interpration: model we are using. Please let me ask you a question:
What will be your further attempts to put your model U-potential into the
regular Kohen-Sham equation when you are going from LDA to GGA? If the
answer is nothing, so how can the further correction of GGA be compensated
by a fixed model U-potential? Else, I am interested to know that  further
attempts.

Although I am not an expert and afraid to come closer, but I would say that:

The story of +U is different from GGA or other systematic approximations for
exchange-correlation potential. In one sight, U is coming to improve LDA,
but in the other hand U is attacking to the original concept of density
functional theory, as U is bringing with itself a new guest, Yankee, for DFT
to show DFT should be replaced by a model Hamiltonian which is another
approach. One may believe that U cannot be instead of stoner I. Stoner I is
less than U: I=~0.1*U. But this is in LDA. This means that if one can
improve LDA systematically, then stoner I will be again instead of U. As far
as I know many are trying successfully to improve LDA systematically, see
M. Nekovee, W. M. C. Foulkes, and R. J. Needs Phys. Rev. Lett. 87, 036401
(2001),  http://link.aps.org/doi/10.1103/PhysRevLett.87.036401 . So, we can
wait to see.


> It does not mean I say
> it is impossible, just it'd be unexpected, and I never
> heard about such situation being systematically
> observed.
 I don't understand what you want to say here.

> I myself did GGA+U with WIEN2k and did not
> not notice any problem.
I saw that in your SmZn case (GGA92 but not 13!), and would like here to
appreciate you a lot for those files.

> 1. I did not find anywhere any recommendation from the
> authors of WIEN2k not to use GGA with U.

I heard this.

> 2. I would be surprised to find one, for Vienna people
> just started with LDA+U and if from anywhere, I'd
> expect practical recommendation of this sort from
> Ekaterinburg group etc.

Your,
S. Jalali
PS: I am reading your recent submitted letter: cond-mat/0206548, thank you
for that!

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------------------------------

Date: Fri, 16 Aug 2002 16:03:12 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: Two questions

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

Saeid,

You touched upon several serious conceptual problems
of the LDA+U and of the DFT. I believe that many of
your thoughts are in the right direction, but this is
probably not an appropriate topic for a discussion
board like ours. Maybe we will have chance in the
future to talk about this in person. I realize this is
a remote prospective for you in Iran; unfortunately,
there are things beyond our control. But the future
may be brighter than we think.

Limiting ourselves to simpler issues, given loose and
shaky foundation of the LDA+U formalism, the
difference between LDA and GGA seems, to me, of very
secondary importance, and not worth more profound
consideration.
 
- --- Saeid Jalali <sjalali@cc.iut.ac.ir> wrote:
> > heard about such situation being systematically
> > observed.
>  I don't understand what you want to say here.

Just that there is no practical evidence that GGA+U is
worse than LDA+U.

Good luck,
Igor

=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

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------------------------------

Date: Sun, 18 Aug 2002 14:10:35 +0800
From: Wenhui Xie <xiewh@sun20.iphy.ac.cn>
Subject: [WIEN]: The problem in compiling lapw1_mpi

====
Wenhui Xie <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear Wien Users,

Please help me to find the problem in parallel compiling.
I am compiling WIEN2K in a 2-P4(XEON) CPU computer.  
The mahterboard is Tyan S2720(shipset INTEL E7500)
The lib MPI+SCALAPACK+BLACS have been installed, 
and the BLAS lib is pgf3.2 libblas.a, OS is LINUX REDHAT7.3 
Fortran compiler is pgi3.2.

Some config informations are listed below:

1.The config paramater for MPI

./configure --with-device=ch_shmem -prefix=/usr/local/mpich 
- --with-comm-prefix=/usr/local/mpich -c++=pgCC -cc=pgcc -fc=pgf77 
- -cflags="-Msignextend"  -opt=-fast -fflags="-fast -Kieee"      
- -c++flags="-fast -Kieee" -f90flags="-fast -Kieee" -f90=pgf90 
- -prefix=/usr/local/mpich


2.The Bmake.inc file to build BLACS lib

   SHELL = /bin/sh
   BTOPdir = /usr/local/BLACS
   COMMLIB = MPI
   PLAT = LINUX
   BLACSdir    = $(BTOPdir)/LIB
   BLACSDBGLVL = 0
   BLACSFINIT  = $(BLACSdir)/blacsF77init_$(COMMLIB)-$(PLAT)-$(BLACSDBGLVL).a
   BLACSCINIT  = $(BLACSdir)/blacsCinit_$(COMMLIB)-$(PLAT)-$(BLACSDBGLVL).a
   BLACSLIB    = $(BLACSdir)/blacs_$(COMMLIB)-$(PLAT)-$(BLACSDBGLVL).a
   MPIdir = /usr/local/mpich
   MPILIBdir = $(MPIdir)/lib
   MPIINCdir = $(MPIdir)/include
   MPILIB = $(MPILIBdir)/libmpich.a
   BTLIBS = $(BLACSFINIT) $(BLACSLIB) $(BLACSFINIT) $(MPILIB)
   INSTdir = $(BTOPdir)/INSTALL/EXE
   TESTdir = $(BTOPdir)/TESTING/EXE
   FTESTexe = $(TESTdir)/xFbtest_$(COMMLIB)-$(PLAT)-$(BLACSDBGLVL)
   CTESTexe = $(TESTdir)/xCbtest_$(COMMLIB)-$(PLAT)-$(BLACSDBGLVL)
   SYSINC = -I$(MPIINCdir)
   INTFACE = -DAdd_
   SENDIS =
   BUFF =
   TRANSCOMM =
   WHATMPI =
   SYSERRORS =
   DEBUGLVL = -DBlacsDebugLvl=$(BLACSDBGLVL)
   DEFS1 = -DSYSINC $(SYSINC) $(INTFACE) $(DEFBSTOP) $(DEFCOMBTOP) $(DEBUGLVL)
   BLACSDEFS = $(DEFS1) $(SENDIS) $(BUFF) $(TRANSCOMM) $(WHATMPI) $(SYSERRORS)
   F77            = pgf77
   F77NO_OPTFLAGS =
   F77FLAGS       = $(F77NO_OPTFLAGS) -fast -Kieee
   F77LOADER      = $(F77)
   F77LOADFLAGS   =
   CC             = pgcc
   CCFLAGS        = -fast -Kieee
   CCLOADER       = $(CC)
   CCLOADFLAGS    =
   ARCH      = ar
   ARCHFLAGS = r
   RANLIB    = ranlib

3.The SLmake.inc file used to build SCALAPACK Lib

SHELL         = /bin/sh
home          = /usr/local/SCALAPACK
PLAT          = LINUX
BLACSDBGLVL   = 0
BLACSdir      = /usr/local/BLACS/LIB
USEMPI        = -DUsingMpiBlacs
SMPLIB        = /usr/local/mpich/lib/libmpich.a
BLACSFINIT    = $(BLACSdir)/blacsF77init_MPI-$(PLAT)-$(BLACSDBGLVL).a
BLACSCINIT    = $(BLACSdir)/blacsCinit_MPI-$(PLAT)-$(BLACSDBGLVL).a
BLACSLIB      = $(BLACSdir)/blacs_MPI-$(PLAT)-$(BLACSDBGLVL).a
TESTINGdir    = $(home)/TESTING
CBLACSLIB     = $(BLACSCINIT) $(BLACSLIB) $(BLACSCINIT)
FBLACSLIB     = $(BLACSFINIT) $(BLACSLIB) $(BLACSFINIT)
PBLASdir      = $(home)/PBLAS
SRCdir        = $(home)/SRC
TESTdir       = $(home)/TESTING
PBLASTSTdir   = $(TESTINGdir)
TOOLSdir      = $(home)/TOOLS
REDISTdir     = $(home)/REDIST
REDISTTSTdir  = $(TESTINGdir)
F77           = mpif77
CC            = mpicc
NOOPT         =
F77FLAGS      = -fast -Kieee
DRVOPTS       = $(F77FLAGS)
CCFLAGS       = -fast -Kieee
SRCFLAG       =
F77LOADER     = $(F77)
CCLOADER      = $(CC)
F77LOADFLAGS  =
CCLOADFLAGS   =
CDEFS         = -DAdd_ -DNO_IEEE $(USEMPI)
ARCH          = ar
ARCHFLAGS     = cr
RANLIB        = ranlib
SCALAPACKLIB  = $(home)/libscalapack.a
BLASLIB       = /usr/local/pgi/linux86/lib/libblas.a
PBLIBS        = $(SCALAPACKLIB) $(FBLACSLIB) $(BLASLIB) $(SMPLIB)
PRLIBS        = $(SCALAPACKLIB) $(CBLACSLIB) $(SMPLIB)
RLIBS         = $(SCALAPACKLIB) $(FBLACSLIB) $(CBLACSLIB) $(BLASLIB) $(SMPLIB)
LIBS          = $(PBLIBS)

4. the compiler parameter of WIEN2k
Current settings:
RP  RP_LIB(SCALAPACK+PBLAS): /usr/local/mpich/lib/libmpich.a 
/usr/local/SCALAPACK/libscalapack.a /usr/local/BLACS/LIB/blacs_MPI-LINUX-0.a 
/usr/local/BLACS/LIB/blacsF77init_MPI-LINUX-0.a
 FP  FPOPT(par.comp.options): -Mfreeform -fast -Kieee
 MP  MPIRUN commando        : mpirun -np 4 -machinefile .machine executable


5. the error information given by wien2k installer:
mpif90  -o ./lapw1c_mpi abc.o atpar.o bandv1.o calkpt.o cbcomb.o coors.o 
cputim.o dblr2k.o dgeqrl.o dgewy.o dgewyg.o dlbrfg.o dsbein1.o dscgst.o 
dstebz2.o dsyevx2.o dsymm2.o dsyr2m.o dsyrb4.o dsyrb5l.o dsyrdt4.o dsytrd2.o 
dsywyv.o dsyxev4.o dvbes1.o eisps.o errclr.o errflg.o forfhs.o gaunt1.o 
gaunt2.o gbass.o gtfnam.o hamilt.o hns.o horb.o inikpt.o inilpw.o lapw1.o 
latgen.o lmsort.o locdef.o lohns.o lopw.o matmm.o modules.o nn.o outerr.o 
outwin.o pdsyevx16.o prtkpt.o prtres.o pzheevx16.o rdswar.o rint13.o rotate.o 
rotdef.o seclit.o seclr4.o seclr5.o select.o service.o setkpt.o setwar.o 
sphbes.o stern.o tapewf.o ustphx.o vectf.o warpin.o wfpnt.o wfpnt1.o ylm.o 
zhcgst.o zheevx2.o zhemm2.o zher2m.o zhetrd2.o pdsyr2m.o pzher2m.o 
- -L../SRC_lib -llapack_lapw -lblas /usr/local/mpich/lib/libmpich.a 
/usr/local/SCALAPACK/libscalapack.a /usr/local/BLACS/LIB/blacs_MPI-LINUX-0.a 
/usr/local/BLACS/LIB/blacsF77init_MPI-LINUX-0.a
/usr/local/SCALAPACK/libscalapack.a(PB_Cdtypeset.o): In function 
`PB_Cdtypeset':
PB_Cdtypeset.o(.text+0x1f4): undefined reference to `dsyr_'
/usr/local/SCALAPACK/libscalapack.a(PB_Cztypeset.o): In function 
`PB_Cztypeset':
PB_Cztypeset.o(.text+0x21f): undefined reference to `zgeru_'
PB_Cztypeset.o(.text+0x235): undefined reference to `zher_'
PB_Cztypeset.o(.text+0x25f): undefined reference to `zsymm_'
PB_Cztypeset.o(.text+0x275): undefined reference to `zsyrk_'
PB_Cztypeset.o(.text+0x28a): undefined reference to `zsyr2k_'
/usr/local/SCALAPACK/libscalapack.a(zvvdotu.o): In function `zvvdotu_':
zvvdotu.o(.text+0x47): undefined reference to `zdotu_'
/usr/local/BLACS/LIB/blacsF77init_MPI-LINUX-0.a(blacs_pinfo_.o): In function 
`blacs_pinfo_':
blacs_pinfo_.o(.text+0x37): undefined reference to `bi_f77_init_'
blacs_pinfo_.o(.text+0x82): undefined reference to `bi_f77_get_constants_'
/usr/local/BLACS/LIB/blacsF77init_MPI-LINUX-0.a(Cblacs_pinfo.o): In function 
`Cblacs_pinfo':
Cblacs_pinfo.o(.text+0x37): undefined reference to `bi_f77_init_'

Thanks very much.
Look forward to your reply!

Yours 
Wenhui Xie
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------------------------------

Date: Sun, 18 Aug 2002 10:38:58 +0200 (MET DST)
From: Pavel Novak <novakp@fzu.cz>
Subject: Re: [WIEN]: Two questions

====
Pavel Novak <novakp@fzu.cz>
submitted the following contribution:
====

Dear Saeid and Igor,

from our experience follows that GGA contains more correlation than LDA.
As a consequence using GGA+U (U=UGGA) would give, as a rule, similar
results as LDA+U (U=ULDA) for UGGA<ULDA. Because of the double counting
term GGA+U is more questionable than LDA+U. To my knowledge the only GGA+U
paper is by Savrasov and Kotliar: PRL 84, 3670 (2000). Note that these
authors use the original (Anisimov 1991) approach denoted as LDA+U(MFH) in
WIEN2k.

Regards
Pavel Novak

On Fri, 16 Aug 2002, Igor Mazin wrote:

> ====
> Igor Mazin <wienuser1@yahoo.com>
> submitted the following contribution:
> ====
>
> 1. I did not find anywhere any recommendation from the
> authors of WIEN2k not to use GGA with U.
> 2. I would be surprised to find one, for Vienna people
> just started with LDA+U and if from anywhere, I'd
> expect practical recommendation of this sort from
> Ekaterinburg group etc.
> 3. I am not aware of any statistics showing GGA+U to
> be more inferior/superior to LDA+U than GGA to LDA.
> 4. If such statistics existed, it'd be strange, for
> GGA and +U strive to correct entirely different and
> unrelated deficiencies in LDA. It does not mean I say
> it is impossible, just it'd be unexpected, and I never
> heard about such situation being systematically
> observed. I myself did GGA+U with WIEN2k and did not
> not notice any problem.
>
> --- Saeid Jalali <sjalali@cc.iut.ac.ir> wrote:
> > ====
> > "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> > submitted the following contribution:
> > ====
> >
> > > > As far as I remember, it is recommended by the
> > > > authors to use LDA for LDA+U
> > > > calculation and not any more advanced extended
> > > > approximations for the
> > > > exchange correlation potential. This says that
> > one
> > > > should not compare GGA+U
> > > > with GGA
> >
> > > I do not see any reason why not.
> > Let's below give it a try:
> > Basically, taking the LDA+U into account,
> > (T+Vei+VH+VXC+VLDA+U) ji = ei ji ,
> > and comparing obtained total energy with the regular
> > DFT equation, where the
> > later LDA+U potential is not there, allows to
> > utilize any versions of
> > exchange correlation approximations. This means that
> > in general comparing
> > GGA+U and GGA is also permitted. Why it is
> > recommended to only use LDA
> > turning on the light of U, maybe is to not take into
> > account further
> > correction in correlation potential. This means that
> > any correlation
> > corrections have been entrusted to U and J
> > parameters. Using GGA+U leads to
> > a U which may differ from the U value obtained via
> > LDA+U. Thus maybe to find
> > a U and a J for a case at least employing wien code
> > it is recommended to use
> > one version of exchange correlation potential which
> > is selected to be LDA by
> > the wien author. Although U and J are considered as
> > external parameters,
> > they are not so far from experiment within LDA.
> >
> > > Case.scf has Fermi energy in it, from iteration to
> > > iteration. Make several iterations with U=0.0001
> > and
> > > J=0.0001 and then one without -orb. If you are
> > > converged, nothing should change, including Fermi.
> > >
> > > If this is so, but your bands are plotted with an
> > > incorrect Ef, you will know were to look then.
> >
> > Here you touch a good point, and Thomas would pay
> > attention to put manually
> > the correct Ef from the last iteration: grepline
> > :FER *.scf 1.
> >
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
> > majordomo@zeus.theochem.tuwien.ac.at
> > ====
>
>
> =====
> *****************************************************************************
> Igor Mazin, Naval Research Laboratory, Washington, DC 20375
> Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin
> *****************************************************************************
>
> __________________________________________________
> Do You Yahoo!?
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> ====
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> ====
>
>
>



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------------------------------

Date: Mon, 19 Aug 2002 17:01:05 +0800
From: gyguo <gyguo@phys.ntu.edu.tw>
Subject: [WIEN]: LDA+U for systems without inversion symmetry

====
gyguo <gyguo@phys.ntu.edu.tw>
submitted the following contribution:
====


Dear Prof. Blaha and WIEN users,

We have been trying to perform LDA+U calculations without SO
for systems without inversion symmetry, and we have failed.
We have used both runsp_lapw -orb and runsp_c_lapw -orb.
I think that the problem is due to the fact that lapwdm -dn -c
is not executed, as one can see from the 'dayfile' and 'error message'
enclosed below. We have no problem for systems with inversion
symmetry or for LDA+U+SO calculations. I don't know runsp_lapw
and x_lapw well enough to modify it.

Could anyone modify runsp_lapw and x_lapw so that we can
do LDA+U calculations for systems without inversion symmetry
(no SO) in both serial and parallel executions?
Thank you very much in advance.

Regards,
Guang-Yu Guo





- ---------------- dayfile
- ------------------------------------------------------------------------
    start       (Sat Aug 17 16:17:44 CST 2002) with lapw0 (20/20 to go)
>   lapw0       (16:17:44) 48.210u 0.560s 0:50.68 96.2% 0+0k 0+0io 274pf+0w
>   lapw1  -c -up   -orb        (16:18:35) 1649.100u 20.790s 27:56.19 99.6%
0+0k 0+0io 390pf+0w
>   lapw2 -c -up        (16:46:32) 118.960u 7.450s 2:14.88 93.7%        0+0k 0+0
io 318pf+0w
>   lapw2 -c -dn        (16:48:47) 61.270u 3.420s 1:05.48 98.7% 0+0k 0+0io 316pf
+0w
>   lapwdm -up   -c     (16:49:53) 2.600u 0.870s 0:04.00 86.7%  0+0k 0+0io 233pf
+0w
>   lcore -up   (16:49:57) 0.580u 0.010s 0:00.71 83.0%  0+0k 0+0io 176pf+0w
>   lcore -dn   (16:49:58) 0.600u 0.000s 0:00.63 95.2%  0+0k 0+0io 176pf+0w
>   mixer       (16:49:59) 6.730u 0.450s 0:10.18 70.5%  0+0k 0+0io 201pf+0w
:ENERGY convergence:  0 0 1.2786595000000000
:CHARGE convergence:  0 0.00001 .5435234

- ------------------- error message
- ------------------------------------------------------------
 LAPW0 END
 LAPW1 END
 LAPW2 END
 LAPW2 END
 lapwdm END
total_exec: Command not found.
 CORE  END
 CORE  END
 MIXER END
in cycle 2    ETEST: 1.2786595000000000   CTEST: .5435234
 LAPW0 END
PGFIO-F-217/list-directed read/unit=9/attempt to read past end of file.
 File name = su-1ceco2-2sp+u.dmatdn    formatted, sequential access   record = 1
 In source file init.f, at line number 226
PGFIO-F-217/list-directed read/unit=10/attempt to read past end of file.
 File name = su-1ceco2-2sp+u.dmatdn    formatted, sequential access   record = 1
 In source file init.f, at line number 226
 LAPW1 END
 LAPW2 END
 LAPW2 END
 lapwdm END


- --
Dr. G.Y. Guo
Professor
Department of Physics
National Taiwan University
1 Roosevelt Road, Sec. 4
Taipei 106, Taiwan, R.O.C.
Tel. ++886-2-33665180
Fax. ++886-2-23639984
E-mail: gyguo@phys.ntu.edu.tw


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------------------------------

Date: Mon, 19 Aug 2002 18:26:28 +0800
From: gyguo <gyguo@phys.ntu.edu.tw>
Subject: [WIEN]: errors from lapwdm in parallel

====
gyguo <gyguo@phys.ntu.edu.tw>
submitted the following contribution:
====


Dear Prof. Blaha and WIEN users,

We found that lapwdm does not work in parallel,
as shown in the following error message.
We use a PC cluster with MPI and PGI compiler.
We did go into the SRC_lapwdm directory,
trying to solve the problem. However,
we cannot find the 'dmatscf.f' program.
Any help to solve the problem will be highly
appreciated.

Regards,

Guang-Yu Guo

- -------- error message ---------------------------------------
x lapwdm -so -up -p
running LAPWDM in parallel mode
[1] 17142
[2] 17157
[3] 17179
[4] 17184
[5] 17189
[6] 17195
[7] 17226

 lapwdm END

 lapwdm END
 lapwdm END
 lapwdm END
 lapwdm END
 lapwdm END
 lapwdm END
[7]    Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
[6]  - Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ... ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
[5]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
[4]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
[3]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
[2]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
[1]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
      node10 4.970u 0.370s 0:26.09 20.4% 0+0k 0+0io 235pf+0w
      node11 5.020u 0.390s 0:27.77 19.4% 0+0k 0+0io 234pf+0w
      node12 4.950u 0.400s 0:27.04 19.7% 0+0k 0+0io 235pf+0w
      node13 5.090u 0.280s 0:26.56 20.2% 0+0k 0+0io 235pf+0w
      node14 5.040u 0.320s 0:26.09 20.5% 0+0k 0+0io 235pf+0w
      node15 4.940u 0.320s 0:25.32 20.7% 0+0k 0+0io 235pf+0w
      node16 4.970u 0.330s 0:24.48 21.6% 0+0k 0+0io 235pf+0w
   Summary of lapwdmpara:
   node10        user=4.97       wallclock=26.09
   node11        user=5.02       wallclock=27.77
   node12        user=4.95       wallclock=27.04
   node13        user=5.09       wallclock=26.56
   node14        user=5.04       wallclock=26.09
   node15        user=4.94       wallclock=25.32
   node16        user=4.97       wallclock=24.48
PGFIO-F-231/formatted read/internal file/error on data conversion.
 In source file dmatscf.f, at line number 69
35.220u 2.680s 0:32.19 117.7%   0+0k 0+0io 26239pf+0w


- --
Dr. G.Y. Guo
Professor
Department of Physics
National Taiwan University
1 Roosevelt Road, Sec. 4
Taipei 106, Taiwan, R.O.C.
Tel. ++886-2-33665180
Fax. ++886-2-23639984
E-mail: gyguo@phys.ntu.edu.tw


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------------------------------

Date: Mon, 19 Aug 2002 14:39:38 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: LDA+U for systems without inversion symmetry

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> We have been trying to perform LDA+U calculations without SO
> for systems without inversion symmetry, and we have failed.
> We have used both runsp_lapw -orb and runsp_c_lapw -orb.
> I think that the problem is due to the fact that lapwdm -dn -c
> is not executed, as one can see from the 'dayfile' and 'error message'
> enclosed below. We have no problem for systems with inversion
> symmetry or for LDA+U+SO calculations. I don't know runsp_lapw
> and x_lapw well enough to modify it.
>
> Could anyone modify runsp_lapw and x_lapw so that we can
> do LDA+U calculations for systems without inversion symmetry
> (no SO) in both serial and parallel executions?

Please download the latest WIEN2k versions. These problems have been fixed
some time ago.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 19 Aug 2002 10:13:47 -0400
From: gpzhang <gpzhang@utk.edu>
Subject: [WIEN]: problem with band structure

====
gpzhang <gpzhang@utk.edu>
submitted the following contribution:
====

Dear Wien Users and Developers,


I thought that I know how to calculate the band structure with wien97,
but clearly not. I tried several different schemes but failed.  So, I
wonder whether you could help me.

I succeeded to calculate TiC and MgB2 band structures, but when I
tried to calculate the potassium vanadate, the band structure looks
messy, meaning that the lines do not form a clear continuous curve.  I
should note that my present compound has no inversion symmetry and
appears a little frustrated.

Here is what I did. I first created a special K-list and attached it
to *.in1c and changed the unit 4 to 5. I ran x lapw1 -c.  (By the way,
is there a way to run this in parallel? The code complains if I do x
lapw1 -c -p). After I finished it, I edited case.insp by inserting Ef
(from case.scf). Then do x spaghetti -c.

I got an error message like

`1525-097 A READ statement using decimal base input found the invalid
digit '.' in the input file.  The program will recover by assuming a
zero in its place.  STOP end OK 0.4u 0.1s 0:01 56% 36+314k 0+0io
21pf+0w RETURN key to continue ...'

In addition, I found that my case.qtl has zero bytes in it.

I can attach both case.klist and case.spaghetti_ps if necessary though both 
files are big.

Many thanks in advance!

Guoping



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------------------------------

Date: Mon, 19 Aug 2002 09:49:45 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: [WIEN]: bct-U

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_003A_01C24765.BF944730
Content-Type: text/plain;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

Dear all,
There was a discussion in the mailing-list some times ago about the =
bct-U (a=3Db=3D7.5 au, c=3D8.5 au). Since the problem was not closed =
clearly, I worked on it as my interesting subject and would like here to =
share the results to use your possibly expert comments. First, let's =
below paste the discussion to see/remember the problem:

">I tried exactly the same now (bct-U, a=3Db=3D7.5 au, c=3D8.5=20
> au, case.inm=3D0.1+BROYD, U=3D0.45 Ry, J=3D0.05 Ry) with the newest =
version. I used=20
> RKM=3D7 and 99 k-points in IBZ (not much, just to see whether it =
works). These=20
> cases converge both with and without -orb (in both cases -so is used). =
It=20
> takes many iterations however (>250). Are these results comparable =
with what=20
> you found :
>=20
> :HFF01 :MMI01 :EFG01
> -so -in1new 1 -283.949 2.64145 6.15215
> -so -in1new 1 -orb -39.481 0.00698 1.93274=20
Actually I get rather different results. I've attached scf files from =
the
three runs. Maybe you'll find the differences.
My calculations converge in just 20 cycles. I used only 18 k-points so
maybe it's because of k-mesh, but the differences seem to be to big.=20
I can only think of two things
1) Try not using the -in1new switch. The standard scheme should be ok =
for
a case like this.

2) Try changing your inst to=20
U=20
Rn 3 5=20
5, 3,3.0 N=20
5, 3,0.0 N=20
6, 2,0.5 N=20
6, 2,0.5 N=20
7,-1,1.0 N=20
7,-1,1.0 N
****=20
When you start from a configuration where only the f-electrons are spin
polarized sometimes improves convergence tremendiously."


So, you see the problem is to obtain different results by two individual =
expert persons. Comparing the above reported results of (:HFF01, :MMI01, =
:EFG01) Shows that there are also dramatic differences between the =
results before and after adding -orb switch, which is expectable after =
250 iterations. Here we believe that the role of -so is marginal for =
this problem. Hence, we go through the problem using the default =
parameters of wien2k_02 (updated 30-July-2002) and get the following =
self-consistent results:
1) runsp_lapw -orb -in1new 5 -cc 0.0001 -i 99 ; (:ITE37)=3D=3D>
:HFF01=3D-404.991,:MMI01=3D1.50924,:EFG01=3D3.38281.

2) runsp_c_lapw -orb -in1new 5 -cc 0.0001 -i 99 ; (:ITE24)=3D=3D>
:HFF01=3D0.000,:MMI01=3D0.00000,:EFG01=3D-7.62824.

3) runsp_c_lapw -orb -in1new 5 -cc 0.0001 -i 99 + above suggested =
case.inst;  (:ITE21)=3D=3D>
:HFF01=3D0.000,:MMI01=3D0.00001,:EFG01=3D-7.55947.

4) run_lapw -in1new 5 -cc 0.0001 -i 99 ; (:ITE13)=3D=3D>
:HFF01=3D---,:MMI01=3D---,:EFG01=3D3.26087.

5) runsp_lapw -in1new 5 -cc 0.0001 -i 99 ; (:ITE=3D13)=3D=3D>
:HFF01=3D-350.370,:MMI01=3D1.95919,:EFG01=3D+7.04996.

Now my questions are as follows:

1.Why the calculated EFG within step 1 (imposing magnetic) and 2 =
(forcing zero magnet) are not alike with identical initial conditions, =
same case.indmup&dn for each cases regarding the same EFG's within step1 =
and 4?

The later same EFG's (comparing 1 and 4) show that the EFG has not been =
substantially affected by -orb and sp (spin-polarization). But Steps 4 =
and 5 show the effect of sp! Step 2 and 3 show the suggestion about =
case.inst is not the case. From 2 and 4 we also see the effect of U =
parameter.
2.Why these counted evidences are not agree with each other?

Anyway, I am at least willing to inform that all my calculations are =
well converged in a few iterations in contrast to the 250 reported =
iterations: maybe due to the latest wien2k version. In addition such =
substantially different reported results with and without -orb are not =
observed.
Thank you for your attention in this respect,
Your,
S. Jalali.

- ------=_NextPart_000_003A_01C24765.BF944730
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
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<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT face=3DArial size=3D2>Dear all,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>There was a discussion in the =
mailing-list some=20
times ago about the bct-U (a=3Db=3D7.5 au, c=3D8.5 au). Since the =
problem was not=20
closed clearly, I worked on it as my interesting subject and would like =
here to=20
share the results to use your possibly expert comments. First, let's =
below paste=20
the discussion to see/remember the problem:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>"&gt;I tried exactly the same now =
(bct-U, a=3Db=3D7.5=20
au, c=3D8.5 <BR>&gt; au, case.inm=3D0.1+BROYD, U=3D0.45 Ry, J=3D0.05 Ry) =
with the newest=20
version. I used <BR>&gt; RKM=3D7 and 99 k-points in IBZ (not much, just =
to see=20
whether it works). These <BR>&gt; cases converge both with and without =
- -orb (in=20
both cases -so is used). It <BR>&gt; takes many iterations however =
(&gt;250).=20
Are these results comparable with what <BR>&gt; you found :<BR>&gt; =
<BR>&gt;=20
:HFF01 :MMI01 :EFG01<BR>&gt; -so -in1new 1 -283.949 2.64145 =
6.15215<BR>&gt; -so=20
- -in1new 1 -orb -39.481 0.00698 1.93274 <BR>Actually I get rather =
different=20
results. I've attached scf files from the<BR>three runs. Maybe you'll =
find the=20
differences.<BR>My calculations converge in just 20 cycles. I used only =
18=20
k-points so<BR>maybe it's because of k-mesh, but the differences seem to =
be to=20
big. <BR>I can only think of two things<BR>1) Try not using the -in1new =
switch.=20
The standard scheme should be ok for<BR>a case like this.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>2) Try changing your inst to <BR>U =
<BR>Rn 3 5=20
<BR>5, 3,3.0 N <BR>5, 3,0.0 N <BR>6, 2,0.5 N <BR>6, 2,0.5 N <BR>7,-1,1.0 =
N=20
<BR>7,-1,1.0 N<BR>**** <BR>When you start from a configuration where =
only the=20
f-electrons are spin<BR>polarized sometimes improves convergence=20
tremendiously."</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV><FONT face=3DArial =
size=3D2>
<DIV><BR>So, you see the problem is to obtain different results by two=20
individual expert persons. Comparing the above reported results of =
(:HFF01,=20
:MMI01, :EFG01) Shows that there are also dramatic differences between =
the=20
results before and after adding -orb switch, which is expectable after =
250=20
iterations. Here we believe that the role of -so is marginal for this =
problem.=20
Hence, we go through the problem using the default parameters of =
wien2k_02=20
(updated 30-July-2002) and get the following self-consistent =
results:<BR>1)=20
runsp_lapw -orb -in1new 5 -cc 0.0001 -i 99 ;=20
(:ITE37)=3D=3D&gt;<BR>:HFF01=3D-404.991,:MMI01=3D1.50924,:EFG01=3D3.38281=
.</DIV>
<DIV>&nbsp;</DIV>
<DIV>2) runsp_c_lapw -orb -in1new 5 -cc 0.0001 -i 99 ;=20
(:ITE24)=3D=3D&gt;<BR>:HFF01=3D0.000,:MMI01=3D0.00000,:EFG01=3D-7.62824.<=
/DIV>
<DIV>&nbsp;</DIV>
<DIV>3) runsp_c_lapw -orb -in1new 5 -cc 0.0001 -i 99 + above suggested=20
case.inst;&nbsp;=20
(:ITE21)=3D=3D&gt;<BR>:HFF01=3D0.000,:MMI01=3D0.00001,:EFG01=3D-7.55947.<=
/DIV>
<DIV>&nbsp;</DIV>
<DIV>4) run_lapw -in1new 5 -cc 0.0001 -i 99 ;=20
(:ITE13)=3D=3D&gt;<BR>:HFF01=3D---,:MMI01=3D---,:EFG01=3D3.26087.</DIV>
<DIV>&nbsp;</DIV>
<DIV>5) runsp_lapw -in1new 5 -cc 0.0001 -i 99 ;=20
(:ITE=3D13)=3D=3D&gt;<BR>:HFF01=3D-350.370,:MMI01=3D1.95919,:EFG01=3D+7.0=
4996.</DIV>
<DIV>&nbsp;</DIV>
<DIV>Now my questions are as follows:</DIV>
<DIV>&nbsp;</DIV>
<DIV>1.Why the calculated EFG within step&nbsp;1 (imposing magnetic) =
and&nbsp;2=20
(forcing zero magnet) are&nbsp;not alike with identical initial =
conditions,=20
same&nbsp;case.indmup&amp;dn for each cases regarding the same EFG's =
within=20
step1 and 4?</DIV>
<DIV>&nbsp;</DIV>
<DIV>The later same EFG's (comparing 1 and 4) show that the EFG has=20
not&nbsp;been substantially affected by -orb and sp (spin-polarization). =
But=20
Steps 4 and 5 show the effect of sp! Step 2 and 3 show the =
suggestion&nbsp;about=20
case.inst is not the case. From 2 and 4 we also see the effect of U=20
parameter.</DIV>
<DIV>2.Why these counted evidences are not agree with each other?</DIV>
<DIV>&nbsp;</DIV>
<DIV>Anyway, I am at least willing to inform that all my calculations =
are well=20
converged&nbsp;in a few iterations in contrast to the 250 reported =
iterations:=20
maybe due to the latest wien2k version. In addition =
such&nbsp;substantially=20
different&nbsp;reported results with and without -orb are not =
observed.</DIV>
<DIV>Thank you for your attention in this respect,</DIV>
<DIV>Your,</DIV>
<DIV>S. Jalali.</FONT></DIV></BODY></HTML>

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Date: Tue, 20 Aug 2002 10:32:58 +0800 (CST)
From: yshzhang@theory.issp.ac.cn
Subject: [WIEN]: Coulomb interaction strengths

====
yshzhang@theory.issp.ac.cn
submitted the following contribution:
====

Dear all

Did anyone know how to calculate the nearest-neighbour Coulomb interaction 
strengths between different orbitals ?

- -- 
Best Regards
YS Zhang

- ------------------------------------------------------------------------
 Address: Institute of Solid State Physics
          Chinese Academy of Sciences
          P.O.BOX 1129,230031 Hefei 
          P.R~China
 Tel:     086-551-5591464(Office)
          086-551-5592837(Home)
 Fax:     086-551-5591434
 WWW:     http://theory.issp.ac.cn/~yshzhang
- ------------------------------------------------------------------------


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Date: Tue, 20 Aug 2002 10:24:00 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: The problem in band character plot

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I tried TiC Bandstructure (with band character) as routine manner.
> (Generate k-list, edit tic.in1, lapw1 -up, edit tic.in2, and
> lapw2 -up -qtl.)
>
> When I start lapw2 with -up spin option, the program seems to search
> opposite down spin (tic.energydn) file. (see below)

Of course it does! You must not use the   -up    switch.

I suppose you tried TiC (as in the manual) WITHOUT spinpolarization, i.e.
using    run_lapw

Why would you then use   x lapw1/2 -up   ???
The -up switch is just for spinpolarized cases, but this requires that
you also run a spinpolarized scf cycle (runsp_lapw).

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
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Date: Tue, 20 Aug 2002 14:05:00 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: single vs. double cells

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> 	I am investigating a AFM compound and therefore have to double my
> unit cell.  In the compound I am looking at the single cell is the cubic
> space group #221 (Pm-3m).  This is a peroskite structure and the afm order
> is along the (111) axis and therefore I end up with a rhombohedral cell
> which is space group #166 (R-3m).  The problem is that if I calculate the
> ferromagnetic solution in the doubled cell, my energy doesn't look
> anything like that of double the single cell energy.  In fact, there is an
> approximately 30 Ryd difference!!

Hi!

I guess you own me a beer should we ever meet at a conference!!!!!

It took me 3 hours to find out that your atttched struct file had a Ga-Z
of 31.1 instead of 31.0 and then of course the total energies are off by
30 Ry.

PS: You also had different RMT values, but this does not account for 30 Ry.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Tue, 20 Aug 2002 14:20:42 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: bct-U

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> There was a discussion in the mailing-list some times ago about the bct-U

The inital reason for the problem with U (AND spin-orbit!!) was that a
filename with just ONE character (like u.struct) lead to a problem with
the normalization of the SO-charge density. This also explains why different
tests lead to different results (all doing bct-U, but some called the
directory just u, others bctu).

The problem was in lapw2, but this has been fixed in the latest version.


> 1) runsp_lapw -orb -in1new 5 -cc 0.0001 -i 99 ; (:ITE37)==>
> :HFF01=-404.991,:MMI01=1.50924,:EFG01=3.38281.
>
> 2) runsp_c_lapw -orb -in1new 5 -cc 0.0001 -i 99 ; (:ITE24)==>
> :HFF01=0.000,:MMI01=0.00000,:EFG01=-7.62824.
>
> 3) runsp_c_lapw -orb -in1new 5 -cc 0.0001 -i 99 + above suggested case.inst;  (:ITE21)==>
> :HFF01=0.000,:MMI01=0.00001,:EFG01=-7.55947.
>
> 4) run_lapw -in1new 5 -cc 0.0001 -i 99 ; (:ITE13)==>
> :HFF01=---,:MMI01=---,:EFG01=3.26087.
>
> 5) runsp_lapw -in1new 5 -cc 0.0001 -i 99 ; (:ITE=13)==>
> :HFF01=-350.370,:MMI01=1.95919,:EFG01=+7.04996.
>
> 1.Why the calculated EFG within step 1 (imposing magnetic) and 2 (forcing zero magnet) are not alike with identical initial conditions, same case.indmup&dn for each cases regarding the same EFG's within step1 and 4?

Why should it be ??? Agreement between 1 and 4 is just accidental and not
perfect either. Similar (but not identical) EFGs do not mean that all the
results are identical under all circumstances.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Tue, 20 Aug 2002 15:13:03 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: problem with band structure

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Here is what I did. I first created a special K-list and attached it
> to *.in1c and changed the unit 4 to 5. I ran x lapw1 -c.  (By the way,
> is there a way to run this in parallel? The code complains if I do x
> lapw1 -c -p).

I guess the code also tells you, that you can run in parallel only with a
klist from unit 4, not 5 !!! You could insert the special k-mesh into
case.klist, leave unit=4 and run x lapw1 -p -c
Then concatenate all output1_x files into one single file.

> After I finished it, I edited case.insp by inserting Ef
> (from case.scf). Then do x spaghetti -c.

You should not use the -c
PS: If the options are not clear, always use:   x spaghetti -h
It tells you all allowed options for this program.

> `1525-097 A READ statement using decimal base input found the invalid
> digit '.' in the input file.  The program will recover by assuming a
> zero in its place.  STOP end OK 0.4u 0.1s 0:01 56% 36+314k 0+0io
> 21pf+0w RETURN key to continue ...'

I suggest to remove case.insp and recreate it from the template.

> In addition, I found that my case.qtl has zero bytes in it.

This should be ok, since you did not x lapw2 -qtl -c   (and you don't need
it unless you want a "character-plot").

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
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Date: Tue, 20 Aug 2002 07:56:09 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: Coulomb interaction strengths

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

You first want to define orbitals - in LAPW it's
hardly possible.

In LMTO-TB, where orbitals are well defined, this was
addressed about 15 years ago by Pawlowska (sp?) and
Andersen.

Igor
- --- yshzhang@theory.issp.ac.cn wrote:
> ====
> yshzhang@theory.issp.ac.cn
> submitted the following contribution:
> ====
> 
> Dear all
> 
> Did anyone know how to calculate the
> nearest-neighbour Coulomb interaction 
> strengths between different orbitals ?
> 
> -- 
> Best Regards
> YS Zhang
> 
>
- ------------------------------------------------------------------------
>  Address: Institute of Solid State Physics
>           Chinese Academy of Sciences
>           P.O.BOX 1129,230031 Hefei 
>           P.R~China
>  Tel:     086-551-5591464(Office)
>           086-551-5592837(Home)
>  Fax:     086-551-5591434
>  WWW:     http://theory.issp.ac.cn/~yshzhang
>
- ------------------------------------------------------------------------
> 
> 
> ====
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=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

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Date: Tue, 20 Aug 2002 08:23:53 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: Two questions

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

Hi Pavel,

It depends on waht kind of similarity do you seek:
say, in the elastic properties (equilibrium lattice
structure, phonons), magnetic properties, excitations.
The physics is different in all cases. For instance,
re magnetism, I can making the following predictions
(I honestly never tried this):

1) Since Stoner I is larger in GGA, and DFT+U has
additional I prop to (U-J), to keep the same magnetic
moment in GGA+U as in LDA+U you need to decreas U *or*
increase J (the latter makes more sense). Needed
changes are smaller in the FLL (SIC) than in the AMF.
2) The UHB-LHB splitting is defined by U-J, but in an
AFM Mott insulator like NiO part of the splitting
comes from I, so again similar changes are need to
reproduce the same splitting in GGA+U as in LDA+U.
3) I still fail to see any reasin why DC is more
questionable in GGA than in LDA. I disagree with both
your asessments: that GGA includes more [Hubbard]
correlations than LDA, and, even if it did, that DC
procedure would have been in any sense more
questionable because of that.

Best,
Igor
- --- Pavel Novak <novakp@fzu.cz> wrote:
> ====
> Pavel Novak <novakp@fzu.cz>
> submitted the following contribution:
> ====
> 
> Dear Saeid and Igor,
> 
> from our experience follows that GGA contains more
> correlation than LDA.
> As a consequence using GGA+U (U=UGGA) would give, as
> a rule, similar
> results as LDA+U (U=ULDA) for UGGA<ULDA. Because of
> the double counting
> term GGA+U is more questionable than LDA+U. To my
> knowledge the only GGA+U
> paper is by Savrasov and Kotliar: PRL 84, 3670
> (2000). Note that these
> authors use the original (Anisimov 1991) approach
> denoted as LDA+U(MFH) in
> WIEN2k.
> 
> Regards
> Pavel Novak
> 

=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

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Date: Tue, 20 Aug 2002 17:35:25 +0200
From: Thomas Claesson <tcl@kth.se>
Subject: Re: [WIEN]: Two questions

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien developers and users!

Thanks for your advice, Igor! I followed your instructions below and 
found out that starting from a converged case run without -orb the 
following happend when I made one extra iteration with -orb added 
(U=0.0001, J=0.0001). The Fermi energy changed from 0.41860 Ry to 
0.62029 and the total energy from -6387.862958 to -6384.289129. The 
changes in the bandstructure plot were also quite drastic, so I am still 
a bit puzzled about what is going on.

Perhaps I should add that I have not used too many k-points, 600 in 
whole BZ, 65 in IBZ, RKmax=7.0.

I would really appreciate it if some could explain to me what happens here.

Best regards,
Thomas Claesson

Igor Mazin wrote:

>>
>Case.scf has Fermi energy in it, from iteration to
>iteration. Make several iterations with U=0.0001 and
>J=0.0001 and then one without -orb. If you are
>converged, nothing should change, including Fermi.
>
>If this is so, but your bands are plotted with an
>incorrect Ef, you will know were to look then.
>
>Igor
>

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Date: Tue, 20 Aug 2002 09:05:49 -0700 (PDT)
From: Michelle Johannes <johannes@maugre.ucdavis.edu>
Subject: Re: [WIEN]: single vs. double cells

====
Michelle Johannes <johannes@maugre.ucdavis.edu>
submitted the following contribution:
====

Peter-
	Wow, I'm really sorry about that.  I have no idea why my z would
have been increased so I never even checked it.  I ran this calculation
quite a few times to make sure the problem wasn't something spurious but I
never thought to remake the .struct file from scratch.  If its any
consolation, I am very, very happy to have the answer.

	Michelle


On Tue, 20 Aug 2002, Peter Blaha wrote:

> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> > 	I am investigating a AFM compound and therefore have to double my
> > unit cell.  In the compound I am looking at the single cell is the cubic
> > space group #221 (Pm-3m).  This is a peroskite structure and the afm order
> > is along the (111) axis and therefore I end up with a rhombohedral cell
> > which is space group #166 (R-3m).  The problem is that if I calculate the
> > ferromagnetic solution in the doubled cell, my energy doesn't look
> > anything like that of double the single cell energy.  In fact, there is an
> > approximately 30 Ryd difference!!
> 
> Hi!
> 
> I guess you own me a beer should we ever meet at a conference!!!!!
> 
> It took me 3 hours to find out that your atttched struct file had a Ga-Z
> of 31.1 instead of 31.0 and then of course the total energies are off by
> 30 Ry.
> 
> PS: You also had different RMT values, but this does not account for 30 Ry.
> 
> Regards
> 
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
> 
> ====
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> To (un)subscribe send mail to
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------------------------------

Date: Mon, 19 Aug 2002 17:01:05 +0800
From: gyguo <gyguo@phys.ntu.edu.tw>
Subject: [WIEN]: LDA+U for systems without inversion symmetry

====
gyguo <gyguo@phys.ntu.edu.tw>
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====

====
gyguo <gyguo@phys.ntu.edu.tw>
submitted the following contribution:
====


Dear Prof. Blaha and WIEN users,

We have been trying to perform LDA+U calculations without SO
for systems without inversion symmetry, and we have failed.
We have used both runsp_lapw -orb and runsp_c_lapw -orb.
I think that the problem is due to the fact that lapwdm -dn -c
is not executed, as one can see from the 'dayfile' and 'error message'
enclosed below. We have no problem for systems with inversion
symmetry or for LDA+U+SO calculations. I don't know runsp_lapw
and x_lapw well enough to modify it.

Could anyone modify runsp_lapw and x_lapw so that we can
do LDA+U calculations for systems without inversion symmetry
(no SO) in both serial and parallel executions?
Thank you very much in advance.

Regards,
Guang-Yu Guo





- ---------------- dayfile
- ------------------------------------------------------------------------
    start       (Sat Aug 17 16:17:44 CST 2002) with lapw0 (20/20 to go)
>   lapw0       (16:17:44) 48.210u 0.560s 0:50.68 96.2% 0+0k 0+0io 274pf+0w
>   lapw1  -c -up   -orb        (16:18:35) 1649.100u 20.790s 27:56.19 99.6%
0+0k 0+0io 390pf+0w
>   lapw2 -c -up        (16:46:32) 118.960u 7.450s 2:14.88 93.7%        0+0k 0+0
io 318pf+0w
>   lapw2 -c -dn        (16:48:47) 61.270u 3.420s 1:05.48 98.7% 0+0k 0+0io 316pf
+0w
>   lapwdm -up   -c     (16:49:53) 2.600u 0.870s 0:04.00 86.7%  0+0k 0+0io 233pf
+0w
>   lcore -up   (16:49:57) 0.580u 0.010s 0:00.71 83.0%  0+0k 0+0io 176pf+0w
>   lcore -dn   (16:49:58) 0.600u 0.000s 0:00.63 95.2%  0+0k 0+0io 176pf+0w
>   mixer       (16:49:59) 6.730u 0.450s 0:10.18 70.5%  0+0k 0+0io 201pf+0w
:ENERGY convergence:  0 0 1.2786595000000000
:CHARGE convergence:  0 0.00001 .5435234

- ------------------- error message
- ------------------------------------------------------------
 LAPW0 END
 LAPW1 END
 LAPW2 END
 LAPW2 END
 lapwdm END
total_exec: Command not found.
 CORE  END
 CORE  END
 MIXER END
in cycle 2    ETEST: 1.2786595000000000   CTEST: .5435234
 LAPW0 END
PGFIO-F-217/list-directed read/unit=9/attempt to read past end of file.
 File name = su-1ceco2-2sp+u.dmatdn    formatted, sequential access   record = 1
 In source file init.f, at line number 226
PGFIO-F-217/list-directed read/unit=10/attempt to read past end of file.
 File name = su-1ceco2-2sp+u.dmatdn    formatted, sequential access   record = 1
 In source file init.f, at line number 226
 LAPW1 END
 LAPW2 END
 LAPW2 END
 lapwdm END


- --
Dr. G.Y. Guo
Professor
Department of Physics
National Taiwan University
1 Roosevelt Road, Sec. 4
Taipei 106, Taiwan, R.O.C.
Tel. ++886-2-33665180
Fax. ++886-2-23639984
E-mail: gyguo@phys.ntu.edu.tw


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------------------------------

Date: Tue, 20 Aug 2002 14:05:00 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: single vs. double cells

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
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====

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> 	I am investigating a AFM compound and therefore have to double my
> unit cell.  In the compound I am looking at the single cell is the cubic
> space group #221 (Pm-3m).  This is a peroskite structure and the afm order
> is along the (111) axis and therefore I end up with a rhombohedral cell
> which is space group #166 (R-3m).  The problem is that if I calculate the
> ferromagnetic solution in the doubled cell, my energy doesn't look
> anything like that of double the single cell energy.  In fact, there is an
> approximately 30 Ryd difference!!

Hi!

I guess you own me a beer should we ever meet at a conference!!!!!

It took me 3 hours to find out that your atttched struct file had a Ga-Z
of 31.1 instead of 31.0 and then of course the total energies are off by
30 Ry.

PS: You also had different RMT values, but this does not account for 30 Ry.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 20 Aug 2002 10:32:58 +0800 (CST)
From: yshzhang@theory.issp.ac.cn
Subject: [WIEN]: Coulomb interaction strengths

====
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====

====
yshzhang@theory.issp.ac.cn
submitted the following contribution:
====

Dear all

Did anyone know how to calculate the nearest-neighbour Coulomb interaction 
strengths between different orbitals ?

- -- 
Best Regards
YS Zhang

- ------------------------------------------------------------------------
 Address: Institute of Solid State Physics
          Chinese Academy of Sciences
          P.O.BOX 1129,230031 Hefei 
          P.R~China
 Tel:     086-551-5591464(Office)
          086-551-5592837(Home)
 Fax:     086-551-5591434
 WWW:     http://theory.issp.ac.cn/~yshzhang
- ------------------------------------------------------------------------


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------------------------------

Date: Tue, 20 Aug 2002 17:35:25 +0200
From: Thomas Claesson <tcl@kth.se>
Subject: Re: [WIEN]: Two questions

====
Thomas Claesson <tcl@kth.se>
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====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien developers and users!

Thanks for your advice, Igor! I followed your instructions below and 
found out that starting from a converged case run without -orb the 
following happend when I made one extra iteration with -orb added 
(U=0.0001, J=0.0001). The Fermi energy changed from 0.41860 Ry to 
0.62029 and the total energy from -6387.862958 to -6384.289129. The 
changes in the bandstructure plot were also quite drastic, so I am still 
a bit puzzled about what is going on.

Perhaps I should add that I have not used too many k-points, 600 in 
whole BZ, 65 in IBZ, RKmax=7.0.

I would really appreciate it if some could explain to me what happens here.

Best regards,
Thomas Claesson

Igor Mazin wrote:

>>
>Case.scf has Fermi energy in it, from iteration to
>iteration. Make several iterations with U=0.0001 and
>J=0.0001 and then one without -orb. If you are
>converged, nothing should change, including Fermi.
>
>If this is so, but your bands are plotted with an
>incorrect Ef, you will know were to look then.
>
>Igor
>

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------------------------------

Date: Mon, 19 Aug 2002 14:39:38 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: LDA+U for systems without inversion symmetry

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> We have been trying to perform LDA+U calculations without SO
> for systems without inversion symmetry, and we have failed.
> We have used both runsp_lapw -orb and runsp_c_lapw -orb.
> I think that the problem is due to the fact that lapwdm -dn -c
> is not executed, as one can see from the 'dayfile' and 'error message'
> enclosed below. We have no problem for systems with inversion
> symmetry or for LDA+U+SO calculations. I don't know runsp_lapw
> and x_lapw well enough to modify it.
>
> Could anyone modify runsp_lapw and x_lapw so that we can
> do LDA+U calculations for systems without inversion symmetry
> (no SO) in both serial and parallel executions?

Please download the latest WIEN2k versions. These problems have been fixed
some time ago.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 20 Aug 2002 10:24:00 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: The problem in band character plot

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I tried TiC Bandstructure (with band character) as routine manner.
> (Generate k-list, edit tic.in1, lapw1 -up, edit tic.in2, and
> lapw2 -up -qtl.)
>
> When I start lapw2 with -up spin option, the program seems to search
> opposite down spin (tic.energydn) file. (see below)

Of course it does! You must not use the   -up    switch.

I suppose you tried TiC (as in the manual) WITHOUT spinpolarization, i.e.
using    run_lapw

Why would you then use   x lapw1/2 -up   ???
The -up switch is just for spinpolarized cases, but this requires that
you also run a spinpolarized scf cycle (runsp_lapw).

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 19 Aug 2002 10:13:47 -0400
From: gpzhang <gpzhang@utk.edu>
Subject: [WIEN]: problem with band structure

====
gpzhang <gpzhang@utk.edu>
submitted the following contribution:
====

====
gpzhang <gpzhang@utk.edu>
submitted the following contribution:
====

Dear Wien Users and Developers,


I thought that I know how to calculate the band structure with wien97,
but clearly not. I tried several different schemes but failed.  So, I
wonder whether you could help me.

I succeeded to calculate TiC and MgB2 band structures, but when I
tried to calculate the potassium vanadate, the band structure looks
messy, meaning that the lines do not form a clear continuous curve.  I
should note that my present compound has no inversion symmetry and
appears a little frustrated.

Here is what I did. I first created a special K-list and attached it
to *.in1c and changed the unit 4 to 5. I ran x lapw1 -c.  (By the way,
is there a way to run this in parallel? The code complains if I do x
lapw1 -c -p). After I finished it, I edited case.insp by inserting Ef
(from case.scf). Then do x spaghetti -c.

I got an error message like

`1525-097 A READ statement using decimal base input found the invalid
digit '.' in the input file.  The program will recover by assuming a
zero in its place.  STOP end OK 0.4u 0.1s 0:01 56% 36+314k 0+0io
21pf+0w RETURN key to continue ...'

In addition, I found that my case.qtl has zero bytes in it.

I can attach both case.klist and case.spaghetti_ps if necessary though both 
files are big.

Many thanks in advance!

Guoping



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Date: Tue, 20 Aug 2002 13:25:46 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: Two questions

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

If you are puzzled a bit, I am puzzled entirely.
Fortunately Peter is back; after the magic with which
he fished out the wrong Z in Michelle's case, I start
to believe in his omnipotency.

I have no clue of how what you describe may be
possible. My last lame suggestion: I assume you had
deleted all vorb files before doing this experiment.
If you hadn't, you should. And BTW repeat -orb
itereation twice, to produce new vorbs.

> drastic, so I am still 
> a bit puzzled about what is going on.

=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

__________________________________________________
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Date: Tue, 20 Aug 2002 15:13:03 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: problem with band structure

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Here is what I did. I first created a special K-list and attached it
> to *.in1c and changed the unit 4 to 5. I ran x lapw1 -c.  (By the way,
> is there a way to run this in parallel? The code complains if I do x
> lapw1 -c -p).

I guess the code also tells you, that you can run in parallel only with a
klist from unit 4, not 5 !!! You could insert the special k-mesh into
case.klist, leave unit=4 and run x lapw1 -p -c
Then concatenate all output1_x files into one single file.

> After I finished it, I edited case.insp by inserting Ef
> (from case.scf). Then do x spaghetti -c.

You should not use the -c
PS: If the options are not clear, always use:   x spaghetti -h
It tells you all allowed options for this program.

> `1525-097 A READ statement using decimal base input found the invalid
> digit '.' in the input file.  The program will recover by assuming a
> zero in its place.  STOP end OK 0.4u 0.1s 0:01 56% 36+314k 0+0io
> 21pf+0w RETURN key to continue ...'

I suggest to remove case.insp and recreate it from the template.

> In addition, I found that my case.qtl has zero bytes in it.

This should be ok, since you did not x lapw2 -qtl -c   (and you don't need
it unless you want a "character-plot").

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 19 Aug 2002 09:49:45 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: [WIEN]: bct-U

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

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Dear all,
There was a discussion in the mailing-list some times ago about the =
bct-U (a=3Db=3D7.5 au, c=3D8.5 au). Since the problem was not closed =
clearly, I worked on it as my interesting subject and would like here to =
share the results to use your possibly expert comments. First, let's =
below paste the discussion to see/remember the problem:

">I tried exactly the same now (bct-U, a=3Db=3D7.5 au, c=3D8.5=20
> au, case.inm=3D0.1+BROYD, U=3D0.45 Ry, J=3D0.05 Ry) with the newest =
version. I used=20
> RKM=3D7 and 99 k-points in IBZ (not much, just to see whether it =
works). These=20
> cases converge both with and without -orb (in both cases -so is used). =
It=20
> takes many iterations however (>250). Are these results comparable =
with what=20
> you found :
>=20
> :HFF01 :MMI01 :EFG01
> -so -in1new 1 -283.949 2.64145 6.15215
> -so -in1new 1 -orb -39.481 0.00698 1.93274=20
Actually I get rather different results. I've attached scf files from =
the
three runs. Maybe you'll find the differences.
My calculations converge in just 20 cycles. I used only 18 k-points so
maybe it's because of k-mesh, but the differences seem to be to big.=20
I can only think of two things
1) Try not using the -in1new switch. The standard scheme should be ok =
for
a case like this.

2) Try changing your inst to=20
U=20
Rn 3 5=20
5, 3,3.0 N=20
5, 3,0.0 N=20
6, 2,0.5 N=20
6, 2,0.5 N=20
7,-1,1.0 N=20
7,-1,1.0 N
****=20
When you start from a configuration where only the f-electrons are spin
polarized sometimes improves convergence tremendiously."


So, you see the problem is to obtain different results by two individual =
expert persons. Comparing the above reported results of (:HFF01, :MMI01, =
:EFG01) Shows that there are also dramatic differences between the =
results before and after adding -orb switch, which is expectable after =
250 iterations. Here we believe that the role of -so is marginal for =
this problem. Hence, we go through the problem using the default =
parameters of wien2k_02 (updated 30-July-2002) and get the following =
self-consistent results:
1) runsp_lapw -orb -in1new 5 -cc 0.0001 -i 99 ; (:ITE37)=3D=3D>
:HFF01=3D-404.991,:MMI01=3D1.50924,:EFG01=3D3.38281.

2) runsp_c_lapw -orb -in1new 5 -cc 0.0001 -i 99 ; (:ITE24)=3D=3D>
:HFF01=3D0.000,:MMI01=3D0.00000,:EFG01=3D-7.62824.

3) runsp_c_lapw -orb -in1new 5 -cc 0.0001 -i 99 + above suggested =
case.inst;  (:ITE21)=3D=3D>
:HFF01=3D0.000,:MMI01=3D0.00001,:EFG01=3D-7.55947.

4) run_lapw -in1new 5 -cc 0.0001 -i 99 ; (:ITE13)=3D=3D>
:HFF01=3D---,:MMI01=3D---,:EFG01=3D3.26087.

5) runsp_lapw -in1new 5 -cc 0.0001 -i 99 ; (:ITE=3D13)=3D=3D>
:HFF01=3D-350.370,:MMI01=3D1.95919,:EFG01=3D+7.04996.

Now my questions are as follows:

1.Why the calculated EFG within step 1 (imposing magnetic) and 2 =
(forcing zero magnet) are not alike with identical initial conditions, =
same case.indmup&dn for each cases regarding the same EFG's within step1 =
and 4?

The later same EFG's (comparing 1 and 4) show that the EFG has not been =
substantially affected by -orb and sp (spin-polarization). But Steps 4 =
and 5 show the effect of sp! Step 2 and 3 show the suggestion about =
case.inst is not the case. From 2 and 4 we also see the effect of U =
parameter.
2.Why these counted evidences are not agree with each other?

Anyway, I am at least willing to inform that all my calculations are =
well converged in a few iterations in contrast to the 250 reported =
iterations: maybe due to the latest wien2k version. In addition such =
substantially different reported results with and without -orb are not =
observed.
Thank you for your attention in this respect,
Your,
S. Jalali.

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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT face=3DArial size=3D2>Dear all,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>There was a discussion in the =
mailing-list some=20
times ago about the bct-U (a=3Db=3D7.5 au, c=3D8.5 au). Since the =
problem was not=20
closed clearly, I worked on it as my interesting subject and would like =
here to=20
share the results to use your possibly expert comments. First, let's =
below paste=20
the discussion to see/remember the problem:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>"&gt;I tried exactly the same now =
(bct-U, a=3Db=3D7.5=20
au, c=3D8.5 <BR>&gt; au, case.inm=3D0.1+BROYD, U=3D0.45 Ry, J=3D0.05 Ry) =
with the newest=20
version. I used <BR>&gt; RKM=3D7 and 99 k-points in IBZ (not much, just =
to see=20
whether it works). These <BR>&gt; cases converge both with and without =
- -orb (in=20
both cases -so is used). It <BR>&gt; takes many iterations however =
(&gt;250).=20
Are these results comparable with what <BR>&gt; you found :<BR>&gt; =
<BR>&gt;=20
:HFF01 :MMI01 :EFG01<BR>&gt; -so -in1new 1 -283.949 2.64145 =
6.15215<BR>&gt; -so=20
- -in1new 1 -orb -39.481 0.00698 1.93274 <BR>Actually I get rather =
different=20
results. I've attached scf files from the<BR>three runs. Maybe you'll =
find the=20
differences.<BR>My calculations converge in just 20 cycles. I used only =
18=20
k-points so<BR>maybe it's because of k-mesh, but the differences seem to =
be to=20
big. <BR>I can only think of two things<BR>1) Try not using the -in1new =
switch.=20
The standard scheme should be ok for<BR>a case like this.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>2) Try changing your inst to <BR>U =
<BR>Rn 3 5=20
<BR>5, 3,3.0 N <BR>5, 3,0.0 N <BR>6, 2,0.5 N <BR>6, 2,0.5 N <BR>7,-1,1.0 =
N=20
<BR>7,-1,1.0 N<BR>**** <BR>When you start from a configuration where =
only the=20
f-electrons are spin<BR>polarized sometimes improves convergence=20
tremendiously."</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV><FONT face=3DArial =
size=3D2>
<DIV><BR>So, you see the problem is to obtain different results by two=20
individual expert persons. Comparing the above reported results of =
(:HFF01,=20
:MMI01, :EFG01) Shows that there are also dramatic differences between =
the=20
results before and after adding -orb switch, which is expectable after =
250=20
iterations. Here we believe that the role of -so is marginal for this =
problem.=20
Hence, we go through the problem using the default parameters of =
wien2k_02=20
(updated 30-July-2002) and get the following self-consistent =
results:<BR>1)=20
runsp_lapw -orb -in1new 5 -cc 0.0001 -i 99 ;=20
(:ITE37)=3D=3D&gt;<BR>:HFF01=3D-404.991,:MMI01=3D1.50924,:EFG01=3D3.38281=
</DIV>
<DIV>&nbsp;</DIV>
<DIV>2) runsp_c_lapw -orb -in1new 5 -cc 0.0001 -i 99 ;=20
(:ITE24)=3D=3D&gt;<BR>:HFF01=3D0.000,:MMI01=3D0.00000,:EFG01=3D-7.62824.<=
/DIV>
<DIV>&nbsp;</DIV>
<DIV>3) runsp_c_lapw -orb -in1new 5 -cc 0.0001 -i 99 + above suggested=20
case.inst;&nbsp;=20
(:ITE21)=3D=3D&gt;<BR>:HFF01=3D0.000,:MMI01=3D0.00001,:EFG01=3D-7.55947.<=
/DIV>
<DIV>&nbsp;</DIV>
<DIV>4) run_lapw -in1new 5 -cc 0.0001 -i 99 ;=20
(:ITE13)=3D=3D&gt;<BR>:HFF01=3D---,:MMI01=3D---,:EFG01=3D3.26087.</DIV>
<DIV>&nbsp;</DIV>
<DIV>5) runsp_lapw -in1new 5 -cc 0.0001 -i 99 ;=20
(:ITE=3D13)=3D=3D&gt;<BR>:HFF01=3D-350.370,:MMI01=3D1.95919,:EFG01=3D+7.0=
4996.</DIV>
<DIV>&nbsp;</DIV>
<DIV>Now my questions are as follows:</DIV>
<DIV>&nbsp;</DIV>
<DIV>1.Why the calculated EFG within step&nbsp;1 (imposing magnetic) =
and&nbsp;2=20
(forcing zero magnet) are&nbsp;not alike with identical initial =
conditions,=20
same&nbsp;case.indmup&amp;dn for each cases regarding the same EFG's =
within=20
step1 and 4?</DIV>
<DIV>&nbsp;</DIV>
<DIV>The later same EFG's (comparing 1 and 4) show that the EFG has=20
not&nbsp;been substantially affected by -orb and sp (spin-polarization). =
But=20
Steps 4 and 5 show the effect of sp! Step 2 and 3 show the =
suggestion&nbsp;about=20
case.inst is not the case. From 2 and 4 we also see the effect of U=20
parameter.</DIV>
<DIV>2.Why these counted evidences are not agree with each other?</DIV>
<DIV>&nbsp;</DIV>
<DIV>Anyway, I am at least willing to inform that all my calculations =
are well=20
converged&nbsp;in a few iterations in contrast to the 250 reported =
iterations:=20
maybe due to the latest wien2k version. In addition =
such&nbsp;substantially=20
different&nbsp;reported results with and without -orb are not =
observed.</DIV>
<DIV>Thank you for your attention in this respect,</DIV>
<DIV>Your,</DIV>
<DIV>S. Jalali.</FONT></DIV></BODY></HTML>

- ------=_NextPart_000_003A_01C24765.BF944730--

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Date: Tue, 20 Aug 2002 14:20:42 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: bct-U

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> There was a discussion in the mailing-list some times ago about the bct-U

The inital reason for the problem with U (AND spin-orbit!!) was that a
filename with just ONE character (like u.struct) lead to a problem with
the normalization of the SO-charge density. This also explains why different
tests lead to different results (all doing bct-U, but some called the
directory just u, others bctu).

The problem was in lapw2, but this has been fixed in the latest version.


> 1) runsp_lapw -orb -in1new 5 -cc 0.0001 -i 99 ; (:ITE37)==>
> :HFF01=-404.991,:MMI01=1.50924,:EFG01=3.38281.
>
> 2) runsp_c_lapw -orb -in1new 5 -cc 0.0001 -i 99 ; (:ITE24)==>
> :HFF01=0.000,:MMI01=0.00000,:EFG01=-7.62824.
>
> 3) runsp_c_lapw -orb -in1new 5 -cc 0.0001 -i 99 + above suggested case.inst;  (:ITE21)==>
> :HFF01=0.000,:MMI01=0.00001,:EFG01=-7.55947.
>
> 4) run_lapw -in1new 5 -cc 0.0001 -i 99 ; (:ITE13)==>
> :HFF01=---,:MMI01=---,:EFG01=3.26087.
>
> 5) runsp_lapw -in1new 5 -cc 0.0001 -i 99 ; (:ITE=13)==>
> :HFF01=-350.370,:MMI01=1.95919,:EFG01=+7.04996.
>
> 1.Why the calculated EFG within step 1 (imposing magnetic) and 2 (forcing zero magnet) are not alike with identical initial conditions, same case.indmup&dn for each cases regarding the same EFG's within step1 and 4?

Why should it be ??? Agreement between 1 and 4 is just accidental and not
perfect either. Similar (but not identical) EFGs do not mean that all the
results are identical under all circumstances.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 19 Aug 2002 18:26:28 +0800
From: gyguo <gyguo@phys.ntu.edu.tw>
Subject: [WIEN]: errors from lapwdm in parallel

====
gyguo <gyguo@phys.ntu.edu.tw>
submitted the following contribution:
====

====
gyguo <gyguo@phys.ntu.edu.tw>
submitted the following contribution:
====


Dear Prof. Blaha and WIEN users,

We found that lapwdm does not work in parallel,
as shown in the following error message.
We use a PC cluster with MPI and PGI compiler.
We did go into the SRC_lapwdm directory,
trying to solve the problem. However,
we cannot find the 'dmatscf.f' program.
Any help to solve the problem will be highly
appreciated.

Regards,

Guang-Yu Guo

- -------- error message ---------------------------------------
x lapwdm -so -up -p
running LAPWDM in parallel mode
[1] 17142
[2] 17157
[3] 17179
[4] 17184
[5] 17189
[6] 17195
[7] 17226

 lapwdm END

 lapwdm END
 lapwdm END
 lapwdm END
 lapwdm END
 lapwdm END
 lapwdm END
[7]    Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
[6]  - Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ... ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
[5]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
[4]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
[3]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
[2]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
[1]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
; rm -f .lock_$lockfile[$p] ) >>  ...
      node10 4.970u 0.370s 0:26.09 20.4% 0+0k 0+0io 235pf+0w
      node11 5.020u 0.390s 0:27.77 19.4% 0+0k 0+0io 234pf+0w
      node12 4.950u 0.400s 0:27.04 19.7% 0+0k 0+0io 235pf+0w
      node13 5.090u 0.280s 0:26.56 20.2% 0+0k 0+0io 235pf+0w
      node14 5.040u 0.320s 0:26.09 20.5% 0+0k 0+0io 235pf+0w
      node15 4.940u 0.320s 0:25.32 20.7% 0+0k 0+0io 235pf+0w
      node16 4.970u 0.330s 0:24.48 21.6% 0+0k 0+0io 235pf+0w
   Summary of lapwdmpara:
   node10        user=4.97       wallclock=26.09
   node11        user=5.02       wallclock=27.77
   node12        user=4.95       wallclock=27.04
   node13        user=5.09       wallclock=26.56
   node14        user=5.04       wallclock=26.09
   node15        user=4.94       wallclock=25.32
   node16        user=4.97       wallclock=24.48
PGFIO-F-231/formatted read/internal file/error on data conversion.
 In source file dmatscf.f, at line number 69
35.220u 2.680s 0:32.19 117.7%   0+0k 0+0io 26239pf+0w


- --
Dr. G.Y. Guo
Professor
Department of Physics
National Taiwan University
1 Roosevelt Road, Sec. 4
Taipei 106, Taiwan, R.O.C.
Tel. ++886-2-33665180
Fax. ++886-2-23639984
E-mail: gyguo@phys.ntu.edu.tw


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------------------------------

Date: Tue, 20 Aug 2002 09:05:49 -0700 (PDT)
From: Michelle Johannes <johannes@maugre.ucdavis.edu>
Subject: Re: [WIEN]: single vs. double cells

====
Michelle Johannes <johannes@maugre.ucdavis.edu>
submitted the following contribution:
====

====
Michelle Johannes <johannes@maugre.ucdavis.edu>
submitted the following contribution:
====

Peter-
	Wow, I'm really sorry about that.  I have no idea why my z would
have been increased so I never even checked it.  I ran this calculation
quite a few times to make sure the problem wasn't something spurious but I
never thought to remake the .struct file from scratch.  If its any
consolation, I am very, very happy to have the answer.

	Michelle


On Tue, 20 Aug 2002, Peter Blaha wrote:

> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> > 	I am investigating a AFM compound and therefore have to double my
> > unit cell.  In the compound I am looking at the single cell is the cubic
> > space group #221 (Pm-3m).  This is a peroskite structure and the afm order
> > is along the (111) axis and therefore I end up with a rhombohedral cell
> > which is space group #166 (R-3m).  The problem is that if I calculate the
> > ferromagnetic solution in the doubled cell, my energy doesn't look
> > anything like that of double the single cell energy.  In fact, there is an
> > approximately 30 Ryd difference!!
> 
> Hi!
> 
> I guess you own me a beer should we ever meet at a conference!!!!!
> 
> It took me 3 hours to find out that your atttched struct file had a Ga-Z
> of 31.1 instead of 31.0 and then of course the total energies are off by
> 30 Ry.
> 
> PS: You also had different RMT values, but this does not account for 30 Ry.
> 
> Regards
> 
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
> 
> ====
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------------------------------

Date: Tue, 20 Aug 2002 16:05:09 -0700 (PDT)
From: yanming Ma <ymma66@yahoo.com>
Subject: Re: [WIEN]: About AIM

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-796074058-1029884709=:605
Content-Type: text/plain; charset=us-ascii


Dear wien2k users, 
I think I have gotten neccessay references for the AIM from all the replies. 
I really appreciate all your kind replies. 
Thanks very much for all of you, Alexander, Torsten, Jorge, Xiangyuan, and Victor.

Cheers

 

Yanming Ma Ph.D

National research council of Canada, Steacie institute for molecular Sciences.

ottawa, ontario

  

 "Dr. Alexander Hofmann" wrote:Dear Yanming,

The basic articles are attached below.

For some reasons I made in my molecular life tests with Baders program (PROAIMV) on the water molecule with different basis sets. I did the same with the Mulliken analysis (very common in molecular chemistry) and the Gaussian98 NPA (=Natural Population Analysis). And it turned out that the NPA is the most stable analysis with respect to varying basis sets. 
We can learn at least a couple of things from this (comments welcome):
- - Even the conceptually best analysis (Bader) gives widely spreaded _absolute_ numbers. 
- - charge difference are quite reliable
- - NPA is best for water, but it seems this due to some error cancellation.

My take home message is: Carefully with absolute charges, trends are surely ok.


with best regards

Alex

PS: attached the mentioned table (TeX-Format)

@article{bader81,
TITLE={Quantum Theory of Atoms in Molecules - Dalton Revisited},
AUTHOR={R. F. W. Bader
and T. T. Nguyen-Dang},
JOURNAL={Adv. Quantum Chem.},
YEAR={1981},
VOLUME={14},
PAGES={63}
}

@book{bader90,
TITLE={Atoms in Molecules - A Quantum Theory},
AUTHOR={R. F. W. Bader},
PUBLISHER={Oxford University Press},
YEAR={1990},
address={Oxford},
}

@article{bader91,
TITLE={A Quantum Theory of Molecular Structure and Its Applications},
AUTHOR={R. F. W. Bader},
JOURNAL={Chem. Rev.},
YEAR={1991},
VOLUME={91},
PAGES={893}
}

- -- 

Dr. Alexander Hofmann

Humboldt-Universitaet zu Berlin
Institut fuer Chemie
Arbeitsgruppe Quantenchemie

Brook-Taylor-Strasse 2

12489 Berlin

ah@chemie.hu-berlin.de

Tel.: +49-30-2093-7138
Fax.: +49-30-2093-7136

http://www.chemie.hu-berlin.de/ag_sauer/index.html

PGP-Key: wwwkeys.de.pgp.net ID: D9D62D35
> ATTACHMENT part 2 application/x-tex 


- ---------------------------------
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- --0-796074058-1029884709=:605
Content-Type: text/html; charset=us-ascii

<P>Dear wien2k users, 
<P>I think I have gotten neccessay references for the AIM from all the replies. 
<P>I really appreciate all your kind replies. 
<P>Thanks very much for all of you, Alexander, Torsten, Jorge, Xiangyuan,&nbsp;and Victor.</P>
<P>Cheers</P>
<P>&nbsp;</P>
<P>Yanming Ma Ph.D</P>
<P>National research council of Canada, Steacie institute for molecular Sciences.</P>
<P>ottawa,&nbsp;ontario</P>
<P>&nbsp;&nbsp;</P>
<P>&nbsp;<B><I>"Dr. Alexander Hofmann" <AH@CHEMIE.HU-BERLIN.DE></I></B>wrote:
<BLOCKQUOTE style="PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #1010ff 2px solid">Dear Yanming,<BR><BR>The basic articles are attached below.<BR><BR>For some reasons I made in my molecular life tests with Baders program (PROAIMV) on the water molecule with different basis sets. I did the same with the Mulliken analysis (very common in molecular chemistry) and the Gaussian98 NPA (=Natural Population Analysis). And it turned out that the NPA is the most stable analysis with respect to varying basis sets. <BR>We can learn at least a couple of things from this (comments welcome):<BR>- Even the conceptually best analysis (Bader) gives widely spreaded _absolute_ numbers. <BR>- charge difference are quite reliable<BR>- NPA is best for water, but it seems this due to some error cancellation.<BR><BR>My take home message is: Carefully with absolute charges, trends are surely ok.<BR><BR><BR>with best regards<BR><BR>Alex<BR><BR>PS: attached the mentioned table (TeX-Format)<BR><BR>!
@article{bader81,<BR>TITLE={Quantum Theory of Atoms in Molecules - Dalton Revisited},<BR>AUTHOR={R. F. W. Bader<BR>and T. T. Nguyen-Dang},<BR>JOURNAL={Adv. Quantum Chem.},<BR>YEAR={1981},<BR>VOLUME={14},<BR>PAGES={63}<BR>}<BR><BR>@book{bader90,<BR>TITLE={Atoms in Molecules - A Quantum Theory},<BR>AUTHOR={R. F. W. Bader},<BR>PUBLISHER={Oxford University Press},<BR>YEAR={1990},<BR>address={Oxford},<BR>}<BR><BR>@article{bader91,<BR>TITLE={A Quantum Theory of Molecular Structure and Its Applications},<BR>AUTHOR={R. F. W. Bader},<BR>JOURNAL={Chem. Rev.},<BR>YEAR={1991},<BR>VOLUME={91},<BR>PAGES={893}<BR>}<BR><BR>-- <BR><BR>Dr. Alexander Hofmann<BR><BR>Humboldt-Universitaet zu Berlin<BR>Institut fuer Chemie<BR>Arbeitsgruppe Quantenchemie<BR><BR>Brook-Taylor-Strasse 2<BR><BR>12489 Berlin<BR><BR>ah@chemie.hu-berlin.de<BR><BR>Tel.: +49-30-2093-7138<BR>Fax.: +49-30-2093-7136<BR><BR>http://www.chemie.hu-berlin.de/ag_sauer/index.html<BR><BR>PGP-Key: wwwkeys.de.pgp.net ID: D9D62D35<BR>&g!
t; ATTACHMENT part 2 application/x-tex </BLOCKQUOTE><p><br><hr size=1><b>Do You Yahoo!?</b><br>
<a href="http://rd.yahoo.com/careers/mailsig/new/*http://www.hotjobs.com">HotJobs, a Yahoo! service</a> - Search Thousands of New Jobs
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Date: Wed, 21 Aug 2002 08:32:34 +0200 (MET DST)
From: Pavel Novak <novakp@fzu.cz>
Subject: Re: [WIEN]: LDA+U for systems without inversion symmetry

====
Pavel Novak <novakp@fzu.cz>
submitted the following contribution:
====

Dear colleague,

there is a problem when running LDA+U on systems without the inversion
symmetry - during the calculation a spurious orbital moment may develop
and scf procedure may not converge. When considering (YCa)2BaNiO5 (LDA+U,
without s-o, no inversion symmetry) I solved this problem by averaging out
the orbital potential.

Best regards
Pavel Novak

On Mon, 19 Aug 2002, gyguo wrote:

> ====
> gyguo <gyguo@phys.ntu.edu.tw>
> submitted the following contribution:
> ====
>
> ====
> gyguo <gyguo@phys.ntu.edu.tw>
> submitted the following contribution:
> ====
>
>
> Dear Prof. Blaha and WIEN users,
>
> We have been trying to perform LDA+U calculations without SO
> for systems without inversion symmetry, and we have failed.
> We have used both runsp_lapw -orb and runsp_c_lapw -orb.
> I think that the problem is due to the fact that lapwdm -dn -c
> is not executed, as one can see from the 'dayfile' and 'error message'
> enclosed below. We have no problem for systems with inversion
> symmetry or for LDA+U+SO calculations. I don't know runsp_lapw
> and x_lapw well enough to modify it.
>
> Could anyone modify runsp_lapw and x_lapw so that we can
> do LDA+U calculations for systems without inversion symmetry
> (no SO) in both serial and parallel executions?
> Thank you very much in advance.
>
> Regards,
> Guang-Yu Guo
>
>
>
>
>
> ---------------- dayfile
> ------------------------------------------------------------------------
>     start       (Sat Aug 17 16:17:44 CST 2002) with lapw0 (20/20 to go)
> >   lapw0       (16:17:44) 48.210u 0.560s 0:50.68 96.2% 0+0k 0+0io 274pf+0w
> >   lapw1  -c -up   -orb        (16:18:35) 1649.100u 20.790s 27:56.19 99.6%
> 0+0k 0+0io 390pf+0w
> >   lapw2 -c -up        (16:46:32) 118.960u 7.450s 2:14.88 93.7%        0+0k 0+0
> io 318pf+0w
> >   lapw2 -c -dn        (16:48:47) 61.270u 3.420s 1:05.48 98.7% 0+0k 0+0io 316pf
> +0w
> >   lapwdm -up   -c     (16:49:53) 2.600u 0.870s 0:04.00 86.7%  0+0k 0+0io 233pf
> +0w
> >   lcore -up   (16:49:57) 0.580u 0.010s 0:00.71 83.0%  0+0k 0+0io 176pf+0w
> >   lcore -dn   (16:49:58) 0.600u 0.000s 0:00.63 95.2%  0+0k 0+0io 176pf+0w
> >   mixer       (16:49:59) 6.730u 0.450s 0:10.18 70.5%  0+0k 0+0io 201pf+0w
> :ENERGY convergence:  0 0 1.2786595000000000
> :CHARGE convergence:  0 0.00001 .5435234
>
> ------------------- error message
> ------------------------------------------------------------
>  LAPW0 END
>  LAPW1 END
>  LAPW2 END
>  LAPW2 END
>  lapwdm END
> total_exec: Command not found.
>  CORE  END
>  CORE  END
>  MIXER END
> in cycle 2    ETEST: 1.2786595000000000   CTEST: .5435234
>  LAPW0 END
> PGFIO-F-217/list-directed read/unit=9/attempt to read past end of file.
>  File name = su-1ceco2-2sp+u.dmatdn    formatted, sequential access   record = 1
>  In source file init.f, at line number 226
> PGFIO-F-217/list-directed read/unit=10/attempt to read past end of file.
>  File name = su-1ceco2-2sp+u.dmatdn    formatted, sequential access   record = 1
>  In source file init.f, at line number 226
>  LAPW1 END
>  LAPW2 END
>  LAPW2 END
>  lapwdm END
>
>
> --
> Dr. G.Y. Guo
> Professor
> Department of Physics
> National Taiwan University
> 1 Roosevelt Road, Sec. 4
> Taipei 106, Taiwan, R.O.C.
> Tel. ++886-2-33665180
> Fax. ++886-2-23639984
> E-mail: gyguo@phys.ntu.edu.tw
>
>
> ====
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------------------------------

Date: Wed, 21 Aug 2002 15:41:04 +0800 (CST)
From: yshzhang@theory.issp.ac.cn
Subject: [WIEN]: DOS

====
yshzhang@theory.issp.ac.cn
submitted the following contribution:
====

Dear all

I meet a confused question.
I am caculating the V2O3 with U.After SCF,I plot the  partial DOS of 
vanadium(d,dz2,dx2y2,dxy,dxz,dyz).But in the DOS, the summary of 
dz2,dx2y2,dxy,dxz,dyz is much larger than d.and the figures of dxy,dxz,dyz
are absoulte sameness.I don't know why.
In the SCF,there is no any error occur.

The following is a line in case.dos1evup.
 E,d,dz2,dx2y2,dxy,dxz,dyz
 -5.02081     0.58548264    0.08934838 0.14079606    2.69683133   
               2.69683133   2.69683133

- -- 
Best Regards
YS Zhang

- ------------------------------------------------------------------------
 Address: Institute of Solid State Physics
          Chinese Academy of Sciences
          P.O.BOX 1129,230031 Hefei 
          P.R~China
 Tel:     086-551-5591464(Office)
          086-551-5592837(Home)
 Fax:     086-551-5591434
 WWW:     http://theory.issp.ac.cn/~yshzhang
- ------------------------------------------------------------------------


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------------------------------

Date: Wed, 21 Aug 2002 16:29:08 +0800
From: gyguo <gyguo@phys.ntu.edu.tw>
Subject: Re: [WIEN]: errors from lapwdm in parallel

====
gyguo <gyguo@phys.ntu.edu.tw>
submitted the following contribution:
====

Dear Prof. Blaha and WIEN users,

The following e-mail was sent recently.
The problem remains even when we use
the latest version of WIEN2k
(downloaded 19 August 2002).
If anyone knows how to solve the problem,
please let us know. Thank you.

Guang-Yu Guo

gyguo ¼g¹D¡G

> ====
> gyguo <gyguo@phys.ntu.edu.tw>
> submitted the following contribution:
> ====
>
> Dear Prof. Blaha and WIEN users,
>
> We found that lapwdm does not work in parallel,
> as shown in the following error message.
> We use a PC cluster with MPI and PGI compiler.
> We did go into the SRC_lapwdm directory,
> trying to solve the problem. However,
> we cannot find the 'dmatscf.f' program.
> Any help to solve the problem will be highly
> appreciated.
>
> Regards,
>
> Guang-Yu Guo
>
> -------- error message ---------------------------------------
> x lapwdm -so -up -p
> running LAPWDM in parallel mode
> [1] 17142
> [2] 17157
> [3] 17179
> [4] 17184
> [5] 17189
> [6] 17195
> [7] 17226
>
>  lapwdm END
>
>  lapwdm END
>  lapwdm END
>  lapwdm END
>  lapwdm END
>  lapwdm END
>  lapwdm END
> [7]    Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
> ; rm -f .lock_$lockfile[$p] ) >>  ...
> [6]  - Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
> ; rm -f .lock_$lockfile[$p] ) >>  ... ( cd $PWD; $t $exe ${def}_${loop}.def $loop
> ; rm -f .lock_$lockfile[$p] ) >>  ...
> [5]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
> ; rm -f .lock_$lockfile[$p] ) >>  ...
> [4]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
> ; rm -f .lock_$lockfile[$p] ) >>  ...
> [3]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
> ; rm -f .lock_$lockfile[$p] ) >>  ...
> [2]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
> ; rm -f .lock_$lockfile[$p] ) >>  ...
> [1]  + Done                          ( cd $PWD; $t $exe ${def}_${loop}.def $loop
> ; rm -f .lock_$lockfile[$p] ) >>  ...
>       node10 4.970u 0.370s 0:26.09 20.4% 0+0k 0+0io 235pf+0w
>       node11 5.020u 0.390s 0:27.77 19.4% 0+0k 0+0io 234pf+0w
>       node12 4.950u 0.400s 0:27.04 19.7% 0+0k 0+0io 235pf+0w
>       node13 5.090u 0.280s 0:26.56 20.2% 0+0k 0+0io 235pf+0w
>       node14 5.040u 0.320s 0:26.09 20.5% 0+0k 0+0io 235pf+0w
>       node15 4.940u 0.320s 0:25.32 20.7% 0+0k 0+0io 235pf+0w
>       node16 4.970u 0.330s 0:24.48 21.6% 0+0k 0+0io 235pf+0w
>    Summary of lapwdmpara:
>    node10        user=4.97       wallclock=26.09
>    node11        user=5.02       wallclock=27.77
>    node12        user=4.95       wallclock=27.04
>    node13        user=5.09       wallclock=26.56
>    node14        user=5.04       wallclock=26.09
>    node15        user=4.94       wallclock=25.32
>    node16        user=4.97       wallclock=24.48
> PGFIO-F-231/formatted read/internal file/error on data conversion.
>  In source file dmatscf.f, at line number 69
> 35.220u 2.680s 0:32.19 117.7%   0+0k 0+0io 26239pf+0w
>
> --
> Dr. G.Y. Guo
> Professor
> Department of Physics
> National Taiwan University
> 1 Roosevelt Road, Sec. 4
> Taipei 106, Taiwan, R.O.C.
> Tel. ++886-2-33665180
> Fax. ++886-2-23639984
> E-mail: gyguo@phys.ntu.edu.tw
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====

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------------------------------

Date: Wed, 21 Aug 2002 12:36:33 +0400
From: "Alexander Korlyukov" <alex@xrlab.ineos.ac.ru>
Subject: [WIEN]: X-ray structural factors

====
"Alexander Korlyukov" <alex@xrlab.ineos.ac.ru>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0044_01C2490F.62181E00
Content-Type: text/plain;
	charset="koi8-r"
Content-Transfer-Encoding: quoted-printable

Dear Wien2k users.

I am quite newbie in Wien2k
So I have a couple of questions to more experienced users, which dealt =
with lapw3 program.=20

When I run lapw3 on hydrogen peroxide (space group P4(3)2(1)2), most of =
X-ray structural factors obtained have negative sign. Obviously, that =
such a set of X-ray structural factors contradicts to the experimental =
data.=20
What kind of input parameters (in files case.in1, case.in2 and so on) =
may influnce on sign of structural factor?
Is this (obtainig of negative structural factors) deal with Struct Gen? =
(Calculation of cubic groups (TiO2, Si, Ge etc.) always give only =
positive ones)

Alexander Korlyukov,

Ph. D. Student

INEOS RAS, Russia



- ------=_NextPart_000_0044_01C2490F.62181E00
Content-Type: text/html;
	charset="koi8-r"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META content=3D"text/html; charset=3Dkoi8-r" http-equiv=3DContent-Type>
<META content=3D"MSHTML 5.00.2314.1000" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#c0c0c0>
<DIV><FONT face=3DArial size=3D2>Dear Wien2k users.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3D"Arial CYR" size=3D2>I am quite newbie in =
Wien2k</FONT></DIV>
<DIV><FONT face=3D"Arial CYR" size=3D2>So I have a couple of questions =
to more=20
experienced users,&nbsp;which dealt with lapw3 program. </FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>When I run lapw3 on hydrogen peroxide =
(space group=20
P4(3)2(1)2), most of X-ray structural factors&nbsp;obtained have =
negative=20
sign.&nbsp;Obviously, that such a set of X-ray structural factors =
contradicts to=20
the experimental data. </FONT></DIV>
<DIV><FONT face=3DArial size=3D2>What kind of input parameters (in files =
case.in1,=20
case.in2 and so on) may influnce on sign of structural =
factor?</FONT></DIV>
<DIV><FONT face=3D"Arial CYR" size=3D2>Is this (obtainig of negative =
structural=20
factors) deal with Struct Gen? (Calculation of cubic groups (TiO2, Si, =
Ge etc.)=20
always give only positive ones)</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3D"Arial CYR" size=3D2>Alexander Korlyukov,</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3D"Arial CYR" size=3D2>Ph. D. Student</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3D"Arial CYR" size=3D2>INEOS RAS, Russia</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV>&nbsp;</DIV></BODY></HTML>

- ------=_NextPart_000_0044_01C2490F.62181E00--

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------------------------------

Date: Wed, 21 Aug 2002 11:00:47 +0200
From: Enrique Lomba <E.Lomba@iqfr.csic.es>
Subject: [WIEN]: Problem calculating DOS

====
Enrique Lomba <E.Lomba@iqfr.csic.es>
submitted the following contribution:
====

Hello all,
I am trying to calculate the DOS of trigonal Te, I have a converged 
calculation with the corresponding Te.vector file and when running
x lapw2 -qtl -c to generate the partial charges I got the following error

x lapw2 -qtl -c
PGFIO-F-231/formatted read/unit=1001/error on data conversion.
  File name = /scratch/enrique/Te.help031    formatted, sequential 
access   record = 13827
  In source file outp.f, at line number 179

Now checking the file Te.help031  it turns out that there are several 
records with ****** and cannot be read, for instance

   L= 2 **********    3778.777  1734.128  8947.667  3946.588 -2872.261
    DZ2:1031.24651     232.066   108.280   561.864   244.372  -179.853
  DX2Y2: 188.48954      44.795    19.674   100.627    44.140   -32.444
    DXY:2452.45155     562.799   256.407  1321.702   580.255  -424.483
    DXZ: 308.16757      85.456    29.708   153.398    69.021   -49.218
    DYZ:**********    2853.661  1320.059  6810.077  3008.800 -2186.264


it seems they all correspond to L=2, could someone give me some hint on 
what is going on ??
			Thanks and regards,
					Enrique


- -- 
- --------------------------------------------------------------
Enrique Lomba
Instituto de Quimica Fisica Rocasolano, CSIC
C/ Serrano 119, 28006 Madrid, Spain

FAX no. 34-915642431
Phone no. 34-915619407 (ext 1301)
e-mail : E.Lomba@iqfr.csic.es
www : http://www.fluid.iqfr.csic.es/enrique.html

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------------------------------

Date: Wed, 21 Aug 2002 02:09:43 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: DOS

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> I meet a confused question.
> I am caculating the V2O3 with U.After SCF,I plot the  partial DOS of
> vanadium(d,dz2,dx2y2,dxy,dxz,dyz).But in the DOS, the summary of
> dz2,dx2y2,dxy,dxz,dyz is much larger than d.and the figures of dxy,dxz,dyz
> are absoulte sameness.I don't know why.
> In the SCF,there is no any error occur.

> The following is a line in case.dos1evup.
>  E,d,dz2,dx2y2,dxy,dxz,dyz
>  -5.02081     0.58548264    0.08934838 0.14079606    2.69683133
>                2.69683133   2.69683133

You would not compare the value of the DOSs at a specific energy -- one line
of case.dos1(ev)up/dn -- as it gives no sense in the solid. Instead, one
will find the physical relation comparing the integral of the DOS's in
specific energy windows: grep :QTLxx partial charges. This means that the
number of electrons in for instance d-orbital should be expected to be equal
to the sum of occupation numbers of d-partial density of states.


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------------------------------

Date: Wed, 21 Aug 2002 11:19:23 +0200
From: Thomas Claesson <tcl@kth.se>
Subject: Re: [WIEN]: Two questions

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Many thanks for your help again, Igor! What I have been doing is 
save_lapw as soon as I reach self consistency, thinking that all files 
that need to be deleted actually were deleted, but perhaps the .vorb 
files are not deleted by save_lapw. So your suggestion is that I do this:
1) Delete .vorb files manually
2) Run to self consistency without -orb
3) save_lapw
4) Calculate bandstructure
5) Run with -orb -i 2 (with U=J=0.0001)
6) save_lapw
7) Calculate bandstructure not forgetting the -orb switch to lapw1

Have I got it right or have I missed anything or perhaps got the order 
wrong?

Thanks in advance!

Best regards,
Thomas Claesson

Igor Mazin wrote:

>====
>Igor Mazin <wienuser1@yahoo.com>
>submitted the following contribution:
>====
>
>If you are puzzled a bit, I am puzzled entirely.
>Fortunately Peter is back; after the magic with which
>he fished out the wrong Z in Michelle's case, I start
>to believe in his omnipotency.
>
>I have no clue of how what you describe may be
>possible. My last lame suggestion: I assume you had
>deleted all vorb files before doing this experiment.
>If you hadn't, you should. And BTW repeat -orb
>itereation twice, to produce new vorbs.
>
>>drastic, so I am still 
>>a bit puzzled about what is going on.
>>
>
>=====
>***************************************************************************** 
>Igor Mazin, Naval Research Laboratory, Washington, DC 20375
>Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
>*****************************************************************************
>
>__________________________________________________
>Do You Yahoo!?
>HotJobs - Search Thousands of New Jobs
>http://www.hotjobs.com
>====
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------------------------------

Date: Wed, 21 Aug 2002 11:35:17 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: X-ray structural factors

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> When I run lapw3 on hydrogen peroxide (space group P4(3)2(1)2), most of X-ray structural factors obtained have negative sign. Obviously, that such a set of X-ray structural factors contradicts to the experimental data.

Negative structure factors are of course possible and correct.
Only experiment has the problem that they measure F**2, i.e. they loose
the sign (and phases).
Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 21 Aug 2002 17:46:37 +0800 (CST)
From: yshzhang@theory.issp.ac.cn
Subject: Re: [WIEN]: DOS

====
yshzhang@theory.issp.ac.cn
submitted the following contribution:
====

> You would not compare the value of the DOSs at a specific energy -- one line
> of case.dos1(ev)up/dn -- as it gives no sense in the solid. Instead, one
> will find the physical relation comparing the integral of the DOS's in
> specific energy windows: grep :QTLxx partial charges. This means that the
> number of electrons in for instance d-orbital should be expected to be equal
> to the sum of occupation numbers of d-partial density of states.

Yes,In case.scf,the number of electrons in d is equal to the sum of 
occupation numbers of d-partial.But we can also check this in DOS,thought
caculate the integral below the plot.Using this method,I found the sum 
of the integral of all partial d is too large to belive. 
Is there something wrong?

- -- 
Best Regards
YS Zhang

- ------------------------------------------------------------------------
 Address: Institute of Solid State Physics
          Chinese Academy of Sciences
          P.O.BOX 1129,230031 Hefei 
          P.R~China
 Tel:     086-551-5591464(Office)
          086-551-5592837(Home)
 Fax:     086-551-5591434
 WWW:     http://theory.issp.ac.cn/~yshzhang
- ------------------------------------------------------------------------


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------------------------------

Date: Wed, 21 Aug 2002 12:49:49 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: errors from lapwdm in parallel

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> > We found that lapwdm does not work in parallel,
> > as shown in the following error message.
> > We use a PC cluster with MPI and PGI compiler.
> > We did go into the SRC_lapwdm directory,
> > trying to solve the problem. However,
> > we cannot find the 'dmatscf.f' program.
> > x lapwdm -so -up -p
> >  In source file dmatscf.f, at line number 69

a) At first I could not reproduce your error, because you did not mention
that you used a "non-standard" case.indmc   (krad ne.0). Standard scf
should have worked.
b) Finally I figured out, that your error in dmatscf.f  (SRC_sumpara)!!
could only occur when krad is .ne.0    and then I could reproduce the
problem.
c) Change in SRC_sumpara/dmatscf.f:
....
     ELSE IF(MARGN(2:4).EQ.'XOP') THEN
        READ(MARGN,'(4x,i2,i3,4f12.5)')IATOM,ll, X,y,z,zm       <== change
        xop(IATOM,ll,1)=xop(IATOM,ll,1)+X
        xop(IATOM,ll,2)=xop(IATOM,ll,2)+y
        xop(IATOM,ll,3)=xop(IATOM,ll,3)+z
        xop(IATOM,ll,4)=xop(IATOM,ll,4)+zm
        IF(ILOOP.EQ.IPROC)THEN
           WRITE(22,724)IATOM,ll,(xop(IATOM,ll,ityp),ityp=1,4)  <== change
....
724 FORMAT(':XOP',i2.2,i3,4f12.5)                               <== add

Update on the web will follow soon.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 21 Aug 2002 12:55:50 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Problem calculating DOS

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Now checking the file Te.help031  it turns out that there are several
> records with ****** and cannot be read, for instance
>
>    L= 2 **********    3778.777  1734.128  8947.667  3946.588 -2872.261
>     DZ2:1031.24651     232.066   108.280   561.864   244.372  -179.853
>   DX2Y2: 188.48954      44.795    19.674   100.627    44.140   -32.444
>     DXY:2452.45155     562.799   256.407  1321.702   580.255  -424.483
>     DXZ: 308.16757      85.456    29.708   153.398    69.021   -49.218
>     DYZ:**********    2853.661  1320.059  6810.077  3008.800 -2186.264
>
>
> it seems they all correspond to L=2, could someone give me some hint on
> what is going on ??

It seems you have problems with the energy parameters of l=2 (d) for the
first atom. Most likely this happened for an unoccupied state at higher
energy (? you did not mention the energy) and thus appears only in the
QTL calculation, but not during scf.

Check in case.scf1  what the effective energy parameters for this channel
are. Most likely you should increase the "0.3" value in the input to a
larger number, but without the last iteration of the scf file + case.in1
I cannot say much more.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 21 Aug 2002 04:24:36 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: Re: [WIEN]: Problem calculating DOS

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear Enrique



I think that you have a spin polarized system but you
are trying to plot a non spin polarized DOS.
May be the up and down switches aren't active in your
w2web interface. May be your problem solved if you run
"x lapw2 -up(dn) -qtl" in command box or terminal.
Bests.
H-Salehi
dept of physics
Ferdowsi university
Mashhad  IRAN
- --- Enrique Lomba <E.Lomba@iqfr.csic.es> wrote:
> ====
> Enrique Lomba <E.Lomba@iqfr.csic.es>
> submitted the following contribution:
> ====
> 
> Hello all,
> I am trying to calculate the DOS of trigonal Te, I
> have a converged 
> calculation with the corresponding Te.vector file
> and when running
> x lapw2 -qtl -c to generate the partial charges I
> got the following error
> 
> x lapw2 -qtl -c
> PGFIO-F-231/formatted read/unit=1001/error on data
> conversion.
>   File name = /scratch/enrique/Te.help031   
> formatted, sequential 
> access   record = 13827
>   In source file outp.f, at line number 179
> 
> Now checking the file Te.help031  it turns out that
> there are several 
> records with ****** and cannot be read, for instance
> 
>    L= 2 **********    3778.777  1734.128  8947.667 
> 3946.588 -2872.261
>     DZ2:1031.24651     232.066   108.280   561.864  
> 244.372  -179.853
>   DX2Y2: 188.48954      44.795    19.674   100.627  
>  44.140   -32.444
>     DXY:2452.45155     562.799   256.407  1321.702  
> 580.255  -424.483
>     DXZ: 308.16757      85.456    29.708   153.398  
>  69.021   -49.218
>     DYZ:**********    2853.661  1320.059  6810.077 
> 3008.800 -2186.264
> 
> 
> it seems they all correspond to L=2, could someone
> give me some hint on 
> what is going on ??
> 			Thanks and regards,
> 					Enrique
> 
> 
> -- 
>
- --------------------------------------------------------------
> Enrique Lomba
> Instituto de Quimica Fisica Rocasolano, CSIC
> C/ Serrano 119, 28006 Madrid, Spain
> 
> FAX no. 34-915642431
> Phone no. 34-915619407 (ext 1301)
> e-mail : E.Lomba@iqfr.csic.es
> www : http://www.fluid.iqfr.csic.es/enrique.html
> 
> ====
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> To (un)subscribe send mail to
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------------------------------

Date: Wed, 21 Aug 2002 04:25:51 -0700
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: DOS

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> > You would not compare the value of the DOSs at a specific energy -- one
line
> > of case.dos1(ev)up/dn -- as it gives no sense in the solid. Instead, one
> > will find the physical relation comparing the integral of the DOS's in
> > specific energy windows: grep :QTLxx partial charges. This means that
the
> > number of electrons in for instance d-orbital should be expected to be
equal
> > to the sum of occupation numbers of d-partial density of states.
>
> Yes,In case.scf,the number of electrons in d is equal to the sum of
> occupation numbers of d-partial.

That's okay.

>But we can also check this in DOS,thought
> caculate the integral below the plot.

Sure, you can.

>Using this method,I found the sum
> of the integral of all partial d is too large to belive.
> Is there something wrong?
Most likely your integrating is wrong. If you send me your file and the
QTLs, I'll can try on it.
Your,
S. Jalali.


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Date: Wed, 21 Aug 2002 17:26:11 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: [WIEN]: Has anybody on the list experience with the IBM p630?

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear All,

yes, I know it is a bit off, but I would like to know if anybody has 
some good experiences to share about Wien2k on the IBM p630 or other 
Power4 based system?

Best regards,
Torsten.

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics


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Date: Wed, 21 Aug 2002 18:26:48 +0200
From: Enrique Lomba <E.Lomba@iqfr.csic.es>
Subject: Re: [WIEN]: Problem calculating DOS

====
Enrique Lomba <E.Lomba@iqfr.csic.es>
submitted the following contribution:
====

This is a multi-part message in MIME format.
- --------------060103070208030202050706
Content-Type: text/plain; charset=ISO-8859-15; format=flowed
Content-Transfer-Encoding: 7bit

Peter Blaha wrote:
> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> 
>>Now checking the file Te.help031  it turns out that there are several
>>records with ****** and cannot be read, for instance
>>
>>   L= 2 **********    3778.777  1734.128  8947.667  3946.588 -2872.261
>>    DZ2:1031.24651     232.066   108.280   561.864   244.372  -179.853
>>  DX2Y2: 188.48954      44.795    19.674   100.627    44.140   -32.444
>>    DXY:2452.45155     562.799   256.407  1321.702   580.255  -424.483
>>    DXZ: 308.16757      85.456    29.708   153.398    69.021   -49.218
>>    DYZ:**********    2853.661  1320.059  6810.077  3008.800 -2186.264
>>
>>
>>it seems they all correspond to L=2, could someone give me some hint on
>>what is going on ??
> 
> 
> It seems you have problems with the energy parameters of l=2 (d) for the
> first atom. Most likely this happened for an unoccupied state at higher
> energy (? you did not mention the energy) and thus appears only in the
> QTL calculation, but not during scf.


Hello again,
I fiddled around with the El paramater in case.in1c file with no 
success. Attached is the file an also the .scf1 file. And here are the 
full contents of the .help031 file with the energy of the band

   BAND#  37  E=  1.24718  WEIGHT= 0.0000000
   L= 0    0.04806       0.537     0.009     0.901    -0.682    -0.018
   L= 1    1.18968       1.161     0.028     0.000     0.000     0.000
     PX:   0.43940       0.427     0.013     0.000     0.000     0.000
     PY:   0.17217       0.166     0.006     0.000     0.000     0.000
     PZ:   0.57811       0.569     0.010     0.000     0.000     0.000
   L= 2 **********   10645.237  3274.629 18533.693  9543.235 -5680.571
    DZ2:4328.57095    1165.961   346.262  1954.711  1030.712  -599.893
  DX2Y2:1166.55372     302.895    96.507   546.875   277.654  -167.515



		Regards, Enrique




- -- 
- --------------------------------------------------------------
Enrique Lomba
Instituto de Quimica Fisica Rocasolano, CSIC
C/ Serrano 119, 28006 Madrid, Spain

FAX no. 34-915642431
Phone no. 34-915619407 (ext 1301)
e-mail : E.Lomba@iqfr.csic.es
www : http://www.fluid.iqfr.csic.es/enrique.html

- --------------060103070208030202050706
Content-Type: text/plain;
 name="Teluro.in1c"
Content-Transfer-Encoding: 7bit
Content-Disposition: inline;
 filename="Teluro.in1c"

WFFIL        (WFPRI, SUPWF)
  7.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  0.30    5  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global APW/LAPW)
 2   -2.70      0.010 CONT 1
 2    0.30      0.000 CONT 1
 0   -0.84      0.010 CONT 1
 0    0.30      0.000 CONT 1
 1    0.30      0.000 CONT 1
K-VECTORS FROM UNIT:4   -7.0       1.5      emin/emax window

- --------------060103070208030202050706
Content-Type: text/plain;
 name="Teluro.scf1"
Content-Transfer-Encoding: 7bit
Content-Disposition: inline;
 filename="Teluro.scf1"


          ATOMIC SPHERE DEPENDENT PARAMETERS FOR ATOM  Te        
          OVERALL ENERGY PARAMETER IS    0.3000
          OVERALL BASIS SET ON ATOM IS LAPW
          E( 2)=   -0.5200   E(BOTTOM)=   -0.690   E(TOP)=   -0.350
             APW+lo
          E( 2)=    0.3000
             LOCAL ORBITAL
          E( 0)=   -0.7500   E(BOTTOM)=   -0.750   E(TOP)= -200.000
             APW+lo
          E( 0)=    0.3000
             LOCAL ORBITAL
          E( 1)=    0.3000
             APW+lo

       K=   0.00000   0.00000   0.00000            1
:RKM  : MATRIX SIZE  282LOs:  45  RKM= 6.75  WEIGHT= 1.00  PGR:    
       EIGENVALUES ARE:
        -0.6343986   -0.6343986   -0.6197216   -0.5772444   -0.5772444
        -0.5600529   -0.5452516   -0.5452516   -0.5412693   -0.3790556
        -0.3786083   -0.3786083   -0.2980131   -0.2952441   -0.2904580
        -0.2904580    0.0213062    0.0213062    0.4682067    0.5016183
         0.5016183    0.5200697    0.5200697    0.5833794    0.7489684
         0.7786758    0.7786758    0.8030406    0.8030406    0.8750556
         0.8876852    0.9481874    0.9481874    0.9718222    0.9995902
         0.9995902    1.1001374    1.1001374
       ********************************************************

       NUMBER OF K-POINTS:          149

- --------------060103070208030202050706--

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Date: Wed, 21 Aug 2002 18:50:10 -0700 (PDT)
From: Wien Wien <wien2kny@yahoo.com>
Subject: [WIEN]: large system with hydrogens

====
Wien Wien <wien2kny@yahoo.com>
submitted the following contribution:
====

Dear Wien2k users,
I would like to run calculations for a fairly large
molecule whose net formula is VS2O3N2C17H17 (a total
of 42 atoms). The space group is P-1, with two
molecules per unit cell. The cell volume is ca. 6000
au^3.

I have selected  the RMT values for V to be 1.8, for S
1.4, for O and N 1.2, for C 1.1, and H 0.49 (these are
the maximal numbers allowed by NN program).

The NPT is currently 781.

With these parameters I am running into a problem in
lstart: it appears that most of the core charge leaks
out of the sphere with the separation energies down to
- -10 Ry.

What set of parameters would you recommend for this
case? Is it the hydrogen atoms that cause the problem?


Is this system feasible to be treated at all (I am
running on a linux workstation with dual 1.8 GHz
Pentium Xeon processor and 1.384 Gb of RDRAM).

Thank you very much for your help.
With best regards
Tatyana Polenova

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------------------------------

Date: Thu, 22 Aug 2002 09:10:49 +0200
From: "Dr. Alexander Hofmann" <ah@chemie.hu-berlin.de>
Subject: Re: [WIEN]: Has anybody on the list experience with the IBM p630?

====
"Dr. Alexander Hofmann" <ah@chemie.hu-berlin.de>
submitted the following contribution:
====

Hi Torsten,

our supercomputer centre is currently setting up a p690 system. The main experience is, that the new xlf version 8.x is very tricky. They try to switch back to version 7. No idea about performance. I'm currently fighting with my work horse program (VASP). But I'll surely try to compile w2k for a colleague later ...

Hth

Alex

> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
> 
> Dear All,
> 
> yes, I know it is a bit off, but I would like to know if anybody has 
> some good experiences to share about Wien2k on the IBM p630 or other 
> Power4 based system?
> 
> Best regards,
> Torsten.
> 
> -- 
> Dr. Torsten Andersen
> Department of Physics, Condensed Matter Theory Group, Uppsala University
> UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
> News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics
> 
> 
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====

- -- 

Dr. Alexander Hofmann

Humboldt-Universitaet zu Berlin
Institut fuer Chemie
Arbeitsgruppe Quantenchemie

Brook-Taylor-Strasse 2

12489 Berlin

ah@chemie.hu-berlin.de

Tel.: +49-30-2093-7138
Fax.: +49-30-2093-7136

http://www.chemie.hu-berlin.de/ag_sauer/index.html

PGP-Key: wwwkeys.de.pgp.net ID: D9D62D35
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------------------------------

Date: Thu, 22 Aug 2002 12:16:21 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: large system with hydrogens

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I would like to run calculations for a fairly large
> molecule whose net formula is VS2O3N2C17H17 (a total
> of 42 atoms). The space group is P-1, with two
> molecules per unit cell. The cell volume is ca. 6000
> au^3.
>
> I have selected  the RMT values for V to be 1.8, for S
> 1.4, for O and N 1.2, for C 1.1, and H 0.49 (these are
> the maximal numbers allowed by NN program).
>
> With these parameters I am running into a problem in
> lstart: it appears that most of the core charge leaks
> out of the sphere with the separation energies down to
> -10 Ry.

I believe the problem for core leakage is sulfur ? Can't you make its
sphere bigger? Which atom is closest to it?
Also H is smaller then I'm used in organic materials, but maybe O-H
is that short ?

> What set of parameters would you recommend for this
> case? Is it the hydrogen atoms that cause the problem?

H has no core, so there's no leakage.

> Is this system feasible to be treated at all (I am
> running on a linux workstation with dual 1.8 GHz
> Pentium Xeon processor and 1.384 Gb of RDRAM).

With 84 DIFFICULT atoms (because of small spheres) it is certainly
a big calculation, but should be feasable eventually (start with RKmax=2.5)

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 22 Aug 2002 09:54:40 -0400
From: gpzhang <gpzhang@utk.edu>
Subject: RE: [WIEN]: problem with band structure persists

====
gpzhang <gpzhang@utk.edu>
submitted the following contribution:
====

Dear Peter and Wien users,

Thank you so much, Peter!

I tried to run with

 x spaghetti

but it gave me a similar band structure, which means the curves do not
look like a band and do not change continuously.

By the way, since my compound does not have inversion symmetry, from
x spaghetti -h, I noticed that I may have to use x spaghetti -c.

Am I wrong?

The following is part of my case.in1c

 K-VECTORS FROM UNIT:5
GAMMA         0    0    0  160 2.00 -.50 0.50
              1    1    0  160  1.0
              2    2    0  160  1.0
.....

             79   79    0  160  1.0
M            80   80    0  160  1.0
END


If you need further information, please feel free let me know.

Again, thanks a lot in advance!


Guoping


>===== Original Message From Peter Blaha <pblaha@theochem.tuwien.ac.at> =====
>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
>> Here is what I did. I first created a special K-list and attached it
>> to *.in1c and changed the unit 4 to 5. I ran x lapw1 -c.  (By the way,
>> is there a way to run this in parallel? The code complains if I do x
>> lapw1 -c -p).
>
>I guess the code also tells you, that you can run in parallel only with a
>klist from unit 4, not 5 !!! You could insert the special k-mesh into
>case.klist, leave unit=4 and run x lapw1 -p -c
>Then concatenate all output1_x files into one single file.
>
>> After I finished it, I edited case.insp by inserting Ef
>> (from case.scf). Then do x spaghetti -c.
>
>You should not use the -c
>PS: If the options are not clear, always use:   x spaghetti -h
>It tells you all allowed options for this program.
>
>> `1525-097 A READ statement using decimal base input found the invalid
>> digit '.' in the input file.  The program will recover by assuming a
>> zero in its place.  STOP end OK 0.4u 0.1s 0:01 56% 36+314k 0+0io
>> 21pf+0w RETURN key to continue ...'
>
>I suggest to remove case.insp and recreate it from the template.
>
>> In addition, I found that my case.qtl has zero bytes in it.
>
>This should be ok, since you did not x lapw2 -qtl -c   (and you don't need
>it unless you want a "character-plot").
>
>Regards
>
>                                      P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
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------------------------------

Date: Thu, 22 Aug 2002 18:32:39 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: large system with hydrogens

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> > Is this system feasible to be treated at all (I am
> > running on a linux workstation with dual 1.8 GHz
> > Pentium Xeon processor and 1.384 Gb of RDRAM).
>
> With 84 DIFFICULT atoms (because of small spheres) it is certainly
> a big calculation, but should be feasable eventually (start with
RKmax=2.5)

What are the recommended number of K points, Gmax, for calculating a
hypothetical protein: a polypeptide chain of amino acids containing 3.6
residues or something around 100 organic atoms? What is the efficiency of
parallel computing in the case of using only one K-point?

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Date: Thu, 22 Aug 2002 07:43:02 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: large system with hydrogens

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

Tanya,

Re H. I was doing solid molecular H eight years ago
with a similar (D. Singh's) code. One unexpected
problem was that a good convergence of the total
energy required anomalously large GMAX (quite larger
than twice RMAX).

Maybe this is a public knowledge by now, at that time
it came as a surprise.

Igor

- --- Wien Wien <wien2kny@yahoo.com> wrote:
> ====
> Wien Wien <wien2kny@yahoo.com>
> submitted the following contribution:
> ====
> 
> Dear Wien2k users,
> I would like to run calculations for a fairly large
> molecule whose net formula is VS2O3N2C17H17 (a total
> of 42 atoms). The space group is P-1, with two
> molecules per unit cell. The cell volume is ca. 6000
> au^3.
> 
> I have selected  the RMT values for V to be 1.8, for
> S
> 1.4, for O and N 1.2, for C 1.1, and H 0.49 (these
> are
> the maximal numbers allowed by NN program).
> 
> The NPT is currently 781.
> 
> With these parameters I am running into a problem in
> lstart: it appears that most of the core charge
> leaks
> out of the sphere with the separation energies down
> to
> -10 Ry.
> 
> What set of parameters would you recommend for this
> case? Is it the hydrogen atoms that cause the
> problem?
> 
> 
> Is this system feasible to be treated at all (I am
> running on a linux workstation with dual 1.8 GHz
> Pentium Xeon processor and 1.384 Gb of RDRAM).
> 
> Thank you very much for your help.
> With best regards
> Tatyana Polenova
> 
> __________________________________________________
> Do You Yahoo!?
> HotJobs - Search Thousands of New Jobs
> http://www.hotjobs.com
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====


=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

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------------------------------

Date: Thu, 22 Aug 2002 16:46:42 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: RE: [WIEN]: problem with band structure persists

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> By the way, since my compound does not have inversion symmetry, from
> x spaghetti -h, I noticed that I may have to use x spaghetti -c.
>
> Am I wrong?

Yes, you are wrong. Not all programs require the -c switch, only those
where inversion symmetry really matters.

Check you case.output1 file if it really contains the eigenvalues for
the k-points listed below, or if you still have a case.output1 with a
tetrahedral mesh ?

>  K-VECTORS FROM UNIT:5
> GAMMA         0    0    0  160 2.00 -.50 0.50
>               1    1    0  160  1.0
>               2    2    0  160  1.0
> .....
>
>              79   79    0  160  1.0
> M            80   80    0  160  1.0
> END

If the output file looks ok, please send this file (+ struct +insp) directly
to me (gzipped).

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 22 Aug 2002 17:25:40 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: problem with band structure persists

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Guoping,

I have had similar problems with some calculations. In some cases it was 
solved by increasing the MT basis. Are you sure the calculation has 
converged (with respect to kmax, gmax, lmax)?

Best regards,
Torsten Andersen.

gpzhang wrote:

>====
>gpzhang <gpzhang@utk.edu>
>submitted the following contribution:
>====
>
>Dear Peter and Wien users,
>
>Thank you so much, Peter!
>
>I tried to run with
>
> x spaghetti
>
>but it gave me a similar band structure, which means the curves do not
>look like a band and do not change continuously.
>
>By the way, since my compound does not have inversion symmetry, from
>x spaghetti -h, I noticed that I may have to use x spaghetti -c.
>
>Am I wrong?
>
>The following is part of my case.in1c
>
> K-VECTORS FROM UNIT:5
>GAMMA         0    0    0  160 2.00 -.50 0.50
>              1    1    0  160  1.0
>              2    2    0  160  1.0
>.....
>
>             79   79    0  160  1.0
>M            80   80    0  160  1.0
>END
>
>
>If you need further information, please feel free let me know.
>
>Again, thanks a lot in advance!
>
>
>Guoping
>
>
>>===== Original Message From Peter Blaha <pblaha@theochem.tuwien.ac.at> =====
>>====
>>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>>submitted the following contribution:
>>====
>>
>>>Here is what I did. I first created a special K-list and attached it
>>>to *.in1c and changed the unit 4 to 5. I ran x lapw1 -c.  (By the way,
>>>is there a way to run this in parallel? The code complains if I do x
>>>lapw1 -c -p).
>>>
>>I guess the code also tells you, that you can run in parallel only with a
>>klist from unit 4, not 5 !!! You could insert the special k-mesh into
>>case.klist, leave unit=4 and run x lapw1 -p -c
>>Then concatenate all output1_x files into one single file.
>>
>>>After I finished it, I edited case.insp by inserting Ef
>>>(from case.scf). Then do x spaghetti -c.
>>>
>>You should not use the -c
>>PS: If the options are not clear, always use:   x spaghetti -h
>>It tells you all allowed options for this program.
>>
>>>`1525-097 A READ statement using decimal base input found the invalid
>>>digit '.' in the input file.  The program will recover by assuming a
>>>zero in its place.  STOP end OK 0.4u 0.1s 0:01 56% 36+314k 0+0io
>>>21pf+0w RETURN key to continue ...'
>>>
>>I suggest to remove case.insp and recreate it from the template.
>>
>>>In addition, I found that my case.qtl has zero bytes in it.
>>>
>>This should be ok, since you did not x lapw2 -qtl -c   (and you don't need
>>it unless you want a "character-plot").
>>
>>Regards
>>
>>                                     P.Blaha
>>--------------------------------------------------------------------------
>>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>>Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
>>--------------------------------------------------------------------------
>>
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>>majordomo@zeus.theochem.tuwien.ac.at
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>>
>
>
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>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Thu, 22 Aug 2002 17:46:19 +0200
From: Michel Penicaud <michel.penicaud@cea.fr>
Subject: [WIEN]: Bug report

====
Michel Penicaud <michel.penicaud@cea.fr>
submitted the following contribution:
====

  In a calculation of  orthorhombic  alpha-U with the experimental
parameters of ambient conditions the  force with respect to the global
coordinate system is:

     FGL01:      0.         -1.745             0.                  in
mRy/a.u.

 But if  p1/2 LO are included in the calculation the force become:

    FGL01:       0.        -2567.561       0.


          I think there is something  wrong  !

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------------------------------

Date: Thu, 22 Aug 2002 09:48:52 -0700 (PDT)
From: Wien Wien <wien2kny@yahoo.com>
Subject: [WIEN]: large system with hydrogens; cont'd

====
Wien Wien <wien2kny@yahoo.com>
submitted the following contribution:
====

- --0-1700026962-1030034932=:19200
Content-Type: text/plain; charset=us-ascii
Content-Disposition: inline

Dear Dr. Blaha,
thank you very much for your response. 
I changed the RMT value for S to 2.1 (the maximum
allowed by the NN), and this didn't solve the problem
of the core charge leakage unfortunately. One of the
sulfur atoms is coordinated to V and bound to C, the
second one is close to two C atoms.

The size of the spheres for the remaining atoms (O, C,
N, and H is the maximum allowed by NN). The C-H bonds
are short. I am attaching the xyz file containing the
X-ray coordinates for this molecule just in case.

In this calculation I am only interested in finding
out the EFG on the vanadium atom, and I was wondering
whether there would be any shortcuts (e.g., whether
there is anything I could ignore).

Thank you very much!
With best regards
Tatyana Polenova



- --- Peter Blaha <pblaha@theochem.tuwien.ac.at> wrote:
> Date: Thu, 22 Aug 2002 12:16:21 +0200 (MEST)
> From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
> To: <wien@zeus.theochem.tuwien.ac.at>
> Subject: Re: [WIEN]: large system with hydrogens
> 
> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> > I would like to run calculations for a fairly
> large
> > molecule whose net formula is VS2O3N2C17H17 (a
> total
> > of 42 atoms). The space group is P-1, with two
> > molecules per unit cell. The cell volume is ca.
> 6000
> > au^3.
> >
> > I have selected  the RMT values for V to be 1.8,
> for S
> > 1.4, for O and N 1.2, for C 1.1, and H 0.49 (these
> are
> > the maximal numbers allowed by NN program).
> >
> > With these parameters I am running into a problem
> in
> > lstart: it appears that most of the core charge
> leaks
> > out of the sphere with the separation energies
> down to
> > -10 Ry.
> 
> I believe the problem for core leakage is sulfur ?
> Can't you make its
> sphere bigger? Which atom is closest to it?
> Also H is smaller then I'm used in organic
> materials, but maybe O-H
> is that short ?
> 
> > What set of parameters would you recommend for
> this
> > case? Is it the hydrogen atoms that cause the
> problem?
> 
> H has no core, so there's no leakage.
> 
> > Is this system feasible to be treated at all (I am
> > running on a linux workstation with dual 1.8 GHz
> > Pentium Xeon processor and 1.384 Gb of RDRAM).
> 
> With 84 DIFFICULT atoms (because of small spheres)
> it is certainly
> a big calculation, but should be feasable eventually
> (start with RKmax=2.5)
> 
> Regards
>                                       P.Blaha
>
- --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna,
> A-1060 Vienna
> Phone: +43-1-58801-15671             FAX:
> +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
> http://www.tuwien.ac.at/theochem/
>
- --------------------------------------------------------------------------
> 
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====



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- --0-1700026962-1030034932=:19200
Content-Type: application/octet-stream; name="Sal50Et_frCIF.xyz"
Content-Transfer-Encoding: base64
Content-Description: Sal50Et_frCIF.xyz
Content-Disposition: attachment; filename="Sal50Et_frCIF.xyz"

NDINCk5vTmFtZSAgMC4wMDAwMDANClYgIDEuNjE1OCAgMi4zNDIzIC0wLjQz
MzYNClMgLTIuODA4NCAgMy4yOTU0ICAxLjE3NjYNClMgLTAuNzE5NSAgMi40
MTUxIC0wLjYzNTINCk8gIDEuOTcxOCAgMS4xNTMwICAwLjU3MjMNCk8gIDEu
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NDY5MyAgMy42OTYwICA0LjY4NDkNCkMgLTEuMjYzNyAgMi45NTg5ICA1Ljg1
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OTUNCkggLTMuNzg4NCAgNC43MTg4ICAyLjc0ODcNCkggIDEuNTAxNyAgNC44
NDExICAyLjUwMjQNCkggIDIuNDU3MyAgMC4yNjE5IC0zLjAwOTcNCkggIDIu
MTkyOCAtMC4yNDE1IC0xLjY0NzMNCkggIDAuNjgyNiAtMS4xOTUwIC0zLjM2
NDUNCkggIDAuMTI4MCAgMC4xNDY1IC0zLjc2NTENCkggIDAuMDY4MyAtMC4y
ODkzIC0yLjUzOTgNCkggIDUuNTgwMiAgMy43Nzg4IC0wLjUzMzENCkggIDYu
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MTQNCkggIDMuNzc5OSAgNS41ODUzICAzLjIxMzENCkggLTAuODM2MiAgNC4z
MTE5ICA0LjM3OTQNCkggLTAuNDc3OCAgMy4wMDE0ICA2LjI3MzMNCkggLTIu
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MDkNCkggLTQuMzM0NSAgMi40OTgxICAzLjg3MjUNCg==

- --0-1700026962-1030034932=:19200--
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------------------------------

Date: Thu, 22 Aug 2002 15:10:02 -0500 (CDT)
From: Anja Verena Mudring <mudring@iastate.edu>
Subject: [WIEN]: executables

====
Anja Verena Mudring <mudring@iastate.edu>
submitted the following contribution:
====

I am using the precompiled executables on a Linux PC as we do not have a f90 
compiler. Now I am meeting a problem with a structure of 52 atoms/cell.
I figure out that changing  NMATMAX  from 5000 to 10000 will help. Is that 
possible?

Regards, Anja Mudring.


Dr. Anja-Verena Mudring
Iowa State University
347 Spedding Hall
Ames, Iowa 50011
Ph.: 515 294-3513
FAX: 515 294-5718
______________

106 University Vlg Apt B
Ames, Iowa 50010
Ph.: 515 572-4931















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------------------------------

Date: Thu, 22 Aug 2002 16:44:46 -0400
From: Jeff Spirko <spirko@lehigh.edu>
Subject: [WIEN]: Bader's aim for non-symmetric atom

====
Jeff Spirko <spirko@lehigh.edu>
submitted the following contribution:
====

I want to run aim for an atom at a general position, without
symmetry.  The manual suggests using LM combinations up to 8 or even
10, but the default NCOM is 49, allowing all LM combinations only up
to 6.  

Should I Increase NCOM in many programs and recompile, then
use LM's up to 8.  If I do this, are there other parameters I have
to increase as well?  (P. Blaha suggested this in an email on 4 Oct
2001.)  If so, what other parameters must be changed?  I am using
WIEN2k_02.

Or, should I Just run it with LM's up to 6?


- -- 
Jeff Spirko   spirko@lehigh.edu   spirko@yahoo.com   WD3V   |=>

The study of non-linear physics is like the study of non-elephant biology.

All theoretical chemistry is really physics;
and all theoretical chemists know it. -- Richard P. Feynman 
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------------------------------

Date: Thu, 22 Aug 2002 20:52:16 GMT
From: "Luis Alberto Terrazos Javier" <lterrazo@fisica.ufs.br>
Subject: [WIEN]: Re: : executables

====
"Luis Alberto Terrazos Javier" <lterrazo@fisica.ufs.br>
submitted the following contribution:
====

Dear Anja
yes it is posible.
You can download the IFC intel compiler free from :
http://www.intel.com/software/products/compilers/
and change NMATMAX=10000 using ./siteconfig_lapw.
best regards
luis 

 


Anja Verena Mudring escritos: 

> ====
> Anja Verena Mudring <mudring@iastate.edu>
> submitted the following contribution:
> ==== 
> 
> I am using the precompiled executables on a Linux PC as we do not have a f90 
> compiler. Now I am meeting a problem with a structure of 52 atoms/cell.
> I figure out that changing  NMATMAX  from 5000 to 10000 will help. Is that 
> possible? 
> 
> Regards, Anja Mudring. 
> 
> 
> Dr. Anja-Verena Mudring
> Iowa State University
> 347 Spedding Hall
> Ames, Iowa 50011
> Ph.: 515 294-3513
> FAX: 515 294-5718
> ______________ 
> 
> 106 University Vlg Apt B
> Ames, Iowa 50010
> Ph.: 515 572-4931 
> 
>  
> 
>  
> 
>  
> 
>  
> 
>  
> 
>  
> 
>  
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
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------------------------------

Date: Thu, 22 Aug 2002 17:48:34 -0700 (PDT)
From: Wien Wien <wien2kny@yahoo.com>
Subject: [WIEN]: NPT and NPT00 for large systems

====
Wien Wien <wien2kny@yahoo.com>
submitted the following contribution:
====

Dear Wien users,
for a large system that I am running I am getting a
complaint from the program:

WARNING!!! For good atomic total energies you should
probably change the
radial mesh (reduce NRAD or increase R0), or increase
PARAMTERS NPT and NPT00

I have changed these parameters in the param.inc file
to
NPT=4971, NPT00=790 on a fairly arbitrary basis (I
tried several smaller values and still got a warning),
and the corresponding IPINST parameter in the dstart
source directory.

Now the program doesn't complain, but the dstart takes
a very long time with just 50 k-points (it has been
running for already 4 hours. I am afraid that the
lapw1 and lapw2 will take weeks if will be feasible at
all.

Does anyone have an idea on what the reasonable upper
limits on NPT and NPT00 should be and what approximate
ratio should I use between these two? Also, what would
be a reasonable number of k-points to start with?

My case consists of 82 atoms per unit cell, which
unfortunately won't allow for many test calculations
to establish the optimal values for the parameters.

Thank you very much for your help!
Tatyana




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------------------------------

Date: Fri, 23 Aug 2002 09:08:47 +0800
From: Wenhui Xie <xiewh@sun20.iphy.ac.cn>
Subject: [WIEN]: The parallel error, please help

====
Wenhui Xie <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear WIEN,

I meeting a problem in sheared memory parallel mode. 

The .machines files is:
granularity:1
1:tayan:4
residue:tyan:4
lapw1:tyan:4

The mpirun switch in siteconfig is:
mpirun -np 4 -machinefile .machines executable
I do not understand executable? What is it?
The computer name or program name?

When I run testpara a error message is printed:
Test: LAPW1 in parallel mode (using .machines)
Granularity set to 1
Extrafine unset
Residue set to tyan
@: Expression Syntax.
Why I get this error?

By the way, I find the parallel version is not compiled
with normal version at ame time. Because the setting of 
R_LIB (LAPACK+BLAS) must be changed from -llapack_lapw -lblas 
for normal version to  -lllapack_lapw -lblas_lapw -latals 
for parallel version.  There is anyone meet the same problem?

Thanks for any reply.

Yours 
Wenhui Xie
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------------------------------

Date: Fri, 23 Aug 2002 08:57:06 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Bug report

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>   In a calculation of  orthorhombic  alpha-U with the experimental
> parameters of ambient conditions the  force with respect to the global
> coordinate system is:
>
>      FGL01:      0.         -1.745             0.                  in
> mRy/a.u.
>
>  But if  p1/2 LO are included in the calculation the force become:
>
>     FGL01:       0.        -2567.561       0.
>
>           I think there is something  wrong  !

I expected something like this, although I haven't done any test with forces
yet.
We know that the EFG becomes wrong, when p1/2 LOs are added.
We also traced this back to a false contribution to the nonspherical
charge density but have not been able to fix this consistently yet.

At the moment I can only say that one should not use any nonspherical
quantities when using p1/2 LOs.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Fri, 23 Aug 2002 09:21:35 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: large system with hydrogens; cont'd

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I changed the RMT value for S to 2.1 (the maximum
> allowed by the NN), and this didn't solve the problem
> of the core charge leakage unfortunately. One of the

Could you tell us which atom has the core leakage ?

(Maybe you send the struct file instead of the xyz file?)

The warnings concerning NPT0,.. and the radial mesh are usually not
important and you can neglect them.

> The size of the spheres for the remaining atoms (O, C,
> N, and H is the maximum allowed by NN). The C-H bonds
> are short. I am attaching the xyz file containing the
> X-ray coordinates for this molecule just in case.

I'm not an expert for organic molecules, but the lenght of an C-H bond
must be fairly constant for all those compounds and from what I
remember it was never necessary to go below 0.6/1.2 bohr for
H and C spheres respectively!?

I expect that dstart will run for many hours and of course also
lapw1 (just one k-point!) will run for a day or so. Nevertheless, in about
a week a scf run could be possible.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Fri, 23 Aug 2002 11:07:39 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Bader's aim for non-symmetric atom

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I want to run aim for an atom at a general position, without
> symmetry.  The manual suggests using LM combinations up to 8 or even
> 10, but the default NCOM is 49, allowing all LM combinations only up
> to 6.
>
> Should I Increase NCOM in many programs and recompile, then
> use LM's up to 8.  If I do this, are there other parameters I have
> to increase as well?  (P. Blaha suggested this in an email on 4 Oct
> 2001.)  If so, what other parameters must be changed?  I am using
> WIEN2k_02.
>
> Or, should I Just run it with LM's up to 6?

My suggestion: Try to find critical points or atomic basins (with very few
directions). If it works, no need for changes, but sometimes small
discontinuities at RMT prevent proper finding of the atomic basins or
of critical points and aim runs "forever".

Also check the sigma (:FIT) in the scf file whether it is small (E-2)
or larger.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://www.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Fri, 23 Aug 2002 15:15:32 +0200
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: Oscillations with LDA+U

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

I am trying to run an LDA+U calculation on NiO in the AF II 
configuration. However, as described in the userguide, I get problems 
with oscillations during the SCF cycle. My question is: is there 
anything I do to reduce oscillations and improve convergence in the new 
Wien2k_02 mixing scheme. Will it make any difference if I reduce the 
mixing parameter and switch to Pratt mixing in case.inorb? Is perhaps 
case.inm the place where I should modify mixing? Could it help to add 
s-o coupling, as described in the userguide. I'm not primarily intersted 
in s-o effects?


Thanks for your replies.
Any suggestions are welcome!

Best reagards,
Thomas Claesson



====
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------------------------------

End of wien-digest V2002 #32
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #33
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
Errors-To: owner-wien-digest@theochem.tuwien.ac.at
Precedence: bulk


wien-digest         Friday, August 30 2002         Volume 2002 : Number 033




----------------------------------------------------------------------

Date: Fri, 23 Aug 2002 08:54:47 -0700 (PDT)
From: Wien Wien <wien2kny@yahoo.com>
Subject: Re: [WIEN]: large system with hydrogens; cont'd

====
Wien Wien <wien2kny@yahoo.com>
submitted the following contribution:
====

- --0-915341040-1030118087=:92109
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Content-Disposition: inline

Dear Dr. Blaha,
thank you very much for your response and for the
comments.

First, I found a typo in the .struct file. I apologize
for taking your time before. I am sending the correct
.struct file along. I rerun the lstart for this
file,and the result doesn't show any core charge
leakage. Now it appears that the core charge is 0 (and
the charge inside the sphere is 0 as well). Is this
reasonable? 

The C-H bond lengths are very short (most of these are
aromatic carbons), and this is probably why the sphere
radii for C and H had to be so small (1.1 and 0.49)...

Thank you very much for your help and your time
With best regards
Tatyana Polenova







__________________________________________________
Do You Yahoo!?
Yahoo! Finance - Get real-time stock quotes
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------------------------------

Date: Fri, 23 Aug 2002 19:19:04 +0200
From: Claudia Ambrosch-Draxl <claudia.ambrosch@uni-graz.at>
Subject: [WIEN]: compiler options

====
Claudia Ambrosch-Draxl <claudia.ambrosch@uni-graz.at>
submitted the following contribution:
====

Dear WIEN2k users,

I am wondering if someone has managed to compile the WIEN2k code on an
NEC or/and on a VPP. On both machines I can compile the WIEN97 version
with the f90 compiler, but not the new version. 

Best regards,
Claudia

- -- 
Claudia Ambrosch-Draxl
Institut f. Theoretische Physik, University Graz
Universitaetsplatz 5, A-8010 Graz
Tel. [43] (316) 380-5235    Fax [43] (316) 380-9820
http://physik.uni-graz.at/~cad
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------------------------------

Date: Mon, 26 Aug 2002 13:32:18 +0200 (SAST)
From: "Dr. K.Osuch" <osuchk@harry.unisa.ac.za>
Subject: [WIEN]: Bug in spaghetti?

====
"Dr. K.Osuch" <osuchk@harry.unisa.ac.za>
submitted the following contribution:
====

There seams to be a bug in the new spaghetti. When one tries to obtain
a character band structure by setting 'jatom ne 0', the band structure
does not show any contribution from the chosen orbitals. The *.ps
structure shows atom=0, independently on what one gives in the *.insp file.
This can be traced back to inview.f file in SRC_spaghetti, where there is a 
line:

   if(iprto(1).eq.0) jatom_list(jatom+1)=0


which sets jatom_list=0 if we want to have the band structure drawn with
dotted lines. I do not know hat the reason was to have this condition in 
inview.f. Commenting out this line helps - the character band structure is 
created then with dots and circles. However if one changes line switch to 1 
(lines), again no character is shown in *.ps. 


K. Osuch

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------------------------------

Date: Mon, 26 Aug 2002 15:54:16 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Bug in spaghetti?

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> There seams to be a bug in the new spaghetti. When one tries to obtain
> a character band structure by setting 'jatom ne 0', the band structure
> does not show any contribution from the chosen orbitals. The *.ps
> structure shows atom=0, independently on what one gives in the *.insp file.
> This can be traced back to inview.f file in SRC_spaghetti, where there is a
> line:
>
>    if(iprto(1).eq.0) jatom_list(jatom+1)=0
>
>
> which sets jatom_list=0 if we want to have the band structure drawn with
> dotted lines. I do not know hat the reason was to have this condition in
> inview.f. Commenting out this line helps - the character band structure is
> created then with dots and circles. However if one changes line switch to 1
> (lines), again no character is shown in *.ps.

I don't know if its a bug or a "feature":

The "character-plot" works if the line switch is set to 2 or 3 (and this was
our intention).

You are right, without the modification you suggested above, it is not
possible to produce the same plot as with the "old" spaghetti.

So maybe it is a good idea to make this change.

Any comments ? I hope it works in all cases.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 26 Aug 2002 14:52:13 -0700 (PDT)
From: Michelle Johannes <johannes@maugre.ucdavis.edu>
Subject: [WIEN]: KPT problem

====
Michelle Johannes <johannes@maugre.ucdavis.edu>
submitted the following contribution:
====

Dear Wien users:
	I am trying to look at the band structure for a compound which I
calculated with both spin-orbit and with an added U.  After calculating a
converged charge density, I performed the following steps:

x lapw1 -up
x lapw1 -dn
x lapwso -up -orb

Then I tried x lapw2 -c -so -up -qtl and got this message:
NKPT TOO SMALL

In case.output2up it gives:
NUMBER OF K-POINTS .GT. NKPT =            52

My actual number of k-pts in case.in1 is 51.  x lapw2 -up -qtl works fine
i.e. it finds the correct number of kpts, so I guess the problem is maybe
with the spin-orbit or complex implementation.

	I have tried reducing the number of k-pts I calculate, but lapw2
always wants one more than I have.  I have not attached any files because
the problem does not seem to me to be specific to my compound, but I can
send them along if it would help.


	Thanks for any input,
		Michelle

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------------------------------

Date: Tue, 27 Aug 2002 10:37:49 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: KPT problem

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> x lapw1 -up
> x lapw1 -dn
> x lapwso -up -orb
>
> Then I tried x lapw2 -c -so -up -qtl and got this message:
> NKPT TOO SMALL
>
> In case.output2up it gives:
> NUMBER OF K-POINTS .GT. NKPT =            52
>
> My actual number of k-pts in case.in1 is 51.  x lapw2 -up -qtl works fine
> i.e. it finds the correct number of kpts, so I guess the problem is maybe
> with the spin-orbit or complex implementation.

The problem is that a "runsp -so" command does not only perform the tree
steps you made at the top of this message, but also copies
     cp $file.energydum $file.energydumup
     cp $file.energydum $file.energydumdn
before running    x lapw2 -c -so -up -qtl

Maybe you want to use     runsp -so -s lapw1 -e lapwso

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 27 Aug 2002 13:00:02 +0100
From: "Xiangyuan Cui" <x.cui@pgr.salford.ac.uk>
Subject: [WIEN]: Ask help for Spin-coupling calculation

====
"Xiangyuan Cui" <x.cui@pgr.salford.ac.uk>
submitted the following contribution:
====

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Dear wien2k users:

I am convinced that spin-orbital coupling is vital to determine the =
magnetic ground state in YCO3 compound.
Unfortunately, I could not set up SO calculation properly.  I wonder if =
anybody is kind enough to point out my=20
errors in the below procedures:

1. normal runsp_lapw converged.
2. initso_lapw:
edit *.inso and *.in1:=20
the magnetization direction is 0001 for hexadral, I used 0 0 1, rather 0 =
0 0 1, Emax=3D5.5
please see the attached file *.inso and *.in1,
3. then ask" Do you have a spinpolarised case(and want to run symmetso)? =
- ---choose "y" and *.outsymso is created.
 the number of symmetry operation changed from 12 to 4.
4. " Do you want to use the ew struct for SO cal.?" ---choose "y"
     " all inversion? " choose No=3D0
     " k-poits" --400, short output and k-mesh shift allowed.
now it says: "Spinorbit is now ready to run"

But "run_lapw -so" crashed immediately and give "Fortune stop" and in =
the *.outputso says: "error in struct file read".
also attached is the two structure file, one is for normal s-p =
calculation, the other one is created by initso.

Thanks a lot in advance for your kindness and I wish you all the best!

Xiangyuan CUI

PhD student, Joule Lab, University of Salford, UK


=20


  =20


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<DIV><FONT face=3DArial size=3D2>Dear wien2k users:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>I am convinced that spin-orbital =
coupling is vital=20
to determine the magnetic ground state in YCO3 compound.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Unfortunately, I could not set up SO =
calculation=20
properly.&nbsp; I wonder if anybody&nbsp;is kind enough to point out my=20
</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>errors in the below =
procedures:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>1.&nbsp;normal runsp_lapw =
converged.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>2. initso_lapw:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>edit *.inso and *.in1: </FONT></DIV>
<DIV><FONT face=3DArial size=3D2>the magnetization direction is 0001 for =
hexadral, I=20
used 0 0 1, rather 0 0 0 1, </FONT><FONT face=3DArial =
size=3D2>Emax=3D5.5</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>please see the attached file *.inso and =

*.in1,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>3. then ask" Do you have a =
spinpolarised case(and=20
want to run symmetso)? ---choose "y" and *.outsymso is =
created.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>&nbsp;the number of symmetry operation =
changed from=20
12 to 4.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>4. " Do you want to use the ew struct =
for SO cal.?"=20
- ---choose "y"</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>&nbsp;&nbsp;&nbsp;&nbsp; " all =
inversion? " choose=20
No=3D0</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>&nbsp;&nbsp;&nbsp;&nbsp; " k-poits" =
- --400, short=20
output and k-mesh shift allowed.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>now it says: "Spinorbit is now ready to =

run"</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>But "run_lapw -so" crashed immediately =
and give=20
"Fortune stop" and&nbsp;in the *.outputso says: "error in&nbsp;struct =
file=20
read".</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>also attached is the two structure =
file, one is for=20
normal s-p calculation, the other one is created by initso.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Thanks a lot in advance for your =
kindness and I=20
wish you all the best!</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Xiangyuan CUI</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>PhD student, Joule Lab, University of =
Salford,=20
UK</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV>&nbsp;<FONT face=3DArial size=3D2>&nbsp;&nbsp;</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2><BR>---<BR>Outgoing mail is certified =
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Virus Database: 211 - Release Date: =
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WFFIL        (WFPRI, SUPWF)=0A=
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  0.30    4  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global =
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 1    0.30      0.000 CONT 1                                             =
      =0A=
 1   -4.57      0.005 STOP 1                                             =
      =0A=
 2    0.30      0.010 CONT 1                                             =
      =0A=
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      =0A=
  0.30    4  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global =
APW/LAPW) =0A=
 1    0.30      0.000 CONT 1                                             =
      =0A=
 1   -4.57      0.005 STOP 1                                             =
      =0A=
 2    0.30      0.010 CONT 1                                             =
      =0A=
 0    0.30      0.000 CONT 1                                             =
      =0A=
K-VECTORS FROM UNIT:4   -7.0       5.5      emin/emax window             =
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WFFIL=0A=
 10  0  0                      llmax,ipr,kpot =0A=
 -10.0000   5.50000           emin,emax (output energy window)=0A=
   0.  0.  1.                 direction of magnetization (lattice =
vectors)=0A=
 0                           number of atoms for which RLO is added=0A=
 0   -3.23      0.005  STOP     atom number,e-lo,de (case.in1), repeat =
NX times=0A=
 0   -3.23      0.005  STOP=0A=
 1   -4.57      0.005  STOP=0A=
 1   -4.34      0.005  STOP=0A=
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Ferri-test                                                               =
      =0A=
R   LATTICE,NONEQUIV. ATOMS: 5166_R-3m                                   =
      =0A=
MODE OF CALC=3DRELA unit=3Dbohr                                          =
          =0A=
  9.490000  9.490000 46.130000 90.000000 90.000000120.000000             =
      =0A=
ATOM=3D -1: X=3D0.00000000 Y=3D0.00000000 Z=3D0.00000000=0A=
          MULT=3D 1          ISPLIT=3D 4=0A=
Y 1        NPT=3D  781  R0=3D0.00010000 RMT=3D    2.5000   Z: 39.0       =
            =0A=
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000=0A=
                     0.0000000 1.0000000 0.0000000=0A=
                     0.0000000 0.0000000 1.0000000=0A=
ATOM=3D -2: X=3D0.86010600 Y=3D0.86010600 Z=3D0.86010600=0A=
          MULT=3D 2          ISPLIT=3D 4=0A=
      -2: X=3D0.13989400 Y=3D0.13989400 Z=3D0.13989400=0A=
Y 2        NPT=3D  781  R0=3D0.00010000 RMT=3D    2.5000   Z: 39.0       =
            =0A=
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000=0A=
                     0.0000000 1.0000000 0.0000000=0A=
                     0.0000000 0.0000000 1.0000000=0A=
ATOM=3D -3: X=3D0.50000000 Y=3D0.50000000 Z=3D0.50000000=0A=
          MULT=3D 1          ISPLIT=3D 4=0A=
Co1        NPT=3D  781  R0=3D0.00010000 RMT=3D    2.3000   Z: 27.0       =
            =0A=
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000=0A=
                     0.0000000 1.0000000 0.0000000=0A=
                     0.0000000 0.0000000 1.0000000=0A=
ATOM=3D -4: X=3D0.66540300 Y=3D0.66540300 Z=3D0.66540300=0A=
          MULT=3D 2          ISPLIT=3D 4=0A=
      -4: X=3D0.33459700 Y=3D0.33459700 Z=3D0.33459700=0A=
Co2        NPT=3D  781  R0=3D0.00010000 RMT=3D    2.3000   Z: 27.0       =
            =0A=
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000=0A=
                     0.0000000 1.0000000 0.0000000=0A=
                     0.0000000 0.0000000 1.0000000=0A=
ATOM=3D -5: X=3D0.91868500 Y=3D0.41857000 Z=3D0.41857000=0A=
          MULT=3D 6          ISPLIT=3D 8=0A=
      -5: X=3D0.08131500 Y=3D0.58143000 Z=3D0.58143000=0A=
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      -5: X=3D0.58143000 Y=3D0.08131500 Z=3D0.58143000=0A=
Co3        NPT=3D  781  R0=3D0.00010000 RMT=3D    2.3000   Z: 27.0       =
            =0A=
LOCAL ROT MATRIX:    0.0000000 0.5000000 0.8660254=0A=
                     0.0000000-0.8660254 0.5000000=0A=
                     1.0000000 0.0000000 0.0000000=0A=
  12      NUMBER OF SYMMETRY OPERATIONS=0A=
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Ferri-test                               s-o calc. M||  0.00  0.00  1.00 =
      =0A=
R                            6 66_R                                      =
      =0A=
             RELA                                                        =
      =0A=
  9.490000  9.490000 46.130000 90.000000 90.000000120.000000             =
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                     0.0000000 0.0000000 1.0000000=0A=
                     1.0000000 0.0000000 0.0000000=0A=
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       4   B  10=0A=

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------------------------------

Date: Tue, 27 Aug 2002 16:16:25 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: [WIEN]: lstart complaining about "good atomic total energies"

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Wien users,

for some cases with small RMT I get the following warning from lstart 
during initialization:

WARNING !!!! For good atomic total energies you should probably
change the radial mesh (reduce NRAD or increase R0), or increase 
PARAMETERS NPT
and NPT00

Since none of the scf-cycle programs contains the NPT and NPT00 
parameters, does this actually mean anything to the result coming out 
after scf?

And yes, I can make them disappear, but can I safely ignore that 
warning, too?

Best regards,
Torsten Andersen.

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics


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------------------------------

Date: Tue, 27 Aug 2002 13:13:06 -0700 (PDT)
From: Michelle Johannes <johannes@maugre.ucdavis.edu>
Subject: Re: [WIEN]: KPT problem

====
Michelle Johannes <johannes@maugre.ucdavis.edu>
submitted the following contribution:
====

	Thank you, Peter.  Copying the files by hand worked
perfectly.  However, the suggestion to use some limited part of the runsp
script seems not to work. Perhaps asking it to stop after lapwso does not
allow it to get to the part of the script where the .energydum files are
copied?  In any case, one working method is quite enough for me - thanks.

	Michelle



On Tue, 27 Aug 2002, Peter Blaha wrote:

> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> > x lapw1 -up
> > x lapw1 -dn
> > x lapwso -up -orb
> >
> > Then I tried x lapw2 -c -so -up -qtl and got this message:
> > NKPT TOO SMALL
> >
> > In case.output2up it gives:
> > NUMBER OF K-POINTS .GT. NKPT =            52
> >
> > My actual number of k-pts in case.in1 is 51.  x lapw2 -up -qtl works fine
> > i.e. it finds the correct number of kpts, so I guess the problem is maybe
> > with the spin-orbit or complex implementation.
> 
> The problem is that a "runsp -so" command does not only perform the tree
> steps you made at the top of this message, but also copies
>      cp $file.energydum $file.energydumup
>      cp $file.energydum $file.energydumdn
> before running    x lapw2 -c -so -up -qtl
> 
> Maybe you want to use     runsp -so -s lapw1 -e lapwso
> 
> Regards
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
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------------------------------

Date: Wed, 28 Aug 2002 08:27:21 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: lstart complaining about "good atomic total energies"

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> for some cases with small RMT I get the following warning from lstart
> during initialization:
>
> WARNING !!!! For good atomic total energies you should probably
> change the radial mesh (reduce NRAD or increase R0), or increase
> PARAMETERS NPT
> and NPT00
>
> Since none of the scf-cycle programs contains the NPT and NPT00
> parameters, does this actually mean anything to the result coming out
> after scf?
>
> And yes, I can make them disappear, but can I safely ignore that
> warning, too?

It gives not only a warning, but also tells you how far the radial mesh
reaches. If it is a "reasonable" value (a little smaller than 15 bohr, but
this depends on the kind of atom), then there is absolutely no problem.
If this maximum r-value is very small (e.g. below 10 bohr for a heavier
element), it might happen that the resulting atomic densities are so poor
that you get problems in the scf cycle.

However, in general I believe you can savely ignore these warnings with
respect to the scf calculation (not for an accurate atomic total energy).

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 28 Aug 2002 10:41:02 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: [WIEN]: DOS in spin.pol SO calculation

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

Dear Wien users,

The total spin-up / dn DOS could not be calculated in a spinpolarized
spin-orbit calculation (since each qtlup/dn file contains all eigenvalues.

We write now into case.qtlup/dn the up and dn-spin "norm" of each
eigenvalue into case.qtlup (at the position of "q-interstital", which was
not correct anyway in SO calculations)

TETRA reads now in spinpol. SO cases (only then) for the "total DOS" these
norms and produces a spin-up or dn total DOS.

See: www.wien2k.at/reg_user/updates

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Wed, 28 Aug 2002 10:58:12 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: lstart complaining about "good atomic total energies"

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Peter,

thank you for the answer. Does this mean that if I later (after the scf 
cycle) need an accurate atomic total energy, I can just change the 
radial mesh in lstart and rerun lstart? Or does the atomic total energy 
also influence the total energy in the scf cycle (which to my 
understanding of "full-potential" it should not)?

Best regards,
Torsten Andersen.

Peter Blaha wrote:

>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
>>for some cases with small RMT I get the following warning from lstart
>>during initialization:
>>
>>WARNING !!!! For good atomic total energies you should probably
>>change the radial mesh (reduce NRAD or increase R0), or increase
>>PARAMETERS NPT
>>and NPT00
>>
>>Since none of the scf-cycle programs contains the NPT and NPT00
>>parameters, does this actually mean anything to the result coming out
>>after scf?
>>
>>And yes, I can make them disappear, but can I safely ignore that
>>warning, too?
>>
>
>It gives not only a warning, but also tells you how far the radial mesh
>reaches. If it is a "reasonable" value (a little smaller than 15 bohr, but
>this depends on the kind of atom), then there is absolutely no problem.
>If this maximum r-value is very small (e.g. below 10 bohr for a heavier
>element), it might happen that the resulting atomic densities are so poor
>that you get problems in the scf cycle.
>
>However, in general I believe you can savely ignore these warnings with
>respect to the scf calculation (not for an accurate atomic total energy).
>
>Regards
>
>
>                                      P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
>====
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>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Wed, 28 Aug 2002 11:26:52 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: lstart complaining about "good atomic total energies"

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> thank you for the answer. Does this mean that if I later (after the scf
> cycle) need an accurate atomic total energy, I can just change the
> radial mesh in lstart and rerun lstart? Or does the atomic total energy
> also influence the total energy in the scf cycle (which to my
> understanding of "full-potential" it should not)?

No, of course the atomic total energy does not influence E-tot of the
scf cycle (unless you have such a bad starting density that the scf cycle
doesnot converge, see my previous comment),

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 29 Aug 2002 16:32:55 +0800
From: joshua xie <joshuaxie@etang.com>
Subject: [WIEN]: one question about case.in2

====
joshua xie <joshuaxie@etang.com>
submitted the following contribution:
====

Dear wien user£¬

    In file 'case.in2', there is a parameter 'ne'. How to determine its value in the energy range from 'emin' to 'eval' if I set 'efmod' to 'ALL'?
¡¡¡¡
Thank you very much!
¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡

Best regards! 				
Joshua Xie.

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------------------------------

Date: Thu, 29 Aug 2002 11:28:46 +0200 (MESZ)
From: "A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
Subject: Re: [WIEN]: one question about case.in2

====
"A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
submitted the following contribution:
====

On Thu, 29 Aug 2002, joshua xie wrote:

> ====
> joshua xie <joshuaxie@etang.com>
> submitted the following contribution:
> ====
> 
> Dear wien user£¬
> 
>     In file 'case.in2', there is a parameter 'ne'. How to determine its value in the energy range from 'emin' to 'eval' if I set 'efmod' to 'ALL'?


I'd guess, NE is only important for the Fermi energy search,
to let the program know how many electrons there are in the occupied bands.
With efmod = ALL, there is no Fermi search, so NE probably has no effect.

(But you shouldnn't use this option in the course of iterations,
only for extractig bands / DOS / charge density!)

Good luck,

Adrei Postnikov

+----------------------------------------------------------------------------+
| Dr. habil. Andrei Postnikov                    postnik@thp.uni-duisburg.de | 
| Gerhard Mercator Universitaet Duisburg - Theoretische Tieftemperaturphysik |
| D-47048 Duisburg          Tel. +49-203-3791608        Fax  +49-203-3793665 |
+----------------------------------------------------------------------------+

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------------------------------

Date: Thu, 29 Aug 2002 14:50:52 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Ask help for Spin-coupling calculation

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---2105530234-1656175879-1030625452=:22620
Content-Type: TEXT/PLAIN; charset=US-ASCII

> I am convinced that spin-orbital coupling is vital to determine the magnetic ground state in YCO3 compound.
> Unfortunately, I could not set up SO calculation properly.  I wonder if anybo

Hi,
It is not really your fault.

If you look into your newly created struct file, you will see that the atoms
number 1 and 3 are missing!!    Thus the error in the so-scf.

The reason for that is a bug in symmetso, which used an old   class.f
subroutine with a few errors.

I have fixed and updated SRC_symmetso on the web.

I also include a correct struct file for SO calculations.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 29 Aug 2002 10:21:48 -0400 (EDT)
From: Neme Nnolim <non6886@alizarin.njit.edu>
Subject: Re: [WIEN]: Ask help for Spin-coupling calculation

====
Neme Nnolim <non6886@alizarin.njit.edu>
submitted the following contribution:
====


Is the SRC_symmetso update valid for all WIEN97 versions, or just WIEN2k?
I use WIEN97.10.

>
> Hi,
> It is not really your fault.
>
> If you look into your newly created struct file, you will see that the atoms
> number 1 and 3 are missing!!    Thus the error in the so-scf.
>
> The reason for that is a bug in symmetso, which used an old   class.f
> subroutine with a few errors.
>
> I have fixed and updated SRC_symmetso on the web.
>
> I also include a correct struct file for SO calculations.
>

- ------------------------------------------------------------------------------
Neme Okechukwu Nnolim
Department of Materials Science, New Jersey Institute of Technology
Room 302, Tiernan Hall, 161 Warren Street, University Heights
Newark, New Jersey 07102-1982
Tel: (973) 596-8283, FAX: (973) 596-5794
- -------------------------------------------------------------------------------


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------------------------------

Date: Thu, 29 Aug 2002 16:24:38 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Ask help for Spin-coupling calculation

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Is the SRC_symmetso update valid for all WIEN97 versions, or just WIEN2k?
> I use WIEN97.10.

SRC_symmetso is not part of WIEN97. It is new in WIEN2k.


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 29 Aug 2002 21:12:41 +0200
From: Liang Ching-Tarng <liangc@physik.fu-berlin.de>
Subject: [WIEN]: Wien and/or SpaceGroups

====
Liang Ching-Tarng <liangc@physik.fu-berlin.de>
submitted the following contribution:
====

Sehr geehrter Herr Blaha,

ich schreibe gleich mal auf deutsch, denn ich denke, daß dieses Problem
trivial und nicht von allgemeinen Interesse ist...

Wir möchten NiO nachrechnen wegen LDA+U. Die antiferromagnetische 
Ordnung reduziert dieses kubische NaCl-System zu einem rhomboedrischen
System, analog zu LiNiO2 mit der Raumgruppe R-3m (166). Der
Kristallographischen Konvention folgend würde man
   a  und alpha eingeben, oder a = b = c  und alpha = beta = gamma,
wobei a_rhom = sqrt(3/2)*a_cub (a_cub = 4.1648 AA) und alpha = 35.56
(cos(alpha) = 5/6 für eine kubische Struktur) sind.

Für die Koordinaten hätte man nach Wyckoff
Ni_1  (0,0,0)
Ni_2  (1/2,1/2,1/2)
0     (1/4,1/4,1/4)   [(3/4, 3/4, 3/4) braucht man nicht anzugeben, weil 
diese Position äquivalent ist mit R-3m]

Ihre Eingabe ist im hexagonalen Systsem, mit Ihren Formeln im WienCode
Handbuch ergibt sich
a_hex = 5.6440 AA und c_hex = 14.440 AA, also eine sehr länglich 
hexagonale Zelle.

Als Eingabe setzt man
b_hex = 0 (???), die Winkel setzt man alle Null??

Dann sagt das Handbuch weiter (Kap. 4.3): man solle als Position den 
Wyckhoffpositionen einsetzen, und zwar für das rhomboedrische System.
Aber wie soll das zusammenpassen? Muß nicht alles konvertieren ins
hexagonale? Ihr Hilfsprogramm hex2rhomb macht aber genau das umgekehrte?
Die Internationale Tabellen und auch Wyckhoff geben auch die hexagonalen
Positionen an.

Ich kann das nicht verstehen, weil das Programm die Eingaben automatisch
ändert. Wenn man es selber die Gruppe suchen läßt, beschwert es sich
das Sauerstoff zweimal da ist, aber es findet schon R-3m = 166!

Gibt es nicht für das NiO ein wie für TiC ein Beispiel-File, den wir
übernehmen können?

Grüße und vielen Dank

C.T. Liang und D. Schotte




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------------------------------

Date: Fri, 30 Aug 2002 12:04:29 +0800
From: Wenhui Xie <xiewh@sun20.iphy.ac.cn>
Subject: [WIEN]: Stop at lapw2 of cycle 2

====
Wenhui Xie <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear WIEN Users,

I get a problem of wien2k. The program stop at :

in cycle 2    ETEST: 0   CTEST: 0
GETARG: argument index (2) out of range
FORTRAN STOP  LAPW0 END
GETARG: argument index (2) out of range
FORTRAN STOP  LAPW1 END
GETARG: argument index (2) out of range
FORTRAN STOP  LAPW1 END
GETARG: argument index (2) out of range
FORTRAN STOP  LAPW2 END
GETARG: argument index (2) out of range
FORTRAN STOP  LAPW2 END
GETARG: argument index (2) out of range

Input/Output Error 148: Invalid character
   In Procedure: insld
        At Line: 95
      Statement: Formatted READ
           Unit: 20
   Connected To: crte_wz.struct
           Form: Formatted
         Access: Sequential
Records Read   : 19
Records Written: 0
Current I/O Buffer:
  12      NUMBER OF SYMMETRY OPERATIONS
            !
End of diagnostics

	
Would you please to tell me what's wrong with it?

Yours sincerely
Wenhui Xie
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------------------------------

Date: Fri, 30 Aug 2002 08:35:39 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Wien and/or SpaceGroups

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---2105530234-1332553899-1030689339=:555
Content-Type: TEXT/PLAIN; charset=US-ASCII

Lieber Hr.Liang

Natuerlich haben wir NiO schon oft gerechnet, es ist ja DAS Paradebeispiel
fuer LDA+U. Struct file liegt bei.

Die Eingabe in WIEN ist for R Gitter wirklich sehr inkonsistent, daher habe ich
auch versucht, sie so genau wie moeglich zu beschreiben.
Es stimmt tatsaechlich: Sie muessen die "hexagonalen" Gitterkonstanten
verwenden, aber die "rhomboedrischen"" Positionen. Das ist, zugegebenermassen,
komplett inkonsistent, denn wie sie sagten, entweder sollte man alles im
R-setting, oder alles im H setting machen.
Leider nicht so programmiert!

MfG


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

- ---2105530234-1332553899-1030689339=:555
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- ---2105530234-1332553899-1030689339=:555--
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------------------------------

Date: Fri, 30 Aug 2002 08:41:56 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Stop at lapw2 of cycle 2

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I get a problem of wien2k. The program stop at :
>
> in cycle 2    ETEST: 0   CTEST: 0
> GETARG: argument index (2) out of range
> FORTRAN STOP  LAPW0 END
> GETARG: argument index (2) out of range
> FORTRAN STOP  LAPW1 END
> GETARG: argument index (2) out of range
> FORTRAN STOP  LAPW1 END
> GETARG: argument index (2) out of range
> FORTRAN STOP  LAPW2 END
> GETARG: argument index (2) out of range
> FORTRAN STOP  LAPW2 END
> GETARG: argument index (2) out of range
>
> Input/Output Error 148: Invalid character
>    In Procedure: insld
>         At Line: 95
>       Statement: Formatted READ
>            Unit: 20
>    Connected To: crte_wz.struct
>            Form: Formatted
>          Access: Sequential
> Records Read   : 19
> Records Written: 0
> Current I/O Buffer:
>   12      NUMBER OF SYMMETRY OPERATIONS
>             !
> End of diagnostics
>
>
> Would you please to tell me what's wrong with it?

It's like a quizz game. Give him just a little bit of information and maybe he
knows the answer!

insld is part of LCORE, so the program stops in lcore. I guess it happens
since it would find a positive energy for one of the core orbitals.

The reasons for this I can again only speculate:
a) You do an "open core" calculation for 4f states ? Increase the shift
b) Your input/ struct file is wrong. Check :NEC01 in your scf file.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Fri, 30 Aug 2002 15:09:37 +0200
From: Enrique Lomba <E.Lomba@iqfr.csic.es>
Subject: [WIEN]: How to set sensible choices for El in case.in1

====
Enrique Lomba <E.Lomba@iqfr.csic.es>
submitted the following contribution:
====

Hello again,
I am trying (desperately) to run a calculation for Trigonal Te, and 
consistently I am getting the message

  QTL-B VALUE .EQ.    5.22752   !!!!!!

in case.scf. From the manual I understand that this is not necesarly the 
result of a ghost band, but from the fact that linearization has reached 
its limit. I have tried to fiddle around with the El values in case.in1 
adding local orbital.... where can I find some guidelines to set this 
values. Here is one of the case.in1c files I used

WFFIL        (WFPRI, SUPWF)
   7.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
   0.30    5  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global 
APW/LAPW)
  0   -2.19      0.020 CONT 0
  0    0.30      0.000 CONT 0
  1   -1.00      0.020 CONT 0
  1    0.30      0.000 CONT 0
  2    0.80      0.020 CONT 1
K-VECTORS FROM UNIT:4   -7.0       1.5      emin/emax window



and here part of the .scf file

- ---------------------------

           ATOMIC SPHERE DEPENDENT PARAMETERS FOR ATOM  Te
           OVERALL ENERGY PARAMETER IS    0.3000
           OVERALL BASIS SET ON ATOM IS LAPW
           E( 0)=   -2.1900   E(BOTTOM)=   -2.520   E(TOP)=   -1.860
              LAPW
           E( 0)=    0.3000
              LOCAL ORBITAL
           E( 1)=   -1.0000   E(BOTTOM)=   -1.540   E(TOP)=   -0.460
              LAPW
           E( 1)=    0.3000
              LOCAL ORBITAL
           E( 2)=    0.8200   E(BOTTOM)=   -0.120   E(TOP)=    1.760
              APW+lo

        K=   0.00000   0.00000   0.00000            1
:RKM  : MATRIX SIZE  240LOs:  27  RKM= 6.92  WEIGHT= 1.00  PGR:
        EIGENVALUES ARE:
         -2.2046804   -2.1377468   -2.1377468   -1.1229720   -1.1229720
         -1.0307893   -0.9778829   -0.9621835   -0.9621835   -0.9192676
         -0.9013458   -0.9013458    0.1820136    0.1887096    0.1887096
          0.2575385    0.2575385    0.2906676    0.3706620    0.3931053
          0.3931053    0.6095509    0.6095509    0.6174805    0.7357479
          0.7707214    0.7707214    0.7788895    0.7919586    0.7919587
          0.9677639    0.9677639    1.1485932    1.2769433    1.2769433
          1.3612111    1.4291974    1.4291974
        ********************************************************

        NUMBER OF K-POINTS:          149
:GMA  : POTENTIAL AND CHARGE CUT-OFF  14.00 Ry**.5
         Energy to separate semicore and valencestates:   0.08584


:NOE  : NUMBER OF ELECTRONS          =  48.000

:FER  : F E R M I - ENERGY(TETRAH.M.)=   0.61477
:POS01: AT.NR. -1  POSITION = 0.26400 0.00000 0.33333  MULTIPLICITY =  3

        LMMAX=25
        LM=  0 0 1 0 2 0 2 2-2 2 3 0 3 2-3 2 4 0 4 2-4 2 4 4-4 4 5 0 5 
2-5 2 5 4
        -5 4 6 0 6 2-6 2 6 4-6 4 6 6-6 6 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 
0 0 0 0
  0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0

:CHA01: TOTAL CHARGE INSIDE SPHERE   1 =    14.757799
:PCS01: PARTIAL CHARGES SPHERE =  1 
S,P,D,F,PX,PY,PZ,D-Z2,D-X2Y2,D-XY,D-XZ,D-YZ
:QTL01: 2.0778 5.5987 6.9971 0.0681 1.8906 1.8453 1.8628 1.2472 1.0846 
1.2167 1.1035 2.3451
         Q-s-low E-s-low   Q-p-low E-p-low   Q-d-low E-d-low   Q-f-low 
E-f-low
:EPL01:  1.9397 -2.1525    5.4135 -0.9915    0.1575 -1.0932    0.0082 
- -1.1322
         Q-s-hi  E-s-hi    Q-p-hi  E-p-hi    Q-d-hi  E-d-hi    Q-f-hi 
E-f-hi
:EPH01:  0.1381  0.3861    0.1853  0.4142    6.8396  0.3981    0.0599 
0.4306

                       QXX         QXY         QYY         QZZ       UP TO R

:VZZ01:            58.79488   -13.59220   -28.30246   -30.49242       2.670

:CHA  : TOTAL CHARGE INSIDE UNIT CELL =      48.000000

:SUM  : SUM OF EIGENVALUES =            -21.520219



    QTL-B VALUE .EQ.    5.22752   !!!!!!



Any help would be appreciated !!!

		Regards,
				Enrique





- -- 
- --------------------------------------------------------------
Enrique Lomba
Instituto de Quimica Fisica Rocasolano, CSIC
C/ Serrano 119, 28006 Madrid, Spain

FAX no. 34-915642431
Phone no. 34-915619407 (ext 1301)
e-mail : E.Lomba@iqfr.csic.es
www : http://www.fluid.iqfr.csic.es/enrique.html

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------------------------------

Date: Fri, 30 Aug 2002 11:05:48 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: Wien and/or SpaceGroups

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

Liebe Herren,

Meine Meinung nach, if you had a problem, there is a
good chance somebody else may, too. Furthermore, since
you do not know the solution, you cannot judge how
trivial it is. This is the whole idea of the mailing
list! Otherwise you could as well write Peter
privately. I refer, of course to your writing in
German (I personally have no problem reading German,
but others may).
 
More to the point, I'd like to raise another question,
pertinent probably to the future releases. In another
popular code, Stuttgart LMTO, the user has a
possibility to describe the unit cell in Cartesian
coordinates as three vectors rather than as three
lengths and three angles. For instance, the AFL NIO
unit cell would be 
a/2 a/2 a
a/2 a 1/2
a a/2 a/2
I found that extremely convenient for doing reduced
symmetry supercells. It looks to me, naively, that
this should be quite a small addition to the existing
code. Did you ever thought about adding such an
option?

Igor 
- --- Peter Blaha <pblaha@theochem.tuwien.ac.at> wrote:
> Lieber Hr.Liang
> 
> Natuerlich haben wir NiO schon oft gerechnet, es ist
> ja DAS Paradebeispiel
> fuer LDA+U. Struct file liegt bei.
> 
> Die Eingabe in WIEN ist for R Gitter wirklich sehr
> inkonsistent, daher habe ich
> auch versucht, sie so genau wie moeglich zu
> beschreiben.
> Es stimmt tatsaechlich: Sie muessen die
> "hexagonalen" Gitterkonstanten
> verwenden, aber die "rhomboedrischen"" Positionen.
> Das ist, zugegebenermassen,
> komplett inkonsistent, denn wie sie sagten, entweder
> sollte man alles im
> R-setting, oder alles im H setting machen.
> Leider nicht so programmiert!
> 
> MfG
> 
> 
>                                       P.Blaha
>
- --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna,
> A-1060 Vienna
> Phone: +43-1-58801-15671             FAX:
> +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
> http://info.tuwien.ac.at/theochem/
>
- --------------------------------------------------------------------------
> > NiO                                               
 
>                           
> R   LATTICE,NONEQUIV. ATOMS: 3                      
>                           
> MODE OF CALC=RELA                                   
>                           
>   5.605236  5.605236 27.459934 90.000000 90.000000
> 90.000000                   
> ATOM= -1: X=0.00000000 Y=0.00000000 Z=0.00000000
>           MULT= 1          ISPLIT= 8
> Ni1        NPT=  381  R0=0.00050000 RMT=    2.3000  
> Z: 28.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM= -2: X=0.50000000 Y=0.50000000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Ni2        NPT=  381  R0=0.00050000 RMT=    2.3000  
> Z: 28.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM= -3: X=0.25000000 Y=0.25000000 Z=0.25000000
>           MULT= 2          ISPLIT= 8
>       -3: X=0.75000000 Y=0.75000000 Z=0.75000000
> O          NPT=  381  R0=0.00050000 RMT=    1.6500  
> Z:  8.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
>   12     NUMBER OF SYMMETRY OPERATIONS
>  1 0 0 0.0000000
>  0 1 0 0.0000000
>  0 0 1 0.0000000
>        1
>  1 0 0 0.0000000
>  0 0 1 0.0000000
>  0 1 0 0.0000000
>        2
>  0 1 0 0.0000000
>  1 0 0 0.0000000
>  0 0 1 0.0000000
>        3
>  0 0 1 0.0000000
>  1 0 0 0.0000000
>  0 1 0 0.0000000
>        4
>  0 1 0 0.0000000
>  0 0 1 0.0000000
>  1 0 0 0.0000000
>        5
>  0 0 1 0.0000000
>  0 1 0 0.0000000
>  1 0 0 0.0000000
>        6
>  0 0-1 0.0000000
>  0-1 0 0.0000000
> -1 0 0 0.0000000
>        7
>  0-1 0 0.0000000
>  0 0-1 0.0000000
> -1 0 0 0.0000000
>        8
>  0 0-1 0.0000000
> -1 0 0 0.0000000
>  0-1 0 0.0000000
>        9
>  0-1 0 0.0000000
> -1 0 0 0.0000000
>  0 0-1 0.0000000
>       10
> -1 0 0 0.0000000
>  0 0-1 0.0000000
>  0-1 0 0.0000000
>       11
> -1 0 0 0.0000000
>  0-1 0 0.0000000
>  0 0-1 0.0000000
>       12
> 


=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

__________________________________________________
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End of wien-digest V2002 #33
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #34
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
Errors-To: owner-wien-digest@theochem.tuwien.ac.at
Precedence: bulk


wien-digest       Tuesday, September 10 2002       Volume 2002 : Number 034




----------------------------------------------------------------------

Date: Sat, 31 Aug 2002 02:11:03 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: [none]

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====


Dear wien2k_02 user:
   I have a CeX system to calculate. I have calculated it with LSDA, 
LSDA+SIC ,LSDA+SO+SIC, but I encounter some questions, now first I list my 
result below:
     
     1: LSDA:  ENE: -28342.456753  FER: 0.63687
               MMTOT: 0.96610   MMI01:0.83685--------note: 01 refer to Ce
                                MMI02:-0.00321
     
     2:LSDA+SIC 
            a:  U=0.43 J=0.05
               ENE:-28342.343906  FER: 0.63843
               MMTOT: 1.31303   MMI01: 1.13621   MMI02:-0.00311

            b:  U=0.48 J=0.06
               ENE:-28342.334611  FER:0.63844
               MMTOT:1.32972   MMI01: 1.15569    MMI02:-0.00340
    
     3:LSDA+SO+SIC:
             a: U=0.48  J=0.06
               ENE:-28342.536933  FER:0.64280
               MMTOT:0.07238   MMINT:0.02410     MMI02:0.00034
               ORB01:0.34208
             
             b: U=0.56  J=0.07
                in this case , the case.scf has message like this:
                
                      warn energy intergal is 28.999918 should be 29
               
     I also calculate the system with LSDA+SO +OP:the result like this :
             ENE;-28342.509503  FER: 0.63745
             MMTOT:0.47180   MMI01:0.42996  MMI02:-0.00010
             ORB01:-2.81328           
    
In all my calculations , I have set EMAX in case.in1 to equal default value 
1.5,
I also set it to 3.5 when I calculate it with LSDA+SO+OP,the MMTOT became 
large, but the  difference is small
       

SO there are several questions I want to know:

    1:according to my understandign,adding  spin-orbit coupling ,the 
magnetis moment of spin will decrease,but in my case when I use 
LSDA+SO+SIC, the MMI01 decrease to 0.02410,it is to small ,I can't believe 
it ? is it reasonable or someting wrong with it?

    2: Why when I increase the values of U and J to 0.56 and 0.07 ,there 
are warning in case.scf ?  what this mean? And how can this affect the 
result? How can I handle with it?

    3: According to the userguider, in case.inc , in the first line ,there 
is a "shift" for "positive" energy ,when I calculate a system with 4f 
element, must I set this "shift" some value insted of zero?  if  must, how 
about the range it is?

Thanks for your help and advice


    Hai

 

              




_________________________________________________________________
ÏíÓÃÊÀ½çÉÏ×î´óµÄµç×ÓÓÊ¼þÏµÍ³¡ª MSN Hotmail¡£http://www.hotmail.com/cn

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------------------------------

Date: Sat, 31 Aug 2002 02:09:51 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: [none]

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====


Dear wien2k_02 user:
   I have a CeX system to calculate. I have calculated it with LSDA, 
LSDA+SIC ,LSDA+SO+SIC, but I encounter some questions, now first I list my 
result below:
     
     1: LSDA:  ENE: -28342.456753  FER: 0.63687
               MMTOT: 0.96610   MMI01:0.83685--------note: 01 refer to Ce
                                MMI02:-0.00321
     
     2:LSDA+SIC 
            a:  U=0.43 J=0.05
               ENE:-28342.343906  FER: 0.63843
               MMTOT: 1.31303   MMI01: 1.13621   MMI02:-0.00311

            b:  U=0.48 J=0.06
               ENE:-28342.334611  FER:0.63844
               MMTOT:1.32972   MMI01: 1.15569    MMI02:-0.00340
    
     3:LSDA+SO+SIC:
             a: U=0.48  J=0.06
               ENE:-28342.536933  FER:0.64280
               MMTOT:0.07238   MMINT:0.02410     MMI02:0.00034
               ORB01:0.34208
             
             b: U=0.56  J=0.07
                in this case , the case.scf has message like this:
                
                      warn energy intergal is 28.999918 should be 29
               
     I also calculate the system with LSDA+SO +OP:the result like this :
             ENE;-28342.509503  FER: 0.63745
             MMTOT:0.47180   MMI01:0.42996  MMI02:-0.00010
             ORB01:-2.81328           
    
In all my calculations , I have set EMAX in case.in1 to equal default value 
1.5,
I also set it to 3.5 when I calculate it with LSDA+SO+OP,the MMTOT became 
large, but the  difference is small
       

SO there are several questions I want to know:

    1:according to my understandign,adding  spin-orbit coupling ,the 
magnetis moment of spin will decrease,but in my case when I use 
LSDA+SO+SIC, the MMI01 decrease to 0.02410,it is to small ,I can't believe 
it ? is it reasonable or someting wrong with it?

    2: Why when I increase the values of U and J to 0.56 and 0.07 ,there 
are warning in case.scf ?  what this mean? And how can this affect the 
result? How can I handle with it?

    3: According to the userguider, in case.inc , in the first line ,there 
is a "shift" for "positive" energy ,when I calculate a system with 4f 
element, must I set this "shift" some value insted of zero?  if  must, how 
about the range it is? 

              




_________________________________________________________________
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Date: Mon, 2 Sep 2002 12:23:57 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Wien and/or SpaceGroups

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> More to the point, I'd like to raise another question,
> pertinent probably to the future releases. In another
> popular code, Stuttgart LMTO, the user has a
> possibility to describe the unit cell in Cartesian
> coordinates as three vectors rather than as three
> lengths and three angles. For instance, the AFL NIO
> unit cell would be
> a/2 a/2 a
> a/2 a 1/2
> a a/2 a/2
> I found that extremely convenient for doing reduced
> symmetry supercells. It looks to me, naively, that
> this should be quite a small addition to the existing
> code. Did you ever thought about adding such an
> option?

So far: no!
I always found it much easier to specify F or B lattice and/or some angles
instead of figuring out the proper Bravais matrix, but we may reconsider
things if it seems usefull.

In The NiO example: With this bravais matrix, how would you specify the
atomic positions ?

Another point: specifying H or R in WIEN means also using a special
coordinate system with all symmetry operations in hex coordinates,....

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Mon, 02 Sep 2002 14:50:22 +0200
From: Enrique Lomba <E.Lomba@iqfr.csic.es>
Subject: [WIEN]: Warning regarding Intel libraries for ia32 Linux and Wien2k code

====
Enrique Lomba <E.Lomba@iqfr.csic.es>
submitted the following contribution:
====

Dear Wien users,
I was having a lot of trouble trying to get results for trigonal Te 
(ghost states, limit of the linearization process, etc ...), but thanks 
to Fred Nastos who repeated the same calculation, I found out that the 
Wien2k code I had compiled was broken. I linked the code with Portland 
Group pgf90 in various linux boxes (p3 and p4) against the optimized 
Intel MathKernel libraries, which in other cases seemed to worked nicely 
  (lib_mklp3 and lib_mklp4) and it worked ok in the test cases. In this 
instance (trigonal Te) it seems the  lapw2c program gives wrong results 
!!!! I recompiled the code using the optimized blas found in 
http://www.cs.utk.edu/~ghenry/distrib/index.htm
and the results now look ok and reproduce the bibliographic data !!
In summary, I guess that there is something wrong (or some 
incompatibility) when lapw2c is compiled using this library. Perhaps 
someone with more expertise in this particular code could take a look 
and determine the BLAS routines which are behaving incorrectly and 
report that to Intel.
			Thanks to all and regards,
						Enrique






- -- 
- --------------------------------------------------------------
Enrique Lomba
Instituto de Quimica Fisica Rocasolano, CSIC
C/ Serrano 119, 28006 Madrid, Spain

FAX no. 34-915642431
Phone no. 34-915619407 (ext 1301)
e-mail : E.Lomba@iqfr.csic.es
www : http://www.fluid.iqfr.csic.es/enrique.html

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------------------------------

Date: Tue, 3 Sep 2002 14:13:10 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: [WIEN]: runsp -so -orb

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_000B_01C25354.087440F0
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	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

Dear all,

We are running the latest version of wien2k code, 29-Aug-2002. In a =
nonmagnetic case, e.g. bct-U, which we
 would keep the original structure even in the presence of spin-orbit =
coupling, lda+u calculation fails at the=20
step of "x lapwdm -up -c -so" in the first cycle. This means that one =
has to let the initso reduce the no. of symmetry
 operations from 48 to 16 (in this case evrything is okay), which is not =
our favorite physics. Is this natural?
One calculating "runsp -so -orb" and not "runsp -orb" or "runsp -so" =
also has to copy case.indm to case.indmc, why?
Is doing "mv case.in1 case.in1c" also necessary for a nonmagnetic case =
with its original case.struct to run "runsp_c -so -orb"?



Your,

S. Jalali.


- ------=_NextPart_000_000B_01C25354.087440F0
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT size=3D2>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><FONT face=3DArial =
size=3D3>Dear=20
all,</FONT></P><PRE><FONT size=3D3><FONT face=3DArial>We are running the =
latest version of wien2k code, <?xml:namespace prefix =3D st1 ns =3D =
"urn:schemas-microsoft-com:office:smarttags" /><st1:date Month=3D"8" =
Day=3D"29" Year=3D"2002">29-Aug-2002.</st1:date></FONT></FONT><FONT =
face=3DArial size=3D3> In a nonmagnetic case, e.g. bct-U, which =
we</FONT></PRE><PRE><FONT face=3DArial size=3D3> would keep the original =
structure even in the presence of spin-orbit coupling, lda+u calculation =
fails at the </FONT></PRE><PRE><FONT face=3DArial size=3D3>step of "x =
lapwdm =96up =96c =96so" in the first cycle. This means that one has to =
let the initso reduce the no. of symmetry</FONT></PRE><PRE><FONT =
face=3DArial size=3D3> operations from 48 to 16 (in this case evrything =
is okay), which is not our favorite physics. Is this =
natural?</FONT></PRE><PRE><FONT face=3DArial size=3D3>One calculating =
=93runsp =96so =96orb=94 and </FONT><FONT face=3DArial size=3D3>not =
=93runsp =96orb=94 or =93runsp =96so=94 also has to copy case.indm to =
case.indmc, why?</FONT></PRE>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><FONT face=3DArial =
size=3D3>Is doing=20
=93mv case.in1 case.in1c=94 also necessary for a nonmagnetic case with =
its original=20
case.struct to run =93runsp_c =96so =96orb=94?</FONT></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><FONT face=3DArial=20
size=3D3></FONT>&nbsp;</P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><FONT face=3DArial=20
size=3D3>Your,</FONT></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><FONT face=3DArial =
size=3D3>S.=20
Jalali.</FONT></P></FONT></DIV></BODY></HTML>

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------------------------------

Date: Tue, 3 Sep 2002 12:01:26 +0200 (MEST)
From: Vidya Ravindran <vidya.ravindran@kjemi.uio.no>
Subject: [WIEN]: Conversion from eV --> Tesla

====
Vidya Ravindran <vidya.ravindran@kjemi.uio.no>
submitted the following contribution:
====


Dear All,
     	I am trying to convert energy given in eV to the magnetic
field intensity given in Tesla. I am unable to find a direct conversion
factor for eV to Tesla
	I am highly thankful if somebody could suggest the conversion
factors or some references where I can find them.
	Thank you.

Yours sincerely,
R. Vidya

****************************************************************
R. Vidya, Department of Chemistry       |Tel: +47 228 55606
University of Oslo, PO Box 1033         |Fax: +47 228 55441/5565
Blindern, N-0315 OSLO, NORWAY           |
Email: ravindran.vidya@kjemi.uio.no     |
URL: http://folk.uio.no/~ravindrv       |
****************************************************************




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------------------------------

Date: Tue, 3 Sep 2002 16:40:55 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Conversion from eV --> Tesla

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0036_01C25368.AC9B0560
Content-Type: text/plain;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

>      I am trying to convert energy given in eV to the magnetic
> field intensity given in Tesla. I am unable to find a direct =
conversion
> factor for eV to Tesla
> I am highly thankful if somebody could suggest the conversion
> factors or some references where I can find them.
I have not seen such a direct formula, but I think it is feasible =
writing fundamental formula as follows:
I hope the used following symbols are visible in your editor:
1Gauss(G)=3D10-4Tessla(T)=3D10-4Weber(Wb)/m2=3D1Oersted(Oe)=3D103/4pA/m
1eV=3D1eWA=3D=3D=3D>4ep10-7Tessla=3DeV/mW

If they are not I would below repeat them in a plain text:
1Gauss(G)=3D10^(-4)Tessla(T)=3D10^(-4)Weber(Wb)/m2=3D1Oersted(Oe)=3D10^3/=
(4*3.14)A/m
1eV=3De*ohm*A=3D=3D=3D>4*e*3.14*10^(-7)Tessla=3DeV/m*ohm


- ------=_NextPart_000_0036_01C25368.AC9B0560
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff background=3D"">
<DIV><FONT face=3DArial size=3D2>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; I am =
trying to=20
convert energy given in eV to the magnetic<BR>&gt; field intensity given =
in=20
Tesla. I am unable to find a direct conversion<BR>&gt; factor for eV to=20
Tesla<BR>&gt; I am highly thankful if somebody could suggest the=20
conversion<BR>&gt; factors or some references where I can find=20
them.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>
<DIV><FONT face=3DArial size=3D2>I have not seen such a direct formula, =
but I think=20
it is feasible writing fundamental formula as follows:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>I hope the used following =
symbols&nbsp;are visible=20
in your editor:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>1Gauss(G)=3D<FONT size=3D3><FONT=20
face=3D"Times New Roman">10<SUP>-4</SUP></FONT><FONT face=3DArial=20
size=3D2>Tessla(T)=3D<FONT size=3D3><FONT=20
face=3D"Times New Roman">10<SUP>-4</SUP></FONT></FONT><FONT face=3DArial =

size=3D2>Weber(Wb)/m<FONT size=3D3><FONT=20
face=3D"Times New Roman"><SUP>2</SUP></FONT><FONT face=3DArial=20
size=3D2>=3D1Oersted(Oe)=3D1<FONT size=3D3><FONT=20
face=3D"Times New Roman">0<SUP>3</SUP>/4</FONT><FONT =
face=3DSymbol>p</FONT><FONT=20
size=3D2>A/m</FONT></FONT></FONT></FONT></FONT></FONT></FONT></FONT></DIV=
><FONT=20
face=3DSymbol size=3D3><FONT face=3DArial size=3D2>1eV=3D1e</FONT>W<FONT =
face=3DArial=20
size=3D2>A=3D=3D=3D&gt;<FONT size=3D3><FONT face=3D"Times New =
Roman">4e</FONT><FONT=20
face=3DSymbol>p</FONT><FONT face=3D"Times New =
Roman">10<SUP>-7</SUP></FONT><FONT=20
face=3DArial>Tessla=3DeV/m</FONT><FONT=20
face=3DSymbol>W</FONT></FONT></FONT></FONT><BR></FONT></DIV>
<DIV><FONT face=3DArial size=3D2>If&nbsp;they are&nbsp;not I would below =

repeat&nbsp;them in a plain text:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>
<DIV><FONT face=3DArial size=3D2>1Gauss(G)=3D10^(-4)<FONT size=3D3><FONT =
face=3DArial=20
size=3D2>Tessla(T)=3D10^(-4)<FONT face=3DArial size=3D2>Weber(Wb)/m<FONT =
size=3D3><FONT=20
face=3D"Times New Roman"><SUP>2</SUP></FONT><FONT face=3DArial=20
size=3D2>=3D1Oersted(Oe)=3D10^3<FONT size=3D3><FONT=20
face=3D"Times New Roman">/(4*3.14)</FONT><FONT=20
size=3D2>A/m</FONT></FONT></FONT></FONT></FONT></FONT></FONT></FONT></DIV=
><FONT=20
face=3DSymbol size=3D3><FONT face=3DArial =
size=3D2>1eV=3De*ohm*</FONT><FONT face=3DArial=20
size=3D2>A=3D=3D=3D&gt;4*e*3.14*10^(-7)<FONT size=3D3><FONT=20
face=3DArial>Tessla=3DeV/m*ohm</FONT></FONT></FONT></FONT><BR></DIV></FON=
T></BODY></HTML>

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------------------------------

Date: Tue, 3 Sep 2002 14:45:49 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: runsp -so -orb

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>In a nonmagnetic case, e.g. bct-U, which we
>  would keep the original structure even in the presence of spin-orbit
coupling, lda+u calculation fails at the
> step of "x lapwdm -up -c -so" in the first cycle. This means that one
has to let the initso reduce the no. of symmetry
>  operations from 48 to 16 (in this case evrything is okay), which is
not our favorite physics. Is this natural?

WIEN has a constraint: LDA+U calculations must be done in "spin-polarized"
mode (But you can use runsp_c_lapw which constrains to zero moment).
When doing spinpolarization and adding SO, symmetry must be reduced. This
follows naturally from the first constraint.

> One calculating "runsp -so -orb" and not "runsp -orb" or "runsp -so"
also has to copy case.indm to case.indmc, why?

After lapwso the eigenvectors are complex, so one must run the complex
versions of lapw2 (always) and lapwdm (this program is called only with -orb)

> Is doing "mv case.in1 case.in1c" also necessary for a nonmagnetic case
with its original case.struct to run "runsp_c -so -orb"?

I think so.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Tue, 3 Sep 2002 18:55:53 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: runsp -so -orb

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

Dear all,
First, I would appreciate Peter for his exact answers as usual, and then ask
one thing more:
Why is only "lapwdm -c -up -so"  called during "runsp_c_lapw -so -orb" and
not "lapwdm -c -dn -so" looking at :log?
Your,
S. Jalali.

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Date: Tue, 3 Sep 2002 10:54:17 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: Conversion from eV --> Tesla

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====


> > I am trying to convert energy given in eV to the magnetic
> > field intensity given in Tesla. I am unable to find a direct conversion
> > factor for eV to Tesla

I believe that is because a direct conversion factor does not exist.

In SI units, the Tesla measures magnetic induction, B, and has dimensions of
[mass][charge]^{-1}[time]^{-1}.  Still in SI units, the magnetic field, H, has 
units of Amperes/m and dimensions of [charge][length]^{-1}[time]^{-1}.
So, I'm not sure what you mean by "magnetic field intensity given in Tesla".

> I have not seen such a direct formula, but I think it is feasible writing
> fundamental formula as follows:

> 1Gauss(G)=10^(-4)Tessla(T)=10^(-4)Weber(Wb)/m2=1Oersted(Oe)
> =10^3/(4*3.14)A/m 1eV=e*ohm*A===>4*e*3.14*10^(-7)Tessla=eV/m*ohm

I believe this is dangerous, since, in Gaussian Units, an induction field of 
one gauss corresponds to a magnetic field of one oersted only in the absence
of magnetic materials. Nonetheless, your result shows that to relate magnetic 
fields and energy you need material information (i.e. the magnetic moment).

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Date: Tue, 3 Sep 2002 14:40:16 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: Conversion from eV --> Tesla

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

You guys are making this way too complicated.

The conversion factor is just the Bohr magneton, 
I check the backpage of my Ashcrift-Mermin, one, two,
three...
1 mu_B=5.7884E-5 eV/T

- --- Fred Nastos <nastos@physics.utoronto.ca> wrote:
> ====
> Fred Nastos <nastos@physics.utoronto.ca>
> submitted the following contribution:
> ====
> 
> 
> > > I am trying to convert energy given in eV to the
> magnetic
> > > field intensity given in Tesla. I am unable to
> find a direct conversion
> > > factor for eV to Tesla
> 
> I believe that is because a direct conversion factor
> does not exist.
> 
> In SI units, the Tesla measures magnetic induction,
> B, and has dimensions of
> [mass][charge]^{-1}[time]^{-1}.  Still in SI units,
> the magnetic field, H, has 
> units of Amperes/m and dimensions of
> [charge][length]^{-1}[time]^{-1}.
> So, I'm not sure what you mean by "magnetic field
> intensity given in Tesla".
> 
> > I have not seen such a direct formula, but I think
> it is feasible writing
> > fundamental formula as follows:
> 
> >
>
1Gauss(G)=10^(-4)Tessla(T)=10^(-4)Weber(Wb)/m2=1Oersted(Oe)
> > =10^3/(4*3.14)A/m
> 1eV=e*ohm*A===>4*e*3.14*10^(-7)Tessla=eV/m*ohm
> 
> I believe this is dangerous, since, in Gaussian
> Units, an induction field of 
> one gauss corresponds to a magnetic field of one
> oersted only in the absence
> of magnetic materials. Nonetheless, your result
> shows that to relate magnetic 
> fields and energy you need material information
> (i.e. the magnetic moment).
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====


=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

__________________________________________________
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Date: Tue, 3 Sep 2002 14:50:13 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: Wien and/or SpaceGroups

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

Well, my position is that it is always nicer to have a
choice. 

- --- Peter Blaha <pblaha@theochem.tuwien.ac.at> wrote:
> > code. Did you ever thought about adding such an
> > option?
> 
> So far: no!
> I always found it much easier to specify F or B
> lattice and/or some angles
> instead of figuring out the proper Bravais matrix,
> but we may reconsider
> things if it seems usefull.
 
Well, my position is that it is always nicer to have a
choice. 

> In The NiO example: With this bravais matrix, how
> would you specify the
> atomic positions ?

The same way. Since the positions are given in terms
of the lattice vectors, and the lattice vectors are
exactly the same as rhombohedral vectors, the atomic
positions are the same.

Specifically, for NiO, the unit celee vectors are, in
units of a,

1.0 0.5 0.5
0.5 1.0 0.5
0.5 0.5 1.0

And positions are
0.00 0.00 0.00 Ni1
0.50 0.50 0.50 Ni2
0.25 0.25 0.25 O
- -.25 -.25 -.25 O

What can be simpler?

> 
> Another point: specifying H or R in WIEN means also
> using a special
> coordinate system with all symmetry operations in
> hex coordinates,....
> 
> Regards
> 
> 
>                                       P.Blaha
>
- --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna,
> A-1060 Vienna
> Phone: +43-1-58801-15671             FAX:
> +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
> http://info.tuwien.ac.at/theochem/
>
- --------------------------------------------------------------------------
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====


=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

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------------------------------

Date: Wed, 04 Sep 2002 01:59:57 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: [none]

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====






Dear wien2k users:
   I have download the version of wien2k,(modified 29 august,) but when I 
use it to calculate , I find there are always the sign of "ghost band"in 
case.scf file. I have test it to calculate a system with SO+LDA+U, but 
whatever I change the value U,J, the sentnece like "QTL_B Value .EQ. 
0.xxxxxxx" always appear in my case.file . I thought it may be my fault in 
add SO+LDA+U, so I change to test it with the example Ni in userguide, but 
to my surprise , the sentence "QTL_B Value .EQ. 7.09128" also appear!!!, I 
can hardly believe it !!!. why can this be?Did anyone else also encounter 
this porblem? I am so puzzled about this






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------------------------------

Date: Wed, 4 Sep 2002 09:45:02 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: [WIEN]: Re: 

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>    I have download the version of wien2k,(modified 29 august,) but when I
> use it to calculate , I find there are always the sign of "ghost band"in
> case.scf file. I have test it to calculate a system with SO+LDA+U, but
> whatever I change the value U,J, the sentnece like "QTL_B Value .EQ.
> 0.xxxxxxx" always appear in my case.file . I thought it may be my fault in
> add SO+LDA+U, so I change to test it with the example Ni in userguide, but
> to my surprise , the sentence "QTL_B Value .EQ. 7.09128" also appear!!!, I
> can hardly believe it !!!. why can this be?Did anyone else also encounter
> this porblem? I am so puzzled about this

Did you see http://www.wien2k.at/reg_user/faq/scf.html ?
Meanwhile, I have found that using "-in1new 5" is very reliable, though many
think it is dangerous.
Your,
S. Jalali.

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------------------------------

Date: Wed, 4 Sep 2002 10:36:32 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: [WIEN]: Re: 

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>     3: According to the userguider, in case.inc , in the first line ,there
> is a "shift" for "positive" energy ,when I calculate a system with 4f
> element, must I set this "shift" some value insted of zero?  if  must, how
> about the range it is?

Did you see http://www.wien2k.at/reg_user/faq/open_core.html ? For sure,
open core calculation is another approach to put some localized 4f-electrons
from valence state into the core. In this approach one cannot make choice
how far from Fermi energy electrons can be. This means that the 4f-electrons
can be regularly (LDA) in the valence state (at the Fermi energy) or using
the open core treatment in the core region. Implemented LDA+U now is more
reliable approach with its adjustable parameters to play with DOS's.
Your,
S. Jalali.

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------------------------------

Date: Wed, 4 Sep 2002 08:44:10 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: runsp -so -orb

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Why is only "lapwdm -c -up -so"  called during "runsp_c_lapw -so -orb" and
> not "lapwdm -c -dn -so" looking at :log?

lapwdm calculates the density matrices inside spheres. This is needed ONLY
for the orbital potentials, not for a standard LDA(GGA) calculation, even
when spin-orbit is included.

After runsp -so has finished, one can use lapwdm to calculate an orbital
moment, but there is no need to do this during scf.

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 4 Sep 2002 09:02:36 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: [WIEN]: Re: your mail

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>    I have download the version of wien2k,(modified 29 august,) but when I
> use it to calculate , I find there are always the sign of "ghost band"in
> case.scf file. I have test it to calculate a system with SO+LDA+U, but
> whatever I change the value U,J, the sentnece like "QTL_B Value .EQ.
> 0.xxxxxxx" always appear in my case.file . I thought it may be my fault in
> add SO+LDA+U, so I change to test it with the example Ni in userguide, but
> to my surprise , the sentence "QTL_B Value .EQ. 7.09128" also appear!!!, I
> can hardly believe it !!!. why can this be?Did anyone else also encounter
> this porblem? I am so puzzled about this

A small QTL-B value does NOT mean that you have ghost bands!

The QTL-B value is the contribution to the wavefunction (charge) from the
B_lm u-dot term in the basis. When you consider that this u-dot term is
used to account for the energy dependence of the radial wavefunction, it is
clear that this B_lm term should always be smaller than the A_lm term
(it should be a correction to the A_lm). Obviously, the better your choice
of the energy parameters is, the smaller the correction. Thus "better"
energy parameters should give smaller QTL-B. However, depending on the
system, you may always find some small QTL-B warnings, since e.g. a 3d
wavefunction has a very strong energy dependence, but may still contribute
over a fairly wide energy range to the eigenvalue spectrum. In such cases
one can further improve the situation by adding a 3d "local-orbital".
However, be carefull, you must be sure that the energy parameters of the
regular 3d-LAPW and the 3d -LO are at least about 0.5 Ry apart, otherwise
you may get real ghostbands due to nearly degenerate basis functions.

Only QTL-B values larger than 20-30 mean that you have actual ghostbands.

QTL-B between 5 and 10 suggests that you analyse the situation (check the
help files and/or the :EPL :EPH lines in the scf file), change the
energy parameters by hand (case.in1) or use the -in1new switch of run_lapw.
But there may be examples where you can (or must) stay with such QTL-B.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 4 Sep 2002 13:15:49 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: runsp -so -orb

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====


> > Why is only "lapwdm -c -up -so"  called during "runsp_c_lapw -so -orb"
and
> > not "lapwdm -c -dn -so" looking at :log?
>
> lapwdm calculates the density matrices inside spheres. This is needed ONLY
> for the orbital potentials, not for a standard LDA(GGA) calculation, even
> when spin-orbit is included.
> After runsp -so has finished, one can use lapwdm to calculate an orbital
> moment, but there is no need to do this during scf.
Yes, you can say that again and I like to thank you very much, but to show I
have not realized yet let me please continue in this respect:
The question is in the presence of orbital potential, as it is indicated
by -orb, and I would emphasis why only up density matrices are calculated
and not down density matrices. Please notice that this is not the case
during "runsp -orb". This means that both "lapwdm -up" and "lapwdm -dn" are
called in the absence of -so, but only "lapwdm -up" in the presence of -so.
Your,
S. Jalali.

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------------------------------

Date: Wed, 4 Sep 2002 10:55:30 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: runsp -so -orb

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> > > Why is only "lapwdm -c -up -so"  called during "runsp_c_lapw -so -orb"
> and
> > > not "lapwdm -c -dn -so" looking at :log?
> >
> > lapwdm calculates the density matrices inside spheres. This is needed ONLY
> > for the orbital potentials, not for a standard LDA(GGA) calculation, even
> > when spin-orbit is included.
> > After runsp -so has finished, one can use lapwdm to calculate an orbital
> > moment, but there is no need to do this during scf.
> Yes, you can say that again and I like to thank you very much, but to show I
> have not realized yet let me please continue in this respect:

> The question is in the presence of orbital potential, as it is indicated
> by -orb, and I would emphasis why only up density matrices are calculated
> and not down density matrices. Please notice that this is not the case
> during "runsp -orb". This means that both "lapwdm -up" and "lapwdm -dn" are
> called in the absence of -so, but only "lapwdm -up" in the presence of -so.

Spin-orbit couples spin-up and dn, i.e. an eigenvector of a single eigenvalue
may contain both, spinup and dn contribution. Thus one cannot seperate the
eigenvalues into spin-up and dn eigenvalues anymore. When processing the i-th
eigenvalue, both spin-up AND spin-dn AND the spin-up-dn cross terms !! are
calculated at once. Thus you need only one call to lapwdm.

Without SO, I must call lapwdm separately for spin-up and dn since for
up ONLY the up eigenvalues and for dn only dn-eigenvalues are present.


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 4 Sep 2002 15:08:47 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: runsp -so -orb

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> Spin-orbit couples spin-up and dn, i.e. an eigenvector of a single
eigenvalue
> may contain both, spinup and dn contribution. Thus one cannot seperate the
> eigenvalues into spin-up and dn eigenvalues anymore. When processing the
i-th
> eigenvalue, both spin-up AND spin-dn AND the spin-up-dn cross terms !! are
> calculated at once. Thus you need only one call to lapwdm.
Therefore, one concludes that with SO even for a magnetic case up-DOSs and
dn-DOSs are alike. To make it more complicated, one can consider a case with
two inequivalent atoms, and turn on the SO only for one atom, which is
possible now in wien code: turning off the SO for another atom. In this
case, up and dn density matrices should be calculated for one atom and only
up density matrices for the other atom. I cannot imagine how practically it
is performed. Partial DOSs can be separated as spheres are separated, but I
cannot think about the total-DOS.
Please forgive me for severely asking trivial questions.
Your,
S. Jalali.

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------------------------------

Date: Wed, 04 Sep 2002 11:04:36 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: Re: [WIEN]: Re:

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====

Dear Sasid:
 According to your help, does it mean that When use LDA+U, it is not need 
to shift potential in case.inc? And LDA+U have a better result than open 
core treament?
Hai

>From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: <wien@zeus.theochem.tuwien.ac.at>
>Subject: [WIEN]: Re: 
>Date: Wed, 4 Sep 2002 10:36:32 +0430
>
>====
>"Saeid Jalali" <sjalali@cc.iut.ac.ir>
>submitted the following contribution:
>====
>
> >     3: According to the userguider, in case.inc , in the first line 
,there
> > is a "shift" for "positive" energy ,when I calculate a system with 4f
> > element, must I set this "shift" some value insted of zero?  if  must, 
how
> > about the range it is?
>
>Did you see http://www.wien2k.at/reg_user/faq/open_core.html ? For sure,
>open core calculation is another approach to put some localized 
4f-electrons
>from valence state into the core. In this approach one cannot make choice
>how far from Fermi energy electrons can be. This means that the 
4f-electrons
>can be regularly (LDA) in the valence state (at the Fermi energy) or using
>the open core treatment in the core region. Implemented LDA+U now is more
>reliable approach with its adjustable parameters to play with DOS's.
>Your,
>S. Jalali.
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====



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------------------------------

Date: Wed, 04 Sep 2002 11:13:11 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: Re: [WIEN]: Re: your mail

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====

Dear Peter:
 Thanks for your help. And I want to know , if the QTL-B is small, can I 
ignore it? And how does it affect our calculation?
Hai

>From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: <wien@zeus.theochem.tuwien.ac.at>
>Subject: [WIEN]: Re: your mail
>Date: Wed, 4 Sep 2002 09:02:36 +0200 (MEST)
>
>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
> >    I have download the version of wien2k,(modified 29 august,) but when 
I
> > use it to calculate , I find there are always the sign of "ghost 
band"in
> > case.scf file. I have test it to calculate a system with SO+LDA+U, but
> > whatever I change the value U,J, the sentnece like "QTL_B Value .EQ.
> > 0.xxxxxxx" always appear in my case.file . I thought it may be my fault 
in
> > add SO+LDA+U, so I change to test it with the example Ni in userguide, 
but
> > to my surprise , the sentence "QTL_B Value .EQ. 7.09128" also 
appear!!!, I
> > can hardly believe it !!!. why can this be?Did anyone else also 
encounter
> > this porblem? I am so puzzled about this
>
>A small QTL-B value does NOT mean that you have ghost bands!
>
>The QTL-B value is the contribution to the wavefunction (charge) from the
>B_lm u-dot term in the basis. When you consider that this u-dot term is
>used to account for the energy dependence of the radial wavefunction, it 
is
>clear that this B_lm term should always be smaller than the A_lm term
>(it should be a correction to the A_lm). Obviously, the better your choice
>of the energy parameters is, the smaller the correction. Thus "better"
>energy parameters should give smaller QTL-B. However, depending on the
>system, you may always find some small QTL-B warnings, since e.g. a 3d
>wavefunction has a very strong energy dependence, but may still contribute
>over a fairly wide energy range to the eigenvalue spectrum. In such cases
>one can further improve the situation by adding a 3d "local-orbital".
>However, be carefull, you must be sure that the energy parameters of the
>regular 3d-LAPW and the 3d -LO are at least about 0.5 Ry apart, otherwise
>you may get real ghostbands due to nearly degenerate basis functions.
>
>Only QTL-B values larger than 20-30 mean that you have actual ghostbands.
>
>QTL-B between 5 and 10 suggests that you analyse the situation (check the
>help files and/or the :EPL :EPH lines in the scf file), change the
>energy parameters by hand (case.in1) or use the -in1new switch of 
run_lapw.
>But there may be examples where you can (or must) stay with such QTL-B.
>
>Regards
>
>                                       P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: 
http://info.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====




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------------------------------

Date: Wed, 4 Sep 2002 17:29:12 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Re:

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>does it mean that When use LDA+U, it is not need
> to shift potential in case.inc?
It is not needed in LDA+U scheme to change case.inc file: it is a trick in
open core calculation.



Indeed, shifting in LDA+U scheme is a job for added orbital dependent
potential, and one controls it using U and J, and in some special cases
changing the diagonal elements of density matrices. The later one, which is
not recommended for any cases by the author, means that changing the initial
values of occupation numbers may change the final result to a better
agreement with experiment. This would not be so surprising as really a
compound is a chaotic system! Even though chaos is a classical phenomena
with exact definition,  one would extend it to quantum mechanics taking into
account different density of states within different initial values.

> And LDA+U have a better result than open
> core treament?
Basically, yes it has, or at least one wishes so as one is free now to
struggle with more flexible parameters.
Your,
S. Jalali.

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------------------------------

Date: Wed, 4 Sep 2002 12:47:57 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: Conversion from eV --> Tesla

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====

> The conversion factor is just the Bohr magneton,
> I check the backpage of my Ashcrift-Mermin, one, two, three...
> 1 mu_B=5.7884E-5 eV/T

The Bohr magneton is the conversion factor to convert magnetic
dipoles given in ev/T to Rydberg atomic units (for Hartree a.u. it is
twice the Bohr magneton).  It is not a conversion factor for Teslas
to eV.
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------------------------------

Date: Wed, 4 Sep 2002 12:16:14 -0700 (PDT)
From: yanming Ma <ymma66@yahoo.com>
Subject: [WIEN]: How to increase the default LM-list to LM =8 or 10

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-232292027-1031166974=:5675
Content-Type: text/plain; charset=us-ascii


Dear wien2k users,

I am  using the AIM program in WIEN2k. When I calculated the critical points for some materials. The AIM runs without stopping. I know the discontinuities appear at the sphere boundary. According to the User guides of wien2k, I have gotten the as little "core-leakage" as possible from LSTART. But I don't know how to increase properly the default LM-list to LM=8 or 10 without causing other problems. 

I would appreciate highly all kinds of comments. 

Thanks in advance. 



- ---------------------------------
Do You Yahoo!?
Yahoo! Finance - Get real-time stock quotes
- --0-232292027-1031166974=:5675
Content-Type: text/html; charset=us-ascii

<P>Dear wien2k users,</P>
<P>I am&nbsp; using the AIM program in WIEN2k. When I calculated the critical points for some materials. The&nbsp;AIM runs without stopping. I know the discontinuities appear at the sphere boundary. According to the User guides&nbsp;of wien2k, I have gotten the as little "core-leakage" as possible from LSTART. But I don't know how to increase properly the default LM-list to LM=8 or 10 without causing other problems.&nbsp;</P>
<P>I&nbsp;would appreciate highly all kinds of comments.&nbsp;</P>
<P>Thanks in advance.&nbsp;</P><p><br><hr size=1><b>Do You Yahoo!?</b><br>
<a href="http://rd.yahoo.com/finance/mailsig/new/*http://finance.yahoo.com">Yahoo! Finance</a> - Get real-time stock quotes
- --0-232292027-1031166974=:5675--
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------------------------------

Date: Wed, 04 Sep 2002 20:26:13 GMT
From: "Luis Alberto Terrazos Javier" <lterrazo@fisica.ufs.br>
Subject: [WIEN]: allocate data object

====
"Luis Alberto Terrazos Javier" <lterrazo@fisica.ufs.br>
submitted the following contribution:
====

Dear wien users and developers
I have a system with 80 atoms per unit cell with 7 non-equivelent atoms in 
this case it are calculating without problem
I have the same system with 80 atoms per unit cell with 13 non-equivalent 
atoms but when are calculating lapw1 stop with this error:
  1525-108 Error encountered while attempting to allocate a data object.  
The prog
ram will stop.
I compiled with NMATMAX=10000 and with a 2gb memory ram in a sp2 machine
in the moment was stop the program it is using only 100Mb of memory ram.
I looking for the similar error in the digest list but I did not encounter 
the solution for this problem.
I would like to know where is the mistake.
Thanks for you help
luis 
====
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Date: Wed, 4 Sep 2002 20:26:26 -0700 (PDT)
From: morteza jamal <m_jamal23@yahoo.com>
Subject: [WIEN]: d Orbital  existence

====
morteza jamal <m_jamal23@yahoo.com>
submitted the following contribution:
====

Dear Win2k users.
Is the d orbital existence, effective in the selection
Muffin tin radius.


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Date: Thu, 5 Sep 2002 10:26:28 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: How to increase the default LM-list to LM =8 or 10

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0130_01C254C6.B20190A0
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>I am  using the AIM program in WIEN2k. When I calculated the critical =
points for some materials. The AIM runs without >stopping. I know the =
discontinuities appear at the sphere boundary. According to the User =
guides of wien2k, I have gotten >the as little "core-leakage" as =
possible from LSTART. But I don't know how to increase properly the =
default LM-list to >LM=3D8 or 10 without causing other problems.=20

To make LM=3D8 one needs to change LM combinations in case.in2 file as =
follows:
0 0 2 0 2 2 4 0 4 2 4 4 6 0 6 2 6 4 6 6 8 0 8 2 8 4 8 6 8 8

0 0 1 0 2 0 2 2 3 0 3 2 4 0 4 2 4 4 5 0 5 2 5 4 6 0 6 2 6 4 6 6 7 0 7 2 =
7 4 7 6 8 0 8 2 8 4 8 6 8 8

One can follow the logic to make higher LM combinations.

Your,

S. Jalali.


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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV>&gt;I am&nbsp; using the AIM program in WIEN2k. When I calculated =
the=20
critical points for some materials. The&nbsp;AIM runs without =
&gt;stopping. I=20
know the discontinuities appear at the sphere boundary. According to the =
User=20
guides&nbsp;of wien2k, I have gotten &gt;the as little "core-leakage" as =

possible from LSTART. But I don't know how to increase properly the =
default=20
LM-list to &gt;LM=3D8 or 10 without causing other problems.&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>To make LM=3D8&nbsp;one needs to =
change&nbsp;LM=20
combinations in case.in2 file as follows:</FONT></DIV>
<DIV><FONT face=3DCourier size=3D1>
<P align=3Dleft>0 0 2 0 2 2 4 0 4 2 4 4 6 0 6 2 6 4 6 6 8 0 8 2 8 4 8 6 =
8 8</P>
<P align=3Dleft>0 0 1 0 2 0 2 2 3 0 3 2 4 0 4 2 4 4 5 0 5 2 5 4 6 0 6 2 =
6 4 6 6 7=20
0 7 2 7 4 7 6 8 0 8 2 8 4 8 6 8 8</P>
<P align=3Dleft><FONT face=3DArial size=3D2>One can follow the logic to =
make higher LM=20
combinations.</FONT></P>
<P align=3Dleft><FONT face=3DArial size=3D2>Your,</FONT></P>
<P align=3Dleft><FONT face=3DArial size=3D2>S. =
Jalali.</FONT></FONT><FONT=20
face=3DURWPalladioL-Roma></P></FONT></DIV></BODY></HTML>

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Date: Thu, 5 Sep 2002 11:21:50 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Conversion from eV --> Tesla

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> > The conversion factor is just the Bohr magneton,
> > I check the backpage of my Ashcrift-Mermin, one, two, three...
> > 1 mu_B=5.7884E-5 eV/T
>
> The Bohr magneton is the conversion factor to convert magnetic
> dipoles given in ev/T to Rydberg atomic units (for Hartree a.u. it is
> twice the Bohr magneton).  It is not a conversion factor for Teslas
> to eV.


I'll say.



> > > I am trying to convert energy given in eV to the magnetic
> > > field intensity given in Tesla. I am unable to find a direct
conversion
> > > factor for eV to Tesla
>
> I believe that is because a direct conversion factor does not exist.



Real part of the complex Poynting vector is the key to establish that such a
conversion factor varies from one case to another case depending on material
information (both geometric shape and magnetic properties).

From Poynting vector we know that there is a relationship between density of
energy (u) and E and B fields: u=1/(16*pi)*( epsilon*E^2+1/mu*B^2).

Since it is easier to think about electric field, I would go through the
problem keeping only the first term of the above equation regardless the
constant factor, i.e. u=epsilon*E^2. This relation between density of energy
(energy per volume) and electric field implies that one can find self-energy
of a known charge distribution via integrating of the generated E field of
the charge distribution over all space. Hence, conversion factor, which is
in general accessible after integrating, varies by the geometry of the
charge distribution and dielectric constants of the substance and its
environment. The same story describes how the conversion factor varies by
the geometry of a current distribution and magnetic permeailities of the
substances and its environment.



Dose this mean that the original question (conversion factor for Tessla to
eV) is meaningless? The answer is: no it is not meaningless but it is
useless due to non-unique-answer.



Your,

S. Jalali.

My previous answer works just for some simple special cases.


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Date: Thu, 5 Sep 2002 11:00:47 +0200 (MEST)
From: Ponniah Vajeeston <ponniah.vajeeston@kjemi.uio.no>
Subject: [WIEN]: reference of the open-core approximation

====
Ponniah Vajeeston <ponniah.vajeeston@kjemi.uio.no>
submitted the following contribution:
====

Dear WIEN users,

	I am looking for the exact reference of the open-core approximation.
I will appreciate if somebody can help me.

Regards,
P.Vajeeston


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Date: Thu, 5 Sep 2002 12:10:49 +0200
From: "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: reference of the open-core approximation

====
"Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> Ponniah Vajeeston <ponniah.vajeeston@kjemi.uio.no>
> submitted the following contribution:
> ====
>
> I am looking for the exact reference of the open-core approximation.
> I will appreciate if somebody can help me.

I don't think there is one unique source. In M. Richter, J. Phys. D: Appl.
Phys. 31 (1998) 1017-1048 you find under par. 2.2 an overview of early
papers that apply and/or devellop this approximation.

Stefaan

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Date: Thu, 5 Sep 2002 14:48:50 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: reference of the open-core approximation

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

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> I am looking for the exact reference of the open-core approximation.
> I will appreciate if somebody can help me.

I do not know what you mean exact, but I find the following references =
useful:
1. M. Richter, J. Phys. D: Appl. Phys. 31, 1017 (1998).
2.M. Divi=A1s, K. Schwarz, P. Blaha, G. Hilscher, H. Michor, and S. =
Khmelevskyi, Phys. Rev. B 62, 6774 (2000).

Your,

S. Jalali.


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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY>
<DIV><FONT face=3DArial size=3D2>&gt; I am looking for the exact =
reference of the=20
open-core approximation.<BR>&gt; I will appreciate if somebody can help=20
me.<BR></FONT><FONT face=3DArial size=3D2></FONT></DIV>
<DIV><FONT face=3DArial size=3D2>I do not know what you mean exact, but =
I find the=20
following references useful:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>1.&nbsp;M. Richter, J. Phys. D: Appl. =
Phys. 31,=20
1017 (1998).</DIV>
<P align=3Dleft><FONT face=3DArial size=3D2>2.M. Divi=A1s, K. Schwarz, =
P. Blaha, G.=20
Hilscher, H. Michor, </FONT><FONT face=3DArial size=3D2>and S. =
Khmelevskyi, Phys.=20
Rev. B 62, 6774 (2000).</FONT></P>
<P align=3Dleft>Your,</P>
<P align=3Dleft>S. Jalali.</P></FONT></BODY></HTML>

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Date: Thu, 05 Sep 2002 14:13:43 +0200
From: Thomas Claesson <thomas@matphys.kth.se>
Subject: [WIEN]: Strange LDA+U behaviour

====
Thomas Claesson <thomas@matphys.kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

I have a very strange behaviour to report, which ocurred when I tried to 
run an LDA+U calculation on NiO in the AF II configuration. I am able to 
run both on an ordinary Linux PC (P4 1.5 GHz) and on a multiprocessor AIX 
system (an IBM SP2), where I run in parallel. This is what I first tried on 
both systems:
1) runsp_c_lapw (i.e. NOT LDA+U)
2) runsp_c_lapw -orb (U=0.59, J=0.07 Ry)

Step 1) converged nicely without any problems on both systems. When I tried 
2) it converged after about 30-40 cycles and some small oscillations on the 
SP2. On my PC however it was impossible to make it converge using this 
approach. When I calculated DOS and bandstructure  (X-gamma-Z direction) on 
the SP2 I found to my great surprise that there was no gap at the Fermi 
level! With LDA+U there should certainly be a gap, see for instance O. 
Bengone et. al, PRB 62,16392 (2000).

Then I tried to make it converge also on the PC, so I started from a low 
U-value, and increased U in steps of about 0.1 Ry, running to self 
consistency for each U-value. With a reduced mixing factor (0.03) I managed 
to converge it on the PC this way. When I calculated DOS and 
bandstructure  (X-gamma-Z direction) again, I now found the expected gap at 
the Fermi level! This made me happy and at the same time very puzzled. How 
can it be that two runs, made on different computers, that should be 
identical can differ so much?

Later I tried the same method on the SP2 (increasing U gradually with a low 
mixing factor), but with the same result (no gap).

When I make runs without LDA+U I get identical results on both machines. I 
have used RKmax = 7.0 and a k-mesh of 300-600 points in the entire BZ. The 
only thing I can think of that should differ between these two systems is 
the precision, probably the SP2 has greater precision than my PC, where I 
run the executables. On the SP2 I have compiled the source with xlf90. I am 
using the latest version of the code on both machines.

Thanks for your replies! Any suggestions are welcome!

Best regards,
Thomas Claesson

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Date: Thu, 5 Sep 2002 05:35:43 -0700 (PDT)
From: yanming Ma <ymma66@yahoo.com>
Subject: Re: [WIEN]: How to increase the default LM-list to LM =8 or 10

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-1927393837-1031229343=:49205
Content-Type: text/plain; charset=us-ascii


Dear Saeid Jalali,
Thanks very much for your reply. Do I need change the NCOM in param.inc file? I remeber someone in the maillist said " The Maximum LM can be only 6 when the parameter NCOM equal to 49. So question is how large the NCOM should be when LM set to be 8.
Yanming  
 Saeid Jalali wrote:>I am  using the AIM program in WIEN2k. When I calculated the critical points for some materials. The AIM runs without >stopping. I know the discontinuities appear at the sphere boundary. According to the User guides of wien2k, I have gotten >the as little "core-leakage" as possible from LSTART. But I don't know how to increase properly the default LM-list to >LM=8 or 10 without causing other problems.  To make LM=8 one needs to change LM combinations in case.in2 file as follows:
0 0 2 0 2 2 4 0 4 2 4 4 6 0 6 2 6 4 6 6 8 0 8 2 8 4 8 6 8 8

0 0 1 0 2 0 2 2 3 0 3 2 4 0 4 2 4 4 5 0 5 2 5 4 6 0 6 2 6 4 6 6 7 0 7 2 7 4 7 6 8 0 8 2 8 4 8 6 8 8

One can follow the logic to make higher LM combinations.

Your,

S. Jalali.



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- --0-1927393837-1031229343=:49205
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<P>Dear Saeid Jalali,
<P>Thanks very much for your reply. Do I need change the NCOM in param.inc file? I remeber someone in the maillist said " The Maximum LM can be only 6 when the parameter NCOM equal to 49. So question is how large the NCOM&nbsp;should be when LM set to be 8.
<P>Yanming&nbsp;&nbsp;
<P>&nbsp;<B><I>Saeid Jalali <SJALALI@CC.IUT.AC.IR></I></B>wrote:
<BLOCKQUOTE style="PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #1010ff 2px solid">
<META content="MSHTML 6.00.2600.0" name=GENERATOR>
<STYLE></STYLE>

<DIV>&gt;I am&nbsp; using the AIM program in WIEN2k. When I calculated the critical points for some materials. The&nbsp;AIM runs without &gt;stopping. I know the discontinuities appear at the sphere boundary. According to the User guides&nbsp;of wien2k, I have gotten &gt;the as little "core-leakage" as possible from LSTART. But I don't know how to increase properly the default LM-list to &gt;LM=8 or 10 without causing other problems.&nbsp;</DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>To make LM=8&nbsp;one needs to change&nbsp;LM combinations in case.in2 file as follows:</FONT></DIV>
<DIV><FONT face=Courier size=1>
<P align=left>0 0 2 0 2 2 4 0 4 2 4 4 6 0 6 2 6 4 6 6 8 0 8 2 8 4 8 6 8 8</P>
<P align=left>0 0 1 0 2 0 2 2 3 0 3 2 4 0 4 2 4 4 5 0 5 2 5 4 6 0 6 2 6 4 6 6 7 0 7 2 7 4 7 6 8 0 8 2 8 4 8 6 8 8</P>
<P align=left><FONT face=Arial size=2>One can follow the logic to make higher LM combinations.</FONT></P>
<P align=left><FONT face=Arial size=2>Your,</FONT></P>
<P align=left><FONT face=Arial size=2>S. Jalali.</FONT></FONT><FONT face=URWPalladioL-Roma></P></FONT></DIV></BLOCKQUOTE><p><br><hr size=1><b>Do You Yahoo!?</b><br>
<a href="http://rd.yahoo.com/finance/mailsig/new/*http://finance.yahoo.com">Yahoo! Finance</a> - Get real-time stock quotes
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Date: Thu, 5 Sep 2002 19:27:21 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: How to increase the default LM-list to LM =8 or 10

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

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	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

> Do I need change the NCOM in param.inc file? I remeber someone in the =
maillist said " The Maximum LM can be only 6=20
>when the parameter NCOM equal to 49. So question is how large the NCOM =
should be when LM set to be 8.

Default used number of LM components in charge representation is 91, =
which must satisfy the following condition:
NCOM+3>(number of LM with m=3D0)+2*(number of LM with m>0)

Now, let's check it for your LM=3D8 case:
NCOM+3=3D91+3=3D94 which is for sure grater than (9)+2*(16)=3D41.
I am not sure if one should also count the combination with negative M =
or not, but still 94 is grater than (9)+4*(16)=3D73.
So you would go ahead, or at least give the later suspection a check for =
LM>8.
Your,
S. jalali.


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<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
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<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV>&gt;&nbsp;Do I need change the NCOM in param.inc file? I remeber =
someone in=20
the maillist said " The Maximum LM can be only 6 </DIV>
<DIV>&gt;when the parameter NCOM equal to 49. So question is how large =
the=20
NCOM&nbsp;should be when LM set to be 8.</DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV>Default used number of LM components in charge =
representation&nbsp;is 91,=20
which&nbsp;must satisfy the following condition:</DIV>
<DIV>NCOM+3&gt;(number of LM with m=3D0)+2*(number of LM with =
m&gt;0)</DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV>Now, let's check it for your LM=3D8 case:</DIV>
<DIV><FONT face=3DArial size=3D2>NCOM+3<FONT face=3D"Times New Roman" =
size=3D3>=3D91+3=3D94=20
which is for sure grater than</FONT> (9)+2*(16)=3D41.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>I am not sure if one should also =
count&nbsp;the=20
combination with negative M or not, but still 94 is grater than=20
(9)+4*(16)=3D73.</FONT></DIV>
<DIV><FONT face=3DURWPalladioL-Roma size=3D2><FONT face=3DArial>So you =
would go ahead,=20
or at least give&nbsp;the later suspection&nbsp;a check for=20
LM&gt;8.</FONT></FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Your,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>S. jalali.</FONT></DIV>
<DIV><FONT face=3DURWPalladioL-Roma size=3D2><FONT=20
face=3DArial></FONT>&nbsp;</DIV></FONT></BODY></HTML>

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Date: Thu, 5 Sep 2002 11:21:13 -0400
From: Jeff Spirko <spirko@lehigh.edu>
Subject: Re: [WIEN]: How to increase the default LM-list to LM =8 or 10

====
Jeff Spirko <spirko@lehigh.edu>
submitted the following contribution:
====

On Thu, Sep 05, 2002 at 10:26:28AM +0430, Saeid Jalali wrote:
>    >I am  using the AIM program in WIEN2k. When I calculated the critical
>    points  for some materials. The AIM runs without >stopping. I know the
>    discontinuities  appear  at the sphere boundary. According to the User
>    guides of  wien2k,  I  have  gotten  >the  as little "core-leakage" as
>    possible  from  LSTART.  But I don't know how to increase properly the
>    default LM-list to >LM=8 or 10 without causing other problems.

>    To  make  LM=8 one needs to change LM combinations in case.in2 file as
>    follows:
>    0 0 2 0 2 2 4 0 4 2 4 4 6 0 6 2 6 4 6 6 8 0 8 2 8 4 8 6 8 8
>    0  0 1 0 2 0 2 2 3 0 3 2 4 0 4 2 4 4 5 0 5 2 5 4 6 0 6 2 6 4 6 6 7 0 7
>    2 7 4 7 6 8 0 8 2 8 4 8 6 8 8

This is not necessarily true.  You need to look at the symmetry of
the atom (in the .outputs file) and pick the correct LM list from
the WIEN2k usersguide (Section 7.4 on lapw2).

- -- 
Jeff Spirko   spirko@lehigh.edu   spirko@yahoo.com   WD3V   |=>

The study of non-linear physics is like the study of non-elephant biology.

All theoretical chemistry is really physics;
and all theoretical chemists know it. -- Richard P. Feynman 
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Date: Fri, 6 Sep 2002 03:01:19 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: How to increase the default LM-list to LM =8 or 10

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====


> On Thu, Sep 05, 2002 at 10:26:28AM +0430, Saeid Jalali wrote:
> >    >I am  using the AIM program in WIEN2k. When I calculated the
critical
> >    points  for some materials. The AIM runs without >stopping. I know
the
> >    discontinuities  appear  at the sphere boundary. According to the
User
> >    guides of  wien2k,  I  have  gotten  >the  as little "core-leakage"
as
> >    possible  from  LSTART.  But I don't know how to increase properly
the
> >    default LM-list to >LM=8 or 10 without causing other problems.
>
> >    To  make  LM=8 one needs to change LM combinations in case.in2 file
as
> >    follows:
> >    0 0 2 0 2 2 4 0 4 2 4 4 6 0 6 2 6 4 6 6 8 0 8 2 8 4 8 6 8 8
> >    0  0 1 0 2 0 2 2 3 0 3 2 4 0 4 2 4 4 5 0 5 2 5 4 6 0 6 2 6 4 6 6 7 0
7
> >    2 7 4 7 6 8 0 8 2 8 4 8 6 8 8
>
> This is not necessarily true.  You need to look at the symmetry of
> the atom (in the .outputs file) and pick the correct LM list from
> the WIEN2k usersguide (Section 7.4 on lapw2).

Yes, certainly the LM list depends on the point group of the atom, which is
considered by the symmetry program to generate a right LM list for each
inequivalent atom. Thus, it is easier to use the generated list in the in2
file, and just follow the logic of the list to add more combinations to the
list(s) instead of using those complicated tables. Two above listed LM's are
just an example to show how one would follow the logic, and I would here to
thank you for your on time alert. Indeed, lower symmetry corresponds to
longer list. This means that lower symmetry corresponds to higher splitting.
This says that lower symmetry corresponds to more irreducible
representations, which are absolutely depending on the symmetry. For example
in the worst case with no any symmetries one easily sees that for L=6 there
are exactly 49 LM pairs: To show this I am willing to sum the (2L+1) from
L=0 to L=6:

(0+1)+(2*1+1)+(2*2+1)+(2*3+1)+(2*4+1)+(2*5+1)+(2*6+1)=1+3+5+7+9+11+13=49.



>I am not sure if one should also count the combination with negative M or
not



I have checked it out generating many case.in2 files form various
case.struct with different ISPLITs, and found that negative M's are also
considered by the program if they are needed. It is worth to mention that
since the number of LM lists are equal to the number of  inequivalent atoms,
one considers the lowest symmetry or longest LM list to count the LM
combination to check the condition on NCOM: I had done it for the above two
LM lists as an example in my last email.

Your,

S. Jalali.


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Date: Thu, 5 Sep 2002 16:30:24 -0700 (PDT)
From: Michelle Johannes <johannes@maugre.ucdavis.edu>
Subject: [WIEN]: monoclinic cell

====
Michelle Johannes <johannes@maugre.ucdavis.edu>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---307652566-650165112-1031268624=:6826
Content-Type: TEXT/PLAIN; charset=US-ASCII

Dear Wien users:
	I am trying to calculate a monoclinic cell with b as the unique
axis.  The space group is #14, but I am unsure of the setting, although I
know that I want b to be the unique axis (beta is not 90).  Therefore, I
decided to simply put in all the positions by hand rather than selecting a
specific group.  Here is the relevant part of the .struct file:

P   LATTICE,NONEQUIV. ATOMS: 1
MODE OF CALC=RELA
 12.545897 12.893606 11.939294 90.000000104.000000 90.000000


However when I do this and then run sgroup, the output
switches the labels of my axes and angles.  I think it orders them
according to length, with a being the shortest.  Since my b axis is
longest, it is called "c" in the output and though I input beta=104, the
output shows gamma=104:

Bravais lattice: Monoclinic primitive

     a             b            c
 15.08216567    12.54589700   12.89360600
     alpha         beta         gamma
 90.00000000    90.00000000   129.81621960


I have no problem with the renaming of the axes since the angle is
consistent, but should I now switch my atomic coordinates or is it reading
them properly?  I am attaching my .struct file and the .outputsgroup file
in case my explanation is not clear.

	Thank you for your help,
		Michelle


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------------------------------

Date: Fri, 6 Sep 2002 11:08:03 +0200 (CEST)
From: Georg Madsen <gmadsen@zeus.theochem.tuwien.ac.at>
Subject: Re: [WIEN]: monoclinic cell

====
Georg Madsen <gmadsen@zeus.theochem.tuwien.ac.at>
submitted the following contribution:
====

> I have no problem with the renaming of the axes since the angle is
> consistent, but should I now switch my atomic coordinates or is it reading
> them properly?  I am attaching my .struct file and the .outputsgroup file
> in case my explanation is not clear.
If you use the new axes you should also use new coordinates. I guess your
case.struct_sgroup should have the correct new structure.

 Georg

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Date: Fri, 06 Sep 2002 12:43:59 +0200
From: Enrique Lomba <E.Lomba@iqfr.csic.es>
Subject: [WIEN]: Single atom calculations

====
Enrique Lomba <E.Lomba@iqfr.csic.es>
submitted the following contribution:
====

Dear Wien users,
could someone give me some advice on how to calculate single atom 
energies to get a proper cohesive energy calculation ? I read in the 
manual that one should use a sufficiently large fcc cell (how large is 
sufficiently large ?? one must use trial and error ? and another 
question ? does one have to keep the same RMT and no. of k-points than 
in the calculation for the solid whose cohesive energy one wants to 
determine ? One would then have a relatively large number of local 
orbitals in the base .... any help will be appreciated, thanks in advance !
			Enrique


- -- 
- --------------------------------------------------------------
Enrique Lomba
Instituto de Quimica Fisica Rocasolano, CSIC
C/ Serrano 119, 28006 Madrid, Spain

FAX no. 34-915642431
Phone no. 34-915619407 (ext 1301)
e-mail : E.Lomba@iqfr.csic.es
www : http://www.fluid.iqfr.csic.es/enrique.html

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------------------------------

Date: Fri, 6 Sep 2002 06:07:45 -0700 (PDT)
From: yanming Ma <ymma66@yahoo.com>
Subject: Re: [WIEN]: How to increase the default LM-list to LM =8 or 10

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-1660464621-1031317665=:80998
Content-Type: text/plain; charset=us-ascii


Dear Saeid and Jeff,
Thanks very much for your excellent explainations for the LM combination.
Best wishes
Yanming Ma
 Saeid Jalali wrote:====
"Saeid Jalali" 
submitted the following contribution:
====


> On Thu, Sep 05, 2002 at 10:26:28AM +0430, Saeid Jalali wrote:
> > >I am using the AIM program in WIEN2k. When I calculated the
critical
> > points for some materials. The AIM runs without >stopping. I know
the
> > discontinuities appear at the sphere boundary. According to the
User
> > guides of wien2k, I have gotten >the as little "core-leakage"
as
> > possible from LSTART. But I don't know how to increase properly
the
> > default LM-list to >LM=8 or 10 without causing other problems.
>
> > To make LM=8 one needs to change LM combinations in case.in2 file
as
> > follows:
> > 0 0 2 0 2 2 4 0 4 2 4 4 6 0 6 2 6 4 6 6 8 0 8 2 8 4 8 6 8 8
> > 0 0 1 0 2 0 2 2 3 0 3 2 4 0 4 2 4 4 5 0 5 2 5 4 6 0 6 2 6 4 6 6 7 0
7
> > 2 7 4 7 6 8 0 8 2 8 4 8 6 8 8
>
> This is not necessarily true. You need to look at the symmetry of
> the atom (in the .outputs file) and pick the correct LM list from
> the WIEN2k usersguide (Section 7.4 on lapw2).

Yes, certainly the LM list depends on the point group of the atom, which is
considered by the symmetry program to generate a right LM list for each
inequivalent atom. Thus, it is easier to use the generated list in the in2
file, and just follow the logic of the list to add more combinations to the
list(s) instead of using those complicated tables. Two above listed LM's are
just an example to show how one would follow the logic, and I would here to
thank you for your on time alert. Indeed, lower symmetry corresponds to
longer list. This means that lower symmetry corresponds to higher splitting.
This says that lower symmetry corresponds to more irreducible
representations, which are absolutely depending on the symmetry. For example
in the worst case with no any symmetries one easily sees that for L=6 there
are exactly 49 LM pairs: To show this I am willing to sum the (2L+1) from
L=0 to L=6:

(0+1)+(2*1+1)+(2*2+1)+(2*3+1)+(2*4+1)+(2*5+1)+(2*6+1)=1+3+5+7+9+11+13=49.



>I am not sure if one should also count the combination with negative M or
not



I have checked it out generating many case.in2 files form various
case.struct with different ISPLITs, and found that negative M's are also
considered by the program if they are needed. It is worth to mention that
since the number of LM lists are equal to the number of inequivalent atoms,
one considers the lowest symmetry or longest LM list to count the LM
combination to check the condition on NCOM: I had done it for the above two
LM lists as an example in my last email.

Your,

S. Jalali.


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- --0-1660464621-1031317665=:80998
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<P>Dear Saeid and Jeff,
<P>Thanks very much for your excellent explainations for the LM combination.
<P>Best wishes
<P>Yanming Ma
<P>&nbsp;<B><I>Saeid Jalali <SJALALI@CC.IUT.AC.IR></I></B>wrote:
<BLOCKQUOTE style="PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #1010ff 2px solid">====<BR>"Saeid Jalali" <SJALALI@CC.IUT.AC.IR><BR>submitted the following contribution:<BR>====<BR><BR><BR>&gt; On Thu, Sep 05, 2002 at 10:26:28AM +0430, Saeid Jalali wrote:<BR>&gt; &gt; &gt;I am using the AIM program in WIEN2k. When I calculated the<BR>critical<BR>&gt; &gt; points for some materials. The AIM runs without &gt;stopping. I know<BR>the<BR>&gt; &gt; discontinuities appear at the sphere boundary. According to the<BR>User<BR>&gt; &gt; guides of wien2k, I have gotten &gt;the as little "core-leakage"<BR>as<BR>&gt; &gt; possible from LSTART. But I don't know how to increase properly<BR>the<BR>&gt; &gt; default LM-list to &gt;LM=8 or 10 without causing other problems.<BR>&gt;<BR>&gt; &gt; To make LM=8 one needs to change LM combinations in case.in2 file<BR>as<BR>&gt; &gt; follows:<BR>&gt; &gt; 0 0 2 0 2 2 4 0 4 2 4 4 6 0 6 2 6 4 6 6 8 0 8 2 8 4 8 6 8 8<BR>&gt; &gt; 0 0 1 0 2 0 2 2 3!
 0 3 2 4 0 4 2 4 4 5 0 5 2 5 4 6 0 6 2 6 4 6 6 7 0<BR>7<BR>&gt; &gt; 2 7 4 7 6 8 0 8 2 8 4 8 6 8 8<BR>&gt;<BR>&gt; This is not necessarily true. You need to look at the symmetry of<BR>&gt; the atom (in the .outputs file) and pick the correct LM list from<BR>&gt; the WIEN2k usersguide (Section 7.4 on lapw2).<BR><BR>Yes, certainly the LM list depends on the point group of the atom, which is<BR>considered by the symmetry program to generate a right LM list for each<BR>inequivalent atom. Thus, it is easier to use the generated list in the in2<BR>file, and just follow the logic of the list to add more combinations to the<BR>list(s) instead of using those complicated tables. Two above listed LM's are<BR>just an example to show how one would follow the logic, and I would here to<BR>thank you for your on time alert. Indeed, lower symmetry corresponds to<BR>longer list. This means that lower symmetry corresponds to higher splitting.<BR>This says that lower symmetry corresponds to mor!
e irreducible<BR>representations, which are absolutely depending on the symmetry. For example<BR>in the worst case with no any symmetries one easily sees that for L=6 there<BR>are exactly 49 LM pairs: To show this I am willing to sum the (2L+1) from<BR>L=0 to L=6:<BR><BR>(0+1)+(2*1+1)+(2*2+1)+(2*3+1)+(2*4+1)+(2*5+1)+(2*6+1)=1+3+5+7+9+11+13=49.<BR><BR><BR><BR>&gt;I am not sure if one should also count the combination with negative M or<BR>not<BR><BR><BR><BR>I have checked it out generating many case.in2 files form various<BR>case.struct with different ISPLITs, and found that negative M's are also<BR>considered by the program if they are needed. It is worth to mention that<BR>since the number of LM lists are equal to the number of inequivalent atoms,<BR>one considers the lowest symmetry or longest LM list to count the LM<BR>combination to check the condition on NCOM: I had done it for the above two<BR>LM lists as an example in my last email.<BR><BR>Your,<BR><BR>S. Jalali.<BR><!
BR><BR>====<BR>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at<BR>To (un)subscribe send mail to<BR>majordomo@zeus.theochem.tuwien.ac.at<BR>====</BLOCKQUOTE><p><br><hr size=1><b>Do You Yahoo!?</b><br>
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Date: Fri, 6 Sep 2002 06:07:59 -0700 (PDT)
From: yanming Ma <ymma66@yahoo.com>
Subject: Re: [WIEN]: How to increase the default LM-list to LM =8 or 10

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

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Dear Saeid and Jeff, 
Thanks very much for your excellent explainations for the LM combination. 
Best wishes 
Yanming Ma 
 Saeid Jalali wrote: ====
"Saeid Jalali" 
submitted the following contribution:
====


> On Thu, Sep 05, 2002 at 10:26:28AM +0430, Saeid Jalali wrote:
> > >I am using the AIM program in WIEN2k. When I calculated the
critical
> > points for some materials. The AIM runs without >stopping. I know
the
> > discontinuities appear at the sphere boundary. According to the
User
> > guides of wien2k, I have gotten >the as little "core-leakage"
as
> > possible from LSTART. But I don't know how to increase properly
the
> > default LM-list to >LM=8 or 10 without causing other problems.
>
> > To make LM=8 one needs to change LM combinations in case.in2 file
as
> > follows:
> > 0 0 2 0 2 2 4 0 4 2 4 4 6 0 6 2 6 4 6 6 8 0 8 2 8 4 8 6 8 8
> > 0 0 1 0 2 0 2 2 3 0 3 2 4 0 4 2 4 4 5 0 5 2 5 4 6 0 6 2 6 4 6 6 7 0
7
> > 2 7 4 7 6 8 0 8 2 8 4 8 6 8 8
>
> This is not necessarily true. You need to look at the symmetry of
> the atom (in the .outputs file) and pick the correct LM list from
> the WIEN2k usersguide (Section 7.4 on lapw2).

Yes, certainly the LM list depends on the point group of the atom, which is
considered by the symmetry program to generate a right LM list for each
inequivalent atom. Thus, it is easier to use the generated list in the in2
file, and just follow the logic of the list to add more combinations to the
list(s) instead of using those complicated tables. Two above listed LM's are
just an example to show how one would follow the logic, and I would here to
thank you for your on time alert. Indeed, lower symmetry corresponds to
longer list. This means that lower symmetry corresponds to higher splitting.
This says that lower symmetry corresponds to more irreducible
representations, which are absolutely depending on the symmetry. For example
in the worst case with no any symmetries one easily sees that for L=6 there
are exactly 49 LM pairs: To show this I am willing to sum the (2L+1) from
L=0 to L=6:

(0+1)+(2*1+1)+(2*2+1)+(2*3+1)+(2*4+1)+(2*5+1)+(2*6+1)=1+3+5+7+9+11+13=49.



>I am not sure if one should also count the combination with negative M or
not



I have checked it out generating many case.in2 files form various
case.struct with different ISPLITs, and found that negative M's are also
considered by the program if they are needed. It is worth to mention that
since the number of LM lists are equal to the number of inequivalent atoms,
one considers the lowest symmetry or longest LM list to count the LM
combination to check the condition on NCOM: I had done it for the above two
LM lists as an example in my last email.

Your,

S. Jalali.


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<P>Dear Saeid and Jeff, 
<P>Thanks very much for your excellent explainations for the LM combination. 
<P>Best wishes 
<P>Yanming Ma 
<P>&nbsp;<B><I>Saeid Jalali <SJALALI@CC.IUT.AC.IR></I></B>wrote: 
<BLOCKQUOTE style="PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #1010ff 2px solid">====<BR>"Saeid Jalali" <SJALALI@CC.IUT.AC.IR><BR>submitted the following contribution:<BR>====<BR><BR><BR>&gt; On Thu, Sep 05, 2002 at 10:26:28AM +0430, Saeid Jalali wrote:<BR>&gt; &gt; &gt;I am using the AIM program in WIEN2k. When I calculated the<BR>critical<BR>&gt; &gt; points for some materials. The AIM runs without &gt;stopping. I know<BR>the<BR>&gt; &gt; discontinuities appear at the sphere boundary. According to the<BR>User<BR>&gt; &gt; guides of wien2k, I have gotten &gt;the as little "core-leakage"<BR>as<BR>&gt; &gt; possible from LSTART. But I don't know how to increase properly<BR>the<BR>&gt; &gt; default LM-list to &gt;LM=8 or 10 without causing other problems.<BR>&gt;<BR>&gt; &gt; To make LM=8 one needs to change LM combinations in case.in2 file<BR>as<BR>&gt; &gt; follows:<BR>&gt; &gt; 0 0 2 0 2 2 4 0 4 2 4 4 6 0 6 2 6 4 6 6 8 0 8 2 8 4 8 6 8 8<BR>&gt; &gt; 0 0 1 0 2 0 2 2 3!
 0 3 2 4 0 4 2 4 4 5 0 5 2 5 4 6 0 6 2 6 4 6 6 7 0<BR>7<BR>&gt; &gt; 2 7 4 7 6 8 0 8 2 8 4 8 6 8 8<BR>&gt;<BR>&gt; This is not necessarily true. You need to look at the symmetry of<BR>&gt; the atom (in the .outputs file) and pick the correct LM list from<BR>&gt; the WIEN2k usersguide (Section 7.4 on lapw2).<BR><BR>Yes, certainly the LM list depends on the point group of the atom, which is<BR>considered by the symmetry program to generate a right LM list for each<BR>inequivalent atom. Thus, it is easier to use the generated list in the in2<BR>file, and just follow the logic of the list to add more combinations to the<BR>list(s) instead of using those complicated tables. Two above listed LM's are<BR>just an example to show how one would follow the logic, and I would here to<BR>thank you for your on time alert. Indeed, lower symmetry corresponds to<BR>longer list. This means that lower symmetry corresponds to higher splitting.<BR>This says that lower symmetry corresponds to mor!
e irreducible<BR>representations, which are absolutely depending on the symmetry. For example<BR>in the worst case with no any symmetries one easily sees that for L=6 there<BR>are exactly 49 LM pairs: To show this I am willing to sum the (2L+1) from<BR>L=0 to L=6:<BR><BR>(0+1)+(2*1+1)+(2*2+1)+(2*3+1)+(2*4+1)+(2*5+1)+(2*6+1)=1+3+5+7+9+11+13=49.<BR><BR><BR><BR>&gt;I am not sure if one should also count the combination with negative M or<BR>not<BR><BR><BR><BR>I have checked it out generating many case.in2 files form various<BR>case.struct with different ISPLITs, and found that negative M's are also<BR>considered by the program if they are needed. It is worth to mention that<BR>since the number of LM lists are equal to the number of inequivalent atoms,<BR>one considers the lowest symmetry or longest LM list to count the LM<BR>combination to check the condition on NCOM: I had done it for the above two<BR>LM lists as an example in my last email.<BR><BR>Your,<BR><BR>S. Jalali.<BR><!
BR><BR>====<BR>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at<BR>To (un)subscribe send mail to<BR>majordomo@zeus.theochem.tuwien.ac.at<BR>====</BLOCKQUOTE><p><br><hr size=1><b>Do You Yahoo!?</b><br>
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------------------------------

Date: Fri, 6 Sep 2002 21:22:55 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Single atom calculations

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> could someone give me some advice on how to calculate single atom
> energies to get a proper cohesive energy calculation ? I read in the
> manual that one should use a sufficiently large fcc cell (how large is
> sufficiently large ?? one must use trial and error ?
For a quick guess about cohesive energy one can look at the output file of
the atomic lstart program to find atomic energies. But it is not an accurate
way as it is suffering with two different methods of energy calculation:
fully relativistic Dirack-Fock method for calculating atomic energies and
Scalar relativistic FP-LAPW method for calculating total bulk energy. It is
not expected from two individual approaches to obtain an energy, thus it is
suggested by the author to calculate also atomic energies within FP-LAPW to
use cancellation error. Calculating atomic energy within bulk total energy
calculation needs to make a supercell to avoid interacting each atom with
its nearest neighbors to mimic an free atom. In general, one would check the
convergence of the calculated total atomic energy through various lattice
parameters of the supercell to make sure that there is not any interaction
between the atom with the others. You would use F, B, P, or any other space
groups to make supercell for such a simple calculation, but I also have
found F more suitable. Basically, to obtain an accurate atomic energy using
a vary large lattice parameter helps, but starting from a doubled lattice
parameter looks good.

> and another
> question ? does one have to keep the same RMT and no. of k-points than
> in the calculation for the solid whose cohesive energy one wants to
> determine ?

The point is to use cancellation error as much as possible. For bulk
calculation one first finds suitable no. of k-points. This can be the case
also for atomic calculation. About the RMT I think it looks more reasonable
to keep the V_RMT/V_cell: V is Volume. However, according to my experience
using the same RMT's is not bad.



Your,

S. Jalali.




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------------------------------

Date: Fri, 6 Sep 2002 21:27:54 +0200 (MEST)
From: Pio =?ISO-8859-1?Q?B=E4ttig?= <baettigp@gmx.net>
Subject: [WIEN]: Bandstructure plotting

====
Pio =?ISO-8859-1?Q?B=E4ttig?= <baettigp@gmx.net>
submitted the following contribution:
====

Dear Wien users
I encounter a small problem when trying to plot bands with characters (using
Wien2k_02_130802), I can't manage to get wider lines, they stay at standard
thickness. My case.insp file looks as follows:

- -------
### Figure configuration
 5.0   3.0                         # paper offset of plot
10.0  15.0                         # xsize,ysize of plot [cm]
 1.0   4                           # major ticks, minor ticks
 1.0   1                           # character height, font switch
 1.1   1    0                      # line width, line switch, color switch
### Data configuration
  0.0 1.6  1                      # energy range, energy switch (1:Ry, 2:eV)
1      0.70914                     # Fermi switch,  Fermi-level (in Ry
units)
1   999                            # number of bands for heavier plotting 
1,1
2      4    0.2                    # jatom, jtype, size  of heavier plotting
- -------
In the last line (size of heavier plotting), I tried 0.2, 0.4, 3, without
effect. 
The relevant 4 lines from case.qtlup are the following:

- -------
 JATOM= 1  MULT= 2  ISPLIT= 2  tot,0,1,2,D-eg,D-t2g,3
 JATOM= 2  MULT= 1  ISPLIT= 2  tot,0,1,2,D-eg,D-t2g,3
 JATOM= 3  MULT= 1  ISPLIT= 2  tot,0,1,2,D-eg,D-t2g,3
 JATOM= 4  MULT= 6  ISPLIT=-2  tot,0,1,PZ,PX+PY,2,DZ2,DXY,DX2Y2,DXZ+DYZ,3
- -------
I think I might be forgetting something small, but can't figure out what.

Thank you very much for any hint.

Pio Baettig

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------------------------------

Date: Fri, 6 Sep 2002 19:52:19 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: Bandstructure plotting

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====

> I can't manage to get wider lines, they stay at standard thickness. My
> case.insp file looks as follows:
>
> <snip>
>
>  1.1   1    0                      # line width, line switch, color switch

Instead, try:

1.1   2    0                      # line width, line switch, color switch

Choice 1 for the line switch denotes just lines. The character plotting
uses circles, given by switch 2, to denote the character.

> 2      4    0.2                    # jatom, jtype, size  of heavier
> plotting -------
> In the last line (size of heavier plotting), I tried 0.2, 0.4, 3, without
> effect.

A size of 0.2 should be enough.

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------------------------------

Date: Wed, 11 Sep 2002 00:14:48 +0500
From: "Rashid Ahmed" <rasofi@hotmail.com>
Subject: [none]

====
"Rashid Ahmed" <rasofi@hotmail.com>
submitted the following contribution:
====

This is a multi-part message in MIME format.

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------------------------------

End of wien-digest V2002 #34
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #35
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
Errors-To: owner-wien-digest@theochem.tuwien.ac.at
Precedence: bulk


wien-digest      Wednesday, September 18 2002      Volume 2002 : Number 035




----------------------------------------------------------------------

Date: Wed, 11 Sep 2002 07:40:42 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: [none]

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====



Dear wien2k users:
   In the latest version of wien2k,how to calculate the DOS? According to 
Peter,there have changed in wien2k like this:

   "The total spin-up / dn DOS could not be calculated in a spinpolarized
 spin-orbit calculation (since each qtlup/dn file contains all eigenvalues.
 We write now into case.qtlup/dn the up and dn-spin "norm" of each
 eigenvalue into case.qtlup (at the position of "q-interstital", which was
 not correct anyway in SO calculations). TETRA reads now in spinpol. SO 
cases (only then) for the "total DOS" these norms and produces a spin-up or 
dn total DOS."

 but this donn't point out how to get DOS in this wien2k, can somebody eles 
give me some help? when I run : x lapw2 -c -up -qtl, there is always error 
message.




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------------------------------

Date: Wed, 11 Sep 2002 01:37:20 -0700 (PDT)
From: romdhani hedi <hedi_romdhani2002@yahoo.com>
Subject: [WIEN]: ROTDEF ERROR

====
romdhani hedi <hedi_romdhani2002@yahoo.com>
submitted the following contribution:
====

- --0-1229455378-1031733440=:6288
Content-Type: text/plain; charset=us-ascii
Content-Disposition: inline

Dear wien users,
 I am interested of optical properties of In2S3
 compound using the WIEN97 code. When I execute the
 program joint errors appear. In order to clarify the
 problem I send the In2S3.struct file.
 Best Regards.


__________________________________________________
Yahoo! - We Remember
9-11: A tribute to the more than 3,000 lives lost
http://dir.remember.yahoo.com/tribute
- --0-1229455378-1031733440=:6288
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- --0-1229455378-1031733440=:6288--
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------------------------------

Date: Wed, 11 Sep 2002 13:16:18 +0200
From: Claudia Ambrosch-Draxl <claudia.ambrosch@uni-graz.at>
Subject: Re: [WIEN]: ROTDEF ERROR

====
Claudia Ambrosch-Draxl <claudia.ambrosch@uni-graz.at>
submitted the following contribution:
====

romdhani hedi wrote:
> 
> Dear wien users,
>  I am interested of optical properties of In2S3
>  compound using the WIEN97 code. When I execute the
>  program joint errors appear. In order to clarify the
>  problem I send the In2S3.struct file.
>  Best Regards.
> 
This error usually appeared in the old version when the NMAT parameter
was set too small.

Regards,
Claudia Ambrosch-Draxl

Institut f. Theoretische Physik, University Graz
Universitaetsplatz 5, A-8010 Graz
Tel. [43] (316) 380-5235    Fax [43] (316) 380-9820
http://physik.uni-graz.at/~cad
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Date: Wed, 11 Sep 2002 05:25:22 -0700 (PDT)
From: morteza jamal <m_jamal23@yahoo.com>
Subject: [WIEN]: P1/2 calculations

====
morteza jamal <m_jamal23@yahoo.com>
submitted the following contribution:
====

Dear Wien2k users.
We know that using P1/2 orbitals is not true for
calculating EFG.
Is there any other parameters that can not be
calculated using P1/2 orbitals?
Specially i want to know that in HFF(Hyperfine)
calculations P1/2 orbitals can be used or not.

Best wishes.
Morteza Jamal.

__________________________________________________
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9-11: A tribute to the more than 3,000 lives lost
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Date: Wed, 11 Sep 2002 08:16:05 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]: runsp -so -orb

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

In fact, a switch to run lapwdm even without -orb
would be useful. It takes no time and helps monitor
convergence of the orbital moment. 

Igor

- --- Peter Blaha <pblaha@theochem.tuwien.ac.at> wrote:
> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> > Why is only "lapwdm -c -up -so"  called during
> "runsp_c_lapw -so -orb" and
> > not "lapwdm -c -dn -so" looking at :log?
> 
> lapwdm calculates the density matrices inside
> spheres. This is needed ONLY
> for the orbital potentials, not for a standard
> LDA(GGA) calculation, even
> when spin-orbit is included.
> 
> After runsp -so has finished, one can use lapwdm to
> calculate an orbital
> moment, but there is no need to do this during scf.
> 
> Regards
> 
> 
>                                       P.Blaha
>
- --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna,
> A-1060 Vienna
> Phone: +43-1-58801-15671             FAX:
> +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
> http://info.tuwien.ac.at/theochem/
>
- --------------------------------------------------------------------------
> 
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====


=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

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------------------------------

Date: Thu, 12 Sep 2002 10:55:59 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question about SCF convergence

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Hi,

I would like to consult about SCF convergence. How do I know whether SCF 
calculation converge or diverge? What is the default criteria of SCF 
calculation? 

Thank you very much

Martin

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------------------------------

Date: Thu, 12 Sep 2002 11:30:06 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: [WIEN]

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Hi,

I have some question about running scf calculation.

While I am running the SCF calculation, WIEN97 generates a file with 
extension ".vec" in step LAPW1. However, this file is empty but the SCF 
calculation still continues. Is it neccessary to key-in some command to  
print the eigenvector out?  

Thank you very much

Martin

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------------------------------

Date: Thu, 12 Sep 2002 10:28:32 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: [WIEN]

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> While I am running the SCF calculation, WIEN97 generates a file with
> extension ".vec" in step LAPW1. However, this file is empty but the SCF
> calculation still continues. Is it neccessary to key-in some command to
> print the eigenvector out?
As far as I know, we in wien code don't have a file with such an extension.
Instead case.vector is a necessarily generated file by lapw1 containing the
eigenvalues and eigenvectors of all k-points, which is necessarily needed as
an input file for lapw2. Thus, turning on a switch is not needed. In
spin-polarized calculations one looks for case.vectorup and case.vectordn
and not case.vector.

> How do I know whether SCF
>calculation converge or diverge?
grepline_lapw :DIS "*.scf" 1

>What is the default criteria of SCF calculation?
On :ENE it is 0.0001Ry.


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------------------------------

Date: Thu, 12 Sep 2002 16:30:03 +1000
From: chen0130@flinders.edu.au
Subject: [WIEN]: 'LOPW'

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Dear Wien users,

Can someone please tell me what the error message

LOPW Plane waves exhausted

for lapw1 in SCF... I have never come across it before...

Thanks,

Cheng

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Date: Thu, 12 Sep 2002 08:40:19 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: 'LOPW'

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Can someone please tell me what the error message
>
> LOPW Plane waves exhausted
>
> for lapw1 in SCF... I have never come across it before...

Usually, that your struct file is incorrect.(Contains the same atom twice,
not proper symmetry, equivalent atoms,....)

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Thu, 12 Sep 2002 08:56:39 +0200
From: Gilles Hug <gilles.hug@onera.fr>
Subject: [WIEN]: Re: Wien2k & MacOs X

====
Gilles Hug <gilles.hug@onera.fr>
submitted the following contribution:
====

Dear Ching-Tarng & Dieter,


At 18:28 +0200 11/09/02, Liang Ching-Tarng wrote:
>Dear Gilles Hug,
>
>we are trying to use WIEN2k-code on MacOs X (10.1)
>and the Absoft80-Compiler, some recent version(beta?) or demo
>to start with.
>
>Your suggestion in siteconfig_lapw is
>
># as suggested by Gilles Hug  gilles.hug@onera.fr there
>macg4:FC:f95
>macg4:MPF:f95
>macg4:CC:cc
>macg4:FOPT:-O1 -cons -lU77 -w -ffree -N11 -YEXT_SFX='_' -YEXT_NAMES=LCS
>macg4:FPOPT:
>macg4:LDFLAGS:-llapack -lf90math_altivec -lblas_altivec -lfio -lf77math -lU77
>macg4:R_LIBS: -llapack -lf90math_altivec -lblas_altivec -lfio -lf77math -lU77
>macg4:DPARALLEL:
>macg4:RP_LIBS:
>macg4:MPIRUN:mpirun -np _NP_ -machinefile _HOSTS_ _EXEC_
>
>and the compilation is without any problems, except "optic", but
>this is not important and could be fixed. The real problem is we cannot
>run WIEN, lstart ends with a segmentation fault.
>Did you have similar problems?

Yes, Absoft said they have a bug in their compiler which should be 
fixed now. But I have not yet the lastest version.

>Maybe it has to do with the stack size? Should one not compile
>with the static-option -s? We did not understand your option -cons,

Yes, I had put the following lines in my .tcshrc


limit stacksize unlimited
limit datasize unlimited

Please try teh -s option I didn't.

>macg4:FOPT:-O1 -cons -lU77 -w -ffree -N11 -YEXT_SFX='_' -YEXT_NAMES=LCS
>
>looking through the usergide of Absoft-f95.


Ok. May not necessary. I can't find anymore what this option is for.
Acrually I stop searching whan the code was running so...


>Do you have any suggestions? Is it worthwile to let the G4 of 933 Mhz
>do some computional work?

Of course. My old G4-500MHz runs faster than the Dec-alpha (also old) 
as long as I don't use complex calculation. unfortunately Altivec is 
not used for double. This is a limitation. I'm installing Jaguar now 
and it seems significantly faster (the system, I guess not plain 
calculations). And I kind of love the new Mail with IA to clear all 
the Junk mail.

Best,
Gilles

ps : I took the liberty to send also to the Wien list as it might 
interest someone else or someone else might have additional 
improvments.

- -- 
_______________________________________________________
         Gilles Hug
         LEM, UMR 104, ONERA-CNRS, BP72
         92322 Chatillon Cedex, France
         tel : +33 1 46 73 45 42 fax : +33 1 46 73 41 55
         mailto:Gilles.Hug@onera.fr
	http://www.onera.fr/lem/anachistr/index.html
_______________________________________________________
Office National d'Etudes et de Recherches Aerospatiales
                   ------- & ------
      Centre National de la Recherche Scientifique
_______________________________________________________
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------------------------------

Date: Thu, 12 Sep 2002 09:33:52 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: runsp -so -orb

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---2105530234-990962995-1031816032=:2496
Content-Type: TEXT/PLAIN; charset=US-ASCII

> In fact, a switch to run lapwdm even without -orb
> would be useful. It takes no time and helps monitor
> convergence of the orbital moment.

Try the attached runsp_lapw script   with     runsp -so -dm
If you like it, I'll copy it into the standard distribution.
Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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- ---2105530234-990962995-1031816032=:2496--
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Date: Thu, 12 Sep 2002 18:00:39 +1000
From: chen0130@flinders.edu.au
Subject: Thanks Re: [WIEN]: 'LOPW'

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Thankyou!

Quoting Peter Blaha <pblaha@theochem.tuwien.ac.at>:

> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> > Can someone please tell me what the error message
> >
> > LOPW Plane waves exhausted
> >
> > for lapw1 in SCF... I have never come across it before...
> 
> Usually, that your struct file is incorrect.(Contains the same atom twice,
> not proper symmetry, equivalent atoms,....)
> 
> Regards
> 
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
> http://info.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
> 
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> 
> 



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Date: Thu, 12 Sep 2002 14:04:56 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: [WIEN]: bug in lapw0 for cubic magnetic cases 

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---2105530234-747226996-1031832296=:2496
Content-Type: TEXT/PLAIN; charset=US-ASCII

Dear WIEN users,

In all WIEN2k versions released so far, there is a significant bug for

CUBIC pusitions (IATNR is positive in case.struct) in SPINPOLARIZED
calculations.

(When V-xc was calculated, the spin-dn density was calculated from the
spherical spin-dn part, but with the nonspherical density contributions taken
from spin up.)

This leads e.g. for AFM-Cr to a permanent (small, like 0.01 uB) ferromagnetic
moment in an unconstraint runsp_lapw calculation.
From this experience one can estimate that cubic magnetic moments may be wrong
by up to 0.1 uB and also E-tot will be wrong by a few mRy/atom.

Please download the new SRC_lapw0.tar.gz

or replace srolyl.f with the attached file.

Regards



                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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- ---2105530234-747226996-1031832296=:2496--
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------------------------------

Date: Fri, 13 Sep 2002 06:43:33 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: DOS-dn

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started DOS -don and got this
message(PGFIO-F-231/formated read/unit=5/error on data
conversion.
 FILE Name:
home inst
Formated,sequential access record =4
In  source file tetra,at line number 90\

0.010u,0.00s....   0+0k    
 what dose it mean?or What is its reason?
What should be done for eliminating it?
Thank you for the guide.
H-Salehi 
Dept of physics
Ferdowsi University
MASHHAD IRAN



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------------------------------

Date: Fri, 13 Sep 2002 11:47:39 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: [WIEN]: <mk|sigma|nk>

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====


I'm interested in calculating spin-populations and coherences due to
optical excitations. To do this I need the quantities <mk|sigma|nk>
where |mk> are the spinor wavefunctions, and sigma is a Pauli matrix.
I am only interested in the matrix elements between states at the same
k-point.

Presumably, these quantities are somewhere in the code when m=n=valence
band, but I need them for valence and conduction bands. Does any part
of the WIEN2k code explicitly calculate this? If not, does anyone have
any hints as to where to begin if I wanted to calculate these.

Thanks,

Fred
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Date: Fri, 13 Sep 2002 21:30:00 +0000
From: "SOHAIL AFZAL" <safz@hotmail.com>
Subject: [WIEN]: Request to add in your mailing list

====
"SOHAIL AFZAL" <safz@hotmail.com>
submitted the following contribution:
====


Dear Professor,

It will be highly appreciated if you kindly add the fallowing addresses on 
your mailing list.
rasofi@hotmail.com
energy@cyber.net.pk

Hope a favorable action
With best Regards

Sohail Afzal Tahir
Centre for High Energy Physics
University of the Punjab
Quaid-i-Azam Campus
Lahore Pakistan


_________________________________________________________________
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------------------------------

Date: Fri, 13 Sep 2002 23:23:21 -0700
From: Jiang Bin <jiangb@asu.edu>
Subject: [WIEN]: Question on orientation dependence EELS calculation

====
Jiang Bin <jiangb@asu.edu>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- --Boundary_(ID_PwtEJqpq4WIw+naZPXHOeA)
Content-type: text/plain; charset=gb2312
Content-transfer-encoding: 7bit

Dear Prof.

I have question on the EELS calculation. The crystal is MgB2. 

I attached the case.struct file and case.innes file for you to check.

Several question on the orientation calculation EELS

(1) What's the Euler angle's of the observation basis and crystal basis.
(2) How to choose the Euler angle to let q//c and q//x etc.
(3) The procedure to launch programs and modification of case.struct. 
(4) for the case of "H", How to modify the files and procedure to launch
calculation (not for MgB2).
(5) is "F" follow the same procedure for calculation as "H" option.
(when should I change ISPLIT=88 in case.struct file)
(5) For Mg L-edge. Could I modify the core energy to -3.0 Ry to include
Mg-2s orbital into core orbital for EELS calculation?



- -- 

Best regards

Bin Jiang

- ---------------------------------
Department of Physics & Astronomy
Arizona State University
Tempe, AZ 85287-1504
USA
Email: jiangb@asu.edu
- ------------------------------------

- --Boundary_(ID_PwtEJqpq4WIw+naZPXHOeA)
Content-type: text/plain; charset=gb2312; name="mgb2.struct"
Content-transfer-encoding: 7bit
Content-disposition: inline; filename="mgb2.struct"

MgB2                                                                           
H   LATTICE,NONEQUIV. ATOMS: 2191_P6/mmm                                       
MODE OF CALC=RELA unit=bohr                                                    
  5.826784  5.826784  6.654295 90.000000 90.000000120.000000                   
ATOM= -1: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT= 4
Mg1        NPT=  781  R0=0.00010000 RMT=    2.0000   Z: 12.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -2: X=0.33333300 Y=0.66666700 Z=0.50000000
          MULT= 2          ISPLIT= 4
      -2: X=0.66666700 Y=0.33333300 Z=0.50000000
B 1        NPT=  781  R0=0.00010000 RMT=    1.6500   Z:  5.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
  24      NUMBER OF SYMMETRY OPERATIONS
 1 0 0 0.0000000
 0 1 0 0.0000000
 0 0 1 0.0000000
       1
 0-1 0 0.0000000
 1-1 0 0.0000000
 0 0 1 0.0000000
       2
- -1 1 0 0.0000000
- -1 0 0 0.0000000
 0 0 1 0.0000000
       3
- -1 0 0 0.0000000
 0-1 0 0.0000000
 0 0 1 0.0000000
       4
 0 1 0 0.0000000
- -1 1 0 0.0000000
 0 0 1 0.0000000
       5
 1-1 0 0.0000000
 1 0 0 0.0000000
 0 0 1 0.0000000
       6
 0 1 0 0.0000000
 1 0 0 0.0000000
 0 0-1 0.0000000
       7
 1-1 0 0.0000000
 0-1 0 0.0000000
 0 0-1 0.0000000
       8
- -1 0 0 0.0000000
- -1 1 0 0.0000000
 0 0-1 0.0000000
       9
 0-1 0 0.0000000
- -1 0 0 0.0000000
 0 0-1 0.0000000
      10
- -1 1 0 0.0000000
 0 1 0 0.0000000
 0 0-1 0.0000000
      11
 1 0 0 0.0000000
 1-1 0 0.0000000
 0 0-1 0.0000000
      12
- -1 0 0 0.0000000
 0-1 0 0.0000000
 0 0-1 0.0000000
      13
 0 1 0 0.0000000
- -1 1 0 0.0000000
 0 0-1 0.0000000
      14
 1-1 0 0.0000000
 1 0 0 0.0000000
 0 0-1 0.0000000
      15
 1 0 0 0.0000000
 0 1 0 0.0000000
 0 0-1 0.0000000
      16
 0-1 0 0.0000000
 1-1 0 0.0000000
 0 0-1 0.0000000
      17
- -1 1 0 0.0000000
- -1 0 0 0.0000000
 0 0-1 0.0000000
      18
 0-1 0 0.0000000
- -1 0 0 0.0000000
 0 0 1 0.0000000
      19
- -1 1 0 0.0000000
 0 1 0 0.0000000
 0 0 1 0.0000000
      20
 1 0 0 0.0000000
 1-1 0 0.0000000
 0 0 1 0.0000000
      21
 0 1 0 0.0000000
 1 0 0 0.0000000
 0 0 1 0.0000000
      22
 1-1 0 0.0000000
 0-1 0 0.0000000
 0 0 1 0.0000000
      23
- -1 0 0 0.0000000
- -1 1 0 0.0000000
 0 0 1 0.0000000
      24

- --Boundary_(ID_PwtEJqpq4WIw+naZPXHOeA)
Content-type: text/plain; charset=gb2312; name="mgb2.innes"
Content-transfer-encoding: 7bit
Content-disposition: inline; filename="mgb2.innes"

Title: Atom 1 K Peak
2, 1            (atom)
1               (n core)
0               (l core)
0,0.0,100       (EMIN,DE,EMAX)
190, 0, .8	(E-Loss of 1st edge, split between edges, precision, all in eV)
120		(energy of the incident electrons (keV))
0, 0		(ThetaX, ThetaY in mrad)
0		(double of Bragg angle in mrad)
0, 0, 0		(DeltaX, DeltaY, Number of cases - 1: (0=1 case))
4		(LambdaMax)
L		(L for Line and P for Plane)
N		(N: Normal (l' DOS); F: Fine (l' m' DOS); H: HyperFine ...)
0.0, 0.0, 0.0  (Euler's angles between the observator basis and the cristal basis in degrees)
0.2		(Spectrometer aperture in mrad)
0.2		(convergence angle in mrad)
3, 4		(NR, NT)

- --Boundary_(ID_PwtEJqpq4WIw+naZPXHOeA)--
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Date: Sun, 15 Sep 2002 07:30:21 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: [none]

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====



Dear wien2k_02 users:
  In the latest version wien2k_02, when I use it to calculate , there are 
always have some message like this:
    warn ingergation 28.99328888,should be  29
    NOE: number of electrons =29
    ------------
    ------------
    Total "warnning"Total energy in Ry =-28342.5000000Ry

 from the message this mean that the NOE is 29 and during some SCF 
interation ,the intergation value of NOE is not 29.
 So I want to know these question:
     1; what's this warn mean? 
     2: How can I avoid this warn? for example, can I change a larger RMT 
to avoid this ,or can I choose a low energy in lstart?(for : change -6.0 Ry 
to -7.0 Ry?)

     3:How can it affect my result? If the difference between ingergraton 
velue and the true value is small(like in my case ,just 0.006),can I 
neglect it?

Hai




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------------------------------

Date: Mon, 16 Sep 2002 18:23:51 +0800
From: joshua xie <joshuaxie@etang.com>
Subject: [WIEN]: Calculation about diamond

====
joshua xie <joshuaxie@etang.com>
submitted the following contribution:
====

For diamond, I set the two C atoms in FCC with positions (0,0,0) and (1/4,1/4,1/4), respectively.
When initializing the calculation there is a warning which is "YOU MUST MOVE THE ORIGIN".

I do not know how to cope with this porblem, would someone help me?
Thanks in advance.  

Best regards! 				
Joshua                                




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Date: Mon, 16 Sep 2002 12:37:50 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Calculation about diamond

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> For diamond, I set the two C atoms in FCC with positions (0,0,0) and (1/4,1/4,1/4), respectively.
> When initializing the calculation there is a warning which is "YOU MUST MOVE THE ORIGIN".

Use (1/8,1/8,1/8) and (7/8,7/8,7/8)    or WIEN2k !!!

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 17 Sep 2002 18:12:46 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question on maximum number of inequivalent atoms in unit cell

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Hi, 

I am using WIEN97 with graphic interface (WIEN in a Box) to calculate 
CNT. Actually, I have already successful to calculate CNT(5,0) with 
WIEN with inequivalent atoms equals 3. However, I can't perform the 
calculation with CNT(5,5). The problem is that outputnn file only contains 
3 lines as below:

cnt55
P           10
     RELA

Then, below is my input file:

cnt55
P   LATTICE,NONEQUIV. ATOMS: 1
MODE OF CALC=RELA
  4.651079 18.897269 18.897269 90.000000 90.000000 90.000000
Atom= -1: X=0.75000000 Y=0.83923876 Z=0.50000000
          MULT=20          ISPLIT= 8
Atom= -1: X=0.75000000 Y=0.80991003 Z=0.63798083
Atom= -1: X=0.25000000 Y=0.77444992 Z=0.69939954
Atom= -1: X=0.25000000 Y=0.66961938 Z=0.79378939
Atom= -1: X=0.75000000 Y=0.60483054 Z=0.82263523
.......


Then, I would like to consult about the maximum number of inequivalent 
atoms in a unit cell supported by WIEN97. Or there is an option for 
setting the maximum number of inequivalent atoms in a unit cell. If it is 
so, how to set the maximum number of inequivalent atoms in a unit cell?

Thank you

Martin 

- -- 
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
~~ "Here is your country, do not let anyone take its glory away  ~~
~~  from you. Do not let selfish men or greedy interests skin    ~~ 
~~  your country of its beauty, its riches, or its romance. The  ~~
~~  world and the future and your very children shall judge you  ~~
~~  according to the way you deal with this sacred trust."       ~~
~~                                                               ~~
~~                                                               ~~
~~               -- Theodore Roosevelt, Antiquities Act of 1906  ~~
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

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------------------------------

Date: Tue, 17 Sep 2002 19:35:59 +0200 (METDST)
From: John Tatini Titantah <jtitanta@ruca.ua.ac.be>
Subject: [WIEN]: electron density difference

====
John Tatini Titantah <jtitanta@ruca.ua.ac.be>
submitted the following contribution:
====

Dear wien users,
    This question might have been raised some times on this forum but I
would still pose it. I am trying to do calculations on N sibstituted
graphite (1N+15C) and I am interested in studing the charge transfer
processes. For this it is very instructive to look at the charge density
difference, where charge density difference stands for the difference
between the crystalline charge density and the superposed atomic
densities. I thought the DIFF switch in *.in5 would give this quantity but
it does not seem to be the case. I expect to obtain regions of negative
and others of positive charges but I do not get this on my substituted
graphene plane. What is it that I have missed? I even changed EMIN of
*.in2 to the energy of the highest occupied state (which in my
case is -0.01Ry as seen on the eigen values in *.scf. Can someone indicate
to me what aspect I have not considered?   
  Thanks very much for your suggestions

@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@
Dr. Titantah John Tatini 
Theoretical Study of Matter 
Department of Physics
University of Antwerpen
Groenenborgerlaan 171
2020 Antwerpen
BELGIUM
Tel: +32-3-2180-312
fax: +32-3-2180-318
gsm: +32-494-143515
email: jtitanta@ruca.ua.ac.be
@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@

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------------------------------

Date: Tue, 17 Sep 2002 16:05:35 -0300 (ARST)
From: Fabian Dominguez <fabian@iflysib.unlp.edu.ar>
Subject: [WIEN]: Problem with number of states when DOS is doing.

====
Fabian Dominguez <fabian@iflysib.unlp.edu.ar>
submitted the following contribution:
====


Hello Wien users,

I'm running Fe-H with H in different positions and the following problema
arise.

When I do DOS and then I plot it no states appears under -10 eV, this
happens when Total DOS is done or total 'p', 'd','s'...and in all cases, I
mean for differents positions of Hydrogen.

Trying to solve this problem I change the range in *int but nothing
happens.
Then I select in *in1/in1c the lower limit of the energy window, but
nothing happens. I did the same in *klist.
After I try changing in *in2/in2c EMIN from -9 to -14, well my porpuse was
to get this value lower. And nothing happens.

QUESTIONS:

1-/

How can I solve this problem because I think there should be states under
- -10 eV, What coud be the problem?

2-/

Related to change in *in2/*in2c from -9 to -14 does it affect anything the
previous self consistent running done, or I's a enough one more iteration
only?

Thanks to who could help me.

Fabian





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------------------------------

Date: Wed, 18 Sep 2002 09:11:43 +0200
From: "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: electron density difference

====
"Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> John Tatini Titantah <jtitanta@ruca.ua.ac.be>
> submitted the following contribution:
> ====
>
>     This question might have been raised some times on this forum but I
> would still pose it. I am trying to do calculations on N sibstituted
> graphite (1N+15C) and I am interested in studing the charge transfer
> processes. For this it is very instructive to look at the charge density
> difference, where charge density difference stands for the difference
> between the crystalline charge density and the superposed atomic
> densities. I thought the DIFF switch in *.in5 would give this quantity but
> it does not seem to be the case. I expect to obtain regions of negative
> and others of positive charges but I do not get this on my substituted
> graphene plane. What is it that I have missed? I even changed EMIN of
> *.in2 to the energy of the highest occupied state (which in my
> case is -0.01Ry as seen on the eigen values in *.scf. Can someone indicate
> to me what aspect I have not considered?

Have a look in the UG at the first paragraphs of the lstart explanation. The
atomic densities used for subtraction with DIFF in lapw5 are created only if
you include a 'P' with the relevant orbitals. Put the P's there, rerun
lstart, and then lapw5.

Stefaan

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------------------------------

Date: Wed, 18 Sep 2002 09:05:28 +0200
From: =?US-ASCII?Q?Anders_Froseth?= <anders.froseth@phys.ntnu.no>
Subject: SV: [WIEN]: electron density difference

====
=?US-ASCII?Q?Anders_Froseth?= <anders.froseth@phys.ntnu.no>
submitted the following contribution:
====

Dear John!

For lapw5 to calculate the bonding charge density you
need to have the atomic electron densities in the .sigma file.
The .sigma file is created by lstart using the .inst file as input.
For each atomic orbital from which you need the density, you have to replace
an
N with a P in the .inst file. So - edit the .inst file, run lstart and
then run lapw5 again. This will hopefully solve your problem..

Regards
Anders Froseth

> -----Opprinnelig melding-----
> Fra: owner-wien@zeus.theochem.tuwien.ac.at
> [mailto:owner-wien@zeus.theochem.tuwien.ac.at]Pa vegne av John Tatini
> Titantah
> Sendt: 17. september 2002 19:36
> Til: wien@zeus.theochem.tuwien.ac.at
> Emne: [WIEN]: electron density difference
>
>
> ====
> John Tatini Titantah <jtitanta@ruca.ua.ac.be>
> submitted the following contribution:
> ====
>
> Dear wien users,
>     This question might have been raised some times on this forum but I
> would still pose it. I am trying to do calculations on N sibstituted
> graphite (1N+15C) and I am interested in studing the charge transfer
> processes. For this it is very instructive to look at the charge density
> difference, where charge density difference stands for the difference
> between the crystalline charge density and the superposed atomic
> densities. I thought the DIFF switch in *.in5 would give this quantity but
> it does not seem to be the case. I expect to obtain regions of negative
> and others of positive charges but I do not get this on my substituted
> graphene plane. What is it that I have missed? I even changed EMIN of
> *.in2 to the energy of the highest occupied state (which in my
> case is -0.01Ry as seen on the eigen values in *.scf. Can someone indicate
> to me what aspect I have not considered?
>   Thanks very much for your suggestions
>
> @@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@
> Dr. Titantah John Tatini
> Theoretical Study of Matter
> Department of Physics
> University of Antwerpen
> Groenenborgerlaan 171
> 2020 Antwerpen
> BELGIUM
> Tel: +32-3-2180-312
> fax: +32-3-2180-318
> gsm: +32-494-143515
> email: jtitanta@ruca.ua.ac.be
> @@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====

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------------------------------

Date: Wed, 18 Sep 2002 11:48:45 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: electron density difference

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>     This question might have been raised some times on this forum but I
> would still pose it. I am trying to do calculations on N sibstituted
> graphite (1N+15C) and I am interested in studing the charge transfer
> processes. For this it is very instructive to look at the charge density
> difference, where charge density difference stands for the difference
> between the crystalline charge density and the superposed atomic
> densities. I thought the DIFF switch in *.in5 would give this quantity but
> it does not seem to be the case. I expect to obtain regions of negative
> and others of positive charges but I do not get this on my substituted
> graphene plane. What is it that I have missed? I even changed EMIN of
> *.in2 to the energy of the highest occupied state (which in my
> case is -0.01Ry as seen on the eigen values in *.scf. Can someone indicate
> to me what aspect I have not considered?
Is not your case.sigma file empty? If it is change N to P (capital P) in
your case.inst to generate atomic charge densities: only after this DIFF
works.
Your,
S. Jalali.

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------------------------------

Date: Wed, 18 Sep 2002 11:38:48 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Problem with number of states when DOS is doing.

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> I'm running Fe-H with H in different positions and the following problema
> arise.
>
> When I do DOS and then I plot it no states appears under -10 eV, this
> happens when Total DOS is done or total 'p', 'd','s'...and in all cases, I
> mean for differents positions of Hydrogen.
>
> Trying to solve this problem I change the range in *int but nothing
> happens.
> Then I select in *in1/in1c the lower limit of the energy window, but
> nothing happens. I did the same in *klist.
> After I try changing in *in2/in2c EMIN from -9 to -14, well my porpuse was
> to get this value lower. And nothing happens.

Please notice that the unit of energy in input files is in Ry and not in eV,
so if you are looking for something around 10eV, it is not needed to change
EMIN in case.in1 (not case.in2) file. Instead if one is interested in
energies grater than 1.5Ry, it is necessary to increase Emax in case.in1
file.




> QUESTIONS:
>
> 1-/
>
> How can I solve this problem because I think there should be states under
> -10 eV, What coud be the problem?

I don't know if some states should be there at around -10eV or not, but if
you think so just change the Emin in case.int to -1.0 Ry. Below the valence
states towards semi core states the bands are not so broad: they are usually
narrow. To observe narrow bands one would first open the case.dos1evup(dn)
via a plain text editor to find where the narrow bands are. After finding
the interval energy one can plot the state using wien2k interface or any
other graphical tools, e.g. gnuplot or so.


> 2-/
>
> Related to change in *in2/*in2c from -9 to -14 does it affect anything the
> previous self consistent running done, or I's a enough one more iteration
> only?
I guess it would be clear now.



Your,

S. Jalali.


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------------------------------

Date: Wed, 18 Sep 2002 09:23:24 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Problem with number of states when DOS is doing.

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I'm running Fe-H with H in different positions and the following problema
> arise.
>
> When I do DOS and then I plot it no states appears under -10 eV, this
> happens when Total DOS is done or total 'p', 'd','s'...and in all cases, I
> mean for differents positions of Hydrogen.
>
> How can I solve this problem because I think there should be states under
> -10 eV, What coud be the problem?

Why do you think so ? Look into your scf file and check where you have
eigenvalues. Then consider EF and convert from Ry to eV and you KNOW
where your states should be. (Personally I expect for Fe-H systems only states
at about -4 Ry (Fe 3p), which is -50 eV or so. For those atomic like states a
DOS is meaningless (althoug you can get it, when your e-mesh in case.int is
fine enough).

Changing EMIN from -9 to -14 means (Ry units!!!!) nothing for your case.



                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 18 Sep 2002 09:42:22 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Question on maximum number of inequivalent atoms in unit cell

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I am using WIEN97 with graphic interface (WIEN in a Box) to calculate
> CNT. Actually, I have already successful to calculate CNT(5,0) with
> WIEN with inequivalent atoms equals 3. However, I can't perform the
> calculation with CNT(5,5). The problem is that outputnn file only contains
> 3 lines as below:
>
> cnt55
> P           10
>      RELA
>
> Then, below is my input file:
>
> cnt55
> P   LATTICE,NONEQUIV. ATOMS: 1
> MODE OF CALC=RELA
>   4.651079 18.897269 18.897269 90.000000 90.000000 90.000000
> Atom= -1: X=0.75000000 Y=0.83923876 Z=0.50000000
>           MULT=20          ISPLIT= 8
> Atom= -1: X=0.75000000 Y=0.80991003 Z=0.63798083
> Atom= -1: X=0.25000000 Y=0.77444992 Z=0.69939954
> Atom= -1: X=0.25000000 Y=0.66961938 Z=0.79378939
> Atom= -1: X=0.75000000 Y=0.60483054 Z=0.82263523
> .......
>
>
> Then, I would like to consult about the maximum number of inequivalent
> atoms in a unit cell supported by WIEN97. Or there is an option for
> setting the maximum number of inequivalent atoms in a unit cell. If it is
> so, how to set the maximum number of inequivalent atoms in a unit cell?

In WIEN97 you must redimension the program using siteconfig. The relevant
parameters are NATO and NDIF (see the UG for nn and for other programs).
PS: This is not necessary with WIEN2k because of dynamical allocation)

However, your struct file looks strange. There is no spacegroup with
MULT=20,....

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 18 Sep 2002 12:14:58 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Question on maximum number of inequivalent atoms in unit cell

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_006D_01C25F0D.014A8630
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	charset="iso-8859-1"
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> I am using WIEN97 with graphic interface (WIEN in a Box) to calculate=20
> CNT. Actually, I have already successful to calculate CNT(5,0) with=20
> WIEN with inequivalent atoms equals 3. However, I can't perform the=20
> calculation with CNT(5,5). The problem is that outputnn file only =
contains=20
> 3 lines as below:
>=20
> cnt55
> P           10
>      RELA
>=20
> Then, below is my input file:
>=20
> cnt55
> P   LATTICE,NONEQUIV. ATOMS: 1
> MODE OF CALC=3DRELA
>   4.651079 18.897269 18.897269 90.000000 90.000000 90.000000
> Atom=3D -1: X=3D0.75000000 Y=3D0.83923876 Z=3D0.50000000
>           MULT=3D20          ISPLIT=3D 8
> Atom=3D -1: X=3D0.75000000 Y=3D0.80991003 Z=3D0.63798083
> Atom=3D -1: X=3D0.25000000 Y=3D0.77444992 Z=3D0.69939954
> Atom=3D -1: X=3D0.25000000 Y=3D0.66961938 Z=3D0.79378939
> Atom=3D -1: X=3D0.75000000 Y=3D0.60483054 Z=3D0.82263523
> .......
>=20
>=20
> Then, I would like to consult about the maximum number of inequivalent =

> atoms in a unit cell supported by WIEN97. Or there is an option for=20
> setting the maximum number of inequivalent atoms in a unit cell. If it =
is=20
> so, how to set the maximum number of inequivalent atoms in a unit =
cell?

You would check the following default parameters for your case.
PARAMETER (NATO=3D 64)=20

PARAMETER (NNN=3D10000)=20

PARAMETER (NDIF=3D 99)=20

PARAMETER (mshell=3D 100)=20

NATO NUMBER OF NONEQUIVALENT ATOMS=20

NNN NUMBER OF NEIGHBOURS=20

NDIF NUMBER OF ALL ATOMS IN UNITCELL=20

MSHELL Max. Nr. of SHELLS

And if necessary try to change them in nn program, and recompile nn.

Your,

Saeid.


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	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY>
<DIV><FONT face=3DArial size=3D2>&gt; I am using WIEN97 with graphic =
interface (WIEN=20
in a Box) to calculate <BR>&gt; CNT. Actually, I have already successful =
to=20
calculate CNT(5,0) with <BR>&gt; WIEN with inequivalent atoms equals 3. =
However,=20
I can't perform the <BR>&gt; calculation with CNT(5,5). The problem is =
that=20
outputnn file only contains <BR>&gt; 3 lines as below:<BR>&gt; <BR>&gt;=20
cnt55<BR>&gt; =
P&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
10<BR>&gt; &nbsp;&nbsp;&nbsp;&nbsp; RELA<BR>&gt; <BR>&gt; Then, below is =
my=20
input file:<BR>&gt; <BR>&gt; cnt55<BR>&gt; P&nbsp;&nbsp; =
LATTICE,NONEQUIV.=20
ATOMS: 1<BR>&gt; MODE OF CALC=3DRELA<BR>&gt; &nbsp; 4.651079 18.897269 =
18.897269=20
90.000000 90.000000 90.000000<BR>&gt; Atom=3D -1: X=3D0.75000000 =
Y=3D0.83923876=20
Z=3D0.50000000<BR>&gt; =
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
MULT=3D20&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; =
ISPLIT=3D 8<BR>&gt;=20
Atom=3D -1: X=3D0.75000000 Y=3D0.80991003 Z=3D0.63798083<BR>&gt; Atom=3D =
- -1: X=3D0.25000000=20
Y=3D0.77444992 Z=3D0.69939954<BR>&gt; Atom=3D -1: X=3D0.25000000 =
Y=3D0.66961938=20
Z=3D0.79378939<BR>&gt; Atom=3D -1: X=3D0.75000000 Y=3D0.60483054 =
Z=3D0.82263523<BR>&gt;=20
.......<BR>&gt; <BR>&gt; <BR>&gt; Then, I would like to consult about =
the=20
maximum number of inequivalent <BR>&gt; atoms in a unit cell supported =
by=20
WIEN97. Or there is an option for <BR>&gt; setting the maximum number of =

inequivalent atoms in a unit cell. If it is <BR>&gt; so, how to set the =
maximum=20
number of inequivalent atoms in a unit cell?<BR></FONT></DIV>
<DIV><FONT face=3DArial size=3D2>You would check the following default =
parameters=20
for your case.</FONT></DIV>
<DIV>
<P><FONT face=3DArial size=3D2>PARAMETER (NATO=3D 64) </FONT></P>
<P><FONT face=3DArial size=3D2>PARAMETER (NNN=3D10000) </FONT></P>
<P><FONT face=3DArial size=3D2>PARAMETER (NDIF=3D 99) </FONT></P>
<P><FONT face=3DArial size=3D2>PARAMETER (mshell=3D 100) </FONT></P>
<P><FONT face=3DArial size=3D2>NATO NUMBER OF NONEQUIVALENT ATOMS =
</FONT></P>
<P><FONT face=3DArial size=3D2>NNN NUMBER OF NEIGHBOURS </FONT></P>
<P><FONT face=3DArial size=3D2>NDIF NUMBER OF ALL ATOMS IN UNITCELL =
</FONT></P>
<P><FONT face=3DArial size=3D2>MSHELL Max. Nr. of SHELLS</FONT></P>
<P><FONT face=3DArial size=3D2>And if necessary try to change them in nn =
program,=20
and recompile nn.</FONT></P>
<P><FONT face=3DArial size=3D2>Your,</FONT></P>
<P><FONT face=3DArial size=3D2>Saeid.</FONT></P></DIV></BODY></HTML>

- ------=_NextPart_000_006D_01C25F0D.014A8630--

====
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End of wien-digest V2002 #35
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #36
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Sender: owner-wien-digest@theochem.tuwien.ac.at
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Precedence: bulk


wien-digest       Thursday, September 26 2002       Volume 2002 : Number 036




----------------------------------------------------------------------

Date: Wed, 18 Sep 2002 11:59:54 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: [WIEN]: Re: your mail

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>   In the latest version wien2k_02, when I use it to calculate , there are
> always have some message like this:
>     warn ingergation 28.99328888,should be  29
>     NOE: number of electrons =29
>     ------------
>     ------------
>     Total "warnning"Total energy in Ry =-28342.5000000Ry
>
>  from the message this mean that the NOE is 29 and during some SCF
> interation ,the intergation value of NOE is not 29.
>  So I want to know these question:
>      1; what's this warn mean?
>      2: How can I avoid this warn? for example, can I change a larger RMT
> to avoid this ,or can I choose a low energy in lstart?(for : change -6.0 Ry
> to -7.0 Ry?)
>
>      3:How can it affect my result? If the difference between ingergraton
> velue and the true value is small(like in my case ,just 0.006),can I
> neglect it?

If these warnings happen during scf, but at the end of the scf they
disappeared, then don't worry.

However, if they persist, you must either
a) change the k-mesh (x kgen)
b) change the Fermi method  (to gauss or temp)

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 18 Sep 2002 16:15:34 +0100 (BST)
From: Vincent Jennings <V.L.Jennings@warwick.ac.uk>
Subject: [WIEN]: Units.

====
Vincent Jennings <V.L.Jennings@warwick.ac.uk>
submitted the following contribution:
====

Hi,
  This should be an easy question...
  I want to check the units for RKmax and Gmax.  I figure RKmax should be
dimensionless, and Gmax should have dimension of 1/length.
  Thanks,
  Vin.

- -------------------------------------------------------------------------------
Vincent Jennings			"Some days you're the pigeon
email: V.L.Jennings@warwick.ac.uk	 and some days you're the statue."
- -------------------------------------------------------------------------------

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------------------------------

Date: Wed, 18 Sep 2002 18:13:07 +0200
From: Jutta Rogal <rogal@FHI-Berlin.MPG.DE>
Subject: [WIEN]: Gmax convergence

====
Jutta Rogal <rogal@FHI-Berlin.mpg.de>
submitted the following contribution:
====

This is a multi-part message in MIME format.
- --------------00BE623C56E4CD7611E6B667
Content-Type: text/plain; charset=us-ascii
Content-Transfer-Encoding: 7bit

Dear Wien-users,
I have calculated the total energies of Palladium-bulk in an fcc-lattice
with one atom in the unit cell, 72  irred. k-points [12x12x12] and a
cutoff energy of 24 Ry for the wavefunction.  If I now increase the
value of Gmax in *.in2, which determines the cutoff energy for the
potential, the total energy goes up an seems to converge to some value
(as you can see in the attachment).  Now my question is:  If I increase
the cutoff energy for the potential, which means that I'm improving my
basis set, should the total energy of my system according to the
variational principle not acutally decrease and converge to a certain
value instead of increase?
Regards
Jutta

- --
- -----------------------------------------------------------------------
Jutta Rogal                                     phone: 49-30-8413 4807
Fritz-Haber-Institut                            rogal@fhi-berlin.mpg.de
der Max-Planck-Gesellschaft,
Abteilung Theorie
Faradayweg 4-6
14195 Berlin/Germany
- ------------------------------------------------------------------------



- --------------00BE623C56E4CD7611E6B667
Content-Type: text/plain; charset=us-ascii;
 name="Pd_gmax.TXT"
Content-Transfer-Encoding: 7bit
Content-Disposition: inline;
 filename="Pd_gmax.TXT"

Gmax	E_Pd (Ry)	E_Pd (eV)	E_Pd (eV)+137334

10	-10094.104853	-137334.334167	-0.334167
11	-10094.101896	-137334.293936	-0.293936
12	-10094.101878	-137334.293691	-0.293691
13	-10094.101243	-137334.285052	-0.285052
14	-10094.100228	-137334.271242	-0.271242
15	-10094.100221	-137334.271147	-0.271147
16	-10094.099491	-137334.261215	-0.261215
18	-10094.098840	-137334.252358	-0.252358
20	-10094.098540	-137334.248276	-0.248276
24	-10094.097732	-137334.237283	-0.237283
30	-10094.097294	-137334.231324	-0.231324

- --------------00BE623C56E4CD7611E6B667--

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------------------------------

Date: Wed, 18 Sep 2002 11:28:43 -0700 (PDT)
From: morteza jamal <m_jamal23@yahoo.com>
Subject: [WIEN]: very Wonderfull

====
morteza jamal <m_jamal23@yahoo.com>
submitted the following contribution:
====

Dear Wein2k users.
We are using LDA+U for UCd3 .
There is one Wonderfull things in our result. one
ITERATION is REPEATED (for example ITE=14).number of
repeat is 22.
After 22 REPEATS;number of ITERATIONS change from 14
to 15. 
There is no error.
we used this option for running:
"runsp_c_lapw -so -orb -in1new 5 -cc 0.00001 ......."
What has happened?
Please help me.

Best wishes.
Morteza Jamal.


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------------------------------

Date: Wed, 18 Sep 2002 16:24:49 -0300 (ARST)
From: Fabian Dominguez <fabian@iflysib.unlp.edu.ar>
Subject: Re: [WIEN]: Problem with number of states when DOS is doing.

====
Fabian Dominguez <fabian@iflysib.unlp.edu.ar>
submitted the following contribution:
====



Dear Saeid and Wien users,

Ok what you said in your answer saeid but I have no solution to my problem
since in *int I used units in Ry and I'm not using upper limit in energy
window in 1.5 but 3.5, because this is the only way to run lapw2 -qtl
- -up/dn and not to get an error of FERMI type...the use of 3.5 is good
because total number of electrons are totally included in the window...
well this a comment to your answer to  mine related to energy window in
*in1/*in1c.

Another thing is that using TETRA option in *in2/*in2c and upper limit in
1.5 in *in1/*in1c FERMI type error appears, if I use 3.5 no error appears.

The point is that I'm not trying to see states around -10eV what I want to
see is a DOS in a established range, not nessesary between -10 and for
example 5 eV if not a complete DOS, because I think there should be many
states under -10eV, I mean to choose a range and be sure that no states
are under the lower level selected.

thank and I wait for an answer.

Fabian


============================***=================================

Lic. Fabian Alfredo Dominguez Avenalle.
Instituto de Fisica de Liquidos y Sistemas Biologicos (IFLYSIB).
Universidad Nacional de La Plata (UNLP).
Calle 59 N 789 La Plata CP.  1900  BUENOS AIRES  ARGENTINA
CC. 565
TE: 0221-4233283
TELEFAX: 0221-4257317
E-MAIL: fabian@iflysib.unlp.edu.ar
============================***=================================


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------------------------------

Date: Thu, 19 Sep 2002 08:14:21 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Problem with number of states when DOS is doing.

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> The point is that I'm not trying to see states around -10eV what I want to
> see is a DOS in a established range, not nessesary between -10 and for
> example 5 eV if not a complete DOS, because I think there should be many
> states under -10eV, I mean to choose a range and be sure that no states
> are under the lower level selected.

Inspect case.outputt. There you see the bandranges, i.e. the energies
where you have eigenvalues ("states").

If there are no states, then the DOS is simply zero!!!

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 19 Sep 2002 08:18:15 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Gmax convergence

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I have calculated the total energies of Palladium-bulk in an fcc-lattice
> with one atom in the unit cell, 72  irred. k-points [12x12x12] and a
> cutoff energy of 24 Ry for the wavefunction.  If I now increase the
> value of Gmax in *.in2, which determines the cutoff energy for the
> potential, the total energy goes up an seems to converge to some value
> (as you can see in the attachment).  Now my question is:  If I increase
> the cutoff energy for the potential, which means that I'm improving my
> basis set, should the total energy of my system according to the
> variational principle not acutally decrease and converge to a certain
> value instead of increase?

Increasing GMAX does NOT mean improving the basis set !!!
You have only a better description of the coulomb and XC-potential.
Thus the variational principle does not apply.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 19 Sep 2002 14:46:30 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: [WIEN]

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

I am now using WIEN97 with graphic interface (WIEN In A Box). And the 
system I am interested in as below:

Number of inequivalent atoms : 19
Number of atoms per unit cell : 152
Number of electrons in unit cell : 608

Then, I would like to consult about the setting of the following 
parameters in siteconfig :

KMAX1
KMAX2
KMAX3
NATO
NDIF
NKPT
NMAT
NMATIT
NUME
NUMEIT
NWAV

Especially, the parameter of NUME and NUMEIT.

Thank you very much

Martin

- -- 
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
~~ "Here is your country, do not let anyone take its glory away  ~~
~~  from you. Do not let selfish men or greedy interests skin    ~~ 
~~  your country of its beauty, its riches, or its romance. The  ~~
~~  world and the future and your very children shall judge you  ~~
~~  according to the way you deal with this sacred trust."       ~~
~~                                                               ~~
~~                                                               ~~
~~               -- Theodore Roosevelt, Antiquities Act of 1906  ~~
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

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------------------------------

Date: Thu, 19 Sep 2002 09:36:14 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Gmax convergence

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Peter,

Somehow I always thought that an increasing number of planewaves was an 
improvement of the basis set used in a specific calculation. And, since 
increasing GMAX increases the number of planewaves, then why isn't it an 
improvement?

Best regards,
Torsten Andersen.

Peter Blaha wrote:

>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
>>I have calculated the total energies of Palladium-bulk in an fcc-lattice
>>with one atom in the unit cell, 72  irred. k-points [12x12x12] and a
>>cutoff energy of 24 Ry for the wavefunction.  If I now increase the
>>value of Gmax in *.in2, which determines the cutoff energy for the
>>potential, the total energy goes up an seems to converge to some value
>>(as you can see in the attachment).  Now my question is:  If I increase
>>the cutoff energy for the potential, which means that I'm improving my
>>basis set, should the total energy of my system according to the
>>variational principle not acutally decrease and converge to a certain
>>value instead of increase?
>>
>
>Increasing GMAX does NOT mean improving the basis set !!!
>You have only a better description of the coulomb and XC-potential.
>Thus the variational principle does not apply.
>
>                                      P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Thu, 19 Sep 2002 10:14:26 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Gmax convergence

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Somehow I always thought that an increasing number of planewaves was an
> improvement of the basis set used in a specific calculation. And, since
> increasing GMAX increases the number of planewaves, then why isn't it an
> improvement?

GMAX increases the number of Fouriercoefficients ("planewaves") for the
description of rho and V. (The list at the bottom of the case.clmsum and
case.vns files gets "longer").
It has nothing to do with the planewave expansion of your wavefunctions. I.e.
the "matrixsize" in lapw1 (case.scf1) is not changed by GMAX (case.in2), but
by RKMAX (case.in1)
Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 19 Sep 2002 10:18:43 +0200
From: "koitzsch" <Christian.Koitzsch@unifr.ch>
Subject: Re: [WIEN]: Gmax convergence

====
"koitzsch" <Christian.Koitzsch@unifr.ch>
submitted the following contribution:
====

I think there is a mix-up between RKmax and gmax here.

christian koitzsch


- ----- Original Message -----
From: "Torsten Andersen" <Torsten.Andersen@Fysik.UU.se>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Thursday, September 19, 2002 9:36 AM
Subject: Re: [WIEN]: Gmax convergence


> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
>
> Dear Peter,
>
> Somehow I always thought that an increasing number of planewaves was an
> improvement of the basis set used in a specific calculation. And, since
> increasing GMAX increases the number of planewaves, then why isn't it an
> improvement?
>
> Best regards,
> Torsten Andersen.
>
> Peter Blaha wrote:
>
> >====
> >Peter Blaha <pblaha@theochem.tuwien.ac.at>
> >submitted the following contribution:
> >====
> >
> >>I have calculated the total energies of Palladium-bulk in an fcc-lattice
> >>with one atom in the unit cell, 72  irred. k-points [12x12x12] and a
> >>cutoff energy of 24 Ry for the wavefunction.  If I now increase the
> >>value of Gmax in *.in2, which determines the cutoff energy for the
> >>potential, the total energy goes up an seems to converge to some value
> >>(as you can see in the attachment).  Now my question is:  If I increase
> >>the cutoff energy for the potential, which means that I'm improving my
> >>basis set, should the total energy of my system according to the
> >>variational principle not acutally decrease and converge to a certain
> >>value instead of increase?
> >>
> >
> >Increasing GMAX does NOT mean improving the basis set !!!
> >You have only a better description of the coulomb and XC-potential.
> >Thus the variational principle does not apply.
> >
> >                                      P.Blaha
>
>--------------------------------------------------------------------------
> >Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> >Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> >Email: blaha@theochem.tuwien.ac.at    WWW:
http://info.tuwien.ac.at/theochem/
>
>--------------------------------------------------------------------------
> >
> >====
> >WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> >To (un)subscribe send mail to
> >majordomo@zeus.theochem.tuwien.ac.at
> >====
> >
> >
>
> --
> Dr. Torsten Andersen
> Department of Physics, Condensed Matter Theory Group, Uppsala University
> UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
> News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics
>
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>


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------------------------------

Date: Thu, 19 Sep 2002 12:36:46 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Gmax convergence

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Thank you for the clarification... yes, it seems logical, since a larger 
RKmax gives a larger Gmin, and thereby requires a larger Gmax.

Best regards,
Torsten Andersen.

koitzsch wrote:

>====
>"koitzsch" <Christian.Koitzsch@unifr.ch>
>submitted the following contribution:
>====
>
>I think there is a mix-up between RKmax and gmax here.
>
>christian koitzsch
>
>
>----- Original Message -----
>From: "Torsten Andersen" <Torsten.Andersen@Fysik.UU.se>
>To: <wien@zeus.theochem.tuwien.ac.at>
>Sent: Thursday, September 19, 2002 9:36 AM
>Subject: Re: [WIEN]: Gmax convergence
>
>
>>====
>>Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
>>submitted the following contribution:
>>====
>>
>>Dear Peter,
>>
>>Somehow I always thought that an increasing number of planewaves was an
>>improvement of the basis set used in a specific calculation. And, since
>>increasing GMAX increases the number of planewaves, then why isn't it an
>>improvement?
>>
>>Best regards,
>>Torsten Andersen.
>>
>>Peter Blaha wrote:
>>
>>>====
>>>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>>>submitted the following contribution:
>>>====
>>>
>>>>I have calculated the total energies of Palladium-bulk in an fcc-lattice
>>>>with one atom in the unit cell, 72  irred. k-points [12x12x12] and a
>>>>cutoff energy of 24 Ry for the wavefunction.  If I now increase the
>>>>value of Gmax in *.in2, which determines the cutoff energy for the
>>>>potential, the total energy goes up an seems to converge to some value
>>>>(as you can see in the attachment).  Now my question is:  If I increase
>>>>the cutoff energy for the potential, which means that I'm improving my
>>>>basis set, should the total energy of my system according to the
>>>>variational principle not acutally decrease and converge to a certain
>>>>value instead of increase?
>>>>
>>>Increasing GMAX does NOT mean improving the basis set !!!
>>>You have only a better description of the coulomb and XC-potential.
>>>Thus the variational principle does not apply.
>>>
>>>                                     P.Blaha
>>>
>>--------------------------------------------------------------------------
>>
>>>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>>>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>>>Email: blaha@theochem.tuwien.ac.at    WWW:
>>>
>http://info.tuwien.ac.at/theochem/
>
>>--------------------------------------------------------------------------
>>
>>>====
>>>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>>>To (un)subscribe send mail to
>>>majordomo@zeus.theochem.tuwien.ac.at
>>>====
>>>
>>>
>>--
>>Dr. Torsten Andersen
>>Department of Physics, Condensed Matter Theory Group, Uppsala University
>>UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
>>News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics
>>
>>
>>
>>====
>>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>>To (un)subscribe send mail to
>>majordomo@zeus.theochem.tuwien.ac.at
>>====
>>
>
>
>====
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>majordomo@zeus.theochem.tuwien.ac.at
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>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Thu, 19 Sep 2002 13:20:33 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: [none]

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====

Dear wien2k_2 users:
  I want to use wien2k_02 to calculate an antimagnetism double perovskite 
system.
I have followed the following methods, but encounter some problems:
   
   1: init_lapw and afminput ,then run runafm_lapw -orbc -cc 0.0001, this 
can work and achieve the AFM result. but I found when I change the U value 
in case.inorb, the results are same expect the Fermi level. Because the 
- -orb is not supported in runafm_lapw , so I want to know , in -orbc , how 
does the U and J affect the calculation or not affecting our calculation?

   2:init_lapw(befor lstar , I have flip the spin of AFM atoms and set zero 
of another atoms), then run runfsm_lapw -m 0 -orbc -cc 0.0001, but I found 
the tendency of SCF is to make every atom to become no 
magnetism----paramagnetism.and In the 6th cycle, errors apperared and SCF 
stoped, error in uplapw1.error like these:
     select--no energy limits found for L=1
     select--E-bottom -1.74500  E-top -200.0000

    3.init_lapw(befor lstar , I have flip the spin of AFM atoms and set 
zero of another atoms), then run runsp_lapw -orb  -cc 0.0001, but I cann't 
achieve an AFM 
results


 I have known that the double antimagnetism system has been successfullly 
calculated by other problem, so I want to know if it also can be calculated 
by wien2k_02, and If can , what's the righe way to do it ?  I hope Prof 
Peter or some other experts can give me some advise on this  problem.

Yours 
 Hai

 



_________________________________________________________________
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Date: Thu, 19 Sep 2002 12:21:37 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: Electron density map using w2web

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

I sent my questions about mapping the elctron density for my minerals, I
am still puzzled now, I list the questions again as fellowing, any
instruction, suggestion and comment is highly appreciated!

1. For my crystal (tetragonal symmetry), no case.in2 file was created
after the SCF cycles, but I get the following files:

	tugtupite.in2_ls   tugtupite.in2_st   tugtupite.in2_sy
	tugtupite.in2c

2. After I run "x lapw2", it crashed with the following error message:

	******  FORTRAN RUN-TIME SYSTEM  ******
	End-of-file:  -1
	Location:  the READ statement at line 56 of "fermi.f"
	Unit:  30
	File:  tugtupite.energy
     Abort
     0.0u 0.0s 0:00 0% 0+0k 0+0io 0pf+0w


Thank you in adavance!


Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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Date: Thu, 19 Sep 2002 20:30:04 +0200
From: Cesar Lazo <lazo@FHI-Berlin.MPG.DE>
Subject: Re: [WIEN]: Conversion from eV --> Tesla

====
Cesar Lazo <lazo@fhi-berlin.mpg.de>
submitted the following contribution:
====

Maybe this can help you:


http://www.chemie.fu-berlin.de/chemistry/general/units_en.html

Regards,

Cesar Lazo



Vidya Ravindran wrote:

>====
>Vidya Ravindran <vidya.ravindran@kjemi.uio.no>
>submitted the following contribution:
>====
>
>
>Dear All,
>     	I am trying to convert energy given in eV to the magnetic
>field intensity given in Tesla. I am unable to find a direct conversion
>factor for eV to Tesla
>	I am highly thankful if somebody could suggest the conversion
>factors or some references where I can find them.
>	Thank you.
>
>Yours sincerely,
>R. Vidya
>
>****************************************************************
>R. Vidya, Department of Chemistry       |Tel: +47 228 55606
>University of Oslo, PO Box 1033         |Fax: +47 228 55441/5565
>Blindern, N-0315 OSLO, NORWAY           |
>Email: ravindran.vidya@kjemi.uio.no     |
>URL: http://folk.uio.no/~ravindrv       |
>****************************************************************
>
>
>
>
>====
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Date: Thu, 19 Sep 2002 23:22:18 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Electron density map using w2web

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> After I run "x lapw2", it crashed with the following error message:
You would try "x lapw2 -c".
Your,
S. Jalali.

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Date: Thu, 19 Sep 2002 23:53:37 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: [WIEN]: Re: 

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>    2:init_lapw(befor lstar , I have flip the spin of AFM atoms and set
zero
> of another atoms), then run runfsm_lapw -m 0 -orbc -cc 0.0001, but I found
> the tendency of SCF is to make every atom to become no
> magnetism----paramagnetism.and In the 6th cycle, errors apperared and SCF
> stoped, error in uplapw1.error like these:
>      select--no energy limits found for L=1
>      select--E-bottom -1.74500  E-top -200.0000

I am not sure if you are treating with your system in a right physical way
or not, but I guess the 6th cycle is too soon to make a decision. You would
add "-in1new 5" switch to control linearization, and rerun it in a clean
directory to maybe get ride of that error to see what happen after 6th
cycle.
Your,
S. Jalali.



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Date: Thu, 19 Sep 2002 15:08:04 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: Re: [WIEN]: Electron density map using w2web

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear Dr.Jalali:

Thanks!
I used "x lapw2 -c", it crashed again and the error message is the same as
that from "x lapw2".

Any more suggestion?

Best wishes!


On Thu, 19 Sep 2002, Saeid Jalali wrote:

> ====
> "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> submitted the following contribution:
> ====
>
> > After I run "x lapw2", it crashed with the following error message:
> You would try "x lapw2 -c".
> Your,
> S. Jalali.
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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Date: Thu, 19 Sep 2002 17:38:52 -0500 (CDT)
From: zheng@cz.chem.niu.edu (Chong Zheng)
Subject: [WIEN]: tomach flue and i probably want be in class today. so if you can please email m

====
zheng@cz.chem.niu.edu (Chong Zheng)
submitted the following contribution:
====

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------------------------------

Date: Fri, 20 Sep 2002 09:28:18 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Electron density map using w2web

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0054_01C26088.0E326E40
Content-Type: text/plain;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

> I used "x lapw2 -c", it crashed again and the error message is the =
same as
> that from "x lapw2".
Just to check if "x lapw -c" works or not, one would quickly rerun (only =
1 iteration) the calculation in a clean directory and then give the =
command a retry. If one sees that it works now, one may first save the =
calculation with the name of for instance "old" (save_lapw old),  then =
does "rm case.recprlist" and "x dstart (up and dn)". Now one is ready to =
rerun "x lapw2 -c". But if one sees that it does not work again (!!!), I =
suggest to take a look at :log file to see the history of the performed =
command during scf.
Your,
S. Jalali.

- ------=_NextPart_000_0054_01C26088.0E326E40
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT face=3DArial size=3D2>&gt; I used "x lapw2 -c", it crashed =
again and the=20
error message is the same as<BR>&gt; that from "x lapw2".<BR>Just to =
check if "x=20
lapw -c" works or not, one would quickly rerun&nbsp;(only 1 iteration) =
the=20
calculation in a clean directory and then give the command a =
retry.&nbsp;If one=20
sees that it works now,&nbsp;one may first save&nbsp;the calculation =
with the=20
name of for instance "old" (save_lapw old),&nbsp; then does "rm =
</FONT><FONT=20
face=3DArial size=3D2>case.recprlist" and "x dstart (up and dn)".=20
Now&nbsp;one&nbsp;is ready to rerun "x lapw2 -c". But if one sees that =
it does=20
not work again (!!!), I suggest to take a look at&nbsp;:log file to see =
the=20
history of the performed command during scf.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Your,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>S. Jalali.</FONT></DIV></BODY></HTML>

- ------=_NextPart_000_0054_01C26088.0E326E40--

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------------------------------

Date: Fri, 20 Sep 2002 08:43:55 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Electron density map using w2web

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I sent my questions about mapping the elctron density for my minerals, I
> am still puzzled now, I list the questions again as fellowing, any
> instruction, suggestion and comment is highly appreciated!
>
> 1. For my crystal (tetragonal symmetry), no case.in2 file was created
> after the SCF cycles, but I get the following files:
>
> 	tugtupite.in2_ls   tugtupite.in2_st   tugtupite.in2_sy
> 	tugtupite.in2c
>
> 2. After I run "x lapw2", it crashed with the following error message:
>
> 	******  FORTRAN RUN-TIME SYSTEM  ******
> 	End-of-file:  -1
> 	Location:  the READ statement at line 56 of "fermi.f"
> 	Unit:  30
> 	File:  tugtupite.energy

Let's try a little teaching in solving problems:

1) It is nice that you checked which in2 files you have. Aparently your
mineral does not have inversion and thus case.in2c !!! was created. Thus
many commands need the   "-c" switch.  (Use   x program -h to find out
if "program" needs it or not).
Since you provided us with the information about in2 files, there was
already a proper hint in the mailing list.

2) Now lets do the same for problem 2).   It complained about the file
tugtupite.energy.     Do       ls -als *energ*
What do you see ?
I hope you have done an scf run before ?
I see two choices:  a) you find files *energy_1,... ===> you have done it
in parallel, use    x lapw2 -c -p
b) you find files   *energyup, dn  (or up_1,.) ===> guess what is the problem

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Fri, 20 Sep 2002 07:08:37 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: Re: [WIEN]: Electron density map using w2web

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====

Dear Saeid:
  According to your advice , I have use the -in1new 5 in my AFM LDA+U 
calculation(this has been from an clear directory), there are no 'select' 
error, but in the 10th cycle, the SCF stopped because of other error. The 
following is the screen print message:
     LAPW0 END
     LAPW1 END
     PGFIO-F_231/formatted read/unit=1005/error on date conversion
     File name=/case.helpup035 formatted sequential access record=5
     In source file 01up.f, at line number 181

it looks like that the -in1new just remove my select problem ,and the 
tendency is also to paramagnetism ,not AFM. may be I should change  my 
value of U or J. In some value of U or J, I can achieve my AFM results. Do 
you think it is possible?

Yours 
  Hai

"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>    2:init_lapw(befor lstar , I have flip the spin of AFM atoms and set
zero
> of another atoms), then run runfsm_lapw -m 0 -orbc -cc 0.0001, but I 
found
> the tendency of SCF is to make every atom to become no
> magnetism----paramagnetism.and In the 6th cycle, errors apperared and SCF
> stoped, error in uplapw1.error like these:
>      select--no energy limits found for L=1
>      select--E-bottom -1.74500  E-top -200.0000

I am not sure if you are treating with your system in a right physical way
or not, but I guess the 6th cycle is too soon to make a decision. You would
add "-in1new 5" switch to control linearization, and rerun it in a clean
directory to maybe get ride of that error to see what happen after 6th
cycle.
Your,
S. Jalali.


_________________________________________________________________
ÏíÓÃÊÀ½çÉÏ×î´óµÄµç×ÓÓÊ¼þÏµÍ³¡ª MSN Hotmail¡£http://www.hotmail.com/cn

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Date: Fri, 20 Sep 2002 09:42:01 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: [WIEN]

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I am now using WIEN97 with graphic interface (WIEN In A Box). And the
> system I am interested in as below:
>
> Number of inequivalent atoms : 19
> Number of atoms per unit cell : 152
> Number of electrons in unit cell : 608
>
> Then, I would like to consult about the setting of the following
> parameters in siteconfig :
>
> KMAX1
> KMAX2   must be tested, depens on lattice parameters,if too small, program
> KMAX3    stops and will tell you
> NATO    19
> NDIF   152
> NKPT
> NMAT      7000 - 15000
> NMATIT    1   or if memory permits 7000 - 15000
> NUME       800
> NUMEIT     1   or 800
> NWAV       probably quite large, must be tested, if too small, program stops and will tell you

Remember: A system with 150 atoms requires a large number of plane wave!!!
NMAT must be very large (see above) and you need a computer with huge
memory.   Depending on inversion/or no-inversion and on the nn-distances
(determines RMT) you may / may not be able to perform such calculations.
I hope you have some experience with smaller systems!

PS: WIEN2k has a more efficient basis and NMAT 4000-10000 is probably
sufficient

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Fri, 20 Sep 2002 13:22:15 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Electron density map using w2web

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> I have use the -in1new 5 in my AFM LDA+U
> calculation(this has been from an clear directory), there are no 'select'
> error, but in the 10th cycle, the SCF stopped because of other error. The
> following is the screen print message:
>      LAPW0 END
>      LAPW1 END
>      PGFIO-F_231/formatted read/unit=1005/error on date conversion
>      File name=/case.helpup035 formatted sequential access record=5
>      In source file 01up.f, at line number 181
>
> it looks like that the -in1new just remove my select problem ,and the
> tendency is also to paramagnetism ,not AFM. may be I should change  my
> value of U or J. In some value of U or J, I can achieve my AFM results. Do
> you think it is possible?

You would reduce the 5 to 3.
But I think we need wait to see if we can get a chance to receive a reply
from Peter.

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Date: Fri, 20 Sep 2002 13:00:03 +0100 (BST)
From: Vincent Jennings <V.L.Jennings@warwick.ac.uk>
Subject: Re: [WIEN]: Units.

====
Vincent Jennings <V.L.Jennings@warwick.ac.uk>
submitted the following contribution:
====

I posted this question a few days ago, and I know that it's fairly
trivial, but I would like confirmation that I have the right units as it
is one of the last things that I need to finish off my thesis.  So far I
havn't found anything that states the units explicitly.

As far as I can tell from the comments in lapw2 files Gmax is in 1/a.u.

Thanks for any comments,
  Vin.

> Hi,
>   This should be an easy question...
>   I want to check the units for RKmax and Gmax.  I figure RKmax should be
> dimensionless, and Gmax should have dimension of 1/length.

- -------------------------------------------------------------------------------
Vincent Jennings			"Some days you're the pigeon
email: V.L.Jennings@warwick.ac.uk	 and some days you're the statue."
- -------------------------------------------------------------------------------


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Date: Fri, 20 Sep 2002 18:59:19 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Units.

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> I posted this question a few days ago, and I know that it's fairly
> trivial, but I would like confirmation that I have the right units as it
> is one of the last things that I need to finish off my thesis.  So far I
> havn't found anything that states the units explicitly.
>
> As far as I can tell from the comments in lapw2 files Gmax is in 1/a.u.

> > Hi,
> >   This should be an easy question...
> >   I want to check the units for RKmax and Gmax.  I figure RKmax should
be
> > dimensionless, and Gmax should have dimension of 1/length.

I don't think that looking for the units of physical quantities is trivial.
Many refuse to answer such questions and like to pretend they are trivial as
they come from and return to fundamental physics.
Yes you are right: the unit of Kmax or Gmax is 1/length, and so R*Kmax is
dimensionless.
Your question returns to star space, where we have exp(r.K) with the cutoff
of Kmax as basis for expanding wavefunctions and exp(r.G) with the cutoff of
Gmax as basis for expanding charge density and potential energy. So, Kmax
and Gmax should be dimensionless.
Your,
S. Jalali.


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Date: Fri, 20 Sep 2002 10:41:47 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: Re: [WIEN]: Electron density map using w2web

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear Peter and Saeid:

Thank you for your great help!

First I would let you know what I am doing now:

I finished the SCF cycles with paralellization mode (40 days!),
then I tried to map Electron Density with w2web without success
due to the empty case.vector file. Now I am running mini_lapw for my
sample in single mode because I want to obtain the non-empty case.vector
file. At the same time, I try to manipulate the Electron
Density mapping with w2web so that I can become familar with the
procedures.

I run "ls -als *energ*" as Peter suggested, my computer showed the
following message:

224 -rw-------   1 umbingz  student   106496 Sep 20 09:05 tugtupite.energy
272 -rw-------   1 umbingz  student   122982 Aug 12 11:24 tugtupite.energy_1
272 -rw-------   1 umbingz  student   123009 Aug 12 10:55 tugtupite.energy_2
272 -rw-------   1 umbingz  student   123123 Aug 12 12:05 tugtupite.energy_3
272 -rw-------   1 umbingz  student   123053 Aug 12 09:53 tugtupite.energy_4
 12 -rw-------   1 umbingz  student     5260 Aug 10 04:25 tugtupite.energy_5
 12 -rw-------   1 umbingz  student     5281 Aug 10 04:37 tugtupite.energy_6
 12 -rw-------   1 umbingz  student     5253 Aug 10 05:22 tugtupite.energy_7
  0 -rw-------   1 umbingz  student        0 Jun 22 02:42 tugtupite.energydn
  0 -rw-------   1 umbingz  student        0 Jun 22 02:43 tugtupite.energydn_1
  0 -rw-------   1 umbingz  student        0 Jun 22 02:43 tugtupite.energydn_2
  0 -rw-------   1 umbingz  student        0 Jun 22 02:43 tugtupite.energydn_3
  0 -rw-------   1 umbingz  student        0 Jun 22 02:43 tugtupite.energydn_4
  0 -rw-------   1 umbingz  student        0 Jun 22 02:43 tugtupite.energydn_5
  0 -rw-------   1 umbingz  student        0 Jun 22 02:43 tugtupite.energydn_6
  0 -rw-------   1 umbingz  student        0 Jun 22 02:43 tugtupite.energydn_7

Then I tried the command "x lapw2 -c -p", it seems to work according to
the following message on my screen:

running LAPW2 in parallel mode
STOP: LAPW2 - FERMI; weighs written
[1] 1531
[2] 1535
[3] 1539
[4] 1543


Now I already stoped the excution of "x lapw2 -c -p".

Last question: the w2web requirs case.in2, how can I get one in my case
(only case.in2c available)?



On Fri, 20 Sep 2002, Peter Blaha wrote:

> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
>
> > I sent my questions about mapping the elctron density for my minerals, I
> > am still puzzled now, I list the questions again as fellowing, any
> > instruction, suggestion and comment is highly appreciated!
> >
> > 1. For my crystal (tetragonal symmetry), no case.in2 file was created
> > after the SCF cycles, but I get the following files:
> >
> > 	tugtupite.in2_ls   tugtupite.in2_st   tugtupite.in2_sy
> > 	tugtupite.in2c
> >
> > 2. After I run "x lapw2", it crashed with the following error message:
> >
> > 	******  FORTRAN RUN-TIME SYSTEM  ******
> > 	End-of-file:  -1
> > 	Location:  the READ statement at line 56 of "fermi.f"
> > 	Unit:  30
> > 	File:  tugtupite.energy
>
> Let's try a little teaching in solving problems:
>
> 1) It is nice that you checked which in2 files you have. Aparently your
> mineral does not have inversion and thus case.in2c !!! was created. Thus
> many commands need the   "-c" switch.  (Use   x program -h to find out
> if "program" needs it or not).
> Since you provided us with the information about in2 files, there was
> already a proper hint in the mailing list.
>
> 2) Now lets do the same for problem 2).   It complained about the file
> tugtupite.energy.     Do       ls -als *energ*
> What do you see ?
> I hope you have done an scf run before ?
> I see two choices:  a) you find files *energy_1,... ===> you have done it
> in parallel, use    x lapw2 -c -p
> b) you find files   *energyup, dn  (or up_1,.) ===> guess what is the problem
>
> Regards
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
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> ====
>



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Fri, 20 Sep 2002 18:37:56 +0200
From: "koitzsch" <Christian.Koitzsch@unifr.ch>
Subject: [WIEN]: dummy atom

====
"koitzsch" <Christian.Koitzsch@unifr.ch>
submitted the following contribution:
====


This is a multi-part message in MIME format.

- ------=_NextPart_000_0009_01C260D4.D668A270
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	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

Hi Everybody,

I would like to include "dummy-atoms" with zero charge into a structure =
as some sort of placeholder. This would simplify the analysis since I am =
interested in the partial DOS at an interstitial site, which is not =
occupied by an atom. Does anybody know how to do that? I think the =
general question is, if one can introduce a muffin tin sphere, which is =
not centered around an atom?

Thanks a lot and have a nice weekend

Christian Koitzsch

++++++++++++++++++++++++++++++++++++++++++++
University of Fribourg
Dep. of Physics
Solid State Physics
CH-1700 Fribourg
Switzerland

- ------=_NextPart_000_0009_01C260D4.D668A270
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 5.50.4134.600" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT face=3DArial size=3D2>Hi Everybody,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>I would like to include "dummy-atoms" =
with zero=20
charge into a structure as some sort of placeholder. This would simplify =
the=20
analysis since I am interested in the partial DOS at an interstitial =
site, which=20
is not occupied by an atom. Does anybody know how to do that? I think =
the=20
general question is, if one can introduce a muffin tin sphere, which is =
not=20
centered around an atom?</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Thanks a lot and have a nice =
weekend</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Christian Koitzsch</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial=20
size=3D2>++++++++++++++++++++++++++++++++++++++++++++</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>University of Fribourg</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Dep. of Physics</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Solid State Physics</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>CH-1700 Fribourg</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Switzerland</FONT></DIV></BODY></HTML>

- ------=_NextPart_000_0009_01C260D4.D668A270--


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------------------------------

Date: Fri, 20 Sep 2002 21:38:01 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Electron density map using w2web

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> Last question: the w2web requirs case.in2, how can I get one in my case
> (only case.in2c available)?
Change session information to include complex calculation (no inversion) to
active -c in the w2web too.
Your,
S. Jalali.

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------------------------------

Date: Sat, 21 Sep 2002 16:32:44 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: 

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Hi,

Actually, I would like to build up a unit-cell with 32 atoms and my input 
file is as below:
- ----------
cnt8010A
P   LATTICE,NONEQUIV. ATOMS: 3
MODE OF CALC=RELA
 18.897269 18.897269  8.055906 90.000000 90.000000 90.000000
Atom= -1: X=0.81337534 Y=0.50000000 Z=0.08333334
          MULT= 8          ISPLIT= 8
Atom= -1: X=0.50000000 Y=0.81337534 Z=0.08333334
Atom= -1: X=0.18662466 Y=0.50000000 Z=0.08333334
Atom= -1: X=0.50000000 Y=0.18662466 Z=0.08333334
Atom= -1: X=0.81337534 Y=0.50000000 Z=0.41666667
Atom= -1: X=0.50000000 Y=0.81337534 Z=0.41666667
Atom= -1: X=0.18662466 Y=0.50000000 Z=0.41666667
Atom= -1: X=0.50000000 Y=0.18662466 Z=0.41666667
C          NPT=  781  R0=0.00010000 RMT=    1.2000   Z:  6.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -2: X=0.72158983 Y=0.72158983 Z=0.08333334
          MULT= 8          ISPLIT= 8
Atom= -2: X=0.27841017 Y=0.72158983 Z=0.08333334
Atom= -2: X=0.27841017 Y=0.27841017 Z=0.08333334
Atom= -2: X=0.72158983 Y=0.27841017 Z=0.08333334
Atom= -2: X=0.72158983 Y=0.72158983 Z=0.41666667
Atom= -2: X=0.27841017 Y=0.72158983 Z=0.41666667
Atom= -2: X=0.27841017 Y=0.27841017 Z=0.41666667
Atom= -2: X=0.72158983 Y=0.27841017 Z=0.41666667
C          NPT=  781  R0=0.00010000 RMT=    1.2000   Z:  6.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -3: X=0.78952107 Y=0.61992355 Z=0.58333334
          MULT=16          ISPLIT= 8
Atom= -3: X=0.61992355 Y=0.78952107 Z=0.58333334
Atom= -3: X=0.38007645 Y=0.78952107 Z=0.58333334
Atom= -3: X=0.21047893 Y=0.61992355 Z=0.58333334
Atom= -3: X=0.21047893 Y=0.38007645 Z=0.58333334
Atom= -3: X=0.38007645 Y=0.21047893 Z=0.58333334
Atom= -3: X=0.61992355 Y=0.21047893 Z=0.58333334
Atom= -3: X=0.78952107 Y=0.38007645 Z=0.58333334
Atom= -3: X=0.78952107 Y=0.61992355 Z=0.91666667
Atom= -3: X=0.61992355 Y=0.78952107 Z=0.91666667
Atom= -3: X=0.38007645 Y=0.78952107 Z=0.91666667
Atom= -3: X=0.21047893 Y=0.61992355 Z=0.91666667
Atom= -3: X=0.21047893 Y=0.38007645 Z=0.91666667
Atom= -3: X=0.38007645 Y=0.21047893 Z=0.91666667
Atom= -3: X=0.61992355 Y=0.21047893 Z=0.91666667
Atom= -3: X=0.78952107 Y=0.38007645 Z=0.91666667
C          NPT=  781  R0=0.00010000 RMT=    1.2000   Z:  6.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
   0 SYMMETRY OPERATIONS:
- ----------

And then I initalize the calulation and inputed the following parameter:

nn	: 2
lstart	: 5 (LSDA), -6.0 (ENERGY to separate core and valence states)

Then, I continue calculate the symmetry. In the output file (.outputs), 
a few sentences appear as below:
- ----------
 PGBSYM: NON-SYMMORPHIC SPACE GROUP OR NON-STANDARD ORIGIN OF COORDINATES
 PGBSYM: SPACE GROUP CONTAINS INVERSION
        BUT ATOMS SHOULD BE SHIFTED BY   0.00000000   0.00000000   
0.25000000
- ----------

Firstly, I ignore the sentence above and continue the calculation but the 
calculation stopped very soon and ask me to shift the coordinates.
 
Then, I convert the coordinates above back to bohr unit and shifted by 
0.25 bohr and then convert the shifted coordinates back to lattice format.  
However, it doesn't work at all and similar sentences appear in file  
(.outputs) again to ask me to shift the coordinates by about 0.21.

Finally, I try to shift the coordinates in lattice format by 0.25 and 
calculate it again. Then, a few sentences appear as below:
- ----------
 PGBSYM: SPACE GROUP IS SYMMORPHIC
 PGBSYM: SPACE GROUP CONTAINS INVERSION
- ----------
Then, I continue the calculation but it also stopped in step "dstart".


My questions are:

How can I fix the above problem?

How does "WIEN In A Box" (wien97 with graphic interface) decide whether my 
coordinates need to be shifted or not? What are the criteria?

Is it possible to have atoms placed outside the unit cell?

Thank you very much

Martin

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------------------------------

Date: Sat, 21 Sep 2002 01:42:24 -0700 (PDT)
From: romdhani hedi <hedi_romdhani2002@yahoo.com>
Subject: Re: [WIEN]: dummy atom

====
romdhani hedi <hedi_romdhani2002@yahoo.com>
submitted the following contribution:
====


- --- koitzsch <Christian.Koitzsch@unifr.ch> wrote:
> Hi Everybody,
> 
> I would like to include "dummy-atoms" with zero
> charge into a structure as some sort of placeholder.
> This would simplify the analysis since I am
> interested in the partial DOS at an interstitial
> site, which is not occupied by an atom. Does anybody
> know how to do that? I think the general question
> is, if one can introduce a muffin tin sphere, which
> is not centered around an atom?
> 
> Thanks a lot and have a nice weekend

Salut
you can introduce empty spheres ( Z=0 ) in different
positions according to your space group ( like LMTO
method ) and run calculations.
best regards
> 
> Christian Koitzsch
> 
> ++++++++++++++++++++++++++++++++++++++++++++
> University of Fribourg
> Dep. of Physics
> Solid State Physics
> CH-1700 Fribourg
> Switzerland
> 


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------------------------------

Date: Sat, 21 Sep 2002 14:32:44 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: dummy atom

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>>I think the general question
> > is, if one can introduce a muffin tin sphere, which
> > is not centered around an atom?

> you can introduce empty spheres ( Z=0 ) in different
> positions according to your space group ( like LMTO
> method ) and run calculations.

What are your interpretation of in1 and in2 files in the case of including
an atom with Z=0?! Would you send us one iteration of your run?
Your,
S. Jalali.

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------------------------------

Date: Sat, 21 Sep 2002 16:48:29 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: 

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0007_01C2618E.B6DD1E30
Content-Type: text/plain;
	charset="iso-8859-1"
Content-Transfer-Encoding: 7bit

> Actually, I would like to build up a unit-cell with 32 atoms and my input
> file is as below:
> ----------
> cnt8010A
> P   LATTICE,NONEQUIV. ATOMS: 3
> MODE OF CALC=RELA
>  18.897269 18.897269  8.055906 90.000000 90.000000 90.000000
> Atom= -1: X=0.81337534 Y=0.50000000 Z=0.08333334
>           MULT= 8          ISPLIT= 8
> Atom= -1: X=0.50000000 Y=0.81337534 Z=0.08333334
> Atom= -1: X=0.18662466 Y=0.50000000 Z=0.08333334
> Atom= -1: X=0.50000000 Y=0.18662466 Z=0.08333334
> Atom= -1: X=0.81337534 Y=0.50000000 Z=0.41666667
> Atom= -1: X=0.50000000 Y=0.81337534 Z=0.41666667
> Atom= -1: X=0.18662466 Y=0.50000000 Z=0.41666667
> Atom= -1: X=0.50000000 Y=0.18662466 Z=0.41666667
> C          NPT=  781  R0=0.00010000 RMT=    1.2000   Z:  6.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -2: X=0.72158983 Y=0.72158983 Z=0.08333334
>           MULT= 8          ISPLIT= 8
> Atom= -2: X=0.27841017 Y=0.72158983 Z=0.08333334
> Atom= -2: X=0.27841017 Y=0.27841017 Z=0.08333334
> Atom= -2: X=0.72158983 Y=0.27841017 Z=0.08333334
> Atom= -2: X=0.72158983 Y=0.72158983 Z=0.41666667
> Atom= -2: X=0.27841017 Y=0.72158983 Z=0.41666667
> Atom= -2: X=0.27841017 Y=0.27841017 Z=0.41666667
> Atom= -2: X=0.72158983 Y=0.27841017 Z=0.41666667
> C          NPT=  781  R0=0.00010000 RMT=    1.2000   Z:  6.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -3: X=0.78952107 Y=0.61992355 Z=0.58333334
>           MULT=16          ISPLIT= 8
> Atom= -3: X=0.61992355 Y=0.78952107 Z=0.58333334
> Atom= -3: X=0.38007645 Y=0.78952107 Z=0.58333334
> Atom= -3: X=0.21047893 Y=0.61992355 Z=0.58333334
> Atom= -3: X=0.21047893 Y=0.38007645 Z=0.58333334
> Atom= -3: X=0.38007645 Y=0.21047893 Z=0.58333334
> Atom= -3: X=0.61992355 Y=0.21047893 Z=0.58333334
> Atom= -3: X=0.78952107 Y=0.38007645 Z=0.58333334
> Atom= -3: X=0.78952107 Y=0.61992355 Z=0.91666667
> Atom= -3: X=0.61992355 Y=0.78952107 Z=0.91666667
> Atom= -3: X=0.38007645 Y=0.78952107 Z=0.91666667
> Atom= -3: X=0.21047893 Y=0.61992355 Z=0.91666667
> Atom= -3: X=0.21047893 Y=0.38007645 Z=0.91666667
> Atom= -3: X=0.38007645 Y=0.21047893 Z=0.91666667
> Atom= -3: X=0.61992355 Y=0.21047893 Z=0.91666667
> Atom= -3: X=0.78952107 Y=0.38007645 Z=0.91666667
> C          NPT=  781  R0=0.00010000 RMT=    1.2000   Z:  6.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
>    0 SYMMETRY OPERATIONS:
> ----------
>
> And then I initalize the calulation and inputed the following parameter:
>
> nn : 2
> lstart : 5 (LSDA), -6.0 (ENERGY to separate core and valence states)
>
> Then, I continue calculate the symmetry. In the output file (.outputs),
> a few sentences appear as below:
> ----------
>  PGBSYM: NON-SYMMORPHIC SPACE GROUP OR NON-STANDARD ORIGIN OF COORDINATES
>  PGBSYM: SPACE GROUP CONTAINS INVERSION
>         BUT ATOMS SHOULD BE SHIFTED BY   0.00000000   0.00000000
> 0.25000000
> ----------
>
> Firstly, I ignore the sentence above and continue the calculation but the
> calculation stopped very soon and ask me to shift the coordinates.
>
> Then, I convert the coordinates above back to bohr unit and shifted by
> 0.25 bohr and then convert the shifted coordinates back to lattice format.
> However, it doesn't work at all and similar sentences appear in file
> (.outputs) again to ask me to shift the coordinates by about 0.21.
>
> Finally, I try to shift the coordinates in lattice format by 0.25 and
> calculate it again. Then, a few sentences appear as below:
> ----------
>  PGBSYM: SPACE GROUP IS SYMMORPHIC
>  PGBSYM: SPACE GROUP CONTAINS INVERSION
> ----------
> Then, I continue the calculation but it also stopped in step "dstart".
>
>
> My questions are:
>
> How can I fix the above problem?

To fix it you would download the attachment which containes proper .struct
and .inst files of your case.

Your,
S. Jalali.

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- ------=_NextPart_000_0007_01C2618E.B6DD1E30--

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------------------------------

Date: Sun, 22 Sep 2002 13:35:12 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: Re: [WIEN]: 

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- --143914132-1161458966-1032672912=:27785
Content-Type: TEXT/PLAIN; charset=US-ASCII

Hi, Saeid Jalali,

Thank you for your files.

Actually, I have changed the unit cell and it is similar to the one you 
sent to me. My input file is as below:

- ------
new10A
P   LATTICE,NONEQUIV. ATOMS: 1
MODE OF CALC=RELA
 18.897269 18.897269  8.055906 90.000000 90.000000 90.000000
Atom= -1: X=0.81337534 Y=0.50000000 Z=0.33333333
          MULT=32 ISPLIT= 8 
Atom= -1: X=0.78952107 Y=0.61992355 Z=0.16666667 
Atom= -1: X=0.72158983 Y=0.72158983 Z=0.33333333 
Atom= -1: X=0.61992355 Y=0.78952107 Z=0.16666667 
Atom= -1: X=0.50000000 Y=0.81337534 Z=0.33333333 
Atom= -1: X=0.38007645 Y=0.78952107 Z=0.16666667 
Atom= -1: X=0.27841017 Y=0.72158983 Z=0.33333333 
Atom= -1: X=0.21047893 Y=0.61992355 Z=0.16666667 
Atom= -1: X=0.18662466 Y=0.50000000 Z=0.33333333 
Atom= -1: X=0.21047893 Y=0.38007645 Z=0.16666667 
Atom= -1: X=0.27841017 Y=0.27841017 Z=0.33333333 
Atom= -1: X=0.38007645 Y=0.21047893 Z=0.16666667 
Atom= -1: X=0.50000000 Y=0.18662466 Z=0.33333333 
Atom= -1: X=0.61992355 Y=0.21047893 Z=0.16666667 
Atom= -1: X=0.72158983 Y=0.27841017 Z=0.33333333 
Atom= -1: X=0.78952107 Y=0.38007645 Z=0.16666667 
Atom= -1: X=0.81337534 Y=0.50000000 Z=0.66666667 
Atom= -1: X=0.78952107 Y=0.61992355 Z=0.83333333 
Atom= -1: X=0.72158983 Y=0.72158983 Z=0.66666667 
Atom= -1: X=0.61992355 Y=0.78952107 Z=0.83333333 
Atom= -1: X=0.50000000 Y=0.81337534 Z=0.66666667 
Atom= -1: X=0.38007645 Y=0.78952107 Z=0.83333333 
Atom= -1: X=0.27841017 Y=0.72158983 Z=0.66666667
Atom= -1: X=0.21047893 Y=0.61992355 Z=0.83333333
Atom= -1: X=0.18662466 Y=0.50000000 Z=0.66666667
Atom= -1: X=0.21047893 Y=0.38007645 Z=0.83333333
Atom= -1: X=0.27841017 Y=0.27841017 Z=0.66666667
Atom= -1: X=0.38007645 Y=0.21047893 Z=0.83333333
Atom= -1: X=0.50000000 Y=0.18662466 Z=0.66666667
Atom= -1: X=0.61992355 Y=0.21047893 Z=0.83333333
Atom= -1: X=0.72158983 Y=0.27841017 Z=0.66666667
Atom= -1: X=0.78952107 Y=0.38007645 Z=0.83333333
C          NPT=  781  R0=0.00010000 RMT=    1.2000   Z:  6.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
   0 SYMMETRY OPERATIONS:
- ------

Then, I initalize the calulation and inputed the following parameter:
nn = 2

Wien97 (WIEN In The Box) finds that it is error for the input file and 
aks me to use a new one that supplied by WIEN. I certainly accept the 
new input file from WIEN. The input file generated by WIEN is attached 
with this mail.

My question is as below:

1. The (.struct) file is different from the one produced by WIEN in terms 
of the classification of the inequivalent atoms. Why? Are they the same?

2. And I found that the bandstructure is plotted automatically by WIEN  
(in the format of ps file). Which files store the information about the  
bandstructure? What information do the following files store? 
Files with extension : (.outputsp),(.spaghetti_ene),(.spaghetti_ps),(.nsh)

3.  Actually, I am trying to get the bandstructure and I am interested in  
the one-directional bandstructure along the c direction and WIEN gives me 
the 3-directional bandstructure. Which part of the bandstructure should I  
look into? 

Thank you very much

Martin


On Sat, 21 Sep 2002, Saeid Jalali wrote:

> > Actually, I would like to build up a unit-cell with 32 atoms and my input
> > file is as below:
> > ----------
> > cnt8010A
> > P   LATTICE,NONEQUIV. ATOMS: 3
> > MODE OF CALC=RELA
> >  18.897269 18.897269  8.055906 90.000000 90.000000 90.000000
> > Atom= -1: X=0.81337534 Y=0.50000000 Z=0.08333334
> >           MULT= 8          ISPLIT= 8
> > Atom= -1: X=0.50000000 Y=0.81337534 Z=0.08333334
> > Atom= -1: X=0.18662466 Y=0.50000000 Z=0.08333334
> > Atom= -1: X=0.50000000 Y=0.18662466 Z=0.08333334
> > Atom= -1: X=0.81337534 Y=0.50000000 Z=0.41666667
> > Atom= -1: X=0.50000000 Y=0.81337534 Z=0.41666667
> > Atom= -1: X=0.18662466 Y=0.50000000 Z=0.41666667
> > Atom= -1: X=0.50000000 Y=0.18662466 Z=0.41666667
> > C          NPT=  781  R0=0.00010000 RMT=    1.2000   Z:  6.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom= -2: X=0.72158983 Y=0.72158983 Z=0.08333334
> >           MULT= 8          ISPLIT= 8
> > Atom= -2: X=0.27841017 Y=0.72158983 Z=0.08333334
> > Atom= -2: X=0.27841017 Y=0.27841017 Z=0.08333334
> > Atom= -2: X=0.72158983 Y=0.27841017 Z=0.08333334
> > Atom= -2: X=0.72158983 Y=0.72158983 Z=0.41666667
> > Atom= -2: X=0.27841017 Y=0.72158983 Z=0.41666667
> > Atom= -2: X=0.27841017 Y=0.27841017 Z=0.41666667
> > Atom= -2: X=0.72158983 Y=0.27841017 Z=0.41666667
> > C          NPT=  781  R0=0.00010000 RMT=    1.2000   Z:  6.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom= -3: X=0.78952107 Y=0.61992355 Z=0.58333334
> >           MULT=16          ISPLIT= 8
> > Atom= -3: X=0.61992355 Y=0.78952107 Z=0.58333334
> > Atom= -3: X=0.38007645 Y=0.78952107 Z=0.58333334
> > Atom= -3: X=0.21047893 Y=0.61992355 Z=0.58333334
> > Atom= -3: X=0.21047893 Y=0.38007645 Z=0.58333334
> > Atom= -3: X=0.38007645 Y=0.21047893 Z=0.58333334
> > Atom= -3: X=0.61992355 Y=0.21047893 Z=0.58333334
> > Atom= -3: X=0.78952107 Y=0.38007645 Z=0.58333334
> > Atom= -3: X=0.78952107 Y=0.61992355 Z=0.91666667
> > Atom= -3: X=0.61992355 Y=0.78952107 Z=0.91666667
> > Atom= -3: X=0.38007645 Y=0.78952107 Z=0.91666667
> > Atom= -3: X=0.21047893 Y=0.61992355 Z=0.91666667
> > Atom= -3: X=0.21047893 Y=0.38007645 Z=0.91666667
> > Atom= -3: X=0.38007645 Y=0.21047893 Z=0.91666667
> > Atom= -3: X=0.61992355 Y=0.21047893 Z=0.91666667
> > Atom= -3: X=0.78952107 Y=0.38007645 Z=0.91666667
> > C          NPT=  781  R0=0.00010000 RMT=    1.2000   Z:  6.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> >    0 SYMMETRY OPERATIONS:
> > ----------
> >
> > And then I initalize the calulation and inputed the following parameter:
> >
> > nn : 2
> > lstart : 5 (LSDA), -6.0 (ENERGY to separate core and valence states)
> >
> > Then, I continue calculate the symmetry. In the output file (.outputs),
> > a few sentences appear as below:
> > ----------
> >  PGBSYM: NON-SYMMORPHIC SPACE GROUP OR NON-STANDARD ORIGIN OF COORDINATES
> >  PGBSYM: SPACE GROUP CONTAINS INVERSION
> >         BUT ATOMS SHOULD BE SHIFTED BY   0.00000000   0.00000000
> > 0.25000000
> > ----------
> >
> > Firstly, I ignore the sentence above and continue the calculation but the
> > calculation stopped very soon and ask me to shift the coordinates.
> >
> > Then, I convert the coordinates above back to bohr unit and shifted by
> > 0.25 bohr and then convert the shifted coordinates back to lattice format.
> > However, it doesn't work at all and similar sentences appear in file
> > (.outputs) again to ask me to shift the coordinates by about 0.21.
> >
> > Finally, I try to shift the coordinates in lattice format by 0.25 and
> > calculate it again. Then, a few sentences appear as below:
> > ----------
> >  PGBSYM: SPACE GROUP IS SYMMORPHIC
> >  PGBSYM: SPACE GROUP CONTAINS INVERSION
> > ----------
> > Then, I continue the calculation but it also stopped in step "dstart".
> >
> >
> > My questions are:
> >
> > How can I fix the above problem?
> 
> To fix it you would download the attachment which containes proper .struct
> and .inst files of your case.
> 
> Your,
> S. Jalali.
> 

- -- 
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~~ "Here is your country, do not let anyone take its glory away  ~~
~~  from you. Do not let selfish men or greedy interests skin    ~~ 
~~  your country of its beauty, its riches, or its romance. The  ~~
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~~                                                               ~~
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~~               -- Theodore Roosevelt, Antiquities Act of 1906  ~~
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

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- --143914132-1161458966-1032672912=:27785--
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------------------------------

Date: Sun, 22 Sep 2002 00:06:55 -0700 (PDT)
From: mehrdad dadsetani <dadsetani_m@yahoo.com>
Subject: [WIEN]: *.inc1

====
mehrdad dadsetani <dadsetani_m@yahoo.com>
submitted the following contribution:
====

dear users wien97(2k)
i have run scf with so, but *.inc1 is empty.


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------------------------------

Date: Sun, 22 Sep 2002 14:12:20 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: 

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

Let's assume your struct works now.

> 1. The (.struct) file is different from the one produced by WIEN in terms
> of the classification of the nonequivalent atoms. Why? Are they the same?
One can not constrain to be equivalent those certain 32 carbons. This means
that you have 3 distinct carbon classes (8, 8, 16) and not one class with 32
atoms. Nature has constrain and wien nicely follows rules: number of space
groups is finite.  Therefore we cannot say that they (a system with 3
distinct carbon classes (8, 8, 16) and a system with one class with 32
atoms) are the same, even though if you plot them they look like the same.

> 2. And I found that the bandstructure is plotted automatically by WIEN
> (in the format of ps file). Which files store the information about the
> bandstructure? What information do the following files store?
> Files with extension : (.outputsp),(.spaghetti_ene),(.spaghetti_ps),(.nsh)
case.spaghetti_ene, which can be used for an XY-plot -- see the description
of line 10 of .insp file.


> 3.  Actually, I am trying to get the bandstructure and I am interested in
> the one-directional bandstructure along the c direction and WIEN gives me
> the 3-directional bandstructure. Which part of the bandstructure should I
> look into?
I suggest to use xcrsden program to generate klist along your favorite
symmetry direction.

Your,

S. jalali

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------------------------------

Date: Sun, 22 Sep 2002 14:48:06 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: *.inc1

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> i have run scf with so, but *.inc1 is empty.
Let's suppose you mean *.in1c and not *.inc1, as there is not such a file in
wien. In this case I wonder why one should necessarily look for .in1c file
in the presence of only spin-orbit.
Your,
S. Jalali.

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------------------------------

Date: Sun, 22 Sep 2002 12:23:49 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: [WIEN]: Symmetso A and B type symmetries - bug?

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

This is a multi-part message in MIME format.
- --------------060707020507040209030207
Content-Type: text/plain; charset=us-ascii; format=flowed
Content-Transfer-Encoding: 7bit

Dear all of you,

I just downloaded the newest version of Wien2k_02, and I have a little 
problem with symmetso. It appears to me that it gives wrong sorting of A 
and B symmetry types. I have attached a structure file for illustration. 
In it is 4 symmetries:

       4      NUMBER OF SYMMETRY OPERATIONS
     1 0 0 0.0000000
     0 1 0 0.0000000
     0 0 1 0.0000000
           1
    -1 0 0 0.0000000
     0-1 0 0.0000000
     0 0 1 0.0000000
           2
     1 0 0 0.0000000
     0-1 0 0.0000000
     0 0 1 0.0000000
           3
    -1 0 0 0.0000000
     0 1 0 0.0000000
     0 0 1 0.0000000
           4

Choosing M as 1.0 0.0 0.0 in .inso I would by hand expect symmetries 1 
and 4 to be of the A type, since M transforms as M_i=det(s)*s_ij*M_j 
under a symmetry operation with the 3x3 matrix s. Then why does symmetso 
tell me that symmetries 1 and 2 are the A type?

Best regards,
Torsten.

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics


- --------------060707020507040209030207
Content-Type: text/plain;
 name="W5Fe110.struct"
Content-Transfer-Encoding: 7bit
Content-Disposition: inline;
 filename="W5Fe110.struct"

5W layers + 1 Fe layer with 10% contraction in the first Fe-W distance         
CXY LATTICE,NONEQUIV. ATOMS: 6 35 Cmm2                                         
MODE OF CALC=RELA                                                              
  8.564901  6.056302 101.06580 90.000000 90.000000 90.000000                   
ATOM= -1: X=0.50000000 Y=0.00000000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Fe1        NPT=  781  R0=0.00000100 RMT=    2.3500   Z: 26.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -2: X=0.00000000 Y=0.00000000 Z=0.46309345
          MULT= 1          ISPLIT= 8
W 1        NPT=  781  R0=0.00000100 RMT=    2.3500   Z: 74.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -3: X=0.50000000 Y=0.00000000 Z=0.42077460
          MULT= 1          ISPLIT= 8
W 2        NPT=  781  R0=0.00000100 RMT=    2.3500   Z: 74.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -4: X=0.00000000 Y=0.00000000 Z=0.37869270
          MULT= 1          ISPLIT= 8
W 3        NPT=  781  R0=0.00000100 RMT=    2.3500   Z: 74.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -5: X=0.50000000 Y=0.00000000 Z=0.33661080
          MULT= 1          ISPLIT= 8
W 4        NPT=  781  R0=0.00000100 RMT=    2.3500   Z: 74.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -6: X=0.00000000 Y=0.00000000 Z=0.29452890
          MULT= 1          ISPLIT= 8
W 5        NPT=  781  R0=0.00000100 RMT=    2.3500   Z: 74.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
   4      NUMBER OF SYMMETRY OPERATIONS
 1 0 0 0.0000000
 0 1 0 0.0000000
 0 0 1 0.0000000
       1
- -1 0 0 0.0000000
 0-1 0 0.0000000
 0 0 1 0.0000000
       2
 1 0 0 0.0000000
 0-1 0 0.0000000
 0 0 1 0.0000000
       3
- -1 0 0 0.0000000
 0 1 0 0.0000000
 0 0 1 0.0000000
       4

- --------------060707020507040209030207
Content-Type: text/plain;
 name="W5Fe110.inso"
Content-Transfer-Encoding: 7bit
Content-Disposition: inline;
 filename="W5Fe110.inso"

WFFIL
 4  1  0                      llmax,ipr,kpot 
 -10.0000   1.50000           emin,emax (output energy window)
   1.  0.  0.                 direction of magnetization (lattice vectors)
  0                           number of atoms for which RLO is added
 NX1   -4.97      0.005       atom number,e-lo,de (case.in1), repeat NX times
 0 0 0 0 0                    number of atoms for which SO is switch off; atoms

- --------------060707020507040209030207
Content-Type: text/plain;
 name="W5Fe110.outsymso"
Content-Transfer-Encoding: 7bit
Content-Disposition: inline;
 filename="W5Fe110.outsymso"

 Magnetization is along  1.0000  0.0000  0.0000 direction
5W layers + 1 Fe layer with 10% contraction in the first Fe-W distance          
  ATOMIC POSITIONS:
    1     4.28245050     0.00000000    50.53290000
    2     0.00000000     0.00000000    46.80291000
    3     4.28245050     0.00000000    42.52592157
    4     0.00000000     0.00000000    38.27288068
    5     4.28245050     0.00000000    34.01983979
    6     0.00000000     0.00000000    29.76679890
 PGLSYM: THE CRYSTAL SYSTEM IS ORTHORHOMBIC
 PGLSYM: ORDER OF LATTICE POINT GROUP (NO BASE) =             8
 PGBSYM: ORDER OF LATTICE SPACE GROUP (WITH BASE) =           4
 PGBSYM: SPACE GROUP IS SYMMORPHIC
 PGBSYM: SPACE GROUP DOES NOT CONTAIN INVERSION
 Symmetry operation           1
       -1.00000        0.00000        0.00000
        0.00000       -1.00000        0.00000
        0.00000        0.00000        1.00000
        0.00000        0.00000        0.00000
   -1.0000    0.0000    0.0000    0.0000
    0.0000   -1.0000    0.0000    0.0000
    0.0000    0.0000    1.0000    0.0000
           this is operation           2   in struct file
 Symmetry operation           2
       -1.00000        0.00000        0.00000
        0.00000        1.00000        0.00000
        0.00000        0.00000        1.00000
        0.00000        0.00000        0.00000
   -1.0000    0.0000    0.0000    0.0000
    0.0000    1.0000    0.0000    0.0000
    0.0000    0.0000    1.0000    0.0000
           this is operation           4   in struct file
 Symmetry operation           3
        1.00000        0.00000        0.00000
        0.00000       -1.00000        0.00000
        0.00000        0.00000        1.00000
        0.00000        0.00000        0.00000
    1.0000    0.0000    0.0000    0.0000
    0.0000   -1.0000    0.0000    0.0000
    0.0000    0.0000    1.0000    0.0000
           this is operation           3   in struct file
 Symmetry operation           4
        1.00000        0.00000        0.00000
        0.00000        1.00000        0.00000
        0.00000        0.00000        1.00000
        0.00000        0.00000        0.00000
    1.0000    0.0000    0.0000    0.0000
    0.0000    1.0000    0.0000    0.0000
    0.0000    0.0000    1.0000    0.0000
           this is operation           1   in struct file
  LATSYM done
5W layers + 1 Fe layer with 10% contract
CXY                          6 35 C
             RELA
  8.564901  6.056302101.065800 90.000000 90.000000 90.000000
      -1     0.5000000    0.0000000    0.5000000
                1                  8
Fe1        NPT=  781  R0=.000001000 RMT=   2.35000   Z:  26.00000
                      1.000000  0.000000  0.000000
                      0.000000  1.000000  0.000000
                      0.000000  0.000000  1.000000
      -2     0.0000000    0.0000000    0.4630935
                1                  8
W 1        NPT=  781  R0=.000001000 RMT=   2.35000   Z:  74.00000
                      1.000000  0.000000  0.000000
                      0.000000  1.000000  0.000000
                      0.000000  0.000000  1.000000
      -3     0.5000000    0.0000000    0.4207746
                1                  8
W 2        NPT=  781  R0=.000001000 RMT=   2.35000   Z:  74.00000
                      1.000000  0.000000  0.000000
                      0.000000  1.000000  0.000000
                      0.000000  0.000000  1.000000
      -4     0.0000000    0.0000000    0.3786927
                1                  8
W 3        NPT=  781  R0=.000001000 RMT=   2.35000   Z:  74.00000
                      1.000000  0.000000  0.000000
                      0.000000  1.000000  0.000000
                      0.000000  0.000000  1.000000
      -5     0.5000000    0.0000000    0.3366108
                1                  8
W 4        NPT=  781  R0=.000001000 RMT=   2.35000   Z:  74.00000
                      1.000000  0.000000  0.000000
                      0.000000  1.000000  0.000000
                      0.000000  0.000000  1.000000
      -6     0.0000000    0.0000000    0.2945289
                1                  8
W 5        NPT=  781  R0=.000001000 RMT=   2.35000   Z:  74.00000
                      1.000000  0.000000  0.000000
                      0.000000  1.000000  0.000000
                      0.000000  0.000000  1.000000
 THETA, PHI   1.57079632679490       0.000000000000000E+000
  symmetry operation           1
   1   0   0
   0   1   0
   0   0   1
  operation type A preserve M direction

  symmetry operation           2
  -1   0   0
   0  -1   0
   0   0   1
  operation type A preserve M direction

  symmetry operation           3
   1   0   0
   0  -1   0
   0   0   1
  operation type B *(time inv.) preserve M direction

  symmetry operation           4
  -1   0   0
   0   1   0
   0   0   1
  operation type B *(time inv.) preserve M direction

 atom   1 not equivalent, new set    1
 atom   2 not equivalent, new set    2
 atom   3 not equivalent, new set    3
 atom   4 not equivalent, new set    4
 atom   5 not equivalent, new set    5
 atom   6 not equivalent, new set    6
 j ind2,ieq   1   1   1
 j ind2,ieq   2   2   1
 j ind2,ieq   3   3   1
 j ind2,ieq   4   4   1
 j ind2,ieq   5   5   1
 j ind2,ieq   6   6   1
 natso=   6
 multso   1   1   1   1   1   1
 ieq   1   1   1   1   1   1
  jatom,ind1,ind2           1           1           1
  rotloc             rotij              rotlso
  1.0000  0.0000  0.0000     1.0000  0.0000  0.0000     1.0000  0.0000  0.0000
  0.0000  1.0000  0.0000     0.0000  1.0000  0.0000     0.0000  1.0000  0.0000
  0.0000  0.0000  1.0000     0.0000  0.0000  1.0000     0.0000  0.0000  1.0000
  jatom,ind1,ind2           2           2           2
  rotloc             rotij              rotlso
  1.0000  0.0000  0.0000     1.0000  0.0000  0.0000     1.0000  0.0000  0.0000
  0.0000  1.0000  0.0000     0.0000  1.0000  0.0000     0.0000  1.0000  0.0000
  0.0000  0.0000  1.0000     0.0000  0.0000  1.0000     0.0000  0.0000  1.0000
  jatom,ind1,ind2           3           3           3
  rotloc             rotij              rotlso
  1.0000  0.0000  0.0000     1.0000  0.0000  0.0000     1.0000  0.0000  0.0000
  0.0000  1.0000  0.0000     0.0000  1.0000  0.0000     0.0000  1.0000  0.0000
  0.0000  0.0000  1.0000     0.0000  0.0000  1.0000     0.0000  0.0000  1.0000
  jatom,ind1,ind2           4           4           4
  rotloc             rotij              rotlso
  1.0000  0.0000  0.0000     1.0000  0.0000  0.0000     1.0000  0.0000  0.0000
  0.0000  1.0000  0.0000     0.0000  1.0000  0.0000     0.0000  1.0000  0.0000
  0.0000  0.0000  1.0000     0.0000  0.0000  1.0000     0.0000  0.0000  1.0000
  jatom,ind1,ind2           5           5           5
  rotloc             rotij              rotlso
  1.0000  0.0000  0.0000     1.0000  0.0000  0.0000     1.0000  0.0000  0.0000
  0.0000  1.0000  0.0000     0.0000  1.0000  0.0000     0.0000  1.0000  0.0000
  0.0000  0.0000  1.0000     0.0000  0.0000  1.0000     0.0000  0.0000  1.0000
  jatom,ind1,ind2           6           6           6
  rotloc             rotij              rotlso
  1.0000  0.0000  0.0000     1.0000  0.0000  0.0000     1.0000  0.0000  0.0000
  0.0000  1.0000  0.0000     0.0000  1.0000  0.0000     0.0000  1.0000  0.0000
  0.0000  0.0000  1.0000     0.0000  0.0000  1.0000     0.0000  0.0000  1.0000
 so. oper.   1 orig.   1 type   A
 so. oper.   2 orig.   2 type   A
  number of A-type operations=           2
 so. oper.   3 orig.   3 type   B
 so. oper.   4 orig.   4 type   B
  number of B-type operations=           2
  System does not have center of inversion
  Warning: clmfile          25  skipped
  Warning: clmfile          26  skipped
  Warning: clmfile          27  skipped
  Warning: clmfile          28  skipped
 Generating clm file          35
  nw     k     j         knew      rhonew              kold
 Generating clm file          36
  nw     k     j         knew      rhonew              kold
 Generating clm file          37
  nw     k     j         knew      rhonew              kold
  SYMSO done
5W layers + 1 Fe layer with 10% contract s-o calc. M||  1.00  0.00  0.00        
  ATOMIC POSITIONS:
    1     4.28245050     0.00000000    50.53290000
    2     0.00000000     0.00000000    46.80291505
    3     4.28245050     0.00000000    42.52592157
    4     0.00000000     0.00000000    38.27288068
    5     4.28245050     0.00000000    34.01983979
    6     0.00000000     0.00000000    29.76679890
 PGLSYM: THE CRYSTAL SYSTEM IS ORTHORHOMBIC
 PGLSYM: ORDER OF LATTICE POINT GROUP (NO BASE) =             8
 PGBSYM: ORDER OF LATTICE SPACE GROUP (WITH BASE) =           4
 PGBSYM: SPACE GROUP IS SYMMORPHIC
 PGBSYM: SPACE GROUP DOES NOT CONTAIN INVERSION
 Symmetry operation           1
       -1.00000        0.00000        0.00000
        0.00000       -1.00000        0.00000
        0.00000        0.00000        1.00000
        0.00000        0.00000        0.00000
   -1.0000    0.0000    0.0000    0.0000
    0.0000   -1.0000    0.0000    0.0000
    0.0000    0.0000    1.0000    0.0000
           this is operation           2   in struct file
 Symmetry operation           2
       -1.00000        0.00000        0.00000
        0.00000        1.00000        0.00000
        0.00000        0.00000        1.00000
        0.00000        0.00000        0.00000
   -1.0000    0.0000    0.0000    0.0000
    0.0000    1.0000    0.0000    0.0000
    0.0000    0.0000    1.0000    0.0000
           this is operation           4   in struct file
 Symmetry operation           3
        1.00000        0.00000        0.00000
        0.00000       -1.00000        0.00000
        0.00000        0.00000        1.00000
        0.00000        0.00000        0.00000
    1.0000    0.0000    0.0000    0.0000
    0.0000   -1.0000    0.0000    0.0000
    0.0000    0.0000    1.0000    0.0000
           this is operation           3   in struct file
 Symmetry operation           4
        1.00000        0.00000        0.00000
        0.00000        1.00000        0.00000
        0.00000        0.00000        1.00000
        0.00000        0.00000        0.00000
    1.0000    0.0000    0.0000    0.0000
    0.0000    1.0000    0.0000    0.0000
    0.0000    0.0000    1.0000    0.0000
           this is operation           1   in struct file
  LATSYM done
5W layers + 1 Fe layer with 10% contract s-o calc. M||  1.00  0.00  0.00       
Fe1       :   2 Atome, Index   1 bis   2
W 1       :   2 Atome, Index   3 bis   4
W 2       :   2 Atome, Index   5 bis   6
W 3       :   2 Atome, Index   7 bis   8
W 4       :   2 Atome, Index   9 bis  10
W 5       :   2 Atome, Index  11 bis  12
  RSTRUCT done
number of atoms:  12
 
 ATOM:          -1
Fe1        G 1 oper. #  1     1                    GM=
Fe1        G 2 oper. #  5     2 || z               GM=
Fe1        G 3 oper. #  7     m n y                GM=
Fe1        G 4 oper. #  8     m n x                GM=
  check whether the operations form a group
  SYMMETRY OPERATIONS FORM A GROUP ,GROUP MULTIPLICATION TABLE:
   i  1  2  3  4
 j
 1    1  2  3  4
 2    2  1  4  3
 3    3  4  1  2
 4    4  3  2  1
  pointgroup is mm2 (neg. iatnr!!)
  axes should be: 2 || z, m n y
  z-rotation vector:  0.0000  0.0000  1.0000
  y-rotation vector:  0.0000  1.0000  0.0000    2
LOCAL ROT MATRIX:       NEW                                OLD
           1.0000000 0.0000000 0.0000000      1.0000000 0.0000000 0.0000000
           0.0000000 1.0000000 0.0000000      0.0000000 1.0000000 0.0000000
           0.0000000 0.0000000 1.0000000      0.0000000 0.0000000 1.0000000
lm: 0 0  1 0  2 0  2 2  3 0  3 2  4 0  4 2  4 4  5 0  5 2  5 4  6 0  6 2  6 4  6 6
 ==============================================
 
 ATOM:          -2
W 1        G 1 oper. #  1     1                    GM=
W 1        G 2 oper. #  5     2 || z               GM=
W 1        G 3 oper. #  7     m n y                GM=
W 1        G 4 oper. #  8     m n x                GM=
  check whether the operations form a group
  SYMMETRY OPERATIONS FORM A GROUP ,GROUP MULTIPLICATION TABLE:
   i  1  2  3  4
 j
 1    1  2  3  4
 2    2  1  4  3
 3    3  4  1  2
 4    4  3  2  1
  pointgroup is mm2 (neg. iatnr!!)
  axes should be: 2 || z, m n y
  z-rotation vector:  0.0000  0.0000  1.0000
  y-rotation vector:  0.0000  1.0000  0.0000    2
LOCAL ROT MATRIX:       NEW                                OLD
           1.0000000 0.0000000 0.0000000      1.0000000 0.0000000 0.0000000
           0.0000000 1.0000000 0.0000000      0.0000000 1.0000000 0.0000000
           0.0000000 0.0000000 1.0000000      0.0000000 0.0000000 1.0000000
lm: 0 0  1 0  2 0  2 2  3 0  3 2  4 0  4 2  4 4  5 0  5 2  5 4  6 0  6 2  6 4  6 6
 ==============================================
 
 ATOM:          -3
W 2        G 1 oper. #  1     1                    GM=
W 2        G 2 oper. #  5     2 || z               GM=
W 2        G 3 oper. #  7     m n y                GM=
W 2        G 4 oper. #  8     m n x                GM=
  check whether the operations form a group
  SYMMETRY OPERATIONS FORM A GROUP ,GROUP MULTIPLICATION TABLE:
   i  1  2  3  4
 j
 1    1  2  3  4
 2    2  1  4  3
 3    3  4  1  2
 4    4  3  2  1
  pointgroup is mm2 (neg. iatnr!!)
  axes should be: 2 || z, m n y
  z-rotation vector:  0.0000  0.0000  1.0000
  y-rotation vector:  0.0000  1.0000  0.0000    2
LOCAL ROT MATRIX:       NEW                                OLD
           1.0000000 0.0000000 0.0000000      1.0000000 0.0000000 0.0000000
           0.0000000 1.0000000 0.0000000      0.0000000 1.0000000 0.0000000
           0.0000000 0.0000000 1.0000000      0.0000000 0.0000000 1.0000000
lm: 0 0  1 0  2 0  2 2  3 0  3 2  4 0  4 2  4 4  5 0  5 2  5 4  6 0  6 2  6 4  6 6
 ==============================================
 
 ATOM:          -4
W 3        G 1 oper. #  1     1                    GM=
W 3        G 2 oper. #  5     2 || z               GM=
W 3        G 3 oper. #  7     m n y                GM=
W 3        G 4 oper. #  8     m n x                GM=
  check whether the operations form a group
  SYMMETRY OPERATIONS FORM A GROUP ,GROUP MULTIPLICATION TABLE:
   i  1  2  3  4
 j
 1    1  2  3  4
 2    2  1  4  3
 3    3  4  1  2
 4    4  3  2  1
  pointgroup is mm2 (neg. iatnr!!)
  axes should be: 2 || z, m n y
  z-rotation vector:  0.0000  0.0000  1.0000
  y-rotation vector:  0.0000  1.0000  0.0000    2
LOCAL ROT MATRIX:       NEW                                OLD
           1.0000000 0.0000000 0.0000000      1.0000000 0.0000000 0.0000000
           0.0000000 1.0000000 0.0000000      0.0000000 1.0000000 0.0000000
           0.0000000 0.0000000 1.0000000      0.0000000 0.0000000 1.0000000
lm: 0 0  1 0  2 0  2 2  3 0  3 2  4 0  4 2  4 4  5 0  5 2  5 4  6 0  6 2  6 4  6 6
 ==============================================
 
 ATOM:          -5
W 4        G 1 oper. #  1     1                    GM=
W 4        G 2 oper. #  5     2 || z               GM=
W 4        G 3 oper. #  7     m n y                GM=
W 4        G 4 oper. #  8     m n x                GM=
  check whether the operations form a group
  SYMMETRY OPERATIONS FORM A GROUP ,GROUP MULTIPLICATION TABLE:
   i  1  2  3  4
 j
 1    1  2  3  4
 2    2  1  4  3
 3    3  4  1  2
 4    4  3  2  1
  pointgroup is mm2 (neg. iatnr!!)
  axes should be: 2 || z, m n y
  z-rotation vector:  0.0000  0.0000  1.0000
  y-rotation vector:  0.0000  1.0000  0.0000    2
LOCAL ROT MATRIX:       NEW                                OLD
           1.0000000 0.0000000 0.0000000      1.0000000 0.0000000 0.0000000
           0.0000000 1.0000000 0.0000000      0.0000000 1.0000000 0.0000000
           0.0000000 0.0000000 1.0000000      0.0000000 0.0000000 1.0000000
lm: 0 0  1 0  2 0  2 2  3 0  3 2  4 0  4 2  4 4  5 0  5 2  5 4  6 0  6 2  6 4  6 6
 ==============================================
 
 ATOM:          -6
W 5        G 1 oper. #  1     1                    GM=
W 5        G 2 oper. #  5     2 || z               GM=
W 5        G 3 oper. #  7     m n y                GM=
W 5        G 4 oper. #  8     m n x                GM=
  check whether the operations form a group
  SYMMETRY OPERATIONS FORM A GROUP ,GROUP MULTIPLICATION TABLE:
   i  1  2  3  4
 j
 1    1  2  3  4
 2    2  1  4  3
 3    3  4  1  2
 4    4  3  2  1
  pointgroup is mm2 (neg. iatnr!!)
  axes should be: 2 || z, m n y
  z-rotation vector:  0.0000  0.0000  1.0000
  y-rotation vector:  0.0000  1.0000  0.0000    2
LOCAL ROT MATRIX:       NEW                                OLD
           1.0000000 0.0000000 0.0000000      1.0000000 0.0000000 0.0000000
           0.0000000 1.0000000 0.0000000      0.0000000 1.0000000 0.0000000
           0.0000000 0.0000000 1.0000000      0.0000000 0.0000000 1.0000000
lm: 0 0  1 0  2 0  2 2  3 0  3 2  4 0  4 2  4 4  5 0  5 2  5 4  6 0  6 2  6 4  6 6
 ==============================================

- --------------060707020507040209030207--

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Date: Mon, 23 Sep 2002 01:15:35 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Symmetso A and B type symmetries - bug?

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

Dear Torsten,
> I just downloaded the newest version of Wien2k_02, and I have a little
> problem with symmetso.
Are you sure that your struct file is not wrong? Are not you concerned about
lopw.f program even regardless spin-orbit or spin polarization (just a
simple run)? This was indicated by the author as an evidence of having not a
correct structure (specifying an atom twice).
Your,
S. Jalali.

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Date: Sun, 22 Sep 2002 17:50:34 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: Re: [WIEN]: Electron density map using w2web

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear Peter and Saeid:

It works now, thanks!


On Fri, 20 Sep 2002, Saeid Jalali wrote:

> ====
> "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> submitted the following contribution:
> ====
>
> > Last question: the w2web requirs case.in2, how can I get one in my case
> > (only case.in2c available)?
> Change session information to include complex calculation (no inversion) to
> active -c in the w2web too.
> Your,
> S. Jalali.
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
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> majordomo@zeus.theochem.tuwien.ac.at
> ====
>



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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Date: Sun, 22 Sep 2002 22:41:55 -0700 (PDT)
From: mehrdad dadsetani <dadsetani_m@yahoo.com>
Subject: [WIEN]: *.in1c empty

====
mehrdad dadsetani <dadsetani_m@yahoo.com>
submitted the following contribution:
====

dear saeed
i wrote for you that my calculation is with
so(spin-orbit).but file *.in1c is empty.
i have done this process
1-initialise 
2-initso
3- run scf
resut
enrgy and charge and fermi energy is converged.you
Know that *.in1c is necesary for band structure,so i
can't calculated band structure.
why *.in1c is empty.
*.in2c isn't empty.
bets wishes 
M.dadsetani 

__________________________________________________
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New DSL Internet Access from SBC & Yahoo!
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Date: Mon, 23 Sep 2002 08:36:10 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: dummy atom

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I would like to include "dummy-atoms" with zero charge into a structure as some sort of placeholder. This would simplify the analysis since I am interested in the partial DOS at an interstitial site, which is not occupied by an atom. Does anybody know how to do that? I think the general question is, if one can introduce a muffin tin sphere, which is not centered around an atom?

In general I do not recommend to use "empty" spheres, but there might be
exceptions where it is usefull for analysis as you indicate above.

During init_lapw put Z=1 (maybe with reduced, but non-zero occupation in
case.inst). Before starting the scf cycle, put Z to zero and correct the number
of electrons in case.in2.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Mon, 23 Sep 2002 10:47:16 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Symmetso A and B type symmetries - bug?

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Saeid,

no atoms are specified more than once. What is lopw.f? Something new? 
Anyway, nn, sgroup, symmetry, and so on behaves well, and the system 
runs nicely through the scf cycle if I just select the right symmetries 
by hand. Symmetry and sgroup finds the four symmetries if I remove the 
symmetries. I still believe there is an undocumented feature (or bug) in 
symmetso for this CXY case. It also did not remove the B types, as it 
should according to the manual, p. 129, for a system without inversion 
symmetry such as this one. For a similar type of calculation, but with a 
P lattice and Cu in stead of W, it finds the right symmetry.

Best regards,
Torsten.

Saeid Jalali wrote:

>====
>"Saeid Jalali" <sjalali@cc.iut.ac.ir>
>submitted the following contribution:
>====
>
>Dear Torsten,
>
>>I just downloaded the newest version of Wien2k_02, and I have a little
>>problem with symmetso.
>>
>Are you sure that your struct file is not wrong? Are not you concerned about
>lopw.f program even regardless spin-orbit or spin polarization (just a
>simple run)? This was indicated by the author as an evidence of having not a
>correct structure (specifying an atom twice).
>Your,
>S. Jalali.
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Mon, 23 Sep 2002 14:03:57 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Symmetso A and B type symmetries - bug?

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0012_01C2630A.0F7517B0
Content-Type: text/plain;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

> no atoms are specified more than once. What is lopw.f? Something new?=20
LOPW is a SUBROUTINE which generates the LAPW (K+G)-vector for local =
orbitals, and it is not new at all.

> Anyway, nn, sgroup, symmetry, and so on behaves well,
I will say.
> and the system=20
> runs nicely through the scf cycle if I just select the right =
symmetries=20
> by hand.
And if you leave symmeties as defualt?

> Symmetry and sgroup finds the four symmetries if I remove the=20
> symmetries. I still believe there is an undocumented feature (or bug) =
in=20
> symmetso for this CXY case. It also did not remove the B types, as it=20
> should according to the manual, p. 129, for a system without inversion =

> symmetry such as this one. For a similar type of calculation, but with =
a=20
> P lattice and Cu in stead of W, it finds the right symmetry.

I have gone through your case using simple run_lapw c-shell script =
without considering anything more, e.g. -so, and found that lapw1 =
complains about LOPW. Now choice is yours to believe whatever you would =
like.
Your,
S. Jalali.

- ------=_NextPart_000_0012_01C2630A.0F7517B0
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY>
<DIV><FONT face=3DArial size=3D2>&gt; no atoms are specified more than =
once. What is=20
lopw.f? Something new? </FONT></DIV>
<DIV><FONT face=3DArial size=3D2>
<P><FONT face=3DArial size=3D2>LOPW is a SUBROUTINE which </FONT><FONT =
face=3DArial=20
size=3D2>generates the LAPW (K+G)-vector for local orbitals, and it is =
not new at=20
all.</FONT></P></DIV></FONT><FONT face=3DArial size=3D2></FONT>
<DIV><FONT face=3DArial size=3D2>&gt; Anyway, nn, sgroup, symmetry, and =
so on=20
behaves well,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>I will say.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>&gt;&nbsp;and the system <BR>&gt; runs =
nicely=20
through the scf cycle if I just select the right symmetries <BR>&gt; by=20
hand.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>And if you leave symmeties as =
defualt?</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>&gt;&nbsp;Symmetry and sgroup finds the =
four=20
symmetries if I remove the <BR>&gt; symmetries. I still believe there is =
an=20
undocumented feature (or bug) in <BR>&gt; symmetso for this CXY case. It =
also=20
did not remove the B types, as it <BR>&gt; should according to the =
manual, p.=20
129, for a system without inversion <BR>&gt; symmetry such as this one. =
For a=20
similar type of calculation, but with a <BR>&gt; P lattice and Cu in =
stead of W,=20
it finds the right symmetry.<BR></FONT></DIV>
<DIV><FONT face=3DArial size=3D2>I have gone through your case using =
simple run_lapw=20
c-shell script without considering anything more, e.g. -so, and found =
that lapw1=20
complains about LOPW. Now choice is yours to believe whatever you would=20
like.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Your,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>S. Jalali.</FONT><FONT face=3DArial=20
size=3D2></DIV></FONT></BODY></HTML>

- ------=_NextPart_000_0012_01C2630A.0F7517B0--

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------------------------------

Date: Mon, 23 Sep 2002 13:03:55 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Symmetso A and B type symmetries - bug?

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I just downloaded the newest version of Wien2k_02, and I have a little
> problem with symmetso. It appears to me that it gives wrong sorting of A
> and B symmetry types. I have attached a structure file for illustration.
> In it is 4 symmetries:
>
>        4      NUMBER OF SYMMETRY OPERATIONS
>      1 0 0 0.0000000
>      0 1 0 0.0000000
>      0 0 1 0.0000000
>            1
>     -1 0 0 0.0000000
>      0-1 0 0.0000000
>      0 0 1 0.0000000
>            2
>      1 0 0 0.0000000
>      0-1 0 0.0000000
>      0 0 1 0.0000000
>            3
>     -1 0 0 0.0000000
>      0 1 0 0.0000000
>      0 0 1 0.0000000
>            4
>
> Choosing M as 1.0 0.0 0.0 in .inso I would by hand expect symmetries 1
> and 4 to be of the A type, since M transforms as M_i=det(s)*s_ij*M_j
> under a symmetry operation with the 3x3 matrix s. Then why does symmetso
> tell me that symmetries 1 and 2 are the A type?

I have tried this using your struct file.
Symmetso correctly describes the second operation as B type (not as A as
you claim) when magnetization is in 1 0 0 direction.

Operation2 is A type for magnetization in (0 0 1) direction.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 23 Sep 2002 12:15:03 +0100 (BST)
From: Vincent Jennings <V.L.Jennings@warwick.ac.uk>
Subject: Re: [WIEN]: Units.

====
Vincent Jennings <V.L.Jennings@warwick.ac.uk>
submitted the following contribution:
====

Dear Saeid,
  Thanks for your comments.  I'm happy now that I have the right
dimensions.  I am still uncertain about the units for Gmax, though.
I guess that they are (a.u.)^-1, but I can't find anything that states
this in the user guide.

  Thanks again,
  Vin.

On Fri, 20 Sep 2002, Saeid Jalali wrote:

> ====
> "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> submitted the following contribution:
> ====
>
> > I posted this question a few days ago, and I know that it's fairly
> > trivial, but I would like confirmation that I have the right units as it
> > is one of the last things that I need to finish off my thesis.  So far I
> > havn't found anything that states the units explicitly.
> >
> > As far as I can tell from the comments in lapw2 files Gmax is in 1/a.u.
>
> > > Hi,
> > >   This should be an easy question...
> > >   I want to check the units for RKmax and Gmax.  I figure RKmax should
> be
> > > dimensionless, and Gmax should have dimension of 1/length.
>
> I don't think that looking for the units of physical quantities is trivial.
> Many refuse to answer such questions and like to pretend they are trivial as
> they come from and return to fundamental physics.
> Yes you are right: the unit of Kmax or Gmax is 1/length, and so R*Kmax is
> dimensionless.
> Your question returns to star space, where we have exp(r.K) with the cutoff
> of Kmax as basis for expanding wavefunctions and exp(r.G) with the cutoff of
> Gmax as basis for expanding charge density and potential energy. So, Kmax
> and Gmax should be dimensionless.
> Your,
> S. Jalali.
>
>
> ====
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- -------------------------------------------------------------------------------
Vincent Jennings			"Some days you're the pigeon
email: V.L.Jennings@warwick.ac.uk	 and some days you're the statue."
- -------------------------------------------------------------------------------

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Date: Mon, 23 Sep 2002 13:31:20 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Symmetso A and B type symmetries - bug?

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Peter,

So maybe I have misunderstood something. My symmetso just did it again...

Does h,k,l in case.inso in any way correspond to a,b,c in case.struct?

And yes, I know how it should be with M along a,b, or c.

Best regards,
Torsten.

Peter Blaha wrote:

>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
>>I just downloaded the newest version of Wien2k_02, and I have a little
>>problem with symmetso. It appears to me that it gives wrong sorting of A
>>and B symmetry types. I have attached a structure file for illustration.
>>In it is 4 symmetries:
>>
>>       4      NUMBER OF SYMMETRY OPERATIONS
>>     1 0 0 0.0000000
>>     0 1 0 0.0000000
>>     0 0 1 0.0000000
>>           1
>>    -1 0 0 0.0000000
>>     0-1 0 0.0000000
>>     0 0 1 0.0000000
>>           2
>>     1 0 0 0.0000000
>>     0-1 0 0.0000000
>>     0 0 1 0.0000000
>>           3
>>    -1 0 0 0.0000000
>>     0 1 0 0.0000000
>>     0 0 1 0.0000000
>>           4
>>
>>Choosing M as 1.0 0.0 0.0 in .inso I would by hand expect symmetries 1
>>and 4 to be of the A type, since M transforms as M_i=det(s)*s_ij*M_j
>>under a symmetry operation with the 3x3 matrix s. Then why does symmetso
>>tell me that symmetries 1 and 2 are the A type?
>>
>
>I have tried this using your struct file.
>Symmetso correctly describes the second operation as B type (not as A as
>you claim) when magnetization is in 1 0 0 direction.
>
>Operation2 is A type for magnetization in (0 0 1) direction.
>
>Regards
>
>                                      P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
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>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Mon, 23 Sep 2002 15:16:17 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: *.in1c empty

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> you Know that *.in1c is necesary for band structure,so i
> can't calculated band structure.
I don't know that: case.in1c is necessary just in the absent of inversion
symmetry. I paste below a comment in this respect from the Aouther,
"Even in a non-spinpolarized case the eigenvectors from lapwso are always
complex numbers, so one must use lapw2c (and in2c), but not lapw1c or in1c
(if inversion is present)."
> why *.in1c is empty.
> *.in2c isn't empty.
It should be clear now. Anyway if you think that your system does not have
inversion, you can simply move case.in1 to case.in1c.
Your,
S. jalali.

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Date: Mon, 23 Sep 2002 16:56:16 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Units.

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>  I am still uncertain about the units for Gmax, though.
> I guess that they are (a.u.)^-1, but I can't find anything that states
> this in the user guide.
Yes, they are: see description of rkmax.
Your,
S. Jalali.

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------------------------------

Date: Mon, 23 Sep 2002 15:20:14 +0200
From: =?US-ASCII?Q?Anders_Froseth?= <anders.froseth@phys.ntnu.no>
Subject: SV: [WIEN]: Units.

====
=?US-ASCII?Q?Anders_Froseth?= <anders.froseth@phys.ntnu.no>
submitted the following contribution:
====


Dear Vincent,

The units for GMAX, (as stated in the .scf file) are Ry**(1/2).
This makes GMAX "proportional" to the magnitude of the largest vector
in the Fourier expansion of the charge density and potential in 
the interstitial region. You have to play around with atomic units: 

GMAX = (E_max)**(1/2) = h_bar*K_max/(2*m_electron)**(1/2)  
 
and in atomic units the constant
of proportionality is equal to 1 (h_bar**2/2m = 1) and

GMAX = (E_max)**(1/2) = K_max

Regards,

Anders

> -----Opprinnelig melding-----
> Fra: owner-wien@zeus.theochem.tuwien.ac.at
> [mailto:owner-wien@zeus.theochem.tuwien.ac.at]Pa vegne av Vincent
> Jennings
> Sendt: 23. september 2002 13:15
> Til: wien@zeus.theochem.tuwien.ac.at
> Emne: Re: [WIEN]: Units.
> 
> 
> ====
> Vincent Jennings <V.L.Jennings@warwick.ac.uk>
> submitted the following contribution:
> ====
> 
> Dear Saeid,
>   Thanks for your comments.  I'm happy now that I have the right
> dimensions.  I am still uncertain about the units for Gmax, though.
> I guess that they are (a.u.)^-1, but I can't find anything that states
> this in the user guide.
> 
>   Thanks again,
>   Vin.
> 
> On Fri, 20 Sep 2002, Saeid Jalali wrote:
> 
> > ====
> > "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> > submitted the following contribution:
> > ====
> >
> > > I posted this question a few days ago, and I know that it's fairly
> > > trivial, but I would like confirmation that I have the right 
> units as it
> > > is one of the last things that I need to finish off my 
> thesis.  So far I
> > > havn't found anything that states the units explicitly.
> > >
> > > As far as I can tell from the comments in lapw2 files Gmax is 
> in 1/a.u.
> >
> > > > Hi,
> > > >   This should be an easy question...
> > > >   I want to check the units for RKmax and Gmax.  I figure 
> RKmax should
> > be
> > > > dimensionless, and Gmax should have dimension of 1/length.
> >
> > I don't think that looking for the units of physical quantities 
> is trivial.
> > Many refuse to answer such questions and like to pretend they 
> are trivial as
> > they come from and return to fundamental physics.
> > Yes you are right: the unit of Kmax or Gmax is 1/length, and so 
> R*Kmax is
> > dimensionless.
> > Your question returns to star space, where we have exp(r.K) 
> with the cutoff
> > of Kmax as basis for expanding wavefunctions and exp(r.G) with 
> the cutoff of
> > Gmax as basis for expanding charge density and potential 
> energy. So, Kmax
> > and Gmax should be dimensionless.
> > Your,
> > S. Jalali.
> >
> >
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
> > majordomo@zeus.theochem.tuwien.ac.at
> > ====
> >
> 
> ------------------------------------------------------------------
> -------------
> Vincent Jennings			"Some days you're the pigeon
> email: V.L.Jennings@warwick.ac.uk	 and some days you're the statue."
> ------------------------------------------------------------------
> -------------
> 
> ====
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------------------------------

Date: Mon, 23 Sep 2002 15:30:35 +0100 (BST)
From: Vincent Jennings <V.L.Jennings@warwick.ac.uk>
Subject: Re: SV: [WIEN]: Units.

====
Vincent Jennings <V.L.Jennings@warwick.ac.uk>
submitted the following contribution:
====

Thanks Saeid and Anders,
  I should have thought to look in the scf file.  That makes sense now.
  Vincent

On Mon, 23 Sep 2002, Anders Froseth wrote:

> ====
> =?US-ASCII?Q?Anders_Froseth?= <anders.froseth@phys.ntnu.no>
> submitted the following contribution:
> ====
>
>
> Dear Vincent,
>
> The units for GMAX, (as stated in the .scf file) are Ry**(1/2).
> This makes GMAX "proportional" to the magnitude of the largest vector
> in the Fourier expansion of the charge density and potential in
> the interstitial region. You have to play around with atomic units:
>
> GMAX = (E_max)**(1/2) = h_bar*K_max/(2*m_electron)**(1/2)
>
> and in atomic units the constant
> of proportionality is equal to 1 (h_bar**2/2m = 1) and
>
> GMAX = (E_max)**(1/2) = K_max
>
> Regards,
>
> Anders
>
> > -----Opprinnelig melding-----
> > Fra: owner-wien@zeus.theochem.tuwien.ac.at
> > [mailto:owner-wien@zeus.theochem.tuwien.ac.at]Pa vegne av Vincent
> > Jennings
> > Sendt: 23. september 2002 13:15
> > Til: wien@zeus.theochem.tuwien.ac.at
> > Emne: Re: [WIEN]: Units.
> >
> >
> > ====
> > Vincent Jennings <V.L.Jennings@warwick.ac.uk>
> > submitted the following contribution:
> > ====
> >
> > Dear Saeid,
> >   Thanks for your comments.  I'm happy now that I have the right
> > dimensions.  I am still uncertain about the units for Gmax, though.
> > I guess that they are (a.u.)^-1, but I can't find anything that states
> > this in the user guide.
> >
> >   Thanks again,
> >   Vin.
> >
> > On Fri, 20 Sep 2002, Saeid Jalali wrote:
> >
> > > ====
> > > "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> > > submitted the following contribution:
> > > ====
> > >
> > > > I posted this question a few days ago, and I know that it's fairly
> > > > trivial, but I would like confirmation that I have the right
> > units as it
> > > > is one of the last things that I need to finish off my
> > thesis.  So far I
> > > > havn't found anything that states the units explicitly.
> > > >
> > > > As far as I can tell from the comments in lapw2 files Gmax is
> > in 1/a.u.
> > >
> > > > > Hi,
> > > > >   This should be an easy question...
> > > > >   I want to check the units for RKmax and Gmax.  I figure
> > RKmax should
> > > be
> > > > > dimensionless, and Gmax should have dimension of 1/length.
> > >
> > > I don't think that looking for the units of physical quantities
> > is trivial.
> > > Many refuse to answer such questions and like to pretend they
> > are trivial as
> > > they come from and return to fundamental physics.
> > > Yes you are right: the unit of Kmax or Gmax is 1/length, and so
> > R*Kmax is
> > > dimensionless.
> > > Your question returns to star space, where we have exp(r.K)
> > with the cutoff
> > > of Kmax as basis for expanding wavefunctions and exp(r.G) with
> > the cutoff of
> > > Gmax as basis for expanding charge density and potential
> > energy. So, Kmax
> > > and Gmax should be dimensionless.
> > > Your,
> > > S. Jalali.
> > >
> > >
> > > ====
> > > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > > To (un)subscribe send mail to
> > > majordomo@zeus.theochem.tuwien.ac.at
> > > ====
> > >
> >
> > ------------------------------------------------------------------
> > -------------
> > Vincent Jennings			"Some days you're the pigeon
> > email: V.L.Jennings@warwick.ac.uk	 and some days you're the statue."
> > ------------------------------------------------------------------
> > -------------
> >
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
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> > ====
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

- -------------------------------------------------------------------------------
Vincent Jennings			"Some days you're the pigeon
email: V.L.Jennings@warwick.ac.uk	 and some days you're the statue."
- -------------------------------------------------------------------------------




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------------------------------

Date: Mon, 23 Sep 2002 18:45:12 +0430
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Units.

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> >  I am still uncertain about the units for Gmax, though.
> > I guess that they are (a.u.)^-1, but I can't find anything that states
> > this in the user guide.
> Yes, they are: see description of rkmax.
In the description of rkamx, one finds how my fast above confirmation is
unclean in contrast to the clean one of Anders!!!
Thank you Anders.
Your,
S. Jalali.


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------------------------------

Date: Tue, 24 Sep 2002 09:13:44 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: [WIEN]: case.inso

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Hello again,

the symmetso problem was solved, thanks to Peter Blaha.

Now a simple question about case.inso, since it has changed from 
Wien2k_01 to Wien2k_02.

If I don't want rlo's, do I have to delete "line 6"? In the old 
case.inso it was just ignored, I think. In the new case.inso there is a 
"line 7", however. If in "line 5" I have put a zero, what does the 
program expect next, a single line 6 or no line 6, but line 7 in stead?

Yes, I guess it could be read by sifting through the code, but I think 
it should be clear in the manual...

Best regards,
Torsten.

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics


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------------------------------

Date: Tue, 24 Sep 2002 17:43:03 +1000
From: chen0130@flinders.edu.au
Subject: [WIEN]: occupied bands

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Dear Wien users,

Can anyone tell me if there is a way in Wien to find out which bands are
occupied (eg by the bandindex number)?

As there are many bands that emerge from a bandstruct calc for slabs...

Maybe a density of states calc would be helpful?

Thanks for your time!

Cheng


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------------------------------

Date: Tue, 24 Sep 2002 10:03:44 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: occupied bands

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

It can not be done that simple, as bands do cross the Fermi energy in 
many systems.

Thereby I have also said how you can find out... Wien2k gives you the 
Fermi energy and the energies for each k-point, so all those below the 
Fermi energy are occupied and all those above are unoccupied. A density 
of states calculation (or a spaghetti) can, if enough k-points are 
involved, give you a fairly good hint about if crossing bands exists.

Best regards,
Torsten.

chen0130@flinders.edu.au wrote:

>====
>chen0130@flinders.edu.au
>submitted the following contribution:
>====
>
>Dear Wien users,
>
>Can anyone tell me if there is a way in Wien to find out which bands are
>occupied (eg by the bandindex number)?
>
>As there are many bands that emerge from a bandstruct calc for slabs...
>
>Maybe a density of states calc would be helpful?
>
>Thanks for your time!
>
>Cheng
>
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Tue, 24 Sep 2002 10:16:13 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: occupied bands

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Oh... and, if no bands cross the Fermi energy, you indeed can use the 
band index.

Best regards,
Torsten.

Torsten Andersen wrote:

> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
>
> It can not be done that simple, as bands do cross the Fermi energy in 
> many systems.
>
> Thereby I have also said how you can find out... Wien2k gives you the 
> Fermi energy and the energies for each k-point, so all those below the 
> Fermi energy are occupied and all those above are unoccupied. A 
> density of states calculation (or a spaghetti) can, if enough k-points 
> are involved, give you a fairly good hint about if crossing bands exists.
>
> Best regards,
> Torsten.
>
> chen0130@flinders.edu.au wrote:
>
>> ====
>> chen0130@flinders.edu.au
>> submitted the following contribution:
>> ====
>>
>> Dear Wien users,
>>
>> Can anyone tell me if there is a way in Wien to find out which bands are
>> occupied (eg by the bandindex number)?
>>
>> As there are many bands that emerge from a bandstruct calc for slabs...
>>
>> Maybe a density of states calc would be helpful?
>>
>> Thanks for your time!
>>
>> Cheng
>>
>>
>> ====
>> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>> To (un)subscribe send mail to
>> majordomo@zeus.theochem.tuwien.ac.at
>> ====
>>
>>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Tue, 24 Sep 2002 10:57:45 +0200
From: "Antoine Villesuzanne" <ville@icmcb.u-bordeaux.fr>
Subject: [WIEN]: Partial DOS/Tetra

====
"Antoine Villesuzanne" <ville@icmcb.u-bordeaux.fr>
submitted the following contribution:
====

Calculating the partial DOS for :
(i) one atom type
(ii) one atomic orbital for one atom type
does not give consistent results since the atom type mutiplicity is
accounted for in (i), but not in (ii).
In other words, for a given atom type, the sum of atomic orbital
contributions to the DOS is equal to the atom type partial DOS divided by
the multiplicity.
This may lead to wrong conclusions and should be corrected in tetra.

Regards

Antoine Villesuzanne
ICMCB-CNRS
87 Av. Dr. Schweitzer
33608 Pessac cedex
France
ville@icmcb.u-bordeaux.fr


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------------------------------

Date: Tue, 24 Sep 2002 10:56:51 +0200
From: "koitzsch" <Christian.Koitzsch@unifr.ch>
Subject: Re: [WIEN]: occupied bands

====
"koitzsch" <Christian.Koitzsch@unifr.ch>
submitted the following contribution:
====

hope I understood the question correctly:


In principle you know your Fermi Energy from the output of your scf cycle.
This would tell you up to which energy your bands are filled. Then you just
have to see if you have eigenvalues in a particular band below this level,
which would render your band filled.

I think the best way to see that is a conventional band structure plot. It
answers all this, since you have to tell the program the correct Fermi
Energy in case.insp from case.scf


Best Regards

Christian Koitzsch


- ----- Original Message -----
From: <chen0130@flinders.edu.au>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Tuesday, September 24, 2002 9:43 AM
Subject: [WIEN]: occupied bands


> ====
> chen0130@flinders.edu.au
> submitted the following contribution:
> ====
>
> Dear Wien users,
>
> Can anyone tell me if there is a way in Wien to find out which bands are
> occupied (eg by the bandindex number)?
>
> As there are many bands that emerge from a bandstruct calc for slabs...
>
> Maybe a density of states calc would be helpful?
>
> Thanks for your time!
>
> Cheng
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>


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------------------------------

Date: Tue, 24 Sep 2002 18:42:02 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]:

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Hi,

Actually, I am trying to calculate the optical properties of my molecule. 
And after I have performed "optic". I found that the output file ".outmat" 
only containing 4 K-point. Then, I look back to the file ".outputkgen". 

The ".outputkgen" is as below:

ortho=  T
 R1 =  18.897269  0.000000  0.000000
 R2 =   0.000000 18.897269  0.000000
 R3 =   0.000000  0.000000  4.651079
 DEPENDENCE OF DIVISION OF TRANSLATION VECTORS IARB=  0  0  0
 NAME OF POINT GROUP =     INVERSION = 1
 ERROR : POINT GROUP NAME  NOT IN THE LIST, CHECK :   BRADLEY AND CRACKNELL
 NUMBER OF POINT GROUP OPERATIONS =    2
   SYMMETRY MATRIX NR.  1   SYMMETRY MATRIX NR.  2   SYMMETRY MATRIX NR.  3   SYMMETRY MATRIX NR.  4
       1    0    0             -1    0    0              0    0    0              0    0    0
       0    1    0              0   -1    0              0    0    0              0    0    0
       0    0    1              0    0   -1              0    0    0              0    0    0
   SYMMETRY MATRIX NR.  1   SYMMETRY MATRIX NR.  2   SYMMETRY MATRIX NR.  3   SYMMETRY MATRIX NR.  4
      -1    0    0              1    0    0             -1    0    0              1    0    0
       0   -1    0              0    1    0              0   -1    0              0    1    0
       0    0   -1              0    0    1              0    0    1              0    0   -1
   G1        G2        G3
  0.052918  0.000000  0.000000
  0.000000  0.052918  0.000000
  0.000000  0.000000  0.215004
   G1        G2        G3
  0.332492  0.000000  0.000000
  0.000000  0.332492  0.000000
  0.000000  0.000000  1.350909
 length of reciprocal lattic vectors:  1.70109365  1.70109365  6.91151972
 SUBMESH SHIFTED; SHIFT:  0 0 0
 NO. OF MESH POINTS IN THE BRILLOUIN ZONE =     6
 DIVISION OF RECIPROCAL LATTICE VECTORS (INTERVALS)=    1    1    6
 point    coordinates     relation
   1        0   0   0       1   0.12500   0.12500
   2        0   0   1       2   0.25000   0.25000
   3        0   0   2       3   0.25000   0.25000
   4        0   0   3       4   0.25000   0.25000
   5        0   0   4       3   0.25000   0.50000
   6        0   0   5       2   0.25000   0.50000
   7        0   0   6       1   0.12500   0.25000
   8        0   1   0       1   0.12500   0.37500
   9        0   1   1       2   0.25000   0.75000
  10        0   1   2       3   0.25000   0.75000
  11        0   1   3       4   0.25000   0.50000
  12        0   1   4       3   0.25000   1.00000
  13        0   1   5       2   0.25000   1.00000
  14        0   1   6       1   0.12500   0.50000
  15        1   0   0       1   0.12500   0.62500
  16        1   0   1       2   0.25000   1.25000
  17        1   0   2       3   0.25000   1.25000
  18        1   0   3       4   0.25000   0.75000
  19        1   0   4       3   0.25000   1.50000
  20        1   0   5       2   0.25000   1.50000
  21        1   0   6       1   0.12500   0.75000
  22        1   1   0       1   0.12500   0.87500
  23        1   1   1       2   0.25000   1.75000
  24        1   1   2       3   0.25000   1.75000
  25        1   1   3       4   0.25000   1.00000
  26        1   1   4       3   0.25000   2.00000
  27        1   1   5       2   0.25000   2.00000
  28        1   1   6       1   0.12500   1.00000
 weights of k-points:
      1       1    1.000000    0.333333
      2       2    2.000000    0.666667
      3       3    2.000000    0.666667
      4       4    1.000000    0.333333
 sum of weights:     2.000000
 internal and cartesian k-vectors:
  0.00000   0.00000   0.00000             0.00000   0.00000   0.00000
  0.00000   0.00000   0.16667             0.00000   0.00000   0.22515
  0.00000   0.00000   0.33333             0.00000   0.00000   0.45030
  0.00000   0.00000   0.50000             0.00000   0.00000   0.67545
 NO. OF INEQUIVALENT K-POINTS     4
 INEQUIVALENT BLOCH VECTORS
   1(  0.000000  0.000000  0.000000)   2 (  0.000000  0.000000  0.225152)
   3(  0.000000  0.000000  0.450303)   4 (  0.000000  0.000000  0.675455)

NUMBER OF DIFFERENT TETRAHEDRA :    9
NKP,NDIV,afact  4 1 1 6  1.
    0.00000     0.00000     0.00000                0.00000      0.00000      0.00000
    0.00000     0.00000     0.16667                0.00000      0.00000      2.00000
    0.00000     0.00000     0.33333                0.00000      0.00000      4.00000
    0.00000     0.00000     0.50000                0.00000      0.00000      6.00000

My questions are as below:
1. What does the "reciprocal lattic vectors" mean?
2. How does wien get the "NO. OF MESH POINTS IN THE BRILLOUIN ZONE"? What does this value mean?
  

Thank you very much

Martin


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------------------------------

Date: Tue, 24 Sep 2002 14:09:20 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re:  [WIEN]: Partial DOS/Tetra

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> Calculating the partial DOS for :
> (i) one atom type
> (ii) one atomic orbital for one atom type
> does not give consistent results since the atom type mutiplicity is
> accounted for in (i), but not in (ii).
> In other words, for a given atom type, the sum of atomic orbital
> contributions to the DOS is equal to the atom type partial DOS divided by
> the multiplicity.
> This may lead to wrong conclusions and should be corrected in tetra.
This is perfectly recognized by you, is not this?!
You,
S. Jalali.

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Date: Tue, 24 Sep 2002 13:20:17 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: occupied bands

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Can anyone tell me if there is a way in Wien to find out which bands are
> occupied (eg by the bandindex number)?
>
> As there are many bands that emerge from a bandstruct calc for slabs...
>
> Maybe a density of states calc would be helpful?
>
> Thanks for your time!

Have a look into case.output2 (up/dn). At the top you find e-fermi, but
also the emin/emax of each band (ordered by bandindex), so that you
easily can judge how many bands are fully occupied and how many bands
cross EF.

(The same info is also given in case.outputt (after tetra).

Of course in a metallic situation you then must plot a bandstructure to
get more insight.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Tue, 24 Sep 2002 19:38:56 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: 

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Hi,

I would like to consult about the deftinition of somr terms in wien od 
solid-state physics.

1. definition of "momentum matrix elements" (Is it the same as transition 
dipole moment?)
2. definition of k-mesh (What is the differences between k-mesh and 
k-point?)

Thank you very much

Martin

- -- 
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
~~ "Here is your country, do not let anyone take its glory away  ~~
~~  from you. Do not let selfish men or greedy interests skin    ~~ 
~~  your country of its beauty, its riches, or its romance. The  ~~
~~  world and the future and your very children shall judge you  ~~
~~  according to the way you deal with this sacred trust."       ~~
~~                                                               ~~
~~                                                               ~~
~~               -- Theodore Roosevelt, Antiquities Act of 1906  ~~
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

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Date: Tue, 24 Sep 2002 13:31:30 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: case.inso

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

So, I took a dive into the code. In SRC_lapwso/init.f I found:

- --BEGIN QUOTE CODE---
!rschmid
!  read in parameters for basis extension by relativistic basis function.
!rschmid
      do ity=1,nat
      nlr(ity)=0
      end do
      read(5,*,end=644)nrelcase
      do i=1,nrelcase
         read(5,*) ity,edum1,edum2
         extei(ity,1)=edum1
         extde(ity,1)=edum2
         nlr(ity)=1
      enddo
 644      read(5,*,end=345)noff,(iatoff(i),i=1,noff)
        do i=1,noff
        lso(iatoff(i))=.false.
        write(6,*)'SOC on atom ',iatoff(i),'SWITCHED OFF !!!'
        enddo
 345      continue
 5000 format (1x,i1,2f10.5,a4)
- -- END QUOTE CODE ---

It is clear to me what happens up to and including 
read(5,*,end=644)nrelcase. However, do i=1,nrelcase then becomes do 
i=1,0 if nrelcase is put to zero. Now I know that if the standard of 
Fortran90 is followed, the do-loop is not executed [Metcalf & Reid, p. 
73], and thus to get correct input, "line 6" has to be deleted, unless 
the first number in it is 0. I also remember to have seen in some places 
that for certain "default" options of compilers, do-loops gets run at 
least once... so there could be a potential problem there...

So I answered my question first, it seems :-) Any comments?

Torsten Andersen wrote:

> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
>
> Hello again,
>
> the symmetso problem was solved, thanks to Peter Blaha.
>
> Now a simple question about case.inso, since it has changed from 
> Wien2k_01 to Wien2k_02.
>
> If I don't want rlo's, do I have to delete "line 6"? In the old 
> case.inso it was just ignored, I think. In the new case.inso there is 
> a "line 7", however. If in "line 5" I have put a zero, what does the 
> program expect next, a single line 6 or no line 6, but line 7 in stead?
>
> Yes, I guess it could be read by sifting through the code, but I think 
> it should be clear in the manual...
>
> Best regards,
> Torsten.
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Tue, 24 Sep 2002 13:36:12 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: case.inso

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Oops. It should be "line 6" has to be deleted, unless the first number 
in it is 0, or "line 7" is needed.

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Tue, 24 Sep 2002 13:46:43 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]:

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Hi,

1. Momentum matrix elements are usually <r,l|p|r',l'> where the "p" is 
the momentum operator. The transition dipole moment can be the same, but 
is not necessary that. It depends on the context.

2. A k-mesh is the grid of k-points used when calculating. You could 
call it k-point sampling set - it is the sampling points in the 
numerical approximation used to replace integrals with sums.

Was this of any help? Otherwise, ask again...

Best regards,
Torsten Andersen.

Ma Chi Chiu wrote:

>====
>Ma Chi Chiu <martin@yangtze.hku.hk>
>submitted the following contribution:
>====
>
>Hi,
>
>I would like to consult about the deftinition of somr terms in wien od 
>solid-state physics.
>
>1. definition of "momentum matrix elements" (Is it the same as transition 
>dipole moment?)
>2. definition of k-mesh (What is the differences between k-mesh and 
>k-point?)
>
>Thank you very much
>
>Martin
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



====
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------------------------------

Date: Tue, 24 Sep 2002 14:52:56 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Partial DOS/Tetra

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

On Tue, 24 Sep 2002, Antoine Villesuzanne wrote:

> ====
> "Antoine Villesuzanne" <ville@icmcb.u-bordeaux.fr>
> submitted the following contribution:
> ====
>
> Calculating the partial DOS for :
> (i) one atom type
> (ii) one atomic orbital for one atom type
> does not give consistent results since the atom type mutiplicity is
> accounted for in (i), but not in (ii).
> In other words, for a given atom type, the sum of atomic orbital
> contributions to the DOS is equal to the atom type partial DOS divided by
> the multiplicity.
> This may lead to wrong conclusions and should be corrected in tetra.

This is not an error, but a "feature" (documented in the UG (section TETRA))
I admit it might be unusual, but the idea is:

In the decomposition of the total DOS into contributions of
atoms, I want to include the multiplicity, so that I get an idea of which
atoms contribute with which amount to a DOS at a particular energy.

On the other hand, the lm-like DOS I want to see per atom, so that I can get
a feeling about a possible chemical bonding. It is something like the
coefficient in front of a basis function (or an orbital population).

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 24 Sep 2002 15:03:37 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: case.inso

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> If I don't want rlo's, do I have to delete "line 6"? In the old
> case.inso it was just ignored, I think. In the new case.inso there is a
> "line 7", however. If in "line 5" I have put a zero, what does the
> program expect next, a single line 6 or no line 6, but line 7 in stead?
>
> Yes, I guess it could be read by sifting through the code, but I think
> it should be clear in the manual...

The UG states line 6 should be repeated nrl times, i.e. if nrl=0 it should
not be present at all.
I will add this explicitly in the UG.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 24 Sep 2002 09:26:06 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: case.inso

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====

On September 24, 2002 07:31 am, Torsten Andersen wrote:
> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
>
> So, I took a dive into the code. In SRC_lapwso/init.f I found:
>
> <snipped code for brevity>
>
> I also remember to have seen in some places that for certain
> "default" options of compilers, do-loops gets run at least
> once... so there could be a potential problem there...

I have only seen "forcing each do loop to execute at least once" as
a compiler option that is turned off by default. Do you remember which
compiler has this turned on.

> So I answered my question first, it seems :-) Any comments?

For no RLOs I use something like the following case.inso (depending on
details). The older style case.inso (WIEN2k_01) doesn't work sometimes, since
there is the new option of switching off SO for individual atoms.

WFFIL
 4  1  0                      llmax,ipr,kpot
 -10.0000   5.00000           emin,emax (output energy window)
   0.  0.  1.                 direction of magnetization (lattice vectors)
 0                            number of atoms for which RLO is added
 0 0 0 0 0                    number of atoms for which SO is switch off;atoms

Cheers,

Fred

> Torsten Andersen wrote:
> > ====
> > Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> > submitted the following contribution:
> > ====
> >
> > Hello again,
> >
> > the symmetso problem was solved, thanks to Peter Blaha.
> >
> > Now a simple question about case.inso, since it has changed from
> > Wien2k_01 to Wien2k_02.
> >
> > If I don't want rlo's, do I have to delete "line 6"? In the old
> > case.inso it was just ignored, I think. In the new case.inso there is
> > a "line 7", however. If in "line 5" I have put a zero, what does the
> > program expect next, a single line 6 or no line 6, but line 7 in stead?
> >
> > Yes, I guess it could be read by sifting through the code, but I think
> > it should be clear in the manual...
> >
> > Best regards,
> > Torsten.

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Date: Tue, 24 Sep 2002 09:45:07 -0400
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]:

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====

On September 24, 2002 07:38 am, Ma Chi Chiu wrote:
> ====
> Ma Chi Chiu <martin@yangtze.hku.hk>
> submitted the following contribution:
> ====

Before I pushed send, I noticed Dr. Andersen has allready replied. Just
to add though...

> 1. definition of "momentum matrix elements" (Is it the same as transition
> dipole moment?)

The momentum matrix element is defined as,

	<nk|p|mk> = int d^3r <nk|r> i hbar nabla <r|mk>

 where |nk> is a Bloch state. The wien code uses Rydberg atomic units 
(throughout), in which hbar=m=e=1. The atomic unit for momentum (Ry or H)
is hbar/a0 (where a0 is the Bohr radius).

The dipole matrix element is usually <nk|r|mk>. If n and m are different bands
the two matrix elements can be simply related as they are for molecules.

> 2. definition of k-mesh (What is the differences between k-mesh and
> k-point?)

The k-mesh is the set of k-points, i.e. the grid of points. See Bloechl et al. 
[Phys. Rev. B 49, 16223-16233 (1994)] for the details.

Fred
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Date: Tue, 24 Sep 2002 09:50:32 -0400 (EDT)
From: Neme Nnolim <non6886@alizarin.njit.edu>
Subject: [WIEN]: Question about slab calculations

====
Neme Nnolim <non6886@alizarin.njit.edu>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- --Boundary_(ID_58wsaM2GAVOeBTRCg3qraA)
Content-type: TEXT/PLAIN; charset=US-ASCII


Dear WIEN users,

I am attempting to carry out calculations on a 5-layer tantalum
slab periodic in the z-direction (please see attached struct file).

For calculation of properties, I understand one needs to find the optimal
length of empty space in the unit cell as well as the optimal interlayer
spacing for the slab.

WIEN offers 'mini' and the c/a and volume optimization combination for
structural optimization purposes. Which optimization feature is best
suited for the optimization of the slab interlayer spacing?

Can the c/a and volume optimization combination be used to optimize the
amount of unit cell vacuum space?

Thanks for looking. Regards,

Neme



- ------------------------------------------------------------------------------
Neme Okechukwu Nnolim
Department of Materials Science, New Jersey Institute of Technology
Room 302, Tiernan Hall, 161 Warren Street, University Heights
Newark, New Jersey 07102-1982
Tel: (973) 596-8283, FAX: (973) 596-5794
- -------------------------------------------------------------------------------



- --Boundary_(ID_58wsaM2GAVOeBTRCg3qraA)
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- --Boundary_(ID_58wsaM2GAVOeBTRCg3qraA)--
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------------------------------

Date: Tue, 24 Sep 2002 15:54:10 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: case.inso

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

No, I do not remember which compiler (or if it was turned on or off as 
default)... sorry. In Fortran90 it should be off as default, since that 
is what the standard says, but for adapted fortran77-compilers I am not 
sure what happens if the file has a .f extension and not .f90. Some of 
them allows for a lot of things in .f files, so it is hard to keep track of.

But I simply deleted "line 6" after looking into the code, so my inso 
file is something like yours (with other details) now. And the function 
is now clear to me...

Best,
Torsten.

Fred Nastos wrote:

>====
>Fred Nastos <nastos@physics.utoronto.ca>
>submitted the following contribution:
>====
>
>On September 24, 2002 07:31 am, Torsten Andersen wrote:
>
>>====
>>Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
>>submitted the following contribution:
>>====
>>
>>So, I took a dive into the code. In SRC_lapwso/init.f I found:
>>
>><snipped code for brevity>
>>
>>I also remember to have seen in some places that for certain
>>"default" options of compilers, do-loops gets run at least
>>once... so there could be a potential problem there...
>>
>
>I have only seen "forcing each do loop to execute at least once" as
>a compiler option that is turned off by default. Do you remember which
>compiler has this turned on.
>
>>So I answered my question first, it seems :-) Any comments?
>>
>
>For no RLOs I use something like the following case.inso (depending on
>details). The older style case.inso (WIEN2k_01) doesn't work sometimes, since
>there is the new option of switching off SO for individual atoms.
>
>WFFIL
> 4  1  0                      llmax,ipr,kpot
> -10.0000   5.00000           emin,emax (output energy window)
>   0.  0.  1.                 direction of magnetization (lattice vectors)
> 0                            number of atoms for which RLO is added
> 0 0 0 0 0                    number of atoms for which SO is switch off;atoms
>
>Cheers,
>
>Fred
>
>>Torsten Andersen wrote:
>>
>>>====
>>>Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
>>>submitted the following contribution:
>>>====
>>>
>>>Hello again,
>>>
>>>the symmetso problem was solved, thanks to Peter Blaha.
>>>
>>>Now a simple question about case.inso, since it has changed from
>>>Wien2k_01 to Wien2k_02.
>>>
>>>If I don't want rlo's, do I have to delete "line 6"? In the old
>>>case.inso it was just ignored, I think. In the new case.inso there is
>>>a "line 7", however. If in "line 5" I have put a zero, what does the
>>>program expect next, a single line 6 or no line 6, but line 7 in stead?
>>>
>>>Yes, I guess it could be read by sifting through the code, but I think
>>>it should be clear in the manual...
>>>
>>>Best regards,
>>>Torsten.
>>>
>
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>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
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Date: Tue, 24 Sep 2002 16:18:04 +0200
From: "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: Question about slab calculations

====
"Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> I am attempting to carry out calculations on a 5-layer tantalum
> slab periodic in the z-direction (please see attached struct file).
>
> For calculation of properties, I understand one needs to find the optimal
> length of empty space in the unit cell as well as the optimal interlayer
> spacing for the slab.
>
> WIEN offers 'mini' and the c/a and volume optimization combination for
> structural optimization purposes. Which optimization feature is best
> suited for the optimization of the slab interlayer spacing?
>
> Can the c/a and volume optimization combination be used to optimize the
> amount of unit cell vacuum space?

No, you're slightly on the wrong track here. A possible strategy could be :

1) Take a slab with atoms on the bulk positions, and (after having
determined good Rkm and k-mesh) gradually increase the vacuum region. When
you see that e.g. surface properties or the potential in the middle of the
vacuum (directly printed in case.scf) do no change any more, then you have
reached a good vacuum thickness. Keeping this vacuum constant, now repeat
the procedure for the number of layers in the slab. Make it as thick as
needed in order to avoid crosstalk between the two surfaces in your slab
(again a good check would be whether moments, forces, efg's, hyperfine
fields,... at the surface do not change when adding additional layers).

2) With this knowledge, use mini to find the optimized positions.

You cannot use c/a optimization, as together with the vacuum thickness also
the atomic positions would change (fractional coordinates, remember)

Stefaan

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Date: Tue, 24 Sep 2002 14:20:36 -0400 (EDT)
From: Neme Nnolim <non6886@alizarin.njit.edu>
Subject: Re: [WIEN]: Question about slab calculations

====
Neme Nnolim <non6886@alizarin.njit.edu>
submitted the following contribution:
====


Thanks Stefaan. I will probably have more questions as I try your
suggestions.

Regards,

Neme

- ------------------------------------------------------------------------------
Neme Okechukwu Nnolim
Department of Materials Science, New Jersey Institute of Technology
Room 302, Tiernan Hall, 161 Warren Street, University Heights
Newark, New Jersey 07102-1982
Tel: (973) 596-8283, FAX: (973) 596-5794
- -------------------------------------------------------------------------------


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Date: Wed, 25 Sep 2002 11:51:34 +1000
From: chen0130@flinders.edu.au
Subject: Re: [WIEN]: occupied bands

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Thanks Peter, Torsten, Christian for you help! It is greatly appreciated!

I am using Wien97.10, and when I look into the case.output2 file,
I am told the number of electrons, and then half that number is the number of
occupied bands (2 electrons to a band)...

Is it the same case.output2 as Wien2k, as Peter was referring?

None-the-less, I am in a better position now!

Cheng


Quoting Peter Blaha <pblaha@theochem.tuwien.ac.at>:

> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> > Can anyone tell me if there is a way in Wien to find out which bands are
> > occupied (eg by the bandindex number)?
> >
> > As there are many bands that emerge from a bandstruct calc for slabs...
> >
> > Maybe a density of states calc would be helpful?
> >
> > Thanks for your time!
> 
> Have a look into case.output2 (up/dn). At the top you find e-fermi, but
> also the emin/emax of each band (ordered by bandindex), so that you
> easily can judge how many bands are fully occupied and how many bands
> cross EF.
> 
> (The same info is also given in case.outputt (after tetra).
> 
> Of course in a metallic situation you then must plot a bandstructure to
> get more insight.
> 
> Regards
> 
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
> http://info.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
> 
> ====
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> ====
> 
> 



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------------------------------

Date: Wed, 25 Sep 2002 12:47:46 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: Re: [WIEN]:

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Hi,

I got some problems while calculating JOINT(joint density of state). My 
problem is that WIEN always have the following error messages in file 
(.outputjoint). 
- ------
parameter INUME set too small!
check paramter and band indices in *.injoint
- ------
Then, I check back the file "param.inc" in directory "SRC_joint". And 
the file is ias below:
- ------
Cb     
C     .........PARAMETER INCLUDE FILE.............
C     
      PARAMETER(NKPT=2000)
      PARAMETER          (NUME=   300)
C     
      PARAMETER(INUME=5000)
      PARAMETER(INUMEDEN=50)
      PARAMETER(MET=10000)
      PARAMETER(MG=9)
      PARAMETER(NSW=9) 
C..new struct + latgen 
      PARAMETER          (NATO=   10)
      PARAMETER          (NDIF=   24)
      PARAMETER(NSYM= 48)                                              
C     NATO        MAX NUMBER OF INEQ: ATOMS
C
C     NDIF        MAX NUMBER OF ATOMPOSITION IN CELL
C
C     NSYM        MAX NUMBER OF SYM-OPERATION
C
C     NUME        MAX NUMBER OF EIGENVALUES PER K - POINT 
C
C     INUME       MAX NUMBER OF BANDCOMBINATIONS nume*(nume+1)/2 
C
C     INUMEden    MAX NUMBER OF BANDCOMBINATIONS for band analysis     
C
C     MET         MAXIMUM FOR ENERGYMESH
C
C     MG          MAXIMUM NUMBER OF SPECTRA 
c                (polarizations: see input case.inop) 
C
C     NSW         NUMBER OF SWITCHCODES   fixed!
C
C....special: not used in standart application
      PARAMETER   (NEKPT=5)   
      PARAMETER   (NUMTETR= 6)
C     NEKPT       NUMBER OF NOT EQUIVALENT K_POINTS   fixed!
C
C     NUMTETR     NUMBER OF TETRAEDERS        fixed! 
- ------

Then, I tried to change "INUME" from 5000 to 45150{300*(300+1)/2}, 10000, 8000. 
However, I can't compile it. And then, I tried 6000 and it could be 
compiled  but the same error message appears when I run the program. Why? 
What value should I use?

Thank you very much

Martin

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Date: Wed, 25 Sep 2002 08:40:31 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: occupied bands

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I am using Wien97.10, and when I look into the case.output2 file,
> I am told the number of electrons, and then half that number is the number of
> occupied bands (2 electrons to a band)...
>
> Is it the same case.output2 as Wien2k, as Peter was referring?

Sorry, what I described is only in case.output2 of WIEN2k.

You find the same info in case.outputt.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 25 Sep 2002 08:45:56 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]:

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

INUME was very difficult to set in WIEN97 and made the program
easily very big (even several GB).

Try to set INUME using the actual number of bands in your case
(check the output of optic) and not simply the value of parameter NUME.

WIEN2k should be easier to use!


> I got some problems while calculating JOINT(joint density of state). My
> problem is that WIEN always have the following error messages in file
> (.outputjoint).
> ------
> parameter INUME set too small!
> check paramter and band indices in *.injoint
> C
> Then, I tried to change "INUME" from 5000 to 45150{300*(300+1)/2}, 10000, 8000.
> However, I can't compile it. And then, I tried 6000 and it could be
> compiled  but the same error message appears when I run the program. Why?
> What value should I use?


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 25 Sep 2002 18:03:11 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: Re: [WIEN]:

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Hi, 

Can anyone tell me what exactly the input file ".injoint" for JDOS calculation is? 
The reason is that I got nearly all elements in the files ".Im_eps_zz_*" equal 0.

The input file (.injoint) being used is as below:
- ------
   36  44                    : LOWER AND UPPER BANDINDEX
  -5.0000    0.00010   2.2000 : EMIN DE EMAX FOR ENERGYGRID IN ryd
eV                            : output units  eV / ryd  / cm-1
     5                        : SWITCH
     1                        : NUMBER OF COLUMNS
   0.1  0.1  0.3              : BROADENING (FOR DRUDE MODEL - switch 6,7 -
ONLY)

SWITCH:

   0...JOINTDOS FOR EACH BAND COMBINATION
   1...JOINTDOS AS SUM OVER ALL BAND COMBINATIONS
   2...DOS FOR EACH BAND
   3...DOS AS SUM OVER ALL BANDS
   4...Im(EPSILON)
   5...Im(EPSILON) for each band combination
   6...INTRABAND contributions
   7...INTRABAND contributions including band analysis
- ------
Is there anything wrong for my input file?

Thank you very much

Martin

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------------------------------

Date: Thu, 26 Sep 2002 16:01:30 +1000
From: chen0130@flinders.edu.au
Subject: [WIEN]: density of states for occupied states

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Dear Wien users,

I was wondering if there is a possible way to calculate the DOS for occupied
states?

Thanks for you time!

Cheng


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------------------------------

End of wien-digest V2002 #36
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #37
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
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wien-digest        Thursday, October 3 2002        Volume 2002 : Number 037




----------------------------------------------------------------------

Date: Thu, 26 Sep 2002 16:07:13 +1000
From: chen0130@flinders.edu.au
Subject: [WIEN]: DOS for occupied bands...

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Sorry,

I do believe states below the fermi energy are occupied by definition?

Cheng

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------------------------------

Date: Thu, 26 Sep 2002 08:21:23 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: DOS for occupied bands...

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Yeah, you are right... so you get it simply by cutting your DOS figure 
at the Fermi energy :-)

Have fun,
Torsten.

chen0130@flinders.edu.au wrote:

>====
>chen0130@flinders.edu.au
>submitted the following contribution:
>====
>
>Sorry,
>
>I do believe states below the fermi energy are occupied by definition?
>
>Cheng
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Thu, 26 Sep 2002 08:34:35 +0200
From: Claudia Ambrosch-Draxl <claudia.ambrosch@uni-graz.at>
Subject: Re: [WIEN]:

====
Claudia Ambrosch-Draxl <claudia.ambrosch@uni-graz.at>
submitted the following contribution:
====

Ma Chi Chiu wrote:
> 
> ====
> Ma Chi Chiu <martin@yangtze.hku.hk>
> submitted the following contribution:
> ====
> 
> Hi,
> 
> Can anyone tell me what exactly the input file ".injoint" for JDOS calculation is?
> The reason is that I got nearly all elements in the files ".Im_eps_zz_*" equal 0.
> 
> The input file (.injoint) being used is as below:
> ------
>    36  44                    : LOWER AND UPPER BANDINDEX
>   -5.0000    0.00010   2.2000 : EMIN DE EMAX FOR ENERGYGRID IN ryd
> eV                            : output units  eV / ryd  / cm-1
>      5                        : SWITCH
>      1                        : NUMBER OF COLUMNS
>    0.1  0.1  0.3              : BROADENING (FOR DRUDE MODEL - switch 6,7 -
> ONLY)

You are searching for transitions between band 36 and 44 only! Make sure
that you include transitions from occupied bands to empty states.

Regards,
Claudia Ambrosch-Draxl

Institut f. Theoretische Physik, University Graz
Universitaetsplatz 5, A-8010 Graz
Tel. [43] (316) 380-5235    Fax [43] (316) 380-9820
http://physik.uni-graz.at/~cad
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------------------------------

Date: Thu, 26 Sep 2002 08:57:30 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]:

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

If I may add to that... in general you should include at least all the 
bands within the energy window in order to get something representative 
for your system. Limiting the number of bands (I believe) can be used to 
study the transitions in greater detail (e.g., to find out whether the 
response from transitions between two specific bands is dominating all 
other responses), as well as giving you faster results.

Best regards,
Torsten.

Claudia Ambrosch-Draxl wrote:

>====
>Claudia Ambrosch-Draxl <claudia.ambrosch@uni-graz.at>
>submitted the following contribution:
>====
>
>Ma Chi Chiu wrote:
>
>>====
>>Ma Chi Chiu <martin@yangtze.hku.hk>
>>submitted the following contribution:
>>====
>>
>>Hi,
>>
>>Can anyone tell me what exactly the input file ".injoint" for JDOS calculation is?
>>The reason is that I got nearly all elements in the files ".Im_eps_zz_*" equal 0.
>>
>>The input file (.injoint) being used is as below:
>>------
>>   36  44                    : LOWER AND UPPER BANDINDEX
>>  -5.0000    0.00010   2.2000 : EMIN DE EMAX FOR ENERGYGRID IN ryd
>>eV                            : output units  eV / ryd  / cm-1
>>     5                        : SWITCH
>>     1                        : NUMBER OF COLUMNS
>>   0.1  0.1  0.3              : BROADENING (FOR DRUDE MODEL - switch 6,7 -
>>ONLY)
>>
>
>You are searching for transitions between band 36 and 44 only! Make sure
>that you include transitions from occupied bands to empty states.
>
>Regards,
>Claudia Ambrosch-Draxl
>
>Institut f. Theoretische Physik, University Graz
>Universitaetsplatz 5, A-8010 Graz
>Tel. [43] (316) 380-5235    Fax [43] (316) 380-9820
>http://physik.uni-graz.at/~cad
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Thu, 26 Sep 2002 16:57:40 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: Re: [WIEN]:

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

I am wondering whether I should calculate the optical properties 
before or after bandstructre calculation? 
It is beacuse I have tried to calculate the optical properties two time.
The first trial is calulating the optical properties directly after SCF 
calculation and the second trial is calculating the optical properties after 
density of states and bandstructure calculations. Then, I found the 
content in the file .outputjoint are different and certainly the plot for 
joint DOS are different, too.

Thank you very much

Martin

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------------------------------

Date: Thu, 26 Sep 2002 11:48:56 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]:

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

After the scf cycle, if you calculate band structures you have changed 
your case.vector file, and you will need to execute lapw1 with the 
original k-mesh (not the band structure mesh) in order to get a good 
optics result. Then the result should also be the same as if you 
calculate the optics first and the bandstructure afterwards.

Best regards,
Torsten.

Ma Chi Chiu wrote:

>====
>Ma Chi Chiu <martin@yangtze.hku.hk>
>submitted the following contribution:
>====
>
>Dear all,
>
>I am wondering whether I should calculate the optical properties 
>before or after bandstructre calculation? 
>It is beacuse I have tried to calculate the optical properties two time.
>The first trial is calulating the optical properties directly after SCF 
>calculation and the second trial is calculating the optical properties after 
>density of states and bandstructure calculations. Then, I found the 
>content in the file .outputjoint are different and certainly the plot for 
>joint DOS are different, too.
>
>Thank you very much
>
>Martin
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
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------------------------------

Date: Thu, 26 Sep 2002 18:39:26 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: Re: [WIEN]:

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Hi,

I would like to consult about the definition od physical meaning of 
several terms in the file ".inop".

Below is file ".inop" 
- ------ 
1200 1        number of k-points, first k-point
- -5.0 2.2      Emin, Emax for matrix elements
9             number of choices (columns in *outmat)
1             Re xx
2             Re yy
3             Re zz
4             Re xy
5             Re xz
6             Re yz
7             Im xy
8             Im xz
9             Im yz


Choices:
1......Re <x><x>
2......Re <y><y>
3......Re <z><z>
4......Re <x><y>
5......Re <x><z>
6......Re <y><z>
7......Im <x><y>
8......Im <x><z>
9......Im <y><z>
- ------

The terms that I am not really understand are :
1. Emin for matrix elements
2. Emax for matrix elements

How will this two terms affect the JDOS plot?

Also, for the file ".injoint"
- ------
   30   50                    : LOWER AND UPPER BANDINDEX
   0.0000    0.00010   1.0000 : EMIN DE EMAX FOR ENERGYGRID IN ryd
eV                            : output units  eV / ryd  / cm-1
     5                        : SWITCH
     9                        : NUMBER OF COLUMNS
   0.1  0.1  0.3              : BROADENING (FOR DRUDE MODEL - switch 6,7 -
ONLY)

SWITCH:

   0...JOINTDOS FOR EACH BAND COMBINATION
   1...JOINTDOS AS SUM OVER ALL BAND COMBINATIONS
   2...DOS FOR EACH BAND
   3...DOS AS SUM OVER ALL BANDS
   4...Im(EPSILON)
   5...Im(EPSILON) for each band combination
   6...INTRABAND contributions
   7...INTRABAND contributions including band analysis
- ------

How will the below terms affect the JDOS plot? Do they just govern the x-axis of the plot?

Terms : "EMIN" "DE" "EMAX" 


Thank you very much

Martin


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------------------------------

Date: Thu, 26 Sep 2002 13:34:48 +0200
From: Claudia Ambrosch-Draxl <claudia.ambrosch@uni-graz.at>
Subject: Re: [WIEN]:

====
Claudia Ambrosch-Draxl <claudia.ambrosch@uni-graz.at>
submitted the following contribution:
====

Ma Chi Chiu wrote:
> 
> ====
> Ma Chi Chiu <martin@yangtze.hku.hk>
> submitted the following contribution:
> ====
> 
> Dear all,
> 
> I am wondering whether I should calculate the optical properties
> before or after bandstructre calculation?
> It is beacuse I have tried to calculate the optical properties two time.
> The first trial is calulating the optical properties directly after SCF
> calculation and the second trial is calculating the optical properties after
> density of states and bandstructure calculations. Then, I found the
> content in the file .outputjoint are different and certainly the plot for
> joint DOS are different, too.
> 

The different results may have to do wih the fact that you did not use a
dense enough k-point mesh for the optical properties. It seems that you
have used two different meshes for the SCF cycle and the DOS,
repsectively, and that you have used these meshes for the optical
spectra. Right?
Anyway, you should use a much denser grid for calculating the optical
spectra than for the SCF cycle. Such a grid can only be a starting point
for checking the k-point convergence with respect to the optical spectra
and usually does not give reliable results.
A band structure mesh is not uniform and cannot not work at all since in
joint we use the tetrahedron method for the BZ integrations which
requires the case.klist + case.kgen files.

Best regards,
Claudia Ambrosch-Draxl

Institut f. Theoretische Physik, University Graz
Universitaetsplatz 5, A-8010 Graz
Tel. [43] (316) 380-5235    Fax [43] (316) 380-9820
http://physik.uni-graz.at/~cad
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------------------------------

Date: Fri, 27 Sep 2002 00:05:37 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]:Optical properties

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

Firstly, thank for the explaination from Claudia Ambrosch-Draxl and 
Torsten Andersen. However, I don't know how to have a denser k-mesh point. 
Actually, I inputed 20 for the number of k-point during SCF but WIEN 
automatically change it to 4 and the bandstructure looks okay. Is it I 
need to run kgen again with a large value of k-point for optical 
properties' calculation?

Thank you very much

Martin

On Thu, 26 Sep 2002, Claudia Ambrosch-Draxl wrote:

> ====
> Claudia Ambrosch-Draxl <claudia.ambrosch@uni-graz.at>
> submitted the following contribution:
> ====
> 
> Ma Chi Chiu wrote:
> > 
> > ====
> > Ma Chi Chiu <martin@yangtze.hku.hk>
> > submitted the following contribution:
> > ====
> > 
> > Dear all,
> > 
> > I am wondering whether I should calculate the optical properties
> > before or after bandstructre calculation?
> > It is beacuse I have tried to calculate the optical properties two time.
> > The first trial is calulating the optical properties directly after SCF
> > calculation and the second trial is calculating the optical properties after
> > density of states and bandstructure calculations. Then, I found the
> > content in the file .outputjoint are different and certainly the plot for
> > joint DOS are different, too.
> > 
> 
> The different results may have to do wih the fact that you did not use a
> dense enough k-point mesh for the optical properties. It seems that you
> have used two different meshes for the SCF cycle and the DOS,
> repsectively, and that you have used these meshes for the optical
> spectra. Right?
> Anyway, you should use a much denser grid for calculating the optical
> spectra than for the SCF cycle. Such a grid can only be a starting point
> for checking the k-point convergence with respect to the optical spectra
> and usually does not give reliable results.
> A band structure mesh is not uniform and cannot not work at all since in
> joint we use the tetrahedron method for the BZ integrations which
> requires the case.klist + case.kgen files.
> 
> Best regards,
> Claudia Ambrosch-Draxl
> 
> Institut f. Theoretische Physik, University Graz
> Universitaetsplatz 5, A-8010 Graz
> Tel. [43] (316) 380-5235    Fax [43] (316) 380-9820
> http://physik.uni-graz.at/~cad
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 

- -- 
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
~~ "Here is your country, do not let anyone take its glory away  ~~
~~  from you. Do not let selfish men or greedy interests skin    ~~ 
~~  your country of its beauty, its riches, or its romance. The  ~~
~~  world and the future and your very children shall judge you  ~~
~~  according to the way you deal with this sacred trust."       ~~
~~                                                               ~~
~~                                                               ~~
~~               -- Theodore Roosevelt, Antiquities Act of 1906  ~~
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

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------------------------------

Date: Thu, 26 Sep 2002 18:14:24 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]:Optical properties

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

You need "a fair amount" of k-points, and then to run at least lapw1 
again to create the corresponding output files. As the number cannot be 
given as a general rule, you can start with a few hundred, and increase 
the number until you reach convergence in the optical spectrum, but 
expect to use thousands of k-points for that.

Best regards,
Torsten Andersen.

Ma Chi Chiu wrote:

>====
>Ma Chi Chiu <martin@yangtze.hku.hk>
>submitted the following contribution:
>====
>
>Dear all,
>
>Firstly, thank for the explaination from Claudia Ambrosch-Draxl and 
>Torsten Andersen. However, I don't know how to have a denser k-mesh point. 
>Actually, I inputed 20 for the number of k-point during SCF but WIEN 
>automatically change it to 4 and the bandstructure looks okay. Is it I 
>need to run kgen again with a large value of k-point for optical 
>properties' calculation?
>
>Thank you very much
>
>Martin
>
>On Thu, 26 Sep 2002, Claudia Ambrosch-Draxl wrote:
>
<previous comments snipped>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
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------------------------------

Date: Fri, 27 Sep 2002 12:10:22 +1000
From: chen0130@flinders.edu.au
Subject: [WIEN]: DOS matching bandstructures...

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Dear wien users,

I am studying a simple case of solid Li2O. 

My bandstructure reveals bands at 0 to -5 eV (O 2p), -15 eV and -45 eV...

then I changed the k mesh back to the original, run a single SCF cycle, to
ensure lapw1 is done,

and do the DOS... but it only has peaks at around -5 eV (ignoring above E_fermi)

i also tried setting a fresh case and doing the DOS only after the SCF...

i am puzzled, I really expect peaks in the DOS to correspond to the bands at
those energies...

can someone tell me possible errors, hints from their experiences?

thanks for you time!

Cheng

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------------------------------

Date: Fri, 27 Sep 2002 08:10:07 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: DOS matching bandstructures...

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

So you are calculating DOS and band structure from two different 
k-meshes. I am not so surprised you get different results. Of course, 
ideally, if your band structure is representative, you should see at 
least a fingerprint of it in the DOS. Have you tried to calculate the 
DOS with the results from the band structure, just to check how it looks 
compared to what you expect? If that looks like you think it should from 
the band structure, you could try other paths through the Brillouin Zone 
(BZ) for the band structure and see if that is a better representative. 
Remember that the band structure is only along specific paths in the BZ 
and are not by nature representative for the DOS.

Another thing you could do to see the fingerprint of the "missing" 
feature, is to zoom on the scale in the DOS. In gnuplot you can do that 
by "set yrange [0:0.1]" or similar.

Okay, it may be too general a comment... so if somebody has specific 
experiences...

Best regards,
Torsten Andersen.

chen0130@flinders.edu.au wrote:

>====
>chen0130@flinders.edu.au
>submitted the following contribution:
>====
>
>Dear wien users,
>
>I am studying a simple case of solid Li2O. 
>
>My bandstructure reveals bands at 0 to -5 eV (O 2p), -15 eV and -45 eV...
>
>then I changed the k mesh back to the original, run a single SCF cycle, to
>ensure lapw1 is done,
>
>and do the DOS... but it only has peaks at around -5 eV (ignoring above E_fermi)
>
>i also tried setting a fresh case and doing the DOS only after the SCF...
>
>i am puzzled, I really expect peaks in the DOS to correspond to the bands at
>those energies...
>
>can someone tell me possible errors, hints from their experiences?
>
>thanks for you time!
>
>Cheng
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
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------------------------------

Date: Fri, 27 Sep 2002 09:38:17 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: DOS matching bandstructures...

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0015_01C26609.9BF15B20
Content-Type: text/plain;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

> I am studying a simple case of solid Li2O.=20
>=20
> My bandstructure reveals bands at 0 to -5 eV (O 2p), -15 eV and -45 =
eV...
=20
> then I changed the k mesh back to the original, run a single SCF =
cycle, to
> ensure lapw1 is done,



That is okay, but when you want to calculate DOS after the =
bandstructure, you only need to run lapw1 with the original case.in1 =
file to make sure about proper case.vector(s).


> and do the DOS... but it only has peaks at around -5 eV (ignoring =
above E_fermi)
>=20
> i also tried setting a fresh case and doing the DOS only after the =
SCF...

=20

That is okay (making strongly sure), but time consuming.

> i am puzzled, I really expect peaks in the DOS to correspond to the =
bands at
> those energies...
=20

You are right, there should be such a correspondence between DOS and =
band character plotting.

=20

> can someone tell me possible errors, hints from their experiences?

=20

If you would see DOS's from -45eV, change Emin of case.int file to =
- -45/13.6~-3.4Ry, and then run tetra.

=20

Your,

S. Jalali.


- ------=_NextPart_000_0015_01C26609.9BF15B20
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY>
<DIV><FONT face=3DArial size=3D2>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">&gt; I am studying a =
simple case of=20
solid Li2O. <BR>&gt; <BR>&gt; My bandstructure reveals bands at 0 to -5 =
eV (O=20
2p), -15 eV and -45 eV...<BR>&nbsp;<BR>&gt; then I changed the k mesh =
back to=20
the original, run a single SCF cycle, to<BR>&gt; ensure lapw1 is=20
done,</SPAN><?xml:namespace prefix =3D o ns =3D=20
"urn:schemas-microsoft-com:office:office" /><o:p></o:p></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial"></SPAN>&nbsp;</P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">That is okay, but when you =
want to=20
calculate DOS after&nbsp;the bandstructure, =
you&nbsp;only&nbsp;need&nbsp;to run=20
lapw1 with the original case.in1 file to make sure about proper=20
case.vector(s).</SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial"><BR>&gt; and do the DOS... =
but it=20
only has peaks at around -5 eV (ignoring above E_fermi)<BR>&gt; <BR>&gt; =
i also=20
tried setting a fresh case and doing the DOS only after the=20
SCF...</SPAN><o:p></o:p></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><FONT size=3D3><FONT=20
face=3D"Times New Roman">&nbsp;<o:p></o:p></FONT></FONT></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">That is okay (making =
strongly sure),=20
but time consuming.<BR><BR>&gt; i am puzzled, I really expect peaks in =
the DOS=20
to correspond to the bands at<BR>&gt; those=20
energies...<BR>&nbsp;</SPAN><o:p></o:p></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">You are right, there =
should be such=20
a correspondence between DOS and band character =
plotting.</SPAN><o:p></o:p></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><FONT size=3D3><FONT=20
face=3D"Times New Roman">&nbsp;<o:p></o:p></FONT></FONT></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">&gt; can someone tell me =
possible=20
errors, hints from their experiences?</SPAN><o:p></o:p></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><FONT size=3D3><FONT=20
face=3D"Times New Roman">&nbsp;<o:p></o:p></FONT></FONT></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">If you would see =
DOS's&nbsp;from=20
- -45eV, change Emin of case.int file to -45/13.6~-3.4Ry, and then run=20
tetra.</SPAN><o:p></o:p></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><FONT size=3D3><FONT=20
face=3D"Times New Roman">&nbsp;</FONT></FONT></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt">Your,</P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt">S.=20
Jalali.</P></FONT></DIV></BODY></HTML>

- ------=_NextPart_000_0015_01C26609.9BF15B20--

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------------------------------

Date: Fri, 27 Sep 2002 09:56:30 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: [WIEN]: Questions about "mini" vs. "optimize"

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear All,

since I am a newbie to "mini", I am afraid I have to ask a few 
questions, although there is a FAQ on the subject. I am aware that 
"mini" uses a scheme to create a new struct file where some internal 
parameters have been optimized according to "case.inM". My question is 
then:

If I have only one parameter I want to optimize, is there any speed 
advantage in using "mini" compared to doing a "optimize"-like scheme 
where one changes that internal parameter in the struct file, run it 
again with force convergence, and so on... in that case I would be able 
to make a number of changes to the struct file and run each of the 
struct files through run_lapw in parallel, and I would assume that I get 
data in the scf-file for the forces that I then could plot as a function 
of the change of the internal parameter.

If "mini" is really running a "run_lapw" for each change of the internal 
parameter I am afraid I will get very old before it finishes, if I have 
to run it in serial.

Am I missing something?

Best regards,
Torsten Andersen.

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
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------------------------------

Date: Fri, 27 Sep 2002 14:00:11 +0200
From: "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: Questions about "mini" vs. "optimize"

====
"Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> If I have only one parameter I want to optimize, is there any speed
> advantage in using "mini" compared to doing a "optimize"-like scheme
> where one changes that internal parameter in the struct file, run it
> again with force convergence, and so on... in that case I would be able
> to make a number of changes to the struct file and run each of the
> struct files through run_lapw in parallel, and I would assume that I get
> data in the scf-file for the forces that I then could plot as a function
> of the change of the internal parameter.

Yes, this is usually more efficient than mini, as you can learn from the
first results and quickly go to the minimum.

> If "mini" is really running a "run_lapw" for each change of the internal
> parameter I am afraid I will get very old before it finishes, if I have
> to run it in serial.

Unfortunately, you are right. According to my experience, this is the real
bottleneck now in first principles calculations. If your property is
sensitive to the correct internal coordinates (impurities, surfaces, phase
boundaries,...) then you are spending 95% of your cpu time to obtaining the
correct internal coordinates. And only then you can start to do physics.
Maybe this is an occasion to put a more general question to the mailing
list: what are all of you doing to cope with this problem? Do you have
experience with codes that can in an efficient way relax complicated
structures? They need not to be that accurate as LAPW, in many cases it
would be very helpful to have a rough but quick estimate before one starts
mini.

Best regards,
Stefaan

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Date: Fri, 27 Sep 2002 14:21:13 -0200 (DFT)
From: Frederic Lemoigno <lemoigno@lsd.univ-montp2.fr>
Subject: Re: [WIEN]: Questions about "mini" vs. "optimize"

====
Frederic Lemoigno <lemoigno@lsd.univ-montp2.fr>
submitted the following contribution:
====

Hi Stefaan,
	If you're looking for a quick, low memory ab initio code for
relaxing (3D) structures, have a try with SIESTA:
http://www.uam.es/departamentos/ciencias/fismateriac/siesta/ 
The first version is freely available.

Yours
F. Lemoigno

> 
> ====
> "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
> submitted the following contribution:
> ====
> 
.
.
.
> 
> Unfortunately, you are right. According to my experience, this is the real
> bottleneck now in first principles calculations. If your property is
> sensitive to the correct internal coordinates (impurities, surfaces, phase
> boundaries,...) then you are spending 95% of your cpu time to obtaining the
> correct internal coordinates. And only then you can start to do physics.
> Maybe this is an occasion to put a more general question to the mailing
> list: what are all of you doing to cope with this problem? Do you have
> experience with codes that can in an efficient way relax complicated
> structures? They need not to be that accurate as LAPW, in many cases it
> would be very helpful to have a rough but quick estimate before one starts
> mini.
> 
> Best regards,
> Stefaan
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 

====
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------------------------------

Date: Fri, 27 Sep 2002 15:06:03 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Questions about "mini" vs. "optimize"

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Hi Stefaan,

thank you for the very informative answer!

there is possibly the "other Wien-code" VASP, but that is provided that 
good pseudopotentials exist...which is not the case for all the 
structures we like to consider.

Best regards,
Torsten.

Stefaan Cottenier wrote:

>====
>"Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
>submitted the following contribution:
>====
>
>>If I have only one parameter I want to optimize, is there any speed
>>advantage in using "mini" compared to doing a "optimize"-like scheme
>>where one changes that internal parameter in the struct file, run it
>>again with force convergence, and so on... in that case I would be able
>>to make a number of changes to the struct file and run each of the
>>struct files through run_lapw in parallel, and I would assume that I get
>>data in the scf-file for the forces that I then could plot as a function
>>of the change of the internal parameter.
>>
>
>Yes, this is usually more efficient than mini, as you can learn from the
>first results and quickly go to the minimum.
>
>>If "mini" is really running a "run_lapw" for each change of the internal
>>parameter I am afraid I will get very old before it finishes, if I have
>>to run it in serial.
>>
>
>Unfortunately, you are right. According to my experience, this is the real
>bottleneck now in first principles calculations. If your property is
>sensitive to the correct internal coordinates (impurities, surfaces, phase
>boundaries,...) then you are spending 95% of your cpu time to obtaining the
>correct internal coordinates. And only then you can start to do physics.
>Maybe this is an occasion to put a more general question to the mailing
>list: what are all of you doing to cope with this problem? Do you have
>experience with codes that can in an efficient way relax complicated
>structures? They need not to be that accurate as LAPW, in many cases it
>would be very helpful to have a rough but quick estimate before one starts
>mini.
>
>Best regards,
>Stefaan
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



====
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------------------------------

Date: Fri, 27 Sep 2002 22:16:28 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]:

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

I would like to consult about the bandstructure calculation. My question 
is as below:

In chapter three of User's Guide, it tells us to append the appropriate 
template to the .in1 file and change the entry "K-point from unit" 4 to 5. 
In the sample "TiC", it is asked to use $WIENROOT/SRC_templates/fcc.klist. 

And now, I am using a simple cubic lattice and is it I can just append 
$WIENROOT/SRC_templates/simple_cubic.klist to .in1 file? And what is the 
relationship between the simple_cubic.klist and my own .klist file?

Thank you very much

Martin 

- -- 
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
~~ "Here is your country, do not let anyone take its glory away  ~~
~~  from you. Do not let selfish men or greedy interests skin    ~~ 
~~  your country of its beauty, its riches, or its romance. The  ~~
~~  world and the future and your very children shall judge you  ~~
~~  according to the way you deal with this sacred trust."       ~~
~~                                                               ~~
~~                                                               ~~
~~               -- Theodore Roosevelt, Antiquities Act of 1906  ~~
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

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------------------------------

Date: Fri, 27 Sep 2002 17:23:05 +0200
From: "koitzsch" <Christian.Koitzsch@unifr.ch>
Subject: [WIEN]: Re: ma chi chiu

====
"koitzsch" <Christian.Koitzsch@unifr.ch>
submitted the following contribution:
====

Hi,

Oh, it just depends, what directions you are interested in. These sample
klists are just paths in k-space into some conventional Brillouin zone
directions. In principal you can give any k-point and evaluate the
eigenvalues at that specific k-point. If you are e.g. interested in the
dispersion along one specific direction you can either hope that this
direction is included in the sample klists provided, or you can make just
any path in k-space by using XCrysDen.
XcrysDen produces number triples, which yield if multiplied by conventional
reciprocal lattice vectors, the appropriate k-point. (you can even calculate
this by hand and include a conventional spreadsheet text file)
Maybe to give you a physical example: if you calculate graphite and you are
interested in the dispersion perpendicular to the graphite sheats, you
generate a k-list along the hexagonal c-axis (reciprocal space) starting
from Gamma (0,0,0) to the Brillouin zone boundary (0,0,1) and you make sth.
like 200 points in between.

The difference to case.klist is that the k-list for band structure
calculations is along high symmetry directions, while the case.klist for an
scf cycle sort-of samples the irreducible Brillouin zone homogenously. In
simple words: there is nothing you can learn out of the change in
eigenvalues if you go from one point in this case.klist to the next point..

Hope, this helps a little bit


Christian Koitzsch

- ----- Original Message -----
From: "Ma Chi Chiu" <martin@yangtze.hku.hk>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Friday, September 27, 2002 4:16 PM
Subject: [WIEN]:


> ====
> Ma Chi Chiu <martin@yangtze.hku.hk>
> submitted the following contribution:
> ====
>
> Dear all,
>
> I would like to consult about the bandstructure calculation. My question
> is as below:
>
> In chapter three of User's Guide, it tells us to append the appropriate
> template to the .in1 file and change the entry "K-point from unit" 4 to 5.
> In the sample "TiC", it is asked to use $WIENROOT/SRC_templates/fcc.klist.
>
> And now, I am using a simple cubic lattice and is it I can just append
> $WIENROOT/SRC_templates/simple_cubic.klist to .in1 file? And what is the
> relationship between the simple_cubic.klist and my own .klist file?
>
> Thank you very much
>
> Martin
>
> --
> ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
> ~~ "Here is your country, do not let anyone take its glory away  ~~
> ~~  from you. Do not let selfish men or greedy interests skin    ~~
> ~~  your country of its beauty, its riches, or its romance. The  ~~
> ~~  world and the future and your very children shall judge you  ~~
> ~~  according to the way you deal with this sacred trust."       ~~
> ~~                                                               ~~
> ~~                                                               ~~
> ~~               -- Theodore Roosevelt, Antiquities Act of 1906  ~~
> ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>


====
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------------------------------

Date: Fri, 27 Sep 2002 17:22:27 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Questions about "mini" vs. "optimize"

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> > If I have only one parameter I want to optimize, is there any speed
> > advantage in using "mini" compared to doing a "optimize"-like scheme
> > where one changes that internal parameter in the struct file, run it
> > again with force convergence, and so on... in that case I would be able
> > to make a number of changes to the struct file and run each of the
> > struct files through run_lapw in parallel, and I would assume that I get
> > data in the scf-file for the forces that I then could plot as a function
> > of the change of the internal parameter.
>
> Yes, this is usually more efficient than mini, as you can learn from the
> first results and quickly go to the minimum.

If you have just one parameter AND it follows a linear relationship for
the force/position  (or, equivalently, follows a parabolic energy vs. pos
behaviour), then this is such a trivial case that you most likely are better
off doing it by hand. (You can do 2 geometries sequential and calculate
from this the F=0 geometry). Alternatively the BROYD scheme in case.inM
should also be very effective, while NEWT may converge slowly with unfortunate
parameters.

If your potential energy is anharmonic,.....  bad luck.


> > If "mini" is really running a "run_lapw" for each change of the internal
> > parameter I am afraid I will get very old before it finishes, if I have
> > to run it in serial.

Well, the idea would be to use the k-point parallelism, not doing the
structures in parallel, but see above...

Or maybe you do Project 1 on computer one and project 2 on computer 2,...

> Unfortunately, you are right. According to my experience, this is the real
> bottleneck now in first principles calculations. If your property is
> sensitive to the correct internal coordinates (impurities, surfaces, phase
> boundaries,...) then you are spending 95% of your cpu time to obtaining the
> correct internal coordinates. And only then you can start to do physics.
> Maybe this is an occasion to put a more general question to the mailing
> list: what are all of you doing to cope with this problem? Do you have
> experience with codes that can in an efficient way relax complicated
> structures? They need not to be that accurate as LAPW, in many cases it
> would be very helpful to have a rough but quick estimate before one starts
> mini.

In 90% of all electronic structure papers nowadays a structure relaxation
has been performed.
Of course it is true, that this may take quite a long time, since this is
nothing than a long series of sequential scf calculations.

Yes, there are many other programs available, SIESTA and VASP was already
mentioned before.

For a partiular class of compounds these programs can be highly efficient
and much faster than WIEN (e.i. with SIESTA they have simulated biomolecules
with 1000s !! of atoms). However, most of those programs are NOT applicable
to all systems. Try SIESTA for metals and I doubt that you can do more than
WIEN can do, and in addition most likely the results will also be WRONG.

To use such programs, you probably need to be much more experienced than
when using WIEN.

I disagree with the statement:
> They need not to be that accurate as LAPW, in many cases it
> would be very helpful to have a rough but quick estimate before one starts
> mini.
They might even go into the wrong direction!! then you are better off to
start with your estimated (or exp.) structure (and use a very small k-mesh
at the beginning)

I must admit that WIEN could be significantly improved with respect to
structural relaxations.
Mainly 2 points would be important:
a) Better usage of the charge density of the previous geometry, so that one
does not need so many scf cycles for the subsequent geometry steps.
We have some ideas about that, but no manpower.
b) The implemented NEWT algorithm for relaxation is quite stupid! You have to
select proper "timestep"-factors in the input and the handling is clumsy.
Also here many improvements (for both the NEWT scheme, but also other schemes
like conjg gradients) are waiting.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Fri, 27 Sep 2002 18:23:50 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Questions about "mini" vs. "optimize"

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Peter and Stefaan,

thank you for these very interesting and deep answers! It confirmed to 
me that it is a difficult and potentially long-lasting task, but also 
revealed a great deal of insight into the process.

As usual, I am setting up a slab calculation in order to try to optimize 
a metal surface with an overlayer of another metal. Thus, based on your 
answers, I have decided to use a little bit of two worlds (the 
"optimize"-like scheme and VASP separately, and if the latter gives a 
reasonable output it will be followed by another, but finer, 
"optimize"-like scheme to test and possibly fine-tune the result), in 
order to test how easy or difficult it is to find something useful. I 
pretty much know the positions of the atoms in two dimensions from 
experiment, but there are no experimental results on the third 
dimension, as far as I can tell by sifting through the literature. The 
"bulk" material does not change very much at the surface, so to a first 
approximation it is a question of getting the overlayer distance to the 
"bulk" determined.

Unfortunately, at the moment I am confined to do parallelisation on the 
scf-cycle level, since each CPU has its own place in the queueing 
system. Yes, I can play with channels in the queueing system, but that 
would require thousands of k-points to be of any use (and a queue-tuned 
run_lapw, which is possible to write, but clumsy).

Best regards,
Torsten.

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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Date: Sat, 28 Sep 2002 00:58:42 +0800
From: "yulihua-wuhan" <yulihua-wuhan@sohu.com>
Subject: [none]

====
"yulihua-wuhan" <yulihua-wuhan@sohu.com>
submitted the following contribution:
====

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Date: Sat, 28 Sep 2002 09:10:15 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: [WIEN]: Re: 

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

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I suggest looking for recent e-mails with the subject of "Partial =
DOS/Tetra".
Your,
S. Jalali.
  ----- Original Message -----=20
  From: yulihua-wuhan=20
  To: wien@zeus.theochem.tuwien.ac.at=20
  Sent: Friday, September 27, 2002 8:28 PM


  Dear Wien2k Users and developers:

     I have calculated the compound X2YO2 band structure,and find some =
bands are almost only=20
  related to S orbital of O-atom ,and when I plot the DOS curves,I find =
that the O total DOS is=20
  double as the O-atom S partial DOS at the corresponding energy range =
for those bands,so I think=20
  the DOS unit is states/eV/atom for atom partial =
DOS,states/eV/chemistry formula(2 O atoms) for=20
  atom total DOS,and states/eV/chemistry formula for total DOS(all atoms =
in the compound).   Am I=20
  right?

     But this compound has 2 formula units per cell, so maybe we have =
another choice:
     for instance O atom in this compound=20
     states/eV/(2 atom) for atom partial DOS,
     states/eV/cell for atom total DOS,
     states/eV/cell for total DOS(all atoms in the compound).

     I guess some answers above, the answer should be definite. I want =
to ask the DOS units.

     Thank you very much=20



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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; charset=3Dgb2312">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV>
<DIV><FONT face=3DArial size=3D2>I suggest looking for recent e-mails =
with the=20
subject of <FONT size=3D3>"Partial DOS/Tetra".</FONT></FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Your,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>S. Jalali.</FONT></DIV></DIV>
<BLOCKQUOTE dir=3Dltr=20
style=3D"PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; =
BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
  <DIV style=3D"FONT: 10pt arial">----- Original Message ----- </DIV>
  <DIV=20
  style=3D"BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: =
black"><B>From:</B>=20
  <A title=3Dyulihua-wuhan@sohu.com=20
  href=3D"mailto:yulihua-wuhan@sohu.com">yulihua-wuhan</A> </DIV>
  <DIV style=3D"FONT: 10pt arial"><B>To:</B> <A=20
  title=3Dwien@zeus.theochem.tuwien.ac.at=20
  =
href=3D"mailto:wien@zeus.theochem.tuwien.ac.at">wien@zeus.theochem.tuwien=
.ac.at</A>=20
  </DIV>
  <DIV style=3D"FONT: 10pt arial"><B>Sent:</B> Friday, September 27, =
2002 8:28=20
  PM</DIV>
  <DIV><FONT face=3DArial size=3D2></FONT><BR></DIV>
  <DIV>
  <DIV><FONT face=3D"Times New Roman">Dear Wien2k Users and=20
  developers:</FONT></DIV>
  <DIV><FONT face=3D"Times New Roman"></FONT>&nbsp;</DIV>
  <DIV><FONT face=3D"Times New Roman">&nbsp;&nbsp; I have calculated the =
compound=20
  X2YO2 band structure,and find some bands are almost only </FONT></DIV>
  <DIV><FONT face=3D"Times New Roman">related to S orbital of O-atom =
,and when I=20
  plot the DOS curves,I find that the O total DOS is </FONT></DIV>
  <DIV><FONT face=3D"Times New Roman">double as the O-atom S partial DOS =
at the=20
  corresponding energy range for those bands,so I think </FONT></DIV>
  <DIV><FONT face=3D"Times New Roman">the DOS unit is states/eV/atom for =
atom=20
  partial DOS,states/eV/chemistry formula(2 O atoms) for </FONT></DIV>
  <DIV><FONT face=3D"Times New Roman">atom total DOS,and =
states/eV/chemistry=20
  formula for total DOS(all atoms in the compound).&nbsp;&nbsp; Am I=20
  </FONT></DIV>
  <DIV><FONT face=3D"Times New Roman">right?</FONT></DIV>
  <DIV><FONT face=3D"Times New Roman"></FONT>&nbsp;</DIV>
  <DIV><FONT face=3D"Times New Roman">&nbsp;&nbsp; But this compound has =
2 formula=20
  units per cell, so maybe we have another choice:<BR>&nbsp;&nbsp; for =
instance=20
  O atom in this compound <BR>&nbsp;&nbsp; states/eV/(2 atom) for atom =
partial=20
  DOS,<BR>&nbsp;&nbsp; states/eV/cell for atom total =
DOS,<BR>&nbsp;&nbsp;=20
  states/eV/cell for total DOS(all atoms in the compound).</FONT></DIV>
  <DIV><FONT face=3D"Times New Roman"></FONT>&nbsp;</DIV>
  <DIV><FONT face=3D"Times New Roman">&nbsp;&nbsp; I guess some answers =
above, the=20
  answer should be definite. I want to ask the DOS units.</FONT></DIV>
  <DIV><FONT face=3D"Times New Roman"></FONT>&nbsp;</DIV>
  <DIV><FONT face=3D"Times New Roman">&nbsp;&nbsp; Thank you very much=20
  </FONT></DIV>
  <DIV><FONT face=3D"Times New Roman"></FONT>&nbsp;</DIV>
  <DIV><FONT=20
face=3D"Times New =
Roman"></FONT>&nbsp;</DIV></DIV></BLOCKQUOTE></BODY></HTML>

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Date: Sat, 28 Sep 2002 15:01:54 +0800 (CST)
From: music@theory.issp.ac.cn
Subject: [WIEN]: QTL-B about 2

====
music@theory.issp.ac.cn
submitted the following contribution:
====


 
Dear wien users,
   I'm using wien2k to calculate a system including La and H atoms, and 
I've set the RMT=1.2 for H, and RKMAX=6. But the QTL-B equals to 5 at 
first. So I used 'runsp_lapw -inlnew 1' to get updated case.in1c file. 
Then QTL-B equals to about 2. I wonder  how  this small QTL-B values
occur and does it matter  the properties of system ? 
  Many thanks for any help from you !   
 
- -- 
sincerely yours 

Ying.X


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------------------------------

Date: Sat, 28 Sep 2002 12:34:12 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: QTL-B about 2

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>    I'm using wien2k to calculate a system including La and H atoms, and
> I've set the RMT=1.2 for H, and RKMAX=6. But the QTL-B equals to 5 at
> first. So I used 'runsp_lapw -inlnew 1' to get updated case.in1c file.
> Then QTL-B equals to about 2. I wonder  how  this small QTL-B values
> occur and does it matter  the properties of system ?
Your adding the switch "in1new 1" is perfect to get rise accuracy of
linearization both in semi core (:EPL) and valence (:EPH) states to reduce
QTL-B value. This small value occurs, as contribution from linearized basis
to wavefunction is not exactly zero. Although you can don't care, there are
also possibilities to improve it decreasing RMT as you are treating with a
short bondlength system, reducing mixing factor to 0.01 in case.inm file,
and finally give linearization by hand a try to check if in1new is done
perfectly its job or not. To carry out the later step, linearization
manually, one plots DOSs and then finds center of each curve, where the
probability of electrons is maximum for each DOS, to find the best
linearization and compare the result with the last in1 file.
Your,
Saeid.

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Date: Sat, 28 Sep 2002 18:40:44 +0800
From: joshua xie <joshuaxie@etang.com>
Subject: [WIEN]: about 4H and 6H SiC

====
joshua xie <joshuaxie@etang.com>
submitted the following contribution:
====

Dear wien users£¬

     I am not quite clear about the crystal structure of 4H and 6H SiC,so I do not know how to write the struct file of perfect 4H or 6H SiC crystal. Could someone give me the struct file or some hints to do these jobs?

     Thank you very much. 

Best regards! 				
Joshua Xie                               




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Date: Sat, 28 Sep 2002 19:30:35 +0800 (CST)
From: music@theory.issp.ac.cn
Subject: Re: [WIEN]: QTL-B about 2

====
music@theory.issp.ac.cn
submitted the following contribution:
====


      Thank you very much.
      I'll try it. 
On Sat, 28 Sep 2002, Saeid Jalali wrote:

> ====
> "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> submitted the following contribution:
> ====
> 
> >    I'm using wien2k to calculate a system including La and H atoms, and
> > I've set the RMT=1.2 for H, and RKMAX=6. But the QTL-B equals to 5 at
> > first. So I used 'runsp_lapw -inlnew 1' to get updated case.in1c file.
> > Then QTL-B equals to about 2. I wonder  how  this small QTL-B values
> > occur and does it matter  the properties of system ?
> Your adding the switch "in1new 1" is perfect to get rise accuracy of
> linearization both in semi core (:EPL) and valence (:EPH) states to reduce
> QTL-B value. This small value occurs, as contribution from linearized basis
> to wavefunction is not exactly zero. Although you can don't care, there are
> also possibilities to improve it decreasing RMT as you are treating with a
> short bondlength system, reducing mixing factor to 0.01 in case.inm file,
> and finally give linearization by hand a try to check if in1new is done
> perfectly its job or not. To carry out the later step, linearization
> manually, one plots DOSs and then finds center of each curve, where the
> probability of electrons is maximum for each DOS, to find the best
> linearization and compare the result with the last in1 file.
> Your,
> Saeid.
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 
 
- -- 





sincerely yours 

Ying.X


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Date: Sat, 28 Sep 2002 15:27:22 +0200 (MESZ)
From: "A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
Subject: Re: [WIEN]: Questions about "mini" vs. "optimize"

====
"A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
submitted the following contribution:
====

Dear WIEN comunity,

refering to a recent discussion about mini and relaxation -

to my opinion the most annoying feature of WIEN
in what regards structure relaxation is that
internal coordinates and lattice parameters have to be
optimized decoupled, and the optimization of lattice
parameters is essentially done by hand
(in a sequence of volume, c/a, c/b, ... runs).
So it involves a fair amount of hand work
to keep trace on all these optimizations,
ultimately (with a bit of luck) converging them in a sequence
of loops volume - c/a - mini - volume - c/a - ....
- - or does anyone do it in a more automatized way?
For the comparison, the SIESTA code already mentioned
in this discussion includes a very nice
feature of relaxing everything "on the fly",
based on forces and stress tensor. One can e.g.
define a target pressure and/or target stress -
and the computer does (the large part of) the rest.
And this has nothing to do with all-electron/pseudopot
issues. To my opinion, the argumentation that SIESTA 
(or VASP) are fast and conveninet but unfortunately
they don't work for all systems is somehow beyond
the point. The calculation speed is one issue - and here
both SIESTA and VASP pay a certain price for being fast.
But the possibility to do convenient and automatic
structure optimization has nothing to do with the speed.
It can be incorporated in any code where forces and stress
are available.
A certain technical difference is that SIESTA does not care 
about conserving symmetry and proceeds with "general"
(and "noisy") Cartesian forces, whereas in WIEN the forces and stress 
are constrained by the space group. But once we start the
simulation the symmetry won't break by itself and doesn't
need to be recalculated, so all the machinery of  mini
can be hopefully extended over varying lattice parameters.
Although being certainly dependent on careful manpower,
the implementation of such symmetry-constrained 
conjugate gradient search seems to me mostly a technical issue, 
and I am sure many users will appreciate this addition.

Andrei Postnikov
apostnik@uos.de

On Fri, 27 Sep 2002, Peter Blaha wrote:

> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> ....
>
> In 90% of all electronic structure papers nowadays a structure relaxation
> has been performed.
> Of course it is true, that this may take quite a long time, since this is
> nothing than a long series of sequential scf calculations.
> 
> Yes, there are many other programs available, SIESTA and VASP was already
> mentioned before.
> 
> For a partiular class of compounds these programs can be highly efficient
> and much faster than WIEN (e.i. with SIESTA they have simulated biomolecules
> with 1000s !! of atoms). However, most of those programs are NOT applicable
> to all systems. Try SIESTA for metals and I doubt that you can do more than
> WIEN can do, and in addition most likely the results will also be WRONG.
> 
> To use such programs, you probably need to be much more experienced than
> when using WIEN.
> 

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Date: Sat, 28 Sep 2002 19:09:56 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: about 4H and 6H SiC

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

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>      I am not quite clear about the crystal structure of 4H and 6H =
SiC,so I do not know how to write the struct file of perfect 4H or 6H =
SiC crystal. Could someone give me the struct file or some hints to do =
these jobs?


4H and 6H SiC refer to 4 and 6 dimmers of this formula to indicate that =
4 SiC dimmers (4 Si and 4 C totally 8 atoms) are in 4H SiC cell and 6 =
SiC dimmers (6 Si and 6 C totally 12 atoms) are in 6H SiC cell. In 4H =
SiC there are 2 types of Si and 2 type of C. In 6H SiC there are 3 types =
of Si and 3 type of C. In 4H SiC there are 4 internal parameters, while =
the number of internal parameters is only 5 for 6H SiC. The number of =
space group for 4H SiC is "186" and it is similar to the number of space =
group for 6H SiC. So You would select this number using struct generator =
of WIEN2K for both of them, and just try to fill atomic positions. One =
can find these atomic positions via many references, that I would notify =
you from one of them:

4H SiC
B1  =3D  z1c Z  (C-I)
B2  =3D (=C2=BD+ z1)cZ  (C-I)=20
B3  =3D  =C2=BDaX-a/(23=C2=BD)Y+ z2cZ  (C-II)
B4  =3D  =C2=BDaX+ a/(23=C2=BD)Y+(=C2=BD+z2)c Z  (C-II)
B5  =3D  z3c Z  (Si-I) =20
B6  =3D  (=C2=BD+ z3)cZ  (Si-I)
B7  =3D  =C2=BDaX+a/(23=C2=BD)Y+ z4cZ  (Si-II) =20
B8  =3D  =C2=BDaX- a/(23=C2=BD)Y+(=C2=BD+z4)c Z  (Si-II) =20
in where (z1 =3D 0,  z2 =3D 1/4, z3 =3D 3/16, z4 =3D 7/16

- -------------------------------------------------------------------------=
- -------

6H SiC
B1 =3D   0   (Si-I)
B2 =3D =C2=BD c Z (Si-I)
B3 =3D z1 c Z (C-I)
B4 =3D (=C2=BD + z1) c Z (C-I)=20
B5 =3D =C2=BD a X + a/(2 3=C2=BD) Y + z2 c Z (Si-II)
B6 =3D =C2=BD a X - a/(2 3=C2=BD) Y + (=C2=BD + z2) c Z (Si-II)=20
B7 =3D =C2=BD a X + a/(2 3=C2=BD) Y + z3 c Z (C-II)=20
B8 =3D =C2=BD a X - a/(2 3=C2=BD) Y + (=C2=BD + z3) c Z (C-II)=20
B9 =3D =C2=BD a X + a/(2 3=C2=BD) Y + z4 c Z (Si-III)
B10=3D =C2=BD a X - a/(2 3=C2=BD) Y + (=C2=BD + z4) c Z (Si-III)=20
B11 =3D =C2=BD a X + a/(2 3=C2=BD) Y + z5 c Z (C-III)=20
B12 =3D =C2=BD a X - a/(2 3=C2=BD) Y + (=C2=BD + z5) c Z (C-III)=20

2 3=C2=BD  is  2*3^(1/2), zi is internal parameter, X, Y, Z are =
Cartesian axis's, and a=3Db, c are lattice parameters, which you don't =
need to consider them when you are filling the positions.=20

Your,
S. Jalali.
PS: This e-mail is sent as a Unicode message.

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<BODY>
<DIV>&gt; &nbsp;&nbsp;&nbsp;&nbsp; I am not quite clear about the =
crystal=20
structure of 4H and 6H SiC,so I do not know how to write the struct file =
of=20
perfect 4H or 6H SiC crystal. Could someone give me the struct file or =
some=20
hints to do these jobs?<BR></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>4H and 6H SiC&nbsp;refer to 4&nbsp;and =
6 dimmers of=20
this formula to indicate&nbsp;that 4 SiC dimmers (4 Si and 4 C totally 8 =

atoms)&nbsp;are in 4H SiC cell </FONT><FONT face=3DArial =
size=3D2>and&nbsp;6 SiC=20
dimmers (6 Si and&nbsp;6 C totally&nbsp;12 atoms)&nbsp;are in 6H SiC =
cell. In 4H=20
SiC there are 2 types of Si and 2 type of C. In 6H SiC there are&nbsp;3 =
types of=20
Si and&nbsp;3 type of C. In 4H SiC there are 4 internal =
parameters,&nbsp;while=20
the number of internal parameters is only 5 for 6H SiC. The number of =
space=20
group for 4H SiC is "186" and it is similar to the number of space group =
for 6H=20
SiC. So You would select this number using struct generator of WIEN2K =
for both=20
of them, and just try to fill atomic positions.&nbsp;One can find these =
atomic=20
positions via many references, that I would notify you from one of=20
them:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>4H SiC</FONT></DIV>
<DIV><FONT face=3DArial size=3D2><FONT=20
size=3D3><STRONG>B</STRONG><SUB>1</SUB></TD>&nbsp;<TD><SUB>&nbsp;</SUB>=3D=
<SUB>&nbsp;</SUB></TD>=20
<TD>z<SUB>1</SUB>c <STRONG>Z</STRONG></TD>=20
<TD><SUB>&nbsp;</SUB>(C-I)</FONT></FONT></DIV>
<DIV><FONT face=3DArial size=3D2><FONT size=3D3></TR><TR =
align=3D"Center"=20
valign=3D"Bottom"><TD><STRONG>B</STRONG><SUB>2</SUB></TD> =
<TD><SUB>&nbsp;</SUB>=3D=20
<TD>(=C2=BD+ z<SUB>1</SUB>)c<STRONG>Z</STRONG></TD>=20
<TD><SUB>&nbsp;</SUB>(C-I)</TD>&nbsp;</FONT></FONT></DIV>
<DIV><FONT face=3DArial size=3D2><FONT size=3D3></TR><TR =
align=3D"Center"=20
valign=3D"Bottom"><TD><STRONG>B</STRONG><SUB>3</SUB></TD>=20
<TD><SUB>&nbsp;</SUB>=3D<SUB>&nbsp;</SUB></TD>=20
<TD>=C2=BDa<STRONG>X</STRONG>-a/(23<SUP>=C2=BD</SUP>)<STRONG>Y</STRONG>+ =

z<SUB>2</SUB>c<STRONG>Z</STRONG></TD>=20
<TD><SUB>&nbsp;</SUB>(C-II)</FONT></FONT></DIV>
<DIV><FONT face=3DArial size=3D2><FONT=20
size=3D3><STRONG>B</STRONG><SUB>4</SUB>&nbsp;<TD><SUB>&nbsp;</SUB>=3D<SUB=
>&nbsp;</SUB></TD>=20
<TD>=C2=BDa<STRONG>X</STRONG>+=20
a/(23<SUP>=C2=BD</SUP>)<STRONG>Y</STRONG>+(=C2=BD+z<SUB>2</SUB>)c =
<STRONG>Z</STRONG></TD>=20
<TD><SUB>&nbsp;</SUB>(C-II)</FONT></FONT></DIV>
<DIV><FONT face=3DArial size=3D2><FONT =
size=3D3><STRONG>B</STRONG><SUB>5</SUB></TD>=20
<TD><SUB>&nbsp;</SUB>=3D&nbsp; <TD>z<SUB>3</SUB>c =
<STRONG>Z</STRONG></TD>=20
<TD><SUB>&nbsp;</SUB>(Si-I)</TD>&nbsp;<TD><SUB>&nbsp;</SUB></FONT></FONT>=
</DIV>
<DIV><FONT face=3DArial size=3D2><FONT size=3D3></TR><TR =
align=3D"Center"=20
valign=3D"Bottom"><TD><STRONG>B</STRONG><SUB>6</SUB></TD>=20
<TD><SUB>&nbsp;</SUB>=3D<SUB>&nbsp;</SUB> <TD>(=C2=BD+=20
z<SUB>3</SUB>)c<STRONG>Z</STRONG></TD>=20
<TD><SUB>&nbsp;</SUB>(Si-I)</FONT></FONT></DIV>
<DIV><FONT face=3DArial size=3D2><FONT size=3D3></TR><TR =
align=3D"Center"=20
valign=3D"Bottom"><TD><STRONG>B</STRONG><SUB>7</SUB></TD>&nbsp;<TD><SUB>&=
nbsp;</SUB>=3D<SUB>&nbsp;</SUB></TD>=20
<TD>=C2=BDa<STRONG>X</STRONG>+a/(23<SUP>=C2=BD</SUP>)<STRONG>Y</STRONG>+ =

z<SUB>4</SUB>c<STRONG>Z</STRONG></TD>=20
<TD><SUB>&nbsp;</SUB>(Si-II)</TD>&nbsp;<TD><SUB>&nbsp;</SUB></FONT></FONT=
></DIV>
<DIV><FONT face=3DArial size=3D2><FONT size=3D3></TR><TR =
align=3D"Center"=20
valign=3D"Bottom"><TD><STRONG>B</STRONG><SUB>8</SUB></TD>&nbsp;<TD><SUB>&=
nbsp;</SUB>=3D<SUB>&nbsp;</SUB></TD>=20
<TD>=C2=BDa<STRONG>X</STRONG>-=20
a/(23<SUP>=C2=BD</SUP>)<STRONG>Y</STRONG>+(=C2=BD+z<SUB>4</SUB>)c =
<STRONG>Z</STRONG></TD>=20
<TD><SUB>&nbsp;</SUB>(Si-II)</TD>&nbsp;<TD><SUB></SUB></TD></TR>&nbsp;</F=
ONT></FONT></DIV>
<DIV><FONT face=3DArial size=3D2><FONT face=3DArial size=3D2>in where =
(z1 =3D 0,&nbsp; z2=20
=3D 1/4, z3 =3D 3/16, z4 =3D 7/16</DIV></FONT><!-- Footer Starts Here: =
- -->
<DIV>
<HR>
</DIV></FONT>
<DIV><B>6H SiC</B></DIV>
<DIV><B>B</B><SUB>1</SUB> </TD><TD align=3D"Center">=3D</TD> <TD=20
align=3D"Center">&nbsp; </TD><TD align=3D"Center">0 </TD><TD =
align=3D"Center">&nbsp;=20
</TD><TD align=3D"Center">(Si-I)</DIV>
<DIV><STRONG>B</STRONG><SUB>2</SUB>&nbsp;</TD><TD align=3D"Center">=3D =
</TD><TD=20
align=3D"Center">=C2=BD c <STRONG>Z</STRONG> </TD><TD =
align=3D"Center">(Si-I)</DIV>
<DIV><STRONG>B</STRONG><SUB>3</SUB>&nbsp;</TD><TD align=3D"Center">=3D =
</TD><TD=20
align=3D"Center">z<SUB>1</SUB> c <B>Z</B> </TD><TD =
align=3D"Center">(C-I)</DIV>
<DIV><B>B</B><SUB>4</SUB> =3D </TD><TD align=3D"Center">(=C2=BD + =
z<SUB>1</SUB>) c=20
<B>Z</B> </TD><TD align=3D"Center">(C-I) </DIV>
<DIV><B>B</B><SUB>5</SUB>&nbsp;</TD><TD align=3D"Center">=3D </TD><TD=20
align=3D"Center">=C2=BD a <B>X</B> + a/(2 3<SUP>=C2=BD</SUP>) <B>Y</B> + =
z<SUB>2</SUB> c=20
<B>Z</B> </TD><TD align=3D"Center">(Si-II)</DIV>
<DIV></TD></TR><TR><TD align=3D"Center"><B>B</B><SUB>6</SUB> </TD><TD=20
align=3D"Center">=3D</TD>&nbsp;</TD><TD align=3D"Center">=C2=BD a =
<B>X</B> - a/(2=20
3<SUP>=C2=BD</SUP>) <B>Y</B> + (=C2=BD + z<SUB>2</SUB>) c <B>Z</B> =
</TD><TD=20
align=3D"Center">(Si-II) </DIV>
<DIV><B>B</B><SUB>7</SUB> =3D </TD><TD align=3D"Center">=C2=BD a =
<B>X</B> + a/(2=20
3<SUP>=C2=BD</SUP>) <B>Y</B> + z<SUB>3</SUB> c <B>Z</B> </TD><TD=20
align=3D"Center">(C-II) </DIV>
<DIV><B>B</B><SUB>8</SUB>&nbsp;</TD><TD align=3D"Center">=3D </TD><TD=20
align=3D"Center">=C2=BD a <B>X</B> - a/(2 3<SUP>=C2=BD</SUP>) <B>Y</B> + =
(=C2=BD + z<SUB>3</SUB>)=20
c <B>Z</B> </TD><TD align=3D"Center">(C-II) </DIV>
<DIV><B>B</B><SUB>9</SUB> =3D </TD><TD align=3D"Center">=C2=BD a =
<B>X</B> + a/(2=20
3<SUP>=C2=BD</SUP>) <B>Y</B> + z<SUB>4</SUB> c <B>Z</B> </TD><TD=20
align=3D"Center">(Si-III)</DIV>
<DIV></TD></TR><TR><TD align=3D"Center"><B>B</B><SUB>10</SUB></TD><TD=20
align=3D"Center">=3D </TD><TD align=3D"Center">=C2=BD a <B>X</B> - a/(2 =
3<SUP>=C2=BD</SUP>)=20
<B>Y</B> + (=C2=BD + z<SUB>4</SUB>) c <B>Z</B> </TD><TD =
align=3D"Center">(Si-III)=20
</DIV>
<DIV><B>B</B><SUB>11</SUB> </TD><TD =
align=3D"Center">=3D</TD>&nbsp;</TD><TD=20
align=3D"Center">=C2=BD a <B>X</B> + a/(2 3<SUP>=C2=BD</SUP>) <B>Y</B> + =
z<SUB>5</SUB> c=20
<B>Z</B> </TD><TD align=3D"Center">(C-III) </DIV>
<DIV><B>B</B><SUB>12</SUB> </TD><TD =
align=3D"Center">=3D</TD>&nbsp;</TD><TD=20
align=3D"Center">=C2=BD a <B>X</B> - a/(2 3<SUP>=C2=BD</SUP>) <B>Y</B> + =
(=C2=BD + z<SUB>5</SUB>)=20
c <B>Z</B> </TD><TD align=3D"Center">(C-III) </DIV>
<DIV><FONT face=3DArial></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>2 3<SUP>=C2=BD</SUP>&nbsp; is&nbsp; =
2*3^(1/2), z<SUB>i=20
</SUB>is internal parameter, <STRONG>X, Y, Z </STRONG>are Cartesian =
axis's, and=20
a=3Db, c are lattice parameters, which you don't need to&nbsp;consider =
them when=20
you are filling the positions. </FONT><FONT face=3DArial></FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Your,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>S. Jalali.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>PS: This e-mail is sent as a Unicode=20
message.</FONT></DIV></BODY></HTML>

- ------=_NextPart_000_04AF_01C26722.A21613A0--

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Date: Sat, 28 Sep 2002 19:41:47 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: min_lapw

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

Can I run min_lapw in parallelization mode?

Thanks!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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Date: Sun, 29 Sep 2002 09:29:52 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: min_lapw

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> Can I run min_lapw in parallelization mode?
No you cannot use -p directly for series of sequential calculations, but in
the "run_lapw" job to parallelize the k-points. In the case of having one
internal parameter following the rule of E=aX^2 or F=-aX, it is recommended
to minimize in parallel mode manually, selecting at least two X-positions
and fitting the parabolic formula. I am really afraid to say that having
such a rule is a simple but general idea, which may be extended to cases
with more than one internal parameter. This means that if one collects
relaxed positions of studied systems with two internal parameters, one may
find an empirical rule. This may not be just an idea to parallelize serial
mini calculations, as in this case speeding up is another goal of this
story. We know that there are many cases with one internal parameter
following the parabolic rule, an I wonder if it is possible at least to take
an special consideration for these systems.
Your,
S. Jalali.

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Date: Sun, 29 Sep 2002 12:00:05 +0200
From: Stefaan.Cottenier@fys.kuleuven.ac.be
Subject: Re: [WIEN]: min_lapw

====
Stefaan.Cottenier@fys.kuleuven.ac.be
submitted the following contribution:
====

> ====
> Bing Zhou <umbingz@cc.UManitoba.CA>
> submitted the following contribution:
> ====
> 
> Can I run min_lapw in parallelization mode?

Yes. With min_lapw you always specify a run_lapw or runsp_lapw command (either 
as argument or in a jobfile). Include the -p switch there and provide a 
suitable .machines file.

Stefaan


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Date: Sun, 29 Sep 2002 10:05:16 -0400 (EDT)
From: Neme Nnolim <non6886@alizarin.njit.edu>
Subject: [WIEN]: Problems with Eplot 'coa' plotting

====
Neme Nnolim <non6886@alizarin.njit.edu>
submitted the following contribution:
====


Dear All,

Eplot in WIEN works well for 'vol' plots but does not seem to work as
well for 'coa' plots.

My 'coa' energies calculated with x optimize look smooth when plotted with
an external plotting program, but do not plot in Eplot.

Anyone else experienced this?

Neme

- ------------------------------------------------------------------------------
Neme Okechukwu Nnolim
Department of Materials Science, New Jersey Institute of Technology
Room 302, Tiernan Hall, 161 Warren Street, University Heights
Newark, New Jersey 07102-1982
Tel: (973) 596-8283, FAX: (973) 596-5794
- -------------------------------------------------------------------------------


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Date: Sun, 29 Sep 2002 10:44:15 -0400 (EDT)
From: Neme Nnolim <non6886@alizarin.njit.edu>
Subject: [WIEN]: Re: Problems with Eplot 'coa' plotting

====
Neme Nnolim <non6886@alizarin.njit.edu>
submitted the following contribution:
====


Actually I don't see what Eplot could possibly use for abscissa values
for a 'coa' plot in the case.analysis file, unlike the 'vol' plot where
:VOL is used for the abscissa.

On Sun, 29 Sep 2002, Neme Nnolim wrote:

> Date: Sun, 29 Sep 2002 10:05:16 -0400 (EDT)
> From: Neme Nnolim <non6886@alizarin.njit.edu>
> To: WIEN mailing list <wien@zeus.theochem.tuwien.ac.at>
> Subject: Problems with Eplot 'coa' plotting
>
>
> Dear All,
>
> Eplot in WIEN works well for 'vol' plots but does not seem to work as
> well for 'coa' plots.
>
> My 'coa' energies calculated with x optimize look smooth when plotted with
> an external plotting program, but do not plot in Eplot.
>
> Anyone else experienced this?
>
> Neme
>
> ------------------------------------------------------------------------------
> Neme Okechukwu Nnolim
> Department of Materials Science, New Jersey Institute of Technology
> Room 302, Tiernan Hall, 161 Warren Street, University Heights
> Newark, New Jersey 07102-1982
> Tel: (973) 596-8283, FAX: (973) 596-5794
> -------------------------------------------------------------------------------
>
>
>

- -- 

- ------------------------------------------------------------------------------
Neme Okechukwu Nnolim
Department of Materials Science, New Jersey Institute of Technology
Room 302, Tiernan Hall, 161 Warren Street, University Heights
Newark, New Jersey 07102-1982
Tel: (973) 596-8283, FAX: (973) 596-5794
- -------------------------------------------------------------------------------


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------------------------------

Date: Sun, 29 Sep 2002 12:11:19 -0700 (PDT)
From: Igor Mazin <wienuser1@yahoo.com>
Subject: Re: [WIEN]:

====
Igor Mazin <wienuser1@yahoo.com>
submitted the following contribution:
====

Just a follow-up.

A solid is not a molecuel, and no band strusture code
has a complete basis set. Therefore the difference
between these matrix elements may be nontrivial.

See our old paper,

Z.f.Phys., B53, 1983, 263

Good luck
Igor
- --- Fred Nastos <nastos@physics.utoronto.ca> wrote:
> ====
> Fred Nastos <nastos@physics.utoronto.ca>
> submitted the following contribution:
> ====
> 
> On September 24, 2002 07:38 am, Ma Chi Chiu wrote:
> > ====
> > Ma Chi Chiu <martin@yangtze.hku.hk>
> > submitted the following contribution:
> > ====
> 
> Before I pushed send, I noticed Dr. Andersen has
> allready replied. Just
> to add though...
> 
> > 1. definition of "momentum matrix elements" (Is it
> the same as transition
> > dipole moment?)
> 
> The momentum matrix element is defined as,
> 
> 	<nk|p|mk> = int d^3r <nk|r> i hbar nabla <r|mk>
> 
>  where |nk> is a Bloch state. The wien code uses
> Rydberg atomic units 
> (throughout), in which hbar=m=e=1. The atomic unit
> for momentum (Ry or H)
> is hbar/a0 (where a0 is the Bohr radius).
> 
> The dipole matrix element is usually <nk|r|mk>. If n
> and m are different bands
> the two matrix elements can be simply related as
> they are for molecules.
> 
> > 2. definition of k-mesh (What is the differences
> between k-mesh and
> > k-point?)
> 
> The k-mesh is the set of k-points, i.e. the grid of
> points. See Bloechl et al. 
> [Phys. Rev. B 49, 16223-16233 (1994)] for the
> details.
> 
> Fred
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====


=====
***************************************************************************** 
Igor Mazin, Naval Research Laboratory, Washington, DC 20375
Ph.: 202 767-6990; Fax: 202 404-7546; http://cst-www.nrl.navy.mil/~mazin 
*****************************************************************************

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Date: Mon, 30 Sep 2002 10:53:12 +1000
From: chen0130@flinders.edu.au
Subject: Re: [WIEN]: DOS matching bandstructures...

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Thanks Saeid Jalali and Torsten Andersen for you assistance!

Thanks so much! It is a great relief to see the peaks corresponding to the
energy levels of the bands!

thanks for your invaluable help!

Cheng

Quoting Saeid Jalali <sjalali@cc.iut.ac.ir>:

> > I am studying a simple case of solid Li2O. 
> > 
> > My bandstructure reveals bands at 0 to -5 eV (O 2p), -15 eV and -45 eV...
>  
> > then I changed the k mesh back to the original, run a single SCF cycle,
> to
> > ensure lapw1 is done,
> 
> 
> 
> That is okay, but when you want to calculate DOS after the bandstructure, you
> only need to run lapw1 with the original case.in1 file to make sure about
> proper case.vector(s).
> 
> 
> > and do the DOS... but it only has peaks at around -5 eV (ignoring above
> E_fermi)
> > 
> > i also tried setting a fresh case and doing the DOS only after the SCF...
> 
>  
> 
> That is okay (making strongly sure), but time consuming.
> 
> > i am puzzled, I really expect peaks in the DOS to correspond to the bands
> at
> > those energies...
>  
> 
> You are right, there should be such a correspondence between DOS and band
> character plotting.
> 
>  
> 
> > can someone tell me possible errors, hints from their experiences?
> 
>  
> 
> If you would see DOS's from -45eV, change Emin of case.int file to
> -45/13.6~-3.4Ry, and then run tetra.
> 
>  
> 
> Your,
> 
> S. Jalali.
> 
> 



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------------------------------

Date: Mon, 30 Sep 2002 11:20:26 +0900
From: Satoshi Okada <okada@hpc.co.jp>
Subject: [WIEN]: lapw2 & ifc on LINUX

====
Satoshi Okada <okada@hpc.co.jp>
submitted the following contribution:
====


Hi all,

I try to make WIEN2k with ifc(Intel Fortran Compiler) on LINUX.

When WIEN2k(lapw2) read a vector data file ( UNIT 10 ),
the illegal values were inputed for kx_buf,ky_buf,kz_buf
after about 400byte reading.

SRC_lapw2/read_vec.F:
     54   IF(myid.EQ.0) THEN
     55      WRITE(31,205) s,t,z,n,ne,bname
     56      READ(10) (kx_buf(i),ky_buf(i),kz_buf(i),
		i=1,n-(nlo+nlon+nlov)),
                (kxlo(i),kylo(i),kzlo(i),i=1,(nlo+nlon+nlov))
     57   ENDIF

This problem occur in sample input data (TiC , TiO2).

Another compiler ( ex. pgf90 ) can read this data file correctly.
And, when i use FORMATTED vector data file for WRITE & READ, lapw2 can
read all data correctly.
So, i think this problem cases binary data READ(WRITE) for ifc.

Do you have any suggestion for this problem ?
When I asked Intel this problem, Intel said "Give me all program &
data".  And I
 didn't.

=================================

Our environment :
CPU     Intel Pentium4 1.8GHz 256KBcache
M/B     ASUS P4T
Mem     1048MB
OS      SuSE Linux 7.1 kernel 2.4.17
ifc     Intel(R) Fortran Compiler for 32-bit applications, Version 6.0.1
                Build 20020822Z
WIEN2K  WIEN2k_02 (Sep 12)
        OPTION
                current:FOPT:-FR -mp -w
                current:LDFLAGS:-L../SRC_lib -Vaxlib -static
                current:R_LIBS:-lblas_lapw -llapack_lapw

Regards.

- -------------------------------------------------------------------
 Satoshi Okada                              Intel OEM MFG.
 HIT Corporation Ltd.,                     Tel:+81-3-5796-3033
 2-32-3 kitashinagawa                     Fax:+81-3-5796-3034
 Shinagawa 140-0001                    http://www.hpc.co.jp/
 Tokyo, Japan                              mailto:okada@hpc.co.jp
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------------------------------

Date: Mon, 30 Sep 2002 08:41:41 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Questions about "mini" vs. "optimize"

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> thank you for these very interesting and deep answers! It confirmed to
> me that it is a difficult and potentially long-lasting task, but also

I do NOT think that this a difficult and long-lasting task!!

> As usual, I am setting up a slab calculation in order to try to optimize
> a metal surface with an overlayer of another metal. Thus, based on your

In fact, this is even a quite simple task (unless you have a big x-y supercell)

The easiest way:
a) Calculate (using "optimize") the bulk-lattice parameter of your substrate
metal. This should be fairly quick because of the small 3D unitcell.

b) Use this lattice parameter for you slab calculations (If you use the exp.
latticeparameters, you may get a "stain" in the free c-direction, since the
atoms may want to come closer (or further apart) not due to a surface
effect, but because GGA wants another bulk distance).

c) A metal slab with an overlayer does NOT have just one free parameter,
since also the original surface (and possibly the sub-surface) can relax
too, so there are at least 2-3 free parameters. An "optimize" scheme is
in most cases not very suitable (unless you have a system where ONLY the
overlayer distance needs to be determined). min_lapw works usually very good
for these problems and once you got experience and know how to set the
input in case.inM it should converge pretty quickly to zero forces.
(There are many previous wien-mailings how to monitor *.scf_mini and how
to adjust inM).

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Mon, 30 Sep 2002 09:11:05 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Questions about "mini" vs. "optimize"

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> to my opinion the most annoying feature of WIEN
> in what regards structure relaxation is that
> internal coordinates and lattice parameters have to be
> optimized decoupled, and the optimization of lattice
> parameters is essentially done by hand
> (in a sequence of volume, c/a, c/b, ... runs).

I agree, FULL optimizations of noncubic (tetragonal and hexagonal still
can be done in most cases) structures is BEYOND the present WIEN2k.
(For cubic, tetragonal or hexagonal cells use the standard optimize,
but replace the "run_lapw" by "min_lapw" when you have free internal
coordinates)

> But the possibility to do convenient and automatic
> structure optimization has nothing to do with the speed.
> It can be incorporated in any code where forces and stress
> are available.

That's the point: At present the stress tensor is not available in WIEN.
One can try to calculate it directly (C.Ambrosch-Draxl is working on that), or
one could also do it numerically (from a few E-tot calculations) or using
conjg.gradients.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Mon, 30 Sep 2002 09:29:00 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Problems with Eplot 'coa' plotting

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Eplot in WIEN works well for 'vol' plots but does not seem to work as
> well for 'coa' plots.
>
> My 'coa' energies calculated with x optimize look smooth when plotted with
> an external plotting program, but do not plot in Eplot.

The w2web interface does not yet support the c/a plotting at all.

I think you still could use  "eplot_lapw" from the command line, but
you need a file:  case.analysis

grepline :ene '*coa*scf' 1 > case.analysis

Note: it does not plot a line, but just a series of dots.

PS: It gets the c/a ratio not from the scf file, but from the filename using:

grep $type $file.analysis | grep -v "Analysis generated" | grep -v ":VOL " |\
 sed "s/.*$type//" | tr ":a-z" " " | awk '{print $1 " " $NF}'|\
 cut -c1-6,8-  | tr "_" " " |sort -n

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 30 Sep 2002 09:47:01 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: lapw2 & ifc on LINUX

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I try to make WIEN2k with ifc(Intel Fortran Compiler) on LINUX.
>
> When WIEN2k(lapw2) read a vector data file ( UNIT 10 ),
> the illegal values were inputed for kx_buf,ky_buf,kz_buf
> after about 400byte reading.
>
> SRC_lapw2/read_vec.F:
>      54   IF(myid.EQ.0) THEN
>      55      WRITE(31,205) s,t,z,n,ne,bname
>      56      READ(10) (kx_buf(i),ky_buf(i),kz_buf(i),
> 		i=1,n-(nlo+nlon+nlov)),
>                 (kxlo(i),kylo(i),kzlo(i),i=1,(nlo+nlon+nlov))
>      57   ENDIF

On our system we also use the ifc compiler and have no problems at all.
However, since this compiler is still under development, a lot may depend
on the version of the compiler.

I have one suggestion for testing:
Add in     SRC_lapw2/read_vec.F:

  CHARACTER*3        IPGR

and change the following line:
  IF (myid.EQ.0) READ(10,IOSTAT=ios) s,t,z,bname,n,ne,ipgr

ipgr is written by lapw1/tapewf.F
Usually partial reads ignore longer records and with the next read
the next record is read and everything is fine. Maybe the ifc does not like
this.

PS: Please let me know if this fixes your problem. (The final
solution should be to remove   ipgr from tapewf.F since it is no longer needed.

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 30 Sep 2002 08:56:54 -0400 (EDT)
From: Neme Nnolim <non6886@alizarin.njit.edu>
Subject: Re: [WIEN]: Problems with Eplot 'coa' plotting

====
Neme Nnolim <non6886@alizarin.njit.edu>
submitted the following contribution:
====


>
> The w2web interface does not yet support the c/a plotting at all.
>
> I think you still could use  "eplot_lapw" from the command line, but
> you need a file:  case.analysis
>
> grepline :ene '*coa*scf' 1 > case.analysis
>
> Note: it does not plot a line, but just a series of dots.
>
> PS: It gets the c/a ratio not from the scf file, but from the filename using:
>
> grep $type $file.analysis | grep -v "Analysis generated" | grep -v ":VOL " |\
>  sed "s/.*$type//" | tr ":a-z" " " | awk '{print $1 " " $NF}'|\
>  cut -c1-6,8-  | tr "_" " " |sort -n
>


I wanted to use Eplot for c/a plotting because I thought that Eplot would
carry out a fitting to obtain the shear constant in the same way that the
energy points from a 'vol' plot are fitted to obtain the bulk modulus.

That mess you have up there convinces me that I have to fit the
energy points from c/a calculations myself.


- ------------------------------------------------------------------------------
Neme Okechukwu Nnolim
Department of Materials Science, New Jersey Institute of Technology
Room 302, Tiernan Hall, 161 Warren Street, University Heights
Newark, New Jersey 07102-1982
Tel: (973) 596-8283, FAX: (973) 596-5794
- -------------------------------------------------------------------------------


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------------------------------

Date: Mon, 30 Sep 2002 17:53:14 -0600
From: Pablo de la Mora <delamora@servidor.unam.mx>
Subject: [WIEN]: fixed spin moment

====
Pablo de la Mora <delamora@servidor.unam.mx>
submitted the following contribution:
====

Dear Wien users,
    We are trying to do some fixed spin calculations.
    We had a ferrimagnetic system and we wanted to see how it changed 
when the total moment of the cell increased.
    For the unrestricted system the up and down-spin DOS were quite 
different, one shifted from the other. For the fixed-spin-system the up 
and down DOS were quite similar in shape except for the size, now the 
up-spin and the down-spin were not shifted one from the other.
    Is this expected for these type of calculations?
    Yours

        Pablo de la Mora
   

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------------------------------

Date: Tue, 01 Oct 2002 08:00:18 +0530
From: "R.K.Thapa" <rktt@sancharnet.in>
Subject: Re: [WIEN]: fixed spin moment

====
"R.K.Thapa" <rktt@sancharnet.in>
submitted the following contribution:
====

Dear Dr. de la Mora
I am also one of the beneficiaries of WIEN2K which I received freely on
request to Prof. Karlheinz Schwarz, Vienna Univ. of Technology. But I
regret to inform you that I AM NOT ABLE TO DO ANY WORKs with this code
as I do not possess or have  FORTRAN 90 compiler for linux os.
If possible, may I reuest you kindly to send me this fortran compiler
(PGF90) for linux os for the act of which I shall ever remain grateful
to you.
The reason for this special request  to you is that the cost of this in
dollar is  very high and my institute just turned down my request for
its procurement.
Sorry for all the trouibles and I most humbly apologise.
Sincerely yours
R.K.Thapa
=========================
Condensed Matter Theory Research Group
Department of Physics
Mizoram University
Pachhunga University  College
Aizawl 796001
Miizoram
Tel. (0389)-328044(R), 327095(O)
Fax :(0389)-323491
E-mails :       rktt@sancharnet.in
                    ramkumar_thapa@yahoo.com

================================
Pablo de la Mora wrote:

> ====
> Pablo de la Mora <delamora@servidor.unam.mx>
> submitted the following contribution:
> ====
>
> Dear Wien users,
>     We are trying to do some fixed spin calculations.
>     We had a ferrimagnetic system and we wanted to see how it changed
> when the total moment of the cell increased.
>     For the unrestricted system the up and down-spin DOS were quite
> different, one shifted from the other. For the fixed-spin-system the up
> and down DOS were quite similar in shape except for the size, now the
> up-spin and the down-spin were not shifted one from the other.
>     Is this expected for these type of calculations?
>     Yours
>
>         Pablo de la Mora
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====

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------------------------------

Date: Tue, 01 Oct 2002 08:02:17 +0530
From: "R.K.Thapa" <rktt@sancharnet.in>
Subject: [WIEN]: request if possible

====
"R.K.Thapa" <rktt@sancharnet.in>
submitted the following contribution:
====

Dear Dr.Neme Nnolim
I am also one of the beneficiaries of WIEN2K which I received freely on
request to Prof. Karlheinz Schwarz, Vienna Univ. of Technology. But I
regret to inform you that I AM NOT ABLE TO DO ANY WORKs with this code
as I do not possess or have  FORTRAN 90 compiler for linux os.
If possible, may I reuest you kindly to send me this fortran compiler
(PGF90) for linux os for the act of which I shall ever remain grateful
to you.
The reason for this special request  to you is that the cost of this in
dollar is  very high and my institute just turned down my request for
its procurement.
Sorry for all the trouibles and I most humbly apologise.
Sincerely yours
R.K.Thapa
=========================
Condensed Matter Theory Research Group
Department of Physics
Mizoram University
Pachhunga University  College
Aizawl 796001
Miizoram
Tel. (0389)-328044(R), 327095(O)
Fax :(0389)-323491
E-mails :       rktt@sancharnet.in
                    ramkumar_thapa@yahoo.com



Neme Nnolim wrote:

> ====
> Neme Nnolim <non6886@alizarin.njit.edu>
> submitted the following contribution:
> ====
>
> >
> > The w2web interface does not yet support the c/a plotting at all.
> >
> > I think you still could use  "eplot_lapw" from the command line, but
> > you need a file:  case.analysis
> >
> > grepline :ene '*coa*scf' 1 > case.analysis
> >
> > Note: it does not plot a line, but just a series of dots.
> >
> > PS: It gets the c/a ratio not from the scf file, but from the filename using:
> >
> > grep $type $file.analysis | grep -v "Analysis generated" | grep -v ":VOL " |\
> >  sed "s/.*$type//" | tr ":a-z" " " | awk '{print $1 " " $NF}'|\
> >  cut -c1-6,8-  | tr "_" " " |sort -n
> >
>
> I wanted to use Eplot for c/a plotting because I thought that Eplot would
> carry out a fitting to obtain the shear constant in the same way that the
> energy points from a 'vol' plot are fitted to obtain the bulk modulus.
>
> That mess you have up there convinces me that I have to fit the
> energy points from c/a calculations myself.
>
> ------------------------------------------------------------------------------
> Neme Okechukwu Nnolim
> Department of Materials Science, New Jersey Institute of Technology
> Room 302, Tiernan Hall, 161 Warren Street, University Heights
> Newark, New Jersey 07102-1982
> Tel: (973) 596-8283, FAX: (973) 596-5794
> -------------------------------------------------------------------------------
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====

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------------------------------

Date: Tue,  1 Oct 2002 15:20:11 +1000
From: chen0130@flinders.edu.au
Subject: [WIEN]: band gaps with slabs

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Dear Wien users,

I have two questions about bandstructures for slabs,

(1) With slab bandstructures, I have much more bands than the bulk, and at the
GAMMA point, the bands do not meet at the same energy.

Can anyone tell me how I take the band gap?

Would it be acceptable to take the midpoint of a region and take that from the
midpoint from the higher region (at GAMMA)?

As my system is Li2O, and I have valence bands at Li(1s), O(2s) and O(2p), where
each region has a collection of bands which are not all meeting at the GAMMA
point.

(2) It would make sense, that as the slab gets thicker, it becomes closer to the
bulk, yet the bulk is a only 6 bands, whereas a 21 layer slab is 126 (occupied)
bands...

My understanding at this stage is that a bigger cell with more atoms will have
more bands, is that all there is to it?

It seems that the overall electronic structure should not be affected, as the 
'really thick' slab begins to describe something similar to the bulk...


Thanks for you time!

Cheng 


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------------------------------

Date: Tue, 1 Oct 2002 09:14:16 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: request if possible

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> regret to inform you that I AM NOT ABLE TO DO ANY WORKs with this code
> as I do not possess or have  FORTRAN 90 compiler for linux os.
> If possible, may I reuest you kindly to send me this fortran compiler
> (PGF90) for linux os for the act of which I shall ever remain grateful
> to you.

I do not think that one can send you (legally) the pgi f90 compiler.
However, you have two choices:
a) On the download page of WIEN2k we provide also the executables. When
you download them, you do not need a compiler at all!!! (but cannot change the
code)
b) There is a free f90 compiler from intel. You con download (free of charge)
the "unsupported" ifc 6.0 from there homepage.

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 1 Oct 2002 11:23:34 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: band gaps with slabs

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

Your questions about slabs are quite basic and elementary:

Suppose you create a cell with two layers (but no vacuum for the moment). Then
you have "doubled" your primitive unit cell. A doubled real space cell leads
to a smaller reciprocal cell and since you have twice as many atoms you MUST
find twice as many bands. In this simple example, the bands at Gamma (in the
supercell) reflect the original states at gamma (of the small unit cell)
AND the "backfolded" states at the "Z" point of the original cell (where
I suppose that you doubled the z-direction).

I hope the principle is clear by now.

When you now take a thicker slab, you get backfolding along the normal of
your surface (i.e. for a (001) surface you get (at Gamma) all the eigenvalues
from the original gamma-Z line (depending on the number of layers with a
finer or coarser k-grid along this direction).

Of course the vacuum "disturbs" these states to some extend, so they will
not be exactly the backfolded states, but very close to them. In addition
so called "surface states" can appear, which have nothing in common with the
"bulk states".

With this knowledge you should be able to answer your questions alone.

> I have two questions about bandstructures for slabs,
>
> (1) With slab bandstructures, I have much more bands than the bulk, and at the
> GAMMA point, the bands do not meet at the same energy.
>



                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 1 Oct 2002 11:43:10 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: fixed spin moment

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>     We are trying to do some fixed spin calculations.
>     We had a ferrimagnetic system and we wanted to see how it changed
> when the total moment of the cell increased.
>     For the unrestricted system the up and down-spin DOS were quite
> different, one shifted from the other. For the fixed-spin-system the up
> and down DOS were quite similar in shape except for the size, now the
> up-spin and the down-spin were not shifted one from the other.

I guess you misinterprete your results. The sequence of a FSM calculation
is:

x lapw1 -up
cp vector_up vector_dn
cp in2_up in2
x lapw2 -up

x lapw1 -dn
cp vector_dn vector_up
cp in2_dn in2
x lapw2 -dn

Thus at the end of a FSM scf cycle, all you have are the spin-dn vectors
and it does not matter wether you do    x lapw2 -up -qtl   or x lapw2 -dn -qtl,
you get the same qtl-file (and thus DOS)

You must have both vector files for the DOS: i.e. run

x lapw1 -up   (now you have proper spin-up and dn vectors) and

x lapw2 -up -qtl
x lapw2 -dn -qtl

eventually you should also correct for the differences in EF for up/dn
as found in the scf file.

Regards



                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 1 Oct 2002 15:41:48 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: fixed spin moment

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>     We are trying to do some fixed spin calculations.
>     We had a ferrimagnetic system and we wanted to see how it changed
> when the total moment of the cell increased.
>     For the unrestricted system the up and down-spin DOS were quite
> different, one shifted from the other.
> For the fixed-spin-system the up
> and down DOS were quite similar in shape except for the size, now the
> up-spin and the down-spin were not shifted one from the other.
>     Is this expected for these type of calculations?
In one side, splitting of up-DOS and dn-DOS refers to or depends on
correlation. For example in strongly correlated fcc-Gd in its metallic state
the distance between higher (unoccupied) 4f band and lower (occupied) 4f
band within local spin density approximation is 5.5 eV. For fcc-Sm it is
around 0.5 eV, which is much smaller than Hubbard U shifted between up and
down DOSs. On the other hand, within LSDA up and down spin densities will be
different if number of up electrons are not equal to number of down
electrons, which is an indication of magnetic moment. You have nicely
touched two points together. As far as I know in wien2k we can impose zero
magnetic moment even in a spin polarized calculation, but I am not sure if
fixing magnetic moment to a non zero value is also possible. If you don't
think so, please show us how we can do it: changing or increasing magnetic
moment gradually from paramagnetically zero value to the highest value in
its fully ferromagnetic situation.
Your,
S. Jalali.

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------------------------------

Date: Tue, 1 Oct 2002 16:04:41 +0200
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: [WIEN]: lxdos - problems with lapw2 and tetra

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Dear wien users,

I am trying to use wien2k with the parameter lxdos = 3.  I recompiled tetra
and lapw2 after setting this parameter to 3 in param.inc resp. modules.F.
However, I have not succeeded to make either of them function properly.

* When running x lapw2 -qtl after SCF, the program terminates normally and
produces a qtl-file with the correct format for ISPLIT =88 or 99.  However,
the xdos-matrix is equal to zero!

* Tetra on the other hand works fine with lxdos = 1, but seems to fail
regardless the value of ISPLIT when the program is recompiled with lxdos =
3.  I get a core dump - segmentation fault.  Watching case.outputt and
inserting some test lines in tetra.f and arbdos.f, I saw that all statements
up to the invocation of arbdos are executed in tetra, but the routine arbdos
never gets started (a test line in the beginning of the program is never
printed).  The routine has been changed w.r.t. WIEN97 (extra arguments of
which I do not know the meaning, and different declaration of variables of
course).  Lxdos is not used explicitly, but determines the size of certain
objects.

The cases I have used for testing are simple diamond and graphite - nothing
excentric, really.

Discovering small changes in the WIEN2k-code w.r.t. WIEN97 I learned that
someone has obviously been working on the lxdos3-case, so I hope this
someone will be able to help me and maybe bring to my attention new elements
that have to be considered when performing this kind of calculation.  Please
do not hesitate to ask for additional information if necessary.

Kind regards,

Kevin Jorissen
EMAT - University of Antwerp
kevin.jorissen@ua.ac.be

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------------------------------

Date: Tue, 1 Oct 2002 16:41:31 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: lxdos - problems with lapw2 and tetra

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I am trying to use wien2k with the parameter lxdos = 3.  I recompiled tetra
> and lapw2 after setting this parameter to 3 in param.inc resp. modules.F.
> However, I have not succeeded to make either of them function properly.

Have you updated to the latest version from the web ? Older WIEN2k versions
had a bug for lxdos=3.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 1 Oct 2002 08:00:38 -0700 (PDT)
From: sayede adlane <dft22000@yahoo.fr>
Subject: Re: [WIEN]: Problems with Eplot 'coa' plotting

====
sayede adlane <dft22000@yahoo.fr>
submitted the following contribution:
====

- --0-1406971704-1033484438=:7953
Content-Type: text/plain; charset=us-ascii
Content-Disposition: inline

Here is simple script that I use to plot c/a or b/a vs
Energy (plus polyfiting 4th order).
To use it just type :
>Enplot casename
Hope to help you !

Yours A. Sayede.

- --- Peter Blaha <pblaha@theochem.tuwien.ac.at> wrote:
> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> > Eplot in WIEN works well for 'vol' plots but does
> not seem to work as
> > well for 'coa' plots.
> >
> > My 'coa' energies calculated with x optimize look
> smooth when plotted with
> > an external plotting program, but do not plot in
> Eplot.
> 
> The w2web interface does not yet support the c/a
> plotting at all.
> 
> I think you still could use  "eplot_lapw" from the
> command line, but
> you need a file:  case.analysis
> 
> grepline :ene '*coa*scf' 1 > case.analysis
> 
> Note: it does not plot a line, but just a series of
> dots.
> 
> PS: It gets the c/a ratio not from the scf file, but
> from the filename using:
> 
> grep $type $file.analysis | grep -v "Analysis
> generated" | grep -v ":VOL " |\
>  sed "s/.*$type//" | tr ":a-z" " " | awk '{print $1
> " " $NF}'|\
>  cut -c1-6,8-  | tr "_" " " |sort -n
> 
>                                       P.Blaha
>
- --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna,
> A-1060 Vienna
> Phone: +43-1-58801-15671             FAX:
> +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
> http://info.tuwien.ac.at/theochem/
>
- --------------------------------------------------------------------------
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====



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- --0-1406971704-1033484438=:7953
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- --0-1406971704-1033484438=:7953--
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------------------------------

Date: Tue, 1 Oct 2002 17:29:40 +0200
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re:Fw: [WIEN]: lxdos - problems with lapw2 and tetra

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Dear Mr. Blaha,

the VERSION-file in my wien2k-directory reads
WIEN2k_02 (Release 27/05/2002)
If I have not made any mistake, it has, however, been downloaded quite
recently.  I will download the latest version in any case and install it,
and contact you again if problems persist.

Thank you,

Kevin Jorissen
EMAT - University of Antwerp
kevin.jorissen@ua.ac.be

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------------------------------

Date: Tue, 01 Oct 2002 23:55:42 -0400 (EDT)
From: Neme Nnolim <non6886@alizarin.njit.edu>
Subject: Re: [WIEN]: Problems with Eplot 'coa' plotting

====
Neme Nnolim <non6886@alizarin.njit.edu>
submitted the following contribution:
====


Thanks for the script, Adlane.

I can't wait to try it.

Regards,

Neme

On Tue, 1 Oct 2002, sayede adlane wrote:

> Date: Tue, 1 Oct 2002 08:00:38 -0700 (PDT)
> From: sayede adlane <dft22000@yahoo.fr>
> Reply-To: wien@zeus.theochem.tuwien.ac.at
> To: wien@zeus.theochem.tuwien.ac.at
> Subject: Re: [WIEN]: Problems with Eplot 'coa' plotting
>
> Here is simple script that I use to plot c/a or b/a vs
> Energy (plus polyfiting 4th order).
> To use it just type :
> >Enplot casename
> Hope to help you !
>
> Yours A. Sayede.

- ------------------------------------------------------------------------------
Neme Okechukwu Nnolim
Department of Materials Science, New Jersey Institute of Technology
Room 302, Tiernan Hall, 161 Warren Street, University Heights
Newark, New Jersey 07102-1982
Tel: (973) 596-8283, FAX: (973) 596-5794
- -------------------------------------------------------------------------------


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------------------------------

Date: Wed, 2 Oct 2002 09:59:27 +0200
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: [WIEN]: lxdos3 - lapw2 - tetra

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Installing the newest version of WIEN2k (VERSION file still reads 'released
27/5' by the way) didn't change anything, I'm sorry to say.

Thanks for all suggestions,

Kevin Jorissen
EMAT, University of Antwerp
kevin.jorissen@ua.ac.be


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------------------------------

Date: Thu, 3 Oct 2002 14:34:51 +0200
From: "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: [WIEN]: sgroup

====
"Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====


Dear Wien users,

It might be due to my limited knowledge on crystallography, but I see
strange behaviour in sgroup. Using the GUI, I want to create group nr. 225
(Fm-3m), with the atoms on position 8c (point group m-3m). According to
tables, these should have positions 1/4,1/4,1/4 and 1/4,1/4,3/4. In the GUI,
I should enter only 1 position, I choose the 1/4,1/4,1/4. Then, after saving
the structure, it returns two positions: 1/4,1/4,1/4 and the unexpected
3/4,3/4,3/4. So far, I could assume that the GUI uses another setting for
this structure, so I assume everything could still be all right and proceed.
However, sgroup protests :

warning: !!! Bravais lattice has changed.

and recommends group nr. 221 (P m -3 m). If I neglect this warning and go to
symmetry, it asks to shift the origin, and after that the original
multiplicity of 2 becomes 1.

When I make the struct-file manually, with the two positions according to
the tables :

F   LATTICE,NONEQUIV. ATOMS: 1225_Fm-3m
MODE OF CALC=RELA unit=bohr
  7.558900  7.558900  7.558900 90.000000 90.000000 90.000000
ATOM= -1: X=0.25000000 Y=0.25000000 Z=0.25000000
          MULT= 2          ISPLIT= 8
ATOM= -1:X= 0.25000000 Y=0.25000000 Z=0.75000000
Na         NPT=  781  R0=0.00010000 RMT=    1.8000   Z: 11.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
   0      NUMBER OF SYMMETRY OPERATIONS

then the same behaviour happens.

Something similar happens with the most general 192l (1.) position in this
group: the GUI finds only 24 instead of 48 positions, sgroup correctly
detects the group, but symmetry detects as point group m instead of 1
(actually, it has made 96k instead of 192l). Similar behaviour is seen in
group nr. 229 with the 6b position.

I am using the latest Wien version.

Is this a bug, or should I update my crystallography knowledge ?

Stefaan

- ----------------------------------------------------------------------------
- --
Stefaan Cottenier
Instituut voor Kern- en Stralingsfysica
K.U.Leuven
Celestijnenlaan 200 D  tel: + 32 16 32 71 45
B-3001 Leuven   fax: + 32 16 32 79 85
Belgium    e-mail: Stefaan.Cottenier@fys.kuleuven.ac.be

http://www.fys.kuleuven.ac.be/iks/nvsf/nvsf.html
- ----------------------------------------------------------------------------
- --

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------------------------------

End of wien-digest V2002 #37
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #38
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
Errors-To: owner-wien-digest@theochem.tuwien.ac.at
Precedence: bulk


wien-digest         Friday, October 11 2002         Volume 2002 : Number 038




----------------------------------------------------------------------

Date: Thu, 3 Oct 2002 15:16:27 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: case.int file

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

I try to calculate DOS, but I did not found my case.int file when I found
the following files:

tic.in0              tic.in2_st           tic.inm_restart_st
tic.in0_st           tic.in2_sy           tic.inm_st
tic.in1              tic.in5              tic.inso
tic.in1_st           tic.inc              tic.inst
tic.in2              tic.inc_st
tic.in2_ls           tic.inm

What should I do to make it work?

Thank you in adavance!


Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Thu, 3 Oct 2002 16:43:15 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: case.int file

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

Never mind the following question, case.int file only can be produced
after x lapw -qtl is run.

Best wishes!



Dear All:

I try to calculate DOS, but I did not found my case.int file when I found
the following files:

tic.in0              tic.in2_st           tic.inm_restart_st
tic.in0_st           tic.in2_sy           tic.inm_st
tic.in1              tic.in5              tic.inso
tic.in1_st           tic.inc              tic.inst
tic.in2              tic.inc_st
tic.in2_ls           tic.inm

What should I do to make it work?

Thank you in adavance!


Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395


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------------------------------

Date: Thu, 03 Oct 2002 17:06:39 -0600
From: Pablo de la Mora <pm@fciencias.unam.mx>
Subject: Re: [WIEN]: fixed spin moment

====
Pablo de la Mora <pm@fciencias.unam.mx>
submitted the following contribution:
====


- --------------080903050806000100030000
Content-Type: text/plain; charset=us-ascii; format=flowed
Content-Transfer-Encoding: 7bit



Peter Blaha wrote:

>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
>>    We are trying to do some fixed spin calculations.
>>    We had a ferrimagnetic system and we wanted to see how it changed
>>when the total moment of the cell increased.
>>    For the unrestricted system the up and down-spin DOS were quite
>>different, one shifted from the other. For the fixed-spin-system the up
>>and down DOS were quite similar in shape except for the size, now the
>>up-spin and the down-spin were not shifted one from the other.
>>
>
>I guess you misinterprete your results. The sequence of a FSM calculation
>is:
>
>x lapw1 -up
>cp vector_up vector_dn
>cp in2_up in2
>x lapw2 -up
>
>x lapw1 -dn
>cp vector_dn vector_up
>cp in2_dn in2
>x lapw2 -dn
>
>Thus at the end of a FSM scf cycle, all you have are the spin-dn vectors
>and it does not matter wether you do    x lapw2 -up -qtl   or x lapw2 -dn -qtl,
>you get the same qtl-file (and thus DOS)
>
>You must have both vector files for the DOS: i.e. run
>
>x lapw1 -up   (now you have proper spin-up and dn vectors) and
>
>x lapw2 -up -qtl
>x lapw2 -dn -qtl
>
>eventually you should also correct for the differences in EF for up/dn
>as found in the scf file.
>
>Regards
>
>
>
>                                      P.Blaha
>
Thank you very much, now the calculations are going well

- --------------080903050806000100030000
Content-Type: text/html; charset=us-ascii
Content-Transfer-Encoding: 7bit

<html>
<head>
</head>
<body>
<br>
<br>
Peter Blaha wrote:<br>
<blockquote type="cite" cite="mid:Pine.LNX.4.33.0210011137130.22309-100000@susi.theochem.tuwien.ac.at">
  <pre wrap="">====<br>Peter Blaha <a class="moz-txt-link-rfc2396E" href="mailto:pblaha@theochem.tuwien.ac.at">&lt;pblaha@theochem.tuwien.ac.at&gt;</a><br>submitted the following contribution:<br>====<br><br></pre>
  <blockquote type="cite">
    <pre wrap="">    We are trying to do some fixed spin calculations.<br>    We had a ferrimagnetic system and we wanted to see how it changed<br>when the total moment of the cell increased.<br>    For the unrestricted system the up and down-spin DOS were quite<br>different, one shifted from the other. For the fixed-spin-system the up<br>and down DOS were quite similar in shape except for the size, now the<br>up-spin and the down-spin were not shifted one from the other.<br></pre>
    </blockquote>
    <pre wrap=""><!----><br>I guess you misinterprete your results. The sequence of a FSM calculation<br>is:<br><br>x lapw1 -up<br>cp vector_up vector_dn<br>cp in2_up in2<br>x lapw2 -up<br><br>x lapw1 -dn<br>cp vector_dn vector_up<br>cp in2_dn in2<br>x lapw2 -dn<br><br>Thus at the end of a FSM scf cycle, all you have are the spin-dn vectors<br>and it does not matter wether you do    x lapw2 -up -qtl   or x lapw2 -dn -qtl,<br>you get the same qtl-file (and thus DOS)<br><br>You must have both vector files for the DOS: i.e. run<br><br>x lapw1 -up   (now you have proper spin-up and dn vectors) and<br><br>x lapw2 -up -qtl<br>x lapw2 -dn -qtl<br><br>eventually you should also correct for the differences in EF for up/dn<br>as found in the scf file.<br><br>Regards<br><br><br><br>                                      P.Blaha</pre>
    </blockquote>
Thank you very much, now the calculations are going well<br>
    </body>
    </html>

- --------------080903050806000100030000--

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------------------------------

Date: Fri,  4 Oct 2002 15:47:23 +1000
From: chen0130@flinders.edu.au
Subject: Re: [WIEN]: band gaps with slabs

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Thanks for your advice Prof Blaha, I am wondering if you could direct me to some
help about backfolding, and back folded states...i have not heard about these
before.

I am wondering then, to take a band gap from the bandstructure of a slab may not
be a trivial task?

Thanks for your help!

Cheng


Quoting Peter Blaha <pblaha@theochem.tuwien.ac.at>:

> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> Your questions about slabs are quite basic and elementary:
> 
> Suppose you create a cell with two layers (but no vacuum for the moment).
> Then
> you have "doubled" your primitive unit cell. A doubled real space cell
> leads
> to a smaller reciprocal cell and since you have twice as many atoms you
> MUST
> find twice as many bands. In this simple example, the bands at Gamma (in
> the
> supercell) reflect the original states at gamma (of the small unit cell)
> AND the "backfolded" states at the "Z" point of the original cell (where
> I suppose that you doubled the z-direction).
> 
> I hope the principle is clear by now.
> 
> When you now take a thicker slab, you get backfolding along the normal of
> your surface (i.e. for a (001) surface you get (at Gamma) all the
> eigenvalues
> from the original gamma-Z line (depending on the number of layers with a
> finer or coarser k-grid along this direction).
> 
> Of course the vacuum "disturbs" these states to some extend, so they will
> not be exactly the backfolded states, but very close to them. In addition
> so called "surface states" can appear, which have nothing in common with
> the
> "bulk states".
> 
> With this knowledge you should be able to answer your questions alone.
> 
> > I have two questions about bandstructures for slabs,
> >
> > (1) With slab bandstructures, I have much more bands than the bulk, and at
> the
> > GAMMA point, the bands do not meet at the same energy.
> >
> 
> 
> 
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
> http://info.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 
> 



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------------------------------

Date: Fri, 4 Oct 2002 08:04:01 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: case.int file

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I try to calculate DOS, but I did not found my case.int file when I found
> the following files:
>
> tic.in0              tic.in2_st           tic.inm_restart_st
> tic.in0_st           tic.in2_sy           tic.inm_st
> tic.in1              tic.in5              tic.inso
> tic.in1_st           tic.inc              tic.inst
> tic.in2              tic.inc_st
> tic.in2_ls           tic.inm
>
> What should I do to make it work?

Go back to the usersguide, chapter  getting started.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Fri, 4 Oct 2002 08:29:32 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: band gaps with slabs

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Thanks for your advice Prof Blaha, I am wondering if you could direct me to some
> help about backfolding, and back folded states...i have not heard about these
> before.

Trival example for a primitive lattice:
You have a lattice parameter a, so the reciprocal space length is 2pi/a.
Thus your "X" point has the coordinates pi/a, or along the "delta"
line the 1/3 and 2/3 points have the coordinates  pi/3a and 2pi/3a.

Now you make a slab (supercell) with 6a. Thus your reciprocal lattice vector
has a length of 2pi/6a. Therefore the Gamma point of the supercell has all
the k-points of  K=0, pi/3a, 2pi/3a and pi/a which corresponds the four
points mentioned above. In addition, since 1/3 and 2/3 points are inside the
BZ, their "weight" is twice that of Gamma or X, so you also find in your slab
those eigenvalues twice (leading to the factor of 6 in the number of
eigenvalues).
(Try it graphically in one dimension and it should be clear.)

> I am wondering then, to take a band gap from the bandstructure of a slab may not
> be a trivial task?

It is trivial! Still the bandgap is between the highest occupied energy and the
lowest unoccupied! Plot a bandstructure or a DOS, or simply look into
case.output2 to find the band-limits.

What is NOT so trivial is to find out from a slab calculation across which
k-points of the bulk system the gap is ("direct-indirect" ?)


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Fri, 4 Oct 2002 08:57:13 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: sgroup

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> It might be due to my limited knowledge on crystallography, but I see
> strange behaviour in sgroup. Using the GUI, I want to create group nr. 225
> (Fm-3m), with the atoms on position 8c (point group m-3m). According to
> tables, these should have positions 1/4,1/4,1/4 and 1/4,1/4,3/4. In the GUI,
> I should enter only 1 position, I choose the 1/4,1/4,1/4. Then, after saving
> the structure, it returns two positions: 1/4,1/4,1/4 and the unexpected
> 3/4,3/4,3/4. So far, I could assume that the GUI uses another setting for
> this structure, so I assume everything could still be all right and proceed.

Yes, the positions (1/4,1/4,3/4) and (3/4,3/4,3/4) are of course the same,
since they differ only by a "centering" of (1/2,1/2,0).


> However, sgroup protests :
>
> warning: !!! Bravais lattice has changed.
>
> and recommends group nr. 221 (P m -3 m). If I neglect this warning and go to
> symmetry, it asks to shift the origin, and after that the original
> multiplicity of 2 becomes 1.

Just make a small drawing of your proposed unit cell. In the FCC !! lattice
with the 2 position (1/4,1/4,1/4 and 1/4,1/4,3/4) add all "centerings",
i.e. add all (1/2,1/2,0)+permutations. You will see that you can describe
this with a smaller Primitive!! unit cell of just a/2 lattice parameter
and just one atom (at (0,0,0)).

>
> When I make the struct-file manually, with the two positions according to
> the tables :
>
> F   LATTICE,NONEQUIV. ATOMS: 1225_Fm-3m
> MODE OF CALC=RELA unit=bohr
>   7.558900  7.558900  7.558900 90.000000 90.000000 90.000000
> ATOM= -1: X=0.25000000 Y=0.25000000 Z=0.25000000
>           MULT= 2          ISPLIT= 8
> ATOM= -1:X= 0.25000000 Y=0.25000000 Z=0.75000000
> Na         NPT=  781  R0=0.00010000 RMT=    1.8000   Z: 11.0
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
>    0      NUMBER OF SYMMETRY OPERATIONS
>
> then the same behaviour happens.
>
> Something similar happens with the most general 192l (1.) position in this
> group: the GUI finds only 24 instead of 48 positions, sgroup correctly
> detects the group, but symmetry detects as point group m instead of 1
> (actually, it has made 96k instead of 192l). Similar behaviour is seen in
> group nr. 229 with the 6b position.
>
> I am using the latest Wien version.
>
> Is this a bug, or should I update my crystallography knowledge ?

If you select a particular spacegroup X, but occupy just one position
(sometimes even a few) it MAY happen that this corresponds actually to
a smaller cell with a different spacegroup Y.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Fri, 4 Oct 2002 12:48:00 +0200
From: "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: sgroup

====
"Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
>
> If you select a particular spacegroup X, but occupy just one position
> (sometimes even a few) it MAY happen that this corresponds actually to
> a smaller cell with a different spacegroup Y.

Indeed, my three different examples can be traced back to the same wrong
assumption that every spacegroup can be made for any single one of its
special positions. If I repeat the example nr. 225 and put an atom at
position 8c (-43m) AND one at 4a (m-3m), then sgroup and symmetry find the
expected information.

Thanks, that's clear now.

Stefaan

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------------------------------

Date: Fri, 4 Oct 2002 17:20:40 -0500 (GMT)
From: "Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
Subject: [WIEN]: AFM and FM calculations

====
"Dr. Sharat  Chandra" <sharat@igcar.ernet.in>
submitted the following contribution:
====

Hi all

I am trying to calculate the properties of LaMnO3 based compounds in which
La has been doped by Ca and Mn doped by various electron and hole dopants
like Zr, Ru, Al, Fe etc. The space group for LaMnO3 is 62 (Pnma). The
lattice constants are a=5.679 b=7.703 c=5.541 and a=b=g=90, where a b and
c can change on doping. LaMnO3 ground state is antiferromagnetic which on
becomes ferromagnetic when La is doped by >25% Ca. This forms the base
compound for our experiments. For calculating the properties of this
compound, I have constructed a supercell (1X3X1 cells) and replaced La
atoms by Ca. For this configuration, the spacegroup detects triclinic (P
1) space group and symmetry detects orthorhombic system.

My question is that for undoped LaMnO3 I have to flip the Mn spins and
make the up and down spins of La and O equal for getting the proper anti-
ferromagnetic orientation. Do I have to make the up and down spins of La
Ca and O equal for LaCaMnO3 also (which is ferromagnetic)? 

Also, for band structure calculations, should the band structure be
calculated by using the Orthorhombic critical points (G -> Z -> T -> Y ->
G -> X -> S -> R -> U) or triclinic critical points?

Regards
Sharat Chandra


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Date: Fri, 4 Oct 2002 22:21:07 +0800
From: "yulihua-wuhan" <yulihua-wuhan@sohu.com>
Subject: [WIEN]: Ref of LDA

====
"yulihua-wuhan" <yulihua-wuhan@sohu.com>
submitted the following contribution:
====

Dear Wien2k Users and developers:
                In the case.in0 , i only find:
                                       5.......CA-LDA
                                       13.....PBE-GGA
                                       14.....PW2-GGA
                               about the XC potential
              so what is the exact reference of the LDA?
 
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Date: Fri, 4 Oct 2002 17:38:15 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Ref of LDA

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Dear Wien2k Users and developers:
>                 In the case.in0 , i only find:
>                                        5.......CA-LDA
>                                        13.....PBE-GGA
>                                        14.....PW2-GGA
>                                about the XC potential
>               so what is the exact reference of the LDA?

It's in the UG: Perdew-Wang 1992

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Fri, 4 Oct 2002 17:40:38 +0200
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: Ref of LDA

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

5    :   Perdew and Wang 92, reparameterization of Ceperly-Alder data, the
recommended LDA option

kind regards,

Kevin Jorissen
EMAT, University of Antwerp

as stated in the UG (section about lapw0)
- ----- Original Message -----
From: "yulihua-wuhan" <yulihua-wuhan@sohu.com>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Friday, October 04, 2002 4:21 PM
Subject: [WIEN]: Ref of LDA


> ====
> "yulihua-wuhan" <yulihua-wuhan@sohu.com>
> submitted the following contribution:
> ====
>
> Dear Wien2k Users and developers:
>                 In the case.in0 , i only find:
>                                        5.......CA-LDA
>                                        13.....PBE-GGA
>                                        14.....PW2-GGA
>                                about the XC potential
>               so what is the exact reference of the LDA?
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

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Date: Fri, 4 Oct 2002 17:29:45 +0100 (BST)
From: Dave Pankhurst <david.pankhurst@materials.oxford.ac.uk>
Subject: [WIEN]: error in init_lapw

====
Dave Pankhurst <david.pankhurst@materials.oxford.ac.uk>
submitted the following contribution:
====

Dear wien users,

When sgroup finds a new structure you are asked if you would like to
continue or edit case.struct_sgroup.  At the moment, instead of doing
this, the script pops up the case.struct file when you type "y".  I
presume this is a mistake and line 142 should be:

    editor $file.struct_sgroup

rather than

    editor $file.struct

Is this the desired behaviour?

best regards,

	Dave Pankhurst

+---------------------------------+------------------------------------+
| Dr David Pankhurst,             | Tel : +44 1865 283325/283326       |
| Department of Materials,        | Fax : +44 1865 273789              |    
| University of Oxford,           |                                    |
| Parks Road, Oxford OX1 3PH, UK  | david.pankhurst@materials.ox.ac.uk |
+---------------------------------+------------------------------------+

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Date: Sat, 5 Oct 2002 22:07:18 +0800
From: "yulihua-wuhan" <yulihua-wuhan@sohu.com>
Subject: [WIEN]: semi-core states and valence & klist

====
"yulihua-wuhan" <yulihua-wuhan@sohu.com>
submitted the following contribution:
====

Dear Wien2k Users and developers:

   Firstly thanks P. Blaha and K.Jorissen, i have seen the Ref of LDA in the UG.
   Now i have a new question about treating the semi-core states and valence states. I am calculating the band structure of the Ag2PdO2 (semiconductor) using the default choices.
   the case.inc is:
    9 0.00     NUMBER OF ORBITALS (EXCLUDING SPIN), SHIFT
1,-1,2               ( N,KAPPA,OCCUP)
2,-1,2               ( N,KAPPA,OCCUP)
2, 1,2               ( N,KAPPA,OCCUP)
2,-2,4               ( N,KAPPA,OCCUP)
3,-1,2               ( N,KAPPA,OCCUP)
3, 1,2               ( N,KAPPA,OCCUP)
3,-2,4               ( N,KAPPA,OCCUP)
3, 2,4               ( N,KAPPA,OCCUP)
3,-3,6               ( N,KAPPA,OCCUP)
 9 0.00     NUMBER OF ORBITALS (EXCLUDING SPIN), SHIFT
1,-1,2               ( N,KAPPA,OCCUP)
2,-1,2               ( N,KAPPA,OCCUP)
2, 1,2               ( N,KAPPA,OCCUP)
2,-2,4               ( N,KAPPA,OCCUP)
3,-1,2               ( N,KAPPA,OCCUP)
3, 1,2               ( N,KAPPA,OCCUP)
3,-2,4               ( N,KAPPA,OCCUP)
3, 2,4               ( N,KAPPA,OCCUP)
3,-3,6               ( N,KAPPA,OCCUP)
 1 0.00     NUMBER OF ORBITALS (EXCLUDING SPIN), SHIFT
1,-1,2               ( N,KAPPA,OCCUP)
 0 

so i think Ag and Pd core states are (1s2s2p3s3p3d), O core states is (1s).

The case.inst is:
Ag 
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Pd 
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,2.0  N
5,-1,1.0  N
5,-1,0.0  N
O 
He 3 5
2,-1,1.0  N
2,-1,1.0  N
2, 1,1.0  N
2, 1,1.0  N
2,-2,2.0  N
2,-2,0.0  N
****     End of Input
****     End of Input

so i think Ag and Pd valence states are (4d5s), O valence states are (2s2p).

The case.in1 is:
WFFIL        (WFPRI, SUPWF)
  8.50       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  0.30    5  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global APW/LAPW)
 0    0.30      0.000 CONT 0
 0   -6.68      0.005 STOP 0
 1    0.30      0.000 CONT 0
 1   -3.88      0.005 STOP 0
 2    0.30      0.010 CONT 1
  0.30    5  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global APW/LAPW)
 0    0.30      0.000 CONT 0
 0   -6.23      0.005 STOP 0
 1    0.30      0.000 CONT 0
 1   -3.62      0.005 STOP 0
 2    0.30      0.010 CONT 1
  0.30    3  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global APW/LAPW)
 0   -1.55      0.010 CONT 0  ------> 3s  LAPW?
 0    0.30      0.000 CONT 0   ------> 2s  LOs?
 1    0.30      0.000 CONT 1   ------>2p APW+lo
K-VECTORS FROM UNIT:5   -8.0       2.5      emin/emax window

so according to the UG and the step-by-step course of S. Cottenier, i think Ag and Pd  (4s4p) are semi-core states treated with LOs, and add 5p to the valence states (unoccupied) . But for the O atoms, the UG said that " If the same l value is specified twice, ......The first energy is used for the usual LAPW's and the second for the LOs", so i think 2s(semi-core) is treated with LOs, and add 3s(unoccupied) to the valence states. But the energy( -1.55Ry) for 3s <  (0.30Ry) for 2s. And in the case.inst O (2s2p) is valence states.  
                       Where is my errors? 

I use -in1new 5 to get a new case.in1:

WFFIL        (WFPRI, SUPWF)
  7.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
 .28213   5   0      global e-param with N other choices, napw 
 0    0.290     0.000 CONT 0 
 0   -6.090     0.005 CONT 0 
 1    0.308     0.000 CONT 0 
 1   -3.411     0.005 CONT 0 
 2    0.353     0.010 CONT 1 
 .28213   5   0      global e-param with N other choices, napw 
 0    0.298     0.000 CONT 0 
 0   -5.616     0.005 CONT 0 
 1    0.292     0.000 CONT 0 
 1   -3.120     0.005 CONT 0 
 2    0.385     0.010 CONT 1 
 .28213   3   0      global e-param with N other choices, napw 
 0    0.342     0.000 CONT 0   ----->3s LAPW ?
 0   -0.775     0.010 CONT 0   ----->2s LOs ?
 1    0.283     0.000 CONT 1 
K-VECTORS FROM UNIT:5   -8.0       3.5      emin/emax window
 
so the energy (0.342Ry) for 3s, (-0.775Ry) for 2s.This is reasonable. The calculation results of two cases are almost same. 
so i think in the first one:
0   -1.55      0.010 CONT 0  ------> 2s  LOs?  O 2s is semi-core states, not the valence states specified in the case.inst.
 0    0.30      0.000 CONT 0   ------> 3s  LAPW?
Am i right?

And another question about the klist:
 If the k-points specified in the klist is all in the IBZ, and if only these k-points in the IBZ will be calculated while other is not need to be calculated?

At last, In my calculation, like the usual situation, the band gap is underestimated for three versions of the XC potential and LAPW, APW+lo and mixed basis set. So i suggest the developers add the GW quasi-particle correction to this code. Of course maybe that is not need because we obtain many information about the electronic structure.
                                                                                                                  
  Best regards for everyone!                                                                                             Yulihua









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Date: Sat, 5 Oct 2002 21:45:23 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: semi-core states and valence & klist

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

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> I am calculating the band structure of the Ag2PdO2 (semiconductor) =
using the default choices.
>    the case.inc is:
>     9 0.00     NUMBER OF ORBITALS (EXCLUDING SPIN), SHIFT
> 1,-1,2               ( N,KAPPA,OCCUP)
> 2,-1,2               ( N,KAPPA,OCCUP)
> 2, 1,2               ( N,KAPPA,OCCUP)
> 2,-2,4               ( N,KAPPA,OCCUP)
> 3,-1,2               ( N,KAPPA,OCCUP)
> 3, 1,2               ( N,KAPPA,OCCUP)
> 3,-2,4               ( N,KAPPA,OCCUP)
> 3, 2,4               ( N,KAPPA,OCCUP)
> 3,-3,6               ( N,KAPPA,OCCUP)
...

> so i think Ag and Pd core states are (1s2s2p3s3p3d), O core states is =
(1s).



You are right about core states.


> The case.inst is:
> Ag=20
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N

...
> so i think Ag and Pd valence states are (4d5s), O valence states are =
(2s2p).



Although you have also correctly distinguished valence states of O,  =
valence states of Ag and Pd are 4s^2 4p^6 4d^(10) 5s^1. Valence =
(valence+semi core) states are separated from core states selecting =
separation energy (S.E.) in wien2k during initialization procedure. =
Based on your chosen S.E. configurations of your atoms look like:
Ag: [Ar 3d^(10)]  4s^2 4p^6 4d^(10) 5s^1

Pd: [Ar 3d^(10)]  4s^2 4p^6 4d^8 5s^2

O: [He] 2s^2 2p^4

which the ones for Ag and Pd appear different from following standard =
electronic configurations:

Ag: [Kr]  4d^(10) 5s^1=20

Pd: [Kr]  4d^8 5s^2

Changing S.E. will change the core sates and so number of valence =
electrons printed in case.in2 file.

I said these because I would emphasis on this point that one should not =
utilizing case.inst file try to recognize valence electrons. case.inst =
file is an input file for atomic lstart program, and case.inc file is an =
input file for lcore program.


.in1 is:
> WFFIL        (WFPRI, SUPWF)
>   8.50       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
>   0.30    5  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global =
APW/LAPW)
>  0    0.30      0.000 CONT 0
>  0   -6.68      0.005 STOP 0
> ...
> so according to the UG and the step-by-step course of S. Cottenier, i =
think Ag and Pd  (4s4p) are semi-core states treated > with LOs, and add =
5p to the valence states (unoccupied) .

=20

Although you are right again, semi core states of atoms are not what one =
can deduce from case.in1 file: just one can justify about added or not =
LO's. This means that from case.in1 file one can conclude that for which =
orbitals of an atom LO's are added. One may add manually one local =
orbital for an atom if it is not already added. This can be easily done =
specifying once more (maximum twice) a l-value in case.in1 file keeping =
the format.

=20

> But for the O atoms, the UG said that " If the same l value is =
specified twice, ......The first energy is used for the usual=20

> LAPW's and the second for the LOs", so i think 2s(semi-core) is =
treated with LOs, and add 3s(unoccupied) to the valence=20

> states. But the energy( -1.55Ry) for 3s <  (0.30Ry) for 2s. And in the =
case.inst O (2s2p) is valence states. =20

>                        Where is my errors?=20

I think it should be clear now considering described above =
misunderstanding of case.inst, case.inc, and case.in1 files.


=20
> And another question about the klist:
>  If the k-points specified in the klist is all in the IBZ, and if only =
these k-points in the IBZ will be calculated while other is not=20

> need to be calculated?

=20

Yes, the other will be predictable employing symmetry.



Your,

S. Jalali.

=20

=20


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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Dwindows-1252">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY>
<DIV><FONT face=3DArial size=3D2>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">&gt;&nbsp;I am calculating =
the band=20
structure of the Ag2PdO2 (semiconductor) using the default =
choices.<BR>&gt;=20
&nbsp;&nbsp; the case.inc is:<BR>&gt; &nbsp;&nbsp;&nbsp; 9=20
0.00&nbsp;&nbsp;&nbsp;&nbsp; NUMBER OF ORBITALS (EXCLUDING SPIN), =
SHIFT<BR>&gt;=20
1,-1,2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&=
nbsp;&nbsp;&nbsp;=20
( N,KAPPA,OCCUP)<BR>&gt;=20
2,-1,2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&=
nbsp;&nbsp;&nbsp;=20
( N,KAPPA,OCCUP)<BR>&gt; 2,=20
1,2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbs=
p;&nbsp;&nbsp;=20
( N,KAPPA,OCCUP)<BR>&gt;=20
2,-2,4&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&=
nbsp;&nbsp;&nbsp;=20
( N,KAPPA,OCCUP)<BR>&gt;=20
3,-1,2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&=
nbsp;&nbsp;&nbsp;=20
( N,KAPPA,OCCUP)<BR>&gt; 3,=20
1,2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbs=
p;&nbsp;&nbsp;=20
( N,KAPPA,OCCUP)<BR>&gt;=20
3,-2,4&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&=
nbsp;&nbsp;&nbsp;=20
( N,KAPPA,OCCUP)<BR>&gt; 3,=20
2,4&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbs=
p;&nbsp;&nbsp;=20
( N,KAPPA,OCCUP)<BR>&gt;=20
3,-3,6&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&=
nbsp;&nbsp;&nbsp;=20
( N,KAPPA,OCCUP)<BR>...</SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">&gt; so i think Ag and Pd =
core=20
states are (1s2s2p3s3p3d), O core states is (1s).</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><?xml:namespace=20
prefix =3D o ns =3D "urn:schemas-microsoft-com:office:office"=20
/><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial"></SPAN>&nbsp;</P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">You are right about core=20
states.</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><BR>&gt; The =
case.inst=20
is:<BR>&gt; Ag <BR>&gt; Kr 3 5<BR>&gt; 4, 2,2.0&nbsp; N<BR>&gt; 4, =
2,2.0&nbsp;=20
N</P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt">...<BR>&gt; so i =
think Ag and Pd=20
valence states are (4d5s), O valence states are (2s2p).</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial"></SPAN>&nbsp;</P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">Although you have also =
correctly=20
distinguished valence states of O,&nbsp; valence states of Ag and Pd=20
are&nbsp;4s^2 4p^6 4d^(10) 5s^1. </SPAN><?xml:namespace prefix =3D st1 =
ns =3D=20
"urn:schemas-microsoft-com:office:smarttags" =
/><st1:City><st1:place><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: =
Arial">Valence</SPAN></st1:place></st1:City><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial"> (valence+semi core) =
states are=20
separated from core states selecting separation energy (S.E.) in wien2k =
during=20
initialization procedure. Based on your chosen S.E. configurations of =
your atoms=20
look like:<BR>Ag: [Ar 3d^(10)]&nbsp; 4s^2 4p^6 4d^(10) 5s^1</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">Pd: [Ar 3d^(10)]&nbsp; =
4s^2 4p^6=20
4d^8 5s^2</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">O: [He] 2s^2 =
2p^4</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">which the ones for Ag and =
Pd appear=20
different from following standard electronic configurations:</SPAN><SPAN =

style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">Ag: =
[Kr]&nbsp;&nbsp;4d^(10)=20
5s^1</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><FONT=20
size=3D3><FONT face=3D"Times New Roman"> =
<o:p></o:p></FONT></FONT></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">Pd: [Kr]&nbsp;&nbsp;4d^8=20
5s^2</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">Changing S.E. will change =
the core=20
sates and so number of valence electrons printed in case.in2 =
file.</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">I said these&nbsp;because =
I would=20
emphasis on this point that one </SPAN><B><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial; mso-bidi-font-size: =
14.0pt">should=20
not&nbsp;utilizing case.inst</SPAN></B><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial"> file try to recognize =
valence=20
electrons. case.inst file is an input file for atomic lstart program, =
and=20
case.inc file is an input file for lcore program.</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><BR></SPAN><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">.in1 is:<BR>&gt;=20
WFFIL&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; (WFPRI, SUPWF)<BR>&gt; =
&nbsp;=20
8.50&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 10&nbsp;&nbsp;&nbsp; 4 =
(R-MT*K-MAX; MAX=20
L IN WF, V-NMT<BR>&gt; &nbsp; 0.30&nbsp;&nbsp;&nbsp; 5&nbsp;=20
0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; (GLOBAL E-PARAMETER WITH n OTHER =
CHOICES, global=20
APW/LAPW)<BR>&gt; &nbsp;0&nbsp;&nbsp;&nbsp; =
0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
0.000 CONT 0<BR>&gt; &nbsp;0&nbsp;&nbsp; =
- -6.68&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
0.005 STOP 0<BR>&gt; ...<BR>&gt; so according to the UG and the =
step-by-step=20
course of </SPAN><st1:place><SPAN style=3D"FONT-SIZE: 10pt; FONT-FAMILY: =
Arial">S.=20
Cottenier</SPAN></st1:place><SPAN style=3D"FONT-SIZE: 10pt; FONT-FAMILY: =
Arial">,=20
i think Ag and Pd&nbsp; (4s4p) are semi-core states treated &gt; with =
LOs, and=20
add 5p to the valence states (unoccupied) .</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><FONT=20
size=3D3><FONT face=3D"Times New =
Roman">&nbsp;<o:p></o:p></FONT></FONT></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">Although you are right =
again, semi=20
core states of atoms are not what one can deduce from case.in1 file:=20
just&nbsp;one can&nbsp;justify about&nbsp;added or not LO's.&nbsp;This =
means=20
that from case.in1 file one can conclude that for which orbitals of an =
atom LO's=20
are added. One may add manually one local orbital for an atom if it is =
not=20
already added. This can be easily done specifying once more (maximum =
twice)=20
a&nbsp;l-value in case.in1 file keeping the format.</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><FONT=20
size=3D3><FONT face=3D"Times New =
Roman">&nbsp;<o:p></o:p></FONT></FONT></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">&gt;&nbsp;But for the O =
atoms, the=20
UG said that " If the same l value is specified twice, ......The first =
energy is=20
used for the usual </SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">&gt; LAPW's and the second =
for the=20
LOs", so i think 2s(semi-core) is treated with LOs, and add =
3s(unoccupied) to=20
the valence </SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">&gt; states. But the =
energy(=20
- -1.55Ry) for 3s &lt;&nbsp; (0.30Ry) for 2s. And in the case.inst O =
(2s2p) is=20
valence states.&nbsp; </SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">&gt;=20
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&=
nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
Where is my errors? </SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">I think it should be clear =
now=20
considering described above misunderstanding of case.inst, case.inc, and =

case.in1 files.</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><BR></SPAN><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">&nbsp;<BR>&gt; And another =
question=20
about the klist:<BR>&gt; &nbsp;If the k-points specified in the klist is =
all in=20
the IBZ, and if only these k-points in the IBZ will be calculated while =
other is=20
not </SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">&gt; need to be=20
calculated?</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><FONT=20
size=3D3><FONT face=3D"Times New =
Roman">&nbsp;<o:p></o:p></FONT></FONT></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">Yes, the other will be =
predictable=20
employing symmetry.</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial"></SPAN>&nbsp;</P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">Your,</SPAN><SPAN=20
style=3D"mso-bidi-font-size: 12.0pt; mso-bidi-font-family: 'Times New =
Roman'"><o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: Arial">S. =
Jalali.<o:p></o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><SPAN=20
style=3D"FONT-SIZE: 10pt; FONT-FAMILY: =
Arial"><o:p>&nbsp;</o:p></SPAN></P>
<P class=3DMsoNormal style=3D"MARGIN: 0in 0in 0pt"><o:p><FONT =
face=3D"Times New Roman"=20
size=3D3>&nbsp;</FONT></o:p></P></DIV></FONT></BODY></HTML>

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Date: Mon, 7 Oct 2002 00:47:17 +0800
From: "yulihua-wuhan" <yulihua-wuhan@sohu.com>
Subject: [WIEN]: semi-core states and valence states for LOs

====
"yulihua-wuhan" <yulihua-wuhan@sohu.com>
submitted the following contribution:
====

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Date: Mon, 7 Oct 2002 00:10:33 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: semi-core states and valence states for LOs

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

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> Now something is clear and other thing is
> not clear for me.
>   Firstly the clear thing:
>   From the case.outputst file (i select the separation energy =3D -0.7
> Ry):=20
>=20
>      Ag
>       -26.13650      -26.13619
>        -6.97867       -6.97916
>        -4.55733       -4.55681
>        -4.18385       -4.18290
>        -0.57613       -0.56153
>        -0.53564       -0.52018
>        -0.34800       -0.29098
> ...................................
> TOTAL CORE-CHARGE:                   28.00000000001556    =20
> TOTAL CORE-CHARGE INSIDE SPHERE:     27.99999824441523=20

You did perfect reducing S.E. to -7.0Ry. In this case 2 electrons of 4s =
orbital is considered as a valence state. -6.0Ry confines these two =
electrons into core states, and so they leaks out of sphere as they are =
not really core electrons. This is something similar to the nice Fe =
example presented in the beautiful textbook of Stefaan.

>     Pd   =20
>        -23.99693      -23.98606
>        -6.53262       -6.48445
>        -4.24439       -4.19361
>        -3.91695       -3.86501
>        -0.53606       -0.47302
>        -0.50180       -0.43826
>        -0.34905       -0.27655
> ...................................................
>  TOTAL CORE-CHARGE:                   28.00000000001986    =20
>  TOTAL CORE-CHARGE INSIDE SPHERE:     27.99999618024979    =20
> ........................................................

Here in Pd we also have a similar situation to Ag.

>=20
>   O
>        -37.83576      -37.74537
>        -1.85285       -1.61423
>        -0.75278       -0.52946
>        -0.75000       -0.52695
> ...........................................................
>  TOTAL CORE-CHARGE:                   2.000000000001837    =20
>  TOTAL CORE-CHARGE INSIDE SPHERE:     1.999999989304444    =20
> ..........................................................

For O only -2.0Ry seems enough, but considering Ag and Pd atoms one =
should choose still -7.0Ry.
=20
> so i think the configurations of atoms:
> Ag: [Ar 3d^(10)]  4s^2 4p^6 4d^(10) 5s^1
> Pd: [Ar 3d^(10)]  4s^2 4p^6 4d^9     5s^1   --------> not 4d^8 5s^2
>=20
> O:   [He] 2s^2 2p^4
I don't know how you find that configuration for Pd!
> The unclear thing is that from case.in1:
>=20
> WFFIL        (WFPRI, SUPWF)
>   8.50       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
>   0.30    5  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global
> APW/LAPW)
>  0    0.30      0.000 CONT 0  ---->LAPW    for 5s? =20
>  0   -6.68      0.005 STOP 0  ---->LAPW+LO for 4s? =20
>  1    0.30      0.000 CONT 0  ---->LAPW    for 5p?
>  1   -3.88      0.005 STOP 0  ---->LAPW+LO for 4p?
>  2    0.30      0.010 CONT 1  ---->LAPW+lo for 4d (new basis set)
>   0.30    5  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global
> APW/LAPW)
>  0    0.30      0.000 CONT 0
>  0   -6.23      0.005 STOP 0
>  1    0.30      0.000 CONT 0 -----> same as above
>  1   -3.62      0.005 STOP 0
>  2    0.30      0.010 CONT 1
>   0.30    3  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global
> APW/LAPW)
>  0   -1.55      0.010 CONT 0 -----> LAPW    for 2s?           =20
>  0    0.30      0.000 CONT 0 -----> LAPW+LO for 3s?
>  1    0.30      0.000 CONT 1 -----> LAPW+lo for 2p (new basis set)
> K-VECTORS FROM UNIT:4   -8.0       1.5      emin/emax window
>=20
> I just only can conclude that LOs are added to S,P for Ag and Pd =
atoms,
> and LOs are added to S for O atom.
> But how can i know which orbitals are treated with LAPW+LO and which =
are
> semi-core?
Of coarse, you can guess these LO's are added to make a better treatment =
for 4s 4p of Ag and Pd and for 2s of O, as they are deeper in energy =
scale comparing the other valence orbitals. To make more sure which =
orbitals and how many electrons are in semi core states and if added =
LO's have done their jobs one can plot density of states in semi core =
region or look into case.ouputt or case.outpu2.

> If i can distinguish which orbitals of the atom (2s or 3s of O atom) =
are
> treated with LAPW+LO/LAPW using the linearization energy?
Yes, I think you have marked correctly the way of treatments in the =
case.in1 file.

Your,
S. Jalali.

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<DIV><FONT face=3DArial size=3D2>&gt; Now something is clear and other =
thing=20
is<BR>&gt; not clear for me.<BR>&gt;&nbsp;&nbsp; Firstly the clear=20
thing:<BR>&gt;&nbsp;&nbsp; From the case.outputst file (i select the =
separation=20
energy =3D -0.7<BR>&gt; Ry): <BR>&gt; =
<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
Ag<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -26.13650&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -26.13619<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -6.97867&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -6.97916<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -4.55733&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -4.55681<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -4.18385&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -4.18290<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.57613&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.56153<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.53564&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.52018<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.34800&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -0.29098<BR>&gt;=20
...................................<BR>&gt; TOTAL=20
CORE-CHARGE:&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&=
nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
28.00000000001556&nbsp;&nbsp;&nbsp;&nbsp; <BR>&gt; TOTAL CORE-CHARGE =
INSIDE=20
SPHERE:&nbsp;&nbsp;&nbsp;&nbsp; 27.99999824441523&nbsp;<BR></FONT></DIV>
<DIV><FONT face=3DArial size=3D2>You did&nbsp;perfect reducing S.E. to =
- -7.0Ry. In=20
this case 2 electrons of 4s orbital is considered&nbsp;as a&nbsp;valence =
state.=20
- -6.0Ry confines these two electrons into core states, and so they leaks =
out of=20
sphere as they are not really core electrons. This is something similar =
to the=20
nice Fe example presented in the beautiful textbook of =
Stefaan.</DIV></FONT>
<DIV><FONT face=3DArial size=3D2>&nbsp;</DIV></FONT>
<DIV><FONT face=3DArial size=3D2>&gt;&nbsp;&nbsp;&nbsp;&nbsp; =
Pd&nbsp;&nbsp;&nbsp;=20
<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -23.99693&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -23.98606<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -6.53262&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -6.48445<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -4.24439&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -4.19361<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -3.91695&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -3.86501<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.53606&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.47302<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.50180&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.43826<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.34905&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -0.27655<BR>&gt;=20
...................................................<BR>&gt;&nbsp; TOTAL=20
CORE-CHARGE:&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&=
nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
28.00000000001986&nbsp;&nbsp;&nbsp;&nbsp; <BR>&gt;&nbsp; TOTAL =
CORE-CHARGE=20
INSIDE SPHERE:&nbsp;&nbsp;&nbsp;&nbsp; =
27.99999618024979&nbsp;&nbsp;&nbsp;&nbsp;=20
<BR>&gt;=20
........................................................<BR></FONT></DIV>=

<DIV><FONT face=3DArial size=3D2>Here in Pd we also have a similar =
situation to=20
Ag.</DIV></FONT>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>&gt; <BR>&gt;&nbsp;&nbsp;=20
O<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -37.83576&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -37.74537<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -1.85285&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -1.61423<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.75278&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.52946<BR>&gt;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
- -0.75000&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -0.52695<BR>&gt;=20
...........................................................<BR>&gt;&nbsp;=
 TOTAL=20
CORE-CHARGE:&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&=
nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
2.000000000001837&nbsp;&nbsp;&nbsp;&nbsp; <BR>&gt;&nbsp; TOTAL =
CORE-CHARGE=20
INSIDE SPHERE:&nbsp;&nbsp;&nbsp;&nbsp; =
1.999999989304444&nbsp;&nbsp;&nbsp;&nbsp;=20
<BR>&gt;=20
..........................................................<BR></FONT></DI=
V>
<DIV><FONT face=3DArial size=3D2>For O only -2.0Ry seems enough, but =
considering Ag=20
and Pd atoms one should choose still -7.0Ry.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>&nbsp;<BR>&gt; so i think the =
configurations of=20
atoms:<BR>&gt; Ag: [Ar 3d^(10)]&nbsp; 4s^2 4p^6 4d^(10) 5s^1<BR>&gt; Pd: =
[Ar=20
3d^(10)]&nbsp; 4s^2 4p^6 4d^9&nbsp;&nbsp;&nbsp;&nbsp; 5s^1&nbsp;&nbsp;=20
- --------&gt; not 4d^8 5s^2<BR>&gt; <BR>&gt; O:&nbsp;&nbsp; [He] 2s^2=20
2p^4</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>I don't know how you find that =
configuration for=20
Pd!</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>&gt; The unclear thing is that from=20
case.in1:<BR>&gt; <BR>&gt; =
WFFIL&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
(WFPRI, SUPWF)<BR>&gt;&nbsp;&nbsp; =
8.50&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
10&nbsp;&nbsp;&nbsp; 4 (R-MT*K-MAX; MAX L IN WF, =
V-NMT<BR>&gt;&nbsp;&nbsp;=20
0.30&nbsp;&nbsp;&nbsp; 5&nbsp; 0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; (GLOBAL=20
E-PARAMETER WITH n OTHER CHOICES, global<BR>&gt; APW/LAPW)<BR>&gt;&nbsp; =

0&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT =
0&nbsp;=20
- ----&gt;LAPW&nbsp;&nbsp;&nbsp; for 5s?&nbsp; <BR>&gt;&nbsp; =
0&nbsp;&nbsp;=20
- -6.68&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.005 STOP 0&nbsp; ----&gt;LAPW+LO =
for=20
4s?&nbsp; <BR>&gt;&nbsp; 1&nbsp;&nbsp;&nbsp; =
0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
0.000 CONT 0&nbsp; ----&gt;LAPW&nbsp;&nbsp;&nbsp; for 5p?<BR>&gt;&nbsp;=20
1&nbsp;&nbsp; -3.88&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.005 STOP 0&nbsp;=20
- ----&gt;LAPW+LO for 4p?<BR>&gt;&nbsp; 2&nbsp;&nbsp;&nbsp;=20
0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010 CONT 1&nbsp; ----&gt;LAPW+lo =
for 4d=20
(new basis set)<BR>&gt;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp; 5&nbsp;=20
0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; (GLOBAL E-PARAMETER WITH n OTHER =
CHOICES,=20
global<BR>&gt; APW/LAPW)<BR>&gt;&nbsp; 0&nbsp;&nbsp;&nbsp;=20
0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT 0<BR>&gt;&nbsp; =
0&nbsp;&nbsp;=20
- -6.23&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.005 STOP 0<BR>&gt;&nbsp;=20
1&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT 0 =
- -----&gt;=20
same as above<BR>&gt;&nbsp; 1&nbsp;&nbsp; =
- -3.62&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
0.005 STOP 0<BR>&gt;&nbsp; 2&nbsp;&nbsp;&nbsp;=20
0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010 CONT 1<BR>&gt;&nbsp;&nbsp;=20
0.30&nbsp;&nbsp;&nbsp; 3&nbsp; 0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; (GLOBAL=20
E-PARAMETER WITH n OTHER CHOICES, global<BR>&gt; APW/LAPW)<BR>&gt;&nbsp; =

0&nbsp;&nbsp; -1.55&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010 CONT 0 -----&gt; =

LAPW&nbsp;&nbsp;&nbsp; for=20
2s?&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
<BR>&gt;&nbsp; 0&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; =
0.000 CONT=20
0 -----&gt; LAPW+LO for 3s?<BR>&gt;&nbsp; 1&nbsp;&nbsp;&nbsp;=20
0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT 1 -----&gt; LAPW+lo for 2p =
(new=20
basis set)<BR>&gt; K-VECTORS FROM UNIT:4&nbsp;&nbsp;=20
- -8.0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; =
1.5&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;=20
emin/emax window<BR>&gt; <BR>&gt; I just only can conclude that LOs are =
added to=20
S,P for Ag and Pd atoms,<BR>&gt; and LOs are added to S for O =
atom.<BR>&gt; But=20
how can i know which orbitals are treated with LAPW+LO and which =
are<BR>&gt;=20
semi-core?<BR>Of coarse, you can guess these LO's are added to make a =
better=20
treatment for 4s 4p of Ag and Pd and for 2s of O, as they are deeper in =
energy=20
scale comparing the other valence orbitals. To make more sure which =
orbitals and=20
how many electrons are in semi core states and if added LO's have done =
their=20
jobs one can&nbsp;plot density of states in semi core region or =
look&nbsp;into=20
case.ouputt or case.outpu2.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>&gt; If i can distinguish which =
orbitals of the=20
atom (2s or 3s of O atom) are<BR>&gt; treated with LAPW+LO/LAPW using =
the=20
linearization energy?<BR></FONT><FONT face=3DArial size=3D2>Yes, I think =
you have=20
marked correctly the way of&nbsp;treatments in the case.in1 =
file.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Your,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>S. Jalali.</DIV></FONT></BODY></HTML>

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------------------------------

Date: Mon, 7 Oct 2002 09:30:47 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: error in init_lapw

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> When sgroup finds a new structure you are asked if you would like to
> continue or edit case.struct_sgroup.  At the moment, instead of doing
> this, the script pops up the case.struct file when you type "y".  I
> presume this is a mistake and line 142 should be:
>
>     editor $file.struct_sgroup
>
> rather than
>
>     editor $file.struct

Yes, you are right. It will be changed with the next update.

Thanks

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Mon, 7 Oct 2002 15:50:28 +0800
From: "yulihua-wuhan" <yulihua-wuhan@sohu.com>
Subject: Re: [WIEN]: semi-core states and valence states for LOs

====
"yulihua-wuhan" <yulihua-wuhan@sohu.com>
submitted the following contribution:
====

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- ------=_NextPart_000_0030_01C26E19.4236F190--

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Date: Mon, 07 Oct 2002 16:45:39 +0200
From: Ingo Loa <I.Loa@fkf.mpg.de>
Subject: [WIEN]: bcc Cs, convergence of Etot wrt GMAX

====
Ingo Loa <I.Loa@fkf.mpg.de>
submitted the following contribution:
====

Dear Wien2k team & users,

when looking at the pressure-induced bcc-to-fcc transition in Cs by 
total-energy calculations, I recently encountered the following 
difficulties. I could easily converge the total energy as a function of 
RKMAX and number of k-points. Convergence with regard to GMAX, however, was 
extremely slow. Even with GMAX values as large as 50, the total energy of 
the bcc phase was still not converged on the 1-meV/atom level. This appears 
rather unusual to me, especially, because it occurs in a fairly simple 
system. A summary of typical input files is given below, the calculations 
were performed with a recent release of Wien2k.

Does anybody have an idea of what may cause these troubles or how to 
proceed? Any comments/suggestions are welcome.

Regards,
Ingo Loa


*************************************************************************

Cs-bcc.struct:

Cs-bcc
B   LATTICE,NONEQUIV. ATOMS: 1
MODE OF CALC=RELA unit=ang
  11.515569 11.515569 11.515569 90.000000 90.000000 90.000000
ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
           MULT= 1          ISPLIT= 
2
Cs         NPT=  781  R0=0.00001000 RMT=    2.0000   Z: 55.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                      0.0000000 1.0000000 
0.0000000
                      0.0000000 0.0000000 
1.0000000
   48      NUMBER OF SYMMETRY 
OPERATIONS
- --------------------------------------------------------------------------
Cs-bcc.in0:

TOT   13     (5...CA-LDA, 13...PBE-GGA, 14...PW2-GGA)
NR2V      (R2V)
- --------------------------------------------------------------------------
Cs-bcc.in1:

WFFIL        (WFPRI, SUPWF)
   8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  -.14794   6   0      global e-param with N other choices, napw
  0    0.103     0.000 CONT 1
  0   -1.602     0.000 CONT 1
  1    0.116     0.000 CONT 1
  1   -0.633     0.000 CONT 1
  2    0.132     0.000 CONT 1
  2   -5.087     0.000 CONT 1
K-VECTORS FROM UNIT:4    -8.0      2.5      emin/emax window
- --------------------------------------------------------------------------
Cs-bcc.in2:

TOT             (TOT,FOR,QTL,EFG,FERMI)
       -9.0      19.0 0.50 0.05                EMIN, NE, ESEPERMIN, ESEPER0
TETRA    0.000          (GAUSS,ROOT,TEMP,TETRA,ALL      eval)
  0 0 4 0 4 4 6 0 6 4
  55.          GMAX
FILE        FILE/NOFILE  write recprlist
- --------------------------------------------------------------------------
Cs-bcc.klist:

165 k-points in the irreducible wedge, 4913 points in total.
- --------------------------------------------------------------------------





- --------------------------------------------------------------------------
Ingo Loa
Max-Planck-Institut fuer Festkoerperforschung, Stuttgart
Heisenbergstr. 1        //   D-70569 Stuttgart   //   Germany
Tel. +49.711.689-1469   //   Fax. +49.711.689-1444
I.Loa@fkf.mpg.de        //   http://www.mpi-stuttgart.mpg.de/hd
- --------------------------------------------------------------------------

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Date: Mon, 7 Oct 2002 17:45:28 +0200
From: "koitzsch" <Christian.Koitzsch@unifr.ch>
Subject: [WIEN]: open core treatment

====
"koitzsch" <Christian.Koitzsch@unifr.ch>
submitted the following contribution:
====

Hi Everybody,

I have a question regarding an open core treatment of 4f electrons in a rare
earth silicide, specifically GdSi. My Case.struct looks like this:

Title
H   LATTICE,NONEQUIV. ATOMS: 2
MODE OF CALC=RELA
  7.318912  7.318912  7.904728 90.000000 90.000000120.000000
ATOM= -1: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT= 4
Gd         NPT=  781  R0=0.00001000 RMT=    3.0000   Z: 64.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -2: X=0.33333333 Y=0.66666667 Z=0.50000000
          MULT= 2          ISPLIT= 4
      -2: X=0.66666667 Y=0.33333333 Z=0.50000000
Si         NPT=  781  R0=0.00010000 RMT=    2.0000   Z: 14.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
  24      NUMBER OF SYMMETRY OPERATIONS





As outlined in the FAQ section, I ran a SCF cycle conventionally, and
looked, where my 4f's are in case.scf

OVERALL ENERGY PARAMETER IS    0.3000
          E( 0)=    0.3000
          E( 0)=   -2.4675   E(BOTTOM)=   -2.515   E(TOP)=   -2.420
          E( 1)=   -0.8650   E(BOTTOM)=   -1.030   E(TOP)=   -0.700
          E( 1)=    0.3000
          E( 3)=    0.6150   E(BOTTOM)=    0.580   E(TOP)=    0.650
          E( 2)=    0.5100   E(BOTTOM)=    0.510   E(TOP)= -200.000
So, as far as I understand, a shift of 0.7 would be sufficient

I modifief then, case.inc to get the half filled 4f shell into core (number
of orbitals changed from 14 to 16 and inluded 4, 3,3 and 4,-4,4 and
specified a shift of 0.7:

16 0.70     NUMBER OF ORBITALS (EXCLUDING SPIN)
1,-1,2               ( N,KAPPA,OCCUP)
2,-1,2               ( N,KAPPA,OCCUP)
2, 1,2               ( N,KAPPA,OCCUP)
2,-2,4               ( N,KAPPA,OCCUP)
3,-1,2               ( N,KAPPA,OCCUP)
3, 1,2               ( N,KAPPA,OCCUP)
3,-2,4               ( N,KAPPA,OCCUP)
3, 2,4               ( N,KAPPA,OCCUP)
3,-3,6               ( N,KAPPA,OCCUP)
4,-1,2               ( N,KAPPA,OCCUP)
4, 1,2               ( N,KAPPA,OCCUP)
4,-2,4               ( N,KAPPA,OCCUP)
4, 2,4               ( N,KAPPA,OCCUP)
4,-3,6               ( N,KAPPA,OCCUP)
4, 3,3
4,-4,4
 4     NUMBER OF ORBITALS (EXCLUDING SPIN)
1,-1,2               ( N,KAPPA,OCCUP)
2,-1,2               ( N,KAPPA,OCCUP)
2, 1,2               ( N,KAPPA,OCCUP)
2,-2,4               ( N,KAPPA,OCCUP)
 0

Then I modified case.in1 and put the 4f's fixed at -1

WFFIL        (WFPRI, SUPWF)
  8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  0.30    6      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
 0    0.30      0.000 CONT
 0   -3.43      0.005 STOP
 1   -1.67      0.010 CONT
 1    0.30      0.000 CONT
 3   -1.00      0.000 CONT
 2    0.30      0.010 CONT
  0.30    2      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
 0    0.30      0.000 CONT
 1    0.30      0.000 CONT
K-VECTORS FROM UNIT:4    -7.0      1.5      emin/emax window


and finally I removed the 7 4f's from valence charge and reduced therefore
NE from 26 to 19 in case.in2

WFFIL        (WFPRI, SUPWF)
  8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  0.30    6      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
 0    0.30      0.000 CONT
 0   -3.43      0.005 STOP
 1   -1.67      0.010 CONT
 1    0.30      0.000 CONT
 3   -1.00      0.000 CONT
 2    0.30      0.010 CONT
  0.30    2      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
 0    0.30      0.000 CONT
 1    0.30      0.000 CONT
K-VECTORS FROM UNIT:4    -7.0      1.5      emin/emax window

Nevertheless I get then after running again dstart and having a mixing
parameter of 0.01 the following error messages:


 LAPW0 END
 LAPW1 END
 LAPW2 END
forrtl: severe (64): input conversion error, unit 20, file
/home/koitzsch/GdSi/GdSi.struct
   0: _call_remove_gp_range [0x3ff81a6c374]
   1: _call_remove_gp_range [0x3ff81a6c8f4]
   2: _call_remove_gp_range [0x3ff81a93b84]
   3: _call_remove_gp_range [0x3ff81a926e0]
   4: insld_ [insld.f: 92, 0x12000928c]
   5: hfsd_ [hfsd.f: 127, 0x120005ffc]
   6: main [for_main.c: 203, 0x120002554]
   7: __start [0x1200024c8]

Does anybody know, what I am doing wrong here.

Thank you for any suggestions

Christian Koitzsch
University of Fribourg
Department of Physics
CH-1700 Fribourg
Switzerland


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------------------------------

Date: Mon, 07 Oct 2002 17:55:15 +0200
From: Florent Boucher <Florent.Boucher@cnrs-imn.fr>
Subject: [WIEN]: Pb SRC_lapw2/atpar.F and lxdos

====
Florent Boucher <Florent.Boucher@cnrs-imn.fr>
submitted the following contribution:
====

Dear Peter,
we are trying to use the ISPLIT=99 option in WIEN2K (latest version) and 
we have troubles with the atpar.F program. In the distributed version 
they are comments for the following lines:
!
!....overlap integrals for x-dos
!
!!$      do l=0,lxdos
!!$         do lp=0,lxdos
!!$            pu1u2(l,lp)=0.d0
!!$            pueu2(l,lp)=0.d0
!!$            pu2u2(l,lp)=0.d0
!!$            CALL RINT13(REL,rrad1(1,l),rrad2(1,l),rrad1(1,lp) &
!!$                 ,rrad2(1,lp),pu1u1(l,lp),JATOM)        
!!$            CALL RINT13(REL,rrad1(1,l),rrad2(1,l),rade1(1,lp) &
!!$                 ,rade2(1,lp),pu1ue(l,lp),JATOM)        
!!$            if(lp.le.lmax2) CALL RINT13(REL,rrad1(1,l),rrad2(1,l) &
!!$                 ,a1lo(1,lp),b1lo(1,lp),pu1u2(l,lp),JATOM)        
!!$            CALL RINT13(REL,rade1(1,l),rade2(1,l),rade1(1,lp) &
!!$                 ,rade2(1,lp),pueue(l,lp),JATOM)        
!!$            if(lp.le.lmax2) CALL RINT13(REL,rade1(1,l),rade2(1,l) &
!!$                 ,a1lo(1,lp),b1lo(1,lp),pueu2(l,lp),JATOM)        
!!$            if((lp.le.lmax2).and.(l.le.lmax2)) CALL 
RINT13(REL,a1lo(1,l) &
!!$                 ,b1lo(1,l),a1lo(1,lp),b1lo(1,lp),pu2u2(l,lp),JATOM)
!!$         enddo
!!$      enddo

For this reason, the qtl file and help files have only zero values 
(pu1u1, pueue .... are not initialized)

When we try to remove the comments, we are unable to compile.
We have the following errors as the dimension of the array has changed 
in order to use multiple LO.
      a1lo(1:nrad,1:nloat,0:lomax)

Here is the error:
f90: Error: atpar_tmp_.F, line 281: The number of subscripts is 
incorrect.   [A1LO]
                 ,a1lo(1,lp),b1lo(1,lp),pu1u2(l,lp),JATOM)        
- ------------------^
f90: Error: atpar_tmp_.F, line 281: The number of subscripts is 
incorrect.   [B1LO]
                 ,a1lo(1,lp),b1lo(1,lp),pu1u2(l,lp),JATOM)        
- -----------------------------^
f90: Error: atpar_tmp_.F, line 285: The number of subscripts is 
incorrect.   [A1LO]
                 ,a1lo(1,lp),b1lo(1,lp),pueu2(l,lp),JATOM)        
- ------------------^
f90: Error: atpar_tmp_.F, line 285: The number of subscripts is 
incorrect.   [B1LO]
                 ,a1lo(1,lp),b1lo(1,lp),pueu2(l,lp),JATOM)        
- -----------------------------^
f90: Error: atpar_tmp_.F, line 286: The number of subscripts is 
incorrect.   [A1LO]
            if((lp.le.lmax2).and.(l.le.lmax2)) CALL RINT13(REL,a1lo(1,l) &
- ---------------------------------------------------------------^
f90: Error: atpar_tmp_.F, line 287: The number of subscripts is 
incorrect.   [B1LO]
                 ,b1lo(1,l),a1lo(1,lp),b1lo(1,lp),pu2u2(l,lp),JATOM)
- ------------------^
f90: Error: atpar_tmp_.F, line 287: The number of subscripts is 
incorrect.   [A1LO]
                 ,b1lo(1,l),a1lo(1,lp),b1lo(1,lp),pu2u2(l,lp),JATOM)
- ----------------------------^
f90: Error: atpar_tmp_.F, line 287: The number of subscripts is 
incorrect.   [B1LO]
                 ,b1lo(1,l),a1lo(1,lp),b1lo(1,lp),pu2u2(l,lp),JATOM)
- ---------------------------------------^
*
Do you think you can do something about that ?
Regards
Florent

- -- 
 --------------------------------------------------------------------------
| Florent BOUCHER                    |                                     |
| Institut des Matériaux Jean Rouxel | Mailto:Florent.Boucher@cnrs-imn.fr  |
| 2, rue de la Houssinière           | Phone: (33) 2 40 37 39 24           |
| BP 32229                           | Fax:   (33) 2 40 37 39 95           |
| 44322 NANTES CEDEX 3 (FRANCE)      | http://www.cnrs-imn.fr              |
 --------------------------------------------------------------------------


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Date: Mon, 7 Oct 2002 18:01:19 +0200
From: "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: open core treatment

====
"Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

>  LAPW0 END
>  LAPW1 END
>  LAPW2 END
> forrtl: severe (64): input conversion error, unit 20, file
> /home/koitzsch/GdSi/GdSi.struct
>    0: _call_remove_gp_range [0x3ff81a6c374]
>    1: _call_remove_gp_range [0x3ff81a6c8f4]
>    2: _call_remove_gp_range [0x3ff81a93b84]
>    3: _call_remove_gp_range [0x3ff81a926e0]
>    4: insld_ [insld.f: 92, 0x12000928c]
>    5: hfsd_ [hfsd.f: 127, 0x120005ffc]
>    6: main [for_main.c: 203, 0x120002554]
>    7: __start [0x1200024c8]
>
> Does anybody know, what I am doing wrong here.

Your problem is in lcore. Two suggestions :

1) Try to fill first the core orbitals like this (completely fill one, and
only then go to the next):
> 4, 3,6
> 4,-4,1

2) Try a slightly larger shift (0.8, 0.9).

Stefaan


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------------------------------

Date: Mon, 7 Oct 2002 11:08:22 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: min_lapw

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

After the SCF cycles, I run min_lapw, it stoped after 5 cycles with the
following information on my screen:

run_lapw -I -fc 1. -renorm -i 40
hup: Command not found
STOP:  MIXER END
in cycle 2    ETEST: 0   CTEST: 0
hup: Command not found
STOP:  LAPW0 END
STOP:  LAPW1 END
STOP:  LAPW2 END
STOP:  CORE  END
STOP:  MIXER END
in cycle 3    ETEST: 11732.1216010000000000   CTEST: .0410162
hup: Command not found
STOP:  LAPW0 END
STOP:  LAPW1 END
STOP:  LAPW2 END
STOP:  CORE  END
STOP:  MIXER END
in cycle 4    ETEST: 5866.5759085000000000   CTEST: .0398830
hup: Command not found
STOP:  LAPW0 END
STOP:  LAPW1 END
STOP:  LAPW2 END
STOP:  CORE  END
STOP:  MIXER END
in cycle 5    ETEST: .7647320000000000   CTEST: .0390583
hup: Command not found
STOP:  LAPW0 END
STOP:  LAPW1 END
STOP:  LAPW2 END
STOP:  CORE  END
STOP:  MIXER END
STOP: MINI - Error


I checked the case.file as following:

Calculating chiolite in /local/project00/umbingz/mysamples/chiolite
on mira

start       (Wednesday October  2 17:35:21 CDT 2002) with mixer (40/20 to go)
>   mixer       (17:35:21) 13.0u 0.0s 1:05 19% 0+0k 0+0io 0pf+0w
:ENERGY convergence:  0 0 0
:CHARGE convergence:  0 0 0

cycle 2     (Wednesday October  2 17:36:30 CDT 2002)

cycle 2     (39/19 to go)
>   lapw0       (17:36:30) 69.0u 0.0s 4:45 24% 0+0k 0+0io 0pf+0w
:FORCE convergence:  0 1. 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO
>   lapw1       (17:41:43) 45834.0u 108.0s 23:20:29 54% 0+0k 0+0io 0pf+0w
>   lapw2       (17:02:14) 2228.0u 44.0s 46:20 81% 0+0k 0+0io 0pf+0w
>   lcore       (17:48:35) 0.0u 0.0s 0:03 0% 0+0k 0+0io 0pf+0w
>   mixer       (17:48:44) 13.0u 0.0s 0:16 77% 0+0k 0+0io 0pf+0w
:ENERGY convergence:  0 0 11732.1216010000000000
:CHARGE convergence:  0 0 .0410162

cycle 3     (Thursday October  3 17:49:05 CDT 2002)

cycle 3     (38/18 to go)
>   lapw0       (17:49:05) 73.0u 0.0s 1:24 86% 0+0k 0+0io 0pf+0w
:FORCE convergence:  0 1. 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO
>   lapw1       (17:50:44) 46437.0u 143.0s 14:39:53 88% 0+0k 0+0io 0pf+0w
>   lapw2       (08:30:38) 2148.0u 38.0s 42:03 86% 0+0k 0+0io 0pf+0w
>   lcore       (09:12:42) 0.0u 0.0s 0:03 0% 0+0k 0+0io 0pf+0w
>   mixer       (09:12:52) 13.0u 0.0s 0:17 76% 0+0k 0+0io 0pf+0w
:ENERGY convergence:  0 0 5866.5759085000000000
:CHARGE convergence:  0 0 .0398830

 cycle 4 (Friday October 4 09:13:13 CDT 2002)

cycle 4     (37/17 to go)
>   lapw0       (09:13:13) 71.0u 0.0s 1:18 90% 0+0k 0+0io 0pf+0w
:FORCE convergence:  0 1. 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO
>   lapw1       (09:14:44) 45305.0u 117.0s 16:42:28 75% 0+0k 0+0io 0pf+0w
>   lapw2       (01:57:13) 2048.0u 38.0s 39:18 88% 0+0k 0+0io 0pf+0w
>   lcore       (02:36:32) 0.0u 0.0s 0:03 0% 0+0k 0+0io 0pf+0w
>   mixer       (02:36:41) 13.0u 0.0s 0:15 83% 0+0k 0+0io 0pf+0w
:ENERGY convergence:  0 0 .7647320000000000
:CHARGE convergence:  0 0 .0390583

cycle 5 (Saturday October 5 02:36:59 CDT 2002)

cycle 5     (36/16 to go)
>   lapw0       (02:36:59) 68.0u 0.0s 1:13 92% 0+0k 0+0io 0pf+0w
:FORCE convergence:  1 1. 0 XCO 0 XCO 0 XCO 0 XCO 0 XCO .1155000000000000
XCO .2215000000000000 XCO
>   lapw1       (02:38:36) 43686.0u 175.0s 12:45:03 95% 0+0k 0+0io 0pf+0w
>   lapw2       (15:23:40) 16605.0u 39.0s 5:16:03 87% 0+0k 0+0io 0pf+0w

>   lcore       (20:39:44) 0.0u 0.0s 0:01 0% 0+0k 0+0io 0pf+0w
>   mixer       (20:39:55) 13.0u 0.0s 0:16 79% 0+0k 0+0io 0pf+0w
:ENERGY convergence:  0 0 .7540850000000000
:CHARGE convergence:  0 0 .0381198

cycle 6     (Saturday October  5 20:40:14 CDT 2002)

cycle 6     (0/15 to go)

>   stop
>   mini (20:40:15) 0.0u 0.0s 0:00 0% 0+0k 0+0io 0pf+0w

>   stop error


Could you pleaselet me know what is wrong for my min_lapw?

Thank you in adavance!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Mon, 7 Oct 2002 18:15:32 +0200
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: bcc Cs, convergence of Etot wrt GMAX

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Dear Ingo Loa,

in WIEN97 there was an internal limit on the value of GMAX, reducing it to
25 (I think) if the user specified a larger value.  Maybe you could check in
your .in2(c)-file that you are indeed going up to 50, or in your .outputd
that more plane waves are indeed being used.  Perhaps you've just been doing
the same calculation over and over again.
Also, GMAX is not the cutoff of a basis like (r)kmax, so there is no
variational principle for the energy.  So 'convergence wrt gmax' does not
mean quite the same as 'convergence wrt kmax', as was pointed out recently
on the mailing list.

Apart from that, if you still have problems with such incredibly high
GMAX-values, are you sure there are no problems elsewhere in your
calculation?

kind regards,

Kevin Jorissen
EMAT, University of Antwerp



- ----- Original Message -----
From: "Ingo Loa" <I.Loa@fkf.mpg.de>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Monday, October 07, 2002 4:45 PM
Subject: [WIEN]: bcc Cs, convergence of Etot wrt GMAX


> ====
> Ingo Loa <I.Loa@fkf.mpg.de>
> submitted the following contribution:
> ====
>
> Dear Wien2k team & users,
>
> when looking at the pressure-induced bcc-to-fcc transition in Cs by
> total-energy calculations, I recently encountered the following
> difficulties. I could easily converge the total energy as a function of
> RKMAX and number of k-points. Convergence with regard to GMAX, however,
was
> extremely slow. Even with GMAX values as large as 50, the total energy of
> the bcc phase was still not converged on the 1-meV/atom level. This
appears
> rather unusual to me, especially, because it occurs in a fairly simple
> system. A summary of typical input files is given below, the calculations
> were performed with a recent release of Wien2k.
>
> Does anybody have an idea of what may cause these troubles or how to
> proceed? Any comments/suggestions are welcome.
>
> Regards,
> Ingo Loa
>
>
> *************************************************************************
>
> Cs-bcc.struct:
>
> Cs-bcc
> B   LATTICE,NONEQUIV. ATOMS: 1
> MODE OF CALC=RELA unit=ang
>   11.515569 11.515569 11.515569 90.000000 90.000000 90.000000
> ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
>            MULT= 1          ISPLIT=
> 2
> Cs         NPT=  781  R0=0.00001000 RMT=    2.0000   Z: 55.0
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                       0.0000000 1.0000000
> 0.0000000
>                       0.0000000 0.0000000
> 1.0000000
>    48      NUMBER OF SYMMETRY
> OPERATIONS
> --------------------------------------------------------------------------
> Cs-bcc.in0:
>
> TOT   13     (5...CA-LDA, 13...PBE-GGA, 14...PW2-GGA)
> NR2V      (R2V)
> --------------------------------------------------------------------------
> Cs-bcc.in1:
>
> WFFIL        (WFPRI, SUPWF)
>    8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
>   -.14794   6   0      global e-param with N other choices, napw
>   0    0.103     0.000 CONT 1
>   0   -1.602     0.000 CONT 1
>   1    0.116     0.000 CONT 1
>   1   -0.633     0.000 CONT 1
>   2    0.132     0.000 CONT 1
>   2   -5.087     0.000 CONT 1
> K-VECTORS FROM UNIT:4    -8.0      2.5      emin/emax window
> --------------------------------------------------------------------------
> Cs-bcc.in2:
>
> TOT             (TOT,FOR,QTL,EFG,FERMI)
>        -9.0      19.0 0.50 0.05                EMIN, NE, ESEPERMIN,
ESEPER0
> TETRA    0.000          (GAUSS,ROOT,TEMP,TETRA,ALL      eval)
>   0 0 4 0 4 4 6 0 6 4
>   55.          GMAX
> FILE        FILE/NOFILE  write recprlist
> --------------------------------------------------------------------------
> Cs-bcc.klist:
>
> 165 k-points in the irreducible wedge, 4913 points in total.
> --------------------------------------------------------------------------
>
>
>
>
>
> --------------------------------------------------------------------------
> Ingo Loa
> Max-Planck-Institut fuer Festkoerperforschung, Stuttgart
> Heisenbergstr. 1        //   D-70569 Stuttgart   //   Germany
> Tel. +49.711.689-1469   //   Fax. +49.711.689-1444
> I.Loa@fkf.mpg.de        //   http://www.mpi-stuttgart.mpg.de/hd
> --------------------------------------------------------------------------
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

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------------------------------

Date: Mon, 7 Oct 2002 18:18:01 +0200
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: bcc Cs, convergence of Etot wrt GMAX

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====



Here it is (beginning of dstart.f) :

      gmax=9.0
      read(15,*,end=26) gmax1
      if((gmax1.gt.6.d0).and.(gmax1.lt.25.d0)) gmax=gmax1
   26 continue


so by specifying a very large gmax, you'll end up with an unexpectedly small
value instead ...

kind regards,

Kevin Jorissen
EMAT, University of Antwerp

- ----- Original Message -----
From: "Ingo Loa" <I.Loa@fkf.mpg.de>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Monday, October 07, 2002 4:45 PM
Subject: [WIEN]: bcc Cs, convergence of Etot wrt GMAX


> ====
> Ingo Loa <I.Loa@fkf.mpg.de>
> submitted the following contribution:
> ====
>
> Dear Wien2k team & users,
>
> when looking at the pressure-induced bcc-to-fcc transition in Cs by
> total-energy calculations, I recently encountered the following
> difficulties. I could easily converge the total energy as a function of
> RKMAX and number of k-points. Convergence with regard to GMAX, however,
was
> extremely slow. Even with GMAX values as large as 50, the total energy of
> the bcc phase was still not converged on the 1-meV/atom level. This
appears
> rather unusual to me, especially, because it occurs in a fairly simple
> system. A summary of typical input files is given below, the calculations
> were performed with a recent release of Wien2k.
>
> Does anybody have an idea of what may cause these troubles or how to
> proceed? Any comments/suggestions are welcome.
>
> Regards,
> Ingo Loa
>
>
> *************************************************************************
>
> Cs-bcc.struct:
>
> Cs-bcc
> B   LATTICE,NONEQUIV. ATOMS: 1
> MODE OF CALC=RELA unit=ang
>   11.515569 11.515569 11.515569 90.000000 90.000000 90.000000
> ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
>            MULT= 1          ISPLIT=
> 2
> Cs         NPT=  781  R0=0.00001000 RMT=    2.0000   Z: 55.0
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                       0.0000000 1.0000000
> 0.0000000
>                       0.0000000 0.0000000
> 1.0000000
>    48      NUMBER OF SYMMETRY
> OPERATIONS
> --------------------------------------------------------------------------
> Cs-bcc.in0:
>
> TOT   13     (5...CA-LDA, 13...PBE-GGA, 14...PW2-GGA)
> NR2V      (R2V)
> --------------------------------------------------------------------------
> Cs-bcc.in1:
>
> WFFIL        (WFPRI, SUPWF)
>    8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
>   -.14794   6   0      global e-param with N other choices, napw
>   0    0.103     0.000 CONT 1
>   0   -1.602     0.000 CONT 1
>   1    0.116     0.000 CONT 1
>   1   -0.633     0.000 CONT 1
>   2    0.132     0.000 CONT 1
>   2   -5.087     0.000 CONT 1
> K-VECTORS FROM UNIT:4    -8.0      2.5      emin/emax window
> --------------------------------------------------------------------------
> Cs-bcc.in2:
>
> TOT             (TOT,FOR,QTL,EFG,FERMI)
>        -9.0      19.0 0.50 0.05                EMIN, NE, ESEPERMIN,
ESEPER0
> TETRA    0.000          (GAUSS,ROOT,TEMP,TETRA,ALL      eval)
>   0 0 4 0 4 4 6 0 6 4
>   55.          GMAX
> FILE        FILE/NOFILE  write recprlist
> --------------------------------------------------------------------------
> Cs-bcc.klist:
>
> 165 k-points in the irreducible wedge, 4913 points in total.
> --------------------------------------------------------------------------
>
>
>
>
>
> --------------------------------------------------------------------------
> Ingo Loa
> Max-Planck-Institut fuer Festkoerperforschung, Stuttgart
> Heisenbergstr. 1        //   D-70569 Stuttgart   //   Germany
> Tel. +49.711.689-1469   //   Fax. +49.711.689-1444
> I.Loa@fkf.mpg.de        //   http://www.mpi-stuttgart.mpg.de/hd
> --------------------------------------------------------------------------
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

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------------------------------

Date: Mon, 7 Oct 2002 19:03:46 +0200
From: "koitzsch" <Christian.Koitzsch@unifr.ch>
Subject: Re: [WIEN]: open core treatment

====
"koitzsch" <Christian.Koitzsch@unifr.ch>
submitted the following contribution:
====

Hi Stefaan and everybody else in the User List,

I tried both suggestions - first I changed to
4, 3,6
4,-4,1

and then a bigger shift, unfortunately both had no effect, the error message
remains the same.

Christian Koitzsch
University of Fribourg
Department of Physics
CH-1700 Fribourg



- ----- Original Message -----
From: "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Monday, October 07, 2002 6:01 PM
Subject: Re: [WIEN]: open core treatment


> ====
> "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
> submitted the following contribution:
> ====
>
> >  LAPW0 END
> >  LAPW1 END
> >  LAPW2 END
> > forrtl: severe (64): input conversion error, unit 20, file
> > /home/koitzsch/GdSi/GdSi.struct
> >    0: _call_remove_gp_range [0x3ff81a6c374]
> >    1: _call_remove_gp_range [0x3ff81a6c8f4]
> >    2: _call_remove_gp_range [0x3ff81a93b84]
> >    3: _call_remove_gp_range [0x3ff81a926e0]
> >    4: insld_ [insld.f: 92, 0x12000928c]
> >    5: hfsd_ [hfsd.f: 127, 0x120005ffc]
> >    6: main [for_main.c: 203, 0x120002554]
> >    7: __start [0x1200024c8]
> >
> > Does anybody know, what I am doing wrong here.
>
> Your problem is in lcore. Two suggestions :
>
> 1) Try to fill first the core orbitals like this (completely fill one, and
> only then go to the next):
> > 4, 3,6
> > 4,-4,1
>
> 2) Try a slightly larger shift (0.8, 0.9).
>
> Stefaan
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>


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------------------------------

Date: Mon, 7 Oct 2002 13:28:43 -0500 (CDT)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: min_lapw (fwd)

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

The file mini.error contains the following information:

 'MINI' - can't open unit:  5
 'MINI' -        filename: chiolite.inM
 'MINI' -          status: old          form: formatted

It might help you to guess what is wrong with my min_lapw procedure.

Best wishes!



====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

After the SCF cycles, I run min_lapw, it stoped after 5 cycles with the
following information on my screen:

run_lapw -I -fc 1. -renorm -i 40
hup: Command not found
STOP:  MIXER END
in cycle 2    ETEST: 0   CTEST: 0
hup: Command not found
STOP:  LAPW0 END
STOP:  LAPW1 END
STOP:  LAPW2 END
STOP:  CORE  END
STOP:  MIXER END
in cycle 3    ETEST: 11732.1216010000000000   CTEST: .0410162
hup: Command not found
STOP:  LAPW0 END
STOP:  LAPW1 END
STOP:  LAPW2 END
STOP:  CORE  END
STOP:  MIXER END
in cycle 4    ETEST: 5866.5759085000000000   CTEST: .0398830
hup: Command not found
STOP:  LAPW0 END
STOP:  LAPW1 END
STOP:  LAPW2 END
STOP:  CORE  END
STOP:  MIXER END
in cycle 5    ETEST: .7647320000000000   CTEST: .0390583
hup: Command not found
STOP:  LAPW0 END
STOP:  LAPW1 END
STOP:  LAPW2 END
STOP:  CORE  END
STOP:  MIXER END
STOP: MINI - Error


I checked the case.file as following:

Calculating chiolite in /local/project00/umbingz/mysamples/chiolite
on mira

start       (Wednesday October  2 17:35:21 CDT 2002) with mixer (40/20 to go)
>   mixer       (17:35:21) 13.0u 0.0s 1:05 19% 0+0k 0+0io 0pf+0w
:ENERGY convergence:  0 0 0
:CHARGE convergence:  0 0 0

cycle 2     (Wednesday October  2 17:36:30 CDT 2002)

cycle 2     (39/19 to go)
>   lapw0       (17:36:30) 69.0u 0.0s 4:45 24% 0+0k 0+0io 0pf+0w
:FORCE convergence:  0 1. 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO
>   lapw1       (17:41:43) 45834.0u 108.0s 23:20:29 54% 0+0k 0+0io 0pf+0w
>   lapw2       (17:02:14) 2228.0u 44.0s 46:20 81% 0+0k 0+0io 0pf+0w
>   lcore       (17:48:35) 0.0u 0.0s 0:03 0% 0+0k 0+0io 0pf+0w
>   mixer       (17:48:44) 13.0u 0.0s 0:16 77% 0+0k 0+0io 0pf+0w
:ENERGY convergence:  0 0 11732.1216010000000000
:CHARGE convergence:  0 0 .0410162

cycle 3     (Thursday October  3 17:49:05 CDT 2002)

cycle 3     (38/18 to go)
>   lapw0       (17:49:05) 73.0u 0.0s 1:24 86% 0+0k 0+0io 0pf+0w
:FORCE convergence:  0 1. 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO
>   lapw1       (17:50:44) 46437.0u 143.0s 14:39:53 88% 0+0k 0+0io 0pf+0w
>   lapw2       (08:30:38) 2148.0u 38.0s 42:03 86% 0+0k 0+0io 0pf+0w
>   lcore       (09:12:42) 0.0u 0.0s 0:03 0% 0+0k 0+0io 0pf+0w
>   mixer       (09:12:52) 13.0u 0.0s 0:17 76% 0+0k 0+0io 0pf+0w
:ENERGY convergence:  0 0 5866.5759085000000000
:CHARGE convergence:  0 0 .0398830

 cycle 4 (Friday October 4 09:13:13 CDT 2002)

cycle 4     (37/17 to go)
>   lapw0       (09:13:13) 71.0u 0.0s 1:18 90% 0+0k 0+0io 0pf+0w
:FORCE convergence:  0 1. 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO 0 YCO
>   lapw1       (09:14:44) 45305.0u 117.0s 16:42:28 75% 0+0k 0+0io 0pf+0w
>   lapw2       (01:57:13) 2048.0u 38.0s 39:18 88% 0+0k 0+0io 0pf+0w
>   lcore       (02:36:32) 0.0u 0.0s 0:03 0% 0+0k 0+0io 0pf+0w
>   mixer       (02:36:41) 13.0u 0.0s 0:15 83% 0+0k 0+0io 0pf+0w
:ENERGY convergence:  0 0 .7647320000000000
:CHARGE convergence:  0 0 .0390583

cycle 5 (Saturday October 5 02:36:59 CDT 2002)

cycle 5     (36/16 to go)
>   lapw0       (02:36:59) 68.0u 0.0s 1:13 92% 0+0k 0+0io 0pf+0w
:FORCE convergence:  1 1. 0 XCO 0 XCO 0 XCO 0 XCO 0 XCO .1155000000000000
XCO .2215000000000000 XCO
>   lapw1       (02:38:36) 43686.0u 175.0s 12:45:03 95% 0+0k 0+0io 0pf+0w
>   lapw2       (15:23:40) 16605.0u 39.0s 5:16:03 87% 0+0k 0+0io 0pf+0w

>   lcore       (20:39:44) 0.0u 0.0s 0:01 0% 0+0k 0+0io 0pf+0w
>   mixer       (20:39:55) 13.0u 0.0s 0:16 79% 0+0k 0+0io 0pf+0w
:ENERGY convergence:  0 0 .7540850000000000
:CHARGE convergence:  0 0 .0381198

cycle 6     (Saturday October  5 20:40:14 CDT 2002)

cycle 6     (0/15 to go)

>   stop
>   mini (20:40:15) 0.0u 0.0s 0:00 0% 0+0k 0+0io 0pf+0w

>   stop error


Could you pleaselet me know what is wrong for my min_lapw?

Thank you in adavance!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Mon,  7 Oct 2002 22:05:15 +0200
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: min_lapw (fwd)

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> Bing Zhou <umbingz@cc.UManitoba.CA>
> submitted the following contribution:
> ====
> 
> The file mini.error contains the following information:
> 
>  'MINI' - can't open unit:  5
>  'MINI' -        filename: chiolite.inM
>  'MINI' -          status: old          form: formatted
> 
> It might help you to guess what is wrong with my min_lapw procedure.

Take the usersguide and read the sections on mini and min_lapw. You did not 
create a chiolite.inM file (input file for mini), and the fact you didn't do 
that shows that you should first read the basics about mini. The philosophy of 
min_lapw has been dealt with several times in the mailing list, check the 
digests.

Stefaan
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------------------------------

Date: Tue, 8 Oct 2002 08:08:15 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: open core treatment

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> I tried both suggestions - first I changed to
> 4, 3,6
> 4,-4,1
>
> and then a bigger shift, unfortunately both had no effect, the error
message
> remains the same.
I am pretty sure that your problem in lcore will be fixed using the shift of
1.0 in the case.inc file.
Your,
S. Jalali.

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------------------------------

Date: Tue, 08 Oct 2002 09:19:21 +0200
From: Ingo Loa <I.Loa@fkf.mpg.de>
Subject: Re: [WIEN]: bcc Cs, convergence of Etot wrt GMAX

====
Ingo Loa <I.Loa@fkf.mpg.de>
submitted the following contribution:
====

Dear Kevin Jorissen,

thank you for your comments.


At 18:18 07.10.2002 +0200, you wrote:
>====
>"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
>submitted the following contribution:
>====
>
>Here it is (beginning of dstart.f) :
>
>       gmax=9.0
>       read(15,*,end=26) gmax1
>       if((gmax1.gt.6.d0).and.(gmax1.lt.25.d0)) gmax=gmax1
>    26 continue
>
>
>so by specifying a very large gmax, you'll end up with an unexpectedly small
>value instead ...


As far as I understand, GMAX is forced to be less than 25 only in dstart, 
i.e., only during the initialization. In the SCF cycle, lapw2 seems to use 
GMAX as requested by me, see the following line out of <case>.scf.

:GMA  : POTENTIAL AND CHARGE CUT-OFF  55.00 Ry**.5


While you are probably right that the total energy is not variational with 
GMAX, I would still expect it to give some stable solution once the charge 
density and potential are expanded accurately enough. Below you find the 
evolution of ETOT with GMAX for a series of calculations. As you can see, 
ETOT increases monotonically with GMAX, levels off above GMAX ~ 30, but it 
still changes by 0.12 mRy when going from GMAX=45 to GMAX=55.

GMAX    ETOT

20      -15580.55975
24      -15580.55936
28      -15580.55891
35      -15580.55854
45      -15580.55826
55      -15580.55814


The reason why I insist in having a converged solution is that the energy 
difference between bcc and fcc Cs is very small, as it is for all of the 
alkali metals. And it turns out that the bcc-fcc energy difference at 
equilibrium volume decreases with increasing GMAX. In order to make some 
statement on the stable phase and phase transition pressure/volume, one 
needs a well-converged calculation.

Regards,
Ingo Loa


>----- Original Message -----
>From: "Ingo Loa" <I.Loa@fkf.mpg.de>
>To: <wien@zeus.theochem.tuwien.ac.at>
>Sent: Monday, October 07, 2002 4:45 PM
>Subject: [WIEN]: bcc Cs, convergence of Etot wrt GMAX
>
>
> > ====
> > Ingo Loa <I.Loa@fkf.mpg.de>
> > submitted the following contribution:
> > ====
> >
> > Dear Wien2k team & users,
> >
> > when looking at the pressure-induced bcc-to-fcc transition in Cs by
> > total-energy calculations, I recently encountered the following
> > difficulties. I could easily converge the total energy as a function of
> > RKMAX and number of k-points. Convergence with regard to GMAX, however,
>was
> > extremely slow. Even with GMAX values as large as 50, the total energy of
> > the bcc phase was still not converged on the 1-meV/atom level. This
>appears
> > rather unusual to me, especially, because it occurs in a fairly simple
> > system. A summary of typical input files is given below, the calculations
> > were performed with a recent release of Wien2k.
> >
> > Does anybody have an idea of what may cause these troubles or how to
> > proceed? Any comments/suggestions are welcome.
> >
> > Regards,
> > Ingo Loa
> >
> >
> > *************************************************************************
> >
> > Cs-bcc.struct:
> >
> > Cs-bcc
> > B   LATTICE,NONEQUIV. ATOMS: 1
> > MODE OF CALC=RELA unit=ang
> >   11.515569 11.515569 11.515569 90.000000 90.000000 90.000000
> > ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
> >            MULT= 1          ISPLIT=
> > 2
> > Cs         NPT=  781  R0=0.00001000 RMT=    2.0000   Z: 55.0
> > LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
> >                       0.0000000 1.0000000
> > 0.0000000
> >                       0.0000000 0.0000000
> > 1.0000000
> >    48      NUMBER OF SYMMETRY
> > OPERATIONS
> > --------------------------------------------------------------------------
> > Cs-bcc.in0:
> >
> > TOT   13     (5...CA-LDA, 13...PBE-GGA, 14...PW2-GGA)
> > NR2V      (R2V)
> > --------------------------------------------------------------------------
> > Cs-bcc.in1:
> >
> > WFFIL        (WFPRI, SUPWF)
> >    8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
> >   -.14794   6   0      global e-param with N other choices, napw
> >   0    0.103     0.000 CONT 1
> >   0   -1.602     0.000 CONT 1
> >   1    0.116     0.000 CONT 1
> >   1   -0.633     0.000 CONT 1
> >   2    0.132     0.000 CONT 1
> >   2   -5.087     0.000 CONT 1
> > K-VECTORS FROM UNIT:4    -8.0      2.5      emin/emax window
> > --------------------------------------------------------------------------
> > Cs-bcc.in2:
> >
> > TOT             (TOT,FOR,QTL,EFG,FERMI)
> >        -9.0      19.0 0.50 0.05                EMIN, NE, ESEPERMIN,
>ESEPER0
> > TETRA    0.000          (GAUSS,ROOT,TEMP,TETRA,ALL      eval)
> >   0 0 4 0 4 4 6 0 6 4
> >   55.          GMAX
> > FILE        FILE/NOFILE  write recprlist
> > --------------------------------------------------------------------------
> > Cs-bcc.klist:
> >
> > 165 k-points in the irreducible wedge, 4913 points in total.
> > --------------------------------------------------------------------------
> >



- --------------------------------------------------------------------------
Ingo Loa
Max-Planck-Institut fuer Festkoerperforschung, Stuttgart
Heisenbergstr. 1        //   D-70569 Stuttgart   //   Germany
Tel. +49.711.689-1469   //   Fax. +49.711.689-1444
I.Loa@fkf.mpg.de        //   http://www.mpi-stuttgart.mpg.de/hd
- --------------------------------------------------------------------------

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Date: Tue, 8 Oct 2002 10:45:42 +0200
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: bcc Cs, convergence of Etot wrt GMAX

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Dear Ingo Loa,

you are right that the reduced value is only used for the initialisation (I
did not know this).  Lapw2 checks whether the gmax you have requested in
case.in2 is different from the one used to construct the case.recprlist, and
if it is, then a new list will be calculated (by the routine deter.f) using
the 'new' gmax.  So what you did was right (except maybe it would be better
to set gmax < 25 for the initialisation, so you'll have a better starting
potential/density than with the reset value gmax=9; and then increase it
before running the SCF).

I don't know why you cannot converge the energy better.  Maybe someone with
more insight in these potentials can answer that question.

kindly yours,

Kevin Jorissen
EMAT, University of Antwerp




- ----- Original Message -----
From: "Ingo Loa" <I.Loa@fkf.mpg.de>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Tuesday, October 08, 2002 9:19 AM
Subject: Re: [WIEN]: bcc Cs, convergence of Etot wrt GMAX


> ====
> Ingo Loa <I.Loa@fkf.mpg.de>
> submitted the following contribution:
> ====
>
> Dear Kevin Jorissen,
>
> thank you for your comments.
>
>
> At 18:18 07.10.2002 +0200, you wrote:
> >====
> >"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
> >submitted the following contribution:
> >====
> >
> >Here it is (beginning of dstart.f) :
> >
> >       gmax=9.0
> >       read(15,*,end=26) gmax1
> >       if((gmax1.gt.6.d0).and.(gmax1.lt.25.d0)) gmax=gmax1
> >    26 continue
> >
> >
> >so by specifying a very large gmax, you'll end up with an unexpectedly
small
> >value instead ...
>
>
> As far as I understand, GMAX is forced to be less than 25 only in dstart,
> i.e., only during the initialization. In the SCF cycle, lapw2 seems to use
> GMAX as requested by me, see the following line out of <case>.scf.
>
> :GMA  : POTENTIAL AND CHARGE CUT-OFF  55.00 Ry**.5
>
>
> While you are probably right that the total energy is not variational with
> GMAX, I would still expect it to give some stable solution once the charge
> density and potential are expanded accurately enough. Below you find the
> evolution of ETOT with GMAX for a series of calculations. As you can see,
> ETOT increases monotonically with GMAX, levels off above GMAX ~ 30, but it
> still changes by 0.12 mRy when going from GMAX=45 to GMAX=55.
>
> GMAX    ETOT
>
> 20      -15580.55975
> 24      -15580.55936
> 28      -15580.55891
> 35      -15580.55854
> 45      -15580.55826
> 55      -15580.55814
>
>
> The reason why I insist in having a converged solution is that the energy
> difference between bcc and fcc Cs is very small, as it is for all of the
> alkali metals. And it turns out that the bcc-fcc energy difference at
> equilibrium volume decreases with increasing GMAX. In order to make some
> statement on the stable phase and phase transition pressure/volume, one
> needs a well-converged calculation.
>
> Regards,
> Ingo Loa
>
>
> >----- Original Message -----
> >From: "Ingo Loa" <I.Loa@fkf.mpg.de>
> >To: <wien@zeus.theochem.tuwien.ac.at>
> >Sent: Monday, October 07, 2002 4:45 PM
> >Subject: [WIEN]: bcc Cs, convergence of Etot wrt GMAX
> >
> >
> > > ====
> > > Ingo Loa <I.Loa@fkf.mpg.de>
> > > submitted the following contribution:
> > > ====
> > >
> > > Dear Wien2k team & users,
> > >
> > > when looking at the pressure-induced bcc-to-fcc transition in Cs by
> > > total-energy calculations, I recently encountered the following
> > > difficulties. I could easily converge the total energy as a function
of
> > > RKMAX and number of k-points. Convergence with regard to GMAX,
however,
> >was
> > > extremely slow. Even with GMAX values as large as 50, the total energy
of
> > > the bcc phase was still not converged on the 1-meV/atom level. This
> >appears
> > > rather unusual to me, especially, because it occurs in a fairly simple
> > > system. A summary of typical input files is given below, the
calculations
> > > were performed with a recent release of Wien2k.
> > >
> > > Does anybody have an idea of what may cause these troubles or how to
> > > proceed? Any comments/suggestions are welcome.
> > >
> > > Regards,
> > > Ingo Loa
> > >
> > >
> > >
*************************************************************************
> > >
> > > Cs-bcc.struct:
> > >
> > > Cs-bcc
> > > B   LATTICE,NONEQUIV. ATOMS: 1
> > > MODE OF CALC=RELA unit=ang
> > >   11.515569 11.515569 11.515569 90.000000 90.000000 90.000000
> > > ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
> > >            MULT= 1          ISPLIT=
> > > 2
> > > Cs         NPT=  781  R0=0.00001000 RMT=    2.0000   Z: 55.0
> > > LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
> > >                       0.0000000 1.0000000
> > > 0.0000000
> > >                       0.0000000 0.0000000
> > > 1.0000000
> > >    48      NUMBER OF SYMMETRY
> > > OPERATIONS
> >
> --------------------------------------------------------------------------
> > > Cs-bcc.in0:
> > >
> > > TOT   13     (5...CA-LDA, 13...PBE-GGA, 14...PW2-GGA)
> > > NR2V      (R2V)
> >
> --------------------------------------------------------------------------
> > > Cs-bcc.in1:
> > >
> > > WFFIL        (WFPRI, SUPWF)
> > >    8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
> > >   -.14794   6   0      global e-param with N other choices, napw
> > >   0    0.103     0.000 CONT 1
> > >   0   -1.602     0.000 CONT 1
> > >   1    0.116     0.000 CONT 1
> > >   1   -0.633     0.000 CONT 1
> > >   2    0.132     0.000 CONT 1
> > >   2   -5.087     0.000 CONT 1
> > > K-VECTORS FROM UNIT:4    -8.0      2.5      emin/emax window
> >
> --------------------------------------------------------------------------
> > > Cs-bcc.in2:
> > >
> > > TOT             (TOT,FOR,QTL,EFG,FERMI)
> > >        -9.0      19.0 0.50 0.05                EMIN, NE, ESEPERMIN,
> >ESEPER0
> > > TETRA    0.000          (GAUSS,ROOT,TEMP,TETRA,ALL      eval)
> > >   0 0 4 0 4 4 6 0 6 4
> > >   55.          GMAX
> > > FILE        FILE/NOFILE  write recprlist
> >
> --------------------------------------------------------------------------
> > > Cs-bcc.klist:
> > >
> > > 165 k-points in the irreducible wedge, 4913 points in total.
> >
> --------------------------------------------------------------------------
> > >
>
>
>
> --------------------------------------------------------------------------
> Ingo Loa
> Max-Planck-Institut fuer Festkoerperforschung, Stuttgart
> Heisenbergstr. 1        //   D-70569 Stuttgart   //   Germany
> Tel. +49.711.689-1469   //   Fax. +49.711.689-1444
> I.Loa@fkf.mpg.de        //   http://www.mpi-stuttgart.mpg.de/hd
> --------------------------------------------------------------------------
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
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>

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------------------------------

Date: Tue, 8 Oct 2002 11:28:21 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: bcc Cs, convergence of Etot wrt GMAX

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

I must admit I'm also a little bit annoyed by the slow convergence of E-tot
with respect to GMAX.
One possible reason could be the small RMT value of 2.0 for such a heavy
element. (We know that one needs a large GMAX for H with it's small sphere).
I do NOT suggest RMTs as large as possible, but try 2.5-3.0 bohr. (It should
be faster anyway).

I have, however, also some other remarks.
If you are looking for such small energy differences, is RKMAX=8 converged ?
(Probably not absolutely, but the resulting energy differences may be stable).
> > >    8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT

The number of k-points seems incredibly small to me for high accuracy!!
> > > 165 k-points in the irreducible wedge, 4913 points in total.


Regards

> While you are probably right that the total energy is not variational with
> GMAX, I would still expect it to give some stable solution once the charge
> density and potential are expanded accurately enough. Below you find the
> evolution of ETOT with GMAX for a series of calculations. As you can see,
> ETOT increases monotonically with GMAX, levels off above GMAX ~ 30, but it
> still changes by 0.12 mRy when going from GMAX=45 to GMAX=55.
>
> GMAX    ETOT
>
> 20      -15580.55975
> 24      -15580.55936
> 28      -15580.55891
> 35      -15580.55854
> 45      -15580.55826
> 55      -15580.55814
>
>
> The reason why I insist in having a converged solution is that the energy
> difference between bcc and fcc Cs is very small, as it is for all of the
> alkali metals. And it turns out that the bcc-fcc energy difference at
> equilibrium volume decreases with increasing GMAX. In order to make some
> statement on the stable phase and phase transition pressure/volume, one
> needs a well-converged calculation.


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 08 Oct 2002 21:01:46 +0900
From: Satoshi Okada <okada@hpc.co.jp>
Subject: Re: [WIEN]: lapw2 & ifc on LINUX

====
Satoshi Okada <okada@hpc.co.jp>
submitted the following contribution:
====


Dear all,

Thank you for your advice, but extra field of record did't fix my
problem.

And I find another hit of this issue. For my old enviroment,
the variable SCRATCH was set to /tmp. But when I set SCRATCH to current
directory(on Network File System), all binary data can be read correctly
 and lapw2 fin !!

So, I think ifc & NFS read/write of LINUX cause this problem.
I will ask INTEL this problem again.

Regargs.

Peter Blaha wrote:
> > I try to make WIEN2k with ifc(Intel Fortran Compiler) on LINUX.
> >
> > When WIEN2k(lapw2) read a vector data file ( UNIT 10 ),
> > the illegal values were inputed for kx_buf,ky_buf,kz_buf
> > after about 400byte reading.
> >
> > SRC_lapw2/read_vec.F:
> >      54   IF(myid.EQ.0) THEN
> >      55      WRITE(31,205) s,t,z,n,ne,bname
> >      56      READ(10) (kx_buf(i),ky_buf(i),kz_buf(i),
> >               i=1,n-(nlo+nlon+nlov)),
> >                 (kxlo(i),kylo(i),kzlo(i),i=1,(nlo+nlon+nlov))
> >      57   ENDIF
> 
> On our system we also use the ifc compiler and have no problems at all.
> However, since this compiler is still under development, a lot may depend
> on the version of the compiler.
> 
> I have one suggestion for testing:
> Add in     SRC_lapw2/read_vec.F:
> 
>   CHARACTER*3        IPGR
> 
> and change the following line:
>   IF (myid.EQ.0) READ(10,IOSTAT=ios) s,t,z,bname,n,ne,ipgr
> 
> ipgr is written by lapw1/tapewf.F
> Usually partial reads ignore longer records and with the next read
> the next record is read and everything is fine. Maybe the ifc does not like
> this.
> 
> PS: Please let me know if this fixes your problem. (The final
> solution should be to remove   ipgr from tapewf.F since it is no longer needed.
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Date: Tue, 8 Oct 2002 13:42:10 +0100 (BST)
From: Dave Pankhurst <david.pankhurst@materials.oxford.ac.uk>
Subject: [WIEN]: sgroup

====
Dave Pankhurst <david.pankhurst@materials.oxford.ac.uk>
submitted the following contribution:
====

Dear Wien users,

I have a comment I would like to make about sgroup.  First of all, I'd
like to congratulate the authors on an excellent and very useful program.
I am using it to find the symmetry of distorted unit cells for the purpose
of calculating elastic constants in non cubic materials.

My minor niggle concerns numerical precision.  In one particular case
sgroup detects tetragonal body centred symmetry and the output is as
follows.

(case.outputsgroup)

Bravais lattice: Tetragonal body centred

     a             b            c
 5.77803900    5.77803900   16.37833700
     alpha         beta         gamma
 90.00000000    90.00000000   90.00000100

However, as you can see, there is a small error in gamma due, presumably,
to the fact that the lattice parameters in the struct file are only given
to 6 decimal places.  However, having detected that the system is
tetragonal, should not the program _automatically_ set all angles to
exactly 90 degrees?  The problem with this small error is that the
symmetry program that follows in init_lapw seems to be quite pedantic
about angles.  In fact, based on the struct file produced by sgroup in
this case, symmetry thinks the structure is monoclinic.

I have occasionally noticed a few other numerical errors.  Like the
following case where sgroup chooses to shift the atomic z coordinate of a
particular atom

ATOM= -2: X=0.16621400 Y=0.33242800 Z=0.00000000

by half a C lattice vector ...

(case.struct_sgroup)

ATOM=  2: X=0.16621400 Y=0.33242800 Z=0.50000017

again, a small numerical error seems to have been incurred in calculating
the shifted z coordinate.  This time it is not large enough to perturb the
symmetry program but I'm not sure if this is the desired behaviour.

Btw. I have verified that this behaviour occurs using both portland and hp
compilers.

Sorry if these problems seem trivial but, in the first case at least,
there do seem to be some problems of consistency between the separate wien
programs.

best regards,

	Dave Pankhurst

+---------------------------------+------------------------------------+
| Dr David Pankhurst,             | Tel : +44 1865 283325/283326       |
| Department of Materials,        | Fax : +44 1865 273789              |    
| University of Oxford,           |                                    |
| Parks Road, Oxford OX1 3PH, UK  | david.pankhurst@materials.ox.ac.uk |
+---------------------------------+------------------------------------+


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------------------------------

Date: Tue, 8 Oct 2002 16:03:49 +0200
From: "koitzsch" <Christian.Koitzsch@unifr.ch>
Subject: [WIEN]: still open core

====
"koitzsch" <Christian.Koitzsch@unifr.ch>
submitted the following contribution:
====

Hi everybody,

I am still struggling with the open core treatment of 4f electrons. After
some unsuccessfull attempts with GdSi (see previous mails, the suggested
shift of 1.0 did not work either, Saeid), I tried to repeat the fcc Yb
example, but I get the exact same error message, so I am wondering if I miss
something on the FAQ page or do sth. else wrong?

I just ran the normal calculation with 50 kpoints, but this should be
irrelevant for this open core problem?

the struct file:

Title
F   LATTICE,NONEQUIV. ATOMS: 1                     225 Fm-3m
MODE OF CALC=RELA
  8.474000  8.474000  8.474000 90.000000 90.000000 90.000000
ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT= 2
Yb         NPT=  781  R0=0.00001000 RMT=    2.5000   Z: 70.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
  48      NUMBER OF SYMMETRY OPERATIONS


then in Yb.scf:

ATOMIC SPHERE DEPENDENT PARAMETERS FOR ATOM  Yb

          OVERALL ENERGY PARAMETER IS    0.3000
          E( 0)=    0.3000
          E( 0)=   -3.1225   E(BOTTOM)=   -3.240   E(TOP)=   -3.005
          E( 1)=   -1.1000   E(BOTTOM)=   -1.440   E(TOP)=   -0.760
          E( 1)=    0.3000
          E( 3)=    0.6200   E(BOTTOM)=    0.570   E(TOP)=    0.670
          E( 2)=    0.4900   E(BOTTOM)=    0.490   E(TOP)= -200.000
Title
F   LATTICE,NONEQUIV. ATOMS: 1                     225 Fm-3m
MODE OF CALC=RELA
  8.474000  8.474000  8.474000 90.000000 90.000000 90.000000
ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT= 2
Yb         NPT=  781  R0=0.00001000 RMT=    2.5000   Z: 70.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000

so I guess a shift of 0.7 should be fine?

Yb.in1old:

WFFIL        (WFPRI, SUPWF)
  8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  0.30    6      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
 0    0.30      0.000 CONT
 0   -4.06      0.005 STOP
 1   -1.85      0.010 CONT
 1    0.30      0.000 CONT
 3    0.30      0.010 CONT
 2    0.30      0.010 CONT
K-VECTORS FROM UNIT:4    -7.0      1.5      emin/emax window

Yb.in1new

WFFIL        (WFPRI, SUPWF)
  8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  0.30    6      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
 0    0.30      0.000 CONT
 0   -4.06      0.005 STOP
 1   -1.85      0.010 CONT
 1    0.30      0.000 CONT
 3   -1.00      0.000 CONT
 2    0.30      0.010 CONT
K-VECTORS FROM UNIT:4    -7.0      1.5      emin/emax window

Yb.in2old

TOT             (TOT,FOR,QTL,EFG,FERMI)
      -9.0      24.0                EMIN, NE
TETRA    0.000          (GAUSS,ROOT,TEMP,TETRA,ALL      eval)
 0 0 4 0 4 4 6 0 6 4
 10.          GMAX
FILE        FILE/NOFILE  write recprlist

Yb.in2new

TOT             (TOT,FOR,QTL,EFG,FERMI)
      -9.0      11.0                EMIN, NE
TETRA    0.000          (GAUSS,ROOT,TEMP,TETRA,ALL      eval)
 0 0 4 0 4 4 6 0 6 4
 10.          GMAX
FILE        FILE/NOFILE  write recprlist

new Yb.inc

16 0.70     NUMBER OF ORBITALS (EXCLUDING SPIN)
1,-1,2               ( N,KAPPA,OCCUP)
2,-1,2               ( N,KAPPA,OCCUP)
2, 1,2               ( N,KAPPA,OCCUP)
2,-2,4               ( N,KAPPA,OCCUP)
3,-1,2               ( N,KAPPA,OCCUP)
3, 1,2               ( N,KAPPA,OCCUP)
3,-2,4               ( N,KAPPA,OCCUP)
3, 2,4               ( N,KAPPA,OCCUP)
3,-3,6               ( N,KAPPA,OCCUP)
4,-1,2               ( N,KAPPA,OCCUP)
4, 1,2               ( N,KAPPA,OCCUP)
4,-2,4               ( N,KAPPA,OCCUP)
4, 2,4               ( N,KAPPA,OCCUP)
4,-3,6               ( N,KAPPA,OCCUP)
4, 3,6
4,-4,7
 0




Error Message:
LAPW0 END
 LAPW1 END
 LAPW2 END
forrtl: severe (64): input conversion error, unit 20, file
/home/koitzsch/Yb/Yb.struct
   0: _call_remove_gp_range [0x3ff81a6c374]
   1: _call_remove_gp_range [0x3ff81a6c8f4]
   2: _call_remove_gp_range [0x3ff81a93b84]
   3: _call_remove_gp_range [0x3ff81a926e0]
   4: insld_ [insld.f: 92, 0x12000928c]
   5: hfsd_ [hfsd.f: 127, 0x120005ffc]
   6: main [for_main.c: 203, 0x120002554]
   7: __start [0x1200024c8]


Does anybody see, where the error is?


Thanks a lot!



Christian Koitzsch
University of Fribourg
Department of Physics
CH-1700 Fribourg
Switzerland


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------------------------------

Date: Tue, 8 Oct 2002 16:29:23 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: still open core

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I am still struggling with the open core treatment of 4f electrons. After
> some unsuccessfull attempts with GdSi (see previous mails, the suggested
> shift of 1.0 did not work either, Saeid), I tried to repeat the fcc Yb
> example, but I get the exact same error message, so I am wondering if I miss
> something on the FAQ page or do sth. else wrong?

Try a really big shift like -3. or even -10.


> then in Yb.scf:
>
> ATOMIC SPHERE DEPENDENT PARAMETERS FOR ATOM  Yb
>
>           OVERALL ENERGY PARAMETER IS    0.3000
>           E( 0)=    0.3000
>           E( 0)=   -3.1225   E(BOTTOM)=   -3.240   E(TOP)=   -3.005
>           E( 1)=   -1.1000   E(BOTTOM)=   -1.440   E(TOP)=   -0.760
>           E( 1)=    0.3000
>           E( 3)=    0.6200   E(BOTTOM)=    0.570   E(TOP)=    0.670
>           E( 2)=    0.4900   E(BOTTOM)=    0.490   E(TOP)= -200.000
> Title
> F   LATTICE,NONEQUIV. ATOMS: 1                     225 Fm-3m
> MODE OF CALC=RELA
>   8.474000  8.474000  8.474000 90.000000 90.000000 90.000000
> ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
>           MULT= 1          ISPLIT= 2
> Yb         NPT=  781  R0=0.00001000 RMT=    2.5000   Z: 70.0
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
>
> so I guess a shift of 0.7 should be fine?

This is most likely much too small.


> Yb.in1new
>
> WFFIL        (WFPRI, SUPWF)
>   8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
>   0.30    6      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
>  0    0.30      0.000 CONT
>  0   -4.06      0.005 STOP
>  1   -1.85      0.010 CONT
>  1    0.30      0.000 CONT
>  3   -1.00      0.000 CONT

Are you sure this was low enough to avoid any real 4f electrons in the valence?
Did your error happen in the first open core scf-cycle or only afterwards ?


After all:    open core calculations are not state of the art anymore.
Use LDA+U for the 4f systems.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Tue, 08 Oct 2002 18:10:26 +0200
From: Florent Boucher <Florent.Boucher@cnrs-imn.fr>
Subject: Re: [WIEN]: Pb SRC_lapw2/atpar.F and lxdos

====
Florent Boucher <Florent.Boucher@cnrs-imn.fr>
submitted the following contribution:
====

Dear Peter,
it seems to work now.
Just a small error in SRC_tetra/tetra.f because the fermden is not 
initialized

      allocate (RNUMB(jend,MG), DENSTY(jend,MG),fermden(jend))
      allocate (ehelp(jend),denbr(jend,mg))
      DENSTY=0.0
      RNUMB=0.0
      fermden=0.0        <-

In some case it crash ...
Regards and thank you.
Florent


Peter Blaha a écrit:

>Dear Florent and Kevin,
>
>It seems Georg has never converted that part to the f90 version.
>
>I'm attatching a modified atpar.F routine where I uncommented the double loop
>and set a proper index for a1lo,.... Try it and let me know if it
>works.
>PS: It will not work with relativistic LOs!
>
>Regards
>  
>
>>we are trying to use the ISPLIT=99 option in WIEN2K (latest version) and
>>we have troubles with the atpar.F program. In the distributed version
>>they are comments for the following lines:
>>!
>>!....overlap integrals for x-dos
>>!
>>!!$      do l=0,lxdos
>>!!$         do lp=0,lxdos
>>!!$            pu1u2(l,lp)=0.d0
>>!!$            pueu2(l,lp)=0.d0
>>!!$            pu2u2(l,lp)=0.d0
>>!!$            CALL RINT13(REL,rrad1(1,l),rrad2(1,l),rrad1(1,lp) &
>>!!$                 ,rrad2(1,lp),pu1u1(l,lp),JATOM)
>>!!$            CALL RINT13(REL,rrad1(1,l),rrad2(1,l),rade1(1,lp) &
>>!!$                 ,rade2(1,lp),pu1ue(l,lp),JATOM)
>>!!$            if(lp.le.lmax2) CALL RINT13(REL,rrad1(1,l),rrad2(1,l) &
>>!!$                 ,a1lo(1,lp),b1lo(1,lp),pu1u2(l,lp),JATOM)
>>!!$            CALL RINT13(REL,rade1(1,l),rade2(1,l),rade1(1,lp) &
>>!!$                 ,rade2(1,lp),pueue(l,lp),JATOM)
>>!!$            if(lp.le.lmax2) CALL RINT13(REL,rade1(1,l),rade2(1,l) &
>>!!$                 ,a1lo(1,lp),b1lo(1,lp),pueu2(l,lp),JATOM)
>>!!$            if((lp.le.lmax2).and.(l.le.lmax2)) CALL
>>RINT13(REL,a1lo(1,l) &
>>!!$                 ,b1lo(1,l),a1lo(1,lp),b1lo(1,lp),pu2u2(l,lp),JATOM)
>>!!$         enddo
>>!!$      enddo
>>
>>For this reason, the qtl file and help files have only zero values
>>(pu1u1, pueue .... are not initialized)
>>    
>>
>
>
>                                      P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>  
>
>------------------------------------------------------------------------
>
>     SUBROUTINE ATPAR (REL,NAT,JATOM,LATOM,cform,ZZ)                            
>      use param
>      use defs
>      use struk
>      use lo; USE atspdt, only: e=>el,p,dp,pe,dpe,pei
>      USE parallel
>      IMPLICIT REAL*8 (A-H,O-Z)
>#ifdef Parallel
>  INCLUDE 'mpif.h'
>#endif
>      CHARACTER*4      cform                                           
>      LOGICAL          REL
>      dimension        emist2(0:lomax,nloat)
>!                                                                       
>      COMMON /RADFU/   RRAD1(NRAD,0:LMAX2),RADE1(NRAD,0:LMAX2), &
>                       RRAD2(NRAD,0:LMAX2),RADE2(NRAD,0:LMAX2)                
>      COMMON /POTNLC/  VR(NRAD)           
>      COMMON /UHELP/   A(NRAD),B(NRAD),AP(NRAD),BP(NRAD),AE(NRAD),       &
>                       BE(NRAD)                                         
>      common /normal/  pu1u1(0:lxdos,0:lxdos),pu1ue(0:lxdos,0:lxdos) &
>                      ,pu1u2(0:lxdos,0:lxdos),pueue(0:lxdos,0:lxdos) &
>                      ,pueu2(0:lxdos,0:lxdos),pu2u2(0:lxdos,0:lxdos)
>!---------------------------------------------------------------------  
>!.....READ TOTAL SPHERICAL POTENTIAL V(0,0) OF TAPE18=VSP               
>!     NORM OF V(0,0)=V00(R)*R/SQRT(4.D0*PI)                             
>
>      READ(18,1980)                                                     
>      READ(18,2000) IDUMMY                                              
>      READ(18,2031)                                                     
>      READ(18,2022) ( VR(J), J=1,JRI(JATOM) )                           
>      READ(18,2031)                                                     
>      READ(18,2030)                                                     
>      DO J=1,JRI(JATOM)                                             
>         VR(J)=VR(J)/2.0D0                                                 
>      enddo
>!                                                                       
>      nlo=0
>      nlov=0
>      nlon=0
>! nlo #LO on this atom, nlov #LO up til now, nlon #LO left
>      ilo(0:lmax2)=0
>      DO i=1,jatom                                                   
>         IF(myid.EQ.0) THEN
>            READ(10) e
>            READ(10) elo
>         ENDIF
>#ifdef Parallel
>        CALL MPI_BCAST(e,lmax2+1,MPI_DOUBLE_PRECISION, 0, MPI_COMM_WORLD, ierr)
>        CALL MPI_BCAST(elo,(lmax2+1)*nloat,MPI_DOUBLE_PRECISION, 0, MPI_COMM_WORLD, ierr)
>#endif
>        IF(i.EQ.jatom) THEN
>           DO l=0,lmax2
>              lapw(l)=.TRUE.
>              IF(e(l).GT.150.) THEN
>                 e(l)=e(l)-200.d+0
>                 lapw(l)=.FALSE.
>              ENDIF
>           ENDDO
>        ENDIF
>        DO l = 0,lomax
>           DO k=1,nloat
>              loor(k,l)=.FALSE.
>              rlo(k,l)=.FALSE.
>              IF (i.EQ.jatom) THEN 
>                 IF (elo(l,k).LT.(995.d+0)) THEN
>                    ilo(l)=ilo(l)+1
>                    nlo=nlo+((2*l+1))*mult(i)
>                    IF(.NOT.lapw(l).AND.k.EQ.1) GOTO 666
>                    IF(k.EQ.nloat) THEN
>                          rlo(ilo(l),l)=.TRUE.
>                    ENDIF
>                    loor(ilo(l),l)=.TRUE.
>666                 CONTINUE
>                 ENDIF
>              ELSE
>                 IF (elo(l,k).LT.(995.d+0)) nlov=nlov+((2*l+1))*mult(i)
>              ENDIF
>           ENDDO
>        ENDDO
>      ENDDO
>      IF(jatom.EQ.nat) GOTO 30                                          
>      DO i=jatom+1,nat  
>         READ(10) emist                                                    
>         READ(10) emist2
>#ifdef Parallel
>        CALL MPI_BCAST(emist2,(lmax2+1)*nloat,MPI_DOUBLE_PRECISION, 0, MPI_COMM_WORLD, ierr)
>#endif         
>         DO l = 0,lomax
>            DO k=1,nloat
>               IF (emist2(l,k).LT.(995.0d+0))  &
>                    nlon=nlon+((2*l+1))*mult(i)
>            ENDDO
>         ENDDO
>      ENDDO
>  30  CONTINUE     
>      IF(myid.EQ.0) THEN
>         WRITE(6,13)  JATOM,IATNR(JATOM),(POS(I,LATOM),I=1,3) &
>              ,MULT(JATOM)        
>         WRITE(21,13) JATOM,IATNR(JATOM),(POS(I,LATOM),I=1,3) &
>              ,MULT(JATOM)        
>         WRITE(6,1060) ANAME(JATOM)                                    
>         DO JROW=1,3                                               
>            WRITE(6,1070) ( ROTLOC(JCOL,JROW,JATOM),JCOL=1,3 )         
>         ENDDO
>         INDEX=LATOM-1                                                 
>         DO M=1,MULT(JATOM)                                        
>            INDEX=INDEX+1                                               
>            WRITE(6,1080) M,( POS(JC,INDEX),JC=1,3 )                    
>            DO JR=1,3                                               
>               WRITE(6,1090)(ROTIJ(JC,JR,INDEX),JC=1,3),TAUIJ(JR,INDEX)   
>            ENDDO
>         ENDDO
>         WRITE(6,7) ANAME(JATOM)                                           
>         WRITE(6,5) E                                                      
>         WRITE(6,14)                                                       
>      ENDIF
>
>      DO 70 l=0,LMAX2                                                  
>         DELE=2.0D-3                                                       
>         DELEI=0.25D0/DELE                                                 
>         FL=L                                                              
>         EI=E(l)/2.0d0                                                         
>!                                                                       
>!     CALCULATE ENERGY-DERIVATIVE BY FINITE DIFFERENCE                  
>!     DELE IS THE UPWARD AND DOWNWARD ENERGY SHIFT IN HARTREES          
>!                                                                       
>         E1=EI-DELE                                                        
>         CALL OUTWIN(REL,VR,R0(JATOM),DX(JATOM),JRI(JATOM),E1,            &
>              FL,UVB,DUVB,NODEL,ZZ) 
>         CALL RINT13(REL,A,B,A,B,OVLP,JATOM)                               
>         TRX=1.0D0/SQRT(OVLP)                                              
>         IMAX=JRI(JATOM)                                                   
>         DO M=1,IMAX                                                    
>            AE(M)=TRX*A(M)                                                    
>            BE(M)=TRX*B(M)                                                    
>         ENDDO
>         UVB=TRX*UVB                                                       
>         DUVB=TRX*DUVB                                                     
>         E1=EI+DELE                                                        
>         CALL OUTWIN(REL,VR,R0(JATOM),DX(JATOM),JRI(JATOM),E1,            &
>              FL,UVE,DUVE,NODE,ZZ)
>         CALL RINT13(REL,A,B,A,B,OVLP,JATOM)                               
>         TRX=1.0d0/SQRT(OVLP)                                                
>         UVE=DELEI*(TRX*UVE-UVB)                                           
>         DUVE=DELEI*(TRX*DUVE-DUVB)                                        
>         IMAX=JRI(JATOM)                                                   
>         DO M=1,IMAX                                                    
>            AE(M)=DELEI*(TRX*A(M)-AE(M))                                      
>            BE(M)=DELEI*(TRX*B(M)-BE(M))                                      
>         ENDDO
>!                                                                       
>!     CALCULATE FUNCTION AT EI                                          
>!                                                                       
>         CALL OUTWIN(REL,VR(1),R0(JATOM),DX(JATOM),JRI(JATOM),EI,         &
>              FL,UV,DUV,NODES,ZZ)
>         CALL RINT13(REL,A,B,A,B,OVLP,JATOM)                               
>         TRX=1.0d0/SQRT(OVLP)                                                
>         P(l)=TRX*UV                                                       
>         DP(l)=TRX*DUV                                                     
>         IMAX=JRI(JATOM)                                                   
>         DO M=1,IMAX                                                    
>            A(M)=TRX*A(M)
>            B(M)=TRX*B(M)                                                     
>         ENDDO
>!                                                                       
>!     INSURE ORTHOGONALIZATION                                          
>!                                                                       
>         CALL RINT13(REL,A,B,AE,BE,CROSS,JATOM)                            
>         TRY=-CROSS                                                        
>         IF(TRY.LT.(-0.05d0).AND.myid.EQ.0) WRITE(6,9) L,TRY,OVLP
>         IMAX=JRI(JATOM)                                                   
>         DO M=1,IMAX                                                    
>            AE(M)=(AE(M)+TRY*A(M))
>            BE(M)=(BE(M)+TRY*B(M))                                            
>         ENDDO
>         IMAX=JRI(JATOM)                                                   
>        DO 80 I=1,IMAX                                                    
>            RRAD1(I,l)=A(I)                                                   
>            RRAD2(I,l)=B(I)                                                   
>            RADE1(I,l)=AE(I)                                                  
>            RADE2(I,l)=BE(I)                                                  
> 80      CONTINUE
>         PE(l)=UVE+TRY*P(l)                                                
>         DPE(l)=DUVE+TRY*DP(l)                                             
>         CALL RINT13(REL,AE,BE,AE,BE,PEI(l),JATOM)                         
>         IF(myid.EQ.0) WRITE(6,8) L,P(l),DP(l),PE(l),DPE(l),PEI(l),NODEL,NODES,NODE                         
> 70   continue
>!                         
>! nun fur lo
>!
>      pr12lo(1:nloat,1:nloat,0:lomax)=0.0d0
>      pi12lo(1:nloat,0:lomax)=0.0d0
>      pe12lo(1:nloat,0:lomax)=0.0d0
>      a1lo(1:nrad,1:nloat,0:lomax)=0.0d0
>      b1lo(1:nrad,1:nloat,0:lomax)=0.0d0
>
>      lo_loop: DO l=0,lomax 
>         DO jlo=1,ilo(l)
>            if (.not.loor(jlo,l)) CYCLE
>            DELE=2.0D-3                                 
>            DELEI=0.25D0/DELE 
>            FL=L
>            EI=elo(l,jlo)/2.d0 
>!     
>!     CALCULATE FUNCTION AT EI                                          
>!
>            IF(rlo(jlo,l)) THEN
>               ei=elo(l,nloat)/2.d0
>               kappa=l
>!               kappa=-2
>               CALL diracout(rel,vr(1),r0(jatom),dx(jatom),jri(jatom),   &
>                    ei,fl,kappa,uv,duv,nodes,zz)
>!!$               CALL diracout_old(rel,vr(1),r0(jatom),dx(jatom),jri(jatom),   &
>!!$                    ei,fl,kappa,uv,duv,nodes,zz)
>!               do m=1,jri(jatom)
>!                  write(78,'(2f13.7)') a(m),b(m)
>!               enddo
>               CALL dergl(a,b,r0(jatom),dx(jatom),jri(jatom))
>               DO m = 1, jri(jatom)
>                  r_m = r0(jatom)*exp(dx(jatom)*(m-1))
>                  b(m) = b(m)*r_m / (2.d0*clight+(elo(l,jlo)-2.d0*vr(m)/r_m)/(2.d0*clight))
>!                  write(79,'(2f13.7)') r_m,b(m)
>!                  b(m)=b(m)*clight
>!                   b(m)=0.0d0
>               ENDDO
>            ELSE
>               CALL outwin(rel,vr(1),r0(jatom),dx(jatom),jri(jatom),  &
>                    ei,fl,uv,duv,nodes,zz) 
>            ENDIF
>            CALL rint13(rel,a,b,a,b,ovlp,jatom)
>            TRX=1.0d0/SQRT(OVLP)
>            plo(jlo,l)=trx*uv 
>            dplo(jlo,l)=trx*duv 
>            IMAX=JRI(JATOM)
>            DO M=1,IMAX 
>               a1lo(M,jlo,l)=TRX*A(M) 
>               b1lo(M,jlo,l)=TRX*B(M) 
>            ENDDO
>            IF(l.EQ.1) THEN
>               DO m=1,imax
>                  r_m = r0(jatom)*EXP(dx(jatom)*(m-1))
>                  WRITE(94,'(4e14.6)') r_m,a1lo(m,jlo,l),rrad1(m,l),rade1(m,l)
>               ENDDO
>            ENDIF
>           CALL RINT13(REL,rrad1(1,l),rrad2(1,l),a1lo(1,jlo,l),b1lo(1,jlo,l), &
>                 pi12lo(jlo,l),JATOM)
>            CALL RINT13(REL,rade1(1,l),rade2(1,l),a1lo(1,jlo,l),b1lo(1,jlo,l), &
>                 pe12lo(jlo,l),JATOM)         
>            
>            IF(myid.EQ.0) WRITE(6,800) L,Plo(jlo,l),DPlo(jlo,l),NODEL,NODES,NODE
>         ENDDO
>
>         DO jlo=1,ilo(l)
>            CALL ABC(l,jlo,jatom)
>         ENDDO
>
>         DO jlo=1,ilo(l)
>            IF (.NOT.loor(jlo,l)) CYCLE
>            DO jlop=1,ilo(l)
>               IF (.NOT.loor(jlop,l)) CYCLE
>               CALL RINT13(REL,a1lo(1,jlop,l),b1lo(1,jlop,l), &
>                    a1lo(1,jlo,l),b1lo(1,jlo,l), &
>                    pr12lo(jlop,jlo,l),JATOM)
>            ENDDO
>         ENDDO
>      ENDDO lo_loop
>
>!
>!....overlap integrals for x-dos
>!    not for rlo's !!!!
>      do l=0,lxdos
>         do lp=0,lxdos
>            pu1u2(l,lp)=0.d0
>            pueu2(l,lp)=0.d0
>            pu2u2(l,lp)=0.d0
>            CALL RINT13(REL,rrad1(1,l),rrad2(1,l),rrad1(1,lp) &
>                 ,rrad2(1,lp),pu1u1(l,lp),JATOM)         
>            CALL RINT13(REL,rrad1(1,l),rrad2(1,l),rade1(1,lp) &
>                 ,rade2(1,lp),pu1ue(l,lp),JATOM)         
>
>            jlo=max(ilo(lp),1)
>            if(jlo.eq.3) jlo=2   !!! exclude rlo
>            if(lp.le.lmax2.and.loor(jlo,lp)) CALL RINT13(REL,rrad1(1,l),rrad2(1,l) &
>                 ,a1lo(1,jlo,lp),b1lo(1,jlo,lp),pu1u2(l,lp),JATOM)         
>            CALL RINT13(REL,rade1(1,l),rade2(1,l),rade1(1,lp) &
>                 ,rade2(1,lp),pueue(l,lp),JATOM)         
>            if(lp.le.lmax2.and.loor(jlo,lp)) CALL RINT13(REL,rade1(1,l),rade2(1,l) &
>                 ,a1lo(1,jlo,lp),b1lo(1,jlo,lp),pueu2(l,lp),JATOM)         
>            jlop=max(ilo(l),1)
>            if(jlop.eq.3) jlop=2   !!! exclude rlo
>            if((lp.le.lmax2).and.(l.le.lmax2).and.loor(jlo,lp).and.loor(jlop,l)) CALL RINT13(REL,a1lo(1,jlop,l) &
>                 ,b1lo(1,jlop,l),a1lo(1,jlo,lp),b1lo(1,jlo,lp),pu2u2(l,lp),JATOM)
>         enddo
>      enddo
>!
>      RETURN                                                            
>!                                                                       
>    2 FORMAT(5E14.7)                                                    
>    3 FORMAT(16I5)                                                      
>    4 FORMAT(I4,E16.7)                                                  
>    5 FORMAT(10X,' ENERGY PARAMETERS ARE',7F7.2)                        
>    6 FORMAT(10X,'E(',I2,')=',F10.4)                                    
>    7 FORMAT(/10X,'ATOMIC PARAMETERS FOR ',A10/)                        
>   14 FORMAT(/11X,'L',5X,'U(R)',10X,                                     &
>             'U''(R)',9X,'DU/DE',8X,'DU''/DE',6X,'NORM-U''')               
>    8 FORMAT(10X,I2,5E14.6,5X,3I2)                                      
> 800   FORMAT(10X,I2,2E14.6,42X,5X,3I2)                                      
>    9 FORMAT(10X,'FOR L=',I2,' CORRECTION=',E14.5,' OVERLAP=',E14.5)    
>   11 FORMAT(7F10.5)                                                    
>   13 FORMAT(////,':POS',i2.2,':',1x,'AT.NR.',I3,2X,'POSITION =', &
>             3F8.5,2X,'MULTIPLICITY =',I3)
> 1040 FORMAT(8I2)                                                       
> 1050 FORMAT(A10,I5,5X,2F10.9,I5,F5.2)                                  
> 1060 FORMAT(//,3X,'NOT EQUIV ATOM ',A10,'  LOCAL ROTATION MATRIX')     
> 1070 FORMAT(30X,3F10.5)                                                
> 1080 FORMAT(13X,'EQUIV ATOM ',I3,3X,'POSITION: ',3F8.3)                
> 1090 FORMAT(30X,3F10.5,5X,F10.5)                                       
> 1980 FORMAT(3X)                                                        
> 2000 FORMAT(16X,I2//)                                                  
> 2022 FORMAT(3X,4E19.12)                                                 
> 2030 FORMAT(///)                                                       
> 2031 FORMAT(/)                                                         
>      END                                                               
>  
>

- -- 
 --------------------------------------------------------------------------
| Florent BOUCHER                    |                                     |
| Institut des Matériaux Jean Rouxel | Mailto:Florent.Boucher@cnrs-imn.fr  |
| 2, rue de la Houssinière           | Phone: (33) 2 40 37 39 24           |
| BP 32229                           | Fax:   (33) 2 40 37 39 95           |
| 44322 NANTES CEDEX 3 (FRANCE)      | http://www.cnrs-imn.fr              |
 --------------------------------------------------------------------------



====
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------------------------------

Date: Tue, 8 Oct 2002 18:14:47 +0200 (MET DST)
From: Pavel Novak <novakp@fzu.cz>
Subject: Re: [WIEN]: still open core

====
Pavel Novak <novakp@fzu.cz>
submitted the following contribution:
====

Dear Christian,

you can always treat the 4f-electrons as semicore - we checked some years
ago that it is equivalent to puting them in core and there are no problems
with crash of calculation. You have to prevent the hybridization of 4f by
fixing in semicore calculation (.in1) the s, p, d energies at something
like 2Ry and similarly in valence LAPW1 you fix 4f energy at 2Ry. Semicore
calculation may be run with minimal number of k-points.

Regards
Pavel Novak

On Tue, 8 Oct 2002, koitzsch wrote:

> ====
> "koitzsch" <Christian.Koitzsch@unifr.ch>
> submitted the following contribution:
> ====
>
> Hi everybody,
>
> I am still struggling with the open core treatment of 4f electrons. After
> some unsuccessfull attempts with GdSi (see previous mails, the suggested
> shift of 1.0 did not work either, Saeid), I tried to repeat the fcc Yb
> example, but I get the exact same error message, so I am wondering if I miss
> something on the FAQ page or do sth. else wrong?
>
> I just ran the normal calculation with 50 kpoints, but this should be
> irrelevant for this open core problem?
>
> the struct file:
>
> Title
> F   LATTICE,NONEQUIV. ATOMS: 1                     225 Fm-3m
> MODE OF CALC=RELA
>   8.474000  8.474000  8.474000 90.000000 90.000000 90.000000
> ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
>           MULT= 1          ISPLIT= 2
> Yb         NPT=  781  R0=0.00001000 RMT=    2.5000   Z: 70.0
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
>   48      NUMBER OF SYMMETRY OPERATIONS
>
>
> then in Yb.scf:
>
> ATOMIC SPHERE DEPENDENT PARAMETERS FOR ATOM  Yb
>
>           OVERALL ENERGY PARAMETER IS    0.3000
>           E( 0)=    0.3000
>           E( 0)=   -3.1225   E(BOTTOM)=   -3.240   E(TOP)=   -3.005
>           E( 1)=   -1.1000   E(BOTTOM)=   -1.440   E(TOP)=   -0.760
>           E( 1)=    0.3000
>           E( 3)=    0.6200   E(BOTTOM)=    0.570   E(TOP)=    0.670
>           E( 2)=    0.4900   E(BOTTOM)=    0.490   E(TOP)= -200.000
> Title
> F   LATTICE,NONEQUIV. ATOMS: 1                     225 Fm-3m
> MODE OF CALC=RELA
>   8.474000  8.474000  8.474000 90.000000 90.000000 90.000000
> ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
>           MULT= 1          ISPLIT= 2
> Yb         NPT=  781  R0=0.00001000 RMT=    2.5000   Z: 70.0
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
>
> so I guess a shift of 0.7 should be fine?
>
> Yb.in1old:
>
> WFFIL        (WFPRI, SUPWF)
>   8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
>   0.30    6      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
>  0    0.30      0.000 CONT
>  0   -4.06      0.005 STOP
>  1   -1.85      0.010 CONT
>  1    0.30      0.000 CONT
>  3    0.30      0.010 CONT
>  2    0.30      0.010 CONT
> K-VECTORS FROM UNIT:4    -7.0      1.5      emin/emax window
>
> Yb.in1new
>
> WFFIL        (WFPRI, SUPWF)
>   8.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
>   0.30    6      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
>  0    0.30      0.000 CONT
>  0   -4.06      0.005 STOP
>  1   -1.85      0.010 CONT
>  1    0.30      0.000 CONT
>  3   -1.00      0.000 CONT
>  2    0.30      0.010 CONT
> K-VECTORS FROM UNIT:4    -7.0      1.5      emin/emax window
>
> Yb.in2old
>
> TOT             (TOT,FOR,QTL,EFG,FERMI)
>       -9.0      24.0                EMIN, NE
> TETRA    0.000          (GAUSS,ROOT,TEMP,TETRA,ALL      eval)
>  0 0 4 0 4 4 6 0 6 4
>  10.          GMAX
> FILE        FILE/NOFILE  write recprlist
>
> Yb.in2new
>
> TOT             (TOT,FOR,QTL,EFG,FERMI)
>       -9.0      11.0                EMIN, NE
> TETRA    0.000          (GAUSS,ROOT,TEMP,TETRA,ALL      eval)
>  0 0 4 0 4 4 6 0 6 4
>  10.          GMAX
> FILE        FILE/NOFILE  write recprlist
>
> new Yb.inc
>
> 16 0.70     NUMBER OF ORBITALS (EXCLUDING SPIN)
> 1,-1,2               ( N,KAPPA,OCCUP)
> 2,-1,2               ( N,KAPPA,OCCUP)
> 2, 1,2               ( N,KAPPA,OCCUP)
> 2,-2,4               ( N,KAPPA,OCCUP)
> 3,-1,2               ( N,KAPPA,OCCUP)
> 3, 1,2               ( N,KAPPA,OCCUP)
> 3,-2,4               ( N,KAPPA,OCCUP)
> 3, 2,4               ( N,KAPPA,OCCUP)
> 3,-3,6               ( N,KAPPA,OCCUP)
> 4,-1,2               ( N,KAPPA,OCCUP)
> 4, 1,2               ( N,KAPPA,OCCUP)
> 4,-2,4               ( N,KAPPA,OCCUP)
> 4, 2,4               ( N,KAPPA,OCCUP)
> 4,-3,6               ( N,KAPPA,OCCUP)
> 4, 3,6
> 4,-4,7
>  0
>
>
>
>
> Error Message:
> LAPW0 END
>  LAPW1 END
>  LAPW2 END
> forrtl: severe (64): input conversion error, unit 20, file
> /home/koitzsch/Yb/Yb.struct
>    0: _call_remove_gp_range [0x3ff81a6c374]
>    1: _call_remove_gp_range [0x3ff81a6c8f4]
>    2: _call_remove_gp_range [0x3ff81a93b84]
>    3: _call_remove_gp_range [0x3ff81a926e0]
>    4: insld_ [insld.f: 92, 0x12000928c]
>    5: hfsd_ [hfsd.f: 127, 0x120005ffc]
>    6: main [for_main.c: 203, 0x120002554]
>    7: __start [0x1200024c8]
>
>
> Does anybody see, where the error is?
>
>
> Thanks a lot!
>
>
>
> Christian Koitzsch
> University of Fribourg
> Department of Physics
> CH-1700 Fribourg
> Switzerland
>
>
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> majordomo@zeus.theochem.tuwien.ac.at
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>
>
>



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Date: Wed, 9 Oct 2002 08:22:07 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: [WIEN]: research position (fwd)

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====


- ---------- Forwarded message ----------
Date: Tue, 08 Oct 2002 20:10:44 -0600
From: Holmann Brand <brand@lanl.gov>
To: pblaha@theochem.tuwien.ac.at
Subject: research position

Dear Dr. Prof. Blaha:

I would very much appreciate it if you would
kindly forward this message to any students and
postdoctoral researchers that might be interested in
the research position described below:

The Materials Science Group of the Applied Physics Division
at Los Alamos National Laboratory is seeking postdoctoral
candidates to collaborate on the development and
application of periodic quantum mechanical methods for studying
molecular crystals.  The successful candidate will be expected
to interact with a multi-disciplinary team of theoretical and
experimental scientists.  For consideration, please send a resume
to Dr. Holmann Brand at brand@lanl.gov

Salary rates for this postdoctoral position in US dollars are:

Years since PhD:   Salary:
PhD + 0           $56,700
PhD + 1           $58,200
PhD + 2           $59,700
PhD + 3           $61,100
PhD + 4           $62,700

Sincerely,

Holmann V. Brand, Ph.D.
Materials Science Group                 Phone: 505-667-2384
Mail Stop D413                    Group Phone: 505-667-6504
Los Alamos National Laboratory    Group Fax:   505-667-3726
Los Alamos, NM 87545



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------------------------------

Date: Wed, 9 Oct 2002 20:55:38 +0800
From: "yulihua-wuhan" <yulihua-wuhan@sohu.com>
Subject: [WIEN]: charge convergence & U J value

====
"yulihua-wuhan" <yulihua-wuhan@sohu.com>
submitted the following contribution:
====

Dear Wien2k Users and developers:

   In the UG, the charge distance = Integrate[p(n)-p(n-1) ] dr, but the UG didn't tell the integration range.So if I use the charge convergence 0.0001, it means the distance in every MT sphere or the whole cell?? Of course, I think the unit is electron-charge, i.e. 0.0001 electron-charge. Are I right?
      
   I have another question about the SOC and LDA+U caculation.When I perform the "runsp -so -orb" caculation on U-based compound (with f-electron), the iteration show the oscillations of  the energe and the charge, how can I solve the problem? And anyone have the experience of choosing the U,J value in the case.inorb on this kind of compound.

   Thinks                         yulihua 

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Date: Wed, 9 Oct 2002 08:16:35 -0700 (PDT)
From: Battery Wien <batterywien@yahoo.com>
Subject: [WIEN]: Error File- lapw1

====
Battery Wien <batterywien@yahoo.com>
submitted the following contribution:
====

 This is my first time running wien 2k. I am running a
CoO2 trigonal structure. The default parameters were
used for the initialization. The run ended at lapw1
with the following error message:

 'SELECT' - no energy limits found for L= 1           
                        
 'SELECT' - E-bottom   -8.18500   E-top -200.00000

Please Advise.

Thanks.


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Date: Wed, 9 Oct 2002 10:36:31 -0700 (PDT)
From: Claudio Lee <claudio_lee1@yahoo.com>
Subject: [WIEN]: Obital polarization calculation

====
Claudio Lee <claudio_lee1@yahoo.com>
submitted the following contribution:
====

Dear all,
I have this problem, if you know the answer please
help me.
For spin polarized calculation. First step, my
calculation has been included spin-obit coupling, and
now, after this step has been done I want to include
obital polarization into my calculation. Reading the
wien2k menu, I follow the instruction but I dont know
what I am doing wrong. 
Using this script
x lapwd -up   
I got the error as it shows following:
'lapwdm' - can't open unit:  5
 'lapwdm' -        filename: Fe274.indm
 'lapwdm' -          status: old          form:
formatted

So if anyone knows about this please help me, it will
be better if you help me step by step how to include
spin-obit coupling and obital polarization into the
calculation of the spin-polarized case.  
Many thanks in advance.
Sincerely,
Claudio.



 


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Date: Wed, 09 Oct 2002 12:49:14 -0600
From: Pablo de la Mora <pm@fciencias.unam.mx>
Subject: [WIEN]: problems with parallel execution

====
Pablo de la Mora <pm@fciencias.unam.mx>
submitted the following contribution:
====

Dear Wien Users,
    I am having problems with parallel execution. I am doing a supercell 
for doping, it worked fine with a supercell with 4 cells, but with 2 
cells it crashed.

- ------------ End of the 'dayfile'
1.230u 0.930s 3:02.72 1.1%    0+0k 0+0io 60807pf+0w
 >   lapw2 -up -p    (02:06:41) running LAPW2 in parallel mode
**  LAPW2 crashed!
0.080u 0.070s 0:00.15 100.0%    0+0k 0+0io 4056pf+0w

 >   stop error

- --------------- 'uplapw2.error'
Error in LAPW2
**  Error in Parallel LAPW2

- --------------- 'case.struct'
CaCuO2  dopado con Gd 
(50%)                                                   
B   LATTICE,NONEQUIV. ATOMS: 4                    139 
I4/mmm                  
MODE OF 
CALC=RELA                                                             
 10.506193 10.506193 13.108000 90.000000 90.000000 
90.000000                  
ATOM= -1: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT=-2
Ca         NPT=  781  R0=0.00005000 RMT=    2.0000   Z: 
20.0                  
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -2: X=0.00000000 Y=0.00000000 Z=0.50000000
          MULT= 1          ISPLIT=-2
Gd         NPT=  781  R0=0.00001000 RMT=    2.3000   Z: 
64.0                  
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -3: X=0.50000000 Y=0.00000000 Z=0.25000000
          MULT= 2          ISPLIT=-2
      -3: X=0.00000000 Y=0.50000000 Z=0.25000000
Cu         NPT=  781  R0=0.00005000 RMT=    1.9000   Z: 
29.0                  
LOCAL ROT MATRIX:    0.7071068-0.7071068 0.0000000
                     0.7071068 0.7071068 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -4: X=0.75000000 Y=0.25000000 Z=0.25000000
          MULT= 4          ISPLIT= 8
      -4: X=0.25000000 Y=0.75000000 Z=0.25000000
      -4: X=0.25000000 Y=0.25000000 Z=0.75000000
      -4: X=0.25000000 Y=0.25000000 Z=0.25000000
O          NPT=  781  R0=0.00010000 RMT=    1.8100   Z:  
8.0                  
LOCAL ROT MATRIX:    0.0000000 0.7071068 0.7071068
                     0.0000000-0.7071068 0.7071068
                     1.0000000 0.0000000 0.0000000
 16      NUMBER OF SYMMETRY OPERATIONS
 1 0 0 0.0000000
 0-1 0 0.0000000
 0 0-1 0.0000000
etc.

- ------------------
    This has happened before in other cases. Sometimes the same case 
crashes and sometimes it does not!
    The cluster has 6 machines
    two with two 1GHz intel processors each
    four with one 500MHz  intel processor
    Thanks

        Pablo de la Mora


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------------------------------

Date: Wed, 9 Oct 2002 14:04:08 -0500
From: "Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
Subject: [WIEN]: empty sphere

====
"Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
submitted the following contribution:
====


Dear Wien2k users

    I want to deal with some vacancies in the compound. So some "empty" spheres(Zero charge) will be used as vacancies to fill into the lattice. I already have read Dr. Peter's answer to a similar question on Sept 23. But I still am not able to do it. I also can not find the number of electrons in file case.in2. Does anyone has experience on this?    I appreciated your help very much.


Thank you so much

Jinbo Yang
Materials Research Center
University Of Missouri-Rolla
Rolla, MO 65409
Phone:+01-573-341-6165
Fax:   573-341-2071
E-mail:jinbo@umr.edu






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------------------------------

Date: Thu, 10 Oct 2002 01:00:01 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: empty sphere

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>     I want to deal with some vacancies in the compound. So some "empty"
spheres(Zero charge) will be used as vacancies
>  to fill into the lattice. I already have read Dr. Peter's answer to a
similar question on Sept 23. But I still am not able to do it.
Doing calculation including "dummy-atoms" using empty spheres can be
considered as a trick to plot partial l-like DOS at an interstitial
religion, where is not occupied by an atom: this is exactly answered and I
have nothing more to add. This is not a trick to include vacancies: empty
does not refer to vacuum. Although in the empty spheres there are no atoms,
they are not essentially empty of electrons. Charge density illustrates
where is less occupied by electrons.

Your,

S. Jalali

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------------------------------

Date: Wed, 09 Oct 2002 18:39:14 -0600
From: Pablo de la Mora <pm@fciencias.unam.mx>
Subject: Re: [WIEN]: problems with parallel execution

====
Pablo de la Mora <pm@fciencias.unam.mx>
submitted the following contribution:
====

Pablo de la Mora wrote:

> ====
> Pablo de la Mora <pm@fciencias.unam.mx>
> submitted the following contribution:
> ====
>
> Dear Wien Users,
>    I am having problems with parallel execution. I am doing a 
> supercell for doping, it worked fine with a supercell with 4 cells, 
> but with 2 cells it crashed.
>
> ------------ End of the 'dayfile'
> 1.230u 0.930s 3:02.72 1.1%    0+0k 0+0io 60807pf+0w
> >   lapw2 -up -p    (02:06:41) running LAPW2 in parallel mode
> **  LAPW2 crashed!
> 0.080u 0.070s 0:00.15 100.0%    0+0k 0+0io 4056pf+0w
>
> >   stop error
>
> --------------- 'uplapw2.error'
> Error in LAPW2
> **  Error in Parallel LAPW2
>
> --------------- 'case.struct'
> CaCuO2  dopado con Gd 
> (50%)                                                   B   
> LATTICE,NONEQUIV. ATOMS: 4                    139 
> I4/mmm                  MODE OF 
> CALC=RELA                                                             
> 10.506193 10.506193 13.108000 90.000000 90.000000 
> 90.000000                  ATOM= -1: X=0.00000000 Y=0.00000000 
> Z=0.00000000
>          MULT= 1          ISPLIT=-2
> Ca         NPT=  781  R0=0.00005000 RMT=    2.0000   Z: 
> 20.0                  LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                     0.0000000 1.0000000 0.0000000
>                     0.0000000 0.0000000 1.0000000
> ATOM= -2: X=0.00000000 Y=0.00000000 Z=0.50000000
>          MULT= 1          ISPLIT=-2
> Gd         NPT=  781  R0=0.00001000 RMT=    2.3000   Z: 
> 64.0                  LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                     0.0000000 1.0000000 0.0000000
>                     0.0000000 0.0000000 1.0000000
> ATOM= -3: X=0.50000000 Y=0.00000000 Z=0.25000000
>          MULT= 2          ISPLIT=-2
>      -3: X=0.00000000 Y=0.50000000 Z=0.25000000
> Cu         NPT=  781  R0=0.00005000 RMT=    1.9000   Z: 
> 29.0                  LOCAL ROT MATRIX:    0.7071068-0.7071068 0.0000000
>                     0.7071068 0.7071068 0.0000000
>                     0.0000000 0.0000000 1.0000000
> ATOM= -4: X=0.75000000 Y=0.25000000 Z=0.25000000
>          MULT= 4          ISPLIT= 8
>      -4: X=0.25000000 Y=0.75000000 Z=0.25000000
>      -4: X=0.25000000 Y=0.25000000 Z=0.75000000
>      -4: X=0.25000000 Y=0.25000000 Z=0.25000000
> O          NPT=  781  R0=0.00010000 RMT=    1.8100   Z:  
> 8.0                  LOCAL ROT MATRIX:    0.0000000 0.7071068 0.7071068
>                     0.0000000-0.7071068 0.7071068
>                     1.0000000 0.0000000 0.0000000
> 16      NUMBER OF SYMMETRY OPERATIONS
> 1 0 0 0.0000000
> 0-1 0 0.0000000
> 0 0-1 0.0000000
> etc.
>
> ------------------
>    This has happened before in other cases. Sometimes the same case 
> crashes and sometimes it does not!
>    The cluster has 6 machines
>    two with two 1GHz intel processors each
>    four with one 500MHz  intel processor
>    Thanks

I want to add that I did a calculation with the two dual (two 1GHz 
processors per machine; hydra and nodo1) the calculation did not crash:

- -------------------- .machines file
2:hydra
2:hydra
2.nodo1
2:nodo1
- ----------------------

but with the non homogeneous cluster (including the 500MHz processors; 
nodo3,...) it did crash:

- -------------------- .machines file
2:hydra
2:hydra
2.nodo1
2:nodo1
1:nodo3
1:nodo4
1:nodo5
- ------------------

    Pablo de la Mora

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------------------------------

Date: Thu, 24 Jun 1999 15:24:40 -0700 (PDT)
From: Michelle Johannes <johannes@maugre.ucdavis.edu>
Subject: Re: [WIEN]: Obital polarization calculation

====
Michelle Johannes <johannes@maugre.ucdavis.edu>
submitted the following contribution:
====

Claudio-
	Here is (I hope) a simple recipe:

After converging your s.o. calculation:

1) create a case.inorb file (see UG)

2) create a case.indm file (again see UG)

3) Change your case.indm file to case.indmc
(running s-o plus LDA+U requires this)

4) runsp_lapw -so -orb

	Good luck,
		Michelle



On Wed, 9 Oct 2002, Claudio Lee wrote:

> ====
> Claudio Lee <claudio_lee1@yahoo.com>
> submitted the following contribution:
> ====
> 
> Dear all,
> I have this problem, if you know the answer please
> help me.
> For spin polarized calculation. First step, my
> calculation has been included spin-obit coupling, and
> now, after this step has been done I want to include
> obital polarization into my calculation. Reading the
> wien2k menu, I follow the instruction but I dont know
> what I am doing wrong. 
> Using this script
> x lapwd -up   
> I got the error as it shows following:
> 'lapwdm' - can't open unit:  5
>  'lapwdm' -        filename: Fe274.indm
>  'lapwdm' -          status: old          form:
> formatted
> 
> So if anyone knows about this please help me, it will
> be better if you help me step by step how to include
> spin-obit coupling and obital polarization into the
> calculation of the spin-polarized case.  
> Many thanks in advance.
> Sincerely,
> Claudio.
> 
> 
> 
>  
> 
> 
> __________________________________________________
> Do you Yahoo!?
> Faith Hill - Exclusive Performances, Videos & More
> http://faith.yahoo.com
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------------------------------

Date: Thu, 10 Oct 2002 08:23:58 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: problems with parallel execution

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

The problems you have given below may have several reasons and one needs much
more info and tests.

a) Does it never crash with the two 1 GHz machines ?
b) Does it always or sometimes crash when including the 500 MHz processors ?
c) Only this case crashes or all/some others too ?

Common directory NFS mounted ? WIEN2k runs everywhere ?
can you connect to all machines without password ?
Slow network connection ? (In particular when the error occurs only
occasional) Did lapw1 work in parallel ? Do you see all vector_* files
with proper (new) date ? What happens when you run  x lapw2 -p interactively ?

Regards

> >    I am having problems with parallel execution. I am doing a
> > supercell for doping, it worked fine with a supercell with 4 cells,
> > but with 2 cells it crashed.
> >
> > ------------ End of the 'dayfile'
> > 1.230u 0.930s 3:02.72 1.1%    0+0k 0+0io 60807pf+0w
> > >   lapw2 -up -p    (02:06:41) running LAPW2 in parallel mode
> > **  LAPW2 crashed!
> > 0.080u 0.070s 0:00.15 100.0%    0+0k 0+0io 4056pf+0w
> >    This has happened before in other cases. Sometimes the same case
> > crashes and sometimes it does not!
> >    The cluster has 6 machines
> >    two with two 1GHz intel processors each
> >    four with one 500MHz  intel processor
> >    Thanks
>
> I want to add that I did a calculation with the two dual (two 1GHz
> processors per machine; hydra and nodo1) the calculation did not crash:
>
> -------------------- .machines file
> 2:hydra
> 2:hydra
> 2.nodo1
> 2:nodo1
> ----------------------
>
> but with the non homogeneous cluster (including the 500MHz processors;
> nodo3,...) it did crash:
>
> -------------------- .machines file
> 2:hydra
> 2:hydra
> 2.nodo1
> 2:nodo1
> 1:nodo3
> 1:nodo4
> 1:nodo5

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 10 Oct 2002 08:27:13 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Error File- lapw1

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>  This is my first time running wien 2k. I am running a
> CoO2 trigonal structure. The default parameters were
> used for the initialization. The run ended at lapw1
> with the following error message:
>
>  'SELECT' - no energy limits found for L= 1
>
>  'SELECT' - E-bottom   -8.18500   E-top -200.00000

Hi battery!

You need to supply much more information!
Did it crash in the first cycle? Most likely your struct file or input-files
are not ok.
Did it crash after a few cycles ? Reduce mixing in case.inm, rm *.bro* case.scf
x dstart (up/dn) and try another run(sp)


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 10 Oct 2002 08:39:38 +0200
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: problems with parallel execution

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====


> ====
> Pablo de la Mora <pm@fciencias.unam.mx>
> submitted the following contribution:
> ====
> 
>     I am having problems with parallel execution. 

Your problem could be similar to what I had some time ago. Check whether after 
the crash you can continue with 'x lapw2 -up -p'. If you can, then the problem 
most likely is due to a slow network, and you should add a few seconds of extra 
delay at the beginning of the lapw2para script.

Stefaan
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------------------------------

Date: Thu, 10 Oct 2002 15:18:19 +0200
From: Moreau Philippe <Philippe.Moreau@cnrs-imn.fr>
Subject: [WIEN]: ELNES calculations with WIEN2k, wrong .qtl for isplit=99?

====
Moreau Philippe <Philippe.Moreau@cnrs-imn.fr>
submitted the following contribution:
====



  Dear all,


We reported a couple of days ago a problem with the calculation of ELNES spectra with WIEN2K last version (ISPLIT=99).


Thanks to the changes proposed by Peter (changes in atpar.F , thank you) no error message appears anymore and case.qtl is not filled with numerous and only zeros. Nevertheless, the obtained spectra are completely different (totally wrong compared to experiments) from previous WIEN97.10 calculations.


we succesufully used the WIEN2K chain (initelnes, tetra, telnes) on a former case.qtl WIEN97 file.


so the problem probabily comes from lapw2 generating a wrong case.qtl.


has anyone performed ELNES calculations with WIEN2K ? and if yes with what changes if any ?


thanks


Philippe






 ----------------------------------------------------------------------------

| Dr. Philippe MOREAU                                                    
  |

|                                                                        
  | 

| <italic>Maître de Conférences à l'Université de Nantes </italic>       
                   | 

| <italic>Equipe PROSES (Propriétés, Réactivité, Organisation et
Structure Electro- |                                     

| nique des Solides)                     </italic>                       
           |

|                                                                        
  | 

| INSTITUT DES MATERIAUX JEAN ROUXEL   |
Mailto:Philippe.Moreau@cnrs-imn.fr | 

| Laboratoire de Chimie des Solides    |                                 
  | 

| 2, rue de la Houssiniere             |  Phone: (33) 2 40 37 64 14      
  | 

| BP 32229                             |  Fax:   (33) 2 40 37 39 95      
  | 

| 44322 NANTES CEDEX 3                 |  http://www.cnrs-imn.fr         
  | 

| FRANCE                               |                                 
  | 

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Date: Thu, 10 Oct 2002 17:52:12 +0200
From: "Dariusz Chrobak" <dchrobak@us.edu.pl>
Subject: [WIEN]: Spin-up, spin-down calculations

====
"Dariusz Chrobak" <dchrobak@us.edu.pl>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_001A_01C27085.C350AA00
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	charset="iso-8859-2"
Content-Transfer-Encoding: quoted-printable

Dear all,
I am a new wien2k user. Therefore I have a simple (for you) question. I =
have obtain negative parts of the spin-down charge density distribution =
during example calculation for fcc Ni .
I dont know what I am doing wrong.=20
Many thanks in advance.
Sincerely,
Darek

- ------=_NextPart_000_001A_01C27085.C350AA00
Content-Type: text/html;
	charset="iso-8859-2"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-2">
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<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT face=3D"Arial CE">Dear&nbsp;all,</FONT></DIV>
<DIV>I am a new wien2k user. Therefore&nbsp;I have a simple (for you) =
question.=20
I have obtain negative parts of the spin-down&nbsp;charge density =
distribution=20
during example calculation for fcc Ni .</DIV>
<DIV>I dont know what I am doing wrong. <BR>Many thanks in=20
advance.<BR>Sincerely,<BR><FONT face=3D"Arial =
CE">Darek</FONT></DIV></BODY></HTML>

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------------------------------

Date: Fri, 11 Oct 2002 13:30:56 -0700 (PDT)
From: yanming Ma <ymma66@yahoo.com>
Subject: [WIEN]: Problem with compiling the WIEN for Parrallel in SGI machine

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-957832938-1034368256=:1905
Content-Type: text/plain; charset=us-ascii


Dear Dr. Peter and WIEN2k users,

When I try to compile the latest version of WIEN2k for parallel calculation in SGI machine, I met some problems.  

(1) What i have done to configue parallel execution during the compiling is the following. a). I choose "shared Memory Architecture?(y/n)" as "y"

              b).I choose "Do you have MPI and Scalapack installed....to run finergained parrallel?(y/n)" as "y". Because this sgi machine using MPI and PBS. I do have a big calculation should be done.

             c). Following these choices, I have selected the settings for sgi system are 

RP RP_LIB: -L /user/local /SCALAPACK -L/usr/local/BLACS/LIN -lpblas -lredist -ltools -lscalapack -lfblacs -lblacs -lmpi.

FP FPOPT:-O -mpips4 -r10000 -freeform -64

(2) when I compile the Lapw1 package, this kind of error messages occurs.

ld64: ERROR   33 : Unresolved text symbol "MPI_Irecv" -- 1st referenced by /usr/
      Use linker option -v to see when and which objects, archives and dsos ar
ld64: ERROR   33 : Unresolved text symbol "MPI_Pack_size" -- 1st referenced by /
        Use linker option -v to see when and which objects, archives and dsos ar
ld64: ERROR   33 : Unresolved text symbol "MPI_Pack" -- 1st referenced by /usr/l
        Use linker option -v to see when and which objects, archives and dsos ar
ld64: INFO    152: Output file removed because of error.
*** Error code 2 (bu21)
*** Error code 1 (bu21)


Does any one have the same experience. Any comments are welcome. I will highly appreicate your help.

Yanming Ma 

Steacie Institute for molecular Sciences, National Research Council of Canada



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- --0-957832938-1034368256=:1905
Content-Type: text/html; charset=us-ascii

<P>Dear Dr. Peter and WIEN2k users,</P>
<P>When I try to compile the latest version of WIEN2k for parallel calculation&nbsp;in SGI machine, I met some problems.&nbsp; </P>
<P>(1) What i have done to configue parallel execution during the compiling is the following. a). I choose "shared Memory Architecture?(y/n)" as "y"</P>
<P>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; b).I choose "Do you have MPI and Scalapack installed....to run finergained parrallel?(y/n)" as "y". Because this sgi machine using MPI and PBS. I do have a big calculation should be done.</P>
<P>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; c). Following these choices, I have selected the settings&nbsp;for sgi system are </P>
<P>RP RP_LIB: -L /user/local /SCALAPACK -L/usr/local/BLACS/LIN -lpblas -lredist -ltools -lscalapack -lfblacs -lblacs -lmpi.</P>
<P>FP FPOPT:-O -mpips4 -r10000 -freeform -64</P>
<P>(2) when I compile the Lapw1 package, this kind of error messages occurs.</P>
<P>ld64: ERROR&nbsp;&nbsp; 33 : Unresolved text symbol "MPI_Irecv" -- 1st referenced by /usr/<BR>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Use linker option -v to see when and which objects, archives and dsos ar<BR>ld64: ERROR&nbsp;&nbsp; 33 : Unresolved text symbol "MPI_Pack_size" -- 1st referenced by /<BR>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Use linker option -v to see when and which objects, archives and dsos ar<BR>ld64: ERROR&nbsp;&nbsp; 33 : Unresolved text symbol "MPI_Pack" -- 1st referenced by /usr/l<BR>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Use linker option -v to see when and which objects, archives and dsos ar<BR>ld64: INFO&nbsp;&nbsp;&nbsp; 152: Output file removed because of error.<BR>*** Error code 2 (bu21)<BR>*** Error code 1 (bu21)<BR></P>
<P>Does any one have the same experience. Any comments are welcome. I will highly appreicate your help.</P>
<P>Yanming Ma </P>
<P>Steacie Institute for molecular Sciences, National Research Council of Canada</P><p><br><hr size=1>Do you Yahoo!?<br>
<a href="http://faith.yahoo.com">Faith Hill</a> - Exclusive Performances, Videos, & more<br>
<a href="http://faith.yahoo.com">faith.yahoo.com</a>
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------------------------------

End of wien-digest V2002 #38
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #39
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
Errors-To: owner-wien-digest@theochem.tuwien.ac.at
Precedence: bulk


wien-digest        Tuesday, October 22 2002        Volume 2002 : Number 039




----------------------------------------------------------------------

Date: Sun, 13 Oct 2002 10:37:25 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Problem with compiling the WIEN for Parrallel in SGI machine

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Ms. Ma,

either you have not installed MPI, or it is not installed in your 
default library path. Check this. And if it is not in the default 
library path, but installed, add a -L/path/to/directory/of/MPI type of 
directive like you have to SCALAPACK and BLACS below.

Best regards,
Torsten Andersen.

yanming Ma wrote:

> Dear Dr. Peter and WIEN2k users,
>
> When I try to compile the latest version of WIEN2k for parallel 
> calculation in SGI machine, I met some problems. 
>
> (1) What i have done to configue parallel execution during the 
> compiling is the following. a). I choose "shared Memory 
> Architecture?(y/n)" as "y"
>
>               b).I choose "Do you have MPI and Scalapack 
> installed....to run finergained parrallel?(y/n)" as "y". Because this 
> sgi machine using MPI and PBS. I do have a big calculation should be done.
>
>              c). Following these choices, I have selected the 
> settings for sgi system are
>
> RP RP_LIB: -L /user/local /SCALAPACK -L/usr/local/BLACS/LIN -lpblas 
> -lredist -ltools -lscalapack -lfblacs -lblacs -lmpi.
>
> FP FPOPT:-O -mpips4 -r10000 -freeform -64
>
> (2) when I compile the Lapw1 package, this kind of error messages occurs.
>
> ld64: ERROR   33 : Unresolved text symbol "MPI_Irecv" -- 1st 
> referenced by /usr/
>       Use linker option -v to see when and which objects, archives and 
> dsos ar
> ld64: ERROR   33 : Unresolved text symbol "MPI_Pack_size" -- 1st 
> referenced by /
>         Use linker option -v to see when and which objects, archives 
> and dsos ar
> ld64: ERROR   33 : Unresolved text symbol "MPI_Pack" -- 1st referenced 
> by /usr/l
>         Use linker option -v to see when and which objects, archives 
> and dsos ar
> ld64: INFO    152: Output file removed because of error.
> *** Error code 2 (bu21)
> *** Error code 1 (bu21)
>
> Does any one have the same experience. Any comments are welcome. I 
> will highly appreicate your help.
>
> Yanming Ma
>
> Steacie Institute for molecular Sciences, National Research Council of 
> Canada
>
>
> ------------------------------------------------------------------------
> Do you Yahoo!?
> Faith Hill <http://faith.yahoo.com> - Exclusive Performances, Videos, 
> & more
> faith.yahoo.com <http://faith.yahoo.com> 


- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Mon, 14 Oct 2002 11:07:54 +0200
From: =?us-ascii?Q?Anders_Froseth?= <anders.froseth@phys.ntnu.no>
Subject: SV: [WIEN]: Problem with compiling the WIEN for Parrallel in SGI machine

====
=?us-ascii?Q?Anders_Froseth?= <anders.froseth@phys.ntnu.no>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0002_01C27371.F1F0BD20
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	charset="us-ascii"
Content-Transfer-Encoding: 7bit

Dear Yianming,

I have a suggestion for you regarding the flags you are using (independent
of
your mpi part). To get a generally more efficient and numerically stable
code you could replace

- -O

by

- -O3 -OPT:IEEE_arithmetic = 0  -OPT:IEEE_roundoff = 0

you will then get a more agressive optimisation which is also safe with
respect to numerical stability.

Regards,
Anders
  Dear Dr. Peter and WIEN2k users,

  When I try to compile the latest version of WIEN2k for parallel
calculation in SGI machine, I met some problems.

  (1) What i have done to configue parallel execution during the compiling
is the following. a). I choose "shared Memory Architecture?(y/n)" as "y"

                b).I choose "Do you have MPI and Scalapack installed....to
run finergained parrallel?(y/n)" as "y". Because this sgi machine using MPI
and PBS. I do have a big calculation should be done.

               c). Following these choices, I have selected the settings for
sgi system are

  RP RP_LIB: -L /user/local
/SCALAPACK -L/usr/local/BLACS/LIN -lpblas -lredist -ltools -lscalapack -lfbl
acs -lblacs -lmpi.

  FP FPOPT:-O -mpips4 -r10000 -freeform -64

  (2) when I compile the Lapw1 package, this kind of error messages occurs.

  ld64: ERROR   33 : Unresolved text symbol "MPI_Irecv" -- 1st referenced by
/usr/
        Use linker option -v to see when and which objects, archives and
dsos ar
  ld64: ERROR   33 : Unresolved text symbol "MPI_Pack_size" -- 1st
referenced by /
          Use linker option -v to see when and which objects, archives and
dsos ar
  ld64: ERROR   33 : Unresolved text symbol "MPI_Pack" -- 1st referenced by
/usr/l
          Use linker option -v to see when and which objects, archives and
dsos ar
  ld64: INFO    152: Output file removed because of error.
  *** Error code 2 (bu21)
  *** Error code 1 (bu21)


  Does any one have the same experience. Any comments are welcome. I will
highly appreicate your help.

  Yanming Ma

  Steacie Institute for molecular Sciences, National Research Council of
Canada





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- --
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- ------=_NextPart_000_0002_01C27371.F1F0BD20
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	charset="us-ascii"
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Dus-ascii">
<META content=3D"MSHTML 6.00.2719.2200" name=3DGENERATOR></HEAD>
<BODY>
<DIV><FONT face=3DTahoma><SPAN class=3D247295508-14102002></SPAN><FONT =
size=3D2>D<SPAN=20
class=3D247295508-14102002>ear Yianming,</SPAN></FONT></FONT></DIV>
<DIV><FONT face=3DTahoma><FONT size=3D2><SPAN=20
class=3D247295508-14102002></SPAN></FONT></FONT>&nbsp;</DIV>
<DIV><FONT face=3DTahoma><FONT size=3D2><SPAN =
class=3D247295508-14102002>I have a=20
suggestion for you regarding&nbsp;the flags you are using (independent=20
of</SPAN></FONT></FONT></DIV>
<DIV><FONT face=3DTahoma><FONT size=3D2><SPAN =
class=3D247295508-14102002>your mpi=20
part).&nbsp;To get a&nbsp;generally more efficient and numerically =
stable code=20
you could replace</SPAN></FONT></FONT></DIV>
<DIV><FONT face=3DTahoma><FONT size=3D2><SPAN=20
class=3D247295508-14102002></SPAN></FONT></FONT>&nbsp;</DIV>
<DIV><FONT face=3DTahoma><FONT size=3D2><SPAN=20
class=3D247295508-14102002>-O</SPAN></FONT></FONT></DIV>
<DIV><FONT face=3DTahoma><FONT size=3D2><SPAN=20
class=3D247295508-14102002></SPAN></FONT></FONT>&nbsp;</DIV>
<DIV><FONT face=3DTahoma><FONT size=3D2><SPAN =
class=3D247295508-14102002>by=20
</SPAN></FONT></FONT></DIV>
<DIV><FONT face=3DTahoma><FONT size=3D2><SPAN=20
class=3D247295508-14102002></SPAN></FONT></FONT>&nbsp;</DIV>
<DIV><FONT face=3DTahoma><FONT size=3D2><SPAN =
class=3D247295508-14102002>-O3=20
- -OPT:IEEE_arithmetic =3D 0&nbsp;</SPAN><SPAN =
class=3D247295508-14102002><FONT=20
face=3DArial color=3D#0000ff>&nbsp;<FONT face=3DTahoma=20
color=3D#000000>-OPT:IEEE_roundoff =3D =
0</FONT></FONT></SPAN></FONT></FONT></DIV>
<DIV><FONT><FONT face=3DTahoma><FONT size=3D2><SPAN =
class=3D247295508-14102002><FONT=20
face=3DArial color=3D#0000ff>&nbsp;</FONT></SPAN><BR><SPAN=20
class=3D247295508-14102002>you will then get a more agressive =
optimisation which=20
is also safe with respect to numerical=20
stability.</SPAN></FONT></FONT></FONT></DIV>
<DIV><FONT><FONT face=3DTahoma><FONT size=3D2><SPAN=20
class=3D247295508-14102002></SPAN></FONT></FONT></FONT>&nbsp;</DIV>
<DIV><FONT><FONT face=3DTahoma><FONT size=3D2><SPAN=20
class=3D247295508-14102002>Regards,</SPAN></FONT></FONT></FONT></DIV>
<DIV><FONT><FONT face=3DTahoma><FONT size=3D2><SPAN=20
class=3D247295508-14102002>Anders</SPAN></FONT></FONT></DIV></FONT>
<BLOCKQUOTE=20
style=3D"PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #0000ff 2px =
solid">
  <P>Dear Dr. Peter and WIEN2k users,</P>
  <P>When I try to compile the latest version of WIEN2k for parallel=20
  calculation&nbsp;in SGI machine, I met some problems.&nbsp; </P>
  <P>(1) What i have done to configue parallel execution during the =
compiling is=20
  the following. a). I choose "shared Memory Architecture?(y/n)" as =
"y"</P>
  =
<P>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbs=
p;&nbsp;=20
  b).I choose "Do you have MPI and Scalapack installed....to run =
finergained=20
  parrallel?(y/n)" as "y". Because this sgi machine using MPI and PBS. I =
do have=20
  a big calculation should be done.</P>
  =
<P>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbs=
p;=20
  c). Following these choices, I have selected the settings&nbsp;for sgi =
system=20
  are </P>
  <P>RP RP_LIB: -L /user/local /SCALAPACK -L/usr/local/BLACS/LIN -lpblas =

  -lredist -ltools -lscalapack -lfblacs -lblacs -lmpi.</P>
  <P>FP FPOPT:-O -mpips4 -r10000 -freeform -64</P>
  <P>(2) when I compile the Lapw1 package, this kind of error messages=20
  occurs.</P>
  <P>ld64: ERROR&nbsp;&nbsp; 33 : Unresolved text symbol "MPI_Irecv" -- =
1st=20
  referenced by /usr/<BR>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Use linker =
option -v to=20
  see when and which objects, archives and dsos ar<BR>ld64: =
ERROR&nbsp;&nbsp; 33=20
  : Unresolved text symbol "MPI_Pack_size" -- 1st referenced by=20
  /<BR>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Use linker option -v =
to see=20
  when and which objects, archives and dsos ar<BR>ld64: =
ERROR&nbsp;&nbsp; 33 :=20
  Unresolved text symbol "MPI_Pack" -- 1st referenced by=20
  /usr/l<BR>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Use linker option =
- -v to=20
  see when and which objects, archives and dsos ar<BR>ld64:=20
  INFO&nbsp;&nbsp;&nbsp; 152: Output file removed because of =
error.<BR>*** Error=20
  code 2 (bu21)<BR>*** Error code 1 (bu21)<BR></P>
  <P>Does any one have the same experience. Any comments are welcome. I =
will=20
  highly appreicate your help.</P>
  <P>Yanming Ma </P>
  <P>Steacie Institute for molecular Sciences, National Research Council =
of=20
  Canada</P>
  <P><BR>
  <HR SIZE=3D1>
  Do you Yahoo!?<BR><A href=3D"http://faith.yahoo.com">Faith Hill</A> - =
Exclusive=20
  Performances, Videos, &amp; more<BR><A=20
  =
href=3D"http://faith.yahoo.com">faith.yahoo.com</A></BLOCKQUOTE></BODY></=
HTML>

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------------------------------

Date: Mon, 14 Oct 2002 17:50:29 +0200
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: TETRA / Re: [WIEN]: ELNES calculations with WIEN2k, wrong .qtl for isplit=99?

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Dear Philippe,


I perform ELNES calculations with WIEN2k, too.  Sorry for taking so long to
respond.
After receiving Peter's new atpar.F, I too got good qtl-files.  And yes,
from them I also calculate spectra : I calculated H-spectra (orientation
dependent) for graphite and they do compare to those calculated with WIEN97.
I have no idea what the problem might be in your situation (maybe you solved
it already).

I'd like to ask you a question : how do you cope with the reading of the
qtl-file by tetra?  The xdos-matrix elements are written by outp.f as
complex numbers, but read by tetra as real numbers.  To solve this problem,
we use a modified FORMAT-statement for reading, skipping the complex parts
and reading the real parts.  Do you use a similar trick, or do you have
something better?

Good luck with the calculations,
thanks again to Peter Blaha for fixing the atpar.F,

Kevin Jorissen
EMAT, University of Antwerp


- ----- Original Message -----
From: "Moreau Philippe" <Philippe.Moreau@cnrs-imn.fr>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Thursday, October 10, 2002 3:18 PM
Subject: [WIEN]: ELNES calculations with WIEN2k, wrong .qtl for isplit=99?


> ==== Moreau Philippe submitted the following contribution: ====
>
>
> Dear all,
>
> We reported a couple of days ago a problem with the calculation of ELNES
spectra with WIEN2K last version (ISPLIT=99).
>
> Thanks to the changes proposed by Peter (changes in atpar.F , thank you)
no error message appears anymore and case.qtl is not filled with numerous
and only zeros. Nevertheless, the obtained spectra are completely different
(totally wrong compared to experiments) from previous WIEN97.10
calculations.
>
> we succesufully used the WIEN2K chain (initelnes, tetra, telnes) on a
former case.qtl WIEN97 file.
>
> so the problem probabily comes from lapw2 generating a wrong case.qtl.
>
> has anyone performed ELNES calculations with WIEN2K ? and if yes with what
changes if any ?
>
> thanks
>
> Philippe
>
>
>
>
>
> --------------------------------------------------------------------------
- --
> | Dr. Philippe MOREAU |
> | |
> | Maître de Conférences à l'Université de Nantes |
> | Equipe PROSES (Propriétés, Réactivité, Organisation et Structure
Electro- |
> | nique des Solides) |
> | |
> | INSTITUT DES MATERIAUX JEAN ROUXEL | Mailto:Philippe.Moreau@cnrs-imn.fr
|
> | Laboratoire de Chimie des Solides | |
> | 2, rue de la Houssiniere | Phone: (33) 2 40 37 64 14 |
> | BP 32229 | Fax: (33) 2 40 37 39 95 |
> | 44322 NANTES CEDEX 3 | http://www.cnrs-imn.fr |
> | FRANCE | |
> --------------------------------------------------------------------------
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Date: Mon, 14 Oct 2002 10:06:28 +0200
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: ELNES calculations with WIEN2k, wrong .qtl for isplit=99?

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Dear Philippe,


I perform ELNES calculations with WIEN2k, too.  Sorry for taking so long to
respond.
After receiving Peter's new atpar.F, I too got good qtl-files.  And yes,
from them I also calculate spectra : I calculated H-spectra (orientation
dependent) for graphite and they do compare to those calculated with WIEN97.
I have no idea what the problem might be in your situation (maybe you solved
it already).

I'd like to ask you a question : how do you cope with the reading of the
qtl-file by tetra?  The xdos-matrix elements are written by outp.f as
complex numbers, but read by tetra as real numbers.  To solve this problem,
we use a modified FORMAT-statement for reading, skipping the complex parts
and reading the real parts.  Do you use a similar trick, or do you have
something better?

Good luck with the calculations,
thanks again to Peter Blaha for fixing the atpar.F,

Kevin Jorissen
EMAT, University of Antwerp


- ----- Original Message -----
From: "Moreau Philippe" <Philippe.Moreau@cnrs-imn.fr>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Thursday, October 10, 2002 3:18 PM
Subject: [WIEN]: ELNES calculations with WIEN2k, wrong .qtl for isplit=99?


> ==== Moreau Philippe submitted the following contribution: ====
>
>
> Dear all,
>
> We reported a couple of days ago a problem with the calculation of ELNES
spectra with WIEN2K last version (ISPLIT=99).
>
> Thanks to the changes proposed by Peter (changes in atpar.F , thank you)
no error message appears anymore and case.qtl is not filled with numerous
and only zeros. Nevertheless, the obtained spectra are completely different
(totally wrong compared to experiments) from previous WIEN97.10
calculations.
>
> we succesufully used the WIEN2K chain (initelnes, tetra, telnes) on a
former case.qtl WIEN97 file.
>
> so the problem probabily comes from lapw2 generating a wrong case.qtl.
>
> has anyone performed ELNES calculations with WIEN2K ? and if yes with what
changes if any ?
>
> thanks
>
> Philippe
>
>
>
>
>
> --------------------------------------------------------------------------
- --
> | Dr. Philippe MOREAU |
> | |
> | Maître de Conférences à l'Université de Nantes |
> | Equipe PROSES (Propriétés, Réactivité, Organisation et Structure
Electro- |
> | nique des Solides) |
> | |
> | INSTITUT DES MATERIAUX JEAN ROUXEL | Mailto:Philippe.Moreau@cnrs-imn.fr
|
> | Laboratoire de Chimie des Solides | |
> | 2, rue de la Houssiniere | Phone: (33) 2 40 37 64 14 |
> | BP 32229 | Fax: (33) 2 40 37 39 95 |
> | 44322 NANTES CEDEX 3 | http://www.cnrs-imn.fr |
> | FRANCE | |
> --------------------------------------------------------------------------
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send mail to majordomo@zeus.theochem.tuwien.ac.at ====

====
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------------------------------

Date: Tue, 15 Oct 2002 11:29:35 +0200
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: Test

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Sorry, just testing, don't bother.

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------------------------------

Date: Tue, 15 Oct 2002 21:13:22 +0800
From: "whoming" <whoming@sohu.com>
Subject: [WIEN]: About fine grained parallel computation in WIEN2K

====
"whoming" <whoming@sohu.com>
submitted the following contribution:
====

Dear all,
         Has anyone performed fine grained parallel calculation on SGI
Origin 2000/38000?
I have got a pecular result on it.
         I use TiC as the sample.And use all the same parameters to
initialize the computation before
the following three kinds of SCF calculations. "Serial calculation" and
"k-point parallel calculation" get the same
result and both are resonable in physics.But when I perform "fine grained
parallel calculation".There are
some bad results.
After one cycle:
          1) I have carefully compared all the files produced by lapw0,
lapw1 in the three situations.They are all the same
in values.
          2)But the difference appears from lapw2. "TOTAL CHARGE INSIDE
SPHERE" in tic.output2 produced by fine grained
parallel calculation differs from that either in "Serial calculation" or in
"k-point parallel calculation".(In the "k-point parallel
calculation",you have to add up all the correspond "TOTAL CHARGE INSIDE
SPHERE" from all the tic.output2_* files.)
This is the first difference.And also I found that there is "QTL-B Value
.EQ.7.30302!!!!!!" in tic.output2_1 in the fine grained calculation.
          3)When I turn to tic.scf2 or tic.scf2_1 files, there is just one
line like":GMA  : POTENTIAL AND CHARGE CUT-OFF  14.00 Ry**.5"
 in the fine grained calculation. While in the other two calculations there
are much more contents and all are the same in values.
 At the end, Serial calculation and k-point parallel calculation converged
in about the same resonable result.But the fine grained parallel computation
makes the total energy oscillate and appears "QTL-B Value" in tic.output2_1
files.
         Has anyone account the same problems as me?Your kind help will be
appreciated very much! Thanks!!
Yours,
           whoming
P.S.
 The machines file for k-point parallel calculation:
1:localhost
1:localhost
1:localhost
1:localhost
granularity:1
and it for fine grained parallel calculation:
1:localhost:4
granularity:1
There are only four k-points in tic.klist file.



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------------------------------

Date: Tue, 15 Oct 2002 17:54:47 +0200
From: Florent Boucher <Florent.Boucher@cnrs-imn.fr>
Subject: Re: TETRA / Re: [WIEN]: ELNES calculations with WIEN2k, wrong .qtl for isplit=99?

====
Florent Boucher <Florent.Boucher@cnrs-imn.fr>
submitted the following contribution:
====

<!DOCTYPE html PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
  <title></title>
</head>
<body>
Dear Peter,<br>
Dear Kevin,<br>
we did with Philippe some more tests about the problem we found with the
new WIEN2K and qtl files (ISPLIT=99).<br>
If we still use the "old" way (standard LAPW, switch 0 in the in1 file) we
have effectively the same results between wien97 and wien2K.<br>
But if we use the "new" way (APW, switch 1 in the in1 file) we have completely
different results for the elnes calculations. Please have a look at the two
files included in attachments.<br>
Your comments will be appreciated ...<br>
<br>
Besides, concerning the point about the read statment in tetra.<br>
<pre wrap="">
I'd like to ask you a question : how do you cope with the reading of the
qtl-file by tetra?  The xdos-matrix elements are written by outp.f as
complex numbers, but read by tetra as real numbers.  To solve this problem,
we use a modified FORMAT-statement for reading, skipping the complex parts
and reading the real parts.  Do you use a similar trick, or do you have
something better?
</pre>
<br>
All seems to be OK. There is a small trick:<br>
outp.f writes (lxdos2*(lxdos2+1)/2=136 complex numbers -&gt;   lxdos2*(lxdos2+1)=272
real numbers)<br>
tetra.f reads lxdos2*(lxdos2+1)=272 real numbers (The odd numbers correspond
to real part  of qtl and even numbers to the imaginary parts of qtl)<br>
So, normally you do not need to change tetra <br>
<br>
Regards<br>
Philippe, Florent<br>
Kevin Jorissen a écrit:<br>
<blockquote type="cite"
 cite="mid000d01c27399$6bc10e80$7c82818f@ruca.ua.ac.be">
  <pre wrap="">====
"Kevin Jorissen" <a class="moz-txt-link-rfc2396E" href="mailto:kevin.jorissen@ua.ac.be">&lt;kevin.jorissen@ua.ac.be&gt;</a>
submitted the following contribution:
====

Dear Philippe,


I perform ELNES calculations with WIEN2k, too.  Sorry for taking so long to
respond.
After receiving Peter's new atpar.F, I too got good qtl-files.  And yes,
from them I also calculate spectra : I calculated H-spectra (orientation
dependent) for graphite and they do compare to those calculated with WIEN97.
I have no idea what the problem might be in your situation (maybe you solved
it already).

I'd like to ask you a question : how do you cope with the reading of the
qtl-file by tetra?  The xdos-matrix elements are written by outp.f as
complex numbers, but read by tetra as real numbers.  To solve this problem,
we use a modified FORMAT-statement for reading, skipping the complex parts
and reading the real parts.  Do you use a similar trick, or do you have
something better?

Good luck with the calculations,
thanks again to Peter Blaha for fixing the atpar.F,

Kevin Jorissen
EMAT, University of Antwerp


- ----- Original Message -----
From: "Moreau Philippe" <a class="moz-txt-link-rfc2396E" href="mailto:Philippe.Moreau@cnrs-imn.fr">&lt;Philippe.Moreau@cnrs-imn.fr&gt;</a>
To: <a class="moz-txt-link-rfc2396E" href="mailto:wien@zeus.theochem.tuwien.ac.at">&lt;wien@zeus.theochem.tuwien.ac.at&gt;</a>
Sent: Thursday, October 10, 2002 3:18 PM
Subject: [WIEN]: ELNES calculations with WIEN2k, wrong .qtl for isplit=99?


  </pre>
  <blockquote type="cite">
    <pre wrap="">==== Moreau Philippe submitted the following contribution: ====


Dear all,

We reported a couple of days ago a problem with the calculation of ELNES
    </pre>
  </blockquote>
  <pre wrap=""><!---->spectra with WIEN2K last version (ISPLIT=99).
  </pre>
  <blockquote type="cite">
    <pre wrap="">Thanks to the changes proposed by Peter (changes in atpar.F , thank you)
    </pre>
  </blockquote>
  <pre wrap=""><!---->no error message appears anymore and case.qtl is not filled with numerous
and only zeros. Nevertheless, the obtained spectra are completely different
(totally wrong compared to experiments) from previous WIEN97.10
calculations.
  </pre>
  <blockquote type="cite">
    <pre wrap="">we succesufully used the WIEN2K chain (initelnes, tetra, telnes) on a
    </pre>
  </blockquote>
  <pre wrap=""><!---->former case.qtl WIEN97 file.
  </pre>
  <blockquote type="cite">
    <pre wrap="">so the problem probabily comes from lapw2 generating a wrong case.qtl.

has anyone performed ELNES calculations with WIEN2K ? and if yes with what
    </pre>
  </blockquote>
  <pre wrap=""><!---->changes if any ?
  </pre>
  <blockquote type="cite">
    <pre wrap="">thanks

Philippe





- --------------------------------------------------------------------------
    </pre>
  </blockquote>
  <pre wrap=""><!---->--
  </pre>
  <blockquote type="cite">
    <pre wrap="">| Dr. Philippe MOREAU |
| |
| Maître de Conférences à l'Université de Nantes |
| Equipe PROSES (Propriétés, Réactivité, Organisation et Structure
    </pre>
  </blockquote>
  <pre wrap=""><!---->Electro- |
  </pre>
  <blockquote type="cite">
    <pre wrap="">| nique des Solides) |
| |
| INSTITUT DES MATERIAUX JEAN ROUXEL | <a class="moz-txt-link-freetext" href="Mailto:Philippe.Moreau@cnrs-imn.fr">Mailto:Philippe.Moreau@cnrs-imn.fr</a>
    </pre>
  </blockquote>
  <pre wrap=""><!---->|
  </pre>
  <blockquote type="cite">
    <pre wrap="">| Laboratoire de Chimie des Solides | |
| 2, rue de la Houssiniere | Phone: (33) 2 40 37 64 14 |
| BP 32229 | Fax: (33) 2 40 37 39 95 |
| 44322 NANTES CEDEX 3 | <a class="moz-txt-link-freetext" href="http://www.cnrs-imn.fr">http://www.cnrs-imn.fr</a> |
| FRANCE | |
- --------------------------------------------------------------------------
    </pre>
  </blockquote>
  <pre wrap=""><!---->-- ==== WIEN Mailing list: <a class="moz-txt-link-abbreviated" href="mailto:wien@zeus.theochem.tuwien.ac.at">wien@zeus.theochem.tuwien.ac.at</a> To (un)subscribe
send mail to <a class="moz-txt-link-abbreviated" href="mailto:majordomo@zeus.theochem.tuwien.ac.at">majordomo@zeus.theochem.tuwien.ac.at</a> ====

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  </pre>
</blockquote>
<br>
<pre class="moz-signature" cols="$mailwrapcol">-- 
 --------------------------------------------------------------------------
| Florent BOUCHER                    |                                     |
| Institut des Matériaux Jean Rouxel | <a class="moz-txt-link-freetext" href="Mailto:Florent.Boucher@cnrs-imn.fr">Mailto:Florent.Boucher@cnrs-imn.fr</a>  |
| 2, rue de la Houssinière           | Phone: (33) 2 40 37 39 24           |
| BP 32229                           | Fax:   (33) 2 40 37 39 95           |
| 44322 NANTES CEDEX 3 (FRANCE)      | <a class="moz-txt-link-freetext" href="http://www.cnrs-imn.fr">http://www.cnrs-imn.fr</a>              |
 --------------------------------------------------------------------------</pre>
<br>
</body>
</html>

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------------------------------

Date: Tue, 15 Oct 2002 20:45:51 -0200 (BDB)
From: vivienne denise falcao <vdfalcao@dedalus.lcc.ufmg.br>
Subject: [WIEN]: Problems with X-Ray Spectra

====
vivienne denise falcao <vdfalcao@dedalus.lcc.ufmg.br>
submitted the following contribution:
====

Dear All,

	I am using wien 97 to calculate x-ray spectra. I need to exchange
the energy range because in my calculations I wish a energy range between
- -5 and 25 eV for x-ray absorption spectra. But, in my calculations the
maximum energy in the case.xspec is 12 eV. What can I do to exchange the
energy range?
	I hope answer.

Thankfull,

Vivienne.

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------------------------------

Date: Wed, 16 Oct 2002 08:50:23 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Problems with X-Ray Spectra

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> I am using wien 97 to calculate x-ray spectra. I need to exchange
> the energy range because in my calculations I wish a energy range between
> -5 and 25 eV for x-ray absorption spectra. But, in my calculations the
> maximum energy in the case.xspec is 12 eV. What can I do to exchange the
> energy range?
Upper limit of energy window is 1.5Ry in case.in1 file, so to include state
with higher energy one should increase it, and then run lapw1 to make sense
the change.
Upper limit of energy window is 1.5Ry in case.int file, so to see included
state with higher energy one should increase it too, and then run tetra to
produce favorite DOS's, which are essential in this respect.
              Your,
              S. Jalali

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Date: Wed, 16 Oct 2002 08:04:30 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Problems with X-Ray Spectra

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Vivienne,

in addition to what Saeid already said...

There is around 13.6eV on a Ry, so to get up to 25eV, all the upper 
limits of your energy windows must be increased to at least 2Ry.

Best regards,
Torsten Andersen.

vivienne denise falcao wrote:

>====
>vivienne denise falcao <vdfalcao@dedalus.lcc.ufmg.br>
>submitted the following contribution:
>====
>
>Dear All,
>
>	I am using wien 97 to calculate x-ray spectra. I need to exchange
>the energy range because in my calculations I wish a energy range between
>-5 and 25 eV for x-ray absorption spectra. But, in my calculations the
>maximum energy in the case.xspec is 12 eV. What can I do to exchange the
>energy range?
>	I hope answer.
>
>Thankfull,
>
>Vivienne.
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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Date: Wed, 16 Oct 2002 08:07:37 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: About fine grained parallel computation in WIEN2K

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>          Has anyone performed fine grained parallel calculation on SGI
> Origin 2000/38000?
>           2)But the difference appears from lapw2. "TOTAL CHARGE INSIDE
> SPHERE" in tic.output2 produced by fine grained
> parallel calculation differs from that either in "Serial calculation" or in
> "k-point parallel calculation".(In the "k-point parallel
> calculation",you have to add up all the correspond "TOTAL CHARGE INSIDE
> SPHERE" from all the tic.output2_* files.)
> This is the first difference.And also I found that there is "QTL-B Value
> .EQ.7.30302!!!!!!" in tic.output2_1 in the fine grained calculation.

Dear whoming

 Probably you are using more processors than you have "blocks" of basis
functions. check that
#basis fkt/IBLOCK is larger than you number of processors

for  #basis fkt  do grep :rkm in TiC.scf1
for IBLOCK look in modules.F in SRC_lapw2 (usually 128)

Fine grain parallelization makes no sense for small cases like TiC.

Best wishes Georg


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 16 Oct 2002 09:59:55 +0200
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: TETRA / Re: [WIEN]: ELNES calculations with WIEN2k, wrong .qtl for isplit=99?

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Dear Florent and Philippe,

I have used the default .in1-file, specifying global LAPW (0) (as
recommended in the UG) and APW (1) for all the choices on the next lines.
Did you perform a 'full APW'-calculation? (I'll try).
By the way, I did not receive the attachments to your mail.


About the modification of tetra.f : I must apologize for being unclear.  The
modification we make is for F-case (ISPLIT=88), where tetra reads :
 read(4,208)(xqtl(isort,i1),i1=1,lxdos2)
  208 FORMAT((10F10.5))

while outp.f writes :
                 if(isplit(jatom).eq.88) then
                   read(15,208) (xqtl(i,i,1),i=1,lxdos2)
                   IF(jb.EQ.JBAND) WRITE(16,208)  &
                      (xqtl(i,i,1)/100.d0,i=1,lxdos2)
                 ENDIF
  208              FORMAT((10F10.5))


So, while your analysis is correct for the 99-case, there is still a
conflict in the 88-case.  What I did is changing in tetra.f :

                  if(text(isort)(13:20).eq.'xdos(i,j') then
                    if(lxdos.ne.3) stop 'LXDOS must be 3 for ISPLIT 99 or
88'
                  read(4,208)(xqtl(isort,i1),i1=1,(lxdos2)*(lxdos2+1))
                  else if(text(isort)(13:20).eq.'xdos(i,i') then
                  read(4,207)(xqtl(isort,i1),i1=1,lxdos2)
                  endif
  208 FORMAT((10F10.5))
  207 FORMAT(5(F10.5,10x))

and this works.  Perhaps it would be preferable to make tetra read ALL the
numbers, but I don't fully understand the working of tetra - maybe you can
comment on this.
Of course, one can always use 99-option (I don't use 88 often).


Please do send me the files you intended to include, I promise to have a
look at them asap.  bye!

Kevin.



- ----- Original Message -----
From: "Florent Boucher" <Florent.Boucher@cnrs-imn.fr>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Tuesday, October 15, 2002 5:54 PM
Subject: Re: TETRA / Re: [WIEN]: ELNES calculations with WIEN2k, wrong .qtl
for isplit=99?


> ==== Florent Boucher submitted the following contribution: ==== Dear
Peter,
> Dear Kevin,
> we did with Philippe some more tests about the problem we found with the
new WIEN2K and qtl files (ISPLIT=99).
> If we still use the "old" way (standard LAPW, switch 0 in the in1 file) we
have effectively the same results between wien97 and wien2K.
> But if we use the "new" way (APW, switch 1 in the in1 file) we have
completely different results for the elnes calculations. Please have a look
at the two files included in attachments.
> Your comments will be appreciated ...
>
> Besides, concerning the point about the read statment in tetra.
>
> I'd like to ask you a question : how do you cope with the reading of the
> qtl-file by tetra?  The xdos-matrix elements are written by outp.f as
> complex numbers, but read by tetra as real numbers.  To solve this
problem,
> we use a modified FORMAT-statement for reading, skipping the complex parts
> and reading the real parts.  Do you use a similar trick, or do you have
> something better?
>
> All seems to be OK. There is a small trick:
> outp.f writes (lxdos2*(lxdos2+1)/2=136 complex numbers ->
lxdos2*(lxdos2+1)=272 real numbers)
> tetra.f reads lxdos2*(lxdos2+1)=272 real numbers (The odd numbers
correspond to real part of qtl and even numbers to the imaginary parts of
qtl)
> So, normally you do not need to change tetra
>
> Regards
> Philippe, Florent
> Kevin Jorissen a écrit:
>
> ====
> "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
> submitted the following contribution:
> ====
>
> Dear Philippe,
>
>
> I perform ELNES calculations with WIEN2k, too.  Sorry for taking so long
to
> respond.
> After receiving Peter's new atpar.F, I too got good qtl-files.  And yes,
> from them I also calculate spectra : I calculated H-spectra (orientation
> dependent) for graphite and they do compare to those calculated with
WIEN97.
> I have no idea what the problem might be in your situation (maybe you
solved
> it already).
>
> I'd like to ask you a question : how do you cope with the reading of the
> qtl-file by tetra?  The xdos-matrix elements are written by outp.f as
> complex numbers, but read by tetra as real numbers.  To solve this
problem,
> we use a modified FORMAT-statement for reading, skipping the complex parts
> and reading the real parts.  Do you use a similar trick, or do you have
> something better?
>
> Good luck with the calculations,
> thanks again to Peter Blaha for fixing the atpar.F,
>
> Kevin Jorissen
> EMAT, University of Antwerp
>
>
> ----- Original Message -----
> From: "Moreau Philippe" <Philippe.Moreau@cnrs-imn.fr>
> To: <wien@zeus.theochem.tuwien.ac.at>
> Sent: Thursday, October 10, 2002 3:18 PM
> Subject: [WIEN]: ELNES calculations with WIEN2k, wrong .qtl for isplit=99?
>
>
>   ==== Moreau Philippe submitted the following contribution: ====
>
>
> Dear all,
>
> We reported a couple of days ago a problem with the calculation of ELNES
>     spectra with WIEN2K last version (ISPLIT=99).
>   Thanks to the changes proposed by Peter (changes in atpar.F , thank you)
>     no error message appears anymore and case.qtl is not filled with
numerous
> and only zeros. Nevertheless, the obtained spectra are completely
different
> (totally wrong compared to experiments) from previous WIEN97.10
> calculations.
>   we succesufully used the WIEN2K chain (initelnes, tetra, telnes) on a
>     former case.qtl WIEN97 file.
>   so the problem probabily comes from lapw2 generating a wrong case.qtl.
>
> has anyone performed ELNES calculations with WIEN2K ? and if yes with what
>     changes if any ?
>   thanks
>
> Philippe
>
>
>
>
>
> --------------------------------------------------------------------------
>     --
>   | Dr. Philippe MOREAU |
> | |
> | Maître de Conférences à l'Université de Nantes |
> | Equipe PROSES (Propriétés, Réactivité, Organisation et Structure
>     Electro- |
>   | nique des Solides) |
> | |
> | INSTITUT DES MATERIAUX JEAN ROUXEL | Mailto:Philippe.Moreau@cnrs-imn.fr
>     |
>   | Laboratoire de Chimie des Solides | |
> | 2, rue de la Houssiniere | Phone: (33) 2 40 37 64 14 |
> | BP 32229 | Fax: (33) 2 40 37 39 95 |
> | 44322 NANTES CEDEX 3 | http://www.cnrs-imn.fr |
> | FRANCE | |
> --------------------------------------------------------------------------
>     -- ==== WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at To
(un)subscribe
> send mail to majordomo@zeus.theochem.tuwien.ac.at ====
>
> ====
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> ====
>
>
>
> --
>  -------------------------------------------------------------------------
- -
> | Florent BOUCHER                    |
|
> | Institut des Matériaux Jean Rouxel | Mailto:Florent.Boucher@cnrs-imn.fr
|
> | 2, rue de la Houssinière           | Phone: (33) 2 40 37 39 24
|
> | BP 32229                           | Fax:   (33) 2 40 37 39 95
|
> | 44322 NANTES CEDEX 3 (FRANCE)      | http://www.cnrs-imn.fr
|
>  -------------------------------------------------------------------------
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Date: Wed, 16 Oct 2002 18:06:16 +0900
From: Isao TANAKA <tanaka@cms.mtl.kyoto-u.ac.jp>
Subject: [WIEN]: Post-Doc position in Kyoto

====
Isao TANAKA <tanaka@cms.mtl.kyoto-u.ac.jp>
submitted the following contribution:
====

A joint program on computational materials science between Department of 
Materials Chemistry and Department of Materials Science & Engineering of 
Kyoto University, Japan has an immediate opening for a few Post-Doc 
scientists to support on-going activities in the group. Design and 
exploration of advanced materials by means of computational modeling and 
experimental works are the objectives of the group. Intimate collaborations 
with experimental groups in both academic and industry sites are being 
constructed. Materials of our interests include optical, electronic, 
functional, magnetic, structural, energy-storage, catalysis and other kinds 
of materials.
For details visit
http://cms.mtl.kyoto-u.ac.jp/users/tanaka/PostDocE.htm

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------------------------------

Date: Wed, 16 Oct 2002 17:56:36 +0800 (CST)
From: whoming@sohu.com
Subject: Re:Re: [WIEN]: About fine grained parallel computation in WIEN2K

====
whoming@sohu.com
submitted the following contribution:
====

- ------=_Part_928_58566.1034762196703
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Dear Peter Blaha,
           Thanks very much for your replying!
 But I just can understand clearly your comment and suggestions.
I have do grep :RKM of tic.scf1 and it looks like:

:RKM  : MATRIX SIZE  155LOs:  18  RKM= 6.93  WEIGHT= 1.00  PGR:
In modules.F IBLOCK is 128.  
        Would you please give me more suggestions on this problem?Thanks!
Yours,
       whoming
- ----- Original Message -----

From: Peter Blaha 
To: wien@zeus.theochem.tuwien.ac.at 
Subject: Re: [WIEN]: About fine grained parallel computation in WIEN2K
Sent: Wed Oct 16 14:07:37 CST 2002

====
Peter Blaha 
submitted the following contribution:
====

> Has anyone performed fine grained parallel calculation on SGI
> Origin 2000/38000?
> 2)But the difference appears from lapw2. "TOTAL CHARGE INSIDE
> SPHERE" in tic.output2 produced by fine grained
> parallel calculation differs from that either in "Serial calculation" or in
> "k-point parallel calculation".(In the "k-point parallel
> calculation",you have to add up all the correspond "TOTAL CHARGE INSIDE
> SPHERE" from all the tic.output2_* files.)
> This is the first difference.And also I found that there is "QTL-B Value
> .EQ.7.30302!!!!!!" in tic.output2_1 in the fine grained calculation.

Dear whoming

Probably you are using more processors than you have "blocks" of basis
functions. check that
#basis fkt/IBLOCK is larger than you number of processors

for #basis fkt do grep :rkm in TiC.scf1
for IBLOCK look in modules.F in SRC_lapw2 (usually 128)

Fine grain parallelization makes no sense for small cases like TiC.

Best wishes Georg


P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671 FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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<html>
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<body>
<P>Dear Peter Blaha,</P>
<P>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Thanks very much for your replying!</P>
<P>&nbsp;But I just can understand clearly your comment and suggestions.</P>
<P>I have do grep :RKM of tic.scf1 and it looks like:</P>
<P><BR>:RKM&nbsp; : MATRIX SIZE&nbsp; 155LOs:&nbsp; 18&nbsp; RKM= 6.93&nbsp; WEIGHT= 1.00&nbsp; PGR:</P>
<P>In modules.F IBLOCK is 128.&nbsp; </P>
<P>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Would you please give me more suggestions on this problem?Thanks!</P>
<P>Yours,</P>
<P>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; whoming</P>
<BLOCKQUOTE id=ori dir=ltr style="PADDING-RIGHT: 0px; PADDING-LEFT: 5px; FONT: 9pt ??; MARGIN-LEFT: 10px; BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
<DIV style="FONT-WEIGHT: normal; FONT-SIZE: 9pt; LINE-HEIGHT: normal; FONT-STYLE: normal; FONT-VARIANT: normal">----- Original Message -----</DIV><BR><B>From:</B> <A href="mailto:pblaha@theochem.tuwien.ac.at">Peter Blaha</A> <BR><B>To:</B> <A href="mailto:wien@zeus.theochem.tuwien.ac.at">wien@zeus.theochem.tuwien.ac.at</A> <BR><B>Subject:</B> Re: [WIEN]: About fine grained parallel computation in WIEN2K<BR><B>Sent:</B> Wed Oct 16 14:07:37 CST 2002<BR>
<P>====<BR>Peter Blaha <PBLAHA@THEOCHEM.TUWIEN.AC.AT><BR>submitted the following contribution:<BR>====<BR><BR>&gt; Has anyone performed fine grained parallel calculation on SGI<BR>&gt; Origin 2000/38000?<BR>&gt; 2)But the difference appears from lapw2. "TOTAL CHARGE INSIDE<BR>&gt; SPHERE" in tic.output2 produced by fine grained<BR>&gt; parallel calculation differs from that either in "Serial calculation" or in<BR>&gt; "k-point parallel calculation".(In the "k-point parallel<BR>&gt; calculation",you have to add up all the correspond "TOTAL CHARGE INSIDE<BR>&gt; SPHERE" from all the tic.output2_* files.)<BR>&gt; This is the first difference.And also I found that there is "QTL-B Value<BR>&gt; .EQ.7.30302!!!!!!" in tic.output2_1 in the fine grained calculation.<BR><BR>Dear whoming<BR><BR>Probably you are using more processors than you have "blocks" of basis<BR>functions. check that<BR>#basis fkt/IBLOCK is larger than you number of processors<BR><BR>for #basis fkt do grep :rkm in!
 TiC.scf1<BR>for IBLOCK look in modules.F in SRC_lapw2 (usually 128)<BR><BR>Fine grain parallelization makes no sense for small cases like TiC.<BR><BR>Best wishes Georg<BR><BR><BR>P.Blaha<BR>--------------------------------------------------------------------------<BR>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna<BR>Phone: +43-1-58801-15671 FAX: +43-1-58801-15698<BR>Email: blaha@theochem.tuwien.ac.at WWW: http://info.tuwien.ac.at/theochem/<BR>--------------------------------------------------------------------------<BR><BR>====<BR>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at<BR>To (un)subscribe send mail to<BR>majordomo@zeus.theochem.tuwien.ac.at<BR>====<BR></P></BLOCKQUOTE><BR><BR><BR><BR><hr size=1> 
</body>
</html>
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------------------------------

Date: Wed, 16 Oct 2002 14:38:40 +0200
From: Florent Boucher <Florent.Boucher@cnrs-imn.fr>
Subject: Re: TETRA / Re: [WIEN]: ELNES calculations with WIEN2k, wrong .qtl for isplit=99?

====
Florent Boucher <Florent.Boucher@cnrs-imn.fr>
submitted the following contribution:
====

Dear Kevin,
I had also a look for the 88 option. Effectively, in this case there is 
a problem.
outp writes lxdos2 complex numbers and tetra read lxdos2 real numbers...
I check the outp part and it seems that this program should be change in 
order to write only the real part of xqtl (imaginary part is always zero).
So I propose this change for outp.f

                 if(isplit(jatom).eq.88) then
                   read(15,208) (xqtl(i,i,1),i=1,lxdos2)
                   IF(jb.EQ.JBAND) WRITE(16,208)  &
                      (real(xqtl(i,i,1))/100.d0,i=1,lxdos2)   <==
                 ENDIF
  208              FORMAT((10F10.5))


Concerning the in1 options, we used LAPW(0) for all the Ylm except for 
those explicitely written in the in1 file.
Regards
Florent

Kevin Jorissen a écrit:

>====
>"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
>submitted the following contribution:
>====
>
>Dear Florent and Philippe,
>
>I have used the default .in1-file, specifying global LAPW (0) (as
>recommended in the UG) and APW (1) for all the choices on the next lines.
>Did you perform a 'full APW'-calculation? (I'll try).
>By the way, I did not receive the attachments to your mail.
>
>
>About the modification of tetra.f : I must apologize for being unclear.  The
>modification we make is for F-case (ISPLIT=88), where tetra reads :
> read(4,208)(xqtl(isort,i1),i1=1,lxdos2)
>  208 FORMAT((10F10.5))
>
>while outp.f writes :
>                 if(isplit(jatom).eq.88) then
>                   read(15,208) (xqtl(i,i,1),i=1,lxdos2)
>                   IF(jb.EQ.JBAND) WRITE(16,208)  &
>                      (xqtl(i,i,1)/100.d0,i=1,lxdos2)
>                 ENDIF
>  208              FORMAT((10F10.5))
>
>
>So, while your analysis is correct for the 99-case, there is still a
>conflict in the 88-case.  What I did is changing in tetra.f :
>
>                  if(text(isort)(13:20).eq.'xdos(i,j') then
>                    if(lxdos.ne.3) stop 'LXDOS must be 3 for ISPLIT 99 or
>88'
>                  read(4,208)(xqtl(isort,i1),i1=1,(lxdos2)*(lxdos2+1))
>                  else if(text(isort)(13:20).eq.'xdos(i,i') then
>                  read(4,207)(xqtl(isort,i1),i1=1,lxdos2)
>                  endif
>  208 FORMAT((10F10.5))
>  207 FORMAT(5(F10.5,10x))
>
>and this works.  Perhaps it would be preferable to make tetra read ALL the
>numbers, but I don't fully understand the working of tetra - maybe you can
>comment on this.
>Of course, one can always use 99-option (I don't use 88 often).
>
>
>Please do send me the files you intended to include, I promise to have a
>look at them asap.  bye!
>
>Kevin.
>
>
>
>  
>
- -- 
 --------------------------------------------------------------------------
| Florent BOUCHER                    |                                     |
| Institut des Matériaux Jean Rouxel | Mailto:Florent.Boucher@cnrs-imn.fr  |
| 2, rue de la Houssinière           | Phone: (33) 2 40 37 39 24           |
| BP 32229                           | Fax:   (33) 2 40 37 39 95           |
| 44322 NANTES CEDEX 3 (FRANCE)      | http://www.cnrs-imn.fr              |
 --------------------------------------------------------------------------



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------------------------------

Date: Wed, 16 Oct 2002 15:14:51 +0200
From: georg@chem.au.dk
Subject: Re:Re: [WIEN]: About fine grained parallel computation in WIEN2K

====
georg@chem.au.dk
submitted the following contribution:
====

You have 155 basis functions (lo's aren't paralised) and you block size is 128.
This means you have only two blocks and should max use two processors.

Quoting whoming@sohu.com:

> Dear Peter Blaha,
>            Thanks very much for your replying!
>  But I just can understand clearly your comment and suggestions.
> I have do grep :RKM of tic.scf1 and it looks like:
> 
> :RKM  : MATRIX SIZE  155LOs:  18  RKM= 6.93  WEIGHT= 1.00  PGR:
> In modules.F IBLOCK is 128.  
>         Would you please give me more suggestions on this problem?Thanks!
> Yours,
>        whoming
> ----- Original Message -----
> 
> From: Peter Blaha 
> To: wien@zeus.theochem.tuwien.ac.at 
> Subject: Re: [WIEN]: About fine grained parallel computation in WIEN2K
> Sent: Wed Oct 16 14:07:37 CST 2002
> 
> ====
> Peter Blaha 
> submitted the following contribution:
> ====
> 
> > Has anyone performed fine grained parallel calculation on SGI
> > Origin 2000/38000?
> > 2)But the difference appears from lapw2. "TOTAL CHARGE INSIDE
> > SPHERE" in tic.output2 produced by fine grained
> > parallel calculation differs from that either in "Serial calculation" or
> in
> > "k-point parallel calculation".(In the "k-point parallel
> > calculation",you have to add up all the correspond "TOTAL CHARGE INSIDE
> > SPHERE" from all the tic.output2_* files.)
> > This is the first difference.And also I found that there is "QTL-B Value
> > .EQ.7.30302!!!!!!" in tic.output2_1 in the fine grained calculation.
> 
> Dear whoming
> 
> Probably you are using more processors than you have "blocks" of basis
> functions. check that
> #basis fkt/IBLOCK is larger than you number of processors
> 
> for #basis fkt do grep :rkm in TiC.scf1
> for IBLOCK look in modules.F in SRC_lapw2 (usually 128)
> 
> Fine grain parallelization makes no sense for small cases like TiC.
> 
> Best wishes Georg
> 
> 
> P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671 FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at WWW: http://info.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
> 
> ====
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Date: Thu, 17 Oct 2002 17:55:08 -0600
From: Pablo de la Mora <pm@fciencias.unam.mx>
Subject: [WIEN]: total energy

====
Pablo de la Mora <pm@fciencias.unam.mx>
submitted the following contribution:
====

Dear Wien Users,
    Many times the total energy of the system jumps to a high (negative) 
value, most of the time it is not important but in other times it is.
    For example I was doing Ni for testing purposes and when I restarted 
the energy now was different.
aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653578
aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653534
aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -6538.210862
aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -8286.488860
aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =       -10034.766858
aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =       -10034.766826
aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653536
aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653525

On other case a supercell of CaCuO2:
:ENE  : ********** TOTAL ENERGY IN Ry =       -42866.543562
:ENE  : ********** TOTAL ENERGY IN Ry =       -42864.264895
:ENE  : ********** TOTAL ENERGY IN Ry =      -476714.854134
:ENE  : ********** TOTAL ENERGY IN Ry =      -476714.826215
....15 iterations
:ENE  : ********** TOTAL ENERGY IN Ry =      -476831.026046
:ENE  : ********** TOTAL ENERGY IN Ry =      -476870.308446
:ENE  : ********** TOTAL ENERGY IN Ry =       -42863.676057
:ENE  : ********** TOTAL ENERGY IN Ry =       -42871.305960
:ENE  : ********** TOTAL ENERGY IN Ry =       -42863.880914
:ENE  : ********** TOTAL ENERGY IN Ry =       -42864.285966
:ENE  : ********** TOTAL ENERGY IN Ry =       -42863.310026
    Is there something I haven't done (this happens in differents 
computing systems!)
    Thank you

        Pablo de la Mora

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Date: Fri, 18 Oct 2002 09:56:08 +0800 (CST)
From: yshzhang@theory.issp.ac.cn
Subject: [WIEN]: MPI

====
yshzhang@theory.issp.ac.cn
submitted the following contribution:
====

Dear all

I met a question about parallel using MPI.
The system I used is Linux(dell cluster node0-8).I used pgf90 and pgcc as 
the specify compiler.
When it asked "shared Memory achitechtrue?" answer "n"
Remote shell 'rsh'
"do you have MPI and Scalapack ......" y
compiler:pgf90

   Recommended options for system linuxpgi are:
         RP_LIB(SCALAPACK+PBLAS): -L /usr/local/SCALAPACK -L 
/usr/local/BLACS/LIB -lpblas -lredist -ltools -lscalapack -lfblacs -lblacs 
- -lmpi
         FPOPT(par.comp.options): -Mfreeform -fast -Kieee
         MPIRUN commando        : mpirun -np _NP_ -machinefile _HOSTS_ 
_EXEC_

   Current settings:
     RP  RP_LIB(SCALAPACK+PBLAS): -L /usr/local/SCALAPACK -L 
/usr/local/BLACS/LIB -lpblas -lredist -ltools -lscalapack -lfblacs -lblacs 
- -lmpi
     FP  FPOPT(par.comp.options): -Mfreeform -fast -Kieee
     MP  MPIRUN commando        : mpirun -np _NP_ -machinefile _HOSTS_ 
_EXEC_


and I save it. but when I recompile lapw0,lapw1 and lapw2
it gives such error


if [ -f .parallel ]; then \
   rm -f .parallel modules.o reallocate.o energy.o gtfnam.o lapw0.o  
*.mod; \
fi
touch .sequential
make lapw0 FORT=pgf90 FFLAGS=' -Mfreeform -fast -Kieee'
make[1]: Entering directory `/home/ysz/wien2k/SRC_lapw0'
pgcc -c cputim.c
pgf90 -Mfreeform -fast -Kieee -c modules.F
pgf90 -Mfreeform -fast -Kieee -c reallocate.f
pgf90 -Mfreeform -fast -Kieee -c ainv.f
pgf90 -Mfreeform -fast -Kieee -c blyp.f
pgf90 -Mfreeform -fast -Kieee -c charg2.f
pgf90 -Mfreeform -fast -Kieee -c charg3.f
pgf90 -Mfreeform -fast -Kieee -c charge.f
pgf90 -Mfreeform -fast -Kieee -c chfac.f
pgf90 -Mfreeform -fast -Kieee -c chslv.f
pgf90 -Mfreeform -fast -Kieee -c corgga.f
pgf90 -Mfreeform -fast -Kieee -c cub_xc_back.f
pgf90 -Mfreeform -fast -Kieee -c corlsd.f
pgf90 -Mfreeform -fast -Kieee -c dlu.f
pgf90 -Mfreeform -fast -Kieee -c drho.f
pgf90 -Mfreeform -fast -Kieee -c dfxhpbe.f
pgf90 -Mfreeform -fast -Kieee -c dylm.f
pgf90 -Mfreeform -fast -Kieee -c efg.f
pgf90 -Mfreeform -fast -Kieee -c energy.F
pgf90 -Mfreeform -fast -Kieee -c errclr.f
pgf90 -Mfreeform -fast -Kieee -c errflg.f
pgf90 -Mfreeform -fast -Kieee -c ev92.f
pgf90 -Mfreeform -fast -Kieee -c ev92ex.f
pgf90 -Mfreeform -fast -Kieee -c exch.f
pgf90 -Mfreeform -fast -Kieee -c exch17.f
pgf90 -Mfreeform -fast -Kieee -c exrevpbe.f
pgf90 -Mfreeform -fast -Kieee -c fithi.f
pgf90 -Mfreeform -fast -Kieee -c fxhpbe.f
pgf90 -Mfreeform -fast -Kieee -c gbass.f
pgf90 -Mfreeform -fast -Kieee -c gcor.f
pgf90 -Mfreeform -fast -Kieee -c gea.f
pgf90 -Mfreeform -fast -Kieee -c geaex.f
pgf90 -Mfreeform -fast -Kieee -c getfft.f
pgf90 -Mfreeform -fast -Kieee -c getff1.f
pgf90 -Mfreeform -fast -Kieee -c gpoint.f
pgf90 -Mfreeform -fast -Kieee -c grans.f
pgf90 -Mfreeform -fast -Kieee -c gtfnam.F
pgf90 -Mfreeform -fast -Kieee -c hcth.f
pgf90 -Mfreeform -fast -Kieee -c ifflim.f
pgf90 -Mfreeform -fast -Kieee -c kcis.f
pgf90 -Mfreeform -fast -Kieee -c lapw0.F
pgf90 -Mfreeform -fast -Kieee -c latgen.f
pgf90 -Mfreeform -fast -Kieee -c multfc.f
pgf90 -Mfreeform -fast -Kieee -c multsu.f
pgf90 -Mfreeform -fast -Kieee -c outerr.f
pgf90 -Mfreeform -fast -Kieee -c pbe1.f
pgf90 -Mfreeform -fast -Kieee -c poissn.f
pgf90 -Mfreeform -fast -Kieee -c potfac.f
pgf90 -Mfreeform -fast -Kieee -c pwxad4.f
pgf90 -Mfreeform -fast -Kieee -c pwxad5.f
pgf90 -Mfreeform -fast -Kieee -c qranf.f
pgf90 -Mfreeform -fast -Kieee -c readstruct.f
pgf90 -Mfreeform -fast -Kieee -c rean0.f
pgf90 -Mfreeform -fast -Kieee -c rean1.f
pgf90 -Mfreeform -fast -Kieee -c rean3.f
pgf90 -Mfreeform -fast -Kieee -c rean4.f
pgf90 -Mfreeform -fast -Kieee -c rotate.f
pgf90 -Mfreeform -fast -Kieee -c rotdef.f
pgf90 -Mfreeform -fast -Kieee -c setff0.f
pgf90 -Mfreeform -fast -Kieee -c setff1.f
pgf90 -Mfreeform -fast -Kieee -c setfft.f
pgf90 -Mfreeform -fast -Kieee -c setff2.f
pgf90 -Mfreeform -fast -Kieee -c seval.f
pgf90 -Mfreeform -fast -Kieee -c sevald.f
pgf90 -Mfreeform -fast -Kieee -c sevaldd.f
pgf90 -Mfreeform -fast -Kieee -c sevali.f
pgf90 -Mfreeform -fast -Kieee -c sevalin.f
pgf90 -Mfreeform -fast -Kieee -c sicpbe.f
pgf90 -Mfreeform -fast -Kieee -c sphbes.f
pgf90 -Mfreeform -fast -Kieee -c spline.f
pgf90 -Mfreeform -fast -Kieee -c srolyl.f
pgf90 -Mfreeform -fast -Kieee -c stern.f
pgf90 -Mfreeform -fast -Kieee -c sumfac.f
pgf90 -Mfreeform -fast -Kieee -c suml.f
pgf90 -Mfreeform -fast -Kieee -c th1.f
pgf90 -Mfreeform -fast -Kieee -c th2.f
pgf90 -Mfreeform -fast -Kieee -c vpw91.f
pgf90 -Mfreeform -fast -Kieee -c vresp.f
pgf90 -Mfreeform -fast -Kieee -c vs98.f
pgf90 -Mfreeform -fast -Kieee -c ylm.f
pgf90 -Mfreeform -fast -Kieee -c zfft3d.f
pgf90 -o lapw0 cputim.o modules.o reallocate.o ainv.o blyp.o charg2.o  
charg3.o charge.o chfac.o chslv.o  corgga.o  cub_xc_back.o corlsd.o dlu.o 
drho.o  dfxhpbe.o dylm.o  efg.o  energy.o errclr.o errflg.o ev92.o    
ev92ex.o exch.o exch17.o exrevpbe.o  fithi.o fxhpbe.o gbass.o gcor.o  
gea.o geaex.o  getfft.o  getff1.o gpoint.o  grans.o gtfnam.o hcth.o 
ifflim.o kcis.o lapw0.o  latgen.o  multfc.o multsu.o outerr.o  pbe1.o 
poissn.o potfac.o pwxad4.o pwxad5.o  qranf.o readstruct.o rean0.o rean1.o 
rean3.o  rean4.o  rotate.o  rotdef.o setff0.o  setff1.o  setfft.o setff2.o 
seval.o sevald.o sevaldd.o sevali.o sevalin.o sicpbe.o sphbes.o  spline.o 
srolyl.o stern.o sumfac.o  suml.o th1.o th2.o vpw91.o   vresp.o vs98.o 
vxc15.o vxc16.o vxc17.o vxc24.o  vxc26.o  vxclm2.o vxcpw2.o vxi35.o 
vxi35a.o workf1.o xcener.o  xcpot.o  xcpot1.o xcpot3.o ykav.o  ylm.o 
zfft3d.o   -L../SRC_lib
/usr/pgi/linux86/lib/libpgf902.a(cnfg.o): In function 
`__hpfio_scratch_name':
cnfg.o(.text+0x2a): the use of `tempnam' is dangerous, better use 
`mkstemp'
Linking:
make[1]: Leaving directory `/home/ysz/wien2k/SRC_lapw0'
make: *** No rule to make target `complex'.  Stop.
if [ -f .sequential ]; then \ 
   rm -f .sequential modules.o reallocate.o energy.o gtfnam.o lapw0.o  
*.mod; \
fi
touch .parallel
make PARALLEL='-DParallel' lapw0_mpi \
  FORT=pgf90 FFLAGS=' -Mfreeform -fast -Kieee '-DParallel''
make[1]: Entering directory `/home/ysz/wien2k/SRC_lapw0'
pgf90 -Mfreeform -fast -Kieee -DParallel -c modules.F
PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 20)
  0 inform,   0 warnings,   1 severes, 0 fatal for init_parallel
PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 43)
  0 inform,   0 warnings,   1 severes, 0 fatal for begend
make[1]: *** [modules.o] Error 1
make[1]: Leaving directory `/home/ysz/wien2k/SRC_lapw0'
make: *** [para] Error 2


My computer is really exist MPI!!!!!!
I am eager to your help!!!!!!!!
 -- Best Regards
YS Zhang

- ------------------------------------------------------------------------
 Address: Institute of Solid State Physics
          Chinese Academy of Sciences
          P.O.BOX 1129,230031 Hefei 
          P.R~China
 Tel:     086-551-5591464(Office)
          086-551-5592837(Home)
 Fax:     086-551-5591434
 WWW:     http://theory.issp.ac.cn/~yshzhang
- ------------------------------------------------------------------------


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------------------------------

Date: Fri, 18 Oct 2002 08:15:45 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: MPI

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Try to specify the path to the MPI library...

Torsten.

yshzhang@theory.issp.ac.cn wrote:

>====
>yshzhang@theory.issp.ac.cn
>submitted the following contribution:
>====
>
>Dear all
>
>I met a question about parallel using MPI.
>The system I used is Linux(dell cluster node0-8).I used pgf90 and pgcc as 
>the specify compiler.
>When it asked "shared Memory achitechtrue?" answer "n"
>Remote shell 'rsh'
>"do you have MPI and Scalapack ......" y
>compiler:pgf90
>
>   Recommended options for system linuxpgi are:
>         RP_LIB(SCALAPACK+PBLAS): -L /usr/local/SCALAPACK -L 
>/usr/local/BLACS/LIB -lpblas -lredist -ltools -lscalapack -lfblacs -lblacs 
>-lmpi
>         FPOPT(par.comp.options): -Mfreeform -fast -Kieee
>         MPIRUN commando        : mpirun -np _NP_ -machinefile _HOSTS_ 
>_EXEC_
>
>   Current settings:
>     RP  RP_LIB(SCALAPACK+PBLAS): -L /usr/local/SCALAPACK -L 
>/usr/local/BLACS/LIB -lpblas -lredist -ltools -lscalapack -lfblacs -lblacs 
>-lmpi
>     FP  FPOPT(par.comp.options): -Mfreeform -fast -Kieee
>     MP  MPIRUN commando        : mpirun -np _NP_ -machinefile _HOSTS_ 
>_EXEC_
>
>
<snip>

>
>
>My computer is really exist MPI!!!!!!
>I am eager to your help!!!!!!!!
> -- Best Regards
>YS Zhang
>
>------------------------------------------------------------------------
> Address: Institute of Solid State Physics
>          Chinese Academy of Sciences
>          P.O.BOX 1129,230031 Hefei 
>          P.R~China
> Tel:     086-551-5591464(Office)
>          086-551-5592837(Home)
> Fax:     086-551-5591434
> WWW:     http://theory.issp.ac.cn/~yshzhang
>------------------------------------------------------------------------
>
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Fri, 18 Oct 2002 08:54:54 +0200
From: Florent Boucher <Florent.Boucher@cnrs-imn.fr>
Subject: Re: [WIEN]: total energy

====
Florent Boucher <Florent.Boucher@cnrs-imn.fr>
submitted the following contribution:
====

Dear Pablo,
the idea is to erase the scf (and may be broydens files)  before you 
restart the job. It seems to me that this problem appears when you 
restart the same type of job.
However, if you change RKMAX or number of kpoints there is no problem.
Please, have a look  in the :DIS line. I think the charge density is 
already converged. This is just the sum of the different contributions 
to the total energy that is done in a "bad way" by the mixer program.
Regards
Florent

Pablo de la Mora a écrit:

> ====
> Pablo de la Mora <pm@fciencias.unam.mx>
> submitted the following contribution:
> ====
>
> Dear Wien Users,
>    Many times the total energy of the system jumps to a high 
> (negative) value, most of the time it is not important but in other 
> times it is.
>    For example I was doing Ni for testing purposes and when I 
> restarted the energy now was different.
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653578
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653534
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -6538.210862
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -8286.488860
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =       -10034.766858
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =       -10034.766826
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653536
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653525
>
> On other case a supercell of CaCuO2:
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42866.543562
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42864.264895
> :ENE  : ********** TOTAL ENERGY IN Ry =      -476714.854134
> :ENE  : ********** TOTAL ENERGY IN Ry =      -476714.826215
> ....15 iterations
> :ENE  : ********** TOTAL ENERGY IN Ry =      -476831.026046
> :ENE  : ********** TOTAL ENERGY IN Ry =      -476870.308446
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42863.676057
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42871.305960
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42863.880914
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42864.285966
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42863.310026
>    Is there something I haven't done (this happens in differents 
> computing systems!)
>    Thank you
>
>        Pablo de la Mora
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

- -- 
 --------------------------------------------------------------------------
| Florent BOUCHER                    |                                     |
| Institut des Matériaux Jean Rouxel | Mailto:Florent.Boucher@cnrs-imn.fr  |
| 2, rue de la Houssinière           | Phone: (33) 2 40 37 39 24           |
| BP 32229                           | Fax:   (33) 2 40 37 39 95           |
| 44322 NANTES CEDEX 3 (FRANCE)      | http://www.cnrs-imn.fr              |
 --------------------------------------------------------------------------



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------------------------------

Date: Fri, 18 Oct 2002 14:57:38 +0800 (CST)
From: yshzhang@theory.issp.ac.cn
Subject: Re: [WIEN]: MPI

====
yshzhang@theory.issp.ac.cn
submitted the following contribution:
====

Dear Prof.
> Try to specify the path to the MPI library...

Thanks for your replay.
The MPI(the file of mpif.h) is set in /usr/lam-6.5.2/include.and I add a 
path in .cshrc as:
 set path = ( /usr/lam-6.5.2/include $path .)

But it dosen't work.Even I put mpif.h in SRC_lib or modified it in 
./siteconfig_lapw

     Recommended options for system linuxpgi are:
         RP_LIB(SCALAPACK+PBLAS): -L /usr/local/SCALAPACK -L 
/usr/local/BLACS/LIB -lpblas -lredist -ltools -lscalapack -lfblacs -lblacs 
- -lmpi
         FPOPT(par.comp.options): -Mfreeform -fast -Kieee
         MPIRUN commando        : mpirun -np _NP_ -machinefile _HOSTS_ 
_EXEC_

   Current settings:
     RP  RP_LIB(SCALAPACK+PBLAS): -L /usr/local/SCALAPACK -L 
/usr/local/BLACS/LIB -L /usr/lam-6.5.2/include -lpblas -lredist -ltools 
- -lscalapack -lfblacs -lblacs -lmpi
     FP  FPOPT(par.comp.options): -Mfreeform -fast -Kieee
     MP  MPIRUN commando        : mpirun -np _NP_ -machinefile _HOSTS_ 
_EXEC_

The same error is occured as:
PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 20)
  0 inform,   0 warnings,   1 severes, 0 fatal for init_parallel
PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 43)
  0 inform,   0 warnings,   1 severes, 0 fatal for begend
make[1]: *** [modules.o] Error 1
make[1]: Leaving directory `/home/ysz/wien2k/SRC_lapw0'
make: *** [para] Error 2
Copying programs
  SRC_lapw0/lapw0
cp: cannot create regular file `/home/ysz/wien2k/lapw0': Permission denied

done.

Compile messages for each SRC_* directory can be found in the
file "compile.msg".

Compile time errors (if any) were:
SRC_lapw0/compile.msg:make[1]: *** [modules.o] Error 1
SRC_lapw0/compile.msg:make: *** [para] Error 2

- -- 
Best Regards
YS Zhang

- ------------------------------------------------------------------------
 Address: Institute of Solid State Physics
          Chinese Academy of Sciences
          P.O.BOX 1129,230031 Hefei 
          P.R~China
 Tel:     086-551-5591464(Office)
          086-551-5592837(Home)
 Fax:     086-551-5591434
 WWW:     http://theory.issp.ac.cn/~yshzhang
- ------------------------------------------------------------------------


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------------------------------

Date: Fri, 18 Oct 2002 09:43:40 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: MPI

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Mr. Chang,

the mpif.h is only a header file (from C). What you need to do is 
probably two-fold. (1) you need to make sure that the mpif.h is in the 
path the compiler searches for headerfiles in. I am not sure that 
including it in the "path" is enough. It is typically in a shell 
environment variable, or added specifically during compilation. Consult 
the manual of the compiler or the system administrator. (2) You need a 
- -L/path/to/libmpi.a (or libmpi.so or whatever it is called) type of 
specification, just like it is done in the section with BLAS and LAPACK, 
but it appear that you have that, so check if it is correct.

If anyone has specific experiences with linux and mpi, please make 
additional comments...

Best regards,
Torsten Andersen.

yshzhang@theory.issp.ac.cn wrote:

>====
>yshzhang@theory.issp.ac.cn
>submitted the following contribution:
>====
>
>Dear Prof.
>
>>Try to specify the path to the MPI library...
>>
>
>Thanks for your replay.
>The MPI(the file of mpif.h) is set in /usr/lam-6.5.2/include.and I add a 
>path in .cshrc as:
> set path = ( /usr/lam-6.5.2/include $path .)
>
>But it dosen't work.Even I put mpif.h in SRC_lib or modified it in 
>./siteconfig_lapw
>
>     Recommended options for system linuxpgi are:
>         RP_LIB(SCALAPACK+PBLAS): -L /usr/local/SCALAPACK -L 
>/usr/local/BLACS/LIB -lpblas -lredist -ltools -lscalapack -lfblacs -lblacs 
>-lmpi
>         FPOPT(par.comp.options): -Mfreeform -fast -Kieee
>         MPIRUN commando        : mpirun -np _NP_ -machinefile _HOSTS_ 
>_EXEC_
>
>   Current settings:
>     RP  RP_LIB(SCALAPACK+PBLAS): -L /usr/local/SCALAPACK -L 
>/usr/local/BLACS/LIB -L /usr/lam-6.5.2/include -lpblas -lredist -ltools 
>-lscalapack -lfblacs -lblacs -lmpi
>     FP  FPOPT(par.comp.options): -Mfreeform -fast -Kieee
>     MP  MPIRUN commando        : mpirun -np _NP_ -machinefile _HOSTS_ 
>_EXEC_
>
>The same error is occured as:
>PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 20)
>  0 inform,   0 warnings,   1 severes, 0 fatal for init_parallel
>PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 43)
>  0 inform,   0 warnings,   1 severes, 0 fatal for begend
>make[1]: *** [modules.o] Error 1
>make[1]: Leaving directory `/home/ysz/wien2k/SRC_lapw0'
>make: *** [para] Error 2
>Copying programs
>  SRC_lapw0/lapw0
>cp: cannot create regular file `/home/ysz/wien2k/lapw0': Permission denied
>
>done.
>
>Compile messages for each SRC_* directory can be found in the
>file "compile.msg".
>
>Compile time errors (if any) were:
>SRC_lapw0/compile.msg:make[1]: *** [modules.o] Error 1
>SRC_lapw0/compile.msg:make: *** [para] Error 2
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Fri, 18 Oct 2002 11:36:18 +0200
From: Peer Kruse <kruse@lem.uni-karlsruhe.de>
Subject: Re: [WIEN]: MPI

====
Peer Kruse <kruse@lem.uni-karlsruhe.de>
submitted the following contribution:
====

1. Drop the .a after  -L/path/to/libmpi it is inserted automatically
After  -L the path to the Library is set. This is necessary for linking.
You are needing the header files. Their  path is given by 
- -I/path_to_headerfiles

Best Regards
Peer Kruse

Torsten Andersen wrote:

> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
>
> Dear Mr. Chang,
>
> the mpif.h is only a header file (from C). What you need to do is 
> probably two-fold. (1) you need to make sure that the mpif.h is in the 
> path the compiler searches for headerfiles in. I am not sure that 
> including it in the "path" is enough. It is typically in a shell 
> environment variable, or added specifically during compilation. 
> Consult the manual of the compiler or the system administrator. (2) 
> You need a -L/path/to/libmpi.a (or libmpi.so or whatever it is called) 
> type of specification, just like it is done in the section with BLAS 
> and LAPACK, but it appear that you have that, so check if it is correct.
>
> If anyone has specific experiences with linux and mpi, please make 
> additional comments...
>
> Best regards,
> Torsten Andersen.
>
> yshzhang@theory.issp.ac.cn wrote:
>
>> ====
>> yshzhang@theory.issp.ac.cn
>> submitted the following contribution:
>> ====
>>
>> Dear Prof.
>>
>>> Try to specify the path to the MPI library...
>>>
>>
>> Thanks for your replay.
>> The MPI(the file of mpif.h) is set in /usr/lam-6.5.2/include.and I 
>> add a path in .cshrc as:
>> set path = ( /usr/lam-6.5.2/include $path .)
>>
>> But it dosen't work.Even I put mpif.h in SRC_lib or modified it in 
>> ./siteconfig_lapw
>>
>>     Recommended options for system linuxpgi are:
>>         RP_LIB(SCALAPACK+PBLAS): -L /usr/local/SCALAPACK -L 
>> /usr/local/BLACS/LIB -lpblas -lredist -ltools -lscalapack -lfblacs 
>> -lblacs -lmpi
>>         FPOPT(par.comp.options): -Mfreeform -fast -Kieee
>>         MPIRUN commando        : mpirun -np _NP_ -machinefile _HOSTS_ 
>> _EXEC_
>>
>>   Current settings:
>>     RP  RP_LIB(SCALAPACK+PBLAS): -L /usr/local/SCALAPACK -L 
>> /usr/local/BLACS/LIB -L /usr/lam-6.5.2/include -lpblas -lredist 
>> -ltools -lscalapack -lfblacs -lblacs -lmpi
>>     FP  FPOPT(par.comp.options): -Mfreeform -fast -Kieee
>>     MP  MPIRUN commando        : mpirun -np _NP_ -machinefile _HOSTS_ 
>> _EXEC_
>>
>> The same error is occured as:
>> PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 20)
>>  0 inform,   0 warnings,   1 severes, 0 fatal for init_parallel
>> PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 43)
>>  0 inform,   0 warnings,   1 severes, 0 fatal for begend
>> make[1]: *** [modules.o] Error 1
>> make[1]: Leaving directory `/home/ysz/wien2k/SRC_lapw0'
>> make: *** [para] Error 2
>> Copying programs
>>  SRC_lapw0/lapw0
>> cp: cannot create regular file `/home/ysz/wien2k/lapw0': Permission 
>> denied
>>
>> done.
>>
>> Compile messages for each SRC_* directory can be found in the
>> file "compile.msg".
>>
>> Compile time errors (if any) were:
>> SRC_lapw0/compile.msg:make[1]: *** [modules.o] Error 1
>> SRC_lapw0/compile.msg:make: *** [para] Error 2
>>
>



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------------------------------

Date: Fri, 18 Oct 2002 10:31:31 -0600
From: Pablo de la Mora <pm@fciencias.unam.mx>
Subject: Re: [WIEN]: total energy

====
Pablo de la Mora <pm@fciencias.unam.mx>
submitted the following contribution:
====

Dear Florent,
    Thank you for your reply. Many times the total energy jumps when I 
restart the job but I do a clean and a save in between, this erases the 
scf and broyden files, but this time the energy jumped in the middle of 
a run.
    It surely jumps when the number of iterations reaches 99, then it 
changes, so a difficult convergency runs into this problem. Long time 
ago Peter Blaha told me to save before I resatart a run, I have not done 
it for these cases but I don't think it would work since the iterations 
number continues to increase.
    Yours

        Pablo

Florent Boucher wrote:

> ====
> Florent Boucher <Florent.Boucher@cnrs-imn.fr>
> submitted the following contribution:
> ====
>
> Dear Pablo,
> the idea is to erase the scf (and may be broydens files)  before you 
> restart the job. It seems to me that this problem appears when you 
> restart the same type of job.
> However, if you change RKMAX or number of kpoints there is no problem.
> Please, have a look  in the :DIS line. I think the charge density is 
> already converged. This is just the sum of the different contributions 
> to the total energy that is done in a "bad way" by the mixer program.
> Regards
> Florent
>
> Pablo de la Mora a écrit:
>
>> ====
>> Pablo de la Mora <pm@fciencias.unam.mx>
>> submitted the following contribution:
>> ====
>>
>> Dear Wien Users,
>>    Many times the total energy of the system jumps to a high 
>> (negative) value, most of the time it is not important but in other 
>> times it is.
>>    For example I was doing Ni for testing purposes and when I 
>> restarted the energy now was different.
>> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653578
>> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653534
>> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -6538.210862
>> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -8286.488860
>> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =       -10034.766858
>> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =       -10034.766826
>> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653536
>> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653525
>>
>> On other case a supercell of CaCuO2:
>> :ENE  : ********** TOTAL ENERGY IN Ry =       -42866.543562
>> :ENE  : ********** TOTAL ENERGY IN Ry =       -42864.264895
>> :ENE  : ********** TOTAL ENERGY IN Ry =      -476714.854134
>> :ENE  : ********** TOTAL ENERGY IN Ry =      -476714.826215
>> ....15 iterations
>> :ENE  : ********** TOTAL ENERGY IN Ry =      -476831.026046
>> :ENE  : ********** TOTAL ENERGY IN Ry =      -476870.308446
>> :ENE  : ********** TOTAL ENERGY IN Ry =       -42863.676057
>> :ENE  : ********** TOTAL ENERGY IN Ry =       -42871.305960
>> :ENE  : ********** TOTAL ENERGY IN Ry =       -42863.880914
>> :ENE  : ********** TOTAL ENERGY IN Ry =       -42864.285966
>> :ENE  : ********** TOTAL ENERGY IN Ry =       -42863.310026
>>    Is there something I haven't done (this happens in differents 
>> computing systems!)
>>    Thank you
>>
>>        Pablo de la Mora
>>
>> ====
>> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>> To (un)subscribe send mail to
>> majordomo@zeus.theochem.tuwien.ac.at
>> ====
>>
>


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------------------------------

Date: Fri, 18 Oct 2002 17:43:28 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: total energy

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Pablo,

I experienced this a while back. Reducing the compilation optimisation 
was the solution in my case. I do not have a clear picture of what goes 
wrong, but it could have to do with sloppy rounding of numbers at higher 
(agressive) optimisation levels. In cases where an experimentally stable 
phase exists, 99 iterations are usually way too many, unless you have a 
very big system.

Best regards,
Torsten Andersen.

Pablo de la Mora wrote:

> ====
> Pablo de la Mora <pm@fciencias.unam.mx>
> submitted the following contribution:
> ====
>
> Dear Wien Users,
>    Many times the total energy of the system jumps to a high 
> (negative) value, most of the time it is not important but in other 
> times it is.
>    For example I was doing Ni for testing purposes and when I 
> restarted the energy now was different.
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653578
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653534
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -6538.210862
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -8286.488860
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =       -10034.766858
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =       -10034.766826
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653536
> aa.scf::ENE  : ********** TOTAL ENERGY IN Ry =        -3041.653525
>
> On other case a supercell of CaCuO2:
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42866.543562
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42864.264895
> :ENE  : ********** TOTAL ENERGY IN Ry =      -476714.854134
> :ENE  : ********** TOTAL ENERGY IN Ry =      -476714.826215
> ....15 iterations
> :ENE  : ********** TOTAL ENERGY IN Ry =      -476831.026046
> :ENE  : ********** TOTAL ENERGY IN Ry =      -476870.308446
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42863.676057
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42871.305960
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42863.880914
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42864.285966
> :ENE  : ********** TOTAL ENERGY IN Ry =       -42863.310026
>    Is there something I haven't done (this happens in differents 
> computing systems!)
>    Thank you
>
>        Pablo de la Mora
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Fri, 18 Oct 2002 17:40:36 +0100
From: "Xiangyuan Cui" <x.cui@pgr.salford.ac.uk>
Subject: Re: [WIEN]: total energy

====
"Xiangyuan Cui" <x.cui@pgr.salford.ac.uk>
submitted the following contribution:
====

Hi Pablo :)

i think it is not a serious problom if i understand it correctly. when this
behaviour occurs (more than 99 iterations) , i just change the case.scf file
into another name. or delete some lines in the *.scf, then the convergence
will go back to the normal behaviour after two more iterations.

  yours,

        xiangyuan


> Dear Florent,
>     Thank you for your reply. Many times the total energy jumps when I
> restart the job but I do a clean and a save in between, this erases the
> scf and broyden files, but this time the energy jumped in the middle of
> a run.
>     It surely jumps when the number of iterations reaches 99, then it
> changes, so a difficult convergency runs into this problem. Long time
> ago Peter Blaha told me to save before I resatart a run, I have not done
> it for these cases but I don't think it would work since the iterations
> number continues to increase.
>     Yours
>
>         Pablo


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Date: Fri, 18 Oct 2002 18:39:54 -0600
From: Pablo de la Mora <pm@fciencias.unam.mx>
Subject: Re: [WIEN]: problems with parallel execution

====
Pablo de la Mora <pm@fciencias.unam.mx>
submitted the following contribution:
====


- --------------030909060102080607050106
Content-Type: text/plain; charset=us-ascii; format=flowed
Content-Transfer-Encoding: 7bit

Dear Dr. Blaha,
    I did not respond earlier since the error was not reproduced 
immediatlely and I was busy.

>The problems you have given below may have several reasons and one needs much
>more info and tests.
>
>a) Does it never crash with the two 1 GHz machines ?
>
***    So far it works fine.

>b) Does it always or sometimes crash when including the 500 MHz processors ?
>
***    Most all the time but now always

>c) Only this case crashes or all/some others too ?
>
***    Many other cases crash

>Common directory NFS mounted ? WIEN2k runs everywhere ?
>
***    Yes

>can you connect to all machines without password ?
>
***    Yes

>Slow network connection ? (In particular when the error occurs only
>occasional) 
>
***    I don't know but the cluster has a switch, so I presume that the 
connection is fast and good

>Did lapw1 work in parallel ? 
>
***    Yes

>Do you see all vector_* fileswith proper (new) date ? 
>
***    Yes

>What happens when you run  x lapw2 -p interactively ?
>
***    It crashes

- ---------------------------------- end of nohup.out
 LAPW1 END
60.90user 1.16system 2:03.40elapsed 50%CPU (0avgtext+0avgdata 0maxresident)k
0inputs+0outputs (389major+107814minor)pagefaults 0swaps
PGFIO-F-252/list-directed read/unit=29/operation attempted after end of 
file.
 File name = dos.energydn_19    formatted, sequential access   record = 210
 In source file fermi.f, at line number 63
cp: .in.tmp: No such file or directory
rm: cannot remove `.in.tmp': No such file or directory
rm: cannot remove `.in.tmp1': No such file or directory
**************************************************
    On other issues:
First
    I still like 'Wien in the Box', I find it very friendly and using 
the navigator (I use netscape) I find it clumsy in the Struct Generator.
    Unfortunately it is not being mantained and sometimes it gives 
errors when the struct generator is used more than once for the same 
case (for correcting a coordinate or changeing the space group).

Second
    Running lstart one of the important parameters is the charge that 
leaks outside the muffin tin sphere. case.outputst gives:

 TOTAL CORE-CHARGE:                  2.000000000000460    
 TOTAL CORE-CHARGE INSIDE SPHERE:    1.999931688322383    

I suggest that the second line should be changed to

TOTAL CORE-CHARGE OUTSIDE SPHERE:

That is, lstart.f should have:
- -------------
 9120 continue
      CTEST=1.d0
      CALL SOMM (DR,Dp,DQ,DPAS,CTEST,0,NP)
      WRITE(6,*) 'TOTAL CORE-CHARGE:               ',CTEST
      CALL SOMM (DR,Dp,DQ,DPAS,CTEST1,0,NP0)
      WRITE(6,*) 'TOTAL CORE-CHARGE OUTSIDE SPHERE: ',CTEST1-CTEST <===
      if(ctest-ctest1.gt.0.01) write(6,*) 'WARNING:',ctest-ctest1, &
        ' CORE electrons leak out of MT-sphere !!!!'
- -------------------
CTEST1-CTEST has to be less than 0.001 (I think). In this way it is clearer.

    Thanks
            Pablo de la Mora

>Regards
>
>>>   I am having problems with parallel execution. I am doing a
>>>supercell for doping, it worked fine with a supercell with 4 cells,
>>>but with 2 cells it crashed.
>>>
>>>------------ End of the 'dayfile'
>>>1.230u 0.930s 3:02.72 1.1%    0+0k 0+0io 60807pf+0w
>>>
>>>>  lapw2 -up -p    (02:06:41) running LAPW2 in parallel mode
>>>>
>>>**  LAPW2 crashed!
>>>0.080u 0.070s 0:00.15 100.0%    0+0k 0+0io 4056pf+0w
>>>   This has happened before in other cases. Sometimes the same case
>>>crashes and sometimes it does not!
>>>   The cluster has 6 machines
>>>   two with two 1GHz intel processors each
>>>   four with one 500MHz  intel processor
>>>   Thanks
>>>
>>I want to add that I did a calculation with the two dual (two 1GHz
>>processors per machine; hydra and nodo1) the calculation did not crash:
>>
>>-------------------- .machines file
>>2:hydra
>>2:hydra
>>2.nodo1
>>2:nodo1
>>----------------------
>>
>>but with the non homogeneous cluster (including the 500MHz processors;
>>nodo3,...) it did crash:
>>
>>-------------------- .machines file
>>2:hydra
>>2:hydra
>>2.nodo1
>>2:nodo1
>>1:nodo3
>>1:nodo4
>>1:nodo5
>>
>
>                                      P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>



- --------------030909060102080607050106
Content-Type: text/html; charset=us-ascii
Content-Transfer-Encoding: 7bit

<html>
<head>
</head>
<body>
Dear Dr. Blaha,<br>
&nbsp;&nbsp;&nbsp; I did not respond earlier since the error was not reproduced immediatlely
and I was busy.<br>
<blockquote type="cite" cite="mid:Pine.LNX.4.33.0210100816310.9876-100000@susi.theochem.tuwien.ac.at">
  <pre wrap="">The problems you have given below may have several reasons and one needs much<br>more info and tests.<br><br>a) Does it never crash with the two 1 GHz machines ?</pre>
  </blockquote>
 ***&nbsp;&nbsp;&nbsp; So far it works fine.<br>
  <blockquote type="cite" cite="mid:Pine.LNX.4.33.0210100816310.9876-100000@susi.theochem.tuwien.ac.at">
    <pre wrap="">b) Does it always or sometimes crash when including the 500 MHz processors ?</pre>
    </blockquote>
 ***&nbsp;&nbsp;&nbsp; Most all the time but now always<br>
    <blockquote type="cite" cite="mid:Pine.LNX.4.33.0210100816310.9876-100000@susi.theochem.tuwien.ac.at">
      <pre wrap="">c) Only this case crashes or all/some others too ?</pre>
      </blockquote>
 ***&nbsp;&nbsp;&nbsp; Many other cases crash<br>
      <blockquote type="cite" cite="mid:Pine.LNX.4.33.0210100816310.9876-100000@susi.theochem.tuwien.ac.at">
        <pre wrap="">Common directory NFS mounted ? WIEN2k runs everywhere ?</pre>
        </blockquote>
 ***&nbsp;&nbsp;&nbsp; Yes<br>
        <blockquote type="cite" cite="mid:Pine.LNX.4.33.0210100816310.9876-100000@susi.theochem.tuwien.ac.at">
          <pre wrap="">can you connect to all machines without password ?</pre>
          </blockquote>
 ***&nbsp;&nbsp;&nbsp; Yes<br>
          <blockquote type="cite" cite="mid:Pine.LNX.4.33.0210100816310.9876-100000@susi.theochem.tuwien.ac.at">
            <pre wrap="">Slow network connection ? (In particular when the error occurs only<br>occasional) </pre>
            </blockquote>
 ***&nbsp;&nbsp;&nbsp; I don't know but the cluster has a switch, so I presume that the
connection is fast and good<br>
            <blockquote type="cite" cite="mid:Pine.LNX.4.33.0210100816310.9876-100000@susi.theochem.tuwien.ac.at">
              <pre wrap="">Did lapw1 work in parallel ? </pre>
              </blockquote>
 ***&nbsp;&nbsp;&nbsp; Yes<br>
              <blockquote type="cite" cite="mid:Pine.LNX.4.33.0210100816310.9876-100000@susi.theochem.tuwien.ac.at">
                <pre wrap="">Do you see all vector_* fileswith proper (new) date ? </pre>
                </blockquote>
 ***&nbsp;&nbsp;&nbsp; Yes<br>
                <blockquote type="cite" cite="mid:Pine.LNX.4.33.0210100816310.9876-100000@susi.theochem.tuwien.ac.at">
                  <pre wrap="">What happens when you run  x lapw2 -p interactively ?</pre>
                  </blockquote>
 ***&nbsp;&nbsp;&nbsp; It crashes<br>
                  <br>
- ---------------------------------- end of nohup.out<br>
&nbsp;LAPW1 END<br>
60.90user 1.16system 2:03.40elapsed 50%CPU (0avgtext+0avgdata 0maxresident)k<br>
0inputs+0outputs (389major+107814minor)pagefaults 0swaps<br>
PGFIO-F-252/list-directed read/unit=29/operation attempted after end of file.<br>
&nbsp;File name = dos.energydn_19&nbsp;&nbsp;&nbsp; formatted, sequential access&nbsp;&nbsp; record = 210<br>
&nbsp;In source file fermi.f, at line number 63<br>
cp: .in.tmp: No such file or directory<br>
rm: cannot remove `.in.tmp': No such file or directory<br>
rm: cannot remove `.in.tmp1': No such file or directory<br>
**************************************************<br>
&nbsp;&nbsp;&nbsp; On other issues:<br>
First<br>
&nbsp;&nbsp;&nbsp; I still like 'Wien in the Box', I find it very friendly and using the
navigator (I use netscape) I find it clumsy in the Struct Generator.<br>
&nbsp;&nbsp;&nbsp; Unfortunately it is not being mantained and sometimes it gives errors
when the struct generator is used more than once for the same case (for correcting
a coordinate or changeing the space group).<br>
                  <br>
Second<br>
&nbsp;&nbsp; &nbsp;Running lstart one of the important parameters is the charge that leaks
outside the muffin tin sphere. case.outputst gives:<br>
                  <br>
&nbsp;TOTAL CORE-CHARGE:&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 2.000000000000460&nbsp;&nbsp;&nbsp;&nbsp; <br>
&nbsp;TOTAL CORE-CHARGE INSIDE SPHERE:&nbsp;&nbsp;&nbsp; 1.999931688322383&nbsp;&nbsp;&nbsp;&nbsp; <br>
                  <br>
I suggest that the second line should be changed to<br>
                  <br>
TOTAL CORE-CHARGE OUTSIDE SPHERE: <br>
                  <br>
That is, lstart.f should have:<br>
- -------------<br>
&nbsp;9120 continue<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; CTEST=1.d0<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; CALL SOMM (DR,Dp,DQ,DPAS,CTEST,0,NP)<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; WRITE(6,*) 'TOTAL CORE-CHARGE:&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; ',CTEST<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; CALL SOMM (DR,Dp,DQ,DPAS,CTEST1,0,NP0)<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; WRITE(6,*) 'TOTAL CORE-CHARGE OUTSIDE SPHERE: ',CTEST1-CTEST &lt;===<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; if(ctest-ctest1.gt.0.01) write(6,*) 'WARNING:',ctest-ctest1, &amp;<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; ' CORE electrons leak out of MT-sphere !!!!'<br>
- -------------------<br>
CTEST1-CTEST has to be less than 0.001 (I think). In this way it is clearer.<br>
                  <br>
&nbsp;&nbsp;&nbsp; Thanks<br>
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; Pablo de la Mora<br>
                  <blockquote type="cite" cite="mid:Pine.LNX.4.33.0210100816310.9876-100000@susi.theochem.tuwien.ac.at">
                    <pre wrap="">Regards<br><br></pre>
                    <blockquote type="cite">
                      <blockquote type="cite">
                        <pre wrap="">   I am having problems with parallel execution. I am doing a<br>supercell for doping, it worked fine with a supercell with 4 cells,<br>but with 2 cells it crashed.<br><br>------------ End of the 'dayfile'<br>1.230u 0.930s 3:02.72 1.1%    0+0k 0+0io 60807pf+0w<br></pre>
                        <blockquote type="cite">
                          <pre wrap="">  lapw2 -up -p    (02:06:41) running LAPW2 in parallel mode<br></pre>
                          </blockquote>
                          <pre wrap="">**  LAPW2 crashed!<br>0.080u 0.070s 0:00.15 100.0%    0+0k 0+0io 4056pf+0w<br>   This has happened before in other cases. Sometimes the same case<br>crashes and sometimes it does not!<br>   The cluster has 6 machines<br>   two with two 1GHz intel processors each<br>   four with one 500MHz  intel processor<br>   Thanks<br></pre>
                          </blockquote>
                          <pre wrap="">I want to add that I did a calculation with the two dual (two 1GHz<br>processors per machine; hydra and nodo1) the calculation did not crash:<br><br>-------------------- .machines file<br>2:hydra<br>2:hydra<br>2.nodo1<br>2:nodo1<br>----------------------<br><br>but with the non homogeneous cluster (including the 500MHz processors;<br>nodo3,...) it did crash:<br><br>-------------------- .machines file<br>2:hydra<br>2:hydra<br>2.nodo1<br>2:nodo1<br>1:nodo3<br>1:nodo4<br>1:nodo5<br></pre>
                          </blockquote>
                          <pre wrap=""><!----><br>                                      P.Blaha<br>--------------------------------------------------------------------------<br>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna<br>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698<br>Email: <a class="moz-txt-link-abbreviated" href="mailto:blaha@theochem.tuwien.ac.at">blaha@theochem.tuwien.ac.at</a>    WWW: <a class="moz-txt-link-freetext" href="http://info.tuwien.ac.at/theochem/">http://info.tuwien.ac.at/theochem/</a><br>--------------------------------------------------------------------------<br><br>====<br>WIEN Mailing list: <a class="moz-txt-link-abbreviated" href="mailto:wien@zeus.theochem.tuwien.ac.at">wien@zeus.theochem.tuwien.ac.at</a><br>To (un)subscribe send mail to<br><a class="moz-txt-link-abbreviated" href="mailto:majordomo@zeus.theochem.tuwien.ac.at">majordomo@zeus.theochem.tuwien.ac.at</a><br>====<br><br></pre>
                          </blockquote>
                          <br>
                          <br>
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------------------------------

Date: Fri, 18 Oct 2002 22:50:19 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: OPtimize

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started optimize(v,c/a)and in ShowSTDOUT got
this message(PGFIO-F-217/Formatted
read/unit=20/attempt to read past end of file.
ERROR Status in Case_Vol_ -10). what dose it mean?or
What is its reason?
What should be done for eliminating it?
Thank you for the guide.
H-Salehi 
Dept of physics
Ferdowsi University
MASHHAD IRAN



=====
Hamdollah Salehi
Dept of Physics
Ferdowsi University
Mashhad IRAN
Post boxs 1436
Post code 91775
faxs

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Date: Tue, 22 Oct 2002 10:23:45 +0200
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: Problems with save/restore_lapw

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

I have a question regarding saving and restoring a calulation. Working 
on a case I saved it in a new directory (save_lapw  -f -d <dir>). Then I 
made some changes and then I wanted to restore my previous calculation 
(restore_lapw -f -d <dir>). The save and restore scripts seem to be 
workning properly (i.e. they do what they should do), but there is one 
thing I don't understand. After restore I immidiately calculated the 
band structure, but it had changed compared to the calculation I saved 
before. How is this possible? I also tried to run the SCF cycle to self 
consistency again and then calculated the band structure again, but it 
still didn't look like the one I saved before. It is not just the band 
structure that changes, also other quantities like Fermi energi and so 
on change as well.

So I wonder, is there anything I have missed to do? Why can't I get back 
to my previous calculation? Are there any more files I should delete?

Thanks for your replies!

Best regards,
Thomas Claesson



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------------------------------

End of wien-digest V2002 #39
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #40
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
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Precedence: bulk


wien-digest        Tuesday, October 29 2002        Volume 2002 : Number 040




----------------------------------------------------------------------

Date: Tue, 22 Oct 2002 15:40:55 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Problems with save/restore_lapw

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> I have a question regarding saving and restoring a calulation. Working
> on a case I saved it in a new directory (save_lapw  -f -d <dir>). Then I
> made some changes and then I wanted to restore my previous calculation
> (restore_lapw -f -d <dir>). The save and restore scripts seem to be
> workning properly (i.e. they do what they should do), but there is one
> thing I don't understand. After restore I immidiately calculated the
> band structure, but it had changed compared to the calculation I saved
> before. How is this possible? I also tried to run the SCF cycle to self
> consistency again and then calculated the band structure again, but it
> still didn't look like the one I saved before. It is not just the band
> structure that changes, also other quantities like Fermi energi and so
> on change as well.
The case.scf  is also saved and restored employing new scheme of these two
scripts. So there is no possibility to find from one case.scf file different
Fermi energies or other quantities. This shows how one can find what is
going wrong checking the saved case.scf file in the specified directory
right after saving and case.scf file in the work directory right after
restoring: These two case.scf files should be identical, as they are!
              Your,
               S. Jalali.

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------------------------------

Date: Tue, 22 Oct 2002 14:43:41 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Problems with save/restore_lapw

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I have a question regarding saving and restoring a calulation. Working
> on a case I saved it in a new directory (save_lapw  -f -d <dir>). Then I
> made some changes and then I wanted to restore my previous calculation
> (restore_lapw -f -d <dir>). The save and restore scripts seem to be
> workning properly (i.e. they do what they should do), but there is one
> thing I don't understand. After restore I immidiately calculated the
> band structure, but it had changed compared to the calculation I saved
> before. How is this possible?

This is clear! What you restored was the charge density (clmsum) (and all
input files + case.struct). So you must first run    x lapw0
to restore the old potential files (case.vsp, case.vns) and only
then can rerun a bandstructure (x lapw1,.....)

> I also tried to run the SCF cycle to self
> consistency again and then calculated the band structure again, but it
> still didn't look like the one I saved before. It is not just the band
> structure that changes, also other quantities like Fermi energi and so
> on change as well.

Then there are 3 choices:
a) You did not run to selfconsistency previously, therefore new iterations
change the potential,bands, ef,...

b) You made a mistake in saving/restoring ? (file permissions ?)

c) Are you sure you continued to run scf with proper inputs! You did not
change case.in1 for bandstructure,... ??? (Eventually you have even "saved"
those modified standard-inputs.

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 22 Oct 2002 21:18:03 -0400
From: xn22 <xn22@drexel.edu>
Subject: [WIEN]: Questions about H atom

====
xn22 <xn22@drexel.edu>
submitted the following contribution:
====

Hi, Dear WIEN users,

I had some problems for calculating H atom involved systems:

1. The 1s energy level is about -0.5 Ry with LDA for H atom from LSTART
and about 0 Ry with both GGA (PBE and PW91). This looks like very unphysics
since we knew the H 1s level should be around 1 Ry. I tried one molecular
program such as GAMESS for H atom. I got the H 1s level is close to 1 Ry.
Whether does the WIEN (or generally all LDA ab initio programs) work for
H atom?

2. I tried run wien with H atom including system. Two problems in the running
and results. The first one is that the R_MTxK_max is too small. About 
40APW/atom . I don't think the results are converged with respect to the APW 
since I tested
isolated H atom by supercell. It asked about 500 APW/H atom for converged
results. I tried to increase the R_MTxK_max, but there were lots of ghost 
bands. Could you let me know any parameter I can adjust so that I can increase
R_MTxK_max without ghost bands? The second problem I cannot find any H 
s-character charge in energy level in identify the H atom contribution for the
systems. Perhaps my SFC is totally wrong due to small R_MTxK_max or the wrong
initial charge density (since the H 1s level is wrong for atom).

In summary, my questions are:

1. Whether Wien can give right H atom 1s energy level?

2. How to overcome the too small R_MTxK_max in avoiding the ghost bands?

3. Whether we can still see some H s-character charge in certain energy levels
even most of the charge are in interstitial?

Please also cc to this email if you could answer my questions to WIEN 
mail-list
since I am not sure whether I already subscribe to this list. Thanks in 
Advance.

Best regards.

Xiliang Nie

Drexel University


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------------------------------

Date: Wed, 23 Oct 2002 10:08:21 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Questions about H atom

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> 1. The 1s energy level is about -0.5 Ry with LDA for H atom from LSTART
> and about 0 Ry with both GGA (PBE and PW91).
This cannot be true!!! Below you would see the energy of 1s level in the
scheme of GGA96 parametrization for the exchange-correalation, which is
indeed the total enery too for this H case:

       OCCUPANCY    ENERGY(RYD)         (R4)              (R2)
(R)               (R-1)             (R-3)

  1S      0.900    -5.5343654E-01     2.8859964E+01     3.2701173E+00
1.5496451E+00     9.8868262E-01
  1S      0.100    -2.9298928E-01     7.6764833E+01     5.1154057E+00
1.9089852E+00     8.3795718E-01

 TOTAL ENERGY (RYD):               -0.966505
One sees that 5.5343654E-01-2.9298928E-01=-0.966505Ry is close to what is
expected for the ground level of H, -1Ry.

    Your
    Saeid.

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------------------------------

Date: Wed, 23 Oct 2002 09:34:21 +0200
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: Questions about H atom

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

isn't -5,534 - 2,930 = -8,464?

kevin.


- ----- Original Message ----- 
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Wednesday, October 23, 2002 8:38 AM
Subject: Re: [WIEN]: Questions about H atom


> ====
> "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> submitted the following contribution:
> ====
> 
> > 1. The 1s energy level is about -0.5 Ry with LDA for H atom from LSTART
> > and about 0 Ry with both GGA (PBE and PW91).
> This cannot be true!!! Below you would see the energy of 1s level in the
> scheme of GGA96 parametrization for the exchange-correalation, which is
> indeed the total enery too for this H case:
> 
>        OCCUPANCY    ENERGY(RYD)         (R4)              (R2)
> (R)               (R-1)             (R-3)
> 
>   1S      0.900    -5.5343654E-01     2.8859964E+01     3.2701173E+00
> 1.5496451E+00     9.8868262E-01
>   1S      0.100    -2.9298928E-01     7.6764833E+01     5.1154057E+00
> 1.9089852E+00     8.3795718E-01
> 
>  TOTAL ENERGY (RYD):               -0.966505
> One sees that 5.5343654E-01-2.9298928E-01=-0.966505Ry is close to what is
> expected for the ground level of H, -1Ry.
> 
>     Your
>     Saeid.
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 
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------------------------------

Date: Wed, 23 Oct 2002 16:07:59 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Hi,

I get following lines in file .outputs

DETERMINATION OF POINTGROUP FOR ALL POSITIONS
2020
C         :  16 Atoms, Index   1 to  16
C         :  16 Atoms, Index  17 to  32
C         :  16 Atoms, Index  33 to  48
C         :  16 Atoms, Index  49 to  64
C         : 208 Atoms, Index  65 to 272
C         :  16 Atoms, Index 273 to 288
C         :  16 Atoms, Index 289 to 304
C         :  16 Atoms, Index 305 to 320
number of atoms: 320

 ATOM: -1
  no pointgroup found, isym = 0
lm:
 ==============================================

 ATOM: -2
  no pointgroup found, isym = 0
lm:
 ==============================================

 ATOM: -3
  no pointgroup found, isym = 0
lm:
 ==============================================

 ATOM: -4
  no pointgroup found, isym = 0
lm:
 ==============================================

 ATOM: -5
  no pointgroup found, isym = 0
lm:
 ==============================================

 ATOM: -6
  no pointgroup found, isym = 0
lm:
 ==============================================

 ATOM: -7
  no pointgroup found, isym = 0
lm:
 ==============================================

 ATOM: -8
  no pointgroup found, isym = 0
lm:
 ==============================================

Then, Is it something wrong in my structure file?

Thank you very much

Martin 

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------------------------------

Date: Wed, 23 Oct 2002 10:38:40 +0200
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: Question

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Maybe.  Why not send it, so someone may have a look at it?

kind regards,

Kevin Jorissen
University of Antwerp, Belgium


- ----- Original Message ----- 
From: "Ma Chi Chiu" <martin@yangtze.hku.hk>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Wednesday, October 23, 2002 10:07 AM
Subject: [WIEN]: Question


> ====
> Ma Chi Chiu <martin@yangtze.hku.hk>
> submitted the following contribution:
> ====
> 
> Hi,
> 
> I get following lines in file .outputs
> 
> DETERMINATION OF POINTGROUP FOR ALL POSITIONS
> 2020
> C         :  16 Atoms, Index   1 to  16
> C         :  16 Atoms, Index  17 to  32
> C         :  16 Atoms, Index  33 to  48
> C         :  16 Atoms, Index  49 to  64
> C         : 208 Atoms, Index  65 to 272
> C         :  16 Atoms, Index 273 to 288
> C         :  16 Atoms, Index 289 to 304
> C         :  16 Atoms, Index 305 to 320
> number of atoms: 320
> 
>  ATOM: -1
>   no pointgroup found, isym = 0
> lm:
>  ==============================================
> 
>  ATOM: -2
>   no pointgroup found, isym = 0
> lm:
>  ==============================================
> 
>  ATOM: -3
>   no pointgroup found, isym = 0
> lm:
>  ==============================================
> 
>  ATOM: -4
>   no pointgroup found, isym = 0
> lm:
>  ==============================================
> 
>  ATOM: -5
>   no pointgroup found, isym = 0
> lm:
>  ==============================================
> 
>  ATOM: -6
>   no pointgroup found, isym = 0
> lm:
>  ==============================================
> 
>  ATOM: -7
>   no pointgroup found, isym = 0
> lm:
>  ==============================================
> 
>  ATOM: -8
>   no pointgroup found, isym = 0
> lm:
>  ==============================================
> 
> Then, Is it something wrong in my structure file?
> 
> Thank you very much
> 
> Martin 
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
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> 
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------------------------------

Date: Wed, 23 Oct 2002 11:16:41 +0200 (MESZ)
From: "A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
Subject: Re: [WIEN]: Questions about H atom

====
"A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
submitted the following contribution:
====

Dear Xiliang,

hopefully you calculate your H atom in spin-polarized regime?

Recently there was already some discussion about H atom in a box, in
 wien-digest.2002-16
 wien-digest.2002-17
- - check whether this helps.

Good luck,

Andrei Postnikov

On Tue, 22 Oct 2002, xn22 wrote:

> ====
> xn22 <xn22@drexel.edu>
> submitted the following contribution:
> ====
>
> Hi, Dear WIEN users,
>
> I had some problems for calculating H atom involved systems:
>
> 1. The 1s energy level is about -0.5 Ry with LDA for H atom from LSTART
> and about 0 Ry with both GGA (PBE and PW91). This looks like very unphysics
> since we knew the H 1s level should be around 1 Ry. I tried one molecular
> program such as GAMESS for H atom. I got the H 1s level is close to 1 Ry.
> Whether does the WIEN (or generally all LDA ab initio programs) work for
> H atom?
>
> 2. I tried run wien with H atom including system. Two problems in the running
> and results. The first one is that the R_MTxK_max is too small. About
> 40APW/atom . I don't think the results are converged with respect to the APW
> since I tested
> isolated H atom by supercell. It asked about 500 APW/H atom for converged
> results. I tried to increase the R_MTxK_max, but there were lots of ghost
> bands. Could you let me know any parameter I can adjust so that I can increase
> R_MTxK_max without ghost bands? The second problem I cannot find any H
> s-character charge in energy level in identify the H atom contribution for the
> systems. Perhaps my SFC is totally wrong due to small R_MTxK_max or the wrong
> initial charge density (since the H 1s level is wrong for atom).
>
> In summary, my questions are:
>
> 1. Whether Wien can give right H atom 1s energy level?
>
> 2. How to overcome the too small R_MTxK_max in avoiding the ghost bands?
>
> 3. Whether we can still see some H s-character charge in certain energy levels
> even most of the charge are in interstitial?
>
> Please also cc to this email if you could answer my questions to WIEN
> mail-list
> since I am not sure whether I already subscribe to this list. Thanks in
> Advance.
>
> Best regards.
>
> Xiliang Nie
>
> Drexel University
>

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------------------------------

Date: Wed, 23 Oct 2002 12:51:55 +0200 (MEST)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Questions about H atom

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I had some problems for calculating H atom involved systems:
>
> 1. The 1s energy level is about -0.5 Ry with LDA for H atom from LSTART
> and about 0 Ry with both GGA (PBE and PW91). This looks like very unphysics
> since we knew the H 1s level should be around 1 Ry. I tried one molecular
> program such as GAMESS for H atom. I got the H 1s level is close to 1 Ry.
> Whether does the WIEN (or generally all LDA ab initio programs) work for
> H atom?
There was already quite some discussion about H in previous mails. Please
check the digest.
In GGA you cannot set an occupation of 1 and 0 for spin-up/dn
respectively, since the program does not know what to do with zero density.
In LDA you can do so. Nevertheless, you will never get an eigenvalue of -1 Ry.
This resembles the well known fact, that DFT-eigenvalues are not observable
exitation energies (but in principle just lagrange parameters) and that
DFT is a theory of the groundstate.

> 1. Whether Wien can give right H atom 1s energy level?

Wien gives (for LDA) the "correct" H 1s energy level (which is far from
experiment).

> 2. How to overcome the too small R_MTxK_max in avoiding the ghost bands?

I'm not sure what you are doing exactly. 1st, for pure H systems, don't do GGA.
Second, it is perfectly ok that the number of PW changes with the unitcell
size and is different for "bulk-H" or H in a supercell.

> 3. Whether we can still see some H s-character charge in certain energy levels
> even most of the charge are in interstitial?

Yes you should see some H s-character (not 1 electron, but only a fraction.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 23 Oct 2002 14:42:20 +0200
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: Delete case.broydX files?

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

In the usersguide, section 7.9 about Mixer, you can read the following:
"At the outset of a new calculation (for any changed computational 
parameter such as k-mesh, ma-trix size, lattice constant etc.), any 
existing case.broydX files must be deleted."
Here I just wonder etc. includes, i.e. in which cases other than those 
explicitly mentioned above, do I have to delete the case.broydX files?

Thanks for your replies!

Best regards,
Thomas Claesson

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------------------------------

Date: Wed, 23 Oct 2002 21:03:01 -0400
From: xn22 <xn22@drexel.edu>
Subject: RE: [WIEN]: Questions about H atom

====
xn22 <xn22@drexel.edu>
submitted the following contribution:
====

Dear Saeid and WIEN users,

Thanks for your replying. But I could not understand why you
combine two energy levels (I assumed they are spin up and spin down)
to form the energy level of 1s for H atom in your email. Actually
from the data you gave in your email. The lowest 1s level is about
0.5 Ry (spin up) that it is close to my calculation. My question
is that whether we could calculate another lowest 1s level that
is close to 1 Ry? By the way what's the reason you split 1 electron
into 0.9 for spin-up and 0.1 for spin-down in your case.inst file
for H atom? Also I am very strange you got those energy levels by
GGA96 ( I got about 0 Ry). Is this the reason you put some electron
in spin-down as Peter said the GGA cann't work for for 0 of spin-down 
charge?

By the way I know someone did ice calculations from digest. Could you
talk about your treatment for H2O molecular in your calculations if you
read my email. Actually I am interested to do some water molecular supercell
calculations. It is very much appreciated if anybody can send some
suggestions and comments. I have impression that somebody published
paper about water molecular on surface by ab initio but cann't
find it. Anybody can give info about this paper?

Best regards.

Xiliang Nie

Drexel University

>===== Original Message From Saeid Jalali <sjalali@cc.iut.ac.ir> =====
>====
>"Saeid Jalali" <sjalali@cc.iut.ac.ir>
>submitted the following contribution:
>====
>
>> 1. The 1s energy level is about -0.5 Ry with LDA for H atom from LSTART
>> and about 0 Ry with both GGA (PBE and PW91).
>This cannot be true!!! Below you would see the energy of 1s level in the
>scheme of GGA96 parametrization for the exchange-correalation, which is
>indeed the total enery too for this H case:
>
>       OCCUPANCY    ENERGY(RYD)         (R4)              (R2)
>(R)               (R-1)             (R-3)
>
>  1S      0.900    -5.5343654E-01     2.8859964E+01     3.2701173E+00
>1.5496451E+00     9.8868262E-01
>  1S      0.100    -2.9298928E-01     7.6764833E+01     5.1154057E+00
>1.9089852E+00     8.3795718E-01
>
> TOTAL ENERGY (RYD):               -0.966505
>One sees that 5.5343654E-01-2.9298928E-01=-0.966505Ry is close to what is
>expected for the ground level of H, -1Ry.
>
>    Your
>    Saeid.
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====


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------------------------------

Date: Wed, 23 Oct 2002 21:10:39 -0400
From: xn22 <xn22@drexel.edu>
Subject: RE: [WIEN]: Questions about H atom

====
xn22 <xn22@drexel.edu>
submitted the following contribution:
====

Dear Saeid and WIEN users,

Thanks for your replying. But I could not understand why you
combine two energy levels (I assumed they are spin up and spin down)
to form the energy level of 1s for H atom in your email. Actually
from the data you gave in your email. The lowest 1s level is about
0.5 Ry (spin up) that it is close to my calculation. My question
is that whether we could calculate another lowest 1s level that
is close to 1 Ry? By the way what's the reason you split 1 electron
into 0.9 for spin-up and 0.1 for spin-down in your case.inst file
for H atom? Also I am very strange you got those energy levels by
GGA96 ( I got about 0 Ry). Is this the reason you put some electron
in spin-down as Peter said the GGA cann't work for for 0 of spin-down 
charge?

By the way I know someone did ice calculations from digest. Could you
talk about your treatment for H2O molecular in your calculations if you
read my email. Actually I am interested to do some water molecular supercell
calculations. It is very much appreciated if anybody can send some
suggestions and comments. I have impression that somebody published
paper about water molecular on surface by ab initio but cann't
find it. Anybody can give info about this paper?

Best regards.

Xiliang Nie

Drexel University

>===== Original Message From Saeid Jalali <sjalali@cc.iut.ac.ir> =====
>====
>"Saeid Jalali" <sjalali@cc.iut.ac.ir>
>submitted the following contribution:
>====
>
>> 1. The 1s energy level is about -0.5 Ry with LDA for H atom from LSTART
>> and about 0 Ry with both GGA (PBE and PW91).
>This cannot be true!!! Below you would see the energy of 1s level in the
>scheme of GGA96 parametrization for the exchange-correalation, which is
>indeed the total enery too for this H case:
>
>       OCCUPANCY    ENERGY(RYD)         (R4)              (R2)
>(R)               (R-1)             (R-3)
>
>  1S      0.900    -5.5343654E-01     2.8859964E+01     3.2701173E+00
>1.5496451E+00     9.8868262E-01
>  1S      0.100    -2.9298928E-01     7.6764833E+01     5.1154057E+00
>1.9089852E+00     8.3795718E-01
>
> TOTAL ENERGY (RYD):               -0.966505
>One sees that 5.5343654E-01-2.9298928E-01=-0.966505Ry is close to what is
>expected for the ground level of H, -1Ry.
>
>    Your
>    Saeid.
>
>====
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Date: Wed, 23 Oct 2002 21:58:06 -0400
From: xn22 <xn22@drexel.edu>
Subject: RE: [WIEN]: Questions about H atom

====
xn22 <xn22@drexel.edu>
submitted the following contribution:
====

Dear Saeid and WIEN users,

Thanks for your replying. But I could not understand why you
combine two energy levels (I assumed they are spin up and spin down)
to form the energy level of 1s for H atom in your email. Actually
from the data you gave in your email. The lowest 1s level is about
0.5 Ry (spin up) that it is close to my calculation. My question
is that whether we could calculate another lowest 1s level that
is close to 1 Ry? By the way what's the reason you split 1 electron
into 0.9 for spin-up and 0.1 for spin-down in your case.inst file
for H atom? Also I am very strange you got those energy levels by
GGA96 ( I got about 0 Ry). Is this the reason you put some electron
in spin-down as Peter said the GGA cann't work for for 0 of spin-down 
charge?

By the way I know someone did ice calculations from digest. Could you
talk about your treatment for H2O molecular in your calculations if you
read my email. Actually I am interested to do some water molecular supercell
calculations. It is very much appreciated if anybody can send some
suggestions and comments. I have impression that somebody published
paper about water molecular on surface by ab initio but cann't
find it. Anybody can give info about this paper?

Best regards.

Xiliang Nie

Drexel University

>===== Original Message From Saeid Jalali <sjalali@cc.iut.ac.ir> =====
>====
>"Saeid Jalali" <sjalali@cc.iut.ac.ir>
>submitted the following contribution:
>====
>
>> 1. The 1s energy level is about -0.5 Ry with LDA for H atom from LSTART
>> and about 0 Ry with both GGA (PBE and PW91).
>This cannot be true!!! Below you would see the energy of 1s level in the
>scheme of GGA96 parametrization for the exchange-correalation, which is
>indeed the total enery too for this H case:
>
>       OCCUPANCY    ENERGY(RYD)         (R4)              (R2)
>(R)               (R-1)             (R-3)
>
>  1S      0.900    -5.5343654E-01     2.8859964E+01     3.2701173E+00
>1.5496451E+00     9.8868262E-01
>  1S      0.100    -2.9298928E-01     7.6764833E+01     5.1154057E+00
>1.9089852E+00     8.3795718E-01
>
> TOTAL ENERGY (RYD):               -0.966505
>One sees that 5.5343654E-01-2.9298928E-01=-0.966505Ry is close to what is
>expected for the ground level of H, -1Ry.
>
>    Your
>    Saeid.
>
>====
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>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
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Date: Wed, 23 Oct 2002 22:50:02 -0700 (PDT)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: Xdstart

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started Initializ cale for large unite cel(in
Pentium Four by  RAM 768M ) and got this message(X
dstart:Not enough memory). what dose it mean?or What
is its reason?
What should be done for eliminating it?
Thank you for the guide.
H-Salehi 
Dept of physics
Ferdowsi University
MASHHAD IRAN


=====
Hamdollah Salehi
Dept of Physics
Ferdowsi University
Mashhad IRAN
Post boxs 1436
Post code 91775
faxs

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Date: Thu, 24 Oct 2002 09:31:32 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Questions about H atom

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> By the way I know someone did ice calculations from digest. Could you
> talk about your treatment for H2O molecular in your calculations if you
> read my email. Actually I am interested to do some water molecular
supercell
> calculations. It is very much appreciated if anybody can send some
> suggestions and comments.

Ice in its Fcc phase with the space group of 227_Fd-3m is constructed with 2
molecules of H2O in each site. One would use the following structure
checking the lattice parameter surfacing literatures:
Title
F   LATTICE,NONEQUIV. ATOMS: 2227_Fd-3m
MODE OF CALC=RELA unit=bohr
 22.676280 22.676280 22.676280 90.000000 90.000000 90.000000
ATOM=  1: X=0.12500000 Y=0.12500000 Z=0.12500000
          MULT= 2          ISPLIT= 2
       1: X=0.87500000 Y=0.87500000 Z=0.87500000
O          NPT=  781  R0=0.00010000 RMT=    1.0000   Z:  8.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -2: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 4          ISPLIT= 4
      -2: X=0.00000000 Y=0.25000000 Z=0.25000000
      -2: X=0.25000000 Y=0.25000000 Z=0.00000000
      -2: X=0.25000000 Y=0.00000000 Z=0.25000000
H          NPT=  781  R0=0.00010000 RMT=    1.0000   Z:  1.0
LOCAL ROT MATRIX:    0.4082483-0.7071068 0.5773503
                     0.4082483 0.7071068 0.5773503
                    -0.8164966 0.0000000 0.5773503
  48      NUMBER OF SYMMETRY OPERATIONS


> Thanks for your replying. But I could not understand why you
> combine two energy levels (I assumed they are spin up and spin down)
> to form the energy level of 1s for H atom in your email.

Yes, you are right.



> Actually
> from the data you gave in your email. The lowest 1s level is about
> 0.5 Ry (spin up) that it is close to my calculation.

That's okay.

> My question
> is that whether we could calculate another lowest 1s level that
> is close to 1 Ry?

Yes, but we don't need it, as lstart is an atomic program (a modified
version of relativistic Dirack-Fick) to assess an initial case.clmsum for
going through SCF procedure in the bulk.

> By the way what's the reason you split 1 electron
> into 0.9 for spin-up and 0.1 for spin-down in your case.inst file
> for H atom?

There is a technical and not physical restriction to select 0 and 1
occupations for spin down and up in H atom. One also finds that there is
such a restriction for Yb atom to make a divalent configuration. There is a
direct relationship between relativistic aspect and spin. Spin inherently
introduces or defines itself once one writes Dirack equation, which is not
the case once one writes Schrödinger equation. In the later case we should
manually introduce or define spin from our physical knowledge.

> Also I am very strange you got those energy levels by
> GGA96 ( I got about 0 Ry).

Me too! You would send us your case.struct, case.inst, and case.outputst.

> Is this the reason you put some electron
> in spin-down as Peter said the GGA cann't work for for 0 of spin-down
> charge?
Please notice that I did not change case.inst: I have just used the default
case.inst. With 1 and 0 occupation numbers I have found:

TOTAL ENERGY (RYD):               -0.487945

which cannot be the ground level of H, and this is why Peter said that.


> isn't -5,534 - 2,930 = -8,464?

Yes, it is!!! With my roughly and fast choices of RMT and S.E, we have:

 TOTAL CHARGE FOR SPIN            1:                 0.9000000000000002
 TOTAL CHARGE FOR SPIN            1 INSIDE SPHERE:   0.6689781200590000
 TOTAL CHARGE FOR SPIN            2:                 0.1000000000000001
 TOTAL CHARGE FOR SPIN            2 INSIDE SPHERE:   6.1910993220382204E-002
So, there are 0.9-0.668=0.232 up-electrons and 0.1-6.191E-002=0.0381
dn-electrons in the  region. It appears that the energy
of -0.966505-(-0.8464)=-0.12Ry is a contribution of interstitial electrons
to tot-ENE. But it does not, as with a very  large choice of RMT (!!!), one
can confine almost all the electrons into the sphere. In this case we have:


         OCCUPANCY    ENERGY(RYD)         (R4)              (R2)
(R)               (R-1)             (R-3)



  1S      0.900    -5.5343655E-01     2.8859969E+01     3.2701173E+00
1.5496451E+00     9.8868263E-01
  1S      0.100    -2.9298928E-01     7.6766219E+01     5.1154126E+00
1.9089856E+00     8.3795713E-01



 TOTAL CHARGE FOR SPIN            1:                 0.9000000000000005
 TOTAL CHARGE FOR SPIN            1 INSIDE SPHERE:   0.8988648475727096
 TOTAL CHARGE FOR SPIN            2:                 9.9999999999999964E-002
 TOTAL CHARGE FOR SPIN            2 INSIDE SPHERE:   9.9137532098954502E-002

 TOTAL ENERGY (RYD):               -0.966505
     SUM OF EI:-5.2739182E-01     NUC:-1.9472202E+00     COUL:-7.5003038E-01
     V-XC SPIN 1:-6.8721928E-01     E-XC SPIN 1:-5.4051577E-01
     V-XC SPIN 2:-4.1960715E-02     E-XC SPIN 2:-2.9182609E-02

So the difference cannot be due to the interstitial-electrons. Indeed,
energy levels calculation exploiting lstart does not depend on RMT size:
lstart is not lapw method! So, what is the reason? I don't know!

        Your,

        Saeid.





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Date: Thu, 24 Oct 2002 08:17:28 +0200
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Xdstart

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Mr. Salehi,

it is very little information you give, so the answer will be a bit 
general...
It means that either your unit cell is big, or rkmax/gmax is, or your 
computer uses the memory for something else. Try adding some swap space, 
or decrease rkmax and gmax (for a start, the problem will then appear 
later).

Best regards,
Torsten Andersen.

hamid salehi wrote:

>====
>hamid salehi <salehihamid@yahoo.com>
>submitted the following contribution:
>====
>
>Dear wien users.
>Ihave started Initializ cale for large unite cel(in
>Pentium Four by  RAM 768M ) and got this message(X
>dstart:Not enough memory). what dose it mean?or What
>is its reason?
>What should be done for eliminating it?
>Thank you for the guide.
>H-Salehi 
>Dept of physics
>Ferdowsi University
>MASHHAD IRAN
>
>
>=====
>Hamdollah Salehi
>Dept of Physics
>Ferdowsi University
>Mashhad IRAN
>Post boxs 1436
>Post code 91775
>faxs
>
>__________________________________________________
>Do you Yahoo!?
>Y! Web Hosting - Let the expert host your web site
>http://webhosting.yahoo.com/
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>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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Date: Thu, 24 Oct 2002 09:16:57 +0200
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: Convergence problems

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

I am working on a case where I have big troubles with convergence. I 
want to add LDA+U with a U-value of 0.5 - 0.6 Ry and that is where I run 
into trouble. First I run the case without LDA+U to self-consistency and 
that works just fine. Then I
can make it converge with a U-value of 0.15 Ry. After that I try to 
slowly increase U in small steps, running to self-consistency for each 
new value. That works until I get just above 0.2 Ry, but for larger 
U-values I get oscillations and cannot reach self-consistency.


My case (NiO) has three atoms in the unit cell and so far I have been 
using 400 k-points the whole BZ (44 in IBZ) and R*K_max = 7.0. I have 
tried using PRATT mixing with a mixing parameter of just 0.01, still it 
doesn't converge. So I wonder, what can I do to improve convergency for 
larger U-values? Can a denser k-mesh make things better?

Any suggestions are welcome! Thanks for your replies!

Best regards,
Thomas Claesson

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Date: Thu, 24 Oct 2002 11:31:40 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Xdstart

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

Dear Hamid,
Would you send us your struct file? You will make me so happy if you call me
discussing your problem in more detail: +98-0311-391 2690.
        Your,
        Saeid.


> ====
> hamid salehi <salehihamid@yahoo.com>
> submitted the following contribution:
> ====


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Date: Fri, 25 Oct 2002 21:52:13 +0800
From: joshua xie <joshuaxie@etang.com>
Subject: [WIEN]: Fermi level

====
joshua xie <joshuaxie@etang.com>
submitted the following contribution:
====

Dear wien user£¬
    For impurity in semiconductor,such as N impurity which substutites C atom in some semicondcutor. To my knowledge,because the N has one more valence electron than C ,the fermi level should lie within the bottom of conduction band ,therefore make the semiconductor n-type. But After wien calculation, I find the fermi level lies at the bottom of conduction band, not within the conduction band, and also it is not consistent with the LMTO calculation from literatures.
    I do not know if it is a bug. Could someone explain it to me? or do I make a mistake?

Best regards! 				
Joshua xie                                   




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Date: Fri, 25 Oct 2002 19:26:03 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Fermi level

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>     For impurity in semiconductor,such as N impurity which substutites C
atom in some semicondcutor. To my knowledge,because the N has one more
valence electron than C ,the fermi level should lie within the bottom of
conduction band ,therefore make the semiconductor n-type. But After wien
calculation, I find the fermi level lies at the bottom of conduction band,
not within the conduction band, and also it is not consistent with the LMTO
calculation from literatures.
>     I do not know if it is a bug. Could someone explain it to me? or do I
make a mistake?

Integral of total density of state (tot-DOS) over an interval [E1, E2]
yields number of electrons distributed on that interval of energy provided
E2<=Fermi Energy=Ef. The condition is due to the fact that there is no
electron for E2>Ef. This means that one can write at zero temperature (T=0):

Ef=E_c-E0 or Ef=E_v+E0 provided that E0<=Eg, where E_c is the bottom of the
lowest empty conduction band(s), E_v is the top of the highest filled
valence band, and Eg is the gap between Ec and Ev (Eg=Ec-Ev).

In this case charge conservation law is hold for E_c-E0=<Ef<=Ev+E0. For T<>0
the story will be different, which is not the case in wien. Thus, one would
not complain about the right position of E_f in T<>0 employing T=0 theory.

        Your,

        Saeid.


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Date: Sun, 27 Oct 2002 9:48:48 +0800
From: caimengqiu@yahoo.com.cn
Subject: [WIEN]: help

====
caimengqiu@yahoo.com.cn
submitted the following contribution:
====

Dear P.Blaha and Wien user
  I have a problem when I generate a file of case.struct.The 
space_group is B1a1 by the experimental result.But there is not the same 
space_group.I want to know how to transform the B1a1 group to equal 
group.
Thank you very much


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Date: Sun, 27 Oct 2002 10:22:50 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: help

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> caimengqiu@yahoo.com.cn
> submitted the following contribution:
> ====
> 
>   I have a problem when I generate a file of case.struct.The 
> space_group is B1a1 by the experimental result.But there is not the same 
> space_group.I want to know how to transform the B1a1 group to equal 
> group.

This is very little information... At least you should include your 
case.struct. Most probably the structure you defined in case.struct isn't the 
structure you wanted to define. Look at your case.struct by xcrysden, or draw 
it on paper by the coordinates that are abundantly available in case.outputnn. 
Is this what you wanted it to be?

Stefaan
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Date: Sun, 27 Oct 2002 14:11:08 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: help

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0075_01C27DC2.B1F954B0
Content-Type: text/plain;
	charset="GB2312"
Content-Transfer-Encoding: quoted-printable

>   I have a problem when I generate a file of case.struct.The=20
> space_group is B1a1 by the experimental result.But there is not the =
same=20
> space_group.I want to know how to transform the B1a1 group to equal=20
> group.

Most likely the structure of your case is rutile, which is equal to the =
space group of P42/MNM and the number of 136. One can  specify the =
crystallographic space groups using either the space group numbers from =
the international tables or the character strings derived from the =
Hermann Mauguin Symbols. For example  B1A1, ICM2, PMAM, P21CNS, P42/MNM =
are equal. So you would choose this #136 for you case, and fill the =
atomic positions getting help from struct generator of wien, and then =
try to plot your case to find out if you are in a right direction.
        Your,
        Saeid.

- ------=_NextPart_000_0075_01C27DC2.B1F954B0
Content-Type: text/html;
	charset="GB2312"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; charset=3Dgb2312">
<META content=3D"MSHTML 6.00.2600.0" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY>
<DIV><FONT face=3DArial><FONT size=3D2>&gt; &nbsp; I have a problem when =
I generate=20
a file of case.struct.The <BR>&gt; space_group is B1a1 by the =
experimental=20
result.But there is not the same <BR>&gt; space_group.I want to know how =
to=20
transform the B1a1 group to equal <BR>&gt;=20
group.<BR><!--StartFragment --></FONT></FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Most likely the structure of your case =
is rutile,=20
which is equal to the space group of&nbsp;P42/MNM&nbsp;and the number of =
136.=20
One can&nbsp; specify the crystallographic space groups&nbsp;using =
either the=20
space group numbers from the&nbsp;international tables&nbsp;or the =
character=20
strings derived from the Hermann Mauguin Symbols. For =
example&nbsp;<!--StartFragment --><FONT size=3D3> =
</FONT>B1A1,&nbsp;ICM2, PMAM,=20
P21CNS, P42/MNM are equal. So you would choose this #136 for you case, =
and fill=20
the atomic positions getting help from struct generator of wien, and =
then try to=20
plot your case to find out if you are in a right direction.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;=20
Your,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;=20
Saeid.</FONT></DIV></BODY></HTML>

- ------=_NextPart_000_0075_01C27DC2.B1F954B0--

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Date: Mon, 28 Oct 2002 22:00:06 +0800 (CST)
From: =?gb2312?q?mengqiu=20cai?= <caimengqiu@yahoo.com.cn>
Subject: [WIEN]: help

====
=?gb2312?q?mengqiu=20cai?= <caimengqiu@yahoo.com.cn>
submitted the following contribution:
====

Dear Sir:
Thank you much for your help .Now I did not resolve my
problem.I provided the detail information.I am meeting
with a problem when I generate a file of case.struct
of the crystal of Bi3Ti4O12 with the parent struct
that consists of perovskite-like An-1BnO3n+1
(n=3)slabs regularly interleaved with Bi2O2
with the interface wien2k_web.I want to obtain the
equivalent atom coordinates of the characteristic atom
by the crystal space group.The space group of the
crystal Bi3Ti4O12 is B1a1 by the experimental
refercnces.But there is not the same space group in
the wien2k code.So I will not get the file of
case.struct. I want to know how to transform the B1a1
group to equal group and how much is the transformed
atom coordinates.On the other hand,The crystal is
monoclinic struct and with small angle change in
contrast to the orthogonal 
struct ,Whether or not I treat the crystal as
rthogonal subscribe wien  crystal with the crystal
axial angle
¨»=90  &szlig;=90 y =90.

Thank you very much

I am looking forward to hearing from you.

  
Sinecerely yours!

Enclosures: The experimental datas.
space group : B1a1
a=5.450 , b=5.4059 ,c=32.832 &Aring;
&szlig;=90.00   

Bi(1)   0.0030   0.5023   0.5673
Bi(1)'  0.0013   0.4977   0.4336
Bi(2)  -0.0021   0.4793   0.7113
Bi(2)'  0.0021   0.5185   0.2887
Ti(1)   0.0446  -0.0013   0.5007
Ti(2)   0.0520   0.0004   0.6289
Ti(2)'  0.0499   0.0002   0.3717
O(1)    0.2990   0.2760   0.5102
O(1)'   0.3548  -0.2179   0.4942
O(2)    0.2704   0.2442   0.2495
O(2)'   0.2736   0.7571   0.7489
O(3)    0.0913  -0.0705   0.5605
O(3)'   0.0918   0.0587   0.4424
O(4)    0.0552   0.0584   0.6825
O(4)'   0.0568  -0.0441   0.3195
O(5)    0.2904   0.2800   0.6121
O(5)'   0.2962  -0.2659   0.3892
O(6)    0.3677  -0.1959   0.6244
O(6)'   0.3496   0.2164   0.3773

Case.struct without the the equivalent atom
coordinates of the characteristic atom subscribe wien 
by the crystal space group.Because the crystal is
monoclinic struct and with small angle change in
contrast to the  orthogonal struct ,I treat the
crystal as orthogonal crystal with the crystal axial
angle  
¨»=90  &szlig;=90 y =90.



bto
P   LATTICE,NONEQUIV. 

ATOMS:10                              
MODE OF CALC=RELA
10.299011 10.215675 62.043513 90.000000 90.000000
90.000000
Atom= -1: X=0.00300000 Y=0.50230000 subscribe wien
Z=0.56730000
MULT= 2          ISPLIT= 8
Atom= -1: X=0.00130000 Y=0.49770000 Z=0.43360000
Bi         NPT=  781  R0=0.00000500 RMT=    2.0000  
Z: 81.0
1.0000000 0.0000000 0.0000000
0.0000000 1.0000000 0.0000000
0.0000000 0.0000000 1.0000000
Atom= -2: X=0.99790000 Y=0.47930000 Z=0.71130000
MULT= 2          ISPLIT= 8
Atom= -2: X=0.21000000 Y=0.51850000 Z=0.28870000
Bi      NPT=781  R0=0.00000500 RMT=    1.0000   Z:
83.0
1.0000000 0.0000000 0.0000000
0.0000000 1.0000000 0.0000000
0.0000000 0.0000000 1.0000000
Atom= -3: X=0.04360000 Y=0.99870000 Z=0.50070000
MULT= 1          ISPLIT= 8
Tl    NPT=  781  R0=0.00000500 RMT=    1.8000   Z:
81.0
1.0000000 0.0000000 0.0000000
0.0000000 1.0000000 0.0000000
0.0000000 0.0000000 1.0000000
Atom= -4: X=0.05200000 Y=0.99960000 Z=0.62890000
MULT= 2          ISPLIT= 8
Atom= -4: X=0.04990000 Y=0.00020000 Z=0.37170000
Tl  NPT=  781  R0=0.00000500 RMT=    1.8000   Z: 81.0
1.0000000 0.0000000 0.0000000
0.0000000 1.0000000 0.0000000
0.0000000 0.0000000 1.0000000
Atom= -5: X=0.29900000 Y=0.27600000 Z=0.51020000
MULT= 2          ISPLIT= 8
Atom= -5: X=0.35480000 Y=0.78210000 Z=0.49420000
O    NPT=  781  R0=0.00010000 RMT=    1.6000   Z:  8.0
1.0000000 0.0000000 0.0000000
0.0000000 1.0000000 0.0000000
0.0000000 0.0000000 1.0000000
Atom= -6: X=0.27040000 Y=0.24420000 Z=0.24950000
MULT= 2          ISPLIT= 8
Atom= -6: X=0.27360000 Y=0.75710000 Z=0.74890000
O    NPT=  781  R0=0.00010000 RMT=    1.6000   Z:  8.0
1.0000000 0.0000000 0.0000000
0.0000000 1.0000000 0.0000000
0.0000000 0.0000000 1.0000000
Atom= -7: X=0.09130000 Y=0.92950000 Z=0.56050000
MULT= 2          ISPLIT= 8
Atom= -7: X=0.09180000 Y=0.05870000 Z=0.44240000
O     NPT=  781  R0=0.00010000 RMT=    1.6000   Z: 
8.0
1.0000000 0.0000000 0.0000000
0.0000000 1.0000000 0.0000000
0.0000000 0.0000000 1.0000000
Atom= -8: X=0.05520000 Y=0.05840000 Z=0.68250000
MULT= 2          ISPLIT= 8
Atom= -8: X=0.56800000 Y=0.95590000 Z=0.31950000
O     NPT=  781  R0=0.00010000 RMT=    1.6000   Z: 
8.0
1.0000000 0.0000000 0.0000000
0.0000000 1.0000000 0.0000000
0.0000000 0.0000000 1.0000000
Atom= -9: X=0.29040000 Y=0.28000000 Z=0.61210000
       MULT= 2          ISPLIT= 8
Atom= -9: X=0.29620000 Y=0.73410000 Z=0.38920000
O     NPT=  781  R0=0.00010000 RMT=    1.6000   Z: 
8.0
1.0000000 0.0000000 0.0000000
0.0000000 1.0000000 0.0000000
0.0000000 0.0000000 1.0000000
Atom=-10: X=0.36770000 Y=0.80410000 Z=0.62440000
MULT= 2          ISPLIT= 8
Atom=-10: X=0.34960000 Y=0.21640000 Z=0.37730000
O     NPT=  781  R0=0.00010000 RMT=    1.6000   Z: 
8.0
1.0000000 0.0000000 0.0000000
0.0000000 1.0000000 0.0000000
0.0000000 0.0000000 1.0000000
0 SYMMETRY OPERATIONS:

end







   





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------------------------------

Date: Mon, 28 Oct 2002 06:50:43 -0800 (PST)
From: Wenqing ZHANG <dft_flapw@yahoo.com>
Subject: [WIEN]: Pentinum IV cluster workstation

====
Wenqing ZHANG <dft_flapw@yahoo.com>
submitted the following contribution:
====


Deal All,

I noticed that many people began to using cluster
workstation using Pentinum IV CPU recently. May anyone
answer me the following questions? --

1. How is the speed of computation (per CPU) in
comparion with HP PA-8700 (CPU 440MHZ) or SUN ultra-80
(CPU 550MHZ)?

2. Where can I find the product for sale?

3. What is the price if I want to have a Pentinum IV
workstation with 16 CPUs?

Thanks very much for help.

Yours -- Wenqing

=====
Wenqing ZHANG
1970 Crystal Lake Dr. Apt#E79
Shelby Twp., MI 48316
Tel: (810)254-9931(h), (810)323-1551(o)
Fax: (810)323-9898

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------------------------------

Date: Mon, 28 Oct 2002 09:59:02 -0800 (PST)
From: Claudio Lee <claudio_lee1@yahoo.com>
Subject: [WIEN]: OP - Obital polarization

====
Claudio Lee <claudio_lee1@yahoo.com>
submitted the following contribution:
====

Hi all,
Has onyone successfuly calculated the obital
polarization (OP) involved in the spin polarized
calculation. Please help me.
As a test, my system is Fe bcc. First I calculated
this system by running "runsp_lapw -so" (yet I have
already involved spin-obit coupling), the final result
is ok. 
After this first step has been done, what I now want
to do is to get orbital polarization involved in my
calculation. I have created  these two files *.indm
and *. inorb,
they are:
 *.indm:
===
- -9.     Emin cutoff energy
 1      number of atoms 
 1 1 2  index of 1st atom, 
 0 0    r-index, (l,s)0index
===
*.inorb:
 2 1 0          nmod, natorb, ipr, amix
BROYD 0.3       Broyden mixing used with mix...
1 1 2           iatom, nlorb, lorb
0               nmodop
1               Ncalc
0. 0. 1.        direction of M in terms of lattice ..
===
After all I used "runsp_lapw -so -orb" to run the
program. When the program has stopped I got no errors
from *. error files, and in the *.err file it looks
like:
===
hup: Command not found.
STOP  LAPW0 END
STOP  LAPW1 END
STOP  LAPW1 END
STOP LAPWSO END
STOP  LAPW2 END
STOP  LAPW2 END
===
I have tried to find if there are any properly answers
 about this case so far, unfornately, there is no that
answer!
If anyone knows the answer could you please help me.

Thank you in advance.

Claudio.  







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------------------------------

Date: Mon, 28 Oct 2002 21:16:18 +0100 (MET)
From: Pavel Novak <novakp@fzu.cz>
Subject: Re: [WIEN]: OP - Obital polarization

====
Pavel Novak <novakp@fzu.cz>
submitted the following contribution:
====

Dear Claudio,

try to copy *.indm to *.indmc.
Regards
Pavel Novak

On Mon, 28 Oct 2002, Claudio Lee wrote:

> ====
> Claudio Lee <claudio_lee1@yahoo.com>
> submitted the following contribution:
> ====
>
> Hi all,
> Has onyone successfuly calculated the obital
> polarization (OP) involved in the spin polarized
> calculation. Please help me.
> As a test, my system is Fe bcc. First I calculated
> this system by running "runsp_lapw -so" (yet I have
> already involved spin-obit coupling), the final result
> is ok.
> After this first step has been done, what I now want
> to do is to get orbital polarization involved in my
> calculation. I have created  these two files *.indm
> and *. inorb,
> they are:
>  *.indm:
> ===
> -9.     Emin cutoff energy
>  1      number of atoms
>  1 1 2  index of 1st atom,
>  0 0    r-index, (l,s)0index
> ===
> *.inorb:
>  2 1 0          nmod, natorb, ipr, amix
> BROYD 0.3       Broyden mixing used with mix...
> 1 1 2           iatom, nlorb, lorb
> 0               nmodop
> 1               Ncalc
> 0. 0. 1.        direction of M in terms of lattice ..
> ===
> After all I used "runsp_lapw -so -orb" to run the
> program. When the program has stopped I got no errors
> from *. error files, and in the *.err file it looks
> like:
> ===
> hup: Command not found.
> STOP  LAPW0 END
> STOP  LAPW1 END
> STOP  LAPW1 END
> STOP LAPWSO END
> STOP  LAPW2 END
> STOP  LAPW2 END
> ===
> I have tried to find if there are any properly answers
>  about this case so far, unfornately, there is no that
> answer!
> If anyone knows the answer could you please help me.
>
> Thank you in advance.
>
> Claudio.
>
>
>
>
>
>
>
> __________________________________________________
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> http://webhosting.yahoo.com/
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>
>
>



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------------------------------

Date: Mon, 28 Oct 2002 14:10:13 -0800 (PST)
From: yanming Ma <ymma66@yahoo.com>
Subject: [WIEN]: generate k mesh using Xcrysden

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-2049783500-1035843013=:90000
Content-Type: text/plain; charset=us-ascii


Dear wien2k user,

I try to use Xcrysden to generate K-mesh along high symmetry direction. My case structure is Cmca symmetry. After I run the Xcrysden, I choose Conventional BZ, other than primitive BZ because my input atomic positions are from conventional settings of international Crystalgraphic table. Then I select 7 special k points, the total k points along whole path is chosen as 60.  The default value for ISS shringking factor is 2. Minium and Maxium energy are  -1.0 Ry and 1.5 Ry, respectively.  However there are only some zero values generated, the error messages in the generated case.klist file is as following.

ERROR: IDV*NK to big! Decrease number of k points.

I try to decrease K points, but it is useless. 

I try to use primitive BZ. It works. But in my Cmca Case, I can not use primitive BZ. 

Can someone help me to solve this problem? I will highly appreciate your help.

Yanming Ma

 


Yanming Ma Ph.D
Steacie Institute for Molecular Sciences,
National Research Councils of Canada,
Ottawa, Ontario
K1A 0R6
Canada


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- --0-2049783500-1035843013=:90000
Content-Type: text/html; charset=us-ascii

<P>Dear wien2k user,</P>
<P>I try to use Xcrysden to generate K-mesh along high symmetry direction. My case structure is Cmca symmetry. After I run the Xcrysden, I choose Conventional BZ, other than primitive BZ because my input atomic positions are from conventional settings of international Crystalgraphic table. Then I select 7 special k points, the total k points along whole path is chosen as 60.&nbsp; The default value for ISS shringking factor is 2. Minium and Maxium energy&nbsp;are &nbsp;-1.0 Ry and 1.5 Ry, respectively.&nbsp; However there&nbsp;are only some zero values generated,&nbsp;the error messages in the&nbsp;generated case.klist file is as following.</P>
<P>ERROR:&nbsp;IDV*NK to big! Decrease number of k points.</P>
<P>I try to decrease K points, but it is useless. </P>
<P>I try to use primitive BZ. It works. But in my Cmca Case, I&nbsp;can not use primitive BZ. </P>
<P>Can someone help me to solve this problem? I will highly appreciate your help.</P>
<P>Yanming Ma</P>
<P>&nbsp;</P><BR><BR>Yanming Ma Ph.D<br>Steacie Institute for Molecular Sciences,<br>National Research Councils of Canada,<br>Ottawa, Ontario<br>K1A 0R6<br>Canada<p><br><hr size=1>Do you Yahoo!?<br>
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------------------------------

Date: Tue, 29 Oct 2002 14:16:13 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question about symmetry operator

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- --143914132-1867631754-1035872173=:9012
Content-Type: TEXT/PLAIN; charset=US-ASCII

Dear all,

I would like to consult about the symmetry found by wien. I get a .outputs file with lines like :
 ATOM: -1
  no pointgroup found, isym = 0
lm:
 ==============================================
 
 ATOM: -2
  no pointgroup found, isym = 0
lm:
 ==============================================
 
 ATOM: -3
........

What is the problem?

Thank you very much

Martin 

PS .outputs file is attached with this mail

- --143914132-1867631754-1035872173=:9012
Content-Type: TEXT/PLAIN; charset=US-ASCII; name="case.outputs"
Content-Transfer-Encoding: BASE64
Content-ID: <Pine.LNX.4.44.0210291416130.9012@yangtze.hku.hk>
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------------------------------

Date: Tue, 29 Oct 2002 09:18:53 +0100
From: "koitzsch" <Christian.Koitzsch@unifr.ch>
Subject: Re: [WIEN]: generate k mesh using Xcrysden

====
"koitzsch" <Christian.Koitzsch@unifr.ch>
submitted the following contribution:
====

This is a multi-part message in MIME format.

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try to calculate the bandstructure in two steps, first path connecting =
three special k-points and second path over the remaining four - but I =
have to admit I never bothered to figure out, what the error message =
really means, I just noticed that if you have a lot of special k-points =
with not so many points in between, it does not work.

Best Regards=20

Christian Koitzsch

Universite de Fribourg
Departement de Physique
Groupe FK
CH-1700 Fribourg
Suisse

  ----- Original Message -----=20
  From: yanming Ma=20
  To: wien@zeus.theochem.tuwien.ac.at=20
  Sent: Monday, October 28, 2002 11:10 PM
  Subject: [WIEN]: generate k mesh using Xcrysden


  Dear wien2k user,

  I try to use Xcrysden to generate K-mesh along high symmetry =
direction. My case structure is Cmca symmetry. After I run the Xcrysden, =
I choose Conventional BZ, other than primitive BZ because my input =
atomic positions are from conventional settings of international =
Crystalgraphic table. Then I select 7 special k points, the total k =
points along whole path is chosen as 60.  The default value for ISS =
shringking factor is 2. Minium and Maxium energy are  -1.0 Ry and 1.5 =
Ry, respectively.  However there are only some zero values generated, =
the error messages in the generated case.klist file is as following.

  ERROR: IDV*NK to big! Decrease number of k points.

  I try to decrease K points, but it is useless.=20

  I try to use primitive BZ. It works. But in my Cmca Case, I can not =
use primitive BZ.=20

  Can someone help me to solve this problem? I will highly appreciate =
your help.

  Yanming Ma





  Yanming Ma Ph.D
  Steacie Institute for Molecular Sciences,
  National Research Councils of Canada,
  Ottawa, Ontario
  K1A 0R6
  Canada




- -------------------------------------------------------------------------=
- -----
  Do you Yahoo!?
  Y! Web Hosting - Let the expert host your web site

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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
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<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT face=3DArial size=3D2>try to calculate the bandstructure in =
two steps,=20
first path&nbsp;connecting three special&nbsp;k-points and second path =
over the=20
remaining four - but I have to admit I never bothered to figure out, =
what the=20
error message really means, I just noticed that if you have a lot of =
special=20
k-points with not so many points in between, it does not =
work.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Best Regards </FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Christian Koitzsch</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Universite de Fribourg</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Departement de Physique</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Groupe FK</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>CH-1700 Fribourg</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Suisse</FONT></DIV>
<DIV>&nbsp;</DIV>
<BLOCKQUOTE=20
style=3D"PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; =
BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
  <DIV style=3D"FONT: 10pt arial">----- Original Message ----- </DIV>
  <DIV=20
  style=3D"BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: =
black"><B>From:</B>=20
  <A title=3Dymma66@yahoo.com href=3D"mailto:ymma66@yahoo.com">yanming =
Ma</A> </DIV>
  <DIV style=3D"FONT: 10pt arial"><B>To:</B> <A=20
  title=3Dwien@zeus.theochem.tuwien.ac.at=20
  =
href=3D"mailto:wien@zeus.theochem.tuwien.ac.at">wien@zeus.theochem.tuwien=
.ac.at</A>=20
  </DIV>
  <DIV style=3D"FONT: 10pt arial"><B>Sent:</B> Monday, October 28, 2002 =
11:10=20
  PM</DIV>
  <DIV style=3D"FONT: 10pt arial"><B>Subject:</B> [WIEN]: generate k =
mesh using=20
  Xcrysden</DIV>
  <DIV><BR></DIV>
  <P>Dear wien2k user,</P>
  <P>I try to use Xcrysden to generate K-mesh along high symmetry =
direction. My=20
  case structure is Cmca symmetry. After I run the Xcrysden, I choose=20
  Conventional BZ, other than primitive BZ because my input atomic =
positions are=20
  from conventional settings of international Crystalgraphic table. Then =
I=20
  select 7 special k points, the total k points along whole path is =
chosen as=20
  60.&nbsp; The default value for ISS shringking factor is 2. Minium and =
Maxium=20
  energy&nbsp;are &nbsp;-1.0 Ry and 1.5 Ry, respectively.&nbsp; However=20
  there&nbsp;are only some zero values generated,&nbsp;the error =
messages in=20
  the&nbsp;generated case.klist file is as following.</P>
  <P>ERROR:&nbsp;IDV*NK to big! Decrease number of k points.</P>
  <P>I try to decrease K points, but it is useless. </P>
  <P>I try to use primitive BZ. It works. But in my Cmca Case, =
I&nbsp;can not=20
  use primitive BZ. </P>
  <P>Can someone help me to solve this problem? I will highly appreciate =
your=20
  help.</P>
  <P>Yanming Ma</P>
  <P>&nbsp;</P><BR><BR>Yanming Ma Ph.D<BR>Steacie Institute for =
Molecular=20
  Sciences,<BR>National Research Councils of Canada,<BR>Ottawa, =
Ontario<BR>K1A=20
  0R6<BR>Canada
  <P><BR>
  <HR SIZE=3D1>
  Do you Yahoo!?<BR><A href=3D"http://webhosting.yahoo.com/ ">Y! Web =
Hosting</A> -=20
  Let the expert host your web site</BLOCKQUOTE></BODY></HTML>

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------------------------------

Date: Tue, 29 Oct 2002 10:09:14 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: help

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

I'm not a crystallographer, but I think B1A1 is actually the same as
P42/MNM, which is, however, tetragonal and not monoclinic.
Check this structure (using the original paper) with a good crystallographer.

Regards

> Dear Sir:
> Thank you much for your help .Now I did not resolve my
> problem.I provided the detail information.I am meeting
> with a problem when I generate a file of case.struct
> of the crystal of Bi3Ti4O12 with the parent struct
> that consists of perovskite-like An-1BnO3n+1
> (n=3)slabs regularly interleaved with Bi2O2
> with the interface wien2k_web.I want to obtain the
> equivalent atom coordinates of the characteristic atom
> by the crystal space group.The space group of the
> crystal Bi3Ti4O12 is B1a1 by the experimental
> refercnces.But there is not the same space group in
> the wien2k code.So I will not get the file of
> case.struct. I want to know how to transform the B1a1
> group to equal group and how much is the transformed
> atom coordinates.On the other hand,The crystal is
> monoclinic struct and with small angle change in
> contrast to the orthogonal
> struct ,Whether or not I treat the crystal as
> rthogonal subscribe wien  crystal with the crystal
> axial angle
> ¨»=90  &szlig;=90 y =90.
>
> Thank you very much
>
> I am looking forward to hearing from you.
>
>
> Sinecerely yours!
>
> Enclosures: The experimental datas.
> space group : B1a1
> a=5.450 , b=5.4059 ,c=32.832 &Aring;
> &szlig;=90.00
>
> Bi(1)   0.0030   0.5023   0.5673
> Bi(1)'  0.0013   0.4977   0.4336
> Bi(2)  -0.0021   0.4793   0.7113
> Bi(2)'  0.0021   0.5185   0.2887
> Ti(1)   0.0446  -0.0013   0.5007
> Ti(2)   0.0520   0.0004   0.6289
> Ti(2)'  0.0499   0.0002   0.3717
> O(1)    0.2990   0.2760   0.5102
> O(1)'   0.3548  -0.2179   0.4942
> O(2)    0.2704   0.2442   0.2495
> O(2)'   0.2736   0.7571   0.7489
> O(3)    0.0913  -0.0705   0.5605
> O(3)'   0.0918   0.0587   0.4424
> O(4)    0.0552   0.0584   0.6825
> O(4)'   0.0568  -0.0441   0.3195
> O(5)    0.2904   0.2800   0.6121
> O(5)'   0.2962  -0.2659   0.3892
> O(6)    0.3677  -0.1959   0.6244
> O(6)'   0.3496   0.2164   0.3773
>
> Case.struct without the the equivalent atom
> coordinates of the characteristic atom subscribe wien
> by the crystal space group.Because the crystal is
> monoclinic struct and with small angle change in
> contrast to the  orthogonal struct ,I treat the
> crystal as orthogonal crystal with the crystal axial
> angle
> ¨»=90  &szlig;=90 y =90.
>
>
>
> bto
> P   LATTICE,NONEQUIV.
>
> ATOMS:10
> MODE OF CALC=RELA
> 10.299011 10.215675 62.043513 90.000000 90.000000
> 90.000000
> Atom= -1: X=0.00300000 Y=0.50230000 subscribe wien
> Z=0.56730000
> MULT= 2          ISPLIT= 8
> Atom= -1: X=0.00130000 Y=0.49770000 Z=0.43360000
> Bi         NPT=  781  R0=0.00000500 RMT=    2.0000
> Z: 81.0
> 1.0000000 0.0000000 0.0000000
> 0.0000000 1.0000000 0.0000000
> 0.0000000 0.0000000 1.0000000
> Atom= -2: X=0.99790000 Y=0.47930000 Z=0.71130000
> MULT= 2          ISPLIT= 8
> Atom= -2: X=0.21000000 Y=0.51850000 Z=0.28870000
> Bi      NPT=781  R0=0.00000500 RMT=    1.0000   Z:
> 83.0
> 1.0000000 0.0000000 0.0000000
> 0.0000000 1.0000000 0.0000000
> 0.0000000 0.0000000 1.0000000
> Atom= -3: X=0.04360000 Y=0.99870000 Z=0.50070000
> MULT= 1          ISPLIT= 8
> Tl    NPT=  781  R0=0.00000500 RMT=    1.8000   Z:
> 81.0
> 1.0000000 0.0000000 0.0000000
> 0.0000000 1.0000000 0.0000000
> 0.0000000 0.0000000 1.0000000
> Atom= -4: X=0.05200000 Y=0.99960000 Z=0.62890000
> MULT= 2          ISPLIT= 8
> Atom= -4: X=0.04990000 Y=0.00020000 Z=0.37170000
> Tl  NPT=  781  R0=0.00000500 RMT=    1.8000   Z: 81.0
> 1.0000000 0.0000000 0.0000000
> 0.0000000 1.0000000 0.0000000
> 0.0000000 0.0000000 1.0000000
> Atom= -5: X=0.29900000 Y=0.27600000 Z=0.51020000
> MULT= 2          ISPLIT= 8
> Atom= -5: X=0.35480000 Y=0.78210000 Z=0.49420000
> O    NPT=  781  R0=0.00010000 RMT=    1.6000   Z:  8.0
> 1.0000000 0.0000000 0.0000000
> 0.0000000 1.0000000 0.0000000
> 0.0000000 0.0000000 1.0000000
> Atom= -6: X=0.27040000 Y=0.24420000 Z=0.24950000
> MULT= 2          ISPLIT= 8
> Atom= -6: X=0.27360000 Y=0.75710000 Z=0.74890000
> O    NPT=  781  R0=0.00010000 RMT=    1.6000   Z:  8.0
> 1.0000000 0.0000000 0.0000000
> 0.0000000 1.0000000 0.0000000
> 0.0000000 0.0000000 1.0000000
> Atom= -7: X=0.09130000 Y=0.92950000 Z=0.56050000
> MULT= 2          ISPLIT= 8
> Atom= -7: X=0.09180000 Y=0.05870000 Z=0.44240000
> O     NPT=  781  R0=0.00010000 RMT=    1.6000   Z:
> 8.0
> 1.0000000 0.0000000 0.0000000
> 0.0000000 1.0000000 0.0000000
> 0.0000000 0.0000000 1.0000000
> Atom= -8: X=0.05520000 Y=0.05840000 Z=0.68250000
> MULT= 2          ISPLIT= 8
> Atom= -8: X=0.56800000 Y=0.95590000 Z=0.31950000
> O     NPT=  781  R0=0.00010000 RMT=    1.6000   Z:
> 8.0
> 1.0000000 0.0000000 0.0000000
> 0.0000000 1.0000000 0.0000000
> 0.0000000 0.0000000 1.0000000
> Atom= -9: X=0.29040000 Y=0.28000000 Z=0.61210000
>        MULT= 2          ISPLIT= 8
> Atom= -9: X=0.29620000 Y=0.73410000 Z=0.38920000
> O     NPT=  781  R0=0.00010000 RMT=    1.6000   Z:
> 8.0
> 1.0000000 0.0000000 0.0000000
> 0.0000000 1.0000000 0.0000000
> 0.0000000 0.0000000 1.0000000
> Atom=-10: X=0.36770000 Y=0.80410000 Z=0.62440000
> MULT= 2          ISPLIT= 8
> Atom=-10: X=0.34960000 Y=0.21640000 Z=0.37730000
> O     NPT=  781  R0=0.00010000 RMT=    1.6000   Z:
> 8.0
> 1.0000000 0.0000000 0.0000000
> 0.0000000 1.0000000 0.0000000
> 0.0000000 0.0000000 1.0000000
> 0 SYMMETRY OPERATIONS:
>
> end
>
>
>
>
>
>
>
>
>
>
>
>
>
> _________________________________________________________
> Do You Yahoo!?
> "ÊÇIT¾«Ó¢Âð£¿Ð¡ÊÔÅ£µ¶»ñÊ±ÉÐ´ó½±£¡"
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> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

====
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------------------------------

Date: Tue, 29 Oct 2002 10:13:05 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Pentinum IV cluster workstation

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I noticed that many people began to using cluster
> workstation using Pentinum IV CPU recently. May anyone
> answer me the following questions? --
>
> 1. How is the speed of computation (per CPU) in
> comparion with HP PA-8700 (CPU 440MHZ) or SUN ultra-80
> (CPU 550MHZ)?

I would estimate that a  P-IV may be 4-8 times faster than what you listed
above. (Be carefull, I do NOT have any experiences with those CPUs, this is
just an estimate)

> 2. Where can I find the product for sale?

Your next PC dealer...

> 3. What is the price if I want to have a Pentinum IV
> workstation with 16 CPUs?

Just buy 16 PCs (or maybe 8 dual processor PCs) and connect them via a
network (switch).



                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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====

------------------------------

Date: Tue, 29 Oct 2002 10:19:12 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Question about symmetry operator

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I would like to consult about the symmetry found by wien. I get a .outputs file with lines like :
>  ATOM: -1
>   no pointgroup found, isym = 0

Two possibilities:
If you have angles far off from 90, set them close to (but not exactly) to
90 degree and run symmetry. (Reset them afterwards)

Maybe your structure is incorrectly defined in case.struct. Did it pass
through sgroup ?

Without struct file further help is not possible.


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

====
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------------------------------

Date: Tue, 29 Oct 2002 10:50:48 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Pentinum IV cluster workstation

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

This has been discussed before... is there any way to make a 
"representative test suite" for Wien2k that would allow us to build a 
database of performance that could guide hardware buyers?

Just a few comments on the subject...

About the speed of the P-IV, I would say that it is probably an 
exaggeration. However, any business that wants to sell you these 
machines should be able to let you test. Last time I compared PC 
processors to workstation processors, the result was opposite. A PA-RISC 
at 180MHz was as fast as a dual-processor Pentium III at I think it was 
500MHz, using a test based on Wien97. Simple extrapolation from that 
will put the P-IV at best at the same speed as one of the two 
workstation processors you mentioned. However, my test might be biased 
in another direction than your needs.

However, price/performance-wise, if your programs parallelise well (many 
k-points in the Wien code) and use small amounts of memory (the limit 
for PC's is usually 2-3GB per PC), the PC cluster is probably the best 
solution. It probably requires more system administration time, though. 
PC's with more than 4GB are available (Xeon), but the slowdown due to 
addressing problems (more than the 32-bit address space) is rumoured to 
be prohibitively large.

If raw performance per processor, and big memory (larger than the 2-3GB 
mentioned above) is required by some of your programs (assuming you do 
other and more demanding things than DFT, or DFT with big unit cells) is 
an issue, the current top of the line processors are the Alpha 21264C at 
1GHz-1.25GHz and the IBM Power4 at 1GHz-1.3GHz. The Itanium-I/II sure 
looks good on paper, but the practical performance is not worth 
mentioning, imho. The newer UltraSparc III at 1.2GHz are probably also 
worth considering.

In the end, it all depends on your budget. The best performers are the 
most expensive, just like with most other things.

But if you choose the P-IV, I would recommend to stay with the "basic" 
version - no Xeon and no Celeron, and one processor per machine (current 
sweet spot in price seems to be 2.53GHz), and with the "533" MHz bus. 
Use some money on networking, though... a GBit interface from the 
"server" to the switch, and 100Mbit interfaces from the switch to the 
"slaves".

Best regards,
Torsten.


Peter Blaha wrote:

>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
>>I noticed that many people began to using cluster
>>workstation using Pentinum IV CPU recently. May anyone
>>answer me the following questions? --
>>
>>1. How is the speed of computation (per CPU) in
>>comparion with HP PA-8700 (CPU 440MHZ) or SUN ultra-80
>>(CPU 550MHZ)?
>>
>
>I would estimate that a  P-IV may be 4-8 times faster than what you listed
>above. (Be carefull, I do NOT have any experiences with those CPUs, this is
>just an estimate)
>
>>2. Where can I find the product for sale?
>>
>
>Your next PC dealer...
>
>>3. What is the price if I want to have a Pentinum IV
>>workstation with 16 CPUs?
>>
>
>Just buy 16 PCs (or maybe 8 dual processor PCs) and connect them via a
>network (switch).
>
>
>
>                                      P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



====
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------------------------------

Date: Tue, 29 Oct 2002 20:51:52 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: Re: [WIEN]: Question about symmetry operator

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- --143914132-1156411148-1035895912=:9971
Content-Type: TEXT/PLAIN; charset=US-ASCII

Dear Prof. Peter Blaha,

My case.struct file is attached with this mail.

Thank you very much

yours,
Martin

- -- 
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
~~ "Here is your country, do not let anyone take its glory away  ~~
~~  from you. Do not let selfish men or greedy interests skin    ~~ 
~~  your country of its beauty, its riches, or its romance. The  ~~
~~  world and the future and your very children shall judge you  ~~
~~  according to the way you deal with this sacred trust."       ~~
~~                                                               ~~
~~                                                               ~~
~~               -- Theodore Roosevelt, Antiquities Act of 1906  ~~
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

- --143914132-1156411148-1035895912=:9971
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Content-Transfer-Encoding: BASE64
Content-ID: <Pine.LNX.4.44.0210292051520.9971@yangtze.hku.hk>
Content-Description: 
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- --143914132-1156411148-1035895912=:9971--
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------------------------------

End of wien-digest V2002 #40
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #41
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
Errors-To: owner-wien-digest@theochem.tuwien.ac.at
Precedence: bulk


wien-digest        Tuesday, November 5 2002        Volume 2002 : Number 041




----------------------------------------------------------------------

Date: Tue, 29 Oct 2002 04:55:37 -0800 (PST)
From: sayede adlane <dft22000@yahoo.fr>
Subject: Re: [WIEN]: Pentinum IV cluster workstation

====
sayede adlane <dft22000@yahoo.fr>
submitted the following contribution:
====

Hi, get look at :
http://agenda.ictp.trieste.it/agenda/current/askArchive.php?categ=a01127&id=a01127s12t10&ifd=10382&down=1&type=lecture_notes
following My own experience the compaq alpha machine
seems to be very good for clustering. Regards

 


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------------------------------

Date: Mon, 28 Oct 2002 15:37:02 +0100
From: Peer Kruse <kruse@lem.uni-karlsruhe.de>
Subject: [WIEN]: Wien2k on PC: Error in lapw1

====
Peer Kruse <kruse@lem.uni-karlsruhe.de>
submitted the following contribution:
====

Dear Wien users and developers,
I tried to install Wien2k on 2 rather new PC's and get an
"Error in lapw1" after a period of about 2 hours.
This happens only for a larger number of k points, eg >500,
with only 50 it is working fine. I should have Memory in abundance
(1BG) for my structure of 12 atoms (6 atoms inequivalent) nad the memory is not used (in the first hour of the program at least).
The limits are set to

core file size (blocks, -c) 0
data seg size (kbytes, -d) unlimited
file size (blocks, -f) unlimited
max locked memory (kbytes, -l) unlimited
max memory size (kbytes, -m) unlimited
open files (-n) 1024
pipe size (512 bytes, -p) 8
stack size (kbytes, -s) 32768
cpu time (seconds, -t) unlimited
max user processes (-u) 7168
virtual memory (kbytes, -v) unlimited
Is this ok?

I compiled Wien2k with ifc and pgi, no difference, the same for the precompiled version.
I' m running linux redhat 7.3. 
And  it is running with the same parameters/structures
on the old and slow and even smaller machines with every kind of architecture (dec, pc, notebook) without problem.

Has anyone any experience or further ideas?

Thank you

Peer Kruse



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------------------------------

Date: Tue, 29 Oct 2002 16:49:01 +0100
From: Peer Kruse <kruse@lem.uni-karlsruhe.de>
Subject: [WIEN]: PC:  Error in lapw1

====
Peer Kruse <kruse@lem.uni-karlsruhe.de>
submitted the following contribution:
====

Dear Wien users and developers,
I tried to install Wien2k on 2 rather new PC's and get an
"Error in lapw1" after a period of about 2 hours.
This happens only for a larger number of k points, eg >500,
with only 50 it is working fine. I should have Memory in abundance
(1BG) for my structure of 12 atoms (6 atoms inequivalent) nad the memory 
is not used (in the first hour of the program at least).
The limits are set to

core file size (blocks, -c) 0
data seg size (kbytes, -d) unlimited
file size (blocks, -f) unlimited
max locked memory (kbytes, -l) unlimited
max memory size (kbytes, -m) unlimited
open files (-n) 1024
pipe size (512 bytes, -p) 8
stack size (kbytes, -s) 32768
cpu time (seconds, -t) unlimited
max user processes (-u) 7168
virtual memory (kbytes, -v) unlimited
Is this ok?

I compiled Wien2k with ifc and pgi, no difference, the same for the 
precompiled version.
I' m running linux redhat 7.3. And  it is running with the same 
parameters/structures
on the old and slow and even smaller machines with every kind of 
architecture (dec, pc, notebook) without problem.

Has anyone any experience or further ideas?

Thank you

Peer Kruse



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------------------------------

Date: Tue, 29 Oct 2002 10:23:20 -0800 (PST)
From: yanming Ma <ymma66@yahoo.com>
Subject: Re: [WIEN]: generate k mesh using Xcrysden

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-1334150953-1035915800=:80664
Content-Type: text/plain; charset=us-ascii


Dear Christian,
Thank you for your reply. I have tried to generate k mesh using 3 or 4 special k point. Also I tried to increase the points between two special k points. But the same error message appears. Any more comments are welcom.
Best wishes
Yanming Ma
 koitzsch <Christian.Koitzsch@unifr.ch> wrote:try to calculate the bandstructure in two steps, first path connecting three special k-points and second path over the remaining four - but I have to admit I never bothered to figure out, what the error message really means, I just noticed that if you have a lot of special k-points with not so many points in between, it does not work. Best Regards  Christian Koitzsch Universite de FribourgDepartement de PhysiqueGroupe FKCH-1700 FribourgSuisse ----- Original Message ----- From: yanming Ma To: wien@zeus.theochem.tuwien.ac.at Sent: Monday, October 28, 2002 11:10 PMSubject: [WIEN]: generate k mesh using Xcrysden

Dear wien2k user,

I try to use Xcrysden to generate K-mesh along high symmetry direction. My case structure is Cmca symmetry. After I run the Xcrysden, I choose Conventional BZ, other than primitive BZ because my input atomic positions are from conventional settings of international Crystalgraphic table. Then I select 7 special k points, the total k points along whole path is chosen as 60.  The default value for ISS shringking factor is 2. Minium and Maxium energy are  -1.0 Ry and 1.5 Ry, respectively.  However there are only some zero values generated, the error messages in the generated case.klist file is as following.

ERROR: IDV*NK to big! Decrease number of k points.

I try to decrease K points, but it is useless. 

I try to use primitive BZ. It works. But in my Cmca Case, I can not use primitive BZ. 

Can someone help me to solve this problem? I will highly appreciate your help.

Yanming Ma

 


Yanming Ma Ph.D
Steacie Institute for Molecular Sciences,
National Research Councils of Canada,
Ottawa, Ontario
K1A 0R6
Canada 


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Yanming Ma Ph.D
Steacie Institute for Molecular Sciences,
National Research Councils of Canada,
Ottawa, Ontario
K1A 0R6
Canada


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- --0-1334150953-1035915800=:80664
Content-Type: text/html; charset=us-ascii

<P>Dear Christian,
<P>Thank you for your reply. I have tried to generate k mesh using 3 or 4 special k point. Also I tried to increase the points between&nbsp;two special k points.&nbsp;But the same error message appears. Any more comments are welcom.
<P>Best wishes
<P>Yanming Ma
<P>&nbsp;<B><I>koitzsch &lt;Christian.Koitzsch@unifr.ch&gt;</I></B> wrote:
<BLOCKQUOTE style="PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #1010ff 2px solid">
<META content="MSHTML 5.50.4134.600" name=GENERATOR>
<STYLE></STYLE>

<DIV><FONT face=Arial size=2>try to calculate the bandstructure in two steps, first path&nbsp;connecting three special&nbsp;k-points and second path over the remaining four - but I have to admit I never bothered to figure out, what the error message really means, I just noticed that if you have a lot of special k-points with not so many points in between, it does not work.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Best Regards </FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Christian Koitzsch</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Universite de Fribourg</FONT></DIV>
<DIV><FONT face=Arial size=2>Departement de Physique</FONT></DIV>
<DIV><FONT face=Arial size=2>Groupe FK</FONT></DIV>
<DIV><FONT face=Arial size=2>CH-1700 Fribourg</FONT></DIV>
<DIV><FONT face=Arial size=2>Suisse</FONT></DIV>
<DIV>&nbsp;</DIV>
<BLOCKQUOTE style="PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
<DIV style="FONT: 10pt arial">----- Original Message ----- </DIV>
<DIV style="BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: black"><B>From:</B> <A title=ymma66@yahoo.com href="mailto:ymma66@yahoo.com">yanming Ma</A> </DIV>
<DIV style="FONT: 10pt arial"><B>To:</B> <A title=wien@zeus.theochem.tuwien.ac.at href="mailto:wien@zeus.theochem.tuwien.ac.at">wien@zeus.theochem.tuwien.ac.at</A> </DIV>
<DIV style="FONT: 10pt arial"><B>Sent:</B> Monday, October 28, 2002 11:10 PM</DIV>
<DIV style="FONT: 10pt arial"><B>Subject:</B> [WIEN]: generate k mesh using Xcrysden</DIV>
<DIV><BR></DIV>
<P>Dear wien2k user,</P>
<P>I try to use Xcrysden to generate K-mesh along high symmetry direction. My case structure is Cmca symmetry. After I run the Xcrysden, I choose Conventional BZ, other than primitive BZ because my input atomic positions are from conventional settings of international Crystalgraphic table. Then I select 7 special k points, the total k points along whole path is chosen as 60.&nbsp; The default value for ISS shringking factor is 2. Minium and Maxium energy&nbsp;are &nbsp;-1.0 Ry and 1.5 Ry, respectively.&nbsp; However there&nbsp;are only some zero values generated,&nbsp;the error messages in the&nbsp;generated case.klist file is as following.</P>
<P>ERROR:&nbsp;IDV*NK to big! Decrease number of k points.</P>
<P>I try to decrease K points, but it is useless. </P>
<P>I try to use primitive BZ. It works. But in my Cmca Case, I&nbsp;can not use primitive BZ. </P>
<P>Can someone help me to solve this problem? I will highly appreciate your help.</P>
<P>Yanming Ma</P>
<P>&nbsp;</P><BR><BR>Yanming Ma Ph.D<BR>Steacie Institute for Molecular Sciences,<BR>National Research Councils of Canada,<BR>Ottawa, Ontario<BR>K1A 0R6<BR>Canada 
<P><BR>
<HR SIZE=1>
Do you Yahoo!?<BR><A href="http://webhosting.yahoo.com/">Y! Web Hosting</A> - Let the expert host your web site</BLOCKQUOTE></BLOCKQUOTE><BR><BR>Yanming Ma Ph.D<br>Steacie Institute for Molecular Sciences,<br>National Research Councils of Canada,<br>Ottawa, Ontario<br>K1A 0R6<br>Canada<p><br><hr size=1>Do you Yahoo!?<br>
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------------------------------

Date: Tue, 29 Oct 2002 20:05:17 +0100
From: "koitzsch" <Christian.Koitzsch@unifr.ch>
Subject: Re: [WIEN]: generate k mesh using Xcrysden

====
"koitzsch" <Christian.Koitzsch@unifr.ch>
submitted the following contribution:
====


This is a multi-part message in MIME format.

- ------=_NextPart_000_02D2_01C27F86.808350F0
Content-Type: text/plain;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

if you want you can send me your struct file and I try it with our =
version.=20

Bye

Christian


  ----- Original Message -----=20
  From: yanming Ma=20
  To: wien@zeus.theochem.tuwien.ac.at=20
  Sent: Tuesday, October 29, 2002 7:23 PM
  Subject: Re: [WIEN]: generate k mesh using Xcrysden


  Dear Christian,=20

  Thank you for your reply. I have tried to generate k mesh using 3 or 4 =
special k point. Also I tried to increase the points between two special =
k points. But the same error message appears. Any more comments are =
welcom.=20

  Best wishes=20

  Yanming Ma=20

   koitzsch <Christian.Koitzsch@unifr.ch> wrote:=20

    try to calculate the bandstructure in two steps, first path =
connecting three special k-points and second path over the remaining =
four - but I have to admit I never bothered to figure out, what the =
error message really means, I just noticed that if you have a lot of =
special k-points with not so many points in between, it does not work.

    Best Regards=20

    Christian Koitzsch

    Universite de Fribourg
    Departement de Physique
    Groupe FK
    CH-1700 Fribourg
    Suisse

      ----- Original Message -----=20
      From: yanming Ma=20
      To: wien@zeus.theochem.tuwien.ac.at=20
      Sent: Monday, October 28, 2002 11:10 PM
      Subject: [WIEN]: generate k mesh using Xcrysden


      Dear wien2k user,

      I try to use Xcrysden to generate K-mesh along high symmetry =
direction. My case structure is Cmca symmetry. After I run the Xcrysden, =
I choose Conventional BZ, other than primitive BZ because my input =
atomic positions are from conventional settings of international =
Crystalgraphic table. Then I select 7 special k points, the total k =
points along whole path is chosen as 60.  The default value for ISS =
shringking factor is 2. Minium and Maxium energy are  -1.0 Ry and 1.5 =
Ry, respectively.  However there are only some zero values generated, =
the error messages in the generated case.klist file is as following.

      ERROR: IDV*NK to big! Decrease number of k points.

      I try to decrease K points, but it is useless.=20

      I try to use primitive BZ. It works. But in my Cmca Case, I can =
not use primitive BZ.=20

      Can someone help me to solve this problem? I will highly =
appreciate your help.

      Yanming Ma





      Yanming Ma Ph.D
      Steacie Institute for Molecular Sciences,
      National Research Councils of Canada,
      Ottawa, Ontario
      K1A 0R6
      Canada=20




- -------------------------------------------------------------------------=
- -
      Do you Yahoo!?
      Y! Web Hosting - Let the expert host your web site


  Yanming Ma Ph.D
  Steacie Institute for Molecular Sciences,
  National Research Councils of Canada,
  Ottawa, Ontario
  K1A 0R6
  Canada




- -------------------------------------------------------------------------=
- -----
  Do you Yahoo!?
  HotJobs - Search new jobs daily now

- ------=_NextPart_000_02D2_01C27F86.808350F0
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 5.50.4134.600" name=3DGENERATOR></HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT face=3DArial size=3D2>if you want you can send me your struct =
file and I=20
try it with our version. </FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Bye</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Christian</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<BLOCKQUOTE=20
style=3D"PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; =
BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
  <DIV style=3D"FONT: 10pt arial">----- Original Message ----- </DIV>
  <DIV=20
  style=3D"BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: =
black"><B>From:</B>=20
  <A title=3Dymma66@yahoo.com href=3D"mailto:ymma66@yahoo.com">yanming =
Ma</A> </DIV>
  <DIV style=3D"FONT: 10pt arial"><B>To:</B> <A=20
  title=3Dwien@zeus.theochem.tuwien.ac.at=20
  =
href=3D"mailto:wien@zeus.theochem.tuwien.ac.at">wien@zeus.theochem.tuwien=
.ac.at</A>=20
  </DIV>
  <DIV style=3D"FONT: 10pt arial"><B>Sent:</B> Tuesday, October 29, 2002 =
7:23=20
  PM</DIV>
  <DIV style=3D"FONT: 10pt arial"><B>Subject:</B> Re: [WIEN]: generate k =
mesh=20
  using Xcrysden</DIV>
  <DIV><BR></DIV>
  <P>Dear Christian,=20
  <P>Thank you for your reply. I have tried to generate k mesh using 3 =
or 4=20
  special k point. Also I tried to increase the points between&nbsp;two =
special=20
  k points.&nbsp;But the same error message appears. Any more comments =
are=20
  welcom.=20
  <P>Best wishes=20
  <P>Yanming Ma=20
  <P>&nbsp;<B><I>koitzsch &lt;<A=20
  =
href=3D"mailto:Christian.Koitzsch@unifr.ch">Christian.Koitzsch@unifr.ch</=
A>&gt;</I></B>=20
  wrote:=20
  <BLOCKQUOTE=20
  style=3D"PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #1010ff 2px =
solid">
    <META content=3D"MSHTML 5.50.4134.600" name=3DGENERATOR>
    <STYLE></STYLE>

    <DIV><FONT face=3DArial size=3D2>try to calculate the bandstructure =
in two=20
    steps, first path&nbsp;connecting three special&nbsp;k-points and =
second=20
    path over the remaining four - but I have to admit I never bothered =
to=20
    figure out, what the error message really means, I just noticed that =
if you=20
    have a lot of special k-points with not so many points in between, =
it does=20
    not work.</FONT></DIV>
    <DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
    <DIV><FONT face=3DArial size=3D2>Best Regards </FONT></DIV>
    <DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
    <DIV><FONT face=3DArial size=3D2>Christian Koitzsch</FONT></DIV>
    <DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
    <DIV><FONT face=3DArial size=3D2>Universite de Fribourg</FONT></DIV>
    <DIV><FONT face=3DArial size=3D2>Departement de =
Physique</FONT></DIV>
    <DIV><FONT face=3DArial size=3D2>Groupe FK</FONT></DIV>
    <DIV><FONT face=3DArial size=3D2>CH-1700 Fribourg</FONT></DIV>
    <DIV><FONT face=3DArial size=3D2>Suisse</FONT></DIV>
    <DIV>&nbsp;</DIV>
    <BLOCKQUOTE=20
    style=3D"PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; =
BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
      <DIV style=3D"FONT: 10pt arial">----- Original Message ----- =
</DIV>
      <DIV=20
      style=3D"BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: =
black"><B>From:</B>=20
      <A title=3Dymma66@yahoo.com =
href=3D"mailto:ymma66@yahoo.com">yanming Ma</A>=20
      </DIV>
      <DIV style=3D"FONT: 10pt arial"><B>To:</B> <A=20
      title=3Dwien@zeus.theochem.tuwien.ac.at=20
      =
href=3D"mailto:wien@zeus.theochem.tuwien.ac.at">wien@zeus.theochem.tuwien=
.ac.at</A>=20
      </DIV>
      <DIV style=3D"FONT: 10pt arial"><B>Sent:</B> Monday, October 28, =
2002 11:10=20
      PM</DIV>
      <DIV style=3D"FONT: 10pt arial"><B>Subject:</B> [WIEN]: generate k =
mesh=20
      using Xcrysden</DIV>
      <DIV><BR></DIV>
      <P>Dear wien2k user,</P>
      <P>I try to use Xcrysden to generate K-mesh along high symmetry =
direction.=20
      My case structure is Cmca symmetry. After I run the Xcrysden, I =
choose=20
      Conventional BZ, other than primitive BZ because my input atomic =
positions=20
      are from conventional settings of international Crystalgraphic =
table. Then=20
      I select 7 special k points, the total k points along whole path =
is chosen=20
      as 60.&nbsp; The default value for ISS shringking factor is 2. =
Minium and=20
      Maxium energy&nbsp;are &nbsp;-1.0 Ry and 1.5 Ry, =
respectively.&nbsp;=20
      However there&nbsp;are only some zero values generated,&nbsp;the =
error=20
      messages in the&nbsp;generated case.klist file is as =
following.</P>
      <P>ERROR:&nbsp;IDV*NK to big! Decrease number of k points.</P>
      <P>I try to decrease K points, but it is useless. </P>
      <P>I try to use primitive BZ. It works. But in my Cmca Case, =
I&nbsp;can=20
      not use primitive BZ. </P>
      <P>Can someone help me to solve this problem? I will highly =
appreciate=20
      your help.</P>
      <P>Yanming Ma</P>
      <P>&nbsp;</P><BR><BR>Yanming Ma Ph.D<BR>Steacie Institute for =
Molecular=20
      Sciences,<BR>National Research Councils of Canada,<BR>Ottawa,=20
      Ontario<BR>K1A 0R6<BR>Canada=20
      <P><BR>
      <HR SIZE=3D1>
      Do you Yahoo!?<BR><A href=3D"http://webhosting.yahoo.com/">Y! Web=20
      Hosting</A> - Let the expert host your web=20
  site</BLOCKQUOTE></BLOCKQUOTE><BR><BR>Yanming Ma Ph.D<BR>Steacie =
Institute for=20
  Molecular Sciences,<BR>National Research Councils of =
Canada,<BR>Ottawa,=20
  Ontario<BR>K1A 0R6<BR>Canada
  <P><BR>
  <HR SIZE=3D1>
  Do you Yahoo!?<BR><A=20
  href=3D"http://rd.yahoo.com/careers/mailsig/*http://www.hotjobs.com =
">HotJobs</A>=20
  - Search new jobs daily now</BLOCKQUOTE></BODY></HTML>

- ------=_NextPart_000_02D2_01C27F86.808350F0--


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------------------------------

Date: Tue, 29 Oct 2002 22:39:46 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: "x lapw2" error

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

After the convergence of the SCF cycles, I changed the "TOT" to "EFG" in
case.in2 file, and run "x lapw2" but failed with the following
information:

	STOP: L2main - Error
	0.0u 0.0s 0:02 0% 0+0k 0+0io 0pf+0w

The lapw2.error file is as the following line:

	'l2main' - NEFG.GT.23.

Could you please let me how to fix it?

Thank you in adavance!


Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Wed, 30 Oct 2002 10:39:55 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: "x lapw2" error

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> After the convergence of the SCF cycles, I changed the "TOT" to "EFG" in
> case.in2 file, and run "x lapw2" but failed with the following
> information:
>
> STOP: L2main - Error
> 0.0u 0.0s 0:02 0% 0+0k 0+0io 0pf+0w
>
> The lapw2.error file is as the following line:
>
> 'l2main' - NEFG.GT.23.
>
> Could you please let me how to fix it?

Have you changed manually LM combinations in your case.in2 file? I asked
this because the error occurs due to the following restriction:

RHOEFG(NRAD,3,23), LEFG(3,3,23), MEFG(3,3,23), where 23 is the maximum of
NEFG(LQ), and LQ can be 1, 2, or 3 depending on some condition(s) on quantum
numbers.

So, if NEFG >23, then one encounters the 'l2main','NEFG.GT.23.' message.

It appears max. of NEFG is limited to 23 because of a physical restriction
on EFG (L=2, M=0). This means that it is not just a dummy variable. If this
is true, then most likely the point groups of your atoms are not consistent
with your LM combinations. If you have not changed LM combinations manually,
then I think (this is just a guess) the 23 in l2main.F can be increased, at
least to see what is going on.

        Your,
        Saeid.

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------------------------------

Date: Wed, 30 Oct 2002 08:26:28 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: "x lapw2" error

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> > After the convergence of the SCF cycles, I changed the "TOT" to "EFG" in
> > case.in2 file, and run "x lapw2" but failed with the following
> > information:
> >
> > STOP: L2main - Error
> > 0.0u 0.0s 0:02 0% 0+0k 0+0io 0pf+0w
> >
> > The lapw2.error file is as the following line:
> >
> > 'l2main' - NEFG.GT.23.
> >
> > Could you please let me how to fix it?
>
> Have you changed manually LM combinations in your case.in2 file? I asked
> this because the error occurs due to the following restriction:

In fact in a low symmetry case, where you have all possible L=2 combinations
(case.in2), the possible contributions to the EFG might be more than 23,
which is a hardcoded limit.
To overcome this, modify your LM list and run x lapw2 twice, once only with
LM=0 and e.g. 2 0,2 2, -2 2 combinations, then with 0 0 and 2 1 and -2 1.

PS: for low symmetry the analysis is usually less meaningfull, nevertheless
you may find out about the importance of p or d states.

See the very good faq page provided by S.Cottenier (www.wien2k.at/reg_users)




                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 30 Oct 2002 08:46:11 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Pentinum IV cluster workstation

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====


Some benchmark results of lapw1 (large matrices):

Supermicro (dual Xeon 2.4 GHz, 2GB)
ifc/mkl/omp=1:          5m54.817s

ifc/mkl:                4m50.678s
ifc/mkl/ht              5m42.164s


- -----------------------------------------------------------------
Compaq ES45 (Alpha ev7, 1GHz, 16GB)

1 job:
- ------------------------------------------------------------------
f90/cxml                6m29.61s        6m27.55s        0m1.68s
- ------------------------------------------------------------------
2 jobs:
- ------------------------------------------------------------------
f90/cxml                6m55.68s        6m53.51s        0m1.76s
- ------------------------------------------------------------------

IBM SP (PowerIII-2, 375 MHz, 16GB)
1 job:
- ------------------------------------------------------------------
xlf90/essl              10m26.15s       10m20.93s       0m3.40s
- ------------------------------------------------------------------

So the PC-based solutions outperform even a quite new Compaq EV7 (1 GHz).

To my knowledge the fastest Itaniums and IBM Power-IV might be a little
faster than fast P-IV (but only some percentage, not really big factors!!),
but compare the price:

A four processor EV7 costs 80.000 Euro, two dual Xeon machines 10.000 !!!
4 "normal" P-IV PCs 8.000.

Either look for a new dual Xeon (with a new motherboard with two memory buses
so that memory-access is not such a problem) or simply buy the cheapest
P-IV single cpu machines (~2.4 GHz) with RAMBUS (faster) or 533 MHz bus
(slower but cheaper).

In addition one must thing for which systems you want to apply those machines.
If you really need 16 Gb memory and fast communication (only one k-point),
your P4-cluster must have at least a Gbit network (and still you may loose
a lot of performance because of communication agains an e.g. EV7).
However, for 99% of the applications a P4-cluster is certainly the best
solution.


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 30 Oct 2002 09:02:56 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Question about symmetry operator

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> My case.struct file is attached with this mail.

Your struct file violates almost everything:

Atom= -1: X=0.92404845 Y=0.50000000 Z=1.00000000

All positions must be between 0 and .lt. 1 !!!  (put z=0)


Atom= -5: X=0.90329404 Y=0.63103818 Z=1.00000000
          MULT=52          ISPLIT= 8

A multiplicity of 52 is not possible!! (The spacegroup symmetries limit
the multiplicity to 48)



Provided you entered correct positions (which I cannot check) sgroup
provides a new struct file with 20 independent positions. Why did you
not take it ?

warning: !!! Number of inequivalent atoms has changed.
         !!! Old value= 8     New value= 20

warning: !!! Wrong multiplicity for atom 5
         !!! Struct file is not consistent with space group found.



nn can do the same, provided you "label" your atoms "C 1", C 2,....

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 30 Oct 2002 11:58:02 +0100 (CET)
From: Max Winkelmann <max@pinguix.physik.uni-karlsruhe.de>
Subject: [WIEN]: Compiling WIEN2k

====
Max Winkelmann <max@pinguix.physik.uni-karlsruhe.de>
submitted the following contribution:
====

Hi
I have a problem when compiling WIEN2k. Starting ./siteconfig_lapw and
then recompiling (r) I get the error "undefined reference to 'getarg_' ".
I'm using the intel ifc-compiler for linux-PCs. I know already that I have
to implement the portability library. The library is in my library-path
and I used the compiler-option "-Vaxlib". So referring to the manuals
everything should be fine. Anyone any idea?

Greetings

	Max Winkelmann

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------------------------------

Date: Wed, 30 Oct 2002 15:15:53 +0100
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: Adapting files to run with -so

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

I am working on a case where I would like to add spin-orbit coupling, 
since this according to the userguide can reduce problems with charge 
oscillations caused by LDA+U. When I run the initso_lapw script I get 
this information:

Do you have a spinpolarized case (and want to run symmetso) ? (y/N)y
FORTRAN STOP
2.370u 0.060s 0:02.98 81.5%    0+0k 0+0io 213pf+0w
 A new structure for SO calculations has been created (_so).
 If you commit it will create new  Nio.struct, in1(c), in2c, inc,
 clmsum/up/dn, vspup/dn and vnsup/dn files. (Please SAVE any previous
 calculations)

NOTE: Files for -orb (Nio.indm(c),inorb,dmatup/dn) must be adapted manually

My question concerns the last sentence. How should I adapt the files for 
- -orb? What changes must I do to the files I have been using before I 
added SO coupling?

Thanks for your replies! Any suggestions are welcome!

Best regards,
Thomas Claesson

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------------------------------

Date: Wed, 30 Oct 2002 15:30:13 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Adapting files to run with -so

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I am working on a case where I would like to add spin-orbit coupling,
> since this according to the userguide can reduce problems with charge
> oscillations caused by LDA+U. When I run the initso_lapw script I get

If you have problems with LDA+U convergence for NiO, you will also have
these problems when adding SO. NiO converges reasonably quick using LDA+U
starting from a scf LDA (GGA) calculation.

You do something wrong there!

The recommended sequence would be:

runsp
save_lapw
create inorb and indm-files
x lapwdm -up/dn  (to have a case.dmatup/dn file already in the first cycle)
runsp -orb


> Do you have a spinpolarized case (and want to run symmetso) ? (y/N)y
> FORTRAN STOP
> 2.370u 0.060s 0:02.98 81.5%    0+0k 0+0io 213pf+0w
>  A new structure for SO calculations has been created (_so).
>  If you commit it will create new  Nio.struct, in1(c), in2c, inc,
>  clmsum/up/dn, vspup/dn and vnsup/dn files. (Please SAVE any previous
>  calculations)
>
> NOTE: Files for -orb (Nio.indm(c),inorb,dmatup/dn) must be adapted manually
>
> My question concerns the last sentence. How should I adapt the files for
> -orb? What changes must I do to the files I have been using before I
> added SO coupling?

This depends on your case. For NiO probably nothing (exept that you need a
case.indmc file instead of case.indm when SO is used)

In other cases, atomic positions could split creating a new struct file
(with more atoms) and then you must update those files.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 30 Oct 2002 17:45:52 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Compiling WIEN2k

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I have a problem when compiling WIEN2k. Starting ./siteconfig_lapw and
> then recompiling (r) I get the error "undefined reference to 'getarg_' ".
> I'm using the intel ifc-compiler for linux-PCs. I know already that I have
> to implement the portability library. The library is in my library-path
> and I used the compiler-option "-Vaxlib". So referring to the manuals
> everything should be fine. Anyone any idea?

Did you use the default options of the latest WIEN2k-release ? (Maybe download
again).

Just from your comments above:   -Vaxlib must be in the loaderflags, not
in the FOPT compiler options:

LDFLAGS = -L../SRC_lib -Vaxlib -static -L/opt/intel/mkl/lib/32

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 30 Oct 2002 13:55:49 CST
From: Yongbin Lee <yblee@iastate.edu>
Subject: [WIEN]: SRC_lapw2/outp.f

====
Yongbin Lee <yblee@iastate.edu>
submitted the following contribution:
====

Dear WIEN_user

  I got an error by
     x lapw2 -c -up -so -qtl -p
The error was 

    Input/Output Error 153: Input file ended

       In Procedure: outp
            At Line: 245

          Statement: Formatted READ
               Unit: 12
       Connected To: TEST.normsoup
               Form: Formatted
             Access: Sequential
    Records Read   : 0
    Records Written: 0

    End of diagnostics

It came from SRC_lapw2/outp.f
         
    ! Read norm file in spinpol. so case
          if(kso.eq.2.and.nspin1.eq.2) then
          rewind 12
          allocate (sonorm(nbandmax,nk))
          DO JK=1,NK
             read(12,'(4e20.11)')  (sonorm(jb,jk),  JB=1,NB(JK))
             write(6,*) 'jk',jk
             write(6,'(4e20.11)')  (sonorm(jb,jk),  JB=1,NB(JK))
          enddo
          endif
     !

The problem is I got "TEST.normsoup_*" files with the 
"empty TEST.normsoup " file by parallel calculation.
I guess this routine is just for single processor job.
What is this routine for?
What do I need to do?

   Sincerely
   Yongbin


  




   
 
  
 

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------------------------------

Date: Wed, 30 Oct 2002 14:29:31 -0800 (PST)
From: Wenqing ZHANG <dft_flapw@yahoo.com>
Subject: Re: [WIEN]: Pentinum IV cluster workstation

====
Wenqing ZHANG <dft_flapw@yahoo.com>
submitted the following contribution:
====


Peter, 

What do you mean by "Xeon machine"? Is it just a
"supermicro" PC with P-IV-Xeon CPU (2.4GHZ, 1GB/CPU
memory)? Where did you buy the machine?

I noticed there is a type of server using P-IV-Xeon
CPU from Dell company, named PowerEdge 8450 or so.
That is very expensive. Any comment about that
machine?

Yours -- Wenqing


> 
> A four processor EV7 costs 80.000 Euro, two dual
> Xeon machines 10.000 !!!
> 4 "normal" P-IV PCs 8.000.
>  
> 
> Some benchmark results of lapw1 (large matrices):
> 
> Supermicro (dual Xeon 2.4 GHz, 2GB)
> ifc/mkl/omp=1:          5m54.817s
> 
> ifc/mkl:                4m50.678s
> ifc/mkl/ht              5m42.164s
>   


=====
Wenqing ZHANG
1970 Crystal Lake Dr. Apt#E79
Shelby Twp., MI 48316
Tel: (810)254-9931(h), (810)323-1551(o)
Fax: (810)323-9898

__________________________________________________
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------------------------------

Date: Wed, 30 Oct 2002 20:19:08 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: "x lapw2" error

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---559023410-851401618-1036030748=:22886
Content-Type: TEXT/PLAIN; charset=US-ASCII

Dear Saeid and Peter:

Thank you for your help, I appreciate that!

Yes, my sample is a monolinic symmetry mineral, and I tried to change the
LM combinations in case.in2 and run "x lapw2", the results were same as
before. I don't understand what it meant either by "l2main.F" in Saeid
email. So I attach the case.in2 file with this email, could you please
take a look and give me more instructions about how to run "lapw2" for EFG
analysis?

Thank you in adavance!


On Wed, 30 Oct 2002, Saeid Jalali wrote:

> ====
> "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> submitted the following contribution:
> ====
>
> > After the convergence of the SCF cycles, I changed the "TOT" to "EFG" in
> > case.in2 file, and run "x lapw2" but failed with the following
> > information:
> >
> > STOP: L2main - Error
> > 0.0u 0.0s 0:02 0% 0+0k 0+0io 0pf+0w
> >
> > The lapw2.error file is as the following line:
> >
> > 'l2main' - NEFG.GT.23.
> >
> > Could you please let me how to fix it?
>
> Have you changed manually LM combinations in your case.in2 file? I asked
> this because the error occurs due to the following restriction:
>
> RHOEFG(NRAD,3,23), LEFG(3,3,23), MEFG(3,3,23), where 23 is the maximum of
> NEFG(LQ), and LQ can be 1, 2, or 3 depending on some condition(s) on quantum
> numbers.
>
> So, if NEFG >23, then one encounters the 'l2main','NEFG.GT.23.' message.
>
> It appears max. of NEFG is limited to 23 because of a physical restriction
> on EFG (L=2, M=0). This means that it is not just a dummy variable. If this
> is true, then most likely the point groups of your atoms are not consistent
> with your LM combinations. If you have not changed LM combinations manually,
> then I think (this is just a guess) the 23 in l2main.F can be increased, at
> least to see what is going on.
>
>         Your,
>         Saeid.
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

- ---559023410-851401618-1036030748=:22886
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------------------------------

Date: Thu, 31 Oct 2002 09:03:38 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: "x lapw2" error

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> Yes, my sample is a monolinic symmetry mineral, and I tried to change the
> LM combinations in case.in2 and run "x lapw2", the results were same as
> before. I don't understand what it meant either by "l2main.F" in Saeid
> email. So I attach the case.in2 file with this email, could you please
> take a look and give me more instructions about how to run "lapw2" for EFG
> analysis?
Counting no. of LM combinations written in the sent case.in2 show that NEFG
is 23 for the first point group of your case possessing 2 atoms -- that is
okay -- but NEFG>23 for the second point group possessing 4 atoms, which
contravenes the condition exceeding Max(NEFG)=23.
The author nicely recommended that:
"To overcome this, modify your LM list and run x lapw2 twice, once only with
LM=0 and e.g. 2 0,2 2, -2 2 combinations, then with 0 0 and 2 1 and -2 1."
And this is a task for us to realize how to use this way (idea). Breaking
the following LM's
 0 0 1 0 1 1-1 1 2 0 2 1-2 1 2 2-2 2 3 0 3 1-3 1 3 2-3 2 3 3-3 3 4 0 4 1-4 1
4 2-4 2 4 3-4 3 4 4-4 4 5 0 5 1-5 1 5 2-5 2 5 3-5 3 5 4-5 4 5 5-5 5 6 0 6
1-6 1 6 2-6 2 6 3-6 3 6 4-6 4 6 5-6 5 6 6-6 6
 TO
 0 0 1 0 2 0 2 2-2 2 3 0 3 2-3 2 4 0 4 2-4 2 4 4-4 4 5 0 5 2-5 2 5 4-5 4 6 0
6 2-6 2 6 4-6 4 6 6-6 6
AND
 0 0 1 1-1 1 2 1-2 1 3 1-3 1 3 3-3 3 4 1-4 1 4 3-4 3 5 1-5 1 5 3-5 3 5 5-5 5
6 1-6 1 6 3-6 3 6 5-6 5
holds the condition on NEFG. Then one runs lapw2 distinctly for each set
(please check the breaking to see if I did miss some LM's). Please notice
that the condition on NEFG is checked once one turns the light of EFG on, so
one does not need to break the LM's in a regular SCF.
        Your,
        Saeid.

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Date: Thu, 31 Oct 2002 07:15:20 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Pentinum IV cluster workstation

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Wenqing,

he means a machine with P-IV-Xeon CPU's, yes. Any one... and Supermicro 
refers to the motherboard.

what you do is... go down to a local computer store and specify what you 
want (bamboo PC with dual P-IV-Xeon, or with single P-IV) and get a ton 
of them. Buy some switches and connect them. Put Linux on them, and you 
have a many-processor Linux cluster. The system administration is of 
course heavier than using the money on "big iron" but if your needs are 
related mostly to the Wien code, it might be the better option.

Alternatively, take a 19" rack with 1U PC enclosures, buy the 
motherboards, RAM, CPU's and disks needed. Using a dual-processor (with 
angled RAM sockets to keep it inside a 1U box) motherboard, you get 
about 80 CPU's in a standard 42U cabinet + the network switch.

However, stay below 4GB RAM in each Xeon machine for performance reasons.

You might also have a look at "blade" servers, but I am not sure they 
come with P-IV based CPU's yet. They will give you the highest possible 
density of CPU's (working CPU's per cubic foot), if space is an issue.

If space, power, and cooling are non-issues, the cheapest option is to 
go for standard P-IV's with SDRAM - I think there are some VIA-based 
motherboards that support SDRAM in a dual bank configuration - they are 
almost as fast as a single-bank DDR or RDRAM.

Always take the ones with integrated graphics and network, unless you 
need huge calculations for a single k-point - then take "big iron" like 
Compaq ES-45 or IBM p630. Gbit ethernet is too expensive compared to 
what you get out of it with PC's, imho.

Best regards,
Torsten.




Wenqing ZHANG wrote:

>====
>Wenqing ZHANG <dft_flapw@yahoo.com>
>submitted the following contribution:
>====
>
>
>Peter, 
>
>What do you mean by "Xeon machine"? Is it just a
>"supermicro" PC with P-IV-Xeon CPU (2.4GHZ, 1GB/CPU
>memory)? Where did you buy the machine?
>
>I noticed there is a type of server using P-IV-Xeon
>CPU from Dell company, named PowerEdge 8450 or so.
>That is very expensive. Any comment about that
>machine?
>
>Yours -- Wenqing
>
>
>>A four processor EV7 costs 80.000 Euro, two dual
>>Xeon machines 10.000 !!!
>>4 "normal" P-IV PCs 8.000.
>> 
>>
>>Some benchmark results of lapw1 (large matrices):
>>
>>Supermicro (dual Xeon 2.4 GHz, 2GB)
>>ifc/mkl/omp=1:          5m54.817s
>>
>>ifc/mkl:                4m50.678s
>>ifc/mkl/ht              5m42.164s
>>  
>>
>
>
>=====
>Wenqing ZHANG
>1970 Crystal Lake Dr. Apt#E79
>Shelby Twp., MI 48316
>Tel: (810)254-9931(h), (810)323-1551(o)
>Fax: (810)323-9898
>
>__________________________________________________
>Yahoo! - We Remember
>9-11: A tribute to the more than 3,000 lives lost
>http://dir.remember.yahoo.com/tribute
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Thu, 31 Oct 2002 09:10:39 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: SRC_lapw2/outp.f

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>   I got an error by
>      x lapw2 -c -up -so -qtl -p
> The error was
>
>     Input/Output Error 153: Input file ended
>
>        In Procedure: outp
>             At Line: 245
>
>           Statement: Formatted READ
>                Unit: 12
>        Connected To: TEST.normsoup
>
> The problem is I got "TEST.normsoup_*" files with the
> "empty TEST.normsoup " file by parallel calculation.
> I guess this routine is just for single processor job.
> What is this routine for?
> What do I need to do?

Thanks for this report.

I added recently these normsoup/dn files, since this is needed
to calculate the spin-up/dn projected DOS when SO is included.
(So far you would always get the total DOS (spin up+dn) when SO is included,
even when running x tetra -up)

Of course I forgot to support parallel calculations.

Please try simply:

cat TEST.normsoup_1 TEST.normsoup_2 TEST.normsoup_3 ... > TEST.normsoup

And test the up and dn-spin DOS (it should look similar to the non-SO DOS).

If this works I will put it into the lapwso_para script.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 31 Oct 2002 10:04:46 +0100
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: Input for AFM calculations

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

In section 4.5.4 about input for AFM calculations it says, among other 
things, that you must do this:

Edit case.inst and flip the spin of one of the AF atoms (i.e. invert the 
spin up and dn occupation numbers). In addition you must set a zero 
moment (identical spin up and dn oc-cupations) for all  non-magnetic  
atoms, otherwise AFMINPUT cannot determine the proper input for CLMCOPY.

My questions is, should you do these two modifications to the case.inst 
file even if you choose to not use AFMINPUT and runafm_lapw?

Thanks for your replies!

Best regards,
Thomas Claesson


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------------------------------

Date: Thu, 31 Oct 2002 01:17:37 -0800 (PST)
From: sayede adlane <dft22000@yahoo.fr>
Subject: Re: [WIEN]: Pentinum IV cluster workstation

====
sayede adlane <dft22000@yahoo.fr>
submitted the following contribution:
====

>I noticed there is a type of server using P-IV-Xeon
>CPU from Dell company, named PowerEdge 8450 or so.
>That is very expensive. Any comment about that
>machine?
This machine as you noticed is a server not realy a
worksation, it is very expensive because its
integrated a RED, hotplug disk storage etc .... And
you dont need all thoes things to do Parallel
caclulation.

Regrads
A. Sayede

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------------------------------

Date: Thu, 31 Oct 2002 10:24:54 +0100
From: "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: Input for AFM calculations

====
"Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====


> ====
> Thomas Claesson <tcl@kth.se>
> submitted the following contribution:
> ====
>
> In section 4.5.4 about input for AFM calculations it says, among other
> things, that you must do this:
>
> Edit case.inst and flip the spin of one of the AF atoms (i.e. invert the
> spin up and dn occupation numbers). In addition you must set a zero
> moment (identical spin up and dn oc-cupations) for all  non-magnetic
> atoms, otherwise AFMINPUT cannot determine the proper input for CLMCOPY.
>
> My questions is, should you do these two modifications to the case.inst
> file even if you choose to not use AFMINPUT and runafm_lapw?

Even if you don't use runafm_lapw, you at least need to flip one of the
moments, such that you start from an AF configuration. WIEN will never
spontaneously find an AF solution if you start from a ferro or nonmagnetic
one. Using runafm_lapw is equivalent to this, only it saves you one half of
the time.

Putting a zero moment on nonmagnetic atoms is less crucial if you don't use
runafm, I think. Nevertheless, you avoid bias by starting from zero moments.
Imagine that the AF atoms induce some positive or negative moment on a
neighbouring atom. If you have made the moment positive at the beginning and
the real solution is a negative moment, it could take longer to converge or
in the worst case you might get trapped in solution with a positive moment
which is not the ground state. If you don't have a specific reason to start
with a moment on the non-magnetic atoms, then it seems safer to make it
zero.

Stefaan

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------------------------------

Date: Thu, 31 Oct 2002 13:22:29 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: Re: [WIEN]: Adapting files to run with -so

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====

Dear Peter:
 After reading your mail,I have some general questions about the sequence 
of runsp with SO or (and)ORB, I hope can get your help or advice.

  1 : when runsp+SO , is there any difference between the two kinds of 
sequences list below:

     a: init_lapw
        initso_lapw-->accept the files it generated
        runsp_lapw -so

     b:the methods recommanded in the UG:
        run[sp]_lapw --->
        after convergence, then save_lapw 
        initso_lapw 
        run[sp]_lapw -so 

  2:when runsp+ORB, is there any difference between the two kinds of 
sequences list below:

    a:init_lapw
      edit case.indm(c),inorb by hand
      runsp_lapw -orb

    b:the method in your mail:
      runsp
      save_lapw
      create inorb and indm-files
      x lapwdm -up/dn  (to have a case.dmatup/dn file already in the first 
cycle)
      runsp -orb


 3: runsp+SO+ORB, is the sequence listed below is right?

      init_lapw
      initso_lapw -->accept the struct files it generated
      edit case.indmc , case.inorb by hand
      runsp_lapw -so -orb

  is there any different sequence? If It also need to first runsp_lapw to 
achieve convergence, then save the result(like mentioned above), then 
runsp_lapw -so -orb?

   Thanks 
Yours 
  Hai

>From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: WIEN <wien@zeus.theochem.tuwien.ac.at>
>Subject: Re: [WIEN]: Adapting files to run with -so
>Date: Wed, 30 Oct 2002 15:30:13 +0100 (MET)
>
>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
> > I am working on a case where I would like to add spin-orbit coupling,
> > since this according to the userguide can reduce problems with charge
> > oscillations caused by LDA+U. When I run the initso_lapw script I get
>
>If you have problems with LDA+U convergence for NiO, you will also have
>these problems when adding SO. NiO converges reasonably quick using LDA+U
>starting from a scf LDA (GGA) calculation.
>
>You do something wrong there!
>
>The recommended sequence would be:
>
>runsp
>save_lapw
>create inorb and indm-files
>x lapwdm -up/dn  (to have a case.dmatup/dn file already in the first 
cycle)
>runsp -orb
>
>

_________________________________________________________________
ÓëÁª»úµÄÅóÓÑ½øÐÐ½»Á÷£¬ÇëÊ¹ÓÃ MSN Messenger: http://messenger.msn.com/lccn/ 

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------------------------------

Date: Thu, 31 Oct 2002 15:40:00 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Adapting files to run with -so

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>  After reading your mail,I have some general questions about the sequence
> of runsp with SO or (and)ORB, I hope can get your help or advice.

One cannot make general statements about these questions. It depends on
your system which method is the proper one. You must know the physics and
decide wether SO and/or orbital fields should be small corrections or big
effects!!!

In general it is true, that already for spinpolarized calculations without
SO or orb.fields several scf solutions COULD occur (NOT WILL).

It is even more true when SO and/or orbital fields are included.

In particular, scf solution with orbital potentials depend often (NOT ALWAYS)
on the starting density (i.e. an orbital A which is less populated then
orbital B  will usually be even less populated when -orb is added. So when
you start the scf cycle with two densites, one with more A and the other with
more B, there are good chances that you end up with two different scf
solutions - check E-tot)

>   1 : when runsp+SO , is there any difference between the two kinds of
> sequences list below:
>
>      a: init_lapw
>         initso_lapw-->accept the files it generated
>         runsp_lapw -so
>
>      b:the methods recommanded in the UG:
>         run[sp]_lapw --->
>         after convergence, then save_lapw
>         initso_lapw
>         run[sp]_lapw -so

I would always do b) (maybe just because I also want to see the differences
between so and no so).


>   2:when runsp+ORB, is there any difference between the two kinds of
> sequences list below:
>
>     a:init_lapw
>       edit case.indm(c),inorb by hand
>       runsp_lapw -orb
>
>     b:the method in your mail:
>       runsp
>       save_lapw
>       create inorb and indm-files
>       x lapwdm -up/dn  (to have a case.dmatup/dn file already in the first
> cycle)
>       runsp -orb

Again I would always do b). One can "hope", that LDA (better GGA) produces
at least the correct sequence of occupations, i.e. occupy orbital A slightly
more than B (e.g. 0.45 and 0.41), when the "correct" occupation including
orb is 0.8 and 0.06.


>  3: runsp+SO+ORB, is the sequence listed below is right?
>
>       init_lapw
>       initso_lapw -->accept the struct files it generated
>       edit case.indmc , case.inorb by hand
>       runsp_lapw -so -orb
>
>   is there any different sequence? If It also need to first runsp_lapw to
> achieve convergence, then save the result(like mentioned above), then
> runsp_lapw -so -orb?

Here the answer is most difficult. It depends a lot on the system and
which effects are dominating, wether it is metallic or should be an insulator
(but maybe is not in LDA,...).
For 3d elements, where SO is usually the "smallest" correction, I would most
likely do:

init
runsp
runsp -orb
runsp -orb -so

For 5f, where SO is very important, maybe one adds first SO and then -orb


Unfortunately for this advanced topic there is no black box solution.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 31 Oct 2002 15:16:00 -0500 (EST)
From: "G. Steinle-Neumann" <g.steinle-neumann@gl.ciw.edu>
Subject: [WIEN]: [WIEN] orbital moments (s-o)

====
"G. Steinle-Neumann" <g.steinle-neumann@gl.ciw.edu>
submitted the following contribution:
====


Dear all,

performing s-o calculations for a magnetic system I can't find the orbital
moments in any of the ouptut. Two questions:

(1) Is it there, and am I missing it?
(2) If not, where are they calculated, so I could get them output?

Many thanks, Gerd.

- -- 
Gerd Steinle-Neumann
Geophysical Laboratory * 5251 Broad Branch Rd., NW * Washington, DC 20015
phone +1-202-478-8943 * fax +1-202-478-8901 * g.steinle-neumann@gl.ciw.edu

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------------------------------

Date: Thu, 31 Oct 2002 21:26:38 +0100
From: Andres Cantarero <cantarer@netscape.net>
Subject: [WIEN]: question concerning parallel options??

====
Andres Cantarero <cantarer@netscape.net>
submitted the following contribution:
====

I installed the Wien2k version in a SGI. When I run the program it 
starts running several lapw1 processes in the same processor (iterative 
execution). Does anybody know how to eliminate this problem?
Thanks in advance.
Andres Cantarero

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------------------------------

Date: Fri, 01 Nov 2002 02:56:41 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: Re: [WIEN]: Adapting files to run with -so

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====

Dear Peter:
   Thank your instructive email,I think I have partly understood your 
meanning. That is to say, before add SO or(and)ORB, runsp_lapw first can 
creat at least qualitatively "correct" inintial configuration(especially 
for when ORB will be included),Is it right? . And I want to know , when I 
first runsp_lapw , is it necessary to convergence or just some cycles,like 
20 or 40 ,and so on?






>From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: <wien@zeus.theochem.tuwien.ac.at>
>Subject: Re: [WIEN]: Adapting files to run with -so
>Date: Thu, 31 Oct 2002 15:40:00 +0100 (MET)
>
>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
> >  After reading your mail,I have some general questions about the 
sequence
> > of runsp with SO or (and)ORB, I hope can get your help or advice.
>
>One cannot make general statements about these questions. It depends on
>your system which method is the proper one. You must know the physics and
>decide wether SO and/or orbital fields should be small corrections or big
>effects!!!
>
>In general it is true, that already for spinpolarized calculations without
>SO or orb.fields several scf solutions COULD occur (NOT WILL).
>
>It is even more true when SO and/or orbital fields are included.
>
>In particular, scf solution with orbital potentials depend often (NOT 
ALWAYS)
>on the starting density (i.e. an orbital A which is less populated then
>orbital B  will usually be even less populated when -orb is added. So when
>you start the scf cycle with two densites, one with more A and the other 
with
>more B, there are good chances that you end up with two different scf
>solutions - check E-tot)
>
> >   1 : when runsp+SO , is there any difference between the two kinds of
> > sequences list below:
> >
> >      a: init_lapw
> >         initso_lapw-->accept the files it generated
> >         runsp_lapw -so
> >
> >      b:the methods recommanded in the UG:
> >         run[sp]_lapw --->
> >         after convergence, then save_lapw
> >         initso_lapw
> >         run[sp]_lapw -so
>
>I would always do b) (maybe just because I also want to see the 
differences
>between so and no so).
>
>
> >   2:when runsp+ORB, is there any difference between the two kinds of
> > sequences list below:
> >
> >     a:init_lapw
> >       edit case.indm(c),inorb by hand
> >       runsp_lapw -orb
> >
> >     b:the method in your mail:
> >       runsp
> >       save_lapw
> >       create inorb and indm-files
> >       x lapwdm -up/dn  (to have a case.dmatup/dn file already in the 
first
> > cycle)
> >       runsp -orb
>
>Again I would always do b). One can "hope", that LDA (better GGA) produces
>at least the correct sequence of occupations, i.e. occupy orbital A 
slightly
>more than B (e.g. 0.45 and 0.41), when the "correct" occupation including
>orb is 0.8 and 0.06.
>
>
> >  3: runsp+SO+ORB, is the sequence listed below is right?
> >
> >       init_lapw
> >       initso_lapw -->accept the struct files it generated
> >       edit case.indmc , case.inorb by hand
> >       runsp_lapw -so -orb
> >
> >   is there any different sequence? If It also need to first runsp_lapw 
to
> > achieve convergence, then save the result(like mentioned above), then
> > runsp_lapw -so -orb?
>
>Here the answer is most difficult. It depends a lot on the system and
>which effects are dominating, wether it is metallic or should be an 
insulator
>(but maybe is not in LDA,...).
>For 3d elements, where SO is usually the "smallest" correction, I would 
most
>likely do:
>
>init
>runsp
>runsp -orb
>runsp -orb -so
>
>For 5f, where SO is very important, maybe one adds first SO and then -orb
>
>
>Unfortunately for this advanced topic there is no black box solution.
>
>Regards
>                                       P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: 
http://info.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
>====
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>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====

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Date: Fri, 01 Nov 2002 02:55:44 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: Re: [WIEN]: Adapting files to run with -so

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====

Dear Peter:
   Thank your instructive email,I think I have partly understood your 
meanning. That is to say, before add SO or(and)ORB, runsp_lapw first can 
creat at least quantitatively "correct" inintial configuration(especially 
for when ORB will be included),Is it right? . And I want to know , when I 
first runsp_lapw , is it necessary to convergence or just some cycles,like 
20 or 40 ,and so on?






>From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: <wien@zeus.theochem.tuwien.ac.at>
>Subject: Re: [WIEN]: Adapting files to run with -so
>Date: Thu, 31 Oct 2002 15:40:00 +0100 (MET)
>
>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
> >  After reading your mail,I have some general questions about the 
sequence
> > of runsp with SO or (and)ORB, I hope can get your help or advice.
>
>One cannot make general statements about these questions. It depends on
>your system which method is the proper one. You must know the physics and
>decide wether SO and/or orbital fields should be small corrections or big
>effects!!!
>
>In general it is true, that already for spinpolarized calculations without
>SO or orb.fields several scf solutions COULD occur (NOT WILL).
>
>It is even more true when SO and/or orbital fields are included.
>
>In particular, scf solution with orbital potentials depend often (NOT 
ALWAYS)
>on the starting density (i.e. an orbital A which is less populated then
>orbital B  will usually be even less populated when -orb is added. So when
>you start the scf cycle with two densites, one with more A and the other 
with
>more B, there are good chances that you end up with two different scf
>solutions - check E-tot)
>
> >   1 : when runsp+SO , is there any difference between the two kinds of
> > sequences list below:
> >
> >      a: init_lapw
> >         initso_lapw-->accept the files it generated
> >         runsp_lapw -so
> >
> >      b:the methods recommanded in the UG:
> >         run[sp]_lapw --->
> >         after convergence, then save_lapw
> >         initso_lapw
> >         run[sp]_lapw -so
>
>I would always do b) (maybe just because I also want to see the 
differences
>between so and no so).
>
>
> >   2:when runsp+ORB, is there any difference between the two kinds of
> > sequences list below:
> >
> >     a:init_lapw
> >       edit case.indm(c),inorb by hand
> >       runsp_lapw -orb
> >
> >     b:the method in your mail:
> >       runsp
> >       save_lapw
> >       create inorb and indm-files
> >       x lapwdm -up/dn  (to have a case.dmatup/dn file already in the 
first
> > cycle)
> >       runsp -orb
>
>Again I would always do b). One can "hope", that LDA (better GGA) produces
>at least the correct sequence of occupations, i.e. occupy orbital A 
slightly
>more than B (e.g. 0.45 and 0.41), when the "correct" occupation including
>orb is 0.8 and 0.06.
>
>
> >  3: runsp+SO+ORB, is the sequence listed below is right?
> >
> >       init_lapw
> >       initso_lapw -->accept the struct files it generated
> >       edit case.indmc , case.inorb by hand
> >       runsp_lapw -so -orb
> >
> >   is there any different sequence? If It also need to first runsp_lapw 
to
> > achieve convergence, then save the result(like mentioned above), then
> > runsp_lapw -so -orb?
>
>Here the answer is most difficult. It depends a lot on the system and
>which effects are dominating, wether it is metallic or should be an 
insulator
>(but maybe is not in LDA,...).
>For 3d elements, where SO is usually the "smallest" correction, I would 
most
>likely do:
>
>init
>runsp
>runsp -orb
>runsp -orb -so
>
>For 5f, where SO is very important, maybe one adds first SO and then -orb
>
>
>Unfortunately for this advanced topic there is no black box solution.
>
>Regards
>                                       P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: 
http://info.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====

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------------------------------

Date: Fri, 01 Nov 2002 03:24:20 +0000
From: ecat@nfrn-mail.org.uk
Subject: [WIEN]: Stop in lapw1up

====
ecat@nfrn-mail.org.uk
submitted the following contribution:
====

Dear all,

I am a new user of wien2k. When I ran runsp_lapw for the first
time, it stopped in the second cycle. When I changed the mixing
parameter in case.inm from 0.4 to 0.1, it stopped again in the
eleventh cycle. What was written in uplapw1.error is:

 'SELECT' - no energy limits found for L= 1
 'SELECT' - E-bottom -200.00000   E-top   -1.31500

I don't know what to do know.Could you tell me how to solve this
problem,please? Thanks!

Yours,
Ecat


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------------------------------

Date: Fri, 1 Nov 2002 10:37:54 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Stop in lapw1up

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> I am a new user of wien2k. When I ran runsp_lapw for the first
> time, it stopped in the second cycle. When I changed the mixing
> parameter in case.inm from 0.4 to 0.1, it stopped again in the
> eleventh cycle. What was written in uplapw1.error is:
>
>  'SELECT' - no energy limits found for L= 1
>  'SELECT' - E-bottom -200.00000   E-top   -1.31500
>
> I don't know what to do know.Could you tell me how to solve this
> problem,please? Thanks!
You would keep 0.1 and add -in1new 5 to your run to linearize the energies
to get ride of that error: run -in1new 5 -cc 0.00001 -i 99 ... .
        Your,
        Saeid.

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------------------------------

Date: Fri, 1 Nov 2002 10:57:41 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: [WIEN] orbital moments (s-o)

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> performing s-o calculations for a magnetic system I can't find the orbital
> moments in any of the ouptut. Two questions:
>
> (1) Is it there, and am I missing it?
Did you miss -orb?  To get orbital moment one must use orbital dependent
potential(s) including spin-orbit coupling: runsp_lapw -so -orb.
> (2) If not, where are they calculated, so I could get them output?
Please, inspect now the output of lapwdm program or .scf.
        Your,
        Saeid.




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------------------------------

Date: Fri, 01 Nov 2002 09:04:41 +0100
From: Thomas Claesson <tcl@kth.se>
Subject: Re: [WIEN]: Adapting files to run with -so

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Peter, thanks for your answer!

Peter Blaha wrote:

>
>If you have problems with LDA+U convergence for NiO, you will also have
>these problems when adding SO. NiO converges reasonably quick using LDA+U
>starting from a scf LDA (GGA) calculation.
>
>You do something wrong there!
>
Perhaps I do, but what? Could anyone help me out and find my mistake? I 
have been using RKmax = 7.0 and a k-mesh of up to 800 k-points in the 
entire BZ.
These are the input files I am using:

NiO.struct:
NiO                                                                            

R   LATTICE,NONEQUIV. ATOMS: 
3                                                
MODE OF 
CALC=RELA                                                             
  5.605236  5.605236 27.459934 90.000000 90.000000 
90.000000                  
ATOM= -1: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT= 4
Ni1        NPT=  781  R0=0.00050000 RMT=    2.0000   Z: 
28.0                  
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -2: X=0.50000000 Y=0.50000000 Z=0.50000000
          MULT= 1          ISPLIT= 4
Ni2        NPT=  781  R0=0.00050000 RMT=    2.0000   Z: 
28.0                  
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -3: X=0.25000000 Y=0.25000000 Z=0.25000000
          MULT= 2          ISPLIT= 4
      -3: X=0.75000000 Y=0.75000000 Z=0.75000000
O          NPT=  781  R0=0.00050000 RMT=    1.7500   Z:  
8.0                  
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
  12      NUMBER OF SYMMETRY OPERATIONS


Nio.inst:
Ni
Ar 3 5
3, 2,3.0  N
3, 2,1.0  N
3,-3,2.0  N
3,-3,2.0  N
4,-1,1.0  N
4,-1,1.0  N
Ni
Ar 3 5
3, 2,2.0  N
3, 2,2.0  N
3,-3,3.0  N
3,-3,1.0  N
4,-1,1.0  N
4,-1,1.0  N
O
He 3 5
2,-1,1.0  N
2,-1,1.0  N
2, 1,1.0  N
2, 1,1.0  N
2,-2,1.0  N
2,-2,1.0  N
****
****         END of input (instgen_lapw)

Nio.in1:
WFFIL        (WFPRI, SUPWF)
  7.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  0.30    4  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global 
APW/LAPW)
 1    0.30      0.000 CONT 1
 1   -4.96      0.005 STOP 1
 2    0.30      0.010 CONT 1
 0    0.30      0.000 CONT 1
  0.30    4  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global 
APW/LAPW)
 1    0.30      0.000 CONT 1
 1   -4.96      0.005 STOP 1
 2    0.30      0.010 CONT 1
 0    0.30      0.000 CONT 1
  0.30    3  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global 
APW/LAPW)
 0   -1.55      0.010 CONT 1
 0    0.30      0.000 CONT 1
 1    0.30      0.000 CONT 1
K-VECTORS FROM UNIT:4   -7.0       1.5      emin/emax window

Nio.indm:
- -9.
2
1 1 2
2 1 2
0 0

Nio.inorb:
1 2 0
PRATT, 1.0
1 1 2
2 1 2
1
0.59 0.07
0.59 0.07

Any suggestions are welcome! Thanks for your replies!

Best regards,
Thomas Claesson

>
>>Do you have a spinpolarized case (and want to run symmetso) ? (y/N)y
>>FORTRAN STOP
>>2.370u 0.060s 0:02.98 81.5%    0+0k 0+0io 213pf+0w
>> A new structure for SO calculations has been created (_so).
>> If you commit it will create new  Nio.struct, in1(c), in2c, inc,
>> clmsum/up/dn, vspup/dn and vnsup/dn files. (Please SAVE any previous
>> calculations)
>>
>>NOTE: Files for -orb (Nio.indm(c),inorb,dmatup/dn) must be adapted manually
>>
>>My question concerns the last sentence. How should I adapt the files for
>>-orb? What changes must I do to the files I have been using before I
>>added SO coupling?
>>
>
>This depends on your case. For NiO probably nothing (exept that you need a
>case.indmc file instead of case.indm when SO is used)
>
>In other cases, atomic positions could split creating a new struct file
>(with more atoms) and then you must update those files.
>
>Regards
>
>                                      P.Blaha
>


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------------------------------

Date: Fri, 1 Nov 2002 16:39:21 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- --143914132-568929606-1036139961=:15194
Content-Type: TEXT/PLAIN; charset=US-ASCII

Dear all,

I would like to consult about the following problem. Actually, I have 
asked the similar question about .struct file. and wien97 generated 
.struct file with multipicity equals 52 to me last time. 
And now, I make an .struct file with 40 atom position and start the  
calculation. After nn, WIEN97 generates another .struct file to me.  
However, this generated .struct file has 43 atom position. Where is the 
problem? Actually, I have tried to delete the 3 repeated atom 
positions from the generated .struct file but it didn't work, too. The 
molecule that I am interested in is carbon nanotube (10,10) and the unit 
cell should be only 40 atoms.

The original inputed .struct file (1010.struct_init1 and 
1010.struct_init2 (I have tried with 2 different original .struct 
files)) and the generated .struct file (1010.struct)are both attached.

Thank you very much

Martin


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------------------------------

Date: Fri, 01 Nov 2002 15:37:23 +0000
From: Paula <pauhar@chem.gla.ac.uk>
Subject: [WIEN]: TETRA segmentation fault

====
Paula <pauhar@chem.gla.ac.uk>
submitted the following contribution:
====

Dear wien users,

I have recently updated to wien2k and ran the 'TiC' example from UG to 
check for bugs. Using all the same inputs that l had for wien97 i have 
discovered that, though the scf calculation runs smoothly, when i try to 
calculate the DOS, TETRA produces a segmentation fault. Has anyone else had 
similar problems?

Paula

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------------------------------

Date: Fri, 01 Nov 2002 16:33:21 CST
From: Yongbin Lee <yblee@iastate.edu>
Subject: Re: [WIEN]: SRC_lapw2/outp.f 

====
Yongbin Lee <yblee@iastate.edu>
submitted the following contribution:
====

> Please try simply:
>
> cat TEST.normsoup_1 TEST.normsoup_2 TEST.normsoup_3 ... > TEST.normsoup
>
> And test the up and dn-spin DOS (it should look similar to the non-SO DOS).
>
> If this works I will put it into the lapwso_para script.
>

  It seems to work. Thank you !
  I put it into the lapw2c_para script ( "qtl" calculation
routine)

  Another quick question.
  Is it possible "lapwso" has seriously smaller matrix
size (about 3 times) than "lapw1" has?
  Does "lapwso" routine(WIEN2k) have parameters which 
can handle matrix size?

    WIEN97 

  lapw1(scf1)   
  :RKM  : MATRIX SIZE 3267LOs: 120  RKM= 7.00  WEIGHT= 8.00  PGR: 
  lapwso(scfso) 
  MATRIX SIZE= 3267   WEIGHT= 8.00

    WIEN2k
  lapw1(scf1)  
  :RKM  : MATRIX SIZE 3690LOs: 544  RKM= 7.00  WEIGHT= 8.00
  lapwso  
  MATRIX SIZE= 1059   WEIGHT= 8.00

   Thank you again
    
    Yongbin




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Date: Sun, 3 Nov 2002 14:51:29 +0100 (CET)
From: =?iso-8859-1?q?youcef=20cherchab?= <cherchab@yahoo.fr>
Subject: [WIEN]: optical properties

====
=?iso-8859-1?q?youcef=20cherchab?= <cherchab@yahoo.fr>
submitted the following contribution:
====

Dear wien _user
I would like to consult about the following problem .
When i try to calculate optical properties ,step by
step Iget some messages like this in LAPW2(weight
writen statement executed)and in step X JOINT (fault
segmentation ,core demped)
I can't resolve this case ,any suggestion are welcome.
thanks for yours hep.

your cherchab 

___________________________________________________________
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------------------------------

Date: Sun, 3 Nov 2002 15:11:04 +0100 (MET)
From: Gilles Hug <hug@onera.fr>
Subject: Re: [WIEN]: optical properties

====
Gilles Hug <hug@onera.fr>
submitted the following contribution:
====



Hi,
I think the segmentation fault deals with memory allocation.
Either joint is not compiled with enough memory or you don't have the
correct compilation options for your system.
Check with someone with same architecture.
Gilles

On Sun, 3 Nov 2002, [iso-8859-1] youcef cherchab wrote:

> ====
> =?iso-8859-1?q?youcef=20cherchab?= <cherchab@yahoo.fr>
> submitted the following contribution:
> ====
>
> Dear wien _user
> I would like to consult about the following problem .
> When i try to calculate optical properties ,step by
> step Iget some messages like this in LAPW2(weight
> writen statement executed)and in step X JOINT (fault
> segmentation ,core demped)
> I can't resolve this case ,any suggestion are welcome.
> thanks for yours hep.
>
> your cherchab
>
> ___________________________________________________________
> Do You Yahoo!? -- Une adresse @yahoo.fr gratuite et en français !
> Yahoo! Mail : http://fr.mail.yahoo.com
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

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------------------------------

Date: Mon, 4 Nov 2002 08:43:15 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: TETRA segmentation fault

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Hi Paula,

on one of my machines, tetra produces core dumps when it is compiled with
lxdos=3 (even when called with isplit different from 88 or 99).  On other
machines, compiling exactly the same source files gives me well-behaving
executables.  Maybe it's something compiler-dependent, I really don't have a
clue (on the one machine I use f90, on the others ifc/pgi).

I hope you'll work it out,

Kevin.
kevin.jorissen@ua.ac.be


- ----- Original Message -----
From: "Paula" <pauhar@chem.gla.ac.uk>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Friday, November 01, 2002 4:37 PM
Subject: [WIEN]: TETRA segmentation fault

> Paula <pauhar@chem.gla.ac.uk>
> submitted the following contribution:
> ====
>
> Dear wien users,
>
> I have recently updated to wien2k and ran the 'TiC' example from UG to
> check for bugs. Using all the same inputs that l had for wien97 i have
> discovered that, though the scf calculation runs smoothly, when i try to
> calculate the DOS, TETRA produces a segmentation fault. Has anyone else
had
> similar problems?
>
> Paula
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

====
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------------------------------

Date: Mon, 4 Nov 2002 16:14:46 +0800
From: "Wenhui Xie" <xiewh@sun20.iphy.ac.cn>
Subject: [WIEN]: Fortran stop SECLR4 - ERROR

====
"Wenhui Xie" <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear all,

I meet a quite strange error messages.
the program stop at first lapw1dn cycle and give a error message:
Cholesky INFO =      231
"SECLR4' - POTRF (Scalapack/LAPCK) failed

What's wrong with it?

Best Regards.

Wenhui_xie



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Date: Mon, 04 Nov 2002 17:33:22 +0900
From: Kodama <aojiru@hiroshima-u.ac.jp>
Subject: [WIEN]: Si bandstructure

====
Kodama <aojiru@hiroshima-u.ac.jp>
submitted the following contribution:
====


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Dear Wien users,

I am interested in the bandstructure of SiGe and SiC alloys.
I tried to calculate the bandstructure of Si using P lattice (
structure file is attached in this mail).

The bandstructure using P lattice has some strange bands that 
don't exist in normal Si bandstructure. These bands do not 
disappear by changing some parameters (number of k, Rmt, El). I 
don't know the origin of these bands.

Is this calculate wrong? Please give me some advices.

Thank you very much your help.

Hiroyuki Kodama

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- --------------Boundary_:sTbpsx--
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------------------------------

Date: Mon, 04 Nov 2002 09:33:22 +0100
From: Thomas Claesson <tcl@kth.se>
Subject: Re: [WIEN]: TETRA segmentation fault

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Paula

Actually I had similar problems with tetra a while ago. In my case there 
was a problem with the case.int file I was using. When I copied the 
case.int file from the SRC_templates directory and made my modifications 
to it, the problem disappeared.

Best regards,
Thomas Claesson

Paula wrote:

> ====
> Paula <pauhar@chem.gla.ac.uk>
> submitted the following contribution:
> ====
>
> Dear wien users,
>
> I have recently updated to wien2k and ran the 'TiC' example from UG to 
> check for bugs. Using all the same inputs that l had for wien97 i have 
> discovered that, though the scf calculation runs smoothly, when i try 
> to calculate the DOS, TETRA produces a segmentation fault. Has anyone 
> else had similar problems?
>
> Paula
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====




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------------------------------

Date: Mon, 4 Nov 2002 10:34:56 +0100
From: =?iso-8859-1?Q?Anders_Fr=F8seth?= <anders.froseth@phys.ntnu.no>
Subject: [WIEN]: This_file_should_not_exist

====
=?iso-8859-1?Q?Anders_Fr=F8seth?= <anders.froseth@phys.ntnu.no>
submitted the following contribution:
====

Dear wien users!

When running one of my cases in parallel 
I get files with the names "This_file_should_not_exist".
Can anyone tell me what this means?

Anders F.
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------------------------------

Date: Mon, 4 Nov 2002 12:09:04 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: SRC_lapw2/outp.f 

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>   Is it possible "lapwso" has seriously smaller matrix
> size (about 3 times) than "lapw1" has?

Yes of course. This is the "normal" way.
lapwso uses "second variation", i.e. its basis functions are the eigenfunctions
of lapw1 and usually your calculate them only in a small energy window.

In your WIEN97 example below you calculated ALL eigenvalues !! which is
timeconsuming and not the usual way.

In WIEN2k you restrict the energy window in case.in1 (last "regular" line).


>   Does "lapwso" routine(WIEN2k) have parameters which
> can handle matrix size?
>
>     WIEN97
>
>   lapw1(scf1)
>   :RKM  : MATRIX SIZE 3267LOs: 120  RKM= 7.00  WEIGHT= 8.00  PGR:
>   lapwso(scfso)
>   MATRIX SIZE= 3267   WEIGHT= 8.00
>
>     WIEN2k
>   lapw1(scf1)
>   :RKM  : MATRIX SIZE 3690LOs: 544  RKM= 7.00  WEIGHT= 8.00
>   lapwso
>   MATRIX SIZE= 1059   WEIGHT= 8.00

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 4 Nov 2002 19:13:51 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: optics

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

Actually, I got some very reasonable optical spectra from WIEN97 and I 
tried to increase the number of k-point in order to test the convergence  
of the spectra. Then, the spectra look very similiar. Suddenly, the 
spectrum become unreasonable when the number of k-point increased to 
around 1000. Is there any limit for the number of k-point for different 
unit-cell?

Thank you very much

Martin

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------------------------------

Date: Mon, 4 Nov 2002 12:26:04 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Fortran stop SECLR4 - ERROR

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I meet a quite strange error messages.
> the program stop at first lapw1dn cycle and give a error message:
> Cholesky INFO =      231
> "SECLR4' - POTRF (Scalapack/LAPCK) failed
>
> What's wrong with it?

Most likely your struct file.
Double definition of atoms,.... ?

Or unreasonable input parameters ? (RKMAX>10 ?)

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 4 Nov 2002 12:29:23 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Stop in lapw1up

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I am a new user of wien2k. When I ran runsp_lapw for the first
> time, it stopped in the second cycle. When I changed the mixing
> parameter in case.inm from 0.4 to 0.1, it stopped again in the
> eleventh cycle. What was written in uplapw1.error is:
>
>  'SELECT' - no energy limits found for L= 1
>  'SELECT' - E-bottom -200.00000   E-top   -1.31500
>
> I don't know what to do know.Could you tell me how to solve this
> problem,please? Thanks!

Do:
grep :DIS case.scf

Is the "distance" converging ? or (I believe) diverging ?

When you have a difficult case it could be that you need an even smaller
value in case.inm

Just do the same as the first time, but reduce mixing further.

(Of course also other reasons might be possible,...
(grep :NEC01 case.scf  )

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 4 Nov 2002 15:42:57 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: question concerning parallel options??

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I installed the Wien2k version in a SGI. When I run the program it
> starts running several lapw1 processes in the same processor (iterative
> execution). Does anybody know how to eliminate this problem?

I don't know if this is a problem or not.

Is your SGI a shared memory machine or a cluster of machines ?

What did you specify during installation ?

What did you put into your   .machines file ?

If you put 3 lines with "localhost" it will of course span 3 lapw1 on the
"local host".
If you put
1:sgi1
1:sgi2
1:sgi3

it will create 3 jobs (with rsh or ssh (unless you said shared memory!!))
on the 3 computers with names scg1, sgi2 sgi3.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 4 Nov 2002 15:37:14 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: [WIEN] orbital moments (s-o)

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> performing s-o calculations for a magnetic system I can't find the orbital
> moments in any of the ouptut. Two questions:
>
> (1) Is it there, and am I missing it?
> (2) If not, where are they calculated, so I could get them output?

The orbital moment is calculated in    lapwdm, which is not called
during    runsp -so.

I added recently a switch  -dm, so that also the orbital moment is calculated
during scf. You need an input file    case.indmc    and use
  runsp -so -dm     (But you need a recent version or update from www.wien2k.at!)


Of course one can always calculate the orbital moment after scf using the
same program  lapwdm.



(Only in case of   runsp -so -orb  the orbital moment will always be
calculated during scf.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

====
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------------------------------

Date: Mon, 4 Nov 2002 15:52:51 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Adapting files to run with -so

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> >You do something wrong there!
> >
> Perhaps I do, but what? Could anyone help me out and find my mistake? I
> have been using RKmax = 7.0 and a k-mesh of up to 800 k-points in the
> entire BZ.
> Nio.inst:
> Ni
> Ar 3 5
> 3, 2,3.0  N             an occupation of 3 is not possible for kappa=2
> 3, 2,1.0  N             But besides that, you define a spin of +2 in the
> 3,-3,2.0  N             Ni-3d(3/2) orbital
> 3,-3,2.0  N
> 4,-1,1.0  N
> 4,-1,1.0  N
> Ni
> Ar 3 5
> 3, 2,2.0  N
> 3, 2,2.0  N
> 3,-3,3.0  N            here you have again a spin of +2 !!!, but now in the
> 3,-3,1.0  N             Ni-3d(5/2) orbital
> 4,-1,1.0  N
> 4,-1,1.0  N

You want an AF start, so you must flip the spin. Aparently you tried that,
but with this inst file it can't work and I think even lstart must have
complained ?

A reasonable inst file starts with:

Ni
Ar 3 5
3, 2,2.0  N
3, 2,2.0  N
3,-3,3.0  N
3,-3,1.0  N
4,-1,1.0  N
4,-1,1.0  N
Ni
Ar 3 5
3, 2,2.0  N
3, 2,2.0  N
3,-3,1.0  N
3,-3,3.0  N
4,-1,1.0  N
4,-1,1.0  N

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

====
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Date: Mon, 4 Nov 2002 19:20:29 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Question

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---2105530234-1612954989-1036434029=:10223
Content-Type: TEXT/PLAIN; charset=US-ASCII

> I would like to consult about the following problem. Actually, I have
> asked the similar question about .struct file. and wien97 generated
> .struct file with multipicity equals 52 to me last time.
> And now, I make an .struct file with 40 atom position and start the
> calculation. After nn, WIEN97 generates another .struct file to me.
> However, this generated .struct file has 43 atom position. Where is the
> problem? Actually, I have tried to delete the 3 repeated atom
> positions from the generated .struct file but it didn't work, too. The
> molecule that I am interested in is carbon nanotube (10,10) and the unit
> cell should be only 40 atoms.
>
> The original inputed .struct file (1010.struct_init1 and
> 1010.struct_init2 (I have tried with 2 different original .struct
> files)) and the generated .struct file (1010.struct)are both attached.

I can hardly believe your report, that a new struct file with 43 atoms has
been generated.

WIEN2k has no problems with your structure.

I started with  1010.struct_init1 and both, nn and sgroup are able to
split your 40 atoms into 10x4 atoms without "adding" atoms to the unitcell!!!

I suggest you register for WIEN2k.



                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Content-Description: 
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- ---2105530234-1612954989-1036434029=:10223--
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------------------------------

Date: Mon, 4 Nov 2002 19:25:09 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Si bandstructure

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

On Mon, 4 Nov 2002, Kodama wrote:

> Dear Wien users,
>
> I am interested in the bandstructure of SiGe and SiC alloys.
> I tried to calculate the bandstructure of Si using P lattice (
> structure file is attached in this mail).
>
> The bandstructure using P lattice has some strange bands that
> don't exist in normal Si bandstructure. These bands do not
> disappear by changing some parameters (number of k, Rmt, El). I
> don't know the origin of these bands.

You did the calculation in a supercell without symmetry!!!

Did you use the complex versions of the program (do you have a Si.in1c file
or Si.in1 ???)

You know that with this supercell you will find all the backfolded bands,...
so a direct comparison with FCC Si is not so trivial.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 4 Nov 2002 19:54:52 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: This_file_should_not_exist

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> When running one of my cases in parallel
> I get files with the names "This_file_should_not_exist".
> Can anyone tell me what this means?

Don't worry, you can forget about this file.

It is created by sumpara as default when you do not have *dmat* files

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 5 Nov 2002 11:29:30 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: Re: [WIEN]: Question

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Prof. P.Blaha,

Thank you very much for your reply. 
However, I really have tried the .struct files in different machines and I
really get the wrong .struct file from WIEN97. Would you mind trying the 
files I sent to you last time with WIEN97 again? If it works with your 
WIEN97, then I would uninstall my WIEN97 and re-install it again to see whether 
it works or not. (actually, I have already uninstalled WIEN97 and re-installed 
it and try the files but it doesn't work)

Thank you very much

Martin

On Mon, 4 Nov 2002, Peter Blaha wrote:

> > I would like to consult about the following problem. Actually, I have
> > asked the similar question about .struct file. and wien97 generated
> > .struct file with multipicity equals 52 to me last time.
> > And now, I make an .struct file with 40 atom position and start the
> > calculation. After nn, WIEN97 generates another .struct file to me.
> > However, this generated .struct file has 43 atom position. Where is the
> > problem? Actually, I have tried to delete the 3 repeated atom
> > positions from the generated .struct file but it didn't work, too. The
> > molecule that I am interested in is carbon nanotube (10,10) and the unit
> > cell should be only 40 atoms.
> >
> > The original inputed .struct file (1010.struct_init1 and
> > 1010.struct_init2 (I have tried with 2 different original .struct
> > files)) and the generated .struct file (1010.struct)are both attached.
> 
> I can hardly believe your report, that a new struct file with 43 atoms has
> been generated.
> 
> WIEN2k has no problems with your structure.
> 
> I started with  1010.struct_init1 and both, nn and sgroup are able to
> split your 40 atoms into 10x4 atoms without "adding" atoms to the unitcell!!!
> 
> I suggest you register for WIEN2k.
> 
> 
> 
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
> 
- ----------------------------------------------------------------------------

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------------------------------

Date: Mon, 4 Nov 2002 22:24:58 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: L2main problem again

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---559023410-851401618-1036470298=:2334
Content-Type: TEXT/PLAIN; charset=US-ASCII

Dear all:

I met the "L2main problem" in running lapw2 for my new crystal with EFG in
case.in2 again.
This time my crystal is in tetragonal symmetry (I4), the lapw2.error
contains the following line as that for my monoclinic symmetry crytal:

'l2main' - NEFG.GT.23.

Could you please give me some instructions about it?

Thanks!


Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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Date: Tue, 05 Nov 2002 08:54:48 +0100
From: Thomas Claesson <tcl@kth.se>
Subject: Re: [WIEN]: Adapting files to run with -so

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Thanks for your reply, Peter!

So what should I look for in case.outputst and case.scf in order to know 
that I get an AF start? :MMIxx?

Best regards,
Thomas Claesson

Peter Blaha wrote:
> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> 
>>>You do something wrong there!
>>>
>>
>>Perhaps I do, but what? Could anyone help me out and find my mistake? I
>>have been using RKmax = 7.0 and a k-mesh of up to 800 k-points in the
>>entire BZ.
>>Nio.inst:
>>Ni
>>Ar 3 5
>>3, 2,3.0  N             an occupation of 3 is not possible for kappa=2
>>3, 2,1.0  N             But besides that, you define a spin of +2 in the
>>3,-3,2.0  N             Ni-3d(3/2) orbital
>>3,-3,2.0  N
>>4,-1,1.0  N
>>4,-1,1.0  N
>>Ni
>>Ar 3 5
>>3, 2,2.0  N
>>3, 2,2.0  N
>>3,-3,3.0  N            here you have again a spin of +2 !!!, but now in the
>>3,-3,1.0  N             Ni-3d(5/2) orbital
>>4,-1,1.0  N
>>4,-1,1.0  N
> 
> 
> You want an AF start, so you must flip the spin. Aparently you tried that,
> but with this inst file it can't work and I think even lstart must have
> complained ?
> 
> A reasonable inst file starts with:
> 
> Ni
> Ar 3 5
> 3, 2,2.0  N
> 3, 2,2.0  N
> 3,-3,3.0  N
> 3,-3,1.0  N
> 4,-1,1.0  N
> 4,-1,1.0  N
> Ni
> Ar 3 5
> 3, 2,2.0  N
> 3, 2,2.0  N
> 3,-3,1.0  N
> 3,-3,3.0  N
> 4,-1,1.0  N
> 4,-1,1.0  N
> 
> Regards
> 
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
> 
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------------------------------

Date: Tue, 05 Nov 2002 12:44:33 +0100
From: Sabine Wurmehl <wurmehl@uni-mainz.de>
Subject: [WIEN]: Data

====
Sabine Wurmehl <wurmehl@uni-mainz.de>
submitted the following contribution:
====

Dear Wien-users,

I have calculated some DOS in postscript format. Now i would like to
import the ouput-data in origin or excel.  Can you help me?

Thanks S.Wurmehl
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Date: Tue, 05 Nov 2002 12:49:23 +0100
From: Sabine Wurmehl <wurmehl@uni-mainz.de>
Subject: [WIEN]: magnetic moments

====
Sabine Wurmehl <wurmehl@uni-mainz.de>
submitted the following contribution:
====

Dear Wien-users,

The magnetic moment of the complete cell is written in scf-file. Does
the programm  also calculate the magnetic moments of the single atoms
and if, in which file can i find these values?

Thanks S.Wurmehl
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Date: Tue, 05 Nov 2002 12:53:58 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: magnetic moments

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

They are given for all atoms in the scf file... look for :CHA01, etc.

Best regards,
Torsten Andersen.

Sabine Wurmehl wrote:

>====
>Sabine Wurmehl <wurmehl@uni-mainz.de>
>submitted the following contribution:
>====
>
>Dear Wien-users,
>
>The magnetic moment of the complete cell is written in scf-file. Does
>the programm  also calculate the magnetic moments of the single atoms
>and if, in which file can i find these values?
>
>Thanks S.Wurmehl
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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Date: Tue, 05 Nov 2002 13:35:25 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: magnetic moments

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Oops, sorry, I believe it should be :MMI01, etc.

Best,
Torsten.

Torsten Andersen wrote:

> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
>
> They are given for all atoms in the scf file... look for :CHA01, etc.
>
> Best regards,
> Torsten Andersen.
>
> Sabine Wurmehl wrote:
>
>> ====
>> Sabine Wurmehl <wurmehl@uni-mainz.de>
>> submitted the following contribution:
>> ====
>>
>> Dear Wien-users,
>>
>> The magnetic moment of the complete cell is written in scf-file. Does
>> the programm  also calculate the magnetic moments of the single atoms
>> and if, in which file can i find these values?
>>
>> Thanks S.Wurmehl
>> ====
>> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>> To (un)subscribe send mail to
>> majordomo@zeus.theochem.tuwien.ac.at
>> ====
>>
>>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Tue, 5 Nov 2002 17:50:27 +0400 (SAMT)
From: Lyudmila Dobysheva <lyu@otf.fti.udmurtia.su>
Subject: Re: [WIEN]: Adapting files to run with -so

====
Lyudmila Dobysheva <lyu@otf.fti.udmurtia.su>
submitted the following contribution:
====

On Tue, 5 Nov 2002, Thomas Claesson wrote:

> So what should I look for in case.outputst and case.scf in order to know 
> that I get an AF start? :MMIxx?

> >>Perhaps I do, but what? Could anyone help me out and find my mistake? I
> >>have been using RKmax = 7.0 and a k-mesh of up to 800 k-points in the
> >>entire BZ.

Dear Thomas,

Couldn't it be that you have a mistake in inso file? If you take the
magnetization direction 001 in NiO with its Rhombohedral lattice you'll
get such errors.

Best regards
  Lyudmila Dobysheva 
- ------------------------------------------------------------------------
Phys.-Techn. Institute of            |   Tel.(home):   7 (3412) 442118
Ural Branch of Russian Ac. of Sci.   |   Tel.(office): 7 (3412) 218988
426001 Izhevsk, ul.Kirova 132        |   Fax:          7 (3412) 250614
RUSSIA                               |   E-mail: lyu@otf.fti.udmurtia.su
- ------------------------------------------------------------------------
http://fti.udm.ru/ltt/personals/dobysh.htm
- ------------------------------------------------------------------------

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------------------------------

Date: Tue,  5 Nov 2002 14:36:09 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: magnetic moments

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
> 
> Oops, sorry, I believe it should be :MMI01, etc.
> 

In addition to that: be careful when interpreting these values. This is the 
(spin) magnetic moment for each atom inside its muffin tin sphere, and 
therefore this value does depend on the sphere size. The moment in the 
interstitial region is given in :MMI, but that value cannot be attributed to 
any specific atom. These values are therefore always arbitrary to some degree, 
unless you have something simple as bcc-Fe where the moment per atom is 
(:MMI01 + :MMI). But the same ambiguity exist in experiment: every measurement 
of a magnetic moment implicitely or explicitely has to define a boundary for 
the atom.

A way to divide the total unit cell in regions that unambiguously belong to one 
atom each -- and which hence give you a well-defined magnetic moment that does 
not depend on sphere size -- is by Bader analysis. However, this is just a 
convention as any other. There is no physics in it, but it is at least unique.

Stefaan
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------------------------------

End of wien-digest V2002 #41
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #42
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
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wien-digest       Wednesday, November 13 2002       Volume 2002 : Number 042




----------------------------------------------------------------------

Date: Tue,  5 Nov 2002 14:39:03 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: Data

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> Sabine Wurmehl <wurmehl@uni-mainz.de>
> submitted the following contribution:
> ====
> 
> I have calculated some DOS in postscript format. Now i would like to
> import the ouput-data in origin or excel.  Can you help me?

In excel: import the ascii-files case.dos* (or case.dos*ev) and create an 
excel-plot. Similarly for other spreadsheets or plotting programs. It might 
help to remove the firt few comment lines from case.dos*, such that only the 
data columns remain (some programs got confused by this).

Stefaan



====
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Date: Tue, 5 Nov 2002 05:56:37 -0800 (PST)
From: Claudio Lee <claudio_lee1@yahoo.com>
Subject: [WIEN]: error in OP calculation!

====
Claudio Lee <claudio_lee1@yahoo.com>
submitted the following contribution:
====

Hi all,
I'm calculating this spinpolarized Fe bcc as a test.
Using only "runsp_lapw -so" then the final result is
good. However, when  the orbital polarized -orb has
been taken into account,I got problem with the output.
With these two files *.indmc and *inorb were created, 
after running "runsp_lapw -so -orb" I got the result
with the errors appear in the *.err file.
The *.err file looks like:
=====
hup: Command not found.
STOP  LAPW0 END
STOP  LAPW1 END
STOP  LAPW1 END
STOP LAPWSO END
STOP  LAPW2 END
STOP  LAPW2 END
STOP  lapwdm END
1525-097 A READ statement using decimal base input
found the invalid digit '.' in the input file.  The
program will recover by assuming a zero in its place.
STOP  orbital potential calculation END
1525-097 A READ statement using decimal base input
found the invalid digit '.' in the input file.  The
program will recover by assuming a zero in its place.
STOP  orbital potential calculation END
STOP  CORE  END
STOP  CORE  END
STOP  MIXER END
hup: Command not found.
STOP  LAPW0 END
STOP  LAPW1 END
...
...
(repeat for number of iterations, and the error
appears after "lapwdm" has been executed).  
=====  
So I think it must be wrong somewhere in my input
files, *.indmc and *.inorb (or somewhere else?)
Here they are:
*.indmc:
- -9.0          Emin cutoff energy
 1            number of atoms for ...
 1  1  2      index of 1st atom, number of L's, L1
 0  0           r-index, (l,s)0index
- ---
*.inorb:
 2  1  0       nmod, natorb, ipr, amix
 BROYD 0.3      Broyden mixing 
  1  1  2       iatom, nlorb, lorb
  0             nmodop
  1             Ncalc
  1.  0.  0.    direction of M
 
If anyone knows what is wrong in my case please help
me.

Thank you in advance.

Claudio.




  


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Date: Tue, 5 Nov 2002 09:30:43 -0500
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: Data

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====

> I have calculated some DOS in postscript format. Now i would like to
> import the ouput-data in origin or excel.  Can you help me?

I believe the numerical data is in files like case.dos. You can import that 
data into another plotting program with minor editing.
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Date: Tue, 5 Nov 2002 23:41:12 -0800 (PST)
From: hamid salehi <salehihamid@yahoo.com>
Subject: Re: [WIEN]: magnetic moments

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear User
They are  found for all atoms in "SCF-FILE" look for
:CHAO1, CHAO2  ,  et
best wishes
H Salehi 
- --- Sabine Wurmehl <wurmehl@uni-mainz.de> wrote:
> ====
> Sabine Wurmehl <wurmehl@uni-mainz.de>
> submitted the following contribution:
> ====
> 
> Dear Wien-users,
> 
> The magnetic moment of the complete cell is written
> in scf-file. Does
> the programm  also calculate the magnetic moments of
> the single atoms
> and if, in which file can i find these values?
> 
> Thanks S.Wurmehl
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====


=====
Hamdollah Salehi
Dept of Physics
Ferdowsi University
Mashhad IRAN
Post boxs 1436
Post code 91775
faxs

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------------------------------

Date: Wed, 6 Nov 2002 10:13:46 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: error in OP calculation!

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

Did you use initso (with symmetso) ? (Reduced symmetry !!!??).

If not, also your -so calculation is wrong (although it might converge).


> I'm calculating this spinpolarized Fe bcc as a test.
> Using only "runsp_lapw -so" then the final result is
> good. However, when  the orbital polarized -orb has
> been taken into account,I got problem with the output.
> With these two files *.indmc and *inorb were created,
> after running "runsp_lapw -so -orb" I got the result
> with the errors appear in the *.err file.
> The *.err file looks like:
> =====
> hup: Command not found.
> STOP  LAPW0 END
> STOP  LAPW1 END
> STOP  LAPW1 END
> STOP LAPWSO END
> STOP  LAPW2 END
> STOP  LAPW2 END
> STOP  lapwdm END
> 1525-097 A READ statement using decimal base input
> found the invalid digit '.' in the input file.  The
> program will recover by assuming a zero in its place.
> STOP  orbital potential calculation END
> 1525-097 A READ statement using decimal base input
> found the invalid digit '.' in the input file.  The
> program will recover by assuming a zero in its place.
> STOP  orbital potential calculation END
> STOP  CORE  END
> STOP  CORE  END
> STOP  MIXER END
> hup: Command not found.
> STOP  LAPW0 END
> STOP  LAPW1 END
> ...
> ...
> (repeat for number of iterations, and the error
> appears after "lapwdm" has been executed).
> =====
> So I think it must be wrong somewhere in my input
> files, *.indmc and *.inorb (or somewhere else?)
> Here they are:
> *.indmc:
> -9.0          Emin cutoff energy
>  1            number of atoms for ...
>  1  1  2      index of 1st atom, number of L's, L1
>  0  0           r-index, (l,s)0index
> ---
> *.inorb:
>  2  1  0       nmod, natorb, ipr, amix
>  BROYD 0.3      Broyden mixing
>   1  1  2       iatom, nlorb, lorb
>   0             nmodop
>   1             Ncalc
>   1.  0.  0.    direction of M
>
> If anyone knows what is wrong in my case please help
> me.
>
> Thank you in advance.
>
> Claudio.
>
>
>
>
>
>
>
> __________________________________________________
> Do you Yahoo!?
> HotJobs - Search new jobs daily now
> http://hotjobs.yahoo.com/
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>


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Wed, 6 Nov 2002 03:38:21 -0800 (PST)
From: Claudio Lee <claudio_lee1@yahoo.com>
Subject: Re: [WIEN]: error in OP calculation!

====
Claudio Lee <claudio_lee1@yahoo.com>
submitted the following contribution:
====

Dear Peter,
Yes, I did.
After running initso (symmetry reduced from 48 to 16)I
have everything in order to calculate with runsp_lapw
- -so switch. The convergency in "runsp_lapw -so" is 
good, I mean, after the program has finished I have no
any errors in *err file.
And then I have problem (the errors eppear in *err
file) when I created two files *inorb and *.indmc
(following U.G) and run runsp_lapw -so -orb.
Thank you so much for any suggestions.
Claudio.

> Did you use initso (with symmetso) ? (Reduced
> symmetry !!!??).
> 
> If not, also your -so calculation is wrong (although
> it might converge).
> 
> 
> > I'm calculating this spinpolarized Fe bcc as a
> test.
> > Using only "runsp_lapw -so" then the final result
> is
> > good. However, when  the orbital polarized -orb
> has
> > been taken into account,I got problem with the
> output.
> > With these two files *.indmc and *inorb were
> created,
> > after running "runsp_lapw -so -orb" I got the
> result
> > with the errors appear in the *.err file.
> > The *.err file looks like:
> > =====
> > hup: Command not found.
> > STOP  LAPW0 END
> > STOP  LAPW1 END
> > STOP  LAPW1 END
> > STOP LAPWSO END
> > STOP  LAPW2 END
> > STOP  LAPW2 END
> > STOP  lapwdm END
> > 1525-097 A READ statement using decimal base input
> > found the invalid digit '.' in the input file. 
> The
> > program will recover by assuming a zero in its
> place.
> > STOP  orbital potential calculation END
> > 1525-097 A READ statement using decimal base input
> > found the invalid digit '.' in the input file. 
> The
> > program will recover by assuming a zero in its
> place.
> > STOP  orbital potential calculation END
> > STOP  CORE  END
> > STOP  CORE  END
> > STOP  MIXER END
> > hup: Command not found.
> > STOP  LAPW0 END
> > STOP  LAPW1 END
> > ...
> > ...
> > (repeat for number of iterations, and the error
> > appears after "lapwdm" has been executed).
> > =====
> > So I think it must be wrong somewhere in my input
> > files, *.indmc and *.inorb (or somewhere else?)
> > Here they are:
> > *.indmc:
> > -9.0          Emin cutoff energy
> >  1            number of atoms for ...
> >  1  1  2      index of 1st atom, number of L's, L1
> >  0  0           r-index, (l,s)0index
> > ---
> > *.inorb:
> >  2  1  0       nmod, natorb, ipr, amix
> >  BROYD 0.3      Broyden mixing
> >   1  1  2       iatom, nlorb, lorb
> >   0             nmodop
> >   1             Ncalc
> >   1.  0.  0.    direction of M
> >
> > If anyone knows what is wrong in my case please
> help
> > me.
> >
> > Thank you in advance.
> >
> > Claudio.
> >
> >
> >
> >
> >
> >
> >
> > __________________________________________________
> > Do you Yahoo!?
> > HotJobs - Search new jobs daily now
> > http://hotjobs.yahoo.com/
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
> > majordomo@zeus.theochem.tuwien.ac.at
> > ====
> >
> 
> 
>                                       P.Blaha
>
- --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna,
> A-1060 Vienna
> Phone: +43-1-58801-15671             FAX:
> +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
> http://info.tuwien.ac.at/theochem/
>
- --------------------------------------------------------------------------
> 
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------------------------------

Date: Tue, 05 Nov 2002 15:17:41 +0100
From: Peer Kruse <kruse@lem.uni-karlsruhe.de>
Subject: [WIEN]: Wien2k on PC: Error in lapw1

====
Peer Kruse <kruse@lem.uni-karlsruhe.de>
submitted the following contribution:
====

Dear Wien Users and developers,
I still have the Error in lapw1. As nobody seems to have an idea, I' d 
like to ask, if anyone is using
redhat 7.3 and/or newer Athlon processors without problems to exclude 
this possibility.

Thank you

Peer

> ====
> Peer Kruse <kruse@lem.uni-karlsruhe.de>
> submitted the following contribution:
> ====
>
> Dear Wien users and developers,
> I tried to install Wien2k on 2 rather new PC's and get an
> "Error in lapw1" after a period of about 2 hours.
> This happens only for a larger number of k points, eg >500,
> with only 50 it is working fine. I should have Memory in abundance
> (1BG) for my structure of 12 atoms (6 atoms inequivalent) nad the 
> memory is not used (in the first hour of the program at least).
> The limits are set to
>
> core file size (blocks, -c) 0
> data seg size (kbytes, -d) unlimited
> file size (blocks, -f) unlimited
> max locked memory (kbytes, -l) unlimited
> max memory size (kbytes, -m) unlimited
> open files (-n) 1024
> pipe size (512 bytes, -p) 8
> stack size (kbytes, -s) 32768
> cpu time (seconds, -t) unlimited
> max user processes (-u) 7168
> virtual memory (kbytes, -v) unlimited
> Is this ok?
>
> I compiled Wien2k with ifc and pgi, no difference, the same for the 
> precompiled version.
> I' m running linux redhat 7.3. And  it is running with the same 
> parameters/structures
> on the old and slow and even smaller machines with every kind of 
> architecture (dec, pc, notebook) without problem.
>
> Has anyone any experience or further ideas?
>
> Thank you
>
> Peer Kruse
>



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------------------------------

Date: Wed, 06 Nov 2002 15:34:02 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Wien2k on PC: Error in lapw1

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Mr. Kruse,

"Error in lapw1" is not much information. Wasn't there any additional 
information in the dayfile or the output files? Usually when lapw1 
crashes during runtime just by increasing the number of k-points, it has 
to do with memory. And usually, there is additional information in the 
dayfile and/or the screen output (on dec when run in background, the 
default file name here is nohup.out). Is NMATMAX big enough? Do you have 
swap space? On any of the mentioned systems? Did a core dump? Have you 
tried to increase the Stack size?

So that was a few ideas... I am pretty sure it has to do with your 
setup, not the code.

Best regards,
Torsten.

Peer Kruse wrote:

> ====
> Peer Kruse <kruse@lem.uni-karlsruhe.de>
> submitted the following contribution:
> ====
>
> Dear Wien Users and developers,
> I still have the Error in lapw1. As nobody seems to have an idea, I' d 
> like to ask, if anyone is using
> redhat 7.3 and/or newer Athlon processors without problems to exclude 
> this possibility.
>
> Thank you
>
> Peer
>
>> ====
>> Peer Kruse <kruse@lem.uni-karlsruhe.de>
>> submitted the following contribution:
>> ====
>>
>> Dear Wien users and developers,
>> I tried to install Wien2k on 2 rather new PC's and get an
>> "Error in lapw1" after a period of about 2 hours.
>> This happens only for a larger number of k points, eg >500,
>> with only 50 it is working fine. I should have Memory in abundance
>> (1BG) for my structure of 12 atoms (6 atoms inequivalent) nad the 
>> memory is not used (in the first hour of the program at least).
>> The limits are set to
>>
>> core file size (blocks, -c) 0
>> data seg size (kbytes, -d) unlimited
>> file size (blocks, -f) unlimited
>> max locked memory (kbytes, -l) unlimited
>> max memory size (kbytes, -m) unlimited
>> open files (-n) 1024
>> pipe size (512 bytes, -p) 8
>> stack size (kbytes, -s) 32768
>> cpu time (seconds, -t) unlimited
>> max user processes (-u) 7168
>> virtual memory (kbytes, -v) unlimited
>> Is this ok?
>>
>> I compiled Wien2k with ifc and pgi, no difference, the same for the 
>> precompiled version.
>> I' m running linux redhat 7.3. And  it is running with the same 
>> parameters/structures
>> on the old and slow and even smaller machines with every kind of 
>> architecture (dec, pc, notebook) without problem.
>>
>> Has anyone any experience or further ideas?
>>
>> Thank you
>>
>> Peer Kruse
>>
>
>
>
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>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Wed, 6 Nov 2002 14:48:13 -0500
From: "Dadi Dai" <dai@unity.ncsu.edu>
Subject: [WIEN]: w2web and Space Group #15

====
"Dadi Dai" <dai@unity.ncsu.edu>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_00F8_01C285A3.885FFA30
Content-Type: text/plain;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

I was using w2web to generate input files for NiP2 calculations.  The =
cell parameters that I have are: Spacegroup #15 C12/c1 (unique axis b, =
cell choice 1), a=3D6.500, b=3D5.628, c=3D6.156 A, and beta=3D127.07.

The w2web StructGen accepts only B2/b (unique axis a, cell choice 1) for =
space group 15.  Therefore, I changed the order sequence and let =
a=3D5.628, b=3D6.156, c=3D6.500, and alpha=3D127.07.  But the step "x =
sgroup" in "init" gave an error message: "alpha =3D 127.07 and not equal =
90.  Exiting now."

Did I misunderstand the symbol of space group #15 in w2web StuctGen or =
the order sequence of the cell parameters?

Thanks!

Dadi Dai

- ------=_NextPart_000_00F8_01C285A3.885FFA30
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2719.2200" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD><FONT face=3DArial><FONT size=3D2>
<BODY>
<DIV>I was using w2web to generate input files for NiP2 =
calculations.&nbsp; The=20
cell parameters that I have are: Spacegroup #15 C12/c1 (unique axis b, =
cell=20
choice 1), a=3D6.500, b=3D5.628, c=3D6.156 A, and beta=3D127.07.</DIV>
<DIV>&nbsp;</DIV>
<DIV>The w2web StructGen accepts only B2/b (unique axis a, cell choice =
1) for=20
space group 15.&nbsp; Therefore, I changed the order sequence and let =
a=3D5.628,=20
b=3D6.156, c=3D6.500, and alpha=3D127.07.&nbsp; But the step "x sgroup" =
in "init" gave=20
an error message: "alpha =3D 127.07 and not equal 90.&nbsp; Exiting =
now."</DIV>
<DIV>&nbsp;</DIV>
<DIV>Did I misunderstand the symbol of space group #15 in w2web StuctGen =
or the=20
order sequence of the cell parameters?</DIV>
<DIV>&nbsp;</DIV>
<DIV>Thanks!</DIV>
<DIV>&nbsp;</DIV>
<DIV>Dadi Dai</DIV></BODY></HTML></FONT></FONT>

- ------=_NextPart_000_00F8_01C285A3.885FFA30--

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------------------------------

Date: Thu, 7 Nov 2002 07:16:34 +0900 (KST)
From: Joo Yull Rhee <rheejy@office.hoseo.ac.kr>
Subject: Re:[WIEN]: Wien2k on PC: Error in lapw1

====
Joo Yull Rhee <rheejy@office.hoseo.ac.kr>
submitted the following contribution:
====

<HTML>
<HEAD>
<STYLE>P {margin-top:2px;margin-bottom:2px;}</STYLE>
</HEAD>

<BODY style="FONT-SIZE: 10pt; FONT-FAMILY: ±¼¸²"><P>Dear WIEN2k users,</P>
<P>&nbsp;</P>
<P>I want to share my experience with others who are using PC with AMD&nbsp; Athlon processors. I purchased 4 nodes of AMD Athlon Dual-processor&nbsp; machines last year. It kept failed. Initially I thought it was heat&nbsp; problem with AMD CPU. I checked every possible problems. I, actually a&nbsp; guy from the comppany sold these computers, swapped almost everything,&nbsp; mainboard, memories, video cards, and even he installed fancy&nbsp; water-cooling system. It was not successful. I bought new&nbsp; airconditioner to keep the room cool. It did not help. I usually run&nbsp; WIEN2k code in k-point parallelization mode. Sometimes just the&nbsp; program stops. Sometimes the whole computer system just stops. I mean&nbsp; it hangs without any response to the key stroke or mouse movement.&nbsp; Then I have to reboot the system. Eventually, I exchanged the whole&nbsp; system with 4 nodes of XEON dual-processor machines. Now, it is OK-no&nbsp; down, no hanging, no rebooting. Th!
e guy from the company said that&nbsp; this kind of problem never happened. Th! e company sold a systme with&nbsp; a single AMD Athlon Dual-processor machine for main node and 64 AMD&nbsp; Athlon Single-processor machines for subnodes and it did not have any&nbsp; problem except for the notorious heat problem for Athlon processors,&nbsp; but by installing powerful fans or water-cooling system there was no&nbsp; problem. I was not sure, but I realized the problem has happened in&nbsp; the NFS system. If the calculation requires an extensive reading and&nbsp; writing of files to the hard disk through NFS, the AMD CPU, especially&nbsp; for dual-processor machine, could not handle this situation properly.&nbsp; Either CPU or mainboard, or both could be a problem.&nbsp;&nbsp; </P>
<P>I hope this experience will help you. </P>
<P>&nbsp;</P>
<P>Sincerely,</P>
<P>&nbsp;</P>
<P>Joo Yull Rhee&nbsp; <BR><BR></P>
<BLOCKQUOTE style="PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">-----¿øº»¸Þ½ÃÁö-----<BR>
<DIV style="BACKGROUND: #e4e4e4; font-color: black"><B>º¸³½»ç¶÷:</B>&nbsp;kruse@lem.uni-karlsruhe.de</DIV><B>¹Þ´Â»ç¶÷:</B>&nbsp;rheejy@office.hoseo.ac.kr<BR><B>³¯Â¥:</B>&nbsp;2002³â 11¿ù 05ÀÏ 23:17<BR><B>Á¦¸ñ:</B>&nbsp;[WIEN]: Wien2k on PC: Error in lapw1<BR><BR><!--MAIL-TO:wien@zeus.theochem.tuwien.ac.at--><!--MAIL-CC:-->==== Peer Kruse <KRUSE@LEM.UNI-KARLSRUHE.DE>submitted the following contribution: ==== Dear Wien Users and developers, I still have the Error in lapw1. As nobody seems to have an idea, I' d like to ask, if anyone is using redhat 7.3 and/or newer Athlon processors without problems to exclude this possibility. Thank you Peer &gt; ==== &gt; Peer Kruse <KRUSE@LEM.UNI-KARLSRUHE.DE>&gt; submitted the following contribution: &gt; ==== &gt; &gt; Dear Wien users and developers, &gt; I tried to install Wien2k on 2 rather new PC's and get an &gt; "Error in lapw1" after a period of about 2 hours. &gt; This happens only for a larger number of k points, eg &gt;500, &gt; !
with only 50 it is working fine. I should have Memory in abundance &gt; (1BG) for my structure of 12 atoms (6 atoms inequivalent) nad the &gt; memory is not used (in the first hour of the program at least). &gt; The limits are set to &gt; &gt; core file size (blocks, -c) 0 &gt; data seg size (kbytes, -d) unlimited &gt; file size (blocks, -f) unlimited &gt; max locked memory (kbytes, -l) unlimited &gt; max memory size (kbytes, -m) unlimited &gt; open files (-n) 1024 &gt; pipe size (512 bytes, -p) 8 &gt; stack size (kbytes, -s) 32768 &gt; cpu time (seconds, -t) unlimited &gt; max user processes (-u) 7168 &gt; virtual memory (kbytes, -v) unlimited &gt; Is this ok? &gt; &gt; I compiled Wien2k with ifc and pgi, no difference, the same for the &gt; precompiled version. &gt; I' m running linux redhat 7.3. And it is running with the same &gt; parameters/structures &gt; on the old and slow and even smaller machines with every kind of &gt; architecture (dec, pc, notebook) without prob!
lem. &gt; &gt; Has anyone any experience or further ideas? &gt; &gt; Thank you &gt; &gt; Peer Kruse &gt; ==== WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at To (un)subscribe send mail to majordomo@zeus.theochem.tuwien.ac.at ==== </BLOCKQUOTE></BODY>
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------------------------------

Date: Wed, 6 Nov 2002 19:38:00 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: problem with the H atoms in my unit cell

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---559023410-851401618-1036633080=:18249
Content-Type: TEXT/PLAIN; charset=US-ASCII

Dear all:

There is a water (H2O) in my unit cell, I failed in running "lstart"
because nothing came out from running it. I attached the case.struct and
case.inst files with this email, could you please take a look and give
some ideas about how to run it? any instructions, suggestion and comment
is highly appreciated!

Thank you in adavance!


Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Thu, 7 Nov 2002 13:46:11 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

Actually, my question is very straight-forward. 

I put a molecule in a simple cubic lattice and start calculation. Then, 
WIEN detected that my molecule does not contain inversion symmetry but the 
lattice type (simple cubic) should have it. Then, WIEN asks me to add 
INVERSION OR NOT! Actually, my molecule does not contain inversion 
symmetry. Is the inversion here means the below operation?

  X'         -1  0  0    X
( Y' )  =  (  0 -1  0 )( Y )
  Z'          0  0 -1    Z 

Thank you very much

Martin

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------------------------------

Date: Thu, 7 Nov 2002 08:41:42 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: Question

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Dear Ma Chi Chiu,

if you refer to the initialisation procedure kgen, then don't worry too
much.  Inversion will not be added to your struct-file if you accept.  You
will still have to do lapw1C etc.  Inversion symmetry is only used to
generate of the k-mesh.  So, if you accept, you will have a k-mesh with
higher symmetry., ie -k will be equivalent to +k.  But for all other
programs except kgen, your system will not have inversion symmetry.
Usually you should 'add inversion' in kgen.

Kevin Jorissen
University of Antwerp, Belgium
kevin.jorissen@ua.ac.be




- ----- Original Message -----
From: "Ma Chi Chiu" <martin@yangtze.hku.hk>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Thursday, November 07, 2002 6:46 AM
Subject: [WIEN]: Question


> ====
> Ma Chi Chiu <martin@yangtze.hku.hk>
> submitted the following contribution:
> ====
>
> Dear all,
>
> Actually, my question is very straight-forward.
>
> I put a molecule in a simple cubic lattice and start calculation. Then,
> WIEN detected that my molecule does not contain inversion symmetry but the
> lattice type (simple cubic) should have it. Then, WIEN asks me to add
> INVERSION OR NOT! Actually, my molecule does not contain inversion
> symmetry. Is the inversion here means the below operation?
>
>   X'         -1  0  0    X
> ( Y' )  =  (  0 -1  0 )( Y )
>   Z'          0  0 -1    Z
>
> Thank you very much
>
> Martin
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

====
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------------------------------

Date: Thu, 07 Nov 2002 08:53:10 +0100
From: Florent Boucher <Florent.Boucher@cnrs-imn.fr>
Subject: Re: [WIEN]: w2web and Space Group #15

====
Florent Boucher <Florent.Boucher@cnrs-imn.fr>
submitted the following contribution:
====


- --------------000606040101080909000800
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Hi,<br>
I think the space group accepted by WIEN is B112/b.<br>
<table cellpadding="3" border="1" align="center">
  <tbody>
    <tr>
      <td align="left">CXZ</td>
 <td align="left" valign="top" width="113">b-base-centered (orthorh. and
monoclinic)</td>
 <td align="left" valign="top" width="170">[a sin(<img align="top"
 border="0" src="cid:part1.05020504.07040403@cnrs-imn.fr" alt="$\gamma$">
)/2, a cos(<img align="top" border="0"
 src="cid:part2.07090602.05020201@cnrs-imn.fr" alt="$\gamma$">
)/2, -c/2], [0, b, 0], [a sin(<img align="top" border="0"
 src="cid:part3.01020900.05040409@cnrs-imn.fr" alt="$\gamma$">
)/2, a cos(<img align="top" border="0"
 src="cid:part4.09000609.01070205@cnrs-imn.fr" alt="$\gamma$">
)/2, c/2]</td>
    </tr>
  </tbody>
</table>
So the transformation should be<br>
a' = a<br>
b' = c<br>
c' = -b<br>
This should work normally.<br>
Regards<br>
Florent<br>
<br>
Dadi Dai a &eacute;crit:<br>
<blockquote type="cite" cite="mid00fb01c285cd$7174b8e0$b8780198@chmwpc9"> 
 
  <meta http-equiv="Content-Type" content="text/html; ">
 
  <meta content="MSHTML 6.00.2719.2200" name="GENERATOR">
 
  <style></style> <font face="Arial"><font size="2">  
  <div>I was using w2web to generate input files for NiP2 calculations.&nbsp;
The  cell parameters that I have are: Spacegroup #15 C12/c1 (unique axis
b, cell  choice 1), a=6.500, b=5.628, c=6.156 A, and beta=127.07.</div>
 
  <div>&nbsp;</div>
 
  <div>The w2web StructGen accepts only B2/b (unique axis a, cell choice
1) for  space group 15.&nbsp; Therefore, I changed the order sequence and let
a=5.628,  b=6.156, c=6.500, and alpha=127.07.&nbsp; But the step "x sgroup" in
"init" gave  an error message: "alpha = 127.07 and not equal 90.&nbsp; Exiting
now."</div>
 
  <div>&nbsp;</div>
 
  <div>Did I misunderstand the symbol of space group #15 in w2web StuctGen
or the  order sequence of the cell parameters?</div>
 
  <div>&nbsp;</div>
 
  <div>Thanks!</div>
 
  <div>&nbsp;</div>
 
  <div>Dadi Dai</div>
  </font></font>  </blockquote>
<br>
<pre class="moz-signature" cols="$mailwrapcol">-- 
 --------------------------------------------------------------------------
| Florent BOUCHER                    |                                     |
| Institut des Mat&eacute;riaux Jean Rouxel | <a class="moz-txt-link-freetext" href="Mailto:Florent.Boucher@cnrs-imn.fr">Mailto:Florent.Boucher@cnrs-imn.fr</a>  |
| 2, rue de la Houssini&egrave;re           | Phone: (33) 2 40 37 39 24           |
| BP 32229                           | Fax:   (33) 2 40 37 39 95           |
| 44322 NANTES CEDEX 3 (FRANCE)      | <a class="moz-txt-link-freetext" href="http://www.cnrs-imn.fr">http://www.cnrs-imn.fr</a>              |
 --------------------------------------------------------------------------</pre>
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- --------------000606040101080909000800--

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------------------------------

Date: Thu, 07 Nov 2002 09:06:21 +0100
From: Florent Boucher <Florent.Boucher@cnrs-imn.fr>
Subject: Re: [WIEN]: Question

====
Florent Boucher <Florent.Boucher@cnrs-imn.fr>
submitted the following contribution:
====

<!DOCTYPE html PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
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<head>
  <meta http-equiv="Content-Type" content="text/html;charset=ISO-8859-1">
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<body>
Dear Martin,<br>
this problem is a common one for non centrosymmetric space group.<br>
So, if you don't use spin orbit coupling you can introduce the inversion
center for the generation of the irreducible k-points.<br>
Regards<br>
Florent<br>
Here is an answer from Peter (04/08/2002)&nbsp; about this point :<br>
<pre wrap="">====
Peter Blaha <a class="moz-txt-link-rfc2396E"
 href="mailto:pblaha@theochem.tuwien.ac.at">&lt;pblaha@theochem.tuwien.ac.at&gt;</a>
submitted the following contribution:
====

</pre>
<blockquote type="cite">
  <pre wrap=""><span class="moz-txt-citetags">&gt; </span>"Kevin Jorissen" <a
 class="moz-txt-link-rfc2396E" href="mailto:serelenka@hotmail.com">&lt;serelenka@hotmail.com&gt;</a>
  </pre>
</blockquote>
<pre wrap=""><!---->
Thanks to Keven Jorissen, who analized nicely the program KGEN.

I just want to add a few remarks:

</pre>
<blockquote type="cite">
  <pre wrap=""><span class="moz-txt-citetags">&gt; </span>Next is the routine GROUPS.  This is strange.  It contains a list of all
  </pre>
</blockquote>
<pre wrap=""><!---->
GROUPS is not really used anymore, but we use the symmetry operations of
our struct file. (It is a left-over).



Adding inversion: You should always add inversion, except in

     spin-polarized relativistic spin-orbit calculations.

This can be made, since timeinversion
acts usually like the inversion and ensures that +k and -k have identical
eigenvalues.



Shift of k-mesh: This will decrease the number of points at the same k-mesh
density. Consider a 1D case:
A mesh of 3 k-points in 1D: (0; .25; .5) has a "spacing" of 0.25.

The same spacing (i.e. the same density) can be achieved by a mesh of
2 points: (1/8; 3/8). Now these two points have the same weight
(while previously I had Gamma and X with lower weight!) and I do
the calculation at the same density of k-points, but with smaller number of
points.

The counterargument is: Often bandgaps,... originate at Gamma or X, i.e.
at the BZ center or boundary. When you omit those points in your mesh,
don't expect to obtain a correct gap from this k-mesh (E.g. Your EF will be at
the highest energy of band "4", but the fourth band at Gamma is higher!
thus you may overestimate the gap in this example) .
Thus I do the scf calculation with a shifted mesh, but for semiconductors
I change the mesh before I calculate the DOS.

Regards



 </pre>
<br>
<br>
Ma Chi Chiu a &eacute;crit:<br>
<blockquote type="cite"
 cite="midPine.LNX.4.44.0211071337490.12860-100000@yangtze.hku.hk">
  <pre wrap="">====
Ma Chi Chiu <a class="moz-txt-link-rfc2396E" href="mailto:martin@yangtze.hku.hk">&lt;martin@yangtze.hku.hk&gt;</a>
submitted the following contribution:
====

Dear all,

Actually, my question is very straight-forward. 

I put a molecule in a simple cubic lattice and start calculation. Then, 
WIEN detected that my molecule does not contain inversion symmetry but the 
lattice type (simple cubic) should have it. Then, WIEN asks me to add 
INVERSION OR NOT! Actually, my molecule does not contain inversion 
symmetry. Is the inversion here means the below operation?

  X'         -1  0  0    X
( Y' )  =  (  0 -1  0 )( Y )
  Z'          0  0 -1    Z 

Thank you very much

Martin

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  </pre>
</blockquote>
<br>
<pre class="moz-signature" cols="$mailwrapcol">-- 
 --------------------------------------------------------------------------
| Florent BOUCHER                    |                                     |
| Institut des Mat&eacute;riaux Jean Rouxel | <a class="moz-txt-link-freetext" href="Mailto:Florent.Boucher@cnrs-imn.fr">Mailto:Florent.Boucher@cnrs-imn.fr</a>  |
| 2, rue de la Houssini&egrave;re           | Phone: (33) 2 40 37 39 24           |
| BP 32229                           | Fax:   (33) 2 40 37 39 95           |
| 44322 NANTES CEDEX 3 (FRANCE)      | <a class="moz-txt-link-freetext" href="http://www.cnrs-imn.fr">http://www.cnrs-imn.fr</a>              |
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------------------------------

Date: Thu, 7 Nov 2002 09:24:54 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Question

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I put a molecule in a simple cubic lattice and start calculation. Then,
> WIEN detected that my molecule does not contain inversion symmetry but the
> lattice type (simple cubic) should have it. Then, WIEN asks me to add
> INVERSION OR NOT! Actually, my molecule does not contain inversion
> symmetry. Is the inversion here means the below operation?

In addition to what was said before: If you want to study a free molecule,
you need a big box, and then you need only one k-point (gamma).
k-dispersion should be zero.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 7 Nov 2002 20:56:56 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

Thank you very much for the replies. 

Actually, I am interested in the optical properties of my molecule and 
freom the replies, it seems that the inversion symmetry is a must in order 
to generate a better k-mesh. Should I add the inversionif I am interested 
in the optical properties? The reason is that the spectra are quite 
different. 

On the other hand, I have calculated the bandstructure of another molecule 
with only 20 k-point (inequivalent k-point = 4). Then, I get 
case.spaghetti_ps and case.spaghetti_ene. Is it we can get the bandstructure 
by plotting the column 4 and 5 of case.spaghetti_ene file? Also, I found that 
the case.spaghetti_ene file has lines like "bandindex: 1", "bandindex: 2" and
etc. Does it mean the lines below "bandindex: 1" are the components of band 1 
of different k?

Thank you very much

Martin

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------------------------------

Date: Wed, 06 Nov 2002 14:18:22 +0100
From: Peer Kruse <kruse@lem.uni-karlsruhe.de>
Subject: [WIEN]: PC: Error in lapw1

====
Peer Kruse <kruse@lem.uni-karlsruhe.de>
submitted the following contribution:
====

Thank you for your ideas,
I checked the files and indeed I found an   
 > lapw1  -c   (09:40:47) Speicherschutzverletzung
in the dayfile. But how to interpret this? I think it is something 
similar to a segmentation fault.
In the output1 file the table after Initialize parallelization variables 
is interrupted
half way down it's last few lines are

      1667     0.59857210    0    1   -1             0.21216   0.16977  
- -0.37017
      1668     0.59857210    0    0    0             0.21216   0.02425   
0.17534
      1669     0.59857210    0   -1    0             0.21216  -0.12126   
0.17534
      1670     0.59857210

so they are broken in the middle of the line.

But no corefiles were generated and there is no output to the terminal.
And why is it running fine on a much smaller pc (same code so same NMATMAX,
 same init files) but less memory and  same or even  smaller stack?
On the smaller machine is by the way an older system and a intel CPU. I 
still don't understand this.


Best regards


Peer

> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
>
> Dear Mr. Kruse,
>
> "Error in lapw1" is not much information. Wasn't there any additional 
> information in the dayfile or the output files? Usually when lapw1 
> crashes during runtime just by increasing the number of k-points, it 
> has to do with memory. And usually, there is additional information in 
> the dayfile and/or the screen output (on dec when run in background, 
> the default file name here is nohup.out). Is NMATMAX big enough? Do 
> you have swap space? On any of the mentioned systems? Did a core dump? 
> Have you tried to increase the Stack size?
>
> So that was a few ideas... I am pretty sure it has to do with your 
> setup, not the code.
>
> Best regards,
> Torsten.
>
> Peer Kruse wrote:
>
>> ====
>> Peer Kruse <kruse@lem.uni-karlsruhe.de>
>> submitted the following contribution:
>> ====
>>
>> Dear Wien Users and developers,
>> I still have the Error in lapw1. As nobody seems to have an idea, I' 
>> d like to ask, if anyone is using
>> redhat 7.3 and/or newer Athlon processors without problems to exclude 
>> this possibility.
>>
>> Thank you
>>
>> Peer
>>
>>> ====
>>> Peer Kruse <kruse@lem.uni-karlsruhe.de>
>>> submitted the following contribution:
>>> ====
>>>
>>> Dear Wien users and developers,
>>> I tried to install Wien2k on 2 rather new PC's and get an
>>> "Error in lapw1" after a period of about 2 hours.
>>> This happens only for a larger number of k points, eg >500,
>>> with only 50 it is working fine. I should have Memory in abundance
>>> (1BG) for my structure of 12 atoms (6 atoms inequivalent) nad the 
>>> memory is not used (in the first hour of the program at least).
>>> The limits are set to
>>>
>>> core file size (blocks, -c) 0
>>> data seg size (kbytes, -d) unlimited
>>> file size (blocks, -f) unlimited
>>> max locked memory (kbytes, -l) unlimited
>>> max memory size (kbytes, -m) unlimited
>>> open files (-n) 1024
>>> pipe size (512 bytes, -p) 8
>>> stack size (kbytes, -s) 32768
>>> cpu time (seconds, -t) unlimited
>>> max user processes (-u) 7168
>>> virtual memory (kbytes, -v) unlimited
>>> Is this ok?
>>>
>>> I compiled Wien2k with ifc and pgi, no difference, the same for the 
>>> precompiled version.
>>> I' m running linux redhat 7.3. And  it is running with the same 
>>> parameters/structures
>>> on the old and slow and even smaller machines with every kind of 
>>> architecture (dec, pc, notebook) without problem.
>>>
>>> Has anyone any experience or further ideas?
>>>
>>> Thank you
>>>
>>> Peer Kruse
>>>
>>
>>
>>
>> ====
>> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>> To (un)subscribe send mail to
>> majordomo@zeus.theochem.tuwien.ac.at
>> ====
>>
>>
>



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------------------------------

Date: Thu, 7 Nov 2002 21:56:26 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

I get a message likes:

>   dstart      (22:11:51) STOP DSTART ENDS statement executed
245.130u 0.190s 4:05.36 99.9%   0+0k 0+0io 192pf+0w
- -----> check in  80.outputd  if gmax > gmin, normalization

In my case.outputd file, it appears like :

 gmin  12.3076923
 gmax  10.


Then, what and how should I do?


Thank you very much

Martin

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------------------------------

Date: Thu, 07 Nov 2002 14:50:47 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: PC: Error in lapw1

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Yeah, that's a segmentation violation fault. You probably have turned 
core files off (limit coredumpsize=0 or something like that), otherwise 
there would have been a core file. It is an abrupt termination of the 
program due to what the OS or processor sees as an illegal address, and 
the sudden end of the file as you describe is a direct consequence of 
that. As far as I know it is different from "out of memory", but in some 
instances programs terminate with a segmentation fault there, too, 
although I am not sure why.

Did you address the question of swap space? Because newer versions of 
Linux are real memory hogs if you use KDE, for example...

The next question would be "Does it also happen if you compile without 
optimisation?", i.e., with -O0 in stead of whatever value it has now 
(-O5?). Are the Linux kernels identical on the different machines? It 
could be an OS issue... and linux is known to have problems in various 
kernel versions with dual processors when combined with software RAID, 
for example.

Best regards,
Torsten.





Peer Kruse wrote:

> ====
> Peer Kruse <kruse@lem.uni-karlsruhe.de>
> submitted the following contribution:
> ====
>
> Thank you for your ideas,
> I checked the files and indeed I found an   > lapw1  -c   (09:40:47) 
> Speicherschutzverletzung
> in the dayfile. But how to interpret this? I think it is something 
> similar to a segmentation fault.
> In the output1 file the table after Initialize parallelization 
> variables is interrupted
> half way down it's last few lines are
>
>      1667     0.59857210    0    1   -1             0.21216   0.16977  
> -0.37017
>      1668     0.59857210    0    0    0             0.21216   
> 0.02425   0.17534
>      1669     0.59857210    0   -1    0             0.21216  
> -0.12126   0.17534
>      1670     0.59857210
>
> so they are broken in the middle of the line.
>
> But no corefiles were generated and there is no output to the terminal.
> And why is it running fine on a much smaller pc (same code so same 
> NMATMAX,
> same init files) but less memory and  same or even  smaller stack?
> On the smaller machine is by the way an older system and a intel CPU. 
> I still don't understand this.
>
>
> Best regards
>
>
> Peer
>
>> ====
>> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
>> submitted the following contribution:
>> ====
>>
>> Dear Mr. Kruse,
>>
>> "Error in lapw1" is not much information. Wasn't there any additional 
>> information in the dayfile or the output files? Usually when lapw1 
>> crashes during runtime just by increasing the number of k-points, it 
>> has to do with memory. And usually, there is additional information 
>> in the dayfile and/or the screen output (on dec when run in 
>> background, the default file name here is nohup.out). Is NMATMAX big 
>> enough? Do you have swap space? On any of the mentioned systems? Did 
>> a core dump? Have you tried to increase the Stack size?
>>
>> So that was a few ideas... I am pretty sure it has to do with your 
>> setup, not the code.
>>
>> Best regards,
>> Torsten.
>>
>> Peer Kruse wrote:
>>
>>> ====
>>> Peer Kruse <kruse@lem.uni-karlsruhe.de>
>>> submitted the following contribution:
>>> ====
>>>
>>> Dear Wien Users and developers,
>>> I still have the Error in lapw1. As nobody seems to have an idea, I' 
>>> d like to ask, if anyone is using
>>> redhat 7.3 and/or newer Athlon processors without problems to 
>>> exclude this possibility.
>>>
>>> Thank you
>>>
>>> Peer
>>>
>>>> ====
>>>> Peer Kruse <kruse@lem.uni-karlsruhe.de>
>>>> submitted the following contribution:
>>>> ====
>>>>
>>>> Dear Wien users and developers,
>>>> I tried to install Wien2k on 2 rather new PC's and get an
>>>> "Error in lapw1" after a period of about 2 hours.
>>>> This happens only for a larger number of k points, eg >500,
>>>> with only 50 it is working fine. I should have Memory in abundance
>>>> (1BG) for my structure of 12 atoms (6 atoms inequivalent) nad the 
>>>> memory is not used (in the first hour of the program at least).
>>>> The limits are set to
>>>>
>>>> core file size (blocks, -c) 0
>>>> data seg size (kbytes, -d) unlimited
>>>> file size (blocks, -f) unlimited
>>>> max locked memory (kbytes, -l) unlimited
>>>> max memory size (kbytes, -m) unlimited
>>>> open files (-n) 1024
>>>> pipe size (512 bytes, -p) 8
>>>> stack size (kbytes, -s) 32768
>>>> cpu time (seconds, -t) unlimited
>>>> max user processes (-u) 7168
>>>> virtual memory (kbytes, -v) unlimited
>>>> Is this ok?
>>>>
>>>> I compiled Wien2k with ifc and pgi, no difference, the same for the 
>>>> precompiled version.
>>>> I' m running linux redhat 7.3. And  it is running with the same 
>>>> parameters/structures
>>>> on the old and slow and even smaller machines with every kind of 
>>>> architecture (dec, pc, notebook) without problem.
>>>>
>>>> Has anyone any experience or further ideas?
>>>>
>>>> Thank you
>>>>
>>>> Peer Kruse
>>>>
>>>
>>>
>>>
>>> ====
>>> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>>> To (un)subscribe send mail to
>>> majordomo@zeus.theochem.tuwien.ac.at
>>> ====
>>>
>>>
>>
>
>
>
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>

- -- 
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Department of Physics, Condensed Matter Theory Group, Uppsala University
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Date: Thu, 07 Nov 2002 14:53:45 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Question

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Go back to 80.in2 or 80.in2c and change gmax to 13...

Best regards,
Torsten.

Ma Chi Chiu wrote:

>====
>Ma Chi Chiu <martin@yangtze.hku.hk>
>submitted the following contribution:
>====
>
>Dear all,
>
>I get a message likes:
>
>>  dstart      (22:11:51) STOP DSTART ENDS statement executed
>>
>245.130u 0.190s 4:05.36 99.9%   0+0k 0+0io 192pf+0w
>-----> check in  80.outputd  if gmax > gmin, normalization
>
>In my case.outputd file, it appears like :
>
> gmin  12.3076923
> gmax  10.
>
>
>Then, what and how should I do?
>
>
>Thank you very much
>
>Martin
>
>====
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>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
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Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
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------------------------------

Date: Thu, 07 Nov 2002 16:06:59 +0100
From: Vladimir Timochevski <Vladimir.Timochevski@dpm.univ-lyon1.fr>
Subject: Re: [WIEN]: Question

====
Vladimir Timochevski <Vladimir.Timochevski@dpm.univ-lyon1.fr>
submitted the following contribution:
====

Dear Martin,

As it was pointed out in the previous comment by Prof.
Blaha, you have "zero dispersion" for a molecule, cluster,
or any other unperiodic solid. This means that your results
should not depend on the number and position of K-points.
Try to compare eigenvalues for different K-points (or plot
the "spaghetti", if it does not take time). If the
eigenvalues are different, it means that your "box" is not
large enough. Try to increase it. 
When your box is large enough you will need only Gamma-point
sampling.

Yours,
Vladimir


Ma Chi Chiu wrote:
> 
> ====
> Ma Chi Chiu <martin@yangtze.hku.hk>
> submitted the following contribution:
> ====
> 
> Dear all,
> 
> Thank you very much for the replies.
> 
> Actually, I am interested in the optical properties of my molecule and
> freom the replies, it seems that the inversion symmetry is a must in order
> to generate a better k-mesh. Should I add the inversionif I am interested
> in the optical properties? The reason is that the spectra are quite
> different.
> 
> On the other hand, I have calculated the bandstructure of another molecule
> with only 20 k-point (inequivalent k-point = 4). Then, I get
> case.spaghetti_ps and case.spaghetti_ene. Is it we can get the bandstructure
> by plotting the column 4 and 5 of case.spaghetti_ene file? Also, I found that
> the case.spaghetti_ene file has lines like "bandindex: 1", "bandindex: 2" and
> etc. Does it mean the lines below "bandindex: 1" are the components of band 1
> of different k?
> 
> Thank you very much
> 
> Martin
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
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> majordomo@zeus.theochem.tuwien.ac.at
> ====

- -- 
- ---------------------------------------------
Vladimir Timoshevskii
Departement de Physique de Materiaux
Universite Claude Bernard - Lyon 1
Lyon, France
Tel.: +33 472 431564
Fax:  +33 472 432648
email: Vladimir.Timochevski@dpm.univ-lyon1.fr
- ---------------------------------------------
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------------------------------

Date: Thu, 7 Nov 2002 09:46:49 -0700 (MST)
From: Martin Gelfand <gelfand@lamar.colostate.edu>
Subject: Re:[WIEN]: Wien2k on PC: Error in lapw1

====
Martin Gelfand <gelfand@lamar.ColoState.EDU>
submitted the following contribution:
====

It would be interesting to have a bit more information about how
the AMD systems were configured---I'd guess they're running linux,
but what distribution?  Kernel or userland nfsd?  Which kind of 
networking (presumably ethernet, but what chipset)?   Motherboard...?

I'm considering setting up a bunch of single-processor Athlon diskless
nodes because it seems to be the most cost-effective setup, but I'd rather
not go through your pain (particularly since I'd be building everything
myself, and won't be able to return "working" motherboards/CPUs).
Every detail is potentially useful.  Please reply off-list if you
feel this is getting too far afield for Wien2K discussions.

Regards,
Martin Gelfand 

On Thu, 7 Nov 2002, Joo Yull Rhee wrote:

> ==== Joo Yull Rhee submitted the following contribution: ==== P
> {margin-top:2px;margin-bottom:2px;}
> 
> Dear WIEN2k users,
> 
>  
> 
> I want to share my experience with others who are using PC with AMD  Athlon
> processors. I purchased 4 nodes of AMD Athlon Dual-processor  machines last
> year. It kept failed. Initially I thought it was heat  problem with AMD CPU.
> I checked every possible problems. I, actually a  guy from the comppany sold
> these computers, swapped almost everything,  mainboard, memories, video
> cards, and even he installed fancy  water-cooling system. It was not
> successful. I bought new  airconditioner to keep the room cool. It did not
> help. I usually run  WIEN2k code in k-point parallelization mode. Sometimes
> just the  program stops. Sometimes the whole computer system just stops. I
> mean  it hangs without any response to the key stroke or mouse movement. 
> Then I have to reboot the system. Eventually, I exchanged the whole  system
> with 4 nodes of XEON dual-processor machines. Now, it is OK-no  down, no
> hanging, no rebooting. Th! e guy from the company said that  this kind of
> problem never happened. Th! e company sold a systme with  a single AMD
> Athlon Dual-processor machine for main node and 64 AMD  Athlon
> Single-processor machines for subnodes and it did not have any  problem
> except for the notorious heat problem for Athlon processors,  but by
> installing powerful fans or water-cooling system there was no  problem. I
> was not sure, but I realized the problem has happened in  the NFS system. If
> the calculation requires an extensive reading and  writing of files to the
> hard disk through NFS, the AMD CPU, especially  for dual-processor machine,
> could not handle this situation properly.  Either CPU or mainboard, or both
> could be a problem.  
> 
> I hope this experience will help you.
> 
>  
> 
> Sincerely,
> 
>  
> 
> Joo Yull Rhee 
> 

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------------------------------

Date: Thu, 7 Nov 2002 20:09:26 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Question

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====



> I get a message likes:
>
> >   dstart      (22:11:51) STOP DSTART ENDS statement executed
> 245.130u 0.190s 4:05.36 99.9%   0+0k 0+0io 192pf+0w
> -----> check in  80.outputd  if gmax > gmin, normalization
>
> In my case.outputd file, it appears like :
>
>  gmin  12.3076923
>  gmax  10.

It happens (gmin>gmax) when one uses small rmt or large rkmax, i..e. in
organic atoms, due to the relation of gmin=rkm/rrmt*2, and demands a larger
gmax to generate more planewave to expand  charge density and potential (and
not wavefunctions) out of the sphere(s). There is a constraint in dstart on
gmax: it is limited to the upper value 25. Based on  the indicated relation
(gmin=rkm/rrmt*2), upper limit 25, and the case of study one justifies how
to get ride of this problem.

        Your,

        Saeid.




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------------------------------

Date: Fri, 8 Nov 2002 11:37:00 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: Re: [WIEN]: Question

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

Sorry, how to compare eigenvalues for different K-points? Which file 
stores the information?

Also, I always the similar lines in my case.outputsp files:

  band 68  char-min/max:  1.  0.
         ERROR reading QTLs:
  band: 69 k-point: 38
  execution continued ....

Why? And how to fix this problem?

Thank you very much

Martin

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------------------------------

Date: Fri, 8 Nov 2002 15:23:44 +0800
From: "Wenhui Xie" <xiewh@sun20.iphy.ac.cn>
Subject: [WIEN]: "Address error" and  struct error in initso_lapw 

====
"Wenhui Xie" <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear all,

I use WIEN2k to calculate the Spin-orbit effect in CsCl Cr2 (just for training).
Following the usersguide, I first runsp_lapw and save_lapw. However,
In initso_lapw, two error messages occurs and the calcaulation have to stop.
The Messages are pasted below:
 
Do you have a spinpolarized case ( and want to run symmetryso)? (y/N)y
** Address Error **
End of diagnostics

Do you want to use new structure for SO calculation? (y/N)y
 We run kgen to generate a new kmesh for the SO calculation:
Input/Output Error 153: Input file ended
	In Procdure: main program
		At Line: 150
	  Statement: Formatted READ
		Unit   : 20
   Connected To: cr_cscl.struct
        Form   : Formatted 
		Access:  Sequential
Records Read   : 0
Records Writen : 0
End of diagnostics				

And this is my inso file:

WFFIL
 4  1  0                      llmax,ipr,kpot 
 -10.0000   1.50000           emin,emax (output energy window)
   0.  0.  1.                 direction of magnetization (lattice vectors)
 2                            number of atoms for which RLO is added
 1     -4.97      0.005       atom number,e-lo,de (case.in1), repeat NX times
 1     -4.97      0.005
 0 0 0 0 0                    number of atoms for which SO is switch off; atoms

This is my struct files.

Cs                                                                             
P   LATTICE,NONEQUIV. ATOMS: 2                                                 
MODE OF CALC=RELA unit=bohr                                                    
  5.000000  5.000000  5.000000 90.000000 90.000000 90.000000                   
ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT= 2
Cr1        NPT=  781  R0=0.00010000 RMT=    2.0000   Z: 24.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=  2: X=0.50000000 Y=0.50000000 Z=0.50000000
          MULT= 1          ISPLIT= 2
Cr2        NPT=  781  R0=0.00010000 RMT=    2.0000   Z: 24.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
  48      NUMBER OF SYMMETRY OPERATIONS


I would appreciate you if I can share your experience in such a problem.

Best Regards

Wenhui Xie
xiewh@sun20.iphy.ac.cn
¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡2002-11-08



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------------------------------

Date: Fri,  8 Nov 2002 19:57:51 +1100
From: chen0130@flinders.edu.au
Subject: [WIEN]: automatic geometry optimisation

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Dear Wien users,

Can any one tell me if there is any automatic geometry optimisation of any 
degree in Wien97?

Thanks

Cheng


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------------------------------

Date: Fri, 08 Nov 2002 09:55:01 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: "Address error" and  struct error in initso_lapw

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Mr. Xie,

you probably need to recompile symetso (look in SRC_symmetso) with lower 
optimisation. I get other funny errors (wrong A and B symmetry sorting) 
if optimisation is too high. Change FOPT in the Makefile to "-O0".

The other error is a consequence of the first error, I think... so it 
should disappear once you have conquered the first error.

Best regards,
Torsten.

Wenhui Xie wrote:

>====
>"Wenhui Xie" <xiewh@sun20.iphy.ac.cn>
>submitted the following contribution:
>====
>
>Dear all,
>
>I use WIEN2k to calculate the Spin-orbit effect in CsCl Cr2 (just for training).
>Following the usersguide, I first runsp_lapw and save_lapw. However,
>In initso_lapw, two error messages occurs and the calcaulation have to stop.
>The Messages are pasted below:
> 
>Do you have a spinpolarized case ( and want to run symmetryso)? (y/N)y
>** Address Error **
>End of diagnostics
>
>Do you want to use new structure for SO calculation? (y/N)y
> We run kgen to generate a new kmesh for the SO calculation:
>Input/Output Error 153: Input file ended
>	In Procdure: main program
>		At Line: 150
>	  Statement: Formatted READ
>		Unit   : 20
>   Connected To: cr_cscl.struct
>        Form   : Formatted 
>		Access:  Sequential
>Records Read   : 0
>Records Writen : 0
>End of diagnostics				
>
>And this is my inso file:
>
>WFFIL
> 4  1  0                      llmax,ipr,kpot 
> -10.0000   1.50000           emin,emax (output energy window)
>   0.  0.  1.                 direction of magnetization (lattice vectors)
> 2                            number of atoms for which RLO is added
> 1     -4.97      0.005       atom number,e-lo,de (case.in1), repeat NX times
> 1     -4.97      0.005
> 0 0 0 0 0                    number of atoms for which SO is switch off; atoms
>
>This is my struct files.
>
>Cs                                                                             
>P   LATTICE,NONEQUIV. ATOMS: 2                                                 
>MODE OF CALC=RELA unit=bohr                                                    
>  5.000000  5.000000  5.000000 90.000000 90.000000 90.000000                   
>ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
>          MULT= 1          ISPLIT= 2
>Cr1        NPT=  781  R0=0.00010000 RMT=    2.0000   Z: 24.0                   
>LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                     0.0000000 1.0000000 0.0000000
>                     0.0000000 0.0000000 1.0000000
>ATOM=  2: X=0.50000000 Y=0.50000000 Z=0.50000000
>          MULT= 1          ISPLIT= 2
>Cr2        NPT=  781  R0=0.00010000 RMT=    2.0000   Z: 24.0                   
>LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                     0.0000000 1.0000000 0.0000000
>                     0.0000000 0.0000000 1.0000000
>  48      NUMBER OF SYMMETRY OPERATIONS
>
>
>I would appreciate you if I can share your experience in such a problem.
>
>Best Regards
>
>Wenhui Xie
>xiewh@sun20.iphy.ac.cn
>¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡¡2002-11-08
>
>
>
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>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
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------------------------------

Date: Fri, 8 Nov 2002 17:17:58 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

Thank you very much for the replies.

My last question is :

> I get a message likes:
>
> >   dstart      (22:11:51) STOP DSTART ENDS statement executed
> 245.130u 0.190s 4:05.36 99.9%   0+0k 0+0io 192pf+0w
> -----> check in  80.outputd  if gmax > gmin, normalization
>
> In my case.outputd file, it appears like :
>
>  gmin  12.3076923
>  gmax  10.

From the replies, I understand that I need to increase the value of gmax. 
However, actually, how will this two values affect the bandstructure plot 
or the fermi energy level of my calculation? If gmax less than gmax, will 
the bandstructure plot and the fermi energy level become wrong?

Thank you very much

Martin

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Date: Fri, 08 Nov 2002 10:23:21 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: automatic geometry optimisation

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

min_lapw and mini (see, e.g., sec. 8.14 in UG).

chen0130@flinders.edu.au wrote:

>====
>chen0130@flinders.edu.au
>submitted the following contribution:
>====
>
>Dear Wien users,
>
>Can any one tell me if there is any automatic geometry optimisation of any 
>degree in Wien97?
>
>Thanks
>
>Cheng
>
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
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Date: Fri, 8 Nov 2002 19:58:03 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: Re: [WIEN]: automatic geometry optimisation

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

I have a question :

In my .klist file, I have the following lines:
- ------
         1    0    0    0   42  1.0 -7.0  1.5       200 k, div: (  3  3 14)
         2    0    0    3   42  2.0
         3    0    0    6   42  2.0
         .    .    .    .    .   .
        37   14   28   12   42  4.0
        38   14   28   15   42  4.0
        39   14   28   18   42  4.0
        40   14   28   21   42  2.0
END
- ------

In my .outputkgen, I have the following lines:

- ------
  length of reciprocal lattic vectors:  3.66489516  3.66489516  14.8904178
  SUBMESH SHIFTED; SHIFT:  0 0 0
  NO. OF MESH POINTS IN THE BRILLOUIN ZONE =   126
  DIVISION OF RECIPROCAL LATTICE VECTORS (INTERVALS)=    3    3   14
  weights of k-points:
  NO. OF INEQUIVALENT K-POINTS    40
  INEQUIVALENT BLOCH VECTORS
- ------

Then, how do the k-points distribute? What is the meaning for div: (  3  3 14) 
{DIVISION OF RECIPROCAL LATTICE VECTORS (INTERVALS)}? My unit cell parameter is 
10Ax10Ax2.46A. 
Actually, I am interested in how many k-points are distributed along the z-axis. 
How would I get the information or calculated it out?  

Thank you very much

Martin

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------------------------------

Date: Fri, 08 Nov 2002 14:01:16 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: automatic geometry optimisation

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

The k-points are distributed according to what is written in Bloechls 
paper. Read it.

Best regards,
Torsten.

Ma Chi Chiu wrote:

>====
>Ma Chi Chiu <martin@yangtze.hku.hk>
>submitted the following contribution:
>====
>
>Dear all,
>
>I have a question :
>
>In my .klist file, I have the following lines:
>------
>         1    0    0    0   42  1.0 -7.0  1.5       200 k, div: (  3  3 14)
>         2    0    0    3   42  2.0
>         3    0    0    6   42  2.0
>         .    .    .    .    .   .
>        37   14   28   12   42  4.0
>        38   14   28   15   42  4.0
>        39   14   28   18   42  4.0
>        40   14   28   21   42  2.0
>END
>------
>
>In my .outputkgen, I have the following lines:
>
>------
>  length of reciprocal lattic vectors:  3.66489516  3.66489516  14.8904178
>  SUBMESH SHIFTED; SHIFT:  0 0 0
>  NO. OF MESH POINTS IN THE BRILLOUIN ZONE =   126
>  DIVISION OF RECIPROCAL LATTICE VECTORS (INTERVALS)=    3    3   14
>  weights of k-points:
>  NO. OF INEQUIVALENT K-POINTS    40
>  INEQUIVALENT BLOCH VECTORS
>------
>
>Then, how do the k-points distribute? What is the meaning for div: (  3  3 14) 
>{DIVISION OF RECIPROCAL LATTICE VECTORS (INTERVALS)}? My unit cell parameter is 
>10Ax10Ax2.46A. 
>Actually, I am interested in how many k-points are distributed along the z-axis. 
>How would I get the information or calculated it out?  
>
>Thank you very much
>
>Martin
>
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>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Fri, 08 Nov 2002 15:34:31 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: [WIEN]: LDA+U

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====

Dear wien2k_02 users:
   I want to know if someone has the successful experience with wien2k_02 
to calcualte a system with SO and ORB. I have used wien2k_02 to calculate a 
AB system to include SO and ORB.But the result puzzled me, the situtation I 
found is listed as belows(the value list are just for example):

   1.if I runsp_lapw,  the spin momnt is :
       MMTOT :0.81
       MMI01: 0.78____________>the spin moment of A
       MMI02  0.02
   2:runsp_lapw -so, the result is
       MMTOT: 0.67
       MMIO1: 0.66
   3:when I runsp_lapw -so -orb ,the result are puzzled:

      if I use OP,the result:
         MMI01: 0.39
         ORB01  -2.67
      this may be possible , for A is 4f element and the experimental       
  momnet is above 2.0
         
      but if I use SIC(AMf), I found when U and J are increase ,the MMI01 
are decrease,and even change form positive to negative value,for example, 
change form 
0.63 to -0.35 ,and orb01 change form -0.59 to 0.42(just for example) when U 
increase from 0.11 to 0.48(experimental velue), I have change the sequence 
of runsp_lpw with SO and ORB  just like Dear Peter answered several days 
ago. but no improvement. Some one also report this question before, but 
they use lower version
wien, so the in1 must be changed to inlc, but I use the latest wien2k_02, 
real lapw1 is good if system obtain inversion when runsp_Lapw -so -orb 
because orb is added in lapwso, So it seems that in runsp+SO+SIC(AMF), the 
U will decrease the value of spin and orbit mometn and may change the 
positive(negative)value to negative(positive)value. This is obvious 
different from LMTO method and the prediction. Who can tell me the reason?

Thanks
   Hai


my input files are listed below:

case.inso
WFFIL
 4  0  0                      llmax,ipr,kpot 
 -10.0000   1.5000           Emin, Emax
     0 0 1                       h,k,l (direction of magnetization)
   0                             number of atoms with RLO
 1   2                           number of atoms without SO, atomnumbers

case.indmc
- -9.           Emin cutoff energy
 1            number of atoms for which density matrix is calculated
 1  1  3      index of 1st atom, number of L's, L1
 0 0          r-index, (l,s)-index


when use U(SIC)case.inorb

1  1  0                        nmod, natorb, ipr
PRATT,1.0                      mixmod, amix
1 1 3                          iatom nlorb, lorb
1                              nsic (LDA+U(SIC) used)
0.48 0.048                      U J


when use OP, case.inorb is

2  1  0                        nmod, natorb, ipr
PRATT, 1.0                     mixmod, amix
1 1 3                          iatom nlorb, lorb
0                              nmodop
1                              Ncalc
0. 0. 1.                       direction of M in terms of lattice vectors





_________________________________________________________________
ÓëÁª»úµÄÅóÓÑ½øÐÐ½»Á÷£¬ÇëÊ¹ÓÃ MSN Messenger: http://messenger.msn.com/lccn/ 

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Date: Sat,  9 Nov 2002 03:34:59 +1100
From: chen0130@flinders.edu.au
Subject: Re: [WIEN]: automatic geometry optimisation

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Thanks, I guess I am asking a silly question, but my emphasis is on
'automatic'! (ie something done in symmetry?) without the expensive mini_lapw

could someone suggest some generic reasons why geometry optimisations are not 
necessarily performed for solid state structures?

there seems to be publications without relaxing supercells...

sorry to be so broad, appreciating any remarks,

Thanks,

Cheng

Quoting Torsten Andersen <Torsten.Andersen@Fysik.UU.se>:

> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
> 
> min_lapw and mini (see, e.g., sec. 8.14 in UG).
> 
> chen0130@flinders.edu.au wrote:
> 
> >====
> >chen0130@flinders.edu.au
> >submitted the following contribution:
> >====
> >
> >Dear Wien users,
> >
> >Can any one tell me if there is any automatic geometry optimisation of any
> 
> >degree in Wien97?
> >
> >Thanks
> >
> >Cheng
> >
> >
> >====
> >WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> >To (un)subscribe send mail to
> >majordomo@zeus.theochem.tuwien.ac.at
> >====
> >
> >
> 
> -- 
> Dr. Torsten Andersen
> Department of Physics, Condensed Matter Theory Group, Uppsala University
> UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
> News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics
> 
> 
> 
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 
> 



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------------------------------

Date: Fri, 8 Nov 2002 11:36:10 -0500
From: Jeff Spirko <spirko@lehigh.edu>
Subject: [WIEN]: Address Error in lapw1

====
Jeff Spirko <spirko@lehigh.edu>
submitted the following contribution:
====

I'm having a problem with lapw1 in a large (> 1 GB RAM, 10000 matrix
size, RKM=7.0) job.  I have already checked the available RAM,
diskspace, and stack size.

  Version:          WIEN2k_02 from Oct 24, 2002
  Computer:         Pentium IV with 2 GB RDRAM
  Operating System: Redhat Linux 8.0
  Compiler:         IFC 6.0
  FOPT:             -O0 -FR -mp -w -tpp7
  LDFLAGS:          -Vaxlib -L../SRC_lib
  R_LIBS:           -llapack_lapw -lmkl_p4 -lguide -lpthread

I have successfully run the job on an SGI, and I just transferred
over the .struct, .in*, .kgen, .klist, and .clmsum files.  When
lapw1c runs, after about 2 hours it crashes with the following
message printed to the screen:
  ** Address Error **
  End of diagnostics

If I decrease the matrix size by reducing NMATMAX to 5000, so it's
only a 500 MB job, it runs fine.  

Any ideas on why this would be happening?

- -- 
Jeff Spirko   spirko@lehigh.edu   spirko@yahoo.com   WD3V   |=>

The study of non-linear physics is like the study of non-elephant biology.

All theoretical chemistry is really physics;
and all theoretical chemists know it. -- Richard P. Feynman 
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------------------------------

Date: Fri, 08 Nov 2002 19:41:44 +0200
From: thor <thor@mpi-halle.mpg.de>
Subject: Re: [WIEN]: automatic geometry optimisation

====
thor <thor@mpi-halle.mpg.de>
submitted the following contribution:
====

Well, it is the best available option. The only other one is 'by hand', writing
your own automatisation scripts.

Anyway, it is not so difficult to use, once it is started. It is, however,
rather expensive, but if you want to do optimisation of the internal parameters
in the structure, it is the only way to do it.

It seems like vasp takes just as long time (at least for systems containing W
and Fe), and what comes out of it says more about the pseudopotential than about
the structure :-(

The terms of the Hamiltonian that would make it 'do it by itself' are generally
left out in DFT, and they would probably make it much slower, if at all
possible.

Did that answer your question?

Best regards,
Torsten Andersen.

chen0130@flinders.edu.au wrote:

> ====
> chen0130@flinders.edu.au
> submitted the following contribution:
> ====
>
> Thanks, I guess I am asking a silly question, but my emphasis is on
> 'automatic'! (ie something done in symmetry?) without the expensive mini_lapw
>
> could someone suggest some generic reasons why geometry optimisations are not
> necessarily performed for solid state structures?
>
> there seems to be publications without relaxing supercells...
>
> sorry to be so broad, appreciating any remarks,
>
> Thanks,
>
> Cheng
>
> Quoting Torsten Andersen <Torsten.Andersen@Fysik.UU.se>:
>
> > ====
> > Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> > submitted the following contribution:
> > ====
> >
> > min_lapw and mini (see, e.g., sec. 8.14 in UG).
> >
> > chen0130@flinders.edu.au wrote:
> >
> > >====
> > >chen0130@flinders.edu.au
> > >submitted the following contribution:
> > >====
> > >
> > >Dear Wien users,
> > >
> > >Can any one tell me if there is any automatic geometry optimisation of any
> >
> > >degree in Wien97?
> > >
> > >Thanks
> > >
> > >Cheng
> > >
> > >
> > >====
> > >WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > >To (un)subscribe send mail to
> > >majordomo@zeus.theochem.tuwien.ac.at
> > >====
> > >
> > >
> >
> > --
> > Dr. Torsten Andersen
> > Department of Physics, Condensed Matter Theory Group, Uppsala University
> > UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
> > News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics
> >
> >
> >
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
> > majordomo@zeus.theochem.tuwien.ac.at
> > ====
> >
> >
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
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------------------------------

Date: Fri, 8 Nov 2002 16:06:35 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: dstart problem

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

After I run "run_lapw" for my mineral thomsenolite with H2O in the unit
cell, I was told:

no thomsenolite.clmsum(_old) file found, which is necessary for lapw0 !


So I re-run dstart, I meet such a problem as in dstart.error:

'DSTART' - can't open unit: 15
'DSTART' -        filename: thomsenolite.in2
'DSTART' -          status: old          form: formatted

Could you please help me out?


Thanks!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Fri, 8 Nov 2002 17:22:39 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: dstart problem 

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---559023410-1804928587-1036797759=:14957
Content-Type: TEXT/PLAIN; charset=US-ASCII

Hi again:

I attach the case.struct and case.inst files with this email for help.



Dear All:

After I run "run_lapw" for my mineral thomsenolite with H2O in the unit
cell, I was told:

no thomsenolite.clmsum(_old) file found, which is necessary for lapw0 !


So I re-run dstart, I meet such a problem as in dstart.error:

'DSTART' - can't open unit: 15
'DSTART' -        filename: thomsenolite.in2
'DSTART' -          status: old          form: formatted

Could you please help me out?


Thanks!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395


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------------------------------

Date: Sat, 9 Nov 2002 08:57:51 +0330
From: "akbarzad" <akbarzad@cc.iut.ac.ir>
Subject: [WIEN]: Fellowship at Isfahan University of Technology

====
"akbarzad" <akbarzad@cc.iut.ac.ir>
submitted the following contribution:
====

                               Fellowship available at Isfahan University of
Technology
The computational condensed matter group physics department of Isfahan
University of Technology (IUT) is going to expand its regional scientific
activity by acting as an ICTP Affiliated Centre. Following such a mission,
the Abdus Salam International Centre for Theoretical Physics (ICTP) and IUT
have agreed to support the below mentioned fellowships for the year 2003:
One) 2 Fellowship for young researchers ( possessing a PhD degree or at the
final stages of getting it) from the regional countries (Western South Asia,
Central Asia, and Middle East ) to come and work in the center as long term
visitors (3-6 months).
Two) 2  Fellowship for senior researchers from the regional countries to
come and work in the center as short term visitors (4-12 weeks).
The applicants are expected to have a keen interest in computational
condensed matter physics, with some hands on experience on first principle
methods.
The fellowships are available from 1st of January 2003.
Applications including, a full CV, a list of publications, an abstract of
her/his research achievements (within one page of an A4 sheet), a proposal
of about 500 words explaining the details of the research project that the
applicant  is going to perform during the stay in the center, and names and
addresses (email) of two or three referees should be sent to the following
address:

Professor Hadi Akbarzadeh
 Department of Physics , Isfahan University of Technology, Isfahan, Iran
 email: akbarzad@cc.iut.ac.ir, Tel: +98-311-3912375 (or 3913700),  fax:
+98-311-3912376.

Accepted candidates are entitled for the following supports:
1. Travel expenses by economy round trip air ticket.
2. Accommodation in IUT Guest House.
3. 400 Euro per month for living expenses ( For senior researchers it can be
increased to 500 Euro).
4. One full meal per day.

Current research interests of the center
Electronic structure calculations, as a valuable tool for understanding the
properties of condensed matter, are the main current activity in the
computational condensed matter group in physics department of Isfahan
University of Technology.
Our calculations are within the density functional theory using FP-LAPW
method. We have access and hands on experience to work with WIEN2k code
(www.wien2k.at). This general purpose electronic structure code is a very
appropriate tool to calculate many properties of a solid: band structure,
density of states, equilibrium geometry, magnetic structure, electric-field
gradients,  hyperfine fields, and X-ray spectra, etc. The code contains
LDA+U to study highly correlated systems.
The ongoing research projects in the group are as follow:
1. Structural, electronic and magnetic properties of MnAs.
2. Structural and electronic properties of CeFe2.
3. Investigation the valency of rare earth elements  in RIn3 and RSn3: Ab
initio analysis of electric field gradients
4. Investigation of the valency of Actanides in USn3, UIn3, and NpIn3 by
ab-initio methods.
5. First principle calculation of hyperfine fields and local relaxation at
4d and 5sp impurities in bcc Cr.




====
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------------------------------

Date: Sat, 9 Nov 2002 15:22:16 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- --143914132-1593261418-1036826536=:16879
Content-Type: TEXT/PLAIN; charset=US-ASCII

Dear all,

I am sorry that I already have question with WIEN97.

Actually, I would like to put the same molecule (20 carbon atoms) in boxes 
with different dimensions and perform the calculations. And all the 3 
inputed .struct files with only 1 inequivalent atom (I just list all the 
20 carbon atoms together). However, WIEN97 classifies this 3 cases 
differently. Why? 

For my input value of nn=2 for all 3 cases.

Case 1 : The box's dimensions are 10AX10AX2.46124419755538A

After NN, WIEN97 generates 10 inequvialent atoms to me.

Case 2 : The box's dimensions are 12AX12AX2.46124419755538A

After NN, WIEN97 generates 8 inequivalent atoms to me.

Case 3 : The box's dimensions are 14AX14AX2.46124419755538A

After NN, WIEN97 generates 1 inequivalent atoms to me.

I have attached the following files with the mail.

original.xyz ------ original XYZ coordinates file
case10A.struct_init ------ initial .struct file inputed by my own with the  
                           box's dimension of 10X10X2.461244
case12A.struct_init ------ initial .struct file inputed by my own with the  
                           box's dimension of 12X12X2.461244
case14A.struct_orig ------ initial .struct file inputed by my own with the  
                           box's dimension of 14X14X2.461244
case10A.struct ------ .struct file generated by WIEN97 after NN with the  
                      box's dimension of 10X10X2.461244
case12A.struct ------ .struct file generated by WIEN97 after NN with the  
                      box's dimension of 12X12X2.461244
case14A.struct ------ .struct file generated by WIEN97 after NN with the   
                      box's dimension of 14X14X2.461244


Thank you very much

Martin

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- --143914132-1593261418-1036826536=:16879--
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Date: Sat,  9 Nov 2002 21:33:59 +1100
From: chen0130@flinders.edu.au
Subject: Re: [WIEN]: automatic geometry optimisation

====
chen0130@flinders.edu.au
submitted the following contribution:
====

Thanks for you reply!

I wonder then, there are surely good reasons (apart from the expense) that
people will not relax their structures?

Could someone share their experience?

Many thanks!

Cheng

Quoting thor <thor@mpi-halle.mpg.de>:

> ====
> thor <thor@mpi-halle.mpg.de>
> submitted the following contribution:
> ====
> 
> Well, it is the best available option. The only other one is 'by hand',
> writing
> your own automatisation scripts.
> 
> Anyway, it is not so difficult to use, once it is started. It is, however,
> rather expensive, but if you want to do optimisation of the internal
> parameters
> in the structure, it is the only way to do it.
> 
> It seems like vasp takes just as long time (at least for systems containing
> W
> and Fe), and what comes out of it says more about the pseudopotential than
> about
> the structure :-(
> 
> The terms of the Hamiltonian that would make it 'do it by itself' are
> generally
> left out in DFT, and they would probably make it much slower, if at all
> possible.
> 
> Did that answer your question?
> 
> Best regards,
> Torsten Andersen.
> 
> chen0130@flinders.edu.au wrote:
> 
> > ====
> > chen0130@flinders.edu.au
> > submitted the following contribution:
> > ====
> >
> > Thanks, I guess I am asking a silly question, but my emphasis is on
> > 'automatic'! (ie something done in symmetry?) without the expensive
> mini_lapw
> >
> > could someone suggest some generic reasons why geometry optimisations are
> not
> > necessarily performed for solid state structures?
> >
> > there seems to be publications without relaxing supercells...
> >
> > sorry to be so broad, appreciating any remarks,
> >
> > Thanks,
> >
> > Cheng
> >
> > Quoting Torsten Andersen <Torsten.Andersen@Fysik.UU.se>:
> >
> > > ====
> > > Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> > > submitted the following contribution:
> > > ====
> > >
> > > min_lapw and mini (see, e.g., sec. 8.14 in UG).
> > >
> > > chen0130@flinders.edu.au wrote:
> > >
> > > >====
> > > >chen0130@flinders.edu.au
> > > >submitted the following contribution:
> > > >====
> > > >
> > > >Dear Wien users,
> > > >
> > > >Can any one tell me if there is any automatic geometry optimisation of
> any
> > >
> > > >degree in Wien97?
> > > >
> > > >Thanks
> > > >
> > > >Cheng
> > > >
> > > >
> > > >====
> > > >WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > > >To (un)subscribe send mail to
> > > >majordomo@zeus.theochem.tuwien.ac.at
> > > >====
> > > >
> > > >
> > >
> > > --
> > > Dr. Torsten Andersen
> > > Department of Physics, Condensed Matter Theory Group, Uppsala
> University
> > > UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW:
> http://deep.at/myspace
> > > News on TA-WWW: Two publ. articles on ab initio nonlinear
> magneto-optics
> > >
> > >
> > >
> > > ====
> > > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > > To (un)subscribe send mail to
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> > > ====
> > >
> > >
> >
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
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> 
> 



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------------------------------

Date: Sun, 10 Nov 2002 10:04:39 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: automatic geometry optimisation

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> chen0130@flinders.edu.au
> submitted the following contribution:
> ====
> 
> I wonder then, there are surely good reasons (apart from the expense) that
> people will not relax their structures?

Everything depends on the accuracy you need. If you can afford it, relaxing is 
always the better (=more accurate option). If you cannot afford it for all 
aspects of your problem, then you must at least test to what extent omitting 
relaxation will affect the properties in which you're interested. Imagine you 
compare total energies of two cases, and you want to decide which of both is 
lowest. If the difference is 0.1 Ry, and you have checked that relaxation 
affects the energy at the 0.01 Ry level, then it is save to neglect relaxation. 
If relaxation has a 0.1 Ry effect as well, then your results without relaxation 
are useless. Some properties are very sensitive to relaxation (electric-field 
gradients (:EFG) can be changed by 100% or more), others are usually much less 
affected (e.g. magnetic moments (:MMI)).

If you don't need high accuracy because you want to make conclusions on a 
qualitative level, then relaxation is often not needed at all.

Stefaan
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Date: Mon, 11 Nov 2002 15:18:23 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

I get a question like : How to increase the number of k-point in the 
bandstructure plot? 

Actually, I have used 1000 k-point for KGEN and SCF cycle and my  
bandstructure plot only having 20 k-point from R to gramma. After the  
SCF, I modify the .in1 file by inserting the k-point by copying the  
$WIENROOT/SRC_templates/simple_cublic.klist into .in1 file and change 
unit to 5.

Is it something mismatch for my action?

On the other hand, what are the meaning for the data in columns 2 to 6 in 
the file $WIENROOT/SRC_templates/simple_cublic.klist?

Thank you very much

Martin 

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------------------------------

Date: Mon, 11 Nov 2002 09:09:17 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Question

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I am sorry that I already have question with WIEN97.
>
> Actually, I would like to put the same molecule (20 carbon atoms) in boxes
> with different dimensions and perform the calculations. And all the 3
> inputed .struct files with only 1 inequivalent atom (I just list all the
> 20 carbon atoms together). However, WIEN97 classifies this 3 cases
> differently. Why?
>
> For my input value of nn=2 for all 3 cases.
>
> Case 1 : The box's dimensions are 10AX10AX2.46124419755538A
>
> After NN, WIEN97 generates 10 inequvialent atoms to me.
>
> Case 2 : The box's dimensions are 12AX12AX2.46124419755538A
>
> After NN, WIEN97 generates 8 inequivalent atoms to me.
>
> Case 3 : The box's dimensions are 14AX14AX2.46124419755538A
>
> After NN, WIEN97 generates 1 inequivalent atoms to me.

This is because nn has certain limits up to which nn-distances are
considered and for large boxes it will not "count" any cell-cell interactions.

WIEN2k (sgroup) gives for all struct files 10 inequivalent atoms.

Regards

PS: Maybe you should upgrade ? Or get yourself a book about cristallography.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Sun, 10 Nov 2002 09:24:40 +0100
From: Peer Kruse <kruse@lem.uni-karlsruhe.de>
Subject: Re: [WIEN]: Address Error in lapw1

====
Peer Kruse <kruse@lem.uni-karlsruhe.de>
submitted the following contribution:
====

Have you checked the amount of ram with ulimit or the quality of your 
ram with
memtest86? If it's a new machine I would recommend testing the ram as 
well as I have been told
it is rather erraneous in the last time. But I don't know if this
is the reason behind your problem.
Have a look at www.memtest86.com for the (free) software.

Peer


Jeff Spirko wrote:

>====
>Jeff Spirko <spirko@lehigh.edu>
>submitted the following contribution:
>====
>
>I'm having a problem with lapw1 in a large (> 1 GB RAM, 10000 matrix
>size, RKM=7.0) job.  I have already checked the available RAM,
>diskspace, and stack size.
>
>  Version:          WIEN2k_02 from Oct 24, 2002
>  Computer:         Pentium IV with 2 GB RDRAM
>  Operating System: Redhat Linux 8.0
>  Compiler:         IFC 6.0
>  FOPT:             -O0 -FR -mp -w -tpp7
>  LDFLAGS:          -Vaxlib -L../SRC_lib
>  R_LIBS:           -llapack_lapw -lmkl_p4 -lguide -lpthread
>
>I have successfully run the job on an SGI, and I just transferred
>over the .struct, .in*, .kgen, .klist, and .clmsum files.  When
>lapw1c runs, after about 2 hours it crashes with the following
>message printed to the screen:
>  ** Address Error **
>  End of diagnostics
>
>If I decrease the matrix size by reducing NMATMAX to 5000, so it's
>only a 500 MB job, it runs fine.  
>
>Any ideas on why this would be happening?
>



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------------------------------

Date: Mon, 11 Nov 2002 11:10:16 +0100
From: KOITZSCH Christian <christian.koitzsch@unifr.ch>
Subject: [WIEN]: H saturation of slab surface

====
KOITZSCH Christian <christian.koitzsch@unifr.ch>
submitted the following contribution:
====

Hi Everybody,

I have a question regarding slab calculations. I am trying to calculate an
adsorbed layer of atoms A (in my case yttrium) on a substrate B (silicon).
Now I would like to get rid of the contributions from the substrate
"surface" - so I thought about saturating the bottom of my slab with
hydrogen atoms, but it turns out, that this method is really expensive,
since the resulting small muffin tin radii, gives me a lot of plane waves
and correspondingly a lot of computation time. Can somebody give me an
advise, how to proceed in a more clever way? I used a bondlength of 1.55
Angstroem for the Si-H bond, is this reasonable?

Thanks a lot

Christian Koitzsch
University of Fribourg
Department of Physics
CH-1700 Fribourg

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------------------------------

Date: Mon, 11 Nov 2002 12:14:21 +0100 (MEZ)
From: "A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
Subject: Re: [WIEN]: H saturation of slab surface

====
"A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
submitted the following contribution:
====

On Mon, 11 Nov 2002, KOITZSCH Christian wrote:

> ====
> KOITZSCH Christian <christian.koitzsch@unifr.ch>
> submitted the following contribution:
> ====
>
> Hi Everybody,
>
> I have a question regarding slab calculations. I am trying to calculate an
> adsorbed layer of atoms A (in my case yttrium) on a substrate B (silicon).
> Now I would like to get rid of the contributions from the substrate
> "surface" - so I thought about saturating the bottom of my slab with
> hydrogen atoms, but it turns out, that this method is really expensive,
> since the resulting small muffin tin radii, gives me a lot of plane waves
> and correspondingly a lot of computation time. Can somebody give me an
> advise, how to proceed in a more clever way? I used a bondlength of 1.55
> Angstroem for the Si-H bond, is this reasonable?
>

Dear Christian,
why don't you put Y on both sides of your slab?
(if you are not interested in the free Si surface anyway).
Just make sure that your Y-Y distance is large enough
both across the substrate and across the vacuum.
As you'll hopefully make use of some extra symmetry
in your supercell, the introduction of extra atoms will
probably pay off.

Regards,

Andrei Postnikov

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------------------------------

Date: Mon, 11 Nov 2002 15:43:09 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: H saturation of slab surface

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I have a question regarding slab calculations. I am trying to calculate an
> adsorbed layer of atoms A (in my case yttrium) on a substrate B (silicon).
> Now I would like to get rid of the contributions from the substrate
> "surface" - so I thought about saturating the bottom of my slab with
> hydrogen atoms, but it turns out, that this method is really expensive,
> since the resulting small muffin tin radii, gives me a lot of plane waves
> and correspondingly a lot of computation time. Can somebody give me an
> advise, how to proceed in a more clever way? I used a bondlength of 1.55
> Angstroem for the Si-H bond, is this reasonable?

As was mentioned before, at least when you have inversion symmetry, it
often makes sense to add the adlayer on both sides. (I must admit,
sometimes the adlayer-adlayer interaction through the "bulk" is strong and
one needs many layers, but there is also no guarantee that there is not some
spurious interaction between two different surfaces)

If you want to saturate one surface with H, choose small spheres for H
(do not change the Si-radius), and adjust RKMAX according to the ratio
of R_Si/R-H to 3-4.
This way the number of PW is not increased, Si and Y are as accurately
converged as you like and H is even with a RKMax=3 reasonably converged
and in addition poor H-convergence should not matter too much.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 11 Nov 2002 08:35:53 -0800 (PST)
From: Claudio Lee <claudio_lee1@yahoo.com>
Subject: [WIEN]: OP calcualtion (again!)

====
Claudio Lee <claudio_lee1@yahoo.com>
submitted the following contribution:
====

Dear Pavel, Gerd and all,
After I have installeded for the latest vesion I got a
new problem when runing -so -orb (my system is still
the same as my previous mentioned one). 
After initialling for input files (with initso has
been involved in it, files *inorb and *indmc have been
created as well), I use runsp_lapw -so -orb -i 5 to
calculate it. The first iteration seems okay but after
that (second iteraion and so on) the errors happen in
*err file as I give below:
====
hup: Command not found.
STOP  LAPW0 END
STOP  LAPW1 END
STOP  LAPW1 END
STOP LAPWSO END
STOP  LAPW2 END
STOP  LAPW2 END
STOP  lapwdm END
STOP  CORE  END
STOP  CORE  END
STOP  MIXER END
hup: Command not found.
STOP  LAPW0 END
1525-097 A READ statement using decimal base input
found the invalid digit '.' in the input file.
 The program will recover by assuming a zero in its
place.
STOP  orbital potential calculation END
1525-097 A READ statement using decimal base input
found the invalid digit '.' in the input file.
 The program will recover by assuming a zero in its
place.
STOP  orbital potential calculation END
if: Badly formed number.
====   
If however, after runsp_lapw -so (not yet -orb) has
converged I allowed -orb to be involved following this
by running runsp_lapw -so -orb  then the program has
been stopped just after lapw2 done (from first
iteration), in *err it looks like (nothing happens in
*error files):
===
hup: Command not found.
STOP  LAPW0 END
STOP  LAPW1 END
STOP  LAPW1 END
STOP LAPWSO END
STOP  LAPW2 END
===
So Pavel or Gerd (or anyone), if you do know how to
solve this problem could you please help me?

Thank you so much in advance.

Claudio.


__________________________________________________
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U2 on LAUNCH - Exclusive greatest hits videos
http://launch.yahoo.com/u2
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------------------------------

Date: Tue, 12 Nov 2002 09:20:04 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: [WIEN]: NWAV too small in rdswar.f

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear developers,

after upgrading to Wien2k_02 (19/9-2) I get a peculiar little message 
from lapw1, telling me that "NWAV too small in rdswar.f" in the 
case.dayfile. Is that something to worry about? What can I do about it?

I don't see NWAV in rdswar.f, and in the param.inc file it is not 
present, so it must be internal. I have 50749 plane-waves, but I 
remember that in Wien2k_01 the maximum allowed PW's were increased to 1 
million.

Best regards,
Torsten Andersen.

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics


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------------------------------

Date: Tue, 12 Nov 2002 14:02:43 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: NWAV too small in rdswar.f

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

I am sorry for that... I mixed up my path, so the wrong executable was 
selected. Now it is ok.

Best regards,
Torsten Andersen.

Torsten Andersen wrote:

> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
>
> Dear developers,
>
> after upgrading to Wien2k_02 (19/9-2) I get a peculiar little message 
> from lapw1, telling me that "NWAV too small in rdswar.f" in the 
> case.dayfile. Is that something to worry about? What can I do about it?
>
> I don't see NWAV in rdswar.f, and in the param.inc file it is not 
> present, so it must be internal. I have 50749 plane-waves, but I 
> remember that in Wien2k_01 the maximum allowed PW's were increased to 
> 1 million.
>
> Best regards,
> Torsten Andersen.
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Tue, 12 Nov 2002 12:01:51 -0800 (PST)
From: yanming Ma <ymma66@yahoo.com>
Subject: [WIEN]: fblacs lib error

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-877359211-1037131311=:47798
Content-Type: text/plain; charset=us-ascii


Dear wien2k users,

When I try to setup Wien2k in our SGI machines to use Fine Grained parallel calculation, I get a error message from library "fblacs" as the following

I/O error (-Lfblacs): no such file or directory.

I just wonder where can I get the library "lfblacs".

Please help me. I will highly appreciate your help. 


Yanming Ma Ph.D
Steacie Institute for Molecular Sciences,
National Research Councils of Canada,
Ottawa, Ontario
K1A 0R6
Canada


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- --0-877359211-1037131311=:47798
Content-Type: text/html; charset=us-ascii

<P>Dear wien2k users,</P>
<P>When I try to setup Wien2k in our SGI machines to use Fine Grained parallel calculation, I get a error message from library "fblacs" as the following</P>
<P>I/O error (-Lfblacs): no such file or directory.</P>
<P>I just wonder&nbsp;where can I&nbsp;get the library "lfblacs".</P>
<P>Please help me. I will highly appreciate your help.&nbsp;</P><BR><BR>Yanming Ma Ph.D<br>Steacie Institute for Molecular Sciences,<br>National Research Councils of Canada,<br>Ottawa, Ontario<br>K1A 0R6<br>Canada<p><br><hr size=1>Do you Yahoo!?<br>
<a href="http://rd.yahoo.com/launch/mailsig/*http://launch.yahoo.com/u2">U2 on LAUNCH</a> - Exclusive medley & videos from Greatest Hits CD
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------------------------------

Date: Tue, 12 Nov 2002 20:57:58 -0500 (EST)
From: Harry Gotsis <gotsis@dave.nrl.navy.mil>
Subject: Re: [WIEN]: Question

====
Harry Gotsis <gotsis@dave.nrl.navy.mil>
submitted the following contribution:
====

On Mon, 11 Nov 2002, Ma Chi Chiu wrote:
Dear Martin:

In order to have more k-points (let's say twice) in
the band-structure plot, simply double the number 
of divisions in simple_cubic.klist (i.e. change idv 
from 40 to 80) and then add manually more k-points.

Regards,

Harry Gotsis
> ====
> Ma Chi Chiu <martin@yangtze.hku.hk>
> submitted the following contribution:
> ====
> 
> Dear all,
> 
> I get a question like : How to increase the number of k-point in the 
> bandstructure plot? 
> 
> Actually, I have used 1000 k-point for KGEN and SCF cycle and my  
> bandstructure plot only having 20 k-point from R to gramma. After the  
> SCF, I modify the .in1 file by inserting the k-point by copying the  
> $WIENROOT/SRC_templates/simple_cublic.klist into .in1 file and change 
> unit to 5.
> 
> Is it something mismatch for my action?
> 
> On the other hand, what are the meaning for the data in columns 2 to 6 in 
> the file $WIENROOT/SRC_templates/simple_cublic.klist?
> 
> Thank you very much
> 
> Martin 
> 
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End of wien-digest V2002 #42
****************************

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To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #43
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Sender: owner-wien-digest@theochem.tuwien.ac.at
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wien-digest       Thursday, November 14 2002       Volume 2002 : Number 043




----------------------------------------------------------------------

Date: Wed, 13 Nov 2002 09:20:55 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: fblacs lib error

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Ms. Ma,

you can search for it using the "find" command. If it is not there, 
maybe MPI is not installed correct? As this is supposed to be a 
"standard library", ask your system administrator, or search for it in 
SGI's documentation, which should be online on your system.

Best regards,
Torsten Andersen.

yanming Ma wrote:

> Dear wien2k users,
>
> When I try to setup Wien2k in our SGI machines to use Fine Grained 
> parallel calculation, I get a error message from library "fblacs" as 
> the following
>
> I/O error (-Lfblacs): no such file or directory.
>
> I just wonder where can I get the library "lfblacs".
>
> Please help me. I will highly appreciate your help. 
>
>
>
> Yanming Ma Ph.D
> Steacie Institute for Molecular Sciences,
> National Research Councils of Canada,
> Ottawa, Ontario
> K1A 0R6
> Canada
>
>
> ------------------------------------------------------------------------
> Do you Yahoo!?
> U2 on LAUNCH 
> <http://rd.yahoo.com/launch/mailsig/*http://launch.yahoo.com/u2> - 
> Exclusive medley & videos from Greatest Hits CD 


- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Wed, 13 Nov 2002 13:50:54 +0000
From: ecat@nfrn-mail.org.uk
Subject: [WIEN]: To ask about case.vector

====
ecat@nfrn-mail.org.uk
submitted the following contribution:
====

Dear all,

We often need this file case.vector when we calculate properties.
Please,tell me, how and when is this file created? Thanks!

Ecat
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------------------------------

Date: Wed, 13 Nov 2002 14:59:43 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: To ask about case.vector

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

in LAPW1, every time you run it. But wait, that information is in the 
manual... so read the manual.

Best regards,
Torsten Andersen.

ecat@nfrn-mail.org.uk wrote:

>====
>ecat@nfrn-mail.org.uk
>submitted the following contribution:
>====
>
>Dear all,
>
>We often need this file case.vector when we calculate properties.
>Please,tell me, how and when is this file created? Thanks!
>
>Ecat
>====
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>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Wed, 13 Nov 2002 14:21:46 +0000 (GMT)
From: David Pankhurst <david.pankhurst@materials.oxford.ac.uk>
Subject: Re: [WIEN]: fblacs lib error

====
David Pankhurst <david.pankhurst@materials.oxford.ac.uk>
submitted the following contribution:
====

Dear Yanming,

It looks to me like you have mistyped the linker option.  Should be
- -lfblacs, not -Lfblacs.  A big -L should be followed by a directory to add
to the library search path, a little -l should be followed by the name of
the library you want to link with the "lib" prefix removed.  i.e. to link
libfblacs.a use -lfblacs.

best regards,

	Dave Pankhurst

On Tue, 12 Nov 2002, yanming Ma wrote:

> 
> Dear wien2k users,
> 
> When I try to setup Wien2k in our SGI machines to use Fine Grained parallel calculation, I get a error message from library "fblacs" as the following
> 
> I/O error (-Lfblacs): no such file or directory.
> 
> I just wonder where can I get the library "lfblacs".
> 
> Please help me. I will highly appreciate your help. 
> 
> 
> Yanming Ma Ph.D
> Steacie Institute for Molecular Sciences,
> National Research Councils of Canada,
> Ottawa, Ontario
> K1A 0R6
> Canada
> 
> 
> ---------------------------------
> Do you Yahoo!?
> U2 on LAUNCH - Exclusive medley & videos from Greatest Hits CD

+---------------------------------+------------------------------------+
| Dr David Pankhurst,             | Tel : +44 1865 283325/283326       |
| Department of Materials,        | Fax : +44 1865 273789              |    
| University of Oxford,           |                                    |
| Parks Road, Oxford OX1 3PH, UK  | david.pankhurst@materials.ox.ac.uk |
+---------------------------------+------------------------------------+

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------------------------------

Date: Wed, 13 Nov 2002 18:29:43 +0100
From: Maciej Luszczek <maclu@task.gda.pl>
Subject: [WIEN]: kgen

====
Maciej Luszczek <maclu@task.gda.pl>
submitted the following contribution:
====

Dear  WIEN2k users,
I have just installed wien2k on the machine (SGI Origin 2000/Onyx 2, 16
MIPS R12000 and 8 MIPS R10000 processors, 16 GB RAM, 80 GB disk storage, 12.8
GFLOPs) and some problems with kgen are occurring:

> kgen kgen.def  (or  >x kgen)
  Segmentation fault (core dumped)


The program was compiled with the following options (in Makefile):
FC = f90
FOPT     = -O -mips4 -r10000 -freeform -64
FGEN     =
LDFLAGS  = -mips4 -r10000 -64
LIBS     =
DESTDIR  = ./
EXECNAME = kgen

Surprisingly, the previous version of kgen (from WIEN97 package) works
properly...  The compilation has been performed with the low
optimization, so, perhaps it is a bug?

I would be grateful if someone could help me with this.

Best regards,
Maciej Luszczek






- -- 
Dr. Maciej Luszczek
Faculty of Applied Physics and Mathematics
Gdansk University of Technology
G. Narutowicza 11/12
80-952 Gdansk
POLAND

Phone: +4858 3471095
Fax:   +4858 3472821

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------------------------------

Date: Wed, 13 Nov 2002 17:02:27 -0200 (BDB)
From: vivienne denise falcao <vdfalcao@dedalus.lcc.ufmg.br>
Subject: [WIEN]: X-Ray Spectra

====
vivienne denise falcao <vdfalcao@dedalus.lcc.ufmg.br>
submitted the following contribution:
====

                         Dear All,

      My problems with energy range for x-ray absorption spectra remains.
I am using an old version of Wien97 and the case.in1 that I get is


===============================================================================
WFFIL        (WFPRI, SUPWF)
  9.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
   .30    4      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
 1     .30       .000 CONT
 1   -4.49       .005 STOP
 2     .30       .010 CONT
 0     .30       .000 CONT
   .30    5      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
 2     .30       .000 CONT
 2   -2.92       .005 STOP
 0    -.77       .010 CONT
 0     .30       .000 CONT
 1     .30       .000 CONT
K-VECTORS FROM UNIT:4
===============================================================================

In this file there insn't limit of energy window. I tryed to include the
limit of energy window in this file but the maximum energy didn't
change.
The case.int that I obtain is

===============================================================================

Autocreate Title: Atom 1 L3 absorption spectrum
 -0.141130343782713830 0.146996137513085530E-02 1.69632137513085546
 2
    1    3      l+1
    0    1      tot
===============================================================================

I already did all that Saeid and Torsten suggested and I didn't exchange
the energy range.

What can I do?
How can I to obtain a new version of Wien97?

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------------------------------

Date: Thu, 14 Nov 2002 06:09:10 +0530 (IST)
From: Nitya Nath <nitya@iitk.ac.in>
Subject: Re: [WIEN]: kgen

====
Nitya Nath <nitya@iitk.ac.in>
submitted the following contribution:
====



Hi..
Please use this command 'unlimit' before running x kgen.
It is not a bug..
with regards..
Nitya

> ====
> Maciej Luszczek <maclu@task.gda.pl>
> submitted the following contribution:
> ====
> 
> Dear  WIEN2k users,
> I have just installed wien2k on the machine (SGI Origin 2000/Onyx 2, 16
> MIPS R12000 and 8 MIPS R10000 processors, 16 GB RAM, 80 GB disk storage, 12.8
> GFLOPs) and some problems with kgen are occurring:
> 
> > kgen kgen.def  (or  >x kgen)
>   Segmentation fault (core dumped)
> 
> 
> The program was compiled with the following options (in Makefile):
> FC = f90
> FOPT     = -O -mips4 -r10000 -freeform -64
> FGEN     =
> LDFLAGS  = -mips4 -r10000 -64
> LIBS     =
> DESTDIR  = ./
> EXECNAME = kgen
> 
> Surprisingly, the previous version of kgen (from WIEN97 package) works
> properly...  The compilation has been performed with the low
> optimization, so, perhaps it is a bug?
> 
> I would be grateful if someone could help me with this.
> 
> Best regards,
> Maciej Luszczek
> 
> 
> 
> 
> 
> 
> 

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------------------------------

Date: Wed, 13 Nov 2002 15:05:55 -0500
From: Jeff Spirko <spirko@lehigh.edu>
Subject: Re: [WIEN]: kgen

====
Jeff Spirko <spirko@lehigh.edu>
submitted the following contribution:
====

More specifically, if you use a Bourne-type shell (bash, sh, ksh),
enter (You may have to pick a number instead of unlimited.):
  ulimit -s unlimited
If you use a c-shell, enter:
  limit stacksize unlimited
You have to do this every time you log in, so you may want to put it
in your .profile or .login.

On Thu, Nov 14, 2002 at 06:09:10AM +0530, Nitya Nath wrote:
> Please use this command 'unlimit' before running x kgen.
> It is not a bug..
> with regards..
> Nitya

> > > kgen kgen.def  (or  >x kgen)
> >   Segmentation fault (core dumped)

- -- 
Jeff Spirko   spirko@lehigh.edu   spirko@yahoo.com   WD3V   |=>

The study of non-linear physics is like the study of non-elephant biology.

All theoretical chemistry is really physics;
and all theoretical chemists know it. -- Richard P. Feynman 
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------------------------------

Date: Thu, 14 Nov 2002 08:13:29 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: X-Ray Spectra

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

We were just assuming you used Wien2k.

The energy range in Wien97 is in case.klist. 1st line to the right.

Best regards,
Torsten Andersen.

vivienne denise falcao wrote:

>====
>vivienne denise falcao <vdfalcao@dedalus.lcc.ufmg.br>
>submitted the following contribution:
>====
>
>                         Dear All,
>
>      My problems with energy range for x-ray absorption spectra remains.
>I am using an old version of Wien97 and the case.in1 that I get is
>
>
>===============================================================================
>WFFIL        (WFPRI, SUPWF)
>  9.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
>   .30    4      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
> 1     .30       .000 CONT
> 1   -4.49       .005 STOP
> 2     .30       .010 CONT
> 0     .30       .000 CONT
>   .30    5      (GLOBAL E-PARAMETER WITH n OTHER CHOICES)
> 2     .30       .000 CONT
> 2   -2.92       .005 STOP
> 0    -.77       .010 CONT
> 0     .30       .000 CONT
> 1     .30       .000 CONT
>K-VECTORS FROM UNIT:4
>===============================================================================
>
>In this file there insn't limit of energy window. I tryed to include the
>limit of energy window in this file but the maximum energy didn't
>change.
>The case.int that I obtain is
>
>===============================================================================
>
>Autocreate Title: Atom 1 L3 absorption spectrum
> -0.141130343782713830 0.146996137513085530E-02 1.69632137513085546
> 2
>    1    3      l+1
>    0    1      tot
>===============================================================================
>
>I already did all that Saeid and Torsten suggested and I didn't exchange
>the energy range.
>
>What can I do?
>How can I to obtain a new version of Wien97?
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

End of wien-digest V2002 #43
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #44
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
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wien-digest       Thursday, November 21 2002       Volume 2002 : Number 044




----------------------------------------------------------------------

Date: Thu, 14 Nov 2002 08:27:11 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: X-Ray Spectra

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>       My problems with energy range for x-ray absorption spectra remains.
> I am using an old version of Wien97 and the case.in1 that I get is

In WIEN97 the energy range was set in the first line of case.klist.

> How can I to obtain a new version of Wien97?

Have a look at   www.wien2k.at

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 14 Nov 2002 09:06:21 +0000
From: Paula <pauhar@chem.gla.ac.uk>
Subject: [WIEN]: hup: Command not found

====
Paula <pauhar@chem.gla.ac.uk>
submitted the following contribution:
====

Dear Wien users,

I am using wien2k on a dec compaq operating system. The c-shell command 
'hup' is not recognised and l have copied the first part of the STDOUT file 
below. The scf cycle continues, but when l try to run any tasks (elnes, dos 
etc.) they crash. I would like to know if anyone else has found a similar 
error message and what l can do about it. Is it possible to write a script 
to replace this command? What does this command actually do?
Thanks for your help,

Paula

STDOUT:
hup: Command not found.
  LAPW0 END
  LAPW1 END
  LAPW1 END
LAPW2 - FERMI; weighs written
  LAPW2 END
  LAPW2 END
  SUMPARA END
  SUMPARA END
  CORE  END
  MIXER END
in cycle 2    ETEST: 0   CTEST: 0
hup: Command not found.
  LAPW0 END
  LAPW1 END
  LAPW1 END
LAPW2 - FERMI; weighs written
  LAPW2 END
  LAPW2 END
  SUMPARA END
  SUMPARA END
  CORE  END

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------------------------------

Date: Thu, 14 Nov 2002 11:30:22 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: hup: Command not found

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Dear Paula,

the hup command is not important.  You can safely ignore this message.  If
it bothers you, remove the hup command from run_lapw-script.  Or just ignore
it.

kind regards,

Kevin.
kevin.jorissen@ua.ac.be
- ----- Original Message -----
From: "Paula" <pauhar@chem.gla.ac.uk>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Thursday, November 14, 2002 10:06 AM
Subject: [WIEN]: hup: Command not found


> ====
> Paula <pauhar@chem.gla.ac.uk>
> submitted the following contribution:
> ====
>
> Dear Wien users,
>
> I am using wien2k on a dec compaq operating system. The c-shell command
> 'hup' is not recognised and l have copied the first part of the STDOUT
file
> below. The scf cycle continues, but when l try to run any tasks (elnes,
dos
> etc.) they crash. I would like to know if anyone else has found a similar
> error message and what l can do about it. Is it possible to write a script
> to replace this command? What does this command actually do?
> Thanks for your help,
>
> Paula
>
> STDOUT:
> hup: Command not found.
>   LAPW0 END
>   LAPW1 END
>   LAPW1 END
> LAPW2 - FERMI; weighs written
>   LAPW2 END
>   LAPW2 END
>   SUMPARA END
>   SUMPARA END
>   CORE  END
>   MIXER END
> in cycle 2    ETEST: 0   CTEST: 0
> hup: Command not found.
>   LAPW0 END
>   LAPW1 END
>   LAPW1 END
> LAPW2 - FERMI; weighs written
>   LAPW2 END
>   LAPW2 END
>   SUMPARA END
>   SUMPARA END
>   CORE  END
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

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------------------------------

Date: Thu, 14 Nov 2002 11:25:47 -0200 (BDB)
From: vivienne denise falcao <vdfalcao@dedalus.lcc.ufmg.br>
Subject: [WIEN]: Error in LAPW2

====
vivienne denise falcao <vdfalcao@dedalus.lcc.ufmg.br>
submitted the following contribution:
====

                               Dear All,

I changed the energy range in case.klist, ran lapw1 again and began a
calculate of X-Ray Spectra using Wien97 (an old version) but, when I run
lapw2 there is an error. The error message in lapw2.error file is as
follows:
'l2for' - QTL-B VALUE GT. 40.
What is happening? How can I correct this error?
What can I do to calculate the x-ray absorption and emission spectra with
the maximum energy range around 25 eV using Wien97 (an old version)?
Sorry, I`m a beginner and I don`t know a lot about Wien97 package.

Thankfull.

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Date: Thu, 14 Nov 2002 15:40:43 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: Error in LAPW2

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Hello Vivienne,

There's some information on this problem in the UG (usersguide - I don't
know if it was already included in the WIEN97-manual?) about ghostbands
(chapter 12.1, I believe) that you may want to read.  Also check out the
faq-pages on the wien2k-webpage about 'selecting muffin tin radius' and 'scf
cycle fails after some iterations'.

As you know, wien uses an LAPW-basis, which you can think of as a radial
basis function plus a linear correction inside the muffin-tin sphere, and
plane waves in the interstitial region between the spheres.  The QTL-B-value
measures the contribution of this linear correction (a sort of first order
term - the 'B' coefficients in the formula in the introduction of the UG)
basis function to the charge density.  If this contribution becomes large
(for a given atom,band,k-point ...) you may get linearisation errors.  In
WIEN97, the calculation therefore terminates and warns you that you may have
ghost bands.
[In Wien2k, things are more complicated since you also have lo's.  Therefore
the calculation will not stop because of a high QTL-B-value, but a warning
will be printed to case.scf(2) and case.output2.]

What you can try :
- -increase muffin tin size if you have core charge leakage (check in
case.outputst) and if possible
- -check the linearisation energies in case.in1(c) and change them if
necessary, or add LO's
- -restart your calculation with different mixing etc.

There's more info in the UG, on the faq-pages provided by P. Blaha, and in
the wien mail digest.  And you can always ask, of course.

Kevin.
kevin.jorissen@ua.ac.be
PS : If you're not really into WIEN97 yet, why not start straightaway with
WIEN2k?  It's newer, faster, has more options and applications, and it's
what most active users on this mailing list are using anyway.


- ----- Original Message -----
From: "vivienne denise falcao" <vdfalcao@dedalus.lcc.ufmg.br>
To: "Wien" <wien@zeus.theochem.tuwien.ac.at>
Sent: Thursday, November 14, 2002 2:25 PM
Subject: [WIEN]: Error in LAPW2


> ====
> vivienne denise falcao <vdfalcao@dedalus.lcc.ufmg.br>
> submitted the following contribution:
> ====
>
>                                Dear All,
>
> I changed the energy range in case.klist, ran lapw1 again and began a
> calculate of X-Ray Spectra using Wien97 (an old version) but, when I run
> lapw2 there is an error. The error message in lapw2.error file is as
> follows:
> 'l2for' - QTL-B VALUE GT. 40.
> What is happening? How can I correct this error?
> What can I do to calculate the x-ray absorption and emission spectra with
> the maximum energy range around 25 eV using Wien97 (an old version)?
> Sorry, I`m a beginner and I don`t know a lot about Wien97 package.
>
> Thankfull.
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

====
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------------------------------

Date: Fri, 15 Nov 2002 12:39:33 +0000
From: Paula <pauhar@chem.gla.ac.uk>
Subject: [WIEN]: Parallel Testerror

====
Paula <pauhar@chem.gla.ac.uk>
submitted the following contribution:
====

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- --=====================_4123937==.ALT
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Dear wien users,
I have updated to wien2k recently and am having a few problems. When l run 
the scf cycle for the perovskite system, SrTiO3, (which runs fine on 
wien97) i get the message:

hup: Command not found.
  LAPW0 END
  LAPW1 END
  LAPW1 END
LAPW2 - FERMI; weighs written
cp: .in.tmp: No such file or directory
rm: .in.tmp: No such file or directory
rm: .in.tmp1: No such file or directory

when i check error files all l am told is:

lapw2.error 0
**  testerror: Error in Parallel LAPW2

I have enclosed the .struct file and ran it with all the usual inputs 
suggested in the UG with 550 k-points. I have a duel processor machine and 
use the .machines file, also attached. I would appreciate any help that you 
could give.
Paula 
- --=====================_4123937==.ALT
Content-Type: text/html; charset="us-ascii"

<html>
<body>
Dear wien users,<br>
I have updated to wien2k recently and am having a few problems. When l
run the scf cycle for the perovskite system, SrTiO3, (which runs fine on
wien97) i get the message:<br><br>
<pre>hup: Command not found.
&nbsp;LAPW0 END
&nbsp;LAPW1 END
&nbsp;LAPW1 END
LAPW2 - FERMI; weighs written
cp: .in.tmp: No such file or directory
rm: .in.tmp: No such file or directory
rm: .in.tmp1: No such file or directory

when i check error files all l am told is:

</pre>lapw2.error 0<br>
**&nbsp; testerror: Error in Parallel LAPW2<br><br>
I have enclosed the .struct file and ran it with all the usual inputs
suggested in the UG with 550 k-points. I have a duel processor machine
and use the .machines file, also attached. I would appreciate any help
that you could give.<br>
Paula</body>
</html>

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Date: Fri, 15 Nov 2002 17:18:47 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: [WIEN]: min_lapw

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear all,

I am probably missing something with respect to min_lapw. After running 
a few cycles I realised that an atom that should have been fixed in 
position was being moved. I changed the corresponding line in case.inM 
to 0.0 in all four variables (I use NEWT), and to my surprise, min_lapw 
keeps changing the position of that atom several cycles later. I have 
checked several times that case.inM has 0.0 for all variables for that 
atom in case.struct. What do I have to do to make it stop doing that? 
Remove case.tmpM? The atoms that were fixed when I began min_lapw are 
kept fixed...

Best regards,
Torsten Andersen.

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics


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Date: Fri, 15 Nov 2002 17:31:55 +0100
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: Strange message in the output

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

I am running Wien2k on an AIX system and I wonder about some info I keep 
  getting in the output. Both when I run calculations in parallel and 
serial mode I get output like this:

STOP  LAPW0 END
STOP  LAPW1 END
cp: Nio.energyup_1: A file or directory in the path name does not exist.
cp: Nio.energyup_10: A file or directory in the path name does not exist.
cp: Nio.energyup_11: A file or directory in the path name does not exist.
cp: Nio.energyup_12: A file or directory in the path name does not exist.
cp: Nio.energyup_13: A file or directory in the path name does not exist.
cp: Nio.energyup_14: A file or directory in the path name does not exist.
cp: Nio.energyup_15: A file or directory in the path name does not exist.
cp: Nio.energyup_2: A file or directory in the path name does not exist.
STOP  LAPW2 END
STOP  CORE  END
STOP  CORE  END
STOP  MIXER END

Why is it complaining about these case.energyup_* files? Is it serious? 
Can/should I do anything about it?

Thanks for your replies! Any suggestions are welcome!

Best regards,
Thomas Claesson


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Date: Fri, 15 Nov 2002 13:06:50 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: problem with lstart

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

After running "lstart" during "init_lapw", I got the warning in the
case.outputst file as following:

WARNING !!!! For good atomic total energies you should probably change the
radial mesh (reduce NRAD or increase R0), or increase PARAMETERS NPT and
NPT00 1071  RADIAL MESH POINTS REACH UP TO 11.263190327106805  A.U.

I increased NPT and R0, but the warning still persisted. Can I ignore it?
if not, how to remedy it?

Any suggestion, comments and help is highly appreciated!

Best wishes!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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Date: Fri, 15 Nov 2002 20:42:49 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: problem with lstart

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> Bing Zhou <umbingz@cc.UManitoba.CA>
> submitted the following contribution:
> ====
> 
> After running "lstart" during "init_lapw", I got the warning in the
> case.outputst file as following:
> 
> WARNING !!!! For good atomic total energies you should probably change the
> radial mesh (reduce NRAD or increase R0), or increase PARAMETERS NPT and
> NPT00 1071  RADIAL MESH POINTS REACH UP TO 11.263190327106805  A.U.
> 
> I increased NPT and R0, but the warning still persisted. Can I ignore it?
> if not, how to remedy it?

You can ignore this, unless you are interested in properties of the free 
atoms that are calculated by lstart.

Stefaan
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Date: Fri, 15 Nov 2002 15:11:55 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: Re: [WIEN]: problem with lstart

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear Stefaan:

Thank you for your kind help again!

Have a nice weekend!


On Fri, 15 Nov 2002, Stefaan Cottenier wrote:

> ====
> Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
> submitted the following contribution:
> ====
>
> > ====
> > Bing Zhou <umbingz@cc.UManitoba.CA>
> > submitted the following contribution:
> > ====
> >
> > After running "lstart" during "init_lapw", I got the warning in the
> > case.outputst file as following:
> >
> > WARNING !!!! For good atomic total energies you should probably change the
> > radial mesh (reduce NRAD or increase R0), or increase PARAMETERS NPT and
> > NPT00 1071  RADIAL MESH POINTS REACH UP TO 11.263190327106805  A.U.
> >
> > I increased NPT and R0, but the warning still persisted. Can I ignore it?
> > if not, how to remedy it?
>
> You can ignore this, unless you are interested in properties of the free
> atoms that are calculated by lstart.
>
> Stefaan
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Sat, 16 Nov 2002 01:59:39 CST
From: Yongbin Lee <yblee@iastate.edu>
Subject: [WIEN]: ixcpot 4 : VBH

====
Yongbin Lee <yblee@iastate.edu>
submitted the following contribution:
====

Dear WIEN2k users

  I got a question about "ixcpot" option "4" in input *.in0.

       !     IXCPOT :  = 1 :  JMW SPIN-POLARIZED
       !               = 2 :  HL-NEW
       !               = 3 :  HL-OLD (FREEMAN)
       !               = 4 :  VBH

I think option "4" is for U.von.Barth and L.Hedin exchange-correlation and
it should work for spin polarized case.
But it seems not to work for spin polarized case. With this option, 
"*.vnsup" is exactly same with *.vnsdn" and 
"*.vspup also same with *.vspdn" .

I checked SRC_lapw0/xcpot.f, xcener.f.
These functions were written to use just "RHO", not "RHOUP","RHODN".

        RS=(0.75D0/PI/RHO)**(1.D0/3.D0)
        BETA=1.0d0
        RHOH=2.0d0*RHOSP
        IF(IEX.EQ.1) GOTO 100
- ---->   RHOH=RHO
        IF(IEX.EQ.2) THEN
        BETA=1.d0+0.0316D0*RS*LOG(1.D0+24.3D0/RS)
       .
       .
        ELSE IF(IEX.EQ.4) THEN
        BETA=1.d0+0.0545D0*RS*LOG(1.D0+11.4D0/RS)
        ELSE IF(IEX.EQ.5) THEN
        BETA=1.0d0
        RHOH=2.0d0*RHOSP
        END IF
- ---->   XCPOT=-BETA*2.D0*(3.D0/PI*RHOH)**(1.D0/3.D0)
        RETURN

 Here are my questions.
 Are these options(2,3,4) not completely implemented yet?
 Are these options(2,3,4) just for unpolarized case ?
 Can these options(2,3,4) work for polarized case after comment out
that line ?
 What do I need more for spin polarized calculation with option '4' ? 

   Thank you

    Yongbin

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------------------------------

Date: Mon, 18 Nov 2002 09:52:56 +0800 (CST)
From: yshzhang@theory.issp.ac.cn
Subject: [WIEN]: U+SO

====
yshzhang@theory.issp.ac.cn
submitted the following contribution:
====

Dear all

I met a question about caculating a system with U and SO.

After convege of 'runsp', I added U(create case.inorb and case.indm) and 
it converged also.
Then I wanted to add SO, after 'initso', it create a new structure.
And I only mv case.indm to case.indmc. So "runsp -orb -so ' begin to run.
but it gives these errors when 'x orb -du'.

PGFIO-F-217/list-directed read/unit=11/attempt to read past end of file.
 File name = v.dmatud    formatted, sequential access   record = 1
 In source file init.f, at line number 227
0.030u 0.010s 0:00.10 40.0%	0+0k 0+0io 187pf+0w

Another question: I found the struct file is changed after 'initso'. Some
equal V split to unequal V, so I add some corresponing lines in the 
case.indmc and case.inorb. There gives some errors when 'x orb -up',

PGFIO-F-217/list-directed read/unit=10/attempt to read past end of file.
 File name = v.dmatup    formatted, sequential access   record = 35
 In source file init.f, at line number 227

 Did I also change case.inst to adapt the new case.struct.
- -- 
Best Regards
YS Zhang

- ------------------------------------------------------------------------
 Address: Institute of Solid State Physics
          Chinese Academy of Sciences
          P.O.BOX 1129,230031 Hefei 
          P.R~China
 Tel:     086-551-5591464(Office)
          086-551-5592837(Home)
 Fax:     086-551-5591434
 WWW:     http://theory.issp.ac.cn/~yshzhang
- ------------------------------------------------------------------------


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------------------------------

Date: Thu, 14 Nov 2002 11:30:22 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: hup: Command not found

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Dear Paula,

the hup command is not important.  You can safely ignore this message.  If
it bothers you, remove the hup command from run_lapw-script.  Or just ignore
it.

kind regards,

Kevin.
kevin.jorissen@ua.ac.be
- ----- Original Message -----
From: "Paula" <pauhar@chem.gla.ac.uk>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Thursday, November 14, 2002 10:06 AM
Subject: [WIEN]: hup: Command not found


> ====
> Paula <pauhar@chem.gla.ac.uk>
> submitted the following contribution:
> ====
>
> Dear Wien users,
>
> I am using wien2k on a dec compaq operating system. The c-shell command
> 'hup' is not recognised and l have copied the first part of the STDOUT
file
> below. The scf cycle continues, but when l try to run any tasks (elnes,
dos
> etc.) they crash. I would like to know if anyone else has found a similar
> error message and what l can do about it. Is it possible to write a script
> to replace this command? What does this command actually do?
> Thanks for your help,
>
> Paula
>
> STDOUT:
> hup: Command not found.
>   LAPW0 END
>   LAPW1 END
>   LAPW1 END
> LAPW2 - FERMI; weighs written
>   LAPW2 END
>   LAPW2 END
>   SUMPARA END
>   SUMPARA END
>   CORE  END
>   MIXER END
> in cycle 2    ETEST: 0   CTEST: 0
> hup: Command not found.
>   LAPW0 END
>   LAPW1 END
>   LAPW1 END
> LAPW2 - FERMI; weighs written
>   LAPW2 END
>   LAPW2 END
>   SUMPARA END
>   SUMPARA END
>   CORE  END
>
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

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Date: Mon, 18 Nov 2002 16:08:40 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: space group F2/d

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

I have a crystal with monoclinic symmetry, but, the space group is F2/d,
which is not in the list of the 230 space groups!
The F2/d is related to C2/c by the following relationship:

	Af=2Ac+Cc
	Bf=Bc
	Cf=Cc

so can I use C2/c for F2/d? if not, how should I fiddle with the space
group F2/d?

Thank you in adavance!

Best wishes!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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Date: Tue, 19 Nov 2002 12:44:37 +0800 (CST)
From: yshzhang@theory.issp.ac.cn
Subject: [WIEN]: SO

====
yshzhang@theory.issp.ac.cn
submitted the following contribution:
====

Dear all

I have a trivial question about how to choose the direction of 
magnetization (h,k,l) in case.inso.

I am caculating a AFI V2O3. The spin moment of vanadium do not along the 
0 0 1. Must I change the (h,k,l) along the spin moment of vanadium?
If yes, how can use only one (h,k,l) because the spin moments of  two 
vanadium in the cell are antiparallel?

- -- 
Best Regards
YS Zhang

- ------------------------------------------------------------------------
 Address: Institute of Solid State Physics
          Chinese Academy of Sciences
          P.O.BOX 1129,230031 Hefei 
          P.R~China
 Tel:     086-551-5591464(Office)
          086-551-5592837(Home)
 Fax:     086-551-5591434
 WWW:     http://theory.issp.ac.cn/~yshzhang
- ------------------------------------------------------------------------


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Date: Tue, 19 Nov 2002 07:47:18 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: SO

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

yes, and the numbers are floating point, I think.

BR,
Torsten Andersen.

yshzhang@theory.issp.ac.cn wrote:

>====
>yshzhang@theory.issp.ac.cn
>submitted the following contribution:
>====
>
>Dear all
>
>I have a trivial question about how to choose the direction of 
>magnetization (h,k,l) in case.inso.
>
>I am caculating a AFI V2O3. The spin moment of vanadium do not along the 
>0 0 1. Must I change the (h,k,l) along the spin moment of vanadium?
>If yes, how can use only one (h,k,l) because the spin moments of  two 
>vanadium in the cell are antiparallel?
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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Date: Tue, 19 Nov 2002 07:56:41 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: SO

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

sorry, I didn't read the last line too well. I think there should be 
hints about that in the FAQ about doing antiferromagnetic calculations.

Best regards,
Torsten.

Torsten Andersen wrote:

> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
>
> yes, and the numbers are floating point, I think.
>
> BR,
> Torsten Andersen.
>
> yshzhang@theory.issp.ac.cn wrote:
>
>> ====
>> yshzhang@theory.issp.ac.cn
>> submitted the following contribution:
>> ====
>>
>> Dear all
>>
>> I have a trivial question about how to choose the direction of 
>> magnetization (h,k,l) in case.inso.
>>
>> I am caculating a AFI V2O3. The spin moment of vanadium do not along 
>> the 0 0 1. Must I change the (h,k,l) along the spin moment of vanadium?
>> If yes, how can use only one (h,k,l) because the spin moments of  two 
>> vanadium in the cell are antiparallel?
>>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Tue, 19 Nov 2002 15:49:38 +0800 (CST)
From: yshzhang@theory.issp.ac.cn
Subject: [WIEN]: AFI

====
yshzhang@theory.issp.ac.cn
submitted the following contribution:
====

Dear ALL

To AFI system, if I didn't use 'runafm_lapw' but 
'runsp_lapw' during converge.
Do I have to put the spin moment of nonmagnetic atoms to zero in 
case.inst? 

- -- 
Best Regards
YS Zhang

- ------------------------------------------------------------------------
 Address: Institute of Solid State Physics
          Chinese Academy of Sciences
          P.O.BOX 1129,230031 Hefei 
          P.R~China
 Tel:     086-551-5591464(Office)
          086-551-5592837(Home)
 Fax:     086-551-5591434
 WWW:     http://theory.issp.ac.cn/~yshzhang
- ------------------------------------------------------------------------


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Date: Tue, 19 Nov 2002 09:06:15 +0100
From: georg@chem.au.dk
Subject: Re: [WIEN]: space group F2/d

====
georg@chem.au.dk
submitted the following contribution:
====

There are no F centered monoclinic groups!
If you've made your cell by distorting some other F centered unit cell the
easiest thing is to generate all your atoms(make your cell primitive and type in
(or make a little program to do it for you) all the F atoms. Then use sgroup to
find your correct space group.
 Georg


Quoting Bing Zhou <umbingz@cc.UManitoba.CA>:

> ====
> Bing Zhou <umbingz@cc.UManitoba.CA>
> submitted the following contribution:
> ====
> 
> Dear All:
> 
> I have a crystal with monoclinic symmetry, but, the space group is F2/d,
> which is not in the list of the 230 space groups!
> The F2/d is related to C2/c by the following relationship:
> 
> 	Af=2Ac+Cc
> 	Bf=Bc
> 	Cf=Cc
> 
> so can I use C2/c for F2/d? if not, how should I fiddle with the space
> group F2/d?
> 
> Thank you in adavance!
> 
> Best wishes!
> 
> 
> 
> Bing Zhou
> Dept. of Geological Sc.
> The Univ. of Manitoba
> Canada R3T 2N2
> Tel: (204)474-8395
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 


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Date: Tue, 19 Nov 2002 09:07:37 +0100
From: georg@chem.au.dk
Subject: Re: [WIEN]: AFI

====
georg@chem.au.dk
submitted the following contribution:
====

> Do I have to put the spin moment of nonmagnetic atoms to zero in 
> case.inst? 
If you start from a non-magnetic solution you'll probably stay there. You should
start from the AFM solution you're looking for
> 
> -- 
> Best Regards
> YS Zhang
> 
> ------------------------------------------------------------------------
>  Address: Institute of Solid State Physics
>           Chinese Academy of Sciences
>           P.O.BOX 1129,230031 Hefei 
>           P.R~China
>  Tel:     086-551-5591464(Office)
>           086-551-5592837(Home)
>  Fax:     086-551-5591434
>  WWW:     http://theory.issp.ac.cn/~yshzhang
> ------------------------------------------------------------------------
> 
> 
> ====
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> To (un)subscribe send mail to
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> 


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------------------------------

Date: Tue, 19 Nov 2002 09:13:57 +0100
From: "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: SO

====
"Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> yshzhang@theory.issp.ac.cn
> submitted the following contribution:
> ====
>
> If yes, how can use only one (h,k,l) because the spin moments of  two
> vanadium in the cell are antiparallel?

In addition to Torsten : (h,k,l) indicates the direction only, without
indicating the sense. You must make you V-up and V-dn atoms inequivalent in
case.struct, and give them an antiparallel starting configuration in
case.inst (which you probably did already). This takes care of the
antiparallelism. Specifying one (h,k,l) in case.inso takes care of the
(common) direction of both moments.

This would not have been possible for non-collinear magnetism (if one V
would have its moment at 90 deg with the other, e.g.), which is a situation
that cannot be dealt with by wien2k (by the way, are there any plans to add
this feature at some time?)

Stefaan

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Date: Tue, 19 Nov 2002 09:19:35 +0100 (MET)
From: Pavel Novak <novakp@fzu.cz>
Subject: Re: [WIEN]: SO

====
Pavel Novak <novakp@fzu.cz>
submitted the following contribution:
====

In AF calculation spin on one atom is up, on other atom it is down. You
put magnetization along the spin up.

Regards
Pavel Novak

On Tue, 19 Nov 2002 yshzhang@theory.issp.ac.cn wrote:

> ====
> yshzhang@theory.issp.ac.cn
> submitted the following contribution:
> ====
>
> Dear all
>
> I have a trivial question about how to choose the direction of
> magnetization (h,k,l) in case.inso.
>
> I am caculating a AFI V2O3. The spin moment of vanadium do not along the
> 0 0 1. Must I change the (h,k,l) along the spin moment of vanadium?
> If yes, how can use only one (h,k,l) because the spin moments of  two
> vanadium in the cell are antiparallel?
>
> --
> Best Regards
> YS Zhang
>
> ------------------------------------------------------------------------
>  Address: Institute of Solid State Physics
>           Chinese Academy of Sciences
>           P.O.BOX 1129,230031 Hefei
>           P.R~China
>  Tel:     086-551-5591464(Office)
>           086-551-5592837(Home)
>  Fax:     086-551-5591434
>  WWW:     http://theory.issp.ac.cn/~yshzhang
> ------------------------------------------------------------------------
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>
>
>



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Date: Tue, 19 Nov 2002 16:32:36 +0800 (CST)
From: yshzhang@theory.issp.ac.cn
Subject: Re: [WIEN]: AFI

====
yshzhang@theory.issp.ac.cn
submitted the following contribution:
====

> If you start from a non-magnetic solution you'll probably stay there. You should
> start from the AFM solution you're looking for

I have been edited case.inst and fliped the spin of one of the AF atoms (
invert the spin up and dn occupation numbers).

But the userguide also said:
 In addition you must set a zero moment (identical spin up and dn 
 oc-cupations) for all  non-magnetic  atoms, otherwise AFMINPUT cannot 
 determine the proper input for CLMCOPY. 
I don't know these is special for the AFMINPUT.
If I don't use AFMINPUT. Should I also do these(set a zero moment 
for all  non-magnetic  atoms? And does it affect property very large?

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Date: Tue, 19 Nov 2002 10:47:17 +0100
From: georg@chem.au.dk
Subject: Re: [WIEN]: AFI

====
georg@chem.au.dk
submitted the following contribution:
====

> But the userguide also said:
>  In addition you must set a zero moment (identical spin up and dn 
>  oc-cupations) for all  non-magnetic  atoms, otherwise AFMINPUT cannot 
>  determine the proper input for CLMCOPY. 
> I don't know these is special for the AFMINPUT.
> If I don't use AFMINPUT. Should I also do these(set a zero moment 
> for all  non-magnetic  atoms? And does it affect property very large?
This isn't necesarry when you don't use AFMINPUT. However if your magnetism is
strongly localized on some atoms, while others only have very little
spin-density, sometimes you'll get a better convergence if you start with the
"non-magnetic" atoms as non-magnetic.

Whatever you do your starting density shouldn't affect your self consistent
density. Unless off-course, you start so far from the solution that you're
looking for that you never get the correct solution.

 Georg 


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Date: Tue, 19 Nov 2002 11:56:37 +0100
From: Doru-Cristian Torumba <Doru.Torumba@fys.kuleuven.ac.be>
Subject: [WIEN]: MD

====
Doru-Cristian Torumba <Doru.Torumba@fys.kuleuven.ac.be>
submitted the following contribution:
====

Dear Wien-users,  
  
I try to use the molecular dynamics option of wien2k (MOLD or NOSE in  
case.inM). I do not succeed to obtain output. My case is documented below.  
There is not much information in the usersguide about this option. Are there  
references available of work where the MOLD or NOSE have been used ?  
  
Thanks a lot,  
Doru Torumba  
University of Leuven  
  
 - - - -  
  
example case : nonmagnetic bcc Fe, both Fe in the conventional unit cell are  
made inequivalent, all symmetry is removed except for the identity  
(including all symmetry and/or using a B-lattice with 1 inequivalent Fe  
gives the same problems).  
  
 Fe  
 P                            2  
              RELA  
   5.416900  5.416900  5.416900 90.000000 90.000000 90.000000  
 ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000  
           MULT= 1          ISPLIT= 2  
 Fe               781     0.00001000         2.2000      26.0  
 LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000  
                      0.0000000 1.0000000 0.0000000  
                      0.0000000 0.0000000 1.0000000  
 ATOM=  1: X=0.50000000 Y=0.50000000 Z=0.50000000  
           MULT= 1          ISPLIT= 2  
 Fe               781     0.00001000         2.2000      26.0  
 LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000  
                      0.0000000 1.0000000 0.0000000  
                      0.0000000 0.0000000 1.0000000  
    1      NUMBER OF SYMMETRY OPERATIONS  
  1 0 0 0.0000000  
  0 1 0 0.0000000  
  0 0 1 0.0000000  
        1  
  
This is the case.inM (MOLD gives same problem):  
  
 NOSE               #(NOSE, NEWT, BFGS, MOLD, tolf (a4,f5.2))  
 55.845 400.0 300.0 1.0    # Atom1   (NOSE, MOLD:Masse, delta t, T,  
 nose-frequency)  
 55.845 400.0 300.0 1.0    # Atom1   (NOSE, MOLD:Masse, delta t, T,  
 nose-frequency)  
  
Here is the sequence of commands I used (from :log) :  
  
>   (min_lapw) options: -j runfile  
>   (min_lapw) recover inm-file & call job runfile  
>   (run_lapw) options: -i 80 -cc 0.000001  
Mon Nov 18 15:25:45 CET 2002> (x) lapw0 testfe2 lapw0  
Mon Nov 18 15:25:50 CET 2002> (x) lapw1 testfe2 lapw1  
Mon Nov 18 15:25:56 CET 2002> (x) lapw2 testfe2 lapw2  
Mon Nov 18 15:26:01 CET 2002> (x) lcore testfe2 lcore  
Mon Nov 18 15:26:02 CET 2002> (x) mixer testfe2 mixer  
(...)  
Mon Nov 18 15:26:02 CET 2002> (x) mini testfe2 mini  
   
This is the screen output :  
   
doru/testfe2> min_lapw -j runfile  
 runfile  
  LAPW0 END  
  LAPW1 END  
  LAPW2 END  
  CORE  END  
  MIXER END  
 ......  
 (-deleted-)  
 .....  
  LAPW0 END  
  LAPW1 END  
  LAPW2 END  
  CORE  END  
  MIXER END  
 PGFIO-F-217/list-directed read/unit=15/attempt to read past end of file.  
  File name = testfe2.finM    formatted, sequential access   record = 2  
  In source file haupt.f, at line number 224  
   
The case is well-converged, that's not the problem :  
   
:DIS  :  CHARGE DISTANCE       0.0000001  
   
It does not read case.finM correctly. This file contains only 1 line :  
   
  -5090.992118  
   
and this number seems to be the total energy of the last iteration :  
   
:ENE  : ********** TOTAL ENERGY IN Ry =        -5090.992118  
   
Output files related to mini are empty :  
   
- -rw-r--r--    1 doru     users           0 Nov 18 15:26 testfe2.outputM  
- -rw-r--r--    1 doru     users           0 Nov 18 15:24 testfe2.tmpM  
- -rw-r--r--    1 doru     users           0 Nov 18 15:24 testfe2.tmpM1  
   
  
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Date: Tue, 19 Nov 2002 13:08:22 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: SO

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> This would not have been possible for non-collinear magnetism (if one V
> would have its moment at 90 deg with the other, e.g.), which is a situation
> that cannot be dealt with by wien2k (by the way, are there any plans to add
> this feature at some time?)

Yes, there are. Actually, we have a first working version developed by
Robert Laskowsky in our group.

One word of warning: When I see the many problems for inexperienced users
arising from including SO coupling and/or LDA+U, the inclusion of non-collinear
magnetism requires even more knowledge by the user.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Tue, 19 Nov 2002 13:22:37 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: MD

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I try to use the molecular dynamics option of wien2k (MOLD or NOSE in
> case.inM). I do not succeed to obtain output. My case is documented below.
> There is not much information in the usersguide about this option. Are there
> references available of work where the MOLD or NOSE have been used ?


MD (MOLD) is nothing else than structural minimization (NEWT) without a
friction term. NOSE allows in additon to specify a "temperature", i.e. a mean
kinetic energy.

From the above you must have:

i) A setup which allows the atoms to move freely (i.e. usually you must start
with some arbitrarely distorted structure). This is more than just putting
only the identity symmetry operation into case.struct, but also all LM terms
in case.in2c must appear.

>  ATOM=  1: X=0.00000000 Y=0.00000000 Z=0.00000000
>  ATOM=  1: X=0.50000000 Y=0.50000000 Z=0.50000000

Distort the positions!

>  NOSE               #(NOSE, NEWT, BFGS, MOLD, tolf (a4,f5.2))
>  55.845 400.0 300.0 1.0    # Atom1   (NOSE, MOLD:Masse, delta t, T,
>  nose-frequency)
>  55.845 400.0 300.0 1.0    # Atom1   (NOSE, MOLD:Masse, delta t, T,
>  nose-frequency)

A temperature of 1 K will  move the atoms very slowly!

> >   (run_lapw) options: -i 80 -cc 0.000001

Of course for MD one needs the forces on the atoms (otherwise we don't know
where we should move the atoms!). Use    -fc 1.0  instead of -cc


>  PGFIO-F-217/list-directed read/unit=15/attempt to read past end of file.
>   File name = testfe2.finM    formatted, sequential access   record = 2
>   In source file haupt.f, at line number 224
>
> The case is well-converged, that's not the problem :
>
> :DIS  :  CHARGE DISTANCE       0.0000001
>
> It does not read case.finM correctly. This file contains only 1 line :
>
>   -5090.992118
>
> and this number seems to be the total energy of the last iteration :

Yes, and the forces are missing, because your setup is for a highly
symmetric configuration where "symmetry" found out that the atoms are at an
equillibrium position and thus no forces will appear.

Regards

PS: One must find a good example, where MD is usefull at all. Many processes
in solids require a much too long simulation time to learn anything from a
short simulation of a very small ensamble (supercell).
In most cases in literature MD is applied a) to molecules   b) used only
for structural relaxation (with some friction term and not free MD)
c) with some additional constraints


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 19 Nov 2002 13:32:29 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: min_lapw

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I am probably missing something with respect to min_lapw. After running
> a few cycles I realised that an atom that should have been fixed in
> position was being moved. I changed the corresponding line in case.inM
> to 0.0 in all four variables (I use NEWT), and to my surprise, min_lapw
> keeps changing the position of that atom several cycles later. I have
> checked several times that case.inM has 0.0 for all variables for that
> atom in case.struct. What do I have to do to make it stop doing that?
> Remove case.tmpM? The atoms that were fixed when I began min_lapw are
> kept fixed...

Fixing the positions using inM means that the forces on these atoms are
set to zero. However, since you started with some non-zero values, these
attoms aquiered some speed and they continue moving "with constant speed"
even when all forces are zero for this atom.
The speed is calculated using the "history"-file case.tmpM and thus it
is required that you remove this file whenever you make changes to
case.inM. (This is like the "broyden"-files in the scf cycle....)

PS: I know that minimization is unnecessary clumsy because one must always
remove case.tmpM when one changes case.inM.  mini could easily be improved,
but time is lacking so far.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 19 Nov 2002 17:28:11 +0100
From: KOITZSCH Christian <christian.koitzsch@unifr.ch>
Subject: [none]

====
KOITZSCH Christian <christian.koitzsch@unifr.ch>
submitted the following contribution:
====

 Hi Everybody,

I guess I am another of the unexperienced users, who tries to calculate
spin-orbit for a Ferromagnet, in my case Gd...

I used runsp_lapw and everything goes fine, I obtain results very similar to
D. Singh's paper, just that some bands are not split, because I omitted
spin-orbit interaction. Now if I want to include that, I save the
calculation and run initso_lapw. I get the following output:
******************************************************************
 initso_lapw
  Edit input file Gd.inso  
    select the direction of the moment ( h k l ) (For R-lattice in R
coordinates)
    select atoms for which a Relativistic-LO should be added (heavier
elements) 
    or SO should be switched off (light elements) 
edit: Command not found.
  Edit input file Gd.in1  
    select a larger emax value for the energy window in Gd.in1   
edit: Command not found.
The file Gd.in2c has been generated automatically

In spinpolarized case SO may reduce symmetry. 

The program symmetso dedects the proper symmetry and creates new struct and
input files. (Note, equivalent atoms could become inequivalent in some
cases). 

Do you have a spinpolarized case (and want to run symmetso) ? (y/N)y       
FORTRAN STOP
0.380u 0.020s 0:00.40 100.0%    0+0k 0+0io 204pf+0w
edit: Command not found.
 A new structure for SO calculations has been created (_so).
 If you commit it will create new  Gd.struct, in1(c), in2c, inc,
 clmsum/up/dn, vspup/dn and vnsup/dn files. (Please SAVE any previous
 calculations)
NOTE: Files for -orb (Gd.indm(c),inorb,dmatup/dn) must be adapted manually
Do you want to use the new structure for SO calculations ? (y/N)n

Spinorbit is now ready to run.

******************************************************************
I am worried that he does not find "edit", is there way to specify the
default editor?

And if I then try to run runsp_lapw -so I get the following output:

***************************************************************

 LAPW0 END
 LAPW1 END
 LAPW1 END
PGFIO-F-225/list-directed read/unit=5/lexical error-- unknown token type.
 File name = Gd.inso    formatted, sequential access   record = 5
 In source file init.f, at line number 74
PGFIO-F-217/formatted read/unit=30/attempt to read past end of file.
 File name = Gd.energysoup    formatted, sequential access   record = 1
 In source file fermi.f, at line number 41
*************************************************************

my initso looks like this:

*************************************************************
WFFIL
 4  1  0                      llmax,ipr,kpot 
 -10.0000   1.50000           emin,emax (output energy window)
   0.  0.  1.                 direction of magnetization (lattice vectors)
 NX                           number of atoms for which RLO is added
 NX1   -4.97      0.005       atom number,e-lo,de (case.in1), repeat NX
times
 0 0 0 0 0                    number of atoms for which SO is switch off;
atoms


Am I correct that my problem arises because I have to specify something for
NX? And what is this for hcp Gd?

Thanks a lot

Christian Koitzsch
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------------------------------

Date: Tue, 19 Nov 2002 17:46:40 +0100
From: "Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: [WIEN]: Re: 

====
"Stefaan Cottenier" <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> KOITZSCH Christian <christian.koitzsch@unifr.ch>
> submitted the following contribution:
> ====
>
> I am worried that he does not find "edit", is there way to specify the
> default editor?

Yes, the editor is specified in the section that wien2k has added to your
.cshrc (if you use csh, similar for other shells) :

setenv EDITOR "pico"

> *************************************************************
> WFFIL
>  4  1  0                      llmax,ipr,kpot
>  -10.0000   1.50000           emin,emax (output energy window)
>    0.  0.  1.                 direction of magnetization (lattice vectors)
>  NX                           number of atoms for which RLO is added
>  NX1   -4.97      0.005       atom number,e-lo,de (case.in1), repeat NX
> times
>  0 0 0 0 0                    number of atoms for which SO is switch off;
> atoms
>
>
> Am I correct that my problem arises because I have to specify something
for
> NX? And what is this for hcp Gd?

Right. NX should be a number, the number of atoms  for which you want to add
an RLO (Relativistic Local Orbital). See Kunes et al, PRB64-153102.

Stefaan

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------------------------------

Date: Wed, 20 Nov 2002 10:41:37 +0900
From: akai <akai@po.cc.yamaguchi-u.ac.jp>
Subject: [WIEN]: Deleted a part of a vector file in lapw1.

====
akai <akai@po.cc.yamaguchi-u.ac.jp>
submitted the following contribution:
====

Dear WIEN users,

I have a trouble about a vector file. I calculate the band structure 
of Ba8Ga16Ge30.
In the calculation a large vector file about 5GB or more  is, it 
seems,  made in a temporary
area. In running lapw1 the file size become more than 5GB, but when 
the law1 stoped
regularly the file size is only about 2GB. But I can not found any 
other error signals.
When I checked the vector file,the later part of it did not 
exist,i.e. data for last some
k-points are missing. But the output1 file shows that the calculation 
was carried out
until the final k-point. In the calculation I took 172 k-points in 
the irreducible
  wedge. When a k-sampling is 60, I have no trouble.

We use a Pentium 4 machine with 1GB RIMM, OS is Hed hat 7.2, the 
compiler is ifc and
icc with the intel MKL. MPI_CH is installed , but not used in the calculation.

##############
FC = ifc
MPF = f90
CC = icc
FOPT =  -O -FR -mp
FPOPT = -O
DParallel = '-DParallel'
FGEN = $(PARALLEL)
LDFLAGS = -L/opt/intel/mkl/lib/32 -Vaxlib
R_LIBS = -lmkl_p4 -lmkl_lapack -lpthread -lguide
##############


- -- 
##################################
         Akai Koji
         Media and Information Technology Center
         Yamaguchi University


         phone: +81 836 85 9900
         fax: +81 836 85 9901
         e-mail: akai@po.cc.yamaguchi-u.ac.jp
##################################
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------------------------------

Date: Wed, 20 Nov 2002 07:25:09 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Deleted a part of a vector file in lapw1.

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Mr. Akai.

If you at 60 k-points have 2GB, then 172 k-points will give you around 
5.8GB in the vector file. There is no surprise in that. It contains the 
expansion coefficients to the basis set and the eigenenergies, saved per 
k-point, so it should scale with the number of k-points. If some data is 
missing at the end of the vector file, I would worry about the integrity 
of the file system, or a full disk - alternatively that the core dumps 
and the program exits - is the error file empty?

Best regards,
Torsten Andersen.

akai wrote:

> ====
> akai <akai@po.cc.yamaguchi-u.ac.jp>
> submitted the following contribution:
> ====
>
> Dear WIEN users,
>
> I have a trouble about a vector file. I calculate the band structure 
> of Ba8Ga16Ge30.
> In the calculation a large vector file about 5GB or more  is, it 
> seems,  made in a temporary
> area. In running lapw1 the file size become more than 5GB, but when 
> the law1 stoped
> regularly the file size is only about 2GB. But I can not found any 
> other error signals.
> When I checked the vector file,the later part of it did not exist,i.e. 
> data for last some
> k-points are missing. But the output1 file shows that the calculation 
> was carried out
> until the final k-point. In the calculation I took 172 k-points in the 
> irreducible
>  wedge. When a k-sampling is 60, I have no trouble.
>
> We use a Pentium 4 machine with 1GB RIMM, OS is Hed hat 7.2, the 
> compiler is ifc and
> icc with the intel MKL. MPI_CH is installed , but not used in the 
> calculation.
>
> ##############
> FC = ifc
> MPF = f90
> CC = icc
> FOPT =  -O -FR -mp
> FPOPT = -O
> DParallel = '-DParallel'
> FGEN = $(PARALLEL)
> LDFLAGS = -L/opt/intel/mkl/lib/32 -Vaxlib
> R_LIBS = -lmkl_p4 -lmkl_lapack -lpthread -lguide
> ##############
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Wed, 20 Nov 2002 22:11:08 +0900
From: akai <akai@po.cc.yamaguchi-u.ac.jp>
Subject: Re: [WIEN]: Deleted a part of a vector file in lapw1.

====
akai <akai@po.cc.yamaguchi-u.ac.jp>
submitted the following contribution:
====

Dear Mr. Andersen

Thank you for your response.

The trouble does not due to the file system, because I can make a 
unformated output file larger than 6GB by executing  a simple fortran 
program. I could not find any error message: lapw1.error is empty, 
there are no I/O error messages and no core files. I have never seen 
like this trouble; when the lapw1 is running the vector file become 
5GB ormore, but at the time when it stops a part of file is deleted
and the size turns small( about 2GB). I can not guess the reason at all.

If someone know similar behaviors, would you like to let me known about that.

>====
>Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
>submitted the following contribution:
>====
>
>Dear Mr. Akai.
>
>If you at 60 k-points have 2GB, then 172 k-points will give you 
>around 5.8GB in the vector file. There is no surprise in that. It 
>contains the expansion coefficients to the basis set and the 
>eigenenergies, saved per k-point, so it should scale with the number 
>of k-points. If some data is missing at the end of the vector file, 
>I would worry about the integrity of the file system, or a full disk 
>- alternatively that the core dumps and the program exits - is the 
>error file empty?
>
>Best regards,
>Torsten Andersen.
>
>akai wrote:
>
>>====
>>akai <akai@po.cc.yamaguchi-u.ac.jp>
>>submitted the following contribution:
>>====
>>
>>Dear WIEN users,
>>
>>I have a trouble about a vector file. I calculate the band 
>>structure of Ba8Ga16Ge30.
>>In the calculation a large vector file about 5GB or more  is, it 
>>seems,  made in a temporary
>>area. In running lapw1 the file size become more than 5GB, but when 
>>the law1 stoped
>>regularly the file size is only about 2GB. But I can not found any 
>>other error signals.
>>When I checked the vector file,the later part of it did not 
>>exist,i.e. data for last some
>>k-points are missing. But the output1 file shows that the 
>>calculation was carried out
>>until the final k-point. In the calculation I took 172 k-points in 
>>the irreducible
>>  wedge. When a k-sampling is 60, I have no trouble.
>>
>>We use a Pentium 4 machine with 1GB RIMM, OS is Hed hat 7.2, the 
>>compiler is ifc and
>>icc with the intel MKL. MPI_CH is installed , but not used in the 
>>calculation.
>>
>>##############
>>FC = ifc
>>MPF = f90
>>CC = icc
>>FOPT =  -O -FR -mp
>>FPOPT = -O
>>DParallel = '-DParallel'
>>FGEN = $(PARALLEL)
>>LDFLAGS = -L/opt/intel/mkl/lib/32 -Vaxlib
>>R_LIBS = -lmkl_p4 -lmkl_lapack -lpthread -lguide
>>##############
>>
>
>

- -- 
##################################
         Akai Koji
         Media and Information Technology Center
         Yamaguchi University


         phone: +81 836 85 9900
         fax: +81 836 85 9901
         e-mail: akaikoji@po.cc.yamaguchi-u.ac.jp
##################################
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------------------------------

Date: Wed, 20 Nov 2002 14:27:04 +0100
From: georg@chem.au.dk
Subject: Re: [WIEN]: Deleted a part of a vector file in lapw1.

====
georg@chem.au.dk
submitted the following contribution:
====

I know that if you are using the PGI compiler you need to set a -Mlfs swithch to
support large files, but I don't know whether this is necesaary with ifc. The
man-pages might tell you something

 Georg

BTW. We are finishing a paper at the moment on  Ba8Ga16Ge30 (among other
clathrates).

Quoting akai <akai@po.cc.yamaguchi-u.ac.jp>:

> ====
> akai <akai@po.cc.yamaguchi-u.ac.jp>
> submitted the following contribution:
> ====
> 
> Dear Mr. Andersen
> 
> Thank you for your response.
> 
> The trouble does not due to the file system, because I can make a 
> unformated output file larger than 6GB by executing  a simple fortran 
> program. I could not find any error message: lapw1.error is empty, 
> there are no I/O error messages and no core files. I have never seen 
> like this trouble; when the lapw1 is running the vector file become 
> 5GB ormore, but at the time when it stops a part of file is deleted
> and the size turns small( about 2GB). I can not guess the reason at all.
> 
> If someone know similar behaviors, would you like to let me known about
> that.
> 
> >====
> >Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> >submitted the following contribution:
> >====
> >
> >Dear Mr. Akai.
> >
> >If you at 60 k-points have 2GB, then 172 k-points will give you 
> >around 5.8GB in the vector file. There is no surprise in that. It 
> >contains the expansion coefficients to the basis set and the 
> >eigenenergies, saved per k-point, so it should scale with the number 
> >of k-points. If some data is missing at the end of the vector file, 
> >I would worry about the integrity of the file system, or a full disk 
> >- alternatively that the core dumps and the program exits - is the 
> >error file empty?
> >
> >Best regards,
> >Torsten Andersen.
> >
> >akai wrote:
> >
> >>====
> >>akai <akai@po.cc.yamaguchi-u.ac.jp>
> >>submitted the following contribution:
> >>====
> >>
> >>Dear WIEN users,
> >>
> >>I have a trouble about a vector file. I calculate the band 
> >>structure of Ba8Ga16Ge30.
> >>In the calculation a large vector file about 5GB or more  is, it 
> >>seems,  made in a temporary
> >>area. In running lapw1 the file size become more than 5GB, but when 
> >>the law1 stoped
> >>regularly the file size is only about 2GB. But I can not found any 
> >>other error signals.
> >>When I checked the vector file,the later part of it did not 
> >>exist,i.e. data for last some
> >>k-points are missing. But the output1 file shows that the 
> >>calculation was carried out
> >>until the final k-point. In the calculation I took 172 k-points in 
> >>the irreducible
> >>  wedge. When a k-sampling is 60, I have no trouble.
> >>
> >>We use a Pentium 4 machine with 1GB RIMM, OS is Hed hat 7.2, the 
> >>compiler is ifc and
> >>icc with the intel MKL. MPI_CH is installed , but not used in the 
> >>calculation.
> >>
> >>##############
> >>FC = ifc
> >>MPF = f90
> >>CC = icc
> >>FOPT =  -O -FR -mp
> >>FPOPT = -O
> >>DParallel = '-DParallel'
> >>FGEN = $(PARALLEL)
> >>LDFLAGS = -L/opt/intel/mkl/lib/32 -Vaxlib
> >>R_LIBS = -lmkl_p4 -lmkl_lapack -lpthread -lguide
> >>##############
> >>
> >
> >
> 
> -- 
> ##################################
>          Akai Koji
>          Media and Information Technology Center
>          Yamaguchi University
> 
> 
>          phone: +81 836 85 9900
>          fax: +81 836 85 9901
>          e-mail: akaikoji@po.cc.yamaguchi-u.ac.jp
> ##################################
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 


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------------------------------

Date: Wed, 20 Nov 2002 14:31:55 +0100
From: georg@chem.au.dk
Subject: Re: [WIEN]: Deleted a part of a vector file in lapw1.

====
georg@chem.au.dk
submitted the following contribution:
====

Just thought of that you could also run a "parallel" job sequentially:
Make a machines file with f.ex. two entries.
Remove the rsh from the program calls in the parallel scripts
Remove the & after the program calls in the parallel script

Then your vector file will be split into two, but you'll still run sequentially

 Georg

Quoting akai <akai@po.cc.yamaguchi-u.ac.jp>:

> ====
> akai <akai@po.cc.yamaguchi-u.ac.jp>
> submitted the following contribution:
> ====
> 
> Dear Mr. Andersen
> 
> Thank you for your response.
> 
> The trouble does not due to the file system, because I can make a 
> unformated output file larger than 6GB by executing  a simple fortran 
> program. I could not find any error message: lapw1.error is empty, 
> there are no I/O error messages and no core files. I have never seen 
> like this trouble; when the lapw1 is running the vector file become 
> 5GB ormore, but at the time when it stops a part of file is deleted
> and the size turns small( about 2GB). I can not guess the reason at all.
> 
> If someone know similar behaviors, would you like to let me known about
> that.
> 
> >====
> >Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> >submitted the following contribution:
> >====
> >
> >Dear Mr. Akai.
> >
> >If you at 60 k-points have 2GB, then 172 k-points will give you 
> >around 5.8GB in the vector file. There is no surprise in that. It 
> >contains the expansion coefficients to the basis set and the 
> >eigenenergies, saved per k-point, so it should scale with the number 
> >of k-points. If some data is missing at the end of the vector file, 
> >I would worry about the integrity of the file system, or a full disk 
> >- alternatively that the core dumps and the program exits - is the 
> >error file empty?
> >
> >Best regards,
> >Torsten Andersen.
> >
> >akai wrote:
> >
> >>====
> >>akai <akai@po.cc.yamaguchi-u.ac.jp>
> >>submitted the following contribution:
> >>====
> >>
> >>Dear WIEN users,
> >>
> >>I have a trouble about a vector file. I calculate the band 
> >>structure of Ba8Ga16Ge30.
> >>In the calculation a large vector file about 5GB or more  is, it 
> >>seems,  made in a temporary
> >>area. In running lapw1 the file size become more than 5GB, but when 
> >>the law1 stoped
> >>regularly the file size is only about 2GB. But I can not found any 
> >>other error signals.
> >>When I checked the vector file,the later part of it did not 
> >>exist,i.e. data for last some
> >>k-points are missing. But the output1 file shows that the 
> >>calculation was carried out
> >>until the final k-point. In the calculation I took 172 k-points in 
> >>the irreducible
> >>  wedge. When a k-sampling is 60, I have no trouble.
> >>
> >>We use a Pentium 4 machine with 1GB RIMM, OS is Hed hat 7.2, the 
> >>compiler is ifc and
> >>icc with the intel MKL. MPI_CH is installed , but not used in the 
> >>calculation.
> >>
> >>##############
> >>FC = ifc
> >>MPF = f90
> >>CC = icc
> >>FOPT =  -O -FR -mp
> >>FPOPT = -O
> >>DParallel = '-DParallel'
> >>FGEN = $(PARALLEL)
> >>LDFLAGS = -L/opt/intel/mkl/lib/32 -Vaxlib
> >>R_LIBS = -lmkl_p4 -lmkl_lapack -lpthread -lguide
> >>##############
> >>
> >
> >
> 
> -- 
> ##################################
>          Akai Koji
>          Media and Information Technology Center
>          Yamaguchi University
> 
> 
>          phone: +81 836 85 9900
>          fax: +81 836 85 9901
>          e-mail: akaikoji@po.cc.yamaguchi-u.ac.jp
> ##################################
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 


====
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====

------------------------------

Date: Wed, 20 Nov 2002 19:24:41 +0100
From: Peer Kruse <kruse@lem.uni-karlsruhe.de>
Subject: Re: [WIEN]: Deleted a part of a vector file in lapw1.

====
Peer Kruse <kruse@lem.uni-karlsruhe.de>
submitted the following contribution:
====


- --------------010701080109070404040906
Content-Type: text/plain; charset=us-ascii; format=flowed
Content-Transfer-Encoding: 7bit

I have a similar problem but my vector file seems to be to big. I don't 
know how you checked your filesystem
it's at least not only a question of limits.
I did the following:

I created a file of a size half of my partition size  with
dd if=/dev/zero of= bigfile1 bs=131072 count=88888
That worked.  Even
cp bigfile1 bigfile2
works and there is no difference in them tested with
diff bigfile1 bigfile2
*But* deleting  bigfile1 and copying back doesn't work, so I can't check 
the diffs again.
Additionaly random numbers of /dev/random don't even create bigfile1.
This was an indication that it is a hard disc problem. I migrated my 
data to an other disk
an now it seems to run, at least the first cycle is through.

Best wishes

Peer

georg@chem.au.dk wrote:

>====
>georg@chem.au.dk
>submitted the following contribution:
>====
>
>Just thought of that you could also run a "parallel" job sequentially:
>Make a machines file with f.ex. two entries.
>Remove the rsh from the program calls in the parallel scripts
>Remove the & after the program calls in the parallel script
>
>Then your vector file will be split into two, but you'll still run sequentially
>
> Georg
>
>Quoting akai <akai@po.cc.yamaguchi-u.ac.jp>:
>
>  
>
>>====
>>akai <akai@po.cc.yamaguchi-u.ac.jp>
>>submitted the following contribution:
>>====
>>
>>Dear Mr. Andersen
>>
>>Thank you for your response.
>>
>>The trouble does not due to the file system, because I can make a 
>>unformated output file larger than 6GB by executing  a simple fortran 
>>program. I could not find any error message: lapw1.error is empty, 
>>there are no I/O error messages and no core files. I have never seen 
>>like this trouble; when the lapw1 is running the vector file become 
>>5GB ormore, but at the time when it stops a part of file is deleted
>>and the size turns small( about 2GB). I can not guess the reason at all.
>>
>>If someone know similar behaviors, would you like to let me known about
>>that.
>>
>>    
>>
>>>====
>>>Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
>>>submitted the following contribution:
>>>====
>>>
>>>Dear Mr. Akai.
>>>
>>>If you at 60 k-points have 2GB, then 172 k-points will give you 
>>>around 5.8GB in the vector file. There is no surprise in that. It 
>>>contains the expansion coefficients to the basis set and the 
>>>eigenenergies, saved per k-point, so it should scale with the number 
>>>of k-points. If some data is missing at the end of the vector file, 
>>>I would worry about the integrity of the file system, or a full disk 
>>>- alternatively that the core dumps and the program exits - is the 
>>>error file empty?
>>>
>>>Best regards,
>>>Torsten Andersen.
>>>
>>>akai wrote:
>>>
>>>      
>>>
>>>>====
>>>>akai <akai@po.cc.yamaguchi-u.ac.jp>
>>>>submitted the following contribution:
>>>>====
>>>>
>>>>Dear WIEN users,
>>>>
>>>>I have a trouble about a vector file. I calculate the band 
>>>>structure of Ba8Ga16Ge30.
>>>>In the calculation a large vector file about 5GB or more  is, it 
>>>>seems,  made in a temporary
>>>>area. In running lapw1 the file size become more than 5GB, but when 
>>>>the law1 stoped
>>>>regularly the file size is only about 2GB. But I can not found any 
>>>>other error signals.
>>>>When I checked the vector file,the later part of it did not 
>>>>exist,i.e. data for last some
>>>>k-points are missing. But the output1 file shows that the 
>>>>calculation was carried out
>>>>until the final k-point. In the calculation I took 172 k-points in 
>>>>the irreducible
>>>> wedge. When a k-sampling is 60, I have no trouble.
>>>>
>>>>We use a Pentium 4 machine with 1GB RIMM, OS is Hed hat 7.2, the 
>>>>compiler is ifc and
>>>>icc with the intel MKL. MPI_CH is installed , but not used in the 
>>>>calculation.
>>>>
>>>>##############
>>>>FC = ifc
>>>>MPF = f90
>>>>CC = icc
>>>>FOPT =  -O -FR -mp
>>>>FPOPT = -O
>>>>DParallel = '-DParallel'
>>>>FGEN = $(PARALLEL)
>>>>LDFLAGS = -L/opt/intel/mkl/lib/32 -Vaxlib
>>>>R_LIBS = -lmkl_p4 -lmkl_lapack -lpthread -lguide
>>>>##############
>>>>
>>>>        
>>>>
>>>      
>>>
>>-- 
>>##################################
>>         Akai Koji
>>         Media and Information Technology Center
>>         Yamaguchi University
>>
>>
>>         phone: +81 836 85 9900
>>         fax: +81 836 85 9901
>>         e-mail: akaikoji@po.cc.yamaguchi-u.ac.jp
>>##################################
>>====
>>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>>To (un)subscribe send mail to
>>majordomo@zeus.theochem.tuwien.ac.at
>>====
>>
>>    
>>
>
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>  
>



- --------------010701080109070404040906
Content-Type: text/html; charset=us-ascii
Content-Transfer-Encoding: 7bit

<!DOCTYPE html PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
  <title></title>
</head>
<body>
I have a similar problem but my vector file seems to be to big. I don't know
how you checked your filesystem<br>
it's at least not only a question of limits.<br>
I did the following:<br>
<br>
I created a file of a size half of my partition size&nbsp; with<br>
dd if=/dev/zero of= bigfile1 bs=131072 count=88888<br>
That worked. &nbsp;Even <br>
cp bigfile1 bigfile2<br>
works and there is no difference in them tested with <br>
diff bigfile1 bigfile2<br>
*But* deleting &nbsp;bigfile1 and copying back doesn't work, so I can't check
the diffs again.<br>
Additionaly random numbers of /dev/random don't even create bigfile1.<br>
This was an indication that it is a hard disc problem. I migrated my data
to an other disk<br>
an now it seems to run, at least the first cycle is through.<br>
<br>
Best wishes<br>
<br>
Peer<br>
<br>
<a class="moz-txt-link-abbreviated" href="mailto:georg@chem.au.dk">georg@chem.au.dk</a> wrote:<br>
<blockquote type="cite"
 cite="mid1037799115.3ddb8ecbda852@mail.chem.au.dk">
  <pre wrap="">====
<a class="moz-txt-link-abbreviated" href="mailto:georg@chem.au.dk">georg@chem.au.dk</a>
submitted the following contribution:
====

Just thought of that you could also run a "parallel" job sequentially:
Make a machines file with f.ex. two entries.
Remove the rsh from the program calls in the parallel scripts
Remove the &amp; after the program calls in the parallel script

Then your vector file will be split into two, but you'll still run sequentially

 Georg

Quoting akai <a class="moz-txt-link-rfc2396E" href="mailto:akai@po.cc.yamaguchi-u.ac.jp">&lt;akai@po.cc.yamaguchi-u.ac.jp&gt;</a>:

  </pre>
  <blockquote type="cite">
    <pre wrap="">====
akai <a class="moz-txt-link-rfc2396E" href="mailto:akai@po.cc.yamaguchi-u.ac.jp">&lt;akai@po.cc.yamaguchi-u.ac.jp&gt;</a>
submitted the following contribution:
====

Dear Mr. Andersen

Thank you for your response.

The trouble does not due to the file system, because I can make a 
unformated output file larger than 6GB by executing  a simple fortran 
program. I could not find any error message: lapw1.error is empty, 
there are no I/O error messages and no core files. I have never seen 
like this trouble; when the lapw1 is running the vector file become 
5GB ormore, but at the time when it stops a part of file is deleted
and the size turns small( about 2GB). I can not guess the reason at all.

If someone know similar behaviors, would you like to let me known about
that.

    </pre>
    <blockquote type="cite">
      <pre wrap="">====
Torsten Andersen <a class="moz-txt-link-rfc2396E" href="mailto:Torsten.Andersen@Fysik.UU.se">&lt;Torsten.Andersen@Fysik.UU.se&gt;</a>
submitted the following contribution:
====

Dear Mr. Akai.

If you at 60 k-points have 2GB, then 172 k-points will give you 
around 5.8GB in the vector file. There is no surprise in that. It 
contains the expansion coefficients to the basis set and the 
eigenenergies, saved per k-point, so it should scale with the number 
of k-points. If some data is missing at the end of the vector file, 
I would worry about the integrity of the file system, or a full disk 
- - alternatively that the core dumps and the program exits - is the 
error file empty?

Best regards,
Torsten Andersen.

akai wrote:

      </pre>
      <blockquote type="cite">
        <pre wrap="">====
akai <a class="moz-txt-link-rfc2396E" href="mailto:akai@po.cc.yamaguchi-u.ac.jp">&lt;akai@po.cc.yamaguchi-u.ac.jp&gt;</a>
submitted the following contribution:
====

Dear WIEN users,

I have a trouble about a vector file. I calculate the band 
structure of Ba8Ga16Ge30.
In the calculation a large vector file about 5GB or more  is, it 
seems,  made in a temporary
area. In running lapw1 the file size become more than 5GB, but when 
the law1 stoped
regularly the file size is only about 2GB. But I can not found any 
other error signals.
When I checked the vector file,the later part of it did not 
exist,i.e. data for last some
k-points are missing. But the output1 file shows that the 
calculation was carried out
until the final k-point. In the calculation I took 172 k-points in 
the irreducible
 wedge. When a k-sampling is 60, I have no trouble.

We use a Pentium 4 machine with 1GB RIMM, OS is Hed hat 7.2, the 
compiler is ifc and
icc with the intel MKL. MPI_CH is installed , but not used in the 
calculation.

##############
FC = ifc
MPF = f90
CC = icc
FOPT =  -O -FR -mp
FPOPT = -O
DParallel = '-DParallel'
FGEN = $(PARALLEL)
LDFLAGS = -L/opt/intel/mkl/lib/32 -Vaxlib
R_LIBS = -lmkl_p4 -lmkl_lapack -lpthread -lguide
##############

        </pre>
      </blockquote>
      <pre wrap="">
      </pre>
    </blockquote>
    <pre wrap="">-- 
##################################
         Akai Koji
         Media and Information Technology Center
         Yamaguchi University


         phone: +81 836 85 9900
         fax: +81 836 85 9901
         e-mail: <a class="moz-txt-link-abbreviated" href="mailto:akaikoji@po.cc.yamaguchi-u.ac.jp">akaikoji@po.cc.yamaguchi-u.ac.jp</a>
##################################
====
WIEN Mailing list: <a class="moz-txt-link-abbreviated" href="mailto:wien@zeus.theochem.tuwien.ac.at">wien@zeus.theochem.tuwien.ac.at</a>
To (un)subscribe send mail to
<a class="moz-txt-link-abbreviated" href="mailto:majordomo@zeus.theochem.tuwien.ac.at">majordomo@zeus.theochem.tuwien.ac.at</a>
====

    </pre>
  </blockquote>
  <pre wrap=""><!---->

====
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====
  </pre>
</blockquote>
<br>
<br>
</body>
</html>

- --------------010701080109070404040906--

====
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====

------------------------------

Date: Thu, 21 Nov 2002 10:59:06 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: ixcpot 4 : VBH

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>   I got a question about "ixcpot" option "4" in input *.in0.
>
>        !     IXCPOT :  = 1 :  JMW SPIN-POLARIZED
>        !               = 2 :  HL-NEW
>        !               = 3 :  HL-OLD (FREEMAN)
>        !               = 4 :  VBH
>
> I think option "4" is for U.von.Barth and L.Hedin exchange-correlation and
> it should work for spin polarized case.
> But it seems not to work for spin polarized case. With this option,
> "*.vnsup" is exactly same with *.vnsdn" and
> "*.vspup also same with *.vspdn" .
>  Here are my questions.
>  Are these options(2,3,4) not completely implemented yet?
>  Are these options(2,3,4) just for unpolarized case ?

Options 2,3,4 are for unpolarized case only!

>  Can these options(2,3,4) work for polarized case after comment out
> that line ?
>  What do I need more for spin polarized calculation with option '4' ?

I don't know ! From those old options only 1 is spinpolarized and if I
remember correctly, JMW reduces to VBH in unpolarized case (but this is
long time ago...)?

Why would you want to use old and obsolete LSDA Versions ?

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

End of wien-digest V2002 #44
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #45
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
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wien-digest       Thursday, November 28 2002       Volume 2002 : Number 045




----------------------------------------------------------------------

Date: Thu, 21 Nov 2002 11:09:03 +0100
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: Piping stdout to a file

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

I am running wien2k on an AIX multiprocessor system, where I submit my 
jobs to a queuing system. When the job is finished I get an email with 
everything wien2k has written to stdout during the run. I wonder if it 
is possible to pipe the output written by wien to a file that grows 
continuously during the run, so that I don't have to wait until the 
whole run is completed before I can read it?

I found this answer to a similar question in an old email from the list:

 >I can provide an answer if you are using the bash shell (typical for
 >linux).  To background a job, do:

 >  run_lapw options </dev/null &> run.output &

However, I am using the tcsh shell. What should I do to prevent the 
output to go to stdout and instead go to a file?

Thanks for your replies! Any suggestions are welcome!

Best regards,
Thomas Claesson


====
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====

------------------------------

Date: Thu, 21 Nov 2002 12:22:54 +0100 (MET)
From: buero@luitz.at
Subject: Re: [WIEN]: Piping stdout to a file

====
buero@luitz.at
submitted the following contribution:
====

On Thu, 21 Nov 2002, Thomas Claesson wrote:

>  >I can provide an answer if you are using the bash shell (typical for
>  >linux).  To background a job, do:
>
>  >  run_lapw options </dev/null &> run.output &
>
> However, I am using the tcsh shell. What should I do to prevent the
> output to go to stdout and instead go to a file?

This line to me looks like for tcsh for bash it should read however it
contains a severe typo: instead of "&>" it must read ">&"

">" redirects std.out and ">&" redirects std.out and std.err.

&> would try to send the first part of the line to the background and
gives an error because it tries to redirect the output of a null
command.

In bash the line should read

run_lapw -options </dev/null >run.output 2>&1 &

( 2>&1 means send stderr [channel 2] to the same file where stdout
[channel 1] goes)


regards
  joachim

 /---------------------------------------------------------\
(  luitz.at - Interfacing Art, Science and Technology       )
 )---------------------------------------------------------(
(  Büro für Informationstechnologie                         \
 ) und Technisches Büro für Technische Chemie                )
(  Dipl.-Ing. Joachim Luitz KEG         Tel: 022  31 61254  (
 ) Wohlmuthgasse 18                          0676 31 61254   )
(  A-3003 Gablitz                       Fax: 022  31 67443  (
 \ http://www.luitz.at                      buero@luitz.at   )
  \---------------------------------------------------------/


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------------------------------

Date: Thu, 21 Nov 2002 15:19:50 +0100
From: Thomas Claesson <tcl@kth.se>
Subject: Re: [WIEN]: Piping stdout to a file

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Thanks for your reply Joachim!

In principle it works, but the result is not what I want it to be. When 
I submit my job to the queuing system, like this:

 >> spsubmit [submit_options] runsp_lapw [run_options] [pipe_characters]

I get a short message back confirming that my job has been submitted to 
the que and that is all that gets printed in my run.output file. All the 
output produced by wien2k is still directed to stdout as usual. Can I 
modify the suggested pipe command in some way to get around this 
problem, or do I have to modify the wien shell scripts (run_lapw, 
runsp_lapw,...)?

Thanks for your replies!

Best reagrds,
Thomas Claesson

buero@luitz.at wrote:
> ====
> buero@luitz.at
> submitted the following contribution:
> ====
> 
> On Thu, 21 Nov 2002, Thomas Claesson wrote:
> 
> 
>> >I can provide an answer if you are using the bash shell (typical for
>> >linux).  To background a job, do:
>>
>> >  run_lapw options </dev/null &> run.output &
>>
>>However, I am using the tcsh shell. What should I do to prevent the
>>output to go to stdout and instead go to a file?
> 
> 
> This line to me looks like for tcsh for bash it should read however it
> contains a severe typo: instead of "&>" it must read ">&"
> 
> ">" redirects std.out and ">&" redirects std.out and std.err.
> 
> &> would try to send the first part of the line to the background and
> gives an error because it tries to redirect the output of a null
> command.
> 
> In bash the line should read
> 
> run_lapw -options </dev/null >run.output 2>&1 &
> 
> ( 2>&1 means send stderr [channel 2] to the same file where stdout
> [channel 1] goes)
> 
> 
> regards
>   joachim
> 
>  /---------------------------------------------------------\
> (  luitz.at - Interfacing Art, Science and Technology       )
>  )---------------------------------------------------------(
> (  Büro für Informationstechnologie                         \
>  ) und Technisches Büro für Technische Chemie                )
> (  Dipl.-Ing. Joachim Luitz KEG         Tel: 022  31 61254  (
>  ) Wohlmuthgasse 18                          0676 31 61254   )
> (  A-3003 Gablitz                       Fax: 022  31 67443  (
>  \ http://www.luitz.at                      buero@luitz.at   )
>   \---------------------------------------------------------/
> 
> 
> ====
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> To (un)subscribe send mail to
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Date: Thu, 21 Nov 2002 09:32:12 -0500
From: Jeff Spirko <spirko@lehigh.edu>
Subject: Re: [WIEN]: Piping stdout to a file

====
Jeff Spirko <spirko@lehigh.edu>
submitted the following contribution:
====

On Thu, Nov 21, 2002 at 12:22:54PM +0100, buero@luitz.at wrote:
> On Thu, 21 Nov 2002, Thomas Claesson wrote:
> >  >I can provide an answer if you are using the bash shell (typical for
> >  >linux).  To background a job, do:
> >  >  run_lapw options </dev/null &> run.output &

> > However, I am using the tcsh shell. What should I do to prevent the
> > output to go to stdout and instead go to a file?

> This line to me looks like for tcsh for bash it should read however it
> contains a severe typo: instead of "&>" it must read ">&"

> ">" redirects std.out and ">&" redirects std.out and std.err.

> &> would try to send the first part of the line to the background and
> gives an error because it tries to redirect the output of a null
> command.

With bash, both >& and &> are allowed, as well as using the 2>&1
(it must appear after the >run.output).  With tcsh, only >& works.

> In bash the line should read
> run_lapw -options </dev/null >run.output 2>&1 &

It is important to make sure your job doesn't get killed when you
log out or your connection dies.  (Bash protects from a logout, but
not a hangup.)  For that, use nohup.  It has the added benefit of
doing the output redirection for you (to nohup.out).  So my
preferred form of background running is now:

  nohup run_lapw -options </dev/null &

Then I can watch the output with tail -f nohup.out.

I just wish I could watch the case.output* files grow.  For some
reason, they're buffered instead of printing line-by-line.
I've even tried inserting call setlinebuf(6) in SRC_lapw1/inilpw.f,
and it still gets buffered.

- -- 
Jeff Spirko   spirko@lehigh.edu   spirko@yahoo.com   WD3V   |=>

The study of non-linear physics is like the study of non-elephant biology.

All theoretical chemistry is really physics;
and all theoretical chemists know it. -- Richard P. Feynman 
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Date: Thu, 21 Nov 2002 15:32:16 +0100 (MET)
From: buero@luitz.at
Subject: Re: [WIEN]: Piping stdout to a file

====
buero@luitz.at
submitted the following contribution:
====

On Thu, 21 Nov 2002, Thomas Claesson wrote:

> I submit my job to the queuing system, like this:
>
>  >> spsubmit [submit_options] runsp_lapw [run_options] [pipe_characters]


If you redirect this line, it is obvious that every redirection is applied
to the first command specified, and that is spsubmit !

Write your commandline in a small script file like

myscriptfile:
#!/bin/bash
run_lapw [options] [redirection]

and submit this to the queue

spsubmit myscriptfile

or try using w2web, this automatically creates a ".command" file, which is
submitted to the queue and the output redirected to a file called STDOUT

Regards
  Joachim

 /---------------------------------------------------------\
(  luitz.at - Interfacing Art, Science and Technology       )
 )---------------------------------------------------------(
(  Büro für Informationstechnologie                         \
 ) und Technisches Büro für Technische Chemie                )
(  Dipl.-Ing. Joachim Luitz KEG         Tel: 022  31 61254  (
 ) Wohlmuthgasse 18                          0676 31 61254   )
(  A-3003 Gablitz                       Fax: 022  31 67443  (
 \ http://www.luitz.at                      buero@luitz.at   )
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Date: Thu, 21 Nov 2002 15:35:22 +0100 (MET)
From: buero@luitz.at
Subject: Re: [WIEN]: Piping stdout to a file

====
buero@luitz.at
submitted the following contribution:
====

On Thu, 21 Nov 2002, Jeff Spirko wrote:

> I just wish I could watch the case.output* files grow.  For some
> reason, they're buffered instead of printing line-by-line.
> I've even tried inserting call setlinebuf(6) in SRC_lapw1/inilpw.f,
> and it still gets buffered.

That's FORTAN-magic ,-) Only standard output is unbuffered.

Big hello to Lehigh
  Joachim



 /---------------------------------------------------------\
(  luitz.at - Interfacing Art, Science and Technology       )
 )---------------------------------------------------------(
(  Büro für Informationstechnologie                         \
 ) und Technisches Büro für Technische Chemie                )
(  Dipl.-Ing. Joachim Luitz KEG         Tel: 022  31 61254  (
 ) Wohlmuthgasse 18                          0676 31 61254   )
(  A-3003 Gablitz                       Fax: 022  31 67443  (
 \ http://www.luitz.at                      buero@luitz.at   )
  \---------------------------------------------------------/



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Date: Thu, 21 Nov 2002 09:38:49 -0500
From: Jeff Spirko <spirko@lehigh.edu>
Subject: Re: [WIEN]: Piping stdout to a file

====
Jeff Spirko <spirko@lehigh.edu>
submitted the following contribution:
====

On Thu, Nov 21, 2002 at 03:19:50PM +0100, Thomas Claesson wrote:
> In principle it works, but the result is not what I want it to be. When 
> I submit my job to the queuing system, like this:
> 
> >> spsubmit [submit_options] runsp_lapw [run_options] [pipe_characters]
> 
> I get a short message back confirming that my job has been submitted to 
> the que and that is all that gets printed in my run.output file. 

Your current shell is grabbing your redirections instead of passing
them on to the queuing system.  You can try putting the redirection
symbols in quotation marks, or you may have to do something drastic
like:
  spsubmit bash -c "run_lapw ..."
with all of your redirects in the quotes.  Or you can put your
commands in a script file and submit that.

- -- 
Jeff Spirko   spirko@lehigh.edu   spirko@yahoo.com   WD3V   |=>

The study of non-linear physics is like the study of non-elephant biology.

All theoretical chemistry is really physics;
and all theoretical chemists know it. -- Richard P. Feynman 
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Date: Thu, 21 Nov 2002 16:07:37 +0000 (GMT)
From: David Pankhurst <david.pankhurst@materials.oxford.ac.uk>
Subject: Re: [WIEN]: Piping stdout to a file

====
David Pankhurst <david.pankhurst@materials.oxford.ac.uk>
submitted the following contribution:
====

Hi Thomas,

Queue submission commands generally have options to redirect standard
error (stderr) and standard output (stdout).  I've never used spsubmit but
having done a quick web search I think the following might give the
desired result:

spsubmit -Email no -stdout outfilename -stderr errfilename run_lapw

I guess you could also make errfilename and outfilename the same file if 
you want both output streams in one file.

best regards,

	Dave

On Thu, 21 Nov 2002, Thomas Claesson wrote:

> ====
> Thomas Claesson <tcl@kth.se>
> submitted the following contribution:
> ====
> 
> Thanks for your reply Joachim!
> 
> In principle it works, but the result is not what I want it to be. When 
> I submit my job to the queuing system, like this:
> 
>  >> spsubmit [submit_options] runsp_lapw [run_options] [pipe_characters]
> 
> I get a short message back confirming that my job has been submitted to 
> the que and that is all that gets printed in my run.output file. All the 
> output produced by wien2k is still directed to stdout as usual. Can I 
> modify the suggested pipe command in some way to get around this 
> problem, or do I have to modify the wien shell scripts (run_lapw, 
> runsp_lapw,...)?
> 
> Thanks for your replies!
> 
> Best reagrds,
> Thomas Claesson
> 
> buero@luitz.at wrote:
> > ====
> > buero@luitz.at
> > submitted the following contribution:
> > ====
> > 
> > On Thu, 21 Nov 2002, Thomas Claesson wrote:
> > 
> > 
> >> >I can provide an answer if you are using the bash shell (typical for
> >> >linux).  To background a job, do:
> >>
> >> >  run_lapw options </dev/null &> run.output &
> >>
> >>However, I am using the tcsh shell. What should I do to prevent the
> >>output to go to stdout and instead go to a file?
> > 
> > 
> > This line to me looks like for tcsh for bash it should read however it
> > contains a severe typo: instead of "&>" it must read ">&"
> > 
> > ">" redirects std.out and ">&" redirects std.out and std.err.
> > 
> > &> would try to send the first part of the line to the background and
> > gives an error because it tries to redirect the output of a null
> > command.
> > 
> > In bash the line should read
> > 
> > run_lapw -options </dev/null >run.output 2>&1 &
> > 
> > ( 2>&1 means send stderr [channel 2] to the same file where stdout
> > [channel 1] goes)
> > 
> > 
> > regards
> >   joachim
> > 
> >  /---------------------------------------------------------\
> > (  luitz.at - Interfacing Art, Science and Technology       )
> >  )---------------------------------------------------------(
> > (  Büro für Informationstechnologie                         \
> >  ) und Technisches Büro für Technische Chemie                )
> > (  Dipl.-Ing. Joachim Luitz KEG         Tel: 022  31 61254  (
> >  ) Wohlmuthgasse 18                          0676 31 61254   )
> > (  A-3003 Gablitz                       Fax: 022  31 67443  (
> >  \ http://www.luitz.at                      buero@luitz.at   )
> >   \---------------------------------------------------------/
> > 
> > 
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
> > majordomo@zeus.theochem.tuwien.ac.at
> > ====
> 
> 
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> 


+---------------------------------+------------------------------------+
| Dr David Pankhurst,             | Tel : +44 1865 283325/283326       |
| Department of Materials,        | Fax : +44 1865 273789              |    
| University of Oxford,           |                                    |
| Parks Road, Oxford OX1 3PH, UK  | david.pankhurst@materials.ox.ac.uk |
+---------------------------------+------------------------------------+


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------------------------------

Date: Thu, 21 Nov 2002 16:01:43 +0000
From: Paula <pauhar@chem.gla.ac.uk>
Subject: [WIEN]: 'SECLR4'

====
Paula <pauhar@chem.gla.ac.uk>
submitted the following contribution:
====

- --=====================_15541845==_
Content-Type: text/plain; charset="us-ascii"; format=flowed

Hello,

I have tried to run an scf cycle fo the perovskite systen PbTiO3. The 
calculation immediately crashes with the following error message. I have 
not seen this message before, any ideas? I have attached the .struct file 
and the .in1c file.

Thanks,
Paula


**  Error in Parallel LAPW1
**  LAPW1 STOPPED at Thu Nov 21 15:44:49 GMT 2002
**  check ERROR FILES!
  Cholesky INFO =         1147
  'SECLR4' - POTRF (Scalapack/LAPACK) failed.
  Cholesky INFO =         1149
  'SECLR4' - POTRF (Scalapack/LAPACK) failed.
- --=====================_15541845==_
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- --=====================_15541845==_--

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------------------------------

Date: Thu, 21 Nov 2002 18:19:41 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: 'SECLR4'

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Hi Paula,

lstart gives charge leakage of about 0.03 e when you select -6 Ry as
separation energy between core and valence region.  You have to include the
Pb 5p-states to remedy this.  You'll have to select Esep about -7.5 - -8
instead of -6.
Maybe this solves your problem already?

Kevin.
kevin.jorissen@ua.ac.be
- ----- Original Message -----
From: "Paula" <pauhar@chem.gla.ac.uk>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Thursday, November 21, 2002 5:01 PM
Subject: [WIEN]: 'SECLR4'


> Hello,
>
> I have tried to run an scf cycle fo the perovskite systen PbTiO3. The
> calculation immediately crashes with the following error message. I have
> not seen this message before, any ideas? I have attached the .struct file
> and the .in1c file.
>
> Thanks,
> Paula
>
>
> **  Error in Parallel LAPW1
> **  LAPW1 STOPPED at Thu Nov 21 15:44:49 GMT 2002
> **  check ERROR FILES!
>   Cholesky INFO =         1147
>   'SECLR4' - POTRF (Scalapack/LAPACK) failed.
>   Cholesky INFO =         1149
>   'SECLR4' - POTRF (Scalapack/LAPACK) failed.

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------------------------------

Date: Thu, 21 Nov 2002 18:22:31 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: 'SECLR4'

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

a quick test with lower rkmax finished an scf-cycle without any problem
let me know if you still have trouble

kevin.
- ----- Original Message -----
From: "Paula" <pauhar@chem.gla.ac.uk>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Thursday, November 21, 2002 5:01 PM
Subject: [WIEN]: 'SECLR4'


> Hello,
>
> I have tried to run an scf cycle fo the perovskite systen PbTiO3. The
> calculation immediately crashes with the following error message. I have
> not seen this message before, any ideas? I have attached the .struct file
> and the .in1c file.
>
> Thanks,
> Paula
>
>
> **  Error in Parallel LAPW1
> **  LAPW1 STOPPED at Thu Nov 21 15:44:49 GMT 2002
> **  check ERROR FILES!
>   Cholesky INFO =         1147
>   'SECLR4' - POTRF (Scalapack/LAPACK) failed.
>   Cholesky INFO =         1149
>   'SECLR4' - POTRF (Scalapack/LAPACK) failed.

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------------------------------

Date: Thu, 21 Nov 2002 19:14:05 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: 'SECLR4'

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I have tried to run an scf cycle fo the perovskite systen PbTiO3. The
> calculation immediately crashes with the following error message. I have
> not seen this message before, any ideas? I have attached the .struct file
> and the .in1c file.
>   Cholesky INFO =         1147
>   'SECLR4' - POTRF (Scalapack/LAPACK) failed.
>   Cholesky INFO =         1149
>   'SECLR4' - POTRF (Scalapack/LAPACK) failed.

Such messages mean either:

Your struct file is wrong (2 atoms at the same place,....) (Yours seems ok)

You have an numerically overcomplete basis leading to linear dependency:
You are using RKMAX=8, APW+lo method for ALL atoms   AND have quite
different RMT (1.5 for Oxygen and 2.15 for Pb).
This input gives an effective RKMAX=11.5 with APW+lo for Pb (which is a
"soft" element and converges pretty easy.)
I suggest either you reduce RKMAX back to 7 or 7.5, or you remove the
APW+lo basis for Pb.
WFFIL        (WFPRI, SUPWF)
  8.00       12    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  0.30    5  0 (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global APW/LAPW)
 2   -1.15      0.010 CONT 0
 2    0.30      0.000 CONT 0
 0    0.30      0.000 CONT 0
 1    0.30      0.000 CONT 0
 0   -7.30      0.000 CONT 0    <---put zeros here

Regards



                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 21 Nov 2002 22:08:11 -0600
From: "Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
Subject: RE: [WIEN]: Isomer shift

====
"Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
submitted the following contribution:
====


Dear Win2k users:

  I am trying to calculate the Isomer Shift(IS) of the Fe in MgNi3-xFexC compounds. I use the density of the charge at nucleus from *.scf file to calculate the IS. I found that IS is too small. I think that I should take the contact charge density at a certain radius. But I do not know the information about this charge density. Would you please give some suggestions? 

Could someone tell me whether the charge density at nucleus from *.scf can be used or not? What is the unit for this charge density? Is it in e/au^3? Do I need to use the charge density at a  certain radius?  

I calculated the bcc Fe, I got charge density at nucleus: total= 14889.794645. I read Dr. Blaha and Shwarz's paper( J. De Physique 1988, C8-101), and their result was total=15222.00.   

Thank you so much

best regard

Jinbo Yang
Materials Research Center
University Of Missouri-Rolla
Rolla, MO 65409
Phone:+01-573-341-6165
Fax:   573-341-2071
E-mail:jinbo@umr.edu



        
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------------------------------

Date: Fri, 22 Nov 2002 10:50:46 +0100
From: Vladimir Timochevski <Vladimir.Timochevski@dpm.univ-lyon1.fr>
Subject: Re: [WIEN]: Isomer shift

====
Vladimir Timochevski <Vladimir.Timochevski@dpm.univ-lyon1.fr>
submitted the following contribution:
====

"Yang, Jinbo (UMR-Student)" wrote:
> 
> ====
> "Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
> submitted the following contribution:
Dear Jinbo,

The "density at the nucleus", which you find in the *.scf
file is the density taken at the first point of the radial
mesh. Typically this value depends on Rmt, size of the basis
set (if you add LO for Fe3d or not), etc. 
So, to compare this value with somebody else you need to use
exactly the same parameters as they did.

Or, you can calculate your own "calibration constant" by
doing a number of calculations for iron compounds, but still
you need to take exactly the same parameters for Fe atom in
all compounds. After that you do calculation for your system
under study and determine theoretical value of the isomer
shift by using your own "calibration constant".

From my own experience, I obtained better results when I
took "density at the nucleus" not at the first point of the
mesh, but the average value in the sphere with the
approximate nuclear radius:
Rnuc=1.2*(A)^(1/3)*10^(-5) (Ang), where A-number of nucleons
in the nucleus.
The density you take from the file *.clmsum (only the
spherically symmetric Y00 part for Fe atom), but do not
forget that you have a log-scale.

Regards,
Vladimir.


> ====
> 
> Dear Win2k users:
> 
>   I am trying to calculate the Isomer Shift(IS) of the Fe in MgNi3-xFexC compounds. I use the density of the charge at nucleus from *.scf file to calculate the IS. I found that IS is too small. I think that I should take the contact charge density at a certain radius. But I do not know the information about this charge density. Would you please give some suggestions?
> 
> Could someone tell me whether the charge density at nucleus from *.scf can be used or not? What is the unit for this charge density? Is it in e/au^3? Do I need to use the charge density at a  certain radius?
> 
> I calculated the bcc Fe, I got charge density at nucleus: total= 14889.794645. I read Dr. Blaha and Shwarz's paper( J. De Physique 1988, C8-101), and their result was total=15222.00.
> 
> Thank you so much
> 
> best regard
> 
> Jinbo Yang
> Materials Research Center
> University Of Missouri-Rolla
> Rolla, MO 65409
> Phone:+01-573-341-6165
> Fax:   573-341-2071
> E-mail:jinbo@umr.edu
> 
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====

- -- 
- ---------------------------------------------
Vladimir Timoshevskii
Departement de Physique de Materiaux
Universite Claude Bernard - Lyon 1
Lyon, France
Tel.: +33 472 431564
Fax:  +33 472 432648
email: Vladimir.Timochevski@dpm.univ-lyon1.fr
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------------------------------

Date: Fri, 22 Nov 2002 10:59:55 +0000
From: Paula <pauhar@chem.gla.ac.uk>
Subject: Re: [WIEN]: 'SECLR4'

====
Paula <pauhar@chem.gla.ac.uk>
submitted the following contribution:
====

Many thanks to both Peter and Kevin for the advice. lapw1 now runs with no 
problems.

Paula

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Date: Fri, 22 Nov 2002 08:53:27 -0600
From: "Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
Subject: RE: [WIEN]: Isomer shift

====
"Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
submitted the following contribution:
====

Dear Dr. Vladimir


  Thank you so much.
Your advice is very helpful.
Could you tell me what is the unit of this charge density?

best regard


Jinbo Yang
Materials Research Center
University Of Missouri-Rolla
Rolla, MO 65409
Phone:+01-573-341-6165(O), 573-308-1062(H)
Fax:   573-341-2071
E-mail:jinbo@umr.edu




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------------------------------

Date: Fri, 22 Nov 2002 17:31:22 +0100
From: Vladimir Timochevski <Vladimir.Timochevski@dpm.univ-lyon1.fr>
Subject: Re: [WIEN]: Isomer shift

====
Vladimir Timochevski <Vladimir.Timochevski@dpm.univ-lyon1.fr>
submitted the following contribution:
====

Dear Jinbo,

The units of the density are e/bohr.
But the numbers in *.clmsum file are written as r^2*rho(r),
and the spherically symmetric Y00 part (which you are
interested in !!) is written as 4*pi*r^2*rho(r).

Good luck,
Vladimir.


"Yang, Jinbo (UMR-Student)" wrote:
> 
> ====
> "Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
> submitted the following contribution:
> ====
> 
> Dear Dr. Vladimir
> 
>   Thank you so much.
> Your advice is very helpful.
> Could you tell me what is the unit of this charge density?
> 
> best regard
> 
> Jinbo Yang
> Materials Research Center
> University Of Missouri-Rolla
> Rolla, MO 65409
> Phone:+01-573-341-6165(O), 573-308-1062(H)
> Fax:   573-341-2071
> E-mail:jinbo@umr.edu
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====

- ---------------------------------------------
Vladimir Timoshevskii
Departement de Physique de Materiaux
Universite Claude Bernard - Lyon 1
Lyon, France
Tel.: +33 472 431564
Fax:  +33 472 432648
email: Vladimir.Timochevski@dpm.univ-lyon1.fr
- ---------------------------------------------
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------------------------------

Date: Fri, 22 Nov 2002 17:34:09 +0100
From: Vladimir Timochevski <Vladimir.Timochevski@dpm.univ-lyon1.fr>
Subject: Re: [WIEN]: Isomer shift

====
Vladimir Timochevski <Vladimir.Timochevski@dpm.univ-lyon1.fr>
submitted the following contribution:
====

Small correction to my previous email:
the units are e/(borh)^3, of course.
Sorry for that.

Vladimir.


"Yang, Jinbo (UMR-Student)" wrote:
> 
> ====
> "Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
> submitted the following contribution:
> ====
> 
> Dear Dr. Vladimir
> 
>   Thank you so much.
> Your advice is very helpful.
> Could you tell me what is the unit of this charge density?
> 
> best regard
> 
> Jinbo Yang
> Materials Research Center
> University Of Missouri-Rolla
> Rolla, MO 65409
> Phone:+01-573-341-6165(O), 573-308-1062(H)
> Fax:   573-341-2071
> E-mail:jinbo@umr.edu
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====

- -- 
- ---------------------------------------------
Vladimir Timoshevskii
Departement de Physique de Materiaux
Universite Claude Bernard - Lyon 1
Lyon, France
Tel.: +33 472 431564
Fax:  +33 472 432648
email: Vladimir.Timochevski@dpm.univ-lyon1.fr
- ---------------------------------------------
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------------------------------

Date: Fri, 22 Nov 2002 10:26:31 -0700
From: gelfand <gelfand@lamar.colostate.edu>
Subject: [WIEN]: Peculiar error during lapw1 start-up

====
gelfand <gelfand@lamar.colostate.edu>
submitted the following contribution:
====

Recently it has become impossible for me to run lapw1c:
the following message goes to STDOUT and program terminates.

A(an) READ statement cannot be executed for a unit in which the value of the 
ACTION specifier of an OPEN statement is write (unit= 0).
 Error occurs at or near line 401 of inilpw_
 Called from or near line 39 of MAIN__
A(an) READ statement cannot be executed for a unit in which the value of the 
ACTION specifier of an OPEN statement is write (unit= 0).
 Error occurs at or near line 401 of inilpw_
 Called from or near line 39 of MAIN__

This is from lf95-compiled wien2k on x86/linux.
I'm trying to run spin-polarized, parallel calculations
(but I have run this before many times, without this error).  The section
of the code referenced involves reading in k-point information.
There's no unit 0 in the relevant .def file (uplapw1.def, right?).
Does anyone have any idea as to what might be going on?

Thanks,
Martin Gelfand
Department of Physics
Colorado State University

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------------------------------

Date: Fri, 22 Nov 2002 11:33:30 -0600
From: "Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
Subject: RE: [WIEN]: Isomer shift

====
"Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
submitted the following contribution:
====


Dear Dr. Blaha and Wien2k users:

  I am new user of Wien2k.
  I try to obtain the charge density p(r) of Fe atoms using "run program" Task" "Electron density plots". I want to plot total charge density p(r) of Fe, therefore I can use it to average the contact charge density of Fe at a certain radius. I relapce case.clmvalup with case.clmsum in the lapw5.def. I found the value of total charge density p(r=0) is in the order of 100, however, I see the value of charge density at nucleus in *.scf is in the order of 1000. I do not know if there is any differnce between the charge density from *.scf and "Electron density plots". Does anyboday know the difference and how to get the contact charge density p(r) from Wien2K.  

 
thank you so much

Jinbo Yang
Materials Research Center
University Of Missouri-Rolla
Rolla, MO 65409
Phone:+01-573-341-6165(O), 573-308-1062(H)
Fax:   573-341-2071
E-mail:jinbo@umr.edu





       
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------------------------------

Date: Fri, 22 Nov 2002 23:37:54 -0800 (PST)
From: mehrdad dadsetani <dadsetani_m@yahoo.com>
Subject: [WIEN]: optic properties of HgI2

====
mehrdad dadsetani <dadsetani_m@yahoo.com>
submitted the following contribution:
====

I am user wien97
i am study to optic properties of HgI2.i run optic
succecfuly and generate *.outmat and *.outputop.
but when i run joint, i have message that
"invalid integer:read unexpected character
apparent state: unit 5 named HgI2.injoint
last format: list io
lately reading sequential formatted external I0
Abort(core dumped)"
HgI2.inop and HgI2.injoint are

150  1        number of k-points, first k-point 
- -5.0 2.0      Emin, Emax for matrix elements
2             number of choices (columns in *outmat)
1             Re xx
3             Re zz
- ----------------------------------------------

    1    40                    : LOWER AND UPPER
BANDINDEX
  -5.0000    0.0100   2.0000 : EMIN DE EMAX FOR
ENERGYGRID IN ryd 
ryd                           : output units  eV / ryd
 / cm-1
     4                        : SWITCH  
     2                        : NUMBER OF COLUMNS
   0.1  0.1  0.3              : BROADENING (FOR DRUDE
MODEL - switch 6,7 - 
ONLY)
- ------------------------------------------------------
HgI2.outputjoint and HgI2 joint are empyty

Thanks,
Mehrdad dadsetani
Department of Physics
lorestan University

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------------------------------

Date: Sat, 23 Nov 2002 21:09:49 -0600
From: "Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
Subject: RE: [WIEN]: charge density 

====
"Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
submitted the following contribution:
====



Dear Win2k Users:

  I try to obtain the total charge density at different sites by running lapw5. However, no matter where I put my origin of the plot, I always get the same values in the case.rho. I already changed the case.clmval to case.clmsum in the lapw5.def and also change the origin of plot in case.in5. Does anyone has some experience or give some suggestion?

Thank you so much

best regard

Jinbo Yang
Materials Research Center
University Of Missouri-Rolla
Rolla, MO 65409
Phone:+01-573-341-6165(O), 573-308-1062(H)
Fax:   573-341-2071
E-mail:jinbo@umr.edu


    
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------------------------------

Date: Sun, 24 Nov 2002 02:40:50 -0800 (PST)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: SCF

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started SCf  and got this message( in Lapwo
,"SELECT ERROR"
"SELECT" -no energy limits found for l=2
"SELECT" -E-bottom -2.48500,E-top -200.00000). what
dose it mean?or What is its reason?
What should be done for eliminating it?
Thank you for the guide.
H-Salehi 
Dept of physics
Ferdowsi University
MASHHAD IRAN


=====
Hamdollah Salehi
Dept of Physics
Ferdowsi University
Mashhad IRAN
Post boxs 1436
Post code 91775
faxs

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------------------------------

Date: Mon, 25 Nov 2002 14:20:55 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: RE: [WIEN]: Isomer shift

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>   I try to obtain the charge density p(r) of Fe atoms using "run program" Task" "Electron density plots". I want to plot total charge density p(r) of Fe, therefore I can use it to average the contact charge density of Fe at a certain radius. I relapce case.clmvalup with case.clmsum in the lapw5.def. I found the value of total charge density p(r=0) is in the order of 100, however, I see the value of charge density at nucleus in *.scf is in the order of 1000. I do not know if there is any differnce between the charge density from *.scf and "Electron density plots". Does anyboday know the difference and how to get the contact charge density p(r) from Wien2K.

You cannot use lapw5 to calculate rho at the position of the nucleus!!

We use a radial mesh (r_i=R0*exp(dx*(i-1)) for the numerical values of the
density inside the sphere. The first mesh point is called R0 and something
like 0.0005 bohr (Z-dependend), thus when you want to get rho at r=0 you
must extrapolate (in a very clever way!).

Since this extrapolation might be hard to achieve, one usually takes the
density at the first radial mesh point as an approximation for r=0 and
this value is printed in the scf file (Maybe others have more experience
and take some average,... however, I as far as I understand this averaging is
justified only for HFF (where we do it anyway in mixer)).

If you don't want to use the value of the scf file, you must grab the density
directly from the clmsum file.

As was mentioned before, for IS you should make several calculations (at least
"source" and "absorber" with identical r0, RMT, RKMAX and GMAX.



                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 25 Nov 2002 09:31:41 -0600
From: "Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
Subject: RE: [WIEN]: Isomer shift

====
"Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
submitted the following contribution:
====

Dear Dr. Blaha and Wien2k Users:


  Thank you so much for your advice. 

However, I still do not understand why I got same output(case.rho)if I change the origin and end of the x y plot in the case.in5. I used case.clmsum to replace the case.clmval in lapw5.def. 
Did I make any mistake?  Please give me some suggestion.


Thank you again

Jinbo Yang
Materials Research Center
University of Missouri-Rolla
Rolla, MO 65409
Phone:+01-573-341-6165(O), 573-308-1062(H)
Fax:   573-341-2071
E-mail:jinbo@umr.edu


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------------------------------

Date: Mon, 25 Nov 2002 16:36:00 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: RE: [WIEN]: Isomer shift

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> However, I still do not understand why I got same output(case.rho)if I change the origin and end of the x y plot in the case.in5. I used case.clmsum to replace the case.clmval in lapw5.def.
> Did I make any mistake?  Please give me some suggestion.

Yes, you probably did.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 25 Nov 2002 14:49:08 -0800 (PST)
From: Michelle Johannes <johannes@maugre.ucdavis.edu>
Subject: [WIEN]: qtl-b questions

====
Michelle Johannes <johannes@maugre.ucdavis.edu>
submitted the following contribution:
====

Dear users,
	I have a question about the qtl-b values in some of my
calculations.  I noticed in checking through the *.scf* files that I had a
small (approx. 2.1) qtl-b value.  So I carefully checked to see where the
bands were, adjusted the linearization energies and obtained a nicely
converged calculation with no qtl-b value reported.  However, when I run
lapw2 -qtl -up/dn, they return - and much bigger (around 12.0).  Is this
something to worry about?  Are the orbitally resolved DOS values reliable
given this value?  And one more question if anyone yet has
patience:  At what qtl-b value should I begin to fiddle with my
linearization energies?  Can I ignore a small value (1.0 or so) since it
will obviously not cause ghostbands?
	I realize much has been written about qtl-b values in this user's
group as well as the manual and also in S. Cottenier's tutorial, so I
apologize if I have missed the answers.

	Thank you for your input,
			Michelle

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------------------------------

Date: Tue, 26 Nov 2002 10:12:43 +0900
From: "Ichiro Nagano" <nagano@atrc.mhi.co.jp>
Subject: [WIEN]: Large-scale DFT calculations?

====
"Ichiro Nagano" <nagano@atrc.mhi.co.jp>
submitted the following contribution:
====

Dear WIEN2k users,

I would like to try more large-scale crystals (100-300 atoms in a unit
cell).
If it is possible fast and cost effectively, could you give me an advice?

Alternatively, should I use order-N method?

Thanks for any help,

Ichiro Nagano

********************************************************************
Advanced Technology Research Center, Mitsubishi Heavy Industries, Ltd.
8-1, Sachiura, 1-Chome, Kanazawa-ku, Yokohama, 236-8515, Japan
Ichiro Nagano
E-mail: <nagano@atrc.mhi.co.jp>
TEL: + 81 (45) 771-1222
FAX: + 81 (45) 771-3879



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------------------------------

Date: Tue, 26 Nov 2002 12:40:48 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question about parallel calculation

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

I have finished a SCF parallel calculation. Then, I would like to analyse 
the optical properties. However, whenn I start calculate the  x lapw2 -c. 
Error message likes 

executing: x lapw2 -c
start: end of file
apparent state: unit 10 named /tmp/wien97_tmp/opticsp6412A.vector
last format: list io
lately reading sequential unformatted external IO
Abort (core dumped)
0.060u 0.110s 0:01.61 10.5%     0+0k 0+0io 161pf+0w
RETURN key to continue ...

What should I do then?

Thank you very much

Martin

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------------------------------

Date: Tue, 26 Nov 2002 12:30:49 +0800 (CST)
From: yshzhang@theory.issp.ac.cn
Subject: Re: [WIEN]: Question about parallel calculation

====
yshzhang@theory.issp.ac.cn
submitted the following contribution:
====


> I have finished a SCF parallel calculation. Then, I would like to analyse 
> the optical properties. However, whenn I start calculate the  x lapw2 -c. 
> Error message likes 

You'd better use 'x lapw2 -c -p' because of SCF with parallel caculation.
Please try it.

- -- 
Best Regards
YS Zhang

- ------------------------------------------------------------------------
 Address: Institute of Solid State Physics
          Chinese Academy of Sciences
          P.O.BOX 1129,230031 Hefei 
          P.R~China
 Tel:     086-551-5591464(Office)
          086-551-5592837(Home)
 Fax:     086-551-5591434
 WWW:     http://theory.issp.ac.cn/~yshzhang
- ------------------------------------------------------------------------


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------------------------------

Date: Tue, 26 Nov 2002 13:35:54 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: Re: [WIEN]: Question about parallel calculation

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear Prof. Zhang,

Thank you for your reply.

Actually, I have also tried "x lapw2 -c -p", too.

The error message likes:

executing: x lapw2 -c -p
running in single mode
start: end of file
apparent state: unit 10 named /tmp/wien97_tmp/opticsp6412A.vector
last format: list io
lately reading sequential unformatted external IO
Abort (core dumped)
0.050u 0.170s 0:01.71 12.8%     0+0k 0+0io 501pf+0w
RETURN key to continue ...

How could I fix the problem?

Thank you very much

Martin

On Tue, 26 Nov 2002 yshzhang@theory.issp.ac.cn wrote:

> ====
> yshzhang@theory.issp.ac.cn
> submitted the following contribution:
> ====
> 
> 
> > I have finished a SCF parallel calculation. Then, I would like to analyse 
> > the optical properties. However, whenn I start calculate the  x lapw2 -c. 
> > Error message likes 
> 
> You'd better use 'x lapw2 -c -p' because of SCF with parallel caculation.
> Please try it.
> 
> 

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------------------------------

Date: Tue, 26 Nov 2002 08:54:13 +0100
From: Georg Madsen <georg@chem.au.dk>
Subject: Re: [WIEN]: qtl-b questions

====
Georg Madsen <georg@chem.au.dk>
submitted the following contribution:
====

> 	I have a question about the qtl-b values in some of my
> calculations.  I noticed in checking through the *.scf* files that I had a
> small (approx. 2.1) qtl-b value.  So I carefully checked to see where the
> bands were, adjusted the linearization energies and obtained a nicely
> converged calculation with no qtl-b value reported.  However, when I run
> lapw2 -qtl -up/dn, they return - and much bigger (around 12.0).  Is this
> something to worry about?  Are the orbitally resolved DOS values reliable
> given this value?
doing qtl's lapw2 in effect sets the Fermi enrgy to infinite, this means that
the linearization might be strained for bands high above the Fermilevel. It
might mean that your states far above the Fermi level aren't optimal. But I
don't think 12 is a big problem. The problem could be solved by allowing several
LO's for the same l. Setting then far above Ef wouldn't affect the SCF cycle,
but might give better optics/non-occupied bands. This isn't implemented yet.

> And one more question if anyone yet has
> patience:  At what qtl-b value should I begin to fiddle with my
> linearization energies?  Can I ignore a small value (1.0 or so) since it
> will obviously not cause ghostbands?
I think WIEN97 only warned you for qtl-b's above 40. 

> 	I realize much has been written about qtl-b values in this user's
> group as well as the manual and also in S. Cottenier's tutorial, so I
> apologize if I have missed the answers.
> 
> 	Thank you for your input,
> 			Michelle
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 


- ----------------------------
Georg Madsen
Dept. of Inorganic Chemistry
University of Aarhus
DK-8000 Århus C
Denmark
- ----------------------------
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------------------------------

Date: Tue, 26 Nov 2002 09:02:22 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Large-scale DFT calculations?

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I would like to try more large-scale crystals (100-300 atoms in a unit
> cell).
> If it is possible fast and cost effectively, could you give me an advice?
>
> Alternatively, should I use order-N method?

Such decisions depend not only on the number of atoms, but their type and
what's the "goal" of the calculations.

300 atoms of Si or C-H-N-O-atoms or similar, high accuracy not needed:
    I would go for e.g. SIESTA  (order N-method). Be prepared that the actual
    calculations migth be very fast (maybe a factor of 100 ? compared to
    WIEN2k), but that you need long testing about the bet basis set, testing
    of the achievable reliability,... and that for some systems reasonable
    accuracy cannot be reached at all.

300 atoms including some transition metals or even rare earth or 5f atoms:
    Get yourself the biggest and fastest parallel computer available ......

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 26 Nov 2002 09:06:57 +0100
From: Georg Madsen <georg@chem.au.dk>
Subject: Re: [WIEN]: Large-scale DFT calculations?

====
Georg Madsen <georg@chem.au.dk>
submitted the following contribution:
====

depends on what is "cost effective"

We geometry optimized a system with 120 Ba and Ge atoms on a PC. This was very
fast because it was a favorable case of APWs (high symmetry/large spheres).

 I'm doing an organic molecule with a 128 atoms in the unit cell at the moment.
This has no symmetry and very small spheres and is thus a large calculation. But
as we are interested in properties near the core, where APW are very good, it's
worth it.

 It depends on the type of system and the properties you're interested in. If
you want to geometry optimize 300 atoms you can download several pseudo
potential codes for free.

 If you do more than 100 nonequivalent atoms you'll need to modify the code as
the struct file format only supports 99. This will be improved in a future version. 

 Georg

Quoting Ichiro Nagano <nagano@atrc.mhi.co.jp>:

> ====
> "Ichiro Nagano" <nagano@atrc.mhi.co.jp>
> submitted the following contribution:
> ====
> 
> Dear WIEN2k users,
> 
> I would like to try more large-scale crystals (100-300 atoms in a unit
> cell).
> If it is possible fast and cost effectively, could you give me an advice?
> 
> Alternatively, should I use order-N method?
> 
> Thanks for any help,
> 
> Ichiro Nagano
> 
> ********************************************************************
> Advanced Technology Research Center, Mitsubishi Heavy Industries, Ltd.
> 8-1, Sachiura, 1-Chome, Kanazawa-ku, Yokohama, 236-8515, Japan
> Ichiro Nagano
> E-mail: <nagano@atrc.mhi.co.jp>
> TEL: + 81 (45) 771-1222
> FAX: + 81 (45) 771-3879
> 
> 
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 


- ----------------------------
Georg Madsen
Dept. of Inorganic Chemistry
University of Aarhus
DK-8000 Århus C
Denmark
- ----------------------------
====
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------------------------------

Date: Tue, 26 Nov 2002 16:17:48 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]: Question about parallel calculation for optic

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

I have finished the SCF calculation with parallel mode. Then, I tried to 
calculate the Optic. Then, I run "x lapw2 -p" as "x lapw2 " will generate 
error as can't find .vector file. Then, I try to run "x optic" but it get 
error as can't find .vector again. How can I solve the problem? Is it 
possible to run optic in parallel mode (manual claims possible but I got 
"permission denied when I tried "x optic -r")?

Actually, I am using WIEN97 with graphic interface.

Thank you very much

Martin


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------------------------------

Date: Tue, 26 Nov 2002 11:10:59 -0300 (ARST)
From: Ruben Weht <ruweht@cnea.gov.ar>
Subject: [WIEN]: Problems with LDA+U+SO in Cerium systems.

====
Ruben Weht <ruweht@cnea.gov.ar>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- --1621662274-1305773784-1038319859=:2560
Content-Type: TEXT/PLAIN; charset=ISO-8859-1
Content-Transfer-Encoding: 8BIT

Dear Wien's users,

We have a project pointing to perform electronic structure calculations of
several Ce-systems.
As they need the application of both LDA+U formalism and SO coupling in
the last weeks we have tried to gain some experience doing quite simple
examples but have found really very puzzling results.

We will appreciate it a lot if someone in the group could help us.

As a first test we started with Ce-fcc, trying to reproduce a previous
calculation done by Alexander Shick, Warren Pickett and Sasha Lichtenstein
(condmat 0001255).
There they found several metastable states with different occupation
matrix (n_mm´) using another LAPW code. All of these states consist in one
4f electron located at about 2.5eV bellow the Fermi energy, as expected for
the Ce-fcc Gamma phase.
For the ground state the spin magnetic moment was 1.18 and the orbital
magnetic moment -1.87 (bohr magnetons), of course mainly of 4f character.

Our procedure to reproduce those findings was more or less the following
(always using the last version of Wien2k):

- - We first obtained the LDA self-consistent solution.
  Things went as usual giving a spin magnetic moment = 0.7

- - Then we lowered the symmetry to allow SO coupling
  (for this end we used INITSO but also checked by hand that the
   symmetries were OK)

Running LDA+U (SIC option) gives an almost correct result, with magnetic
moment of 1.17 and the f-peak located very near to the Shick´s result.

- - Then we turned on the SO coupling but surprisingly the magnetic moment
went down to almost zero after several iterations (it converges very slowly).
The 4f states split giving an equal occupation for spin up and down (but
always located at about 2eV bellow EF).

We think this is a non-physical result at all.

We have already tried to invert the sequence, applying first the SO
coupling and then LDA+U but the result was the same.

We have also tried other variants as putting the SO coupling along
different directions (changing the corresponding symmetries) or doing
different structures to see if the problem was related with the symmetry.
For instance, we have tried with a rhombohedral structure but again the
result was the same.

To see if our ignorance about SO and LDA+U was so big, we have proved with
Gd and things were fine in this case. Included, we have tried with Gd in a
fictitious FCC structure, similar to Ce-FCC, but as expected the result
was similar to the standard HCP case.

We don't know if we are doing some very stupid mistake and what kind of
error can produce this type of problems.

We have attached in a tarfile inputs we have used (struct, in1, in2c,
indmc, inorb and inso) in case someone wants to check them.

Really we will thank a lot any help the network could give us.

Our best regards,

		Veronica and Ruben


*====================================================================*
|  Ruben Weht                             |  ruweht@cnea.gov.ar      |
|  Departmento de Fisica - CNEA           |  Tel: (54-11) 6772-7104  |
|  Avda. General Paz y Constituyentes     |  Fax: (54-11) 6772-7121  |
|  1650 - San Martin - ARGENTINA          |                          |
*====================================================================*

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- --1621662274-1305773784-1038319859=:2560--
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------------------------------

Date: Tue, 26 Nov 2002 09:36:35 -0500
From: Xing Gao <xinggao@gh1.sims.nrc.ca>
Subject: [WIEN]: About LSTART

====
Xing Gao <xinggao@gh1.sims.nrc.ca>
submitted the following contribution:
====

Dear wien2k user,

When I run the lstart there is an error called:

"lib-4190 : UNRECOVERABLE library error

Encountered during a list-directed READ from unit 100
Fortran unit 100 is connected to a sequential formatted text file
  (standard input).
IOT Trap"

I don't know it is something wrong in the Library of our system, or the
definition of "unit 100" in the code is not suitable, or something
else. If you know please give me some suggestion. Thank you very much.

Xing 

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------------------------------

Date: Tue, 26 Nov 2002 16:34:18 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Problems with LDA+U+SO in Cerium systems.

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> We have a project pointing to perform electronic structure calculations of
> several Ce-systems.
> As they need the application of both LDA+U formalism and SO coupling in
> the last weeks we have tried to gain some experience doing quite simple
> examples but have found really very puzzling results.

Please make the following test:

Edit your runsp_lapw script:

....
lapw1:
...
#if ( "$so" == "-so" ) then
#  total_exec	lapw1 $it0 -up $para $nohns
#else
  total_exec	lapw1 $it0 -up $para $nohns $orb
#endif
...
#if ( "$so" == "-so" ) then
#  total_exec	lapw1 $it0 -dn $para $nohns
#else
  total_exec	lapw1 $it0 -dn $para $nohns $orb
#endif
...
lapwso:
if ( -e $file.scfso ) rm $file.scfso
if ( "$so" == "-so" ) then
   testinput	$file.inso error_input
#   total_exec lapwso -up $orb $para
   total_exec lapwso -up $para

Explanation: Recently WIEN2k was updated such that it adds LDA+U in lapw1
when SO is NOT included, but adds LDA+U in lapwso when SO is switched on.
This has the advantage of a) saving time  b) including crossterms between up/dn

By the above changes you go back to the "non-SO" scheme, i.e.
adding the LDA+U potential in lapw1 and SO in lapwso and I would like to
test this option. Normally, practically the same results should come out.
If not, then there must be a problem somewhere in the code.

Please let me know the results of your tests. If the problems persist, I'll
have a look on them.

Regards

>
> We will appreciate it a lot if someone in the group could help us.
>
> As a first test we started with Ce-fcc, trying to reproduce a previous
> calculation done by Alexander Shick, Warren Pickett and Sasha Lichtenstein
> (condmat 0001255).
> There they found several metastable states with different occupation
> matrix (n_mm´) using another LAPW code. All of these states consist in one
> 4f electron located at about 2.5eV bellow the Fermi energy, as expected for
> the Ce-fcc Gamma phase.
> For the ground state the spin magnetic moment was 1.18 and the orbital
> magnetic moment -1.87 (bohr magnetons), of course mainly of 4f character.
>
> Our procedure to reproduce those findings was more or less the following
> (always using the last version of Wien2k):
>
> - We first obtained the LDA self-consistent solution.
>   Things went as usual giving a spin magnetic moment = 0.7
>
> - Then we lowered the symmetry to allow SO coupling
>   (for this end we used INITSO but also checked by hand that the
>    symmetries were OK)
>
> Running LDA+U (SIC option) gives an almost correct result, with magnetic
> moment of 1.17 and the f-peak located very near to the Shick´s result.
>
> - Then we turned on the SO coupling but surprisingly the magnetic moment
> went down to almost zero after several iterations (it converges very slowly).
> The 4f states split giving an equal occupation for spin up and down (but
> always located at about 2eV bellow EF).
>
> We think this is a non-physical result at all.
>
> We have already tried to invert the sequence, applying first the SO
> coupling and then LDA+U but the result was the same.
>
> We have also tried other variants as putting the SO coupling along
> different directions (changing the corresponding symmetries) or doing
> different structures to see if the problem was related with the symmetry.
> For instance, we have tried with a rhombohedral structure but again the
> result was the same.
>
> To see if our ignorance about SO and LDA+U was so big, we have proved with
> Gd and things were fine in this case. Included, we have tried with Gd in a
> fictitious FCC structure, similar to Ce-FCC, but as expected the result
> was similar to the standard HCP case.
>
> We don't know if we are doing some very stupid mistake and what kind of
> error can produce this type of problems.
>
> We have attached in a tarfile inputs we have used (struct, in1, in2c,
> indmc, inorb and inso) in case someone wants to check them.
>
> Really we will thank a lot any help the network could give us.
>
> Our best regards,
>
> 		Veronica and Ruben
>
>
> *====================================================================*
> |  Ruben Weht                             |  ruweht@cnea.gov.ar      |
> |  Departmento de Fisica - CNEA           |  Tel: (54-11) 6772-7104  |
> |  Avda. General Paz y Constituyentes     |  Fax: (54-11) 6772-7121  |
> |  1650 - San Martin - ARGENTINA          |                          |
> *====================================================================*
>


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

====
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------------------------------

Date: Tue, 26 Nov 2002 08:43:11 -0800 (PST)
From: Claudio Lee <claudio_lee1@yahoo.com>
Subject: [WIEN]: runsp_c_lapw  and  runsp_lapw 

====
Claudio Lee <claudio_lee1@yahoo.com>
submitted the following contribution:
====

Dear all,
Is there anyone out there know the reason why I use
"runsp_c_lapw -so -orb  " to run  for my calculation
then it works, if however, with the same that
calculation, using "runsp_lapw -so -orb  " then it has
trouble after first iteration. For spin-polarized
calculation + SO + (LDA+U), using "runsp_lapw -so -orb
 "  I got the error file like this:
 ===
hup: Command not found.
STOP  LAPW0 END
STOP  LAPW1 END
STOP  LAPW1 END
STOP LAPWSO END
STOP  LAPW2 END
STOP  LAPW2 END
STOP  lapwdm END
STOP  CORE  END
STOP  CORE  END
STOP  MIXER END
hup: Command not found.
STOP  LAPW0 END
STOP  orbital potential calculation END
STOP  orbital potential calculation END
if: Badly formed number.     <=========== what is
this?
 ===
Since I want to obtain magnetic moment in my
calculation so I've got to choose  this "runsp_lapw
- -so -orb". So if you know the answer about this please
help me.
Sincerely,
Claudio



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------------------------------

Date: Tue, 26 Nov 2002 13:48:00 -0300 (ARST)
From: Ruben Weht <ruweht@cnea.gov.ar>
Subject: Re: [WIEN]: Problems with LDA+U+SO in Cerium systems.

====
Ruben Weht <ruweht@cnea.gov.ar>
submitted the following contribution:
====

Dear Peter,
Thanks a lot for your quick reply.

Things worked perfectly with the new script.
After our previous LDA+U calculations, as before, we added SO coupling but
now it converged in just five new iterations giving the correct result.

Do you think there is any problem with the code?

Well, thanks a lot again and with our best regards,

		Veronica and Ruben




On Tue, 26 Nov 2002, Peter Blaha wrote:

> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
>
> > We have a project pointing to perform electronic structure calculations of
> > several Ce-systems.
> > As they need the application of both LDA+U formalism and SO coupling in
> > the last weeks we have tried to gain some experience doing quite simple
> > examples but have found really very puzzling results.
>
> Please make the following test:
>
> Edit your runsp_lapw script:
>
> ....
> lapw1:
> ...
> #if ( "$so" == "-so" ) then
> #  total_exec	lapw1 $it0 -up $para $nohns
> #else
>   total_exec	lapw1 $it0 -up $para $nohns $orb
> #endif
> ...
> #if ( "$so" == "-so" ) then
> #  total_exec	lapw1 $it0 -dn $para $nohns
> #else
>   total_exec	lapw1 $it0 -dn $para $nohns $orb
> #endif
> ...
> lapwso:
> if ( -e $file.scfso ) rm $file.scfso
> if ( "$so" == "-so" ) then
>    testinput	$file.inso error_input
> #   total_exec lapwso -up $orb $para
>    total_exec lapwso -up $para
>
> Explanation: Recently WIEN2k was updated such that it adds LDA+U in lapw1
> when SO is NOT included, but adds LDA+U in lapwso when SO is switched on.
> This has the advantage of a) saving time  b) including crossterms between up/dn
>
> By the above changes you go back to the "non-SO" scheme, i.e.
> adding the LDA+U potential in lapw1 and SO in lapwso and I would like to
> test this option. Normally, practically the same results should come out.
> If not, then there must be a problem somewhere in the code.
>
> Please let me know the results of your tests. If the problems persist, I'll
> have a look on them.
>
> Regards
>
> >
> > We will appreciate it a lot if someone in the group could help us.
> >
> > As a first test we started with Ce-fcc, trying to reproduce a previous
> > calculation done by Alexander Shick, Warren Pickett and Sasha Lichtenstein
> > (condmat 0001255).
> > There they found several metastable states with different occupation
> > matrix (n_mm´) using another LAPW code. All of these states consist in one
> > 4f electron located at about 2.5eV bellow the Fermi energy, as expected for
> > the Ce-fcc Gamma phase.
> > For the ground state the spin magnetic moment was 1.18 and the orbital
> > magnetic moment -1.87 (bohr magnetons), of course mainly of 4f character.
> >
> > Our procedure to reproduce those findings was more or less the following
> > (always using the last version of Wien2k):
> >
> > - We first obtained the LDA self-consistent solution.
> >   Things went as usual giving a spin magnetic moment = 0.7
> >
> > - Then we lowered the symmetry to allow SO coupling
> >   (for this end we used INITSO but also checked by hand that the
> >    symmetries were OK)
> >
> > Running LDA+U (SIC option) gives an almost correct result, with magnetic
> > moment of 1.17 and the f-peak located very near to the Shick´s result.
> >
> > - Then we turned on the SO coupling but surprisingly the magnetic moment
> > went down to almost zero after several iterations (it converges very slowly).
> > The 4f states split giving an equal occupation for spin up and down (but
> > always located at about 2eV bellow EF).
> >
> > We think this is a non-physical result at all.
> >
> > We have already tried to invert the sequence, applying first the SO
> > coupling and then LDA+U but the result was the same.
> >
> > We have also tried other variants as putting the SO coupling along
> > different directions (changing the corresponding symmetries) or doing
> > different structures to see if the problem was related with the symmetry.
> > For instance, we have tried with a rhombohedral structure but again the
> > result was the same.
> >
> > To see if our ignorance about SO and LDA+U was so big, we have proved with
> > Gd and things were fine in this case. Included, we have tried with Gd in a
> > fictitious FCC structure, similar to Ce-FCC, but as expected the result
> > was similar to the standard HCP case.
> >
> > We don't know if we are doing some very stupid mistake and what kind of
> > error can produce this type of problems.
> >
> > We have attached in a tarfile inputs we have used (struct, in1, in2c,
> > indmc, inorb and inso) in case someone wants to check them.
> >
> > Really we will thank a lot any help the network could give us.
> >
> > Our best regards,
> >
> > 		Veronica and Ruben
> >
> >
> > *====================================================================*
> > |  Ruben Weht                             |  ruweht@cnea.gov.ar      |
> > |  Departmento de Fisica - CNEA           |  Tel: (54-11) 6772-7104  |
> > |  Avda. General Paz y Constituyentes     |  Fax: (54-11) 6772-7121  |
> > |  1650 - San Martin - ARGENTINA          |                          |
> > *====================================================================*
> >
>
>
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

- -- 
*====================================================================*
|  Ruben Weht                             |  ruweht@cnea.gov.ar      |
|  Departmento de Fisica - CNEA           |  Tel: (54-11) 6772-7104  |
|  Avda. General Paz y Constituyentes     |  Fax: (54-11) 6772-7121  |
|  1650 - San Martin - ARGENTINA          |                          |
*====================================================================*

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------------------------------

Date: Tue, 26 Nov 2002 09:30:18 -0800 (PST)
From: Michelle Johannes <johannes@maugre.ucdavis.edu>
Subject: Re: [WIEN]: qtl-b questions

====
Michelle Johannes <johannes@maugre.ucdavis.edu>
submitted the following contribution:
====

Thank you, Georg, your answer was very helpful.

	Michelle

On Tue, 26 Nov 2002, Georg Madsen wrote:

> ====
> Georg Madsen <georg@chem.au.dk>
> submitted the following contribution:
> ====
> 
> > 	I have a question about the qtl-b values in some of my
> > calculations.  I noticed in checking through the *.scf* files that I had a
> > small (approx. 2.1) qtl-b value.  So I carefully checked to see where the
> > bands were, adjusted the linearization energies and obtained a nicely
> > converged calculation with no qtl-b value reported.  However, when I run
> > lapw2 -qtl -up/dn, they return - and much bigger (around 12.0).  Is this
> > something to worry about?  Are the orbitally resolved DOS values reliable
> > given this value?
> doing qtl's lapw2 in effect sets the Fermi enrgy to infinite, this means that
> the linearization might be strained for bands high above the Fermilevel. It
> might mean that your states far above the Fermi level aren't optimal. But I
> don't think 12 is a big problem. The problem could be solved by allowing several
> LO's for the same l. Setting then far above Ef wouldn't affect the SCF cycle,
> but might give better optics/non-occupied bands. This isn't implemented yet.
> 
> > And one more question if anyone yet has
> > patience:  At what qtl-b value should I begin to fiddle with my
> > linearization energies?  Can I ignore a small value (1.0 or so) since it
> > will obviously not cause ghostbands?
> I think WIEN97 only warned you for qtl-b's above 40. 
> 
> > 	I realize much has been written about qtl-b values in this user's
> > group as well as the manual and also in S. Cottenier's tutorial, so I
> > apologize if I have missed the answers.
> > 
> > 	Thank you for your input,
> > 			Michelle
> > 
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
> > majordomo@zeus.theochem.tuwien.ac.at
> > ====
> > 
> 
> 
> ----------------------------
> Georg Madsen
> Dept. of Inorganic Chemistry
> University of Aarhus
> DK-8000 Århus C
> Denmark
> ----------------------------
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 

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------------------------------

Date: Wed, 27 Nov 2002 14:56:38 -0600
From: "Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
Subject: RE: [WIEN]: 

====
"Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
submitted the following contribution:
====

Dear Wien2k Users:

  I see there is an item "Nocubic" in the StructGen. Does it represent the symmetry of the atom at that position or something related to MT sphere? Should I neglect it or take a serious consideration about it? I found I got same result whether I select it or not.


Thank you so much

     
Jinbo Yang
Materials Research Center
University Of Missouri-Rolla
Rolla, MO 65409
Phone:+01-573-341-6165
Fax:   573-341-2071
E-mail:jinbo@umr.edu


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------------------------------

Date: Thu, 28 Nov 2002 00:34:40 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: problems with lapw1 and lapw2

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

I can run "x lapw0" and "x mixer" without problem, however, after I run
"x lapw1" or "x lapw2", I met the following problem:

	/home/wt/wien97/lapw1: Command not found
or 	/home/wt/wien97/lapw2: Command not found

What are the possible reasons for that?

Thanks!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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------------------------------

Date: Thu, 28 Nov 2002 08:35:39 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: [WIEN]: [Fwd: MKL 6.0 beta!] - BLAS, FFT, etc... from Intel for free

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear All,

I just thought you should know, too.

Best regards,
Torsten Andersen.

- -------- Original Message --------
Subject: MKL 6.0 beta!
Date: Tue, 26 Nov 2002 21:55:05 +0100
From: Mattias Klintenberg <mkklintenberg@lbl.gov>
Organization: LBNL
To: fysik4@fysik.uu.se



Greetings,

Intel is now offering their Math Kernel Library for free!!! This library 
is highly optimized
so now we will be able to use the true floating point power of PIII and 
PIV processors.

The library includes BLAS, LAPACK, DFT's , 2-D and 3-D FFT's,
VML, VSL, etc.

http://www.intel.com/software/products/perflib/
(see MKL 6.0 beta)

Regards,

/mattias





- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics


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------------------------------

Date: Thu, 28 Nov 2002 03:37:01 -0800 (PST)
From: mehrdad dadsetani <dadsetani_m@yahoo.com>
Subject: [WIEN]: Joint of HgI2

====
mehrdad dadsetani <dadsetani_m@yahoo.com>
submitted the following contribution:
====

I am user wien97
i am study to optic properties of HgI2.i run optic
succecfuly and generate *.outmat and *.outputop.
but when i run joint, i have message that
"invalid integer:read unexpected character
apparent state: unit 5 named HgI2.injoint
last format: list io
lately reading sequential formatted external I0
Abort(core dumped)"
HgI2.inop and HgI2.injoint are

150  1        number of k-points, first k-point 
- -5.0 2.0      Emin, Emax for matrix elements
2             number of choices (columns in *outmat)
1             Re xx
3             Re zz
- ----------------------------------------------

    1    40                    : LOWER AND UPPER
BANDINDEX
  -5.0000    0.0100   2.0000 : EMIN DE EMAX FOR
ENERGYGRID IN ryd 
ryd                           : output units  eV / ryd
 / cm-1
     4                        : SWITCH  
     2                        : NUMBER OF COLUMNS
   0.1  0.1  0.3              : BROADENING (FOR DRUDE
MODEL - switch 6,7 - 
ONLY)
- ------------------------------------------------------
HgI2.outputjoint and HgI2 joint are empyty

Thanks,
Mehrdad dadsetani
Department of Physics
lorestan University



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------------------------------

End of wien-digest V2002 #45
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #46
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
Errors-To: owner-wien-digest@theochem.tuwien.ac.at
Precedence: bulk


wien-digest        Thursday, December 5 2002        Volume 2002 : Number 046




----------------------------------------------------------------------

Date: Thu, 28 Nov 2002 14:33:49 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: 

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

WIEN sets this automatically.  However, if you start editing the struct-file
manually (eg to break symmetry), then you SHOULD also consider
cubic/noncubic case (change atom number to negative values).  If not, some
program (lapw0 or lapw2, I don't remember) fails.
Maybe it works the other way round (negative numbers though you have a cubic
system), but why would you want to do that?

kind regards,

Kevin Jorissen
kevin.jorissen@ua.ac.be

- ----- Original Message -----
From: "Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Wednesday, November 27, 2002 9:56 PM
Subject: RE: [WIEN]:


> ====
> "Yang, Jinbo (UMR-Student)" <jinbo@umr.edu>
> submitted the following contribution:
> ====
>
> Dear Wien2k Users:
>
>   I see there is an item "Nocubic" in the StructGen. Does it represent the
symmetry of the atom at that position or something related to MT sphere?
Should I neglect it or take a serious consideration about it? I found I got
same result whether I select it or not.
>
>
> Thank you so much
>
>
> Jinbo Yang
> Materials Research Center
> University Of Missouri-Rolla
> Rolla, MO 65409
> Phone:+01-573-341-6165
> Fax:   573-341-2071
> E-mail:jinbo@umr.edu
>
>
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
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------------------------------

Date: Thu, 28 Nov 2002 15:21:33 -0300 (ARST)
From: Ruben Weht <ruweht@cnea.gov.ar>
Subject: [WIEN]: Problems with LDA+U+SO in Cerium systems.

====
Ruben Weht <ruweht@cnea.gov.ar>
submitted the following contribution:
====

Dear Peter and members of the Wien club,

We think we were too optimistic in our last message regarding LDA+U+SO
calculations.

We did the changes you suggested and as we told you in our reply it seemed
to work properly: the spin magnetic moment had the correct value and the
density of states looked fine.

However, after a message by Michelle and other tests we did, we realized
that the solution was not completely correct: this time the orbital moment
had gone to zero.

After some thinking, we realized that with the changes you suggested we
should have run the complex version of lapw1 (because you are adding the
orbital potential directly to it).

After doing this new test and (with a quite painful convergence process)
we have obtained the same result than before: the spin magnetic moment
goes to zero again.

We suspect now than the original runsp_lapw is OK but there are some other
problem when both LDA+U and SO coupling are used together.

We really don't understand what kind of error it could be.

We apologize for the confusion we made.

Is there any member of the list who has succeeded in running LDA+U+SO for
other 4f systems? (we have already tried with Gd and it was fine, however,
this system is quite different from Ce because it has a half filled 4f
shell and in fact LDA itself gives a non so bad result).

Thanks a lot for any help,

		Veronica and Ruben

- -- 
*====================================================================*
|  Ruben Weht                             |  ruweht@cnea.gov.ar      |
|  Departmento de Fisica - CNEA           |  Tel: (54-11) 6772-7104  |
|  Avda. General Paz y Constituyentes     |  Fax: (54-11) 6772-7121  |
|  1650 - San Martin - ARGENTINA          |                          |
*====================================================================*

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------------------------------

Date: Thu, 28 Nov 2002 15:30:41 -0300 (ARST)
From: Ruben Weht <ruweht@cnea.gov.ar>
Subject: [WIEN]: Problems with LDA+U+SO in Cerium systems.

====
Ruben Weht <ruweht@cnea.gov.ar>
submitted the following contribution:
====

Peter,
Just in case it can help.
We have also run a fictitious Cerium with HCP structure.
We obtained a reasonable spin magnetic moment and density of states but
zero orbital moment.

Thanks again,

		Veronica and Ruben

- -- 
*====================================================================*
|  Ruben Weht                             |  ruweht@cnea.gov.ar      |
|  Departmento de Fisica - CNEA           |  Tel: (54-11) 6772-7104  |
|  Avda. General Paz y Constituyentes     |  Fax: (54-11) 6772-7121  |
|  1650 - San Martin - ARGENTINA          |                          |
*====================================================================*

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------------------------------

Date: Fri, 29 Nov 2002 08:54:16 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Problems with LDA+U+SO in Cerium systems.

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> We think we were too optimistic in our last message regarding LDA+U+SO
> calculations.
>
> We did the changes you suggested and as we told you in our reply it seemed
> to work properly: the spin magnetic moment had the correct value and the
> density of states looked fine.
>
> However, after a message by Michelle and other tests we did, we realized
> that the solution was not completely correct: this time the orbital moment
> had gone to zero.

I've also done some Ce calculations by now, but I cannot verify your last
message. However, I agree, the solution proposed in my last mail requires
lapw1c.

In my tests I have simply removed after orb:

rm $file.vorbdu

and than apply vorb in lapwso.

Please do not forget, that one can obtain many different LDA+U solutions
depending on the starting density (and density matrix).

When starting with a density from lda + SO and adding LDA+U I get

including cross terms: spin:  -0.26032   orb: -0.54422 (with very poor and
                       very slow convergence)
without crossterms (see above): spin: 1.16665  orb: -1.18953 (nice and quick)

As usual I can also obtain other solutions, starting with

SO + LDA+U (including crossterms): spin -1.18519    orb: 0.07087
  (since I started with a "negative" moment it remains negative)

a density matrix with large m=+3 occupation: -1.18891   2.87868

So you see all three solutions without cross term give a spin moment of 1.2,
while the orbital moment depends crucially on the starting dmat and was
0, 1 or 3 (and I'm sure I could also converge other orbital moments).

However, the solution with +1.2 has by far the lowest total energy of those
three tests and is thus the best solution (and is also the one which you
get from my recommended procedure:

runsp -so
x lapwdm -so -up
runsp -so -orb

I'll test this further and discuss it with others, but my impression is
that the cross-term in case.vorbdu is either not correct (or it's usage in
lapwso is not ok) and at the moment one should remove it. After that LDA+U
+SO gives expected results.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Fri, 29 Nov 2002 21:41:47 +0800
From: "whoming" <whoming@sohu.com>
Subject: [WIEN]: "Word too long" failure after lstart during init_lapw 

====
"whoming" <whoming@sohu.com>
submitted the following contribution:
====

Dear all,
         Today I have met a proble during init_lapw,
just after lstart, it looks like this:

>   lstart      (21:36:49)   SELECT XCPOT:
  recommended: 13: GGA (Perdew-Burke-Ernzerhof 96)
                5: LSDA
               14: GGA (Perdew-Wang 91)
5
  SELECT ENERGY to separate core and valence states:
  recommended: -6.0 Ry (check how much core charge leaks out of MT-sphere)
- -6.0
 STOP LSTART ENDS
 STOP
6.7u 0.0s 0:11 61% 0+0k 0+0io 0pf+0w
Word too long


What's the problem?Thank  you very much!
Yours,
whoming


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------------------------------

Date: Sun, 1 Dec 2002 11:45:16 +0800
From: "whoming" <whoming@sohu.com>
Subject: Re: [WIEN]: "Word too long" failure after lstart during init_lapw 

====
"whoming" <whoming@sohu.com>
submitted the following contribution:
====

Dear all,
         I have found the reason causing this problem.
Just do things following "grep WARNING $file.outputst"!
- ----- Original Message -----
From: "whoming" <whoming@sohu.com>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Friday, November 29, 2002 9:41 PM
Subject: [WIEN]: "Word too long" failure after lstart during init_lapw


> ====
> "whoming" <whoming@sohu.com>
> submitted the following contribution:
> ====
>
> Dear all,
>          Today I have met a proble during init_lapw,
> just after lstart, it looks like this:
>
> >   lstart      (21:36:49)   SELECT XCPOT:
>   recommended: 13: GGA (Perdew-Burke-Ernzerhof 96)
>                 5: LSDA
>                14: GGA (Perdew-Wang 91)
> 5
>   SELECT ENERGY to separate core and valence states:
>   recommended: -6.0 Ry (check how much core charge leaks out of MT-sphere)
> -6.0
>  STOP LSTART ENDS
>  STOP
> 6.7u 0.0s 0:11 61% 0+0k 0+0io 0pf+0w
> Word too long
>
>
> What's the problem?Thank  you very much!
> Yours,
> whoming
>
>
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
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>
>


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------------------------------

Date: Sun, 01 Dec 2002 12:57:51 +0000
From: "Yue Hai" <haiyuechina@hotmail.com>
Subject: Re: [WIEN]: Problems with LDA+U+SO in Cerium systems.

====
"Yue Hai" <haiyuechina@hotmail.com>
submitted the following contribution:
====

Dear Ruben:
   I have also calculate the system include Ce. I have change runsp_lapw 
likes this:

lapw1c:-------->not lapw1
...
#if ( "$so" == "-so" ) then
#  total_exec	lapw1 $it0 -up $para $nohns
#else
  total_exec	lapw1 $it0 -up -c $para $nohns $orb
#endif
...
#if ( "$so" == "-so" ) then
#  total_exec	lapw1 $it0 -dn $para $nohns
#else
  total_exec	lapw1 $it0 -dn -c $para $nohns $orb
#endif
...
lapwsoc:---------->not lapwso
if ( -e $file.scfso ) rm $file.scfso
if ( "$so" == "-so" ) then
   testinput	$file.inso error_input
#   total_exec lapwso -up $orb $para
   total_exec lapwso -up -c $para-------->include parameter "-c"
change in1 to inlc
runsp+so
runsp+so+U

  This means that you use complex version lapw1c, not lapw1.and orb is 
include in
lapw1c, not in lapwso, and the result is good, so you can try it.
The execute is:






>From: Ruben Weht <ruweht@cnea.gov.ar>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: WIEN <wien@zeus.theochem.tuwien.ac.at>
>Subject: [WIEN]: Problems with LDA+U+SO in Cerium systems.
>Date: Thu, 28 Nov 2002 15:21:33 -0300 (ARST)
>
>====
>Ruben Weht <ruweht@cnea.gov.ar>
>submitted the following contribution:
>====
>
>Dear Peter and members of the Wien club,
>
>We think we were too optimistic in our last message regarding LDA+U+SO
>calculations.
>
>We did the changes you suggested and as we told you in our reply it seemed
>to work properly: the spin magnetic moment had the correct value and the
>density of states looked fine.
>
>However, after a message by Michelle and other tests we did, we realized
>that the solution was not completely correct: this time the orbital moment
>had gone to zero.
>
>After some thinking, we realized that with the changes you suggested we
>should have run the complex version of lapw1 (because you are adding the
>orbital potential directly to it).
>
>After doing this new test and (with a quite painful convergence process)
>we have obtained the same result than before: the spin magnetic moment
>goes to zero again.
>
>We suspect now than the original runsp_lapw is OK but there are some other
>problem when both LDA+U and SO coupling are used together.
>
>We really don't understand what kind of error it could be.
>
>We apologize for the confusion we made.
>
>Is there any member of the list who has succeeded in running LDA+U+SO for
>other 4f systems? (we have already tried with Gd and it was fine, however,
>this system is quite different from Ce because it has a half filled 4f
>shell and in fact LDA itself gives a non so bad result).
>
>Thanks a lot for any help,
>
>		Veronica and Ruben
>
>--
>*====================================================================*
>|  Ruben Weht                             |  ruweht@cnea.gov.ar      |
>|  Departmento de Fisica - CNEA           |  Tel: (54-11) 6772-7104  |
>|  Avda. General Paz y Constituyentes     |  Fax: (54-11) 6772-7121  |
>|  1650 - San Martin - ARGENTINA          |                          |
>*====================================================================*
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====


_________________________________________________________________
Ãâ·ÑÏÂÔØ MSN Explorer:  http://explorer.msn.com/lccn/ 

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------------------------------

Date: Sun, 1 Dec 2002 05:13:04 -0800 (PST)
From: Hadi Arabi <arabi_h@yahoo.com>
Subject: [WIEN]: total core charge

====
Hadi Arabi <arabi_h@yahoo.com>
submitted the following contribution:
====

Dear wien user 
I work on Ice Cubic phase. I put Rmt=0.7 for H and
Rmt=1.4 for O. After initialise we found the following
data in case.outputst file for hydrogen.
The total core Charge and total core charge inside
sphere comes out zero. Does it makes sence? and what
is the reason for it?
 

                   H                                  
RHFS

         OCCUPANCY    ENERGY(RYD)         (R4)        
     (R2)              (R)               (R-1)        
    (R-3)

  1S      0.900    -5.5343653E-01     2.8859959E+01   
 3.2701173E+00     1.5496451E+00     9.8868262E-01
  1S      0.100    -2.9298928E-01     7.6763743E+01   
 5.1153976E+00     1.9089845E+00     8.3795725E-01

 TOTAL CHARGE FOR SPIN            1:                
0.9000000000000004
 TOTAL CHARGE FOR SPIN            1 INSIDE SPHERE:  
0.1484428774001257
 TOTAL CHARGE FOR SPIN            2:                
0.1000000000000000
 TOTAL CHARGE FOR SPIN            2 INSIDE SPHERE:  
1.2145117228393798E-002
 TOTAL CHARGE in sigma FOR SPIN            1:
   0.0000000000000000E+000
 TOTAL CHARGE in sigma FOR SPIN            1INSIDE
SPHERE:
   0.0000000000000000E+000
 TOTAL CHARGE in sigma FOR SPIN            2:
   0.0000000000000000E+000
 TOTAL CHARGE in sigma FOR SPIN            2INSIDE
SPHERE:
   0.0000000000000000E+000
 TOTAL CORE-CHARGE:                
0.0000000000000000E+000
 TOTAL CORE-CHARGE INSIDE SPHERE:  
0.0000000000000000E+000

 TOTAL ENERGY (RYD):               -0.966505
     SUM OF EI:-5.2739181E-01     NUC:-1.9472202E+00  
  COUL:-7.5003037E-01
     V-XC SPIN 1:-6.8721924E-01     E-XC SPIN
1:-5.4051577E-01
     V-XC SPIN 2:-4.1960721E-02     E-XC SPIN
2:-2.9182614E-02
  

__________________________________________________
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------------------------------

Date: Mon, 2 Dec 2002 09:08:25 +0800
From: "whoming" <whoming@sohu.com>
Subject: [WIEN]: What's the matter?

====
"whoming" <whoming@sohu.com>
submitted the following contribution:
====

Dear all,
         After 8 cycles, it show such error message:
in cycle 8    ETEST: .0018260000000000   CTEST: .0056579
hup - Command not found
 STOP  LAPW0 END
 STOP
 STOP  LAPW1 END
 STOP
 STOP  LAPW2 END
 STOP
 STOP  CORE  END
 STOP
 STOP  MIXER END
 STOP
tkerror failed to handle background error.
    Original error: can't read "s_lattice": no such variable
    Error in tkerror: can't invoke "after" command:  application has been
destoyed
         Any comments on this? Thank you very much!
yours,
       whoming
- ----- Original Message -----
From: "Peter Blaha" <pblaha@theochem.tuwien.ac.at>
To: "WIEN" <wien@zeus.theochem.tuwien.ac.at>
Sent: Friday, November 29, 2002 3:54 PM
Subject: Re: [WIEN]: Problems with LDA+U+SO in Cerium systems.


> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
>
> > We think we were too optimistic in our last message regarding LDA+U+SO
> > calculations.
> >
> > We did the changes you suggested and as we told you in our reply it
seemed
> > to work properly: the spin magnetic moment had the correct value and the
> > density of states looked fine.
> >
> > However, after a message by Michelle and other tests we did, we realized
> > that the solution was not completely correct: this time the orbital
moment
> > had gone to zero.
>
> I've also done some Ce calculations by now, but I cannot verify your last
> message. However, I agree, the solution proposed in my last mail requires
> lapw1c.
>
> In my tests I have simply removed after orb:
>
> rm $file.vorbdu
>
> and than apply vorb in lapwso.
>
> Please do not forget, that one can obtain many different LDA+U solutions
> depending on the starting density (and density matrix).
>
> When starting with a density from lda + SO and adding LDA+U I get
>
> including cross terms: spin:  -0.26032   orb: -0.54422 (with very poor and
>                        very slow convergence)
> without crossterms (see above): spin: 1.16665  orb: -1.18953 (nice and
quick)
>
> As usual I can also obtain other solutions, starting with
>
> SO + LDA+U (including crossterms): spin -1.18519    orb: 0.07087
>   (since I started with a "negative" moment it remains negative)
>
> a density matrix with large m=+3 occupation: -1.18891   2.87868
>
> So you see all three solutions without cross term give a spin moment of
1.2,
> while the orbital moment depends crucially on the starting dmat and was
> 0, 1 or 3 (and I'm sure I could also converge other orbital moments).
>
> However, the solution with +1.2 has by far the lowest total energy of
those
> three tests and is thus the best solution (and is also the one which you
> get from my recommended procedure:
>
> runsp -so
> x lapwdm -so -up
> runsp -so -orb
>
> I'll test this further and discuss it with others, but my impression is
> that the cross-term in case.vorbdu is either not correct (or it's usage in
> lapwso is not ok) and at the moment one should remove it. After that LDA+U
> +SO gives expected results.
>
> Regards
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
http://info.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>
>


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------------------------------

Date: Mon, 2 Dec 2002 09:52:53 +0800
From: "whoming" <whoming@sohu.com>
Subject: [WIEN]: A question

====
"whoming" <whoming@sohu.com>
submitted the following contribution:
====

Dear all,
         In one of my calculation,there is one WARNING message in case.scf
file:
:WARN :      WARNING: RKmax reduced due to NMATMAX
         How dose it influence the result? To avoid such, what should I do?
Thank you very much!
yours,
whoming
- ----- Original Message -----
From: "Peter Blaha" <pblaha@theochem.tuwien.ac.at>
To: "WIEN" <wien@zeus.theochem.tuwien.ac.at>
Sent: Friday, November 29, 2002 3:54 PM
Subject: Re: [WIEN]: Problems with LDA+U+SO in Cerium systems.


> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
>
> > We think we were too optimistic in our last message regarding LDA+U+SO
> > calculations.
> >
> > We did the changes you suggested and as we told you in our reply it
seemed
> > to work properly: the spin magnetic moment had the correct value and the
> > density of states looked fine.
> >
> > However, after a message by Michelle and other tests we did, we realized
> > that the solution was not completely correct: this time the orbital
moment
> > had gone to zero.
>
> I've also done some Ce calculations by now, but I cannot verify your last
> message. However, I agree, the solution proposed in my last mail requires
> lapw1c.
>
> In my tests I have simply removed after orb:
>
> rm $file.vorbdu
>
> and than apply vorb in lapwso.
>
> Please do not forget, that one can obtain many different LDA+U solutions
> depending on the starting density (and density matrix).
>
> When starting with a density from lda + SO and adding LDA+U I get
>
> including cross terms: spin:  -0.26032   orb: -0.54422 (with very poor and
>                        very slow convergence)
> without crossterms (see above): spin: 1.16665  orb: -1.18953 (nice and
quick)
>
> As usual I can also obtain other solutions, starting with
>
> SO + LDA+U (including crossterms): spin -1.18519    orb: 0.07087
>   (since I started with a "negative" moment it remains negative)
>
> a density matrix with large m=+3 occupation: -1.18891   2.87868
>
> So you see all three solutions without cross term give a spin moment of
1.2,
> while the orbital moment depends crucially on the starting dmat and was
> 0, 1 or 3 (and I'm sure I could also converge other orbital moments).
>
> However, the solution with +1.2 has by far the lowest total energy of
those
> three tests and is thus the best solution (and is also the one which you
> get from my recommended procedure:
>
> runsp -so
> x lapwdm -so -up
> runsp -so -orb
>
> I'll test this further and discuss it with others, but my impression is
> that the cross-term in case.vorbdu is either not correct (or it's usage in
> lapwso is not ok) and at the moment one should remove it. After that LDA+U
> +SO gives expected results.
>
> Regards
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW:
http://info.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>
>


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------------------------------

Date: Mon, 2 Dec 2002 11:43:19 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: [WIEN]:

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,
 
I have some questions about parallel calculation. The parallel calculation 
always dead with the error message in lapw1.error like:
**  Error in Parallel LAPW1
**  LAPW1 STOPPED at Sun Dec 1 22:15:17 HKT 2002
** check ERROR FILES!
Error in LAPW1
Error in LAPW1

Actually, the calculation has already finished 2 SCF cycyles. Then, why does 
the calculation stop not in the 1 cycle if I got some mistake in the 
parallelization? What should I do now?

Also, I got error in doing optic parallelization. The error is "OPTIC CRASHED!" Why?
Thank you 

Martin

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------------------------------

Date: Sun, 01 Dec 2002 10:31:24 +0100
From: Peer Kruse <kruse@lem.uni-karlsruhe.de>
Subject: Re: [WIEN]: A question

====
Peer Kruse <kruse@lem.uni-karlsruhe.de>
submitted the following contribution:
====

Deaer Whoming,
you have two possibilities, you can redeuce RKmax from the start and if 
this gives you not the desired
accuracy you can increase NMATMAX to cover it. But then you have to 
recompile the WIEN code.

yours

Peer

whoming wrote:

>====
>"whoming" <whoming@sohu.com>
>submitted the following contribution:
>====
>
>Dear all,
>         In one of my calculation,there is one WARNING message in case.scf
>file:
>:WARN :      WARNING: RKmax reduced due to NMATMAX
>         How dose it influence the result? To avoid such, what should I do?
>Thank you very much!
>yours,
>whoming
>----- Original Message -----
>From: "Peter Blaha" <pblaha@theochem.tuwien.ac.at>
>To: "WIEN" <wien@zeus.theochem.tuwien.ac.at>
>Sent: Friday, November 29, 2002 3:54 PM
>Subject: Re: [WIEN]: Problems with LDA+U+SO in Cerium systems.
>
>
>  
>
>>====
>>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>>submitted the following contribution:
>>====
>>
>>    
>>
>>>We think we were too optimistic in our last message regarding LDA+U+SO
>>>calculations.
>>>
>>>We did the changes you suggested and as we told you in our reply it
>>>      
>>>
>seemed
>  
>
>>>to work properly: the spin magnetic moment had the correct value and the
>>>density of states looked fine.
>>>
>>>However, after a message by Michelle and other tests we did, we realized
>>>that the solution was not completely correct: this time the orbital
>>>      
>>>
>moment
>  
>
>>>had gone to zero.
>>>      
>>>
>>I've also done some Ce calculations by now, but I cannot verify your last
>>message. However, I agree, the solution proposed in my last mail requires
>>lapw1c.
>>
>>In my tests I have simply removed after orb:
>>
>>rm $file.vorbdu
>>
>>and than apply vorb in lapwso.
>>
>>Please do not forget, that one can obtain many different LDA+U solutions
>>depending on the starting density (and density matrix).
>>
>>When starting with a density from lda + SO and adding LDA+U I get
>>
>>including cross terms: spin:  -0.26032   orb: -0.54422 (with very poor and
>>                       very slow convergence)
>>without crossterms (see above): spin: 1.16665  orb: -1.18953 (nice and
>>    
>>
>quick)
>  
>
>>As usual I can also obtain other solutions, starting with
>>
>>SO + LDA+U (including crossterms): spin -1.18519    orb: 0.07087
>>  (since I started with a "negative" moment it remains negative)
>>
>>a density matrix with large m=+3 occupation: -1.18891   2.87868
>>
>>So you see all three solutions without cross term give a spin moment of
>>    
>>
>1.2,
>  
>
>>while the orbital moment depends crucially on the starting dmat and was
>>0, 1 or 3 (and I'm sure I could also converge other orbital moments).
>>
>>However, the solution with +1.2 has by far the lowest total energy of
>>    
>>
>those
>  
>
>>three tests and is thus the best solution (and is also the one which you
>>get from my recommended procedure:
>>
>>runsp -so
>>x lapwdm -so -up
>>runsp -so -orb
>>
>>I'll test this further and discuss it with others, but my impression is
>>that the cross-term in case.vorbdu is either not correct (or it's usage in
>>lapwso is not ok) and at the moment one should remove it. After that LDA+U
>>+SO gives expected results.
>>
>>Regards
>>                                      P.Blaha
>>--------------------------------------------------------------------------
>>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>>Email: blaha@theochem.tuwien.ac.at    WWW:
>>    
>>
>http://info.tuwien.ac.at/theochem/
>  
>
>>--------------------------------------------------------------------------
>>
>>====
>>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>>To (un)subscribe send mail to
>>majordomo@zeus.theochem.tuwien.ac.at
>>====
>>
>>
>>    
>>
>
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>  
>



====
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------------------------------

Date: Mon, 2 Dec 2002 08:49:20 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: total core charge

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

the energy of your 1s-orbital is higher than the (default) energy (-6.0 Ry)
to distinguish between core and valence states.  So you don't have core
states for H.  The 1s-orbital is treated as a valence orbital.

kind regards,

Kevin Jorissen
kevin.jorissen@ua.ac.be

- ----- Original Message -----
From: "Hadi Arabi" <arabi_h@yahoo.com>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Sunday, December 01, 2002 2:13 PM
Subject: [WIEN]: total core charge


> ====
> Hadi Arabi <arabi_h@yahoo.com>
> submitted the following contribution:
> ====
>
> Dear wien user
> I work on Ice Cubic phase. I put Rmt=0.7 for H and
> Rmt=1.4 for O. After initialise we found the following
> data in case.outputst file for hydrogen.
> The total core Charge and total core charge inside
> sphere comes out zero. Does it makes sence? and what
> is the reason for it?
>
>
>                    H
> RHFS
>
>          OCCUPANCY    ENERGY(RYD)         (R4)
>      (R2)              (R)               (R-1)
>     (R-3)
>
>   1S      0.900    -5.5343653E-01     2.8859959E+01
>  3.2701173E+00     1.5496451E+00     9.8868262E-01
>   1S      0.100    -2.9298928E-01     7.6763743E+01
>  5.1153976E+00     1.9089845E+00     8.3795725E-01
>
>  TOTAL CHARGE FOR SPIN            1:
> 0.9000000000000004
>  TOTAL CHARGE FOR SPIN            1 INSIDE SPHERE:
> 0.1484428774001257
>  TOTAL CHARGE FOR SPIN            2:
> 0.1000000000000000
>  TOTAL CHARGE FOR SPIN            2 INSIDE SPHERE:
> 1.2145117228393798E-002
>  TOTAL CHARGE in sigma FOR SPIN            1:
>    0.0000000000000000E+000
>  TOTAL CHARGE in sigma FOR SPIN            1INSIDE
> SPHERE:
>    0.0000000000000000E+000
>  TOTAL CHARGE in sigma FOR SPIN            2:
>    0.0000000000000000E+000
>  TOTAL CHARGE in sigma FOR SPIN            2INSIDE
> SPHERE:
>    0.0000000000000000E+000
>  TOTAL CORE-CHARGE:
> 0.0000000000000000E+000
>  TOTAL CORE-CHARGE INSIDE SPHERE:
> 0.0000000000000000E+000
>
>  TOTAL ENERGY (RYD):               -0.966505
>      SUM OF EI:-5.2739181E-01     NUC:-1.9472202E+00
>   COUL:-7.5003037E-01
>      V-XC SPIN 1:-6.8721924E-01     E-XC SPIN
> 1:-5.4051577E-01
>      V-XC SPIN 2:-4.1960721E-02     E-XC SPIN
> 2:-2.9182614E-02
>
>
> __________________________________________________
> Do you Yahoo!?
> Yahoo! Mail Plus - Powerful. Affordable. Sign up now.
> http://mailplus.yahoo.com
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

====
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====

------------------------------

Date: Mon, 2 Dec 2002 08:54:59 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: A question

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

There is a compilation parameter called NMATMAX.  This parameter limits the
maximum matrix size allowed for lapw1 and lapw2.  If you have a large
system, then a certain value of rkmax may require such a     large basis
that the resulting matrix is larger than NMATMAX.  In this case, rkmax is
diminished until the matrixsize does not exceed nmatmax anymore.  In your
case.scf1 and case.output1 you can check the resulting rkmax.
If you need larger rkmax, you have to configure wien (siteconfig, then
dimension parameters, then make nmatmax larger and recompile lapw1 and
lapw2).

kind regards,
Kevin Jorissen
kevin.jorissen@ua.ac.be

- ----- Original Message -----
From: "whoming" <whoming@sohu.com>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Monday, December 02, 2002 2:52 AM
Subject: [WIEN]: A question


> ====
> "whoming" <whoming@sohu.com>
> submitted the following contribution:
> ====
>
> Dear all,
>          In one of my calculation,there is one WARNING message in case.scf
> file:
> :WARN :      WARNING: RKmax reduced due to NMATMAX
>          How dose it influence the result? To avoid such, what should I
do?
> Thank you very much!
> yours,
> whoming
> ----- Original Message -----
> From: "Peter Blaha" <pblaha@theochem.tuwien.ac.at>
> To: "WIEN" <wien@zeus.theochem.tuwien.ac.at>
> Sent: Friday, November 29, 2002 3:54 PM
> Subject: Re: [WIEN]: Problems with LDA+U+SO in Cerium systems.
>
>
> > ====
> > Peter Blaha <pblaha@theochem.tuwien.ac.at>
> > submitted the following contribution:
> > ====
> >
> > > We think we were too optimistic in our last message regarding LDA+U+SO
> > > calculations.
> > >
> > > We did the changes you suggested and as we told you in our reply it
> seemed
> > > to work properly: the spin magnetic moment had the correct value and
the
> > > density of states looked fine.
> > >
> > > However, after a message by Michelle and other tests we did, we
realized
> > > that the solution was not completely correct: this time the orbital
> moment
> > > had gone to zero.
> >
> > I've also done some Ce calculations by now, but I cannot verify your
last
> > message. However, I agree, the solution proposed in my last mail
requires
> > lapw1c.
> >
> > In my tests I have simply removed after orb:
> >
> > rm $file.vorbdu
> >
> > and than apply vorb in lapwso.
> >
> > Please do not forget, that one can obtain many different LDA+U solutions
> > depending on the starting density (and density matrix).
> >
> > When starting with a density from lda + SO and adding LDA+U I get
> >
> > including cross terms: spin:  -0.26032   orb: -0.54422 (with very poor
and
> >                        very slow convergence)
> > without crossterms (see above): spin: 1.16665  orb: -1.18953 (nice and
> quick)
> >
> > As usual I can also obtain other solutions, starting with
> >
> > SO + LDA+U (including crossterms): spin -1.18519    orb: 0.07087
> >   (since I started with a "negative" moment it remains negative)
> >
> > a density matrix with large m=+3 occupation: -1.18891   2.87868
> >
> > So you see all three solutions without cross term give a spin moment of
> 1.2,
> > while the orbital moment depends crucially on the starting dmat and was
> > 0, 1 or 3 (and I'm sure I could also converge other orbital moments).
> >
> > However, the solution with +1.2 has by far the lowest total energy of
> those
> > three tests and is thus the best solution (and is also the one which you
> > get from my recommended procedure:
> >
> > runsp -so
> > x lapwdm -so -up
> > runsp -so -orb
> >
> > I'll test this further and discuss it with others, but my impression is
> > that the cross-term in case.vorbdu is either not correct (or it's usage
in
> > lapwso is not ok) and at the moment one should remove it. After that
LDA+U
> > +SO gives expected results.
> >
> > Regards
> >                                       P.Blaha
>
> --------------------------------------------------------------------------
> > Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> > Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> > Email: blaha@theochem.tuwien.ac.at    WWW:
> http://info.tuwien.ac.at/theochem/
>
> --------------------------------------------------------------------------
> >
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
> > majordomo@zeus.theochem.tuwien.ac.at
> > ====
> >
> >
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

====
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------------------------------

Date: Mon, 2 Dec 2002 12:19:46 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: [WIEN]: case.scfdmup

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====


Dear wien-users,

I am puzzled by an unexpected factor 2 in the output of lapwdm. After running 
a converged scf-cycle with spin-polarization and spin-orbit coupling, I want 
to obtain the orbital moment of a Co-atom in my structure. Therefore, I first 
test the output of lapwdm with quantities that are known in the scf-file too.

1) Obtain the number of valence electrons inside Rmt :

case.indmc =

- -9.                      Emin cutoff energy
 5                       number of atoms for which density matrix is 
calculated
 1  4  0 1 2 3     index of 1st atom, number of L's, L1
 1 1           r-index, (l,s)index  

(the Co-atom is the first atom in case.struct) After running 'x lapwdm -c -so 
- -up', this is case.scfdmup :

  atom  L      upup        updn         dndn       total
:XOP01  0     1.16264     0.00000     1.14548     2.30812
:XOP01  1     3.11761     0.00000     3.11894     6.23655
:XOP01  2     4.46323     0.00000     1.53959     6.00282
:XOP01  3     0.00657     0.00000     0.00630     0.01286

The last column sums to 14.5603, which is almost identical to :CHA01up + 
:CHA01dn = 14.5639 in case.scf. No problems here.

2) Obtain the spin moment of Co :

case.indmc = 1 2 for r-index, (l,s)index

case.scfdmup =

  atom  L      upup        updn         dndn       total
:XOP01  0     0.58132     0.00000    -0.57274     0.00858
:XOP01  1     1.55880     0.00000    -1.55947    -0.00067
:XOP01  2     2.23161     0.00000    -0.76980     1.46182
:XOP01  3     0.00328     0.00000    -0.00315     0.00013

The upup and dndn columns are exactly ONE HALF of what is found at :QTL01 in 
case.scf. The sum of the last column (1.4699) too is about ONE HALF of :MMI01 
(2.93994).

QUESTION : For the total charge, lapwdm gives outputd that is directly 
comparable to case.scf. For the spin moment, one has to multiply this by 2. 
What about the other properties, that are not available in case.scf? I have 
the following values calculated by lapwdm :

orbital Co-moment = 0.079
spin Co-hff = -2.5 T
orbital Co-hff = 4.4 T

Should they be multiplied by two or not?

I did these tests (running the scf-cycle and lapwdm) with the release of May 
27 and with the latest release. Both gave identical results.

Thanks !
Stefaan

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------------------------------

Date: Mon, 2 Dec 2002 13:56:16 +0100 (MET)
From: Pavel Novak <novakp@fzu.cz>
Subject: Re: [WIEN]: case.scfdmup

====
Pavel Novak <novakp@fzu.cz>
submitted the following contribution:
====

Dear Stefaan,

there may be some misunderstanding - the factor two is factor which makes
from the electronic spin the spin magnetic moment in Bohr magnetons:
m_S = gS,  g=2.00
You can readily check the density matrix d:
its trace is number of electrons,
trace(d) up - trace(d) dn = m_S in Bohr magnetons,
l_z = sum_m m.d_mm     (sum over both up and down)
orbital momentum is calculated automatically - you do not need to write
the last line in .indmc.

Best regards
Pavel

On Mon, 2 Dec 2002, Stefaan Cottenier wrote:

> ====
> Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
> submitted the following contribution:
> ====
>
>
> Dear wien-users,
>
> I am puzzled by an unexpected factor 2 in the output of lapwdm. After running
> a converged scf-cycle with spin-polarization and spin-orbit coupling, I want
> to obtain the orbital moment of a Co-atom in my structure. Therefore, I first
> test the output of lapwdm with quantities that are known in the scf-file too.
>
> 1) Obtain the number of valence electrons inside Rmt :
>
> case.indmc =
>
> -9.                      Emin cutoff energy
>  5                       number of atoms for which density matrix is
> calculated
>  1  4  0 1 2 3     index of 1st atom, number of L's, L1
>  1 1           r-index, (l,s)index
>
> (the Co-atom is the first atom in case.struct) After running 'x lapwdm -c -so
> -up', this is case.scfdmup :
>
>   atom  L      upup        updn         dndn       total
> :XOP01  0     1.16264     0.00000     1.14548     2.30812
> :XOP01  1     3.11761     0.00000     3.11894     6.23655
> :XOP01  2     4.46323     0.00000     1.53959     6.00282
> :XOP01  3     0.00657     0.00000     0.00630     0.01286
>
> The last column sums to 14.5603, which is almost identical to :CHA01up +
> :CHA01dn = 14.5639 in case.scf. No problems here.
>
> 2) Obtain the spin moment of Co :
>
> case.indmc = 1 2 for r-index, (l,s)index
>
> case.scfdmup =
>
>   atom  L      upup        updn         dndn       total
> :XOP01  0     0.58132     0.00000    -0.57274     0.00858
> :XOP01  1     1.55880     0.00000    -1.55947    -0.00067
> :XOP01  2     2.23161     0.00000    -0.76980     1.46182
> :XOP01  3     0.00328     0.00000    -0.00315     0.00013
>
> The upup and dndn columns are exactly ONE HALF of what is found at :QTL01 in
> case.scf. The sum of the last column (1.4699) too is about ONE HALF of :MMI01
> (2.93994).
>
> QUESTION : For the total charge, lapwdm gives outputd that is directly
> comparable to case.scf. For the spin moment, one has to multiply this by 2.
> What about the other properties, that are not available in case.scf? I have
> the following values calculated by lapwdm :
>
> orbital Co-moment = 0.079
> spin Co-hff = -2.5 T
> orbital Co-hff = 4.4 T
>
> Should they be multiplied by two or not?
>
> I did these tests (running the scf-cycle and lapwdm) with the release of May
> 27 and with the latest release. Both gave identical results.
>
> Thanks !
> Stefaan
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>
>
>



====
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------------------------------

Date: Mon, 2 Dec 2002 21:34:29 +0800
From: "whoming" <whoming@sohu.com>
Subject: Re: [WIEN]: A question

====
"whoming" <whoming@sohu.com>
submitted the following contribution:
====

Thank you very much!
- ----- Original Message -----
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Monday, December 02, 2002 3:54 PM
Subject: Re: [WIEN]: A question


> ====
> "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
> submitted the following contribution:
> ====
>
> There is a compilation parameter called NMATMAX.  This parameter limits
the
> maximum matrix size allowed for lapw1 and lapw2.  If you have a large
> system, then a certain value of rkmax may require such a     large basis
> that the resulting matrix is larger than NMATMAX.  In this case, rkmax is
> diminished until the matrixsize does not exceed nmatmax anymore.  In your
> case.scf1 and case.output1 you can check the resulting rkmax.
> If you need larger rkmax, you have to configure wien (siteconfig, then
> dimension parameters, then make nmatmax larger and recompile lapw1 and
> lapw2).
>
> kind regards,
> Kevin Jorissen
> kevin.jorissen@ua.ac.be
>
> ----- Original Message -----
> From: "whoming" <whoming@sohu.com>
> To: <wien@zeus.theochem.tuwien.ac.at>
> Sent: Monday, December 02, 2002 2:52 AM
> Subject: [WIEN]: A question
>
>
> > ====
> > "whoming" <whoming@sohu.com>
> > submitted the following contribution:
> > ====
> >
> > Dear all,
> >          In one of my calculation,there is one WARNING message in
case.scf
> > file:
> > :WARN :      WARNING: RKmax reduced due to NMATMAX
> >          How dose it influence the result? To avoid such, what should I
> do?
> > Thank you very much!
> > yours,
> > whoming
> > ----- Original Message -----
> > From: "Peter Blaha" <pblaha@theochem.tuwien.ac.at>
> > To: "WIEN" <wien@zeus.theochem.tuwien.ac.at>
> > Sent: Friday, November 29, 2002 3:54 PM
> > Subject: Re: [WIEN]: Problems with LDA+U+SO in Cerium systems.
> >
> >
> > > ====
> > > Peter Blaha <pblaha@theochem.tuwien.ac.at>
> > > submitted the following contribution:
> > > ====
> > >
> > > > We think we were too optimistic in our last message regarding
LDA+U+SO
> > > > calculations.
> > > >
> > > > We did the changes you suggested and as we told you in our reply it
> > seemed
> > > > to work properly: the spin magnetic moment had the correct value and
> the
> > > > density of states looked fine.
> > > >
> > > > However, after a message by Michelle and other tests we did, we
> realized
> > > > that the solution was not completely correct: this time the orbital
> > moment
> > > > had gone to zero.
> > >
> > > I've also done some Ce calculations by now, but I cannot verify your
> last
> > > message. However, I agree, the solution proposed in my last mail
> requires
> > > lapw1c.
> > >
> > > In my tests I have simply removed after orb:
> > >
> > > rm $file.vorbdu
> > >
> > > and than apply vorb in lapwso.
> > >
> > > Please do not forget, that one can obtain many different LDA+U
solutions
> > > depending on the starting density (and density matrix).
> > >
> > > When starting with a density from lda + SO and adding LDA+U I get
> > >
> > > including cross terms: spin:  -0.26032   orb: -0.54422 (with very poor
> and
> > >                        very slow convergence)
> > > without crossterms (see above): spin: 1.16665  orb: -1.18953 (nice and
> > quick)
> > >
> > > As usual I can also obtain other solutions, starting with
> > >
> > > SO + LDA+U (including crossterms): spin -1.18519    orb: 0.07087
> > >   (since I started with a "negative" moment it remains negative)
> > >
> > > a density matrix with large m=+3 occupation: -1.18891   2.87868
> > >
> > > So you see all three solutions without cross term give a spin moment
of
> > 1.2,
> > > while the orbital moment depends crucially on the starting dmat and
was
> > > 0, 1 or 3 (and I'm sure I could also converge other orbital moments).
> > >
> > > However, the solution with +1.2 has by far the lowest total energy of
> > those
> > > three tests and is thus the best solution (and is also the one which
you
> > > get from my recommended procedure:
> > >
> > > runsp -so
> > > x lapwdm -so -up
> > > runsp -so -orb
> > >
> > > I'll test this further and discuss it with others, but my impression
is
> > > that the cross-term in case.vorbdu is either not correct (or it's
usage
> in
> > > lapwso is not ok) and at the moment one should remove it. After that
> LDA+U
> > > +SO gives expected results.
> > >
> > > Regards
> > >                                       P.Blaha
> >
>
> --------------------------------------------------------------------------
> > > Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> > > Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> > > Email: blaha@theochem.tuwien.ac.at    WWW:
> > http://info.tuwien.ac.at/theochem/
> >
>
> --------------------------------------------------------------------------
> > >
> > > ====
> > > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > > To (un)subscribe send mail to
> > > majordomo@zeus.theochem.tuwien.ac.at
> > > ====
> > >
> > >
> >
> >
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
> > majordomo@zeus.theochem.tuwien.ac.at
> > ====
> >
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
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> ====
>


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------------------------------

Date: Mon, 2 Dec 2002 21:34:38 +0800
From: "whoming" <whoming@sohu.com>
Subject: Re: [WIEN]: A question

====
"whoming" <whoming@sohu.com>
submitted the following contribution:
====

Thanks!
- ----- Original Message -----
From: "Peer Kruse" <kruse@lem.uni-karlsruhe.de>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Sunday, December 01, 2002 5:31 PM
Subject: Re: [WIEN]: A question


> ====
> Peer Kruse <kruse@lem.uni-karlsruhe.de>
> submitted the following contribution:
> ====
>
> Deaer Whoming,
> you have two possibilities, you can redeuce RKmax from the start and if
> this gives you not the desired
> accuracy you can increase NMATMAX to cover it. But then you have to
> recompile the WIEN code.
>
> yours
>
> Peer
>
> whoming wrote:
>
> >====
> >"whoming" <whoming@sohu.com>
> >submitted the following contribution:
> >====
> >
> >Dear all,
> >         In one of my calculation,there is one WARNING message in
case.scf
> >file:
> >:WARN :      WARNING: RKmax reduced due to NMATMAX
> >         How dose it influence the result? To avoid such, what should I
do?
> >Thank you very much!
> >yours,
> >whoming
> >----- Original Message -----
> >From: "Peter Blaha" <pblaha@theochem.tuwien.ac.at>
> >To: "WIEN" <wien@zeus.theochem.tuwien.ac.at>
> >Sent: Friday, November 29, 2002 3:54 PM
> >Subject: Re: [WIEN]: Problems with LDA+U+SO in Cerium systems.
> >
> >
> >
> >
> >>====
> >>Peter Blaha <pblaha@theochem.tuwien.ac.at>
> >>submitted the following contribution:
> >>====
> >>
> >>
> >>
> >>>We think we were too optimistic in our last message regarding LDA+U+SO
> >>>calculations.
> >>>
> >>>We did the changes you suggested and as we told you in our reply it
> >>>
> >>>
> >seemed
> >
> >
> >>>to work properly: the spin magnetic moment had the correct value and
the
> >>>density of states looked fine.
> >>>
> >>>However, after a message by Michelle and other tests we did, we
realized
> >>>that the solution was not completely correct: this time the orbital
> >>>
> >>>
> >moment
> >
> >
> >>>had gone to zero.
> >>>
> >>>
> >>I've also done some Ce calculations by now, but I cannot verify your
last
> >>message. However, I agree, the solution proposed in my last mail
requires
> >>lapw1c.
> >>
> >>In my tests I have simply removed after orb:
> >>
> >>rm $file.vorbdu
> >>
> >>and than apply vorb in lapwso.
> >>
> >>Please do not forget, that one can obtain many different LDA+U solutions
> >>depending on the starting density (and density matrix).
> >>
> >>When starting with a density from lda + SO and adding LDA+U I get
> >>
> >>including cross terms: spin:  -0.26032   orb: -0.54422 (with very poor
and
> >>                       very slow convergence)
> >>without crossterms (see above): spin: 1.16665  orb: -1.18953 (nice and
> >>
> >>
> >quick)
> >
> >
> >>As usual I can also obtain other solutions, starting with
> >>
> >>SO + LDA+U (including crossterms): spin -1.18519    orb: 0.07087
> >>  (since I started with a "negative" moment it remains negative)
> >>
> >>a density matrix with large m=+3 occupation: -1.18891   2.87868
> >>
> >>So you see all three solutions without cross term give a spin moment of
> >>
> >>
> >1.2,
> >
> >
> >>while the orbital moment depends crucially on the starting dmat and was
> >>0, 1 or 3 (and I'm sure I could also converge other orbital moments).
> >>
> >>However, the solution with +1.2 has by far the lowest total energy of
> >>
> >>
> >those
> >
> >
> >>three tests and is thus the best solution (and is also the one which you
> >>get from my recommended procedure:
> >>
> >>runsp -so
> >>x lapwdm -so -up
> >>runsp -so -orb
> >>
> >>I'll test this further and discuss it with others, but my impression is
> >>that the cross-term in case.vorbdu is either not correct (or it's usage
in
> >>lapwso is not ok) and at the moment one should remove it. After that
LDA+U
> >>+SO gives expected results.
> >>
> >>Regards
> >>                                      P.Blaha
>
>>--------------------------------------------------------------------------
> >>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> >>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> >>Email: blaha@theochem.tuwien.ac.at    WWW:
> >>
> >>
> >http://info.tuwien.ac.at/theochem/
> >
> >
>
>>--------------------------------------------------------------------------
> >>
> >>====
> >>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> >>To (un)subscribe send mail to
> >>majordomo@zeus.theochem.tuwien.ac.at
> >>====
> >>
> >>
> >>
> >>
> >
> >
> >====
> >WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> >To (un)subscribe send mail to
> >majordomo@zeus.theochem.tuwien.ac.at
> >====
> >
> >
>
>
>
> ====
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> ====
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>


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------------------------------

Date: Mon, 02 Dec 2002 16:47:57 +0100
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: Error message in the output

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

When running wien2k in parallel I error messages like the one below in 
the output:

STOP  LAPW0 END
STOP  orbital potential calculation END
STOP  orbital potential calculation END
STOP  LAPW1 END
STOP  LAPW1 END
STOP  LAPW1 END
STOP  LAPW1 END
STOP  LAPW1 END
STOP  LAPW1 END
STOP LAPW2 - FERMI; weighs written
STOP  LAPW2 END
STOP  LAPW2 END
STOP  LAPW2 END
STOP  LAPW2 END
STOP  LAPW2 END
STOP  LAPW2 END
1525-097 A READ statement using decimal base input found the invalid 
digit '*' in th
e input file.  The program will recover by assuming a zero in its place.
1525-097 A READ statement using decimal base input found the invalid 
digit '*' in th
e input file.  The program will recover by assuming a zero in its place.
STOP  SUMPARA END
STOP  SUMPARA END
STOP LAPW2 - FERMI; weighs written
STOP  LAPW2 END
STOP  LAPW2 END
STOP  LAPW2 END
STOP  LAPW2 END
STOP  LAPW2 END
STOP  LAPW2 END
1525-097 A READ statement using decimal base input found the invalid 
digit '*' in th
e input file.  The program will recover by assuming a zero in its place.
1525-097 A READ statement using decimal base input found the invalid 
digit '*' in th
e input file.  The program will recover by assuming a zero in its place.
1525-097 A READ statement using decimal base input found the invalid 
digit '*' in th
e input file.  The program will recover by assuming a zero in its place.
STOP  SUMPARA END
STOP  SUMPARA END
STOP  lapwdm END
STOP  lapwdm END
STOP  lapwdm END
STOP  lapwdm END
STOP  lapwdm END
STOP  lapwdm END
1525-097 A READ statement using decimal base input found the invalid 
digit '*' in th
e input file.
STOP  SUMPARA END
STOP  lapwdm END
STOP  lapwdm END
STOP  lapwdm END
STOP  lapwdm END
STOP  lapwdm END
STOP  lapwdm END
1525-097 A READ statement using decimal base input found the invalid 
digit '*' in th
e input file.STOP  SUMPARA END
STOP  CORE  END
STOP  CORE  END
STOP  MIXER END
in cycle 2    ETEST: 0   CTEST: 0
hup: Command not found.
STOP  LAPW0 END
STOP  orbital potential calculation END
STOP  orbital potential calculation END
STOP  LAPW1 END
STOP  LAPW1 END
...

As far as I can understand this READ statement error occurrs in SUMPARA 
when it is trying to read the case.scf2_* files. How could the 
case.scf2_* files be wrong in any way, I have NOT manipulated any of 
them? Is this a serious error? How can I avoid it?

Thanks for your replies!
Any suggestions are welcome!

Best regards,
Thomas Claesson


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------------------------------

Date: Mon, 2 Dec 2002 17:00:08 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: Error message in the output

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> Thomas Claesson <tcl@kth.se>
> submitted the following contribution:
> ====
>
> When running wien2k in parallel I error messages like the one below in
> the output:
>
> STOP  LAPW0 END
> STOP  orbital potential calculation END
> STOP  orbital potential calculation END
> STOP  LAPW1 END
>(...)
> STOP  LAPW2 END
> 1525-097 A READ statement using decimal base input found the invalid
> digit '*' in th
> e input file.  The program will recover by assuming a zero in its place.
> 1525-097 A READ statement using decimal base input found the invalid
> digit '*' in th
> e input file.  The program will recover by assuming a zero in its place.
> STOP  SUMPARA END
> STOP  SUMPARA END
>
> As far as I can understand this READ statement error occurrs in SUMPARA
> when it is trying to read the case.scf2_* files. How could the
> case.scf2_* files be wrong in any way, I have NOT manipulated any of
> them? Is this a serious error? How can I avoid it?

Have a look at the case.scf2_* and search for the '*'. Probably you somewhere 
have a field with '*****' where a number should be. This means wien has 
produced an output number that is to large to fit into the provided field, 
and that is usually an indication that something went wrong in the part of 
the scf-cycle prior to the place where the error happens. But what exactly 
could have gone wrong is difficult to tell with this information. Check your 
output for anything unusual, and try to trace back the origin of the error 
that way.

Stefaan

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------------------------------

Date: Mon, 2 Dec 2002 18:00:20 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: case.scfdmup

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====


Hello Pavel,

Thanks for your answer. I understand the reason now, but apparently the 
terminology in the manual is confusing :

> there may be some misunderstanding - the factor two is factor which makes
> from the electronic spin the spin magnetic moment in Bohr magnetons:
> m_S = gS,  g=2.00

According to section 7.7 (lapwdm) of the usersguide, (r,l)=(1,2) is "the 
projection of the spin moment inside the atomic sphere". Maybe this should be 
stated more unambigously?

I keep doubting about the orbital magnetic moment : is its value the number 
given in case.scfdmup/dn, or should this same factor 'g' be used? 

For orbital and dipolar contributions to the hyperfine field, I assume this 
'g'-problem does not occur. And as the header of case.scfdmup/dn states that 
'X' is e.g. the orbital hff in Tesla :

  Calculation of <X>, X=c*Xr(r)*Xls(l,s)
  Xr(r)    = (1/r**3)S (large component only)                 
  Xls(l,s) = L(dzeta)                                                   
  c= 12.51690 X=Bhf(orb) in Tesla  ,

I can be confident that here no conversion is needed.

Thanks !
Stefaan
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------------------------------

Date: Tue, 3 Dec 2002 05:21:38 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: Re: [WIEN]:

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear all,

Actually, I found that I got " LAPW2 crashed!", too. Is there any limit for 
the number of machines to perform the parallel calculation? Or my .machines has problem?

The few lines added to .machines :

1:147.8.148.180
1:147.8.148.181
1:147.8.148.182
1:147.8.148.183
1:147.8.148.184
1:147.8.148.185
1:147.8.148.186
1:147.8.148.187
1:147.8.148.188
1:147.8.148.189
granularity:3

How could I fix the problem? Actually, I have successfully got the results with 4 
machines before with other fewer k-point.

Thank you very much

Martin

On Mon, 2 Dec 2002, Ma Chi Chiu wrote:

> ====
> Ma Chi Chiu <martin@yangtze.hku.hk>
> submitted the following contribution:
> ====
> 
> Dear all,
>  
> I have some questions about parallel calculation. The parallel calculation 
> always dead with the error message in lapw1.error like:
> **  Error in Parallel LAPW1
> **  LAPW1 STOPPED at Sun Dec 1 22:15:17 HKT 2002
> ** check ERROR FILES!
> Error in LAPW1
> Error in LAPW1
> 
> Actually, the calculation has already finished 2 SCF cycyles. Then, why does 
> the calculation stop not in the 1 cycle if I got some mistake in the 
> parallelization? What should I do now?
> 
> Also, I got error in doing optic parallelization. The error is "OPTIC CRASHED!" Why?
> Thank you 
> 
> Martin
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 


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------------------------------

Date: Mon, 2 Dec 2002 18:40:33 -0300 (ARST)
From: Ruben Weht <ruweht@cnea.gov.ar>
Subject: Re: [WIEN]: Problems with LDA+U+SO in Cerium systems.

====
Ruben Weht <ruweht@cnea.gov.ar>
submitted the following contribution:
====

Dear Hai,

You are completely right.
We changed runsp_lapw according to Peter's suggestion but we did it just
in the real version of lapw1 and not in lapw1c.

As you said doing it correctly we have obtained the right result for
Ce-FCC, getting both magnetic and orbital moment different to zero for
the ground state.
We are very sorry for our mistake.

We also agree with you that both cases, using orb in lapw1c or removing
##.vorbdu, seem to prove that crossterms should not be included in
LDA+U+SO calculations.

One more problem we have found regarding this kind of calculations (life
is not so easy sometimes...): We have repeated the calculations starting
with several density matrixes to obtain the metastable states found by
Shick et al.
However, we can say that we have obtained too many states that look like
metastable ones.

For instance if we start with a density matrix (for the majority spin)
n_(m1,m2) equal to a pure (+3,+3) state it ends up very near to the
initial matrix.  But if you begin with a dmat with equal components
for +3 and -1 you will finish in a state much lower in energy (500 meV).
and with components n(-1,-1)=0.73, n(-1,-1)=0.24 and n(-1,+3)=-0.42
that is in a very good agreement with the one obtained by Shick et. al.

We still don't understand why, if the +3 and -1 states can mix in the FCC
structure, you can not go from the pure (+3,+3) state to the one with the
minimum energy inside that subspace.
We think in this way one can get some "false" metastable states.....

Something important is that we did obtain the correct ground state just
starting with the density matrix got from a LDA calculation.

Well, thanks a lot to you and Peter for your replies,
Best regards,

		Veronica and Ruben


*====================================================================*
|  Ruben Weht                             |  ruweht@cnea.gov.ar      |
|  Departmento de Fisica - CNEA           |  Tel: (54-11) 6772-7104  |
|  Avda. General Paz y Constituyentes     |  Fax: (54-11) 6772-7121  |
|  1650 - San Martin - ARGENTINA          |                          |
*====================================================================*




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------------------------------

Date: Tue, 3 Dec 2002 12:26:50 +0800 (CST)
From: =?gb2312?q?=B4=F3=CE=AA=20=D6=DC?= <zouwd1@yahoo.com.cn>
Subject: [WIEN]: Error in Mixer

====
=?gb2312?q?=B4=F3=CE=AA=20=D6=DC?= <zouwd1@yahoo.com.cn>
submitted the following contribution:
====

Dear Prof. P.Blaha and all wien user:
   When I run SCF cycle, there is an error message in
the 43 step (five days later!). Error message just
give me "Error in Mixer". I don't know where the
questions is. I appreciate any help!

With best regardes!
           
                           zouweidong 


_________________________________________________________
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------------------------------

Date: Tue, 3 Dec 2002 07:53:06 +0100 (MET)
From: Pavel Novak <novakp@fzu.cz>
Subject: Re: [WIEN]: case.scfdmup

====
Pavel Novak <novakp@fzu.cz>
submitted the following contribution:
====

Hello Stefaan,

you are right - no conversion factors are needed for Bhf, lapwdm gives the
orbital momentum again no conversion factor.

Regards Pavel

On Mon, 2 Dec 2002, Stefaan Cottenier wrote:

> ====
> Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
> submitted the following contribution:
> ====
>
>
> Hello Pavel,
>
> Thanks for your answer. I understand the reason now, but apparently the
> terminology in the manual is confusing :
>
> > there may be some misunderstanding - the factor two is factor which makes
> > from the electronic spin the spin magnetic moment in Bohr magnetons:
> > m_S = gS,  g=2.00
>
> According to section 7.7 (lapwdm) of the usersguide, (r,l)=(1,2) is "the
> projection of the spin moment inside the atomic sphere". Maybe this should be
> stated more unambigously?
>
> I keep doubting about the orbital magnetic moment : is its value the number
> given in case.scfdmup/dn, or should this same factor 'g' be used?
>
> For orbital and dipolar contributions to the hyperfine field, I assume this
> 'g'-problem does not occur. And as the header of case.scfdmup/dn states that
> 'X' is e.g. the orbital hff in Tesla :
>
>   Calculation of <X>, X=c*Xr(r)*Xls(l,s)
>   Xr(r)    = (1/r**3)S (large component only)
>   Xls(l,s) = L(dzeta)
>   c= 12.51690 X=Bhf(orb) in Tesla  ,
>
> I can be confident that here no conversion is needed.
>
> Thanks !
> Stefaan
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>
>
>



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------------------------------

Date: Tue, 3 Dec 2002 09:23:14 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]:

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> Ma Chi Chiu <martin@yangtze.hku.hk>
> submitted the following contribution:
> ====
>
> Actually, I found that I got " LAPW2 crashed!", too. Is there any limit for
> the number of machines to perform the parallel calculation? Or my .machines
> has problem?
>
> The few lines added to .machines :
>
> 1:147.8.148.180
> 1:147.8.148.181
> 1:147.8.148.182
> 1:147.8.148.183
> 1:147.8.148.184
> 1:147.8.148.185
> 1:147.8.148.186
> 1:147.8.148.187
> 1:147.8.148.188
> 1:147.8.148.189
> granularity:3
>
> How could I fix the problem? Actually, I have successfully got the results
> with 4 machines before with other fewer k-point.

I don't know the details of your case, but pay attention to the following 
points :

* You have 10 machines in your .machines. That means you should have at least 
10 k-points, otherwise it is useless to use that many machines. Use 
testpara_lapw to find an optimal distribution of k-points over your machines. 
For instance, if you have 16 k-points and use 10 machines, 6 machines will do 
2 k-points each, and 4 will do 1 each. If you use 8 machines, then all of 
them will do 2 points, and your calculation will take just as much time as 
with 10 machines, while you now have 2 machines free for other work. All this 
only effects efficiency however, it cannot explain your errors.

* If you are not sure exactly what you are doing, you risk to play too much in 
one directory, and left-over files from previous testing can spoil a next 
scf-cycle. Therefore, try to reinitialize the case your are trying in a clean 
new directory. Often this is sufficient to remove many problems.

Stefaan


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------------------------------

Date: Tue, 3 Dec 2002 02:20:51 -0800 (PST)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: SCF

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien users.
Ihave started SCF and In  Lapw1   got this
message"Cholsky INFO=269
SECLRA-ZPOTRE (LAPACK) failed     what this mean?or
What is its reason?
What should be done for eliminating it?
Thank you for the guide.
H-Salehi 
Dept of physics
Ferdowsi University
MASHHAD IRAN



=====
Hamdollah Salehi
Dept of Physics
Ferdowsi University
Mashhad IRAN
Post boxs 1436
Post code 91775
faxs

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------------------------------

Date: Tue, 3 Dec 2002 14:57:10 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: case.scfdmup

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Thanks for your answer. I understand the reason now, but apparently the
> terminology in the manual is confusing :
>
> > there may be some misunderstanding - the factor two is factor which makes
> > from the electronic spin the spin magnetic moment in Bohr magnetons:
> > m_S = gS,  g=2.00

Thank's, I'll change that for the next release!



                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
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Date: Mon, 02 Dec 2002 17:43:13 +0100
From: Peer Kruse <kruse@lem.uni-karlsruhe.de>
Subject: [WIEN]: This_file_should_not_exist

====
Peer Kruse <kruse@lem.uni-karlsruhe.de>
submitted the following contribution:
====

Dear Wien Community,
I set up two Linux PC for parallel computation and everything seems to 
work fine with the precompiled
Wien2k. But a sequence of This_file_should_not_exist files is generated. 
Is this harmful or is it only
garbage from sumpara initialization?

thank you

Peer

++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
Peer Kruse
Laboratorium für Elektronenmikroskopie
Engesserstr. 7
76128 Universität Karlsruhe

Tel 0721/608 8682
Fax 0721/608 3721

peer.kruse@lem.uni-karlsruhe.de
++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++


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------------------------------

Date: Tue, 3 Dec 2002 17:56:32 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: This_file_should_not_exist

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I set up two Linux PC for parallel computation and everything seems to
> work fine with the precompiled
> Wien2k. But a sequence of This_file_should_not_exist files is generated.
> Is this harmful or is it only
> garbage from sumpara initialization?

It is harmless and is just a "trial_name" when testing wether  case.dmatup/dn
files exist. I agree, it could have been done in a more clever way or at least
a less confusing name would be "This_file_should_be_empty".

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Wed, 4 Dec 2002 02:06:42 -0800 (PST)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: SCF

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

DearMr Hashemifar
salam
I hope you and your family are ok.
Ihave started SCF and    got this
message"SELECT-no energy Limits found for l=2
'SELECT' -E-bottom  -2.48500   E-top  -200.00000    
what this mean?or
What is its reason?What should be done for eliminating
it?

Thank you for the guide.

H-Salehi 



=====
Hamdollah Salehi
Dept of Physics
Ferdowsi University
Mashhad IRAN
Post boxs 1436
Post code 91775
faxs

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------------------------------

Date: Wed, 4 Dec 2002 02:10:00 -0800 (PST)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: SCF

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear  All
Ihave started SCF and    got this
message"SELECT-no energy Limits found for l=2
'SELECT' -E-bottom  -2.48500   E-top  -200.00000    
what this mean?or
What is its reason?What should be done for eliminating
it?

Thank you for the guide.

H-Salehi 



=====
Hamdollah Salehi
Dept of Physics
Ferdowsi University
Mashhad IRAN
Post boxs 1436
Post code 91775
faxs

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------------------------------

Date: Wed, 4 Dec 2002 02:12:05 -0800 (PST)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: SCF-2

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear  All

Ihave started SCF and In  Lapw1   got this
message"Cholsky INFO=269SECLRA-ZPOTRE (LAPACK) failed 
   what this mean?or
What is its reason?What should be done for eliminating
it?
would you please send me paper:

Thank you for the guide.

H-Salehi 


=====
Hamdollah Salehi
Dept of Physics
Ferdowsi University
Mashhad IRAN
Post boxs 1436
Post code 91775
faxs

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------------------------------

Date: Wed, 4 Dec 2002 11:18:23 +0100 (MET)
From: Pio =?ISO-8859-1?Q?B=E4ttig?= <baettigp@gmx.net>
Subject: [WIEN]: Wien Compile Warnings

====
Pio =?ISO-8859-1?Q?B=E4ttig?= <baettigp@gmx.net>
submitted the following contribution:
====

Dear Wien users

I compiled Wien2k, 28.11.02 on a Digital Personal Workstation Alpha
21164-433, using the Compaq F90 compiler and the default settings. I got the
following warnings:

> cat SRC_*/compile.msg | grep -i warn
f90: Warning: i1mach.f, line 881: Variable IMACH is used before its value
has been defined
f90: Warning: joint.f, line 288: Variable ISIWITCH is used before its value
has been defined
f90: Warning: fermi.f, line 348: Variable IUNIT is used before its value has
been defined
f90: Warning: fermi.f, line 352: Variable STATUS is used before its value
has been defined
f90: Warning: fermi.f, line 352: Variable FORM is used before its value has
been defined
f90: Warning: outp.f, line 234: Variable ITAPE is used before its value has
been defined
f90: Warning: fermi.f, line 348: Variable IUNIT is used before its value has
been defined
f90: Warning: fermi.f, line 352: Variable STATUS is used before its value
has been defined
f90: Warning: fermi.f, line 352: Variable FORM is used before its value has
been defined
f90: Warning: outp.f, line 234: Variable ITAPE is used before its value has
been defined
f90: Warning: sumlm.f, line 106: Variable C3 is used before its value has
been defined
f90: Warning: sumlm.f, line 106: Variable C3 is used before its value has
been defined
f90: Warning: gtfnam2.f, line 127: A jump into a block from outside the
block has occurred.   [900]
f90: Warning: gtfnam2.f, line 127: A jump into a block from outside the
block has occurred.   [900]
f90: Warning: couple.f, line 47: Variable THETA is used before its value has
been defined
f90: Warning: parop.f, line 94: Variable IS is used before its value has
been defined
f90: Warning: parop.f, line 94: Variable E3 is used before its value has
been defined
f90: Warning: gtfnam2.f, line 127: A jump into a block from outside the
block has occurred.   [900]
f90: Warning: psplit.f, line 46: Variable DUMMY is used before its value has
been defined
f90: Warning: lomain.f, line 12: Because of COMMON, the alignment of object
is inconsistent with its type   [BKROT]
f90: Warning: lomain.f, line 12: Because of COMMON, the alignment of object
is inconsistent with its type   [BKRLOC]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: param.inc, line 9: Because of COMMON, the alignment of object
is inconsistent with its type   [SHIFTSG]
f90: Warning: gtfnam2.f, line 127: A jump into a block from outside the
block has occurred.   [900]
f90: Warning: atpar.f, line 260: Variable L is used before its value has
been defined
f90: Warning: atpar.f, line 237: Variable L is used before its value has
been defined

Should I change any of the compiler options?

Thank you very much in advance for every hint.

Kind regards

Pio Bättig
University of Fribourg
Department of chemistry

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------------------------------

Date: Wed, 04 Dec 2002 11:21:25 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: About LSTART

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Xing,

there should be no unit 100... look in lstart.def. Some runtime 
environments does not allow Fortran units larger than 99, so if there is 
a unit 100 (the first number in each line of lstart.def is the "unit"), 
change it to something else.

Best regards,
Torsten.

Xing Gao wrote:

>====
>Xing Gao <xinggao@gh1.sims.nrc.ca>
>submitted the following contribution:
>====
>
>Dear wien2k user,
>
>When I run the lstart there is an error called:
>
>"lib-4190 : UNRECOVERABLE library error
>
>Encountered during a list-directed READ from unit 100
>Fortran unit 100 is connected to a sequential formatted text file
>  (standard input).
>IOT Trap"
>
>I don't know it is something wrong in the Library of our system, or the
>definition of "unit 100" in the code is not suitable, or something
>else. If you know please give me some suggestion. Thank you very much.
>
>Xing 
>
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>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Wed, 04 Dec 2002 11:41:27 +0100
From: Thomas Claesson <tcl@kth.se>
Subject: [WIEN]: Data missing in output files

====
Thomas Claesson <tcl@kth.se>
submitted the following contribution:
====

Dear Wien users and developers!

Trying to run AFII NiO with LDA+U I discovered that instead of data 
there are  only "******" in two places in my output files. In 
case.scf2dn and case.scf2up the first line is

:GMA  : POTENTIAL AND CHARGE CUT-OFF  14.00 Ry**.5

In case.outputdmdn and case.outputdmup these lines are present:

:ORB01:  ORBITAL MOMENT:  0.00000  0.00000  0.00000 PROJECTION ON M  0.00000
:SPI01:  SPIN MOMENT:****************************** PROJECTION ON M*********

:ORB02:  ORBITAL MOMENT:  0.00000  0.00000  0.00000 PROJECTION ON M  0.00000
:SPI02:  SPIN MOMENT:****************************** PROJECTION ON M*********

My case.indm file looks like:
- -9.
2
1 1 2
2 1 2
0 0

and my case.in2 looks like:

TOT             (TOT,FOR,QTL,EFG,FERMI)
       -9.0      44.0 0.50 0.05                EMIN, NE, ESEPERMIN, ESEPER0
TETRA    0.000          (GAUSS,ROOT,TEMP,TETRA,ALL      eval)
  0 0 2 0 4 0 4 3 6 0 6 3 6 6
  0 0 2 0 4 0 4 3 6 0 6 3 6 6
  0 0 1 0 2 0 3 0 3 3 4 0 4 3 5 0 5 3 6 0 6 3 6 6
  14.          GMAX
FILE        FILE/NOFILE  write recprlist

Something obviously has gone wrong here! I would appreciate if someone 
could give a hint about what and why.


Thanks for your replies!

Best regards,
Thomas Claesson

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------------------------------

Date: Wed, 4 Dec 2002 10:40:28 -0700 (MST)
From: Martin Gelfand <gelfand@lamar.colostate.edu>
Subject: Re: [WIEN]: Wien Compile Warnings

====
Martin Gelfand <gelfand@lamar.ColoState.EDU>
submitted the following contribution:
====

The "used before defined" warnings are not unique to you,
and you shouldn't worry about them.  They arise because
those variables are "output arguments" in a subroutine,
so they actually _are_ defined before being used in the
routine in question, but there is no way for the compiler
to recognize that.

You could tell your compiler not to report warnings, but
there's not much of a point.

Regards,
Martin Gelfand
Dept of Physics
Colorado State University

On Wed, 4 Dec 2002, Pio [ISO-8859-1] Bättig wrote:

> ====
> Pio =?ISO-8859-1?Q?B=E4ttig?= <baettigp@gmx.net>
> submitted the following contribution:
> ====
> 
> Dear Wien users
> 
> I compiled Wien2k, 28.11.02 on a Digital Personal Workstation Alpha
> 21164-433, using the Compaq F90 compiler and the default settings. I got the
> following warnings:
> 
> > cat SRC_*/compile.msg | grep -i warn
> f90: Warning: i1mach.f, line 881: Variable IMACH is used before its value
> has been defined
>....
> f90: Warning: atpar.f, line 260: Variable L is used before its value has
> been defined
> f90: Warning: atpar.f, line 237: Variable L is used before its value has
> been defined
> 
> Should I change any of the compiler options?
> 
> Thank you very much in advance for every hint.
> 
> Kind regards
> 
> Pio Bättig
> University of Fribourg
> Department of chemistry
> 
> -- 
> +++ GMX - Mail, Messaging & more  http://www.gmx.net +++
> NEU: Mit GMX ins Internet. Rund um die Uhr für 1 ct/ Min. surfen!
> 
> ====
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> ====
> 

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------------------------------

Date: Thu, 05 Dec 2002 08:39:32 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Wien Compile Warnings

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Actually, the "ISIWITCH" should probably be corrected to ISWITCH, but 
otherwise it looks harmless, I think.

Best regards,
Torsten Andersen.

Martin Gelfand wrote:

>====
>Martin Gelfand <gelfand@lamar.ColoState.EDU>
>submitted the following contribution:
>====
>
>The "used before defined" warnings are not unique to you,
>and you shouldn't worry about them.  They arise because
>those variables are "output arguments" in a subroutine,
>so they actually _are_ defined before being used in the
>routine in question, but there is no way for the compiler
>to recognize that.
>
>You could tell your compiler not to report warnings, but
>there's not much of a point.
>
>Regards,
>Martin Gelfand
>Dept of Physics
>Colorado State University
>
>On Wed, 4 Dec 2002, Pio [ISO-8859-1] Bättig wrote:
>
>>====
>>Pio =?ISO-8859-1?Q?B=E4ttig?= <baettigp@gmx.net>
>>submitted the following contribution:
>>====
>>
>>Dear Wien users
>>
>>I compiled Wien2k, 28.11.02 on a Digital Personal Workstation Alpha
>>21164-433, using the Compaq F90 compiler and the default settings. I got the
>>following warnings:
>>
>>>cat SRC_*/compile.msg | grep -i warn
>>>
>>f90: Warning: i1mach.f, line 881: Variable IMACH is used before its value
>>has been defined
>>....
>>f90: Warning: atpar.f, line 260: Variable L is used before its value has
>>been defined
>>f90: Warning: atpar.f, line 237: Variable L is used before its value has
>>been defined
>>
>>Should I change any of the compiler options?
>>
>>Thank you very much in advance for every hint.
>>
>>Kind regards
>>
>>Pio Bättig
>>University of Fribourg
>>Department of chemistry
>>
>>-- 
>>+++ GMX - Mail, Messaging & more  http://www.gmx.net +++
>>NEU: Mit GMX ins Internet. Rund um die Uhr für 1 ct/ Min. surfen!
>>
>>====
>>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>>To (un)subscribe send mail to
>>majordomo@zeus.theochem.tuwien.ac.at
>>====
>>
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Thu, 5 Dec 2002 23:8:17 +0800
From: "Wenhui Xie" <xiewh@sun20.iphy.ac.cn>
Subject: [WIEN]: 'LOPW' - Plane waves exhausted

====
"Wenhui Xie" <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear Sir,

We miss a strange error in a tetrahedral structure.
It stop at the lapw1 of first cycle.
We get a error message in uplapw1.error:
 'LOPW' - Plane waves exhausted

Thanks for your replies!


Yours 
Wenhui Xie
  




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------------------------------

End of wien-digest V2002 #46
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #47
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
Errors-To: owner-wien-digest@theochem.tuwien.ac.at
Precedence: bulk


wien-digest       Thursday, December 12 2002       Volume 2002 : Number 047




----------------------------------------------------------------------

Date: Thu, 05 Dec 2002 16:15:55 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: 'LOPW' - Plane waves exhausted

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

In which version of the wien code? This should not happen for normal 
cases in Wien2k...

Anyway, it has been discussed before, so read the digest.

Best regards,
Torsten.

Wenhui Xie wrote:

>====
>"Wenhui Xie" <xiewh@sun20.iphy.ac.cn>
>submitted the following contribution:
>====
>
>Dear Sir,
>
>We miss a strange error in a tetrahedral structure.
>It stop at the lapw1 of first cycle.
>We get a error message in uplapw1.error:
> 'LOPW' - Plane waves exhausted
>
>Thanks for your replies!
>
>
>Yours 
>Wenhui Xie
>  
>
>
>
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Thu, 5 Dec 2002 17:56:45 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: 'LOPW' - Plane waves exhausted

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> We miss a strange error in a tetrahedral structure.
> It stop at the lapw1 of first cycle.
> We get a error message in uplapw1.error:
>  'LOPW' - Plane waves exhausted

This means your struct file is wrong!

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 5 Dec 2002 23:48:18 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: 'LOPW' - Plane waves exhausted

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> > We miss a strange error in a tetrahedral structure.
> > It stop at the lapw1 of first cycle.
> > We get a error message in uplapw1.error:
> >  'LOPW' - Plane waves exhausted
>
> This means your struct file is wrong!
In addition to the Peter's comment, this error occurs in lapw1 (up/dn) if
Rmt*Kmax<4.45 in case.in1. One can check the above given condition selecting
Rmt*Kmax=4.44 or less than this value even for every simple case, e.g. fcc
structure containing one atom! The version of the code had been nicely
touched by Torsten, which in this point I did agree and remember that old
versions of wien2k code worked even employing cutoff less than 4.45 for the
plane waves. In the mailing list, as it was mentioned by Torsten, there is a
discussion between us in this respect. At that time I used Rmt*Kmax<3 to
just speed up to perform some tests due to many atoms in the structure we
were struggling with it. But, the "LOPW' - Plane waves exhausted" error did
not allow me to conquer the problem. I said this story, since I would
emphasis on this point that I allowed myself to use such an small Rmt*Kmax,
because I had used before even Rmt*Kmax=2 successfully. This would be
considered as a telltale to show that old versions of wien2k worked for
small cutoff's. It will be great if the authors fix this problem, so that we
can use again small cutoff's for doing test to run one cycle or more  to
just see what is going on in the cases containing many atoms per their cells
before going through them within well-converged SCF's.
        Your,
        S. Jalali.

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Date: Thu, 5 Dec 2002 17:52:23 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: .machine file

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====



Dear Wien2k users

       We compiled WIEN2k_02(release 21 Oct 02) on a shared memory IBM
architecture(AIX) (total of 4 nodes, each node having 16 power4
processors) with xlf90 for serial and mpxlf90, MPI, scalapack, pblas etc.
for fine grained parallel compilation. The compilation and linking was
successful producing *.para *_mpi executables in addition to serial
executables. 

We tested the executables on GaAs in serial mode. It works fine.

1) What could be the structure of .machines file for running the 
fine grained parallel mode? For example, suppose I have 8 kpoints
in the IBZ for GaAs. how they  should be distributed for running on only
one node having 16 processors say. The node has a name say name1.
all the processors have same speed so do all the nodes.

I think of the  following .machines file:

8:longhorn1:8

where longhorn1 node(one of the four node) get 8 k-points and it will be 
distributed among 8 processors out of 16 processors in this node.

2) During compilation, the MPI command selected was
 
 poe _EXEC_ -shared_memory yes -procs _NP_ -hfile _HOSTS_

We have poe(parallel opterating environment to run the parallel job). 

will the following command in the batch job file for  
fine-grained parallel run work?

poe ./run_lapw -p -hfile .machines

will poe pick up the lapw0_mpi so on for the run during the scf cycle?
is -p necessary?

( the information about the number of processors will already be there in 
the batch script and poe should recognize the mpi executable so no need
to put -shared_meomory yes in the above "poe" line i feel).

I have gone through the users-manual.

I will appreciate of any help in this regard.

regards
sahu

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Date: Fri, 6 Dec 2002 09:21:00 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: .machine file

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
> submitted the following contribution:
> ====
>
> 1) What could be the structure of .machines file for running the
> fine grained parallel mode? For example, suppose I have 8 kpoints
> in the IBZ for GaAs. how they  should be distributed for running on only
> one node having 16 processors say. The node has a name say name1.
> all the processors have same speed so do all the nodes.
>
> I think of the  following .machines file:
>
> 8:longhorn1:8
>
> where longhorn1 node(one of the four node) get 8 k-points and it will be
> distributed among 8 processors out of 16 processors in this node.

I'm not sure whether I understand your question correctly, but it seems you 
are mixing two things. If you want to use the mpi version, you can in your 
example run a case with 8 k-points on 16 machines simultaneously, i.e. all 16 
machines are effectively used. But from your trial .machines, I assume you 
are satisfied with using 1 machine for each of the 8 k-points, and leaving 
the 8 other machines unused. For that purpose, you don't need mpi. Use the 
following .machines :

1:longhorn1
1:longhorn1
1:longhorn1
1:longhorn1
1:longhorn1
1:longhorn1
1:longhorn1
1:longhorn1
granularity:1

and use the -p switch with your run(sp)-command.

The queing system in our SP3 system distributes the jobs to any machine of the 
system that is available at that time. You never know before which one it 
will be. Therefore, if you are in such a case, you have to create your 
.machines on-the-fly. The following script :

#! /bin/csh
setenv kortenaam `hostname`
setenv langenaam $kortenaam'.cc.kuleuven.ac.be'
setenv lijn1 '14:'$langenaam
setenv lijn2 '14:'$langenaam
setenv lijn3 '14:'$langenaam
setenv gran  'granularity:1'
echo $lijn1 > .machines
echo $lijn2 >> .machines
echo $lijn3 >> .machines
echo $gran  >> .machines
cat .machines

generates the following .machines :

14:sp27.cc.kuleuven.ac.be
14:sp27.cc.kuleuven.ac.be
14:sp27.cc.kuleuven.ac.be
granularity:1

when the queing system detects it has to run the job on machine 
sp27.cc.kuleuven.ac.be.

Stefaan

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------------------------------

Date: Fri, 6 Dec 2002 10:33:06 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: 'LOPW' - Plane waves exhausted

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> In addition to the Peter's comment, this error occurs in lapw1 (up/dn) if
> Rmt*Kmax<4.45 in case.in1. One can check the above given condition selecting
> Rmt*Kmax=4.44 or less than this value even for every simple case, e.g. fcc
> structure containing one atom! The version of the code had been nicely
> touched by Torsten, which in this point I did agree and remember that old
> versions of wien2k code worked even employing cutoff less than 4.45 for the
> plane waves. In the mailing list, as it was mentioned by Torsten, there is a
> discussion between us in this respect. At that time I used Rmt*Kmax<3 to
> just speed up to perform some tests due to many atoms in the structure we
> were struggling with it. But, the "LOPW' - Plane waves exhausted" error did
> not allow me to conquer the problem. I said this story, since I would
> emphasis on this point that I allowed myself to use such an small Rmt*Kmax,
> because I had used before even Rmt*Kmax=2 successfully. This would be
> considered as a telltale to show that old versions of wien2k worked for
> small cutoff's. It will be great if the authors fix this problem, so that we
> can use again small cutoff's for doing test to run one cycle or more  to
> just see what is going on in the cases containing many atoms per their cells
> before going through them within well-converged SCF's.

a) I don't believe that we have changed anything or introduced anything
preventing a small RKMax in newer WIEN2k versions.

b) There could be a difference between WIEN97 and WIEN2k, because in APW+lo
additional "local orbitals" are introduced and you need more PWs for them.
This brings me to the main point:

c) Each LO is attatched to a "symmetry-adapted" plane-wave. So:
   i) when your basis set (RKmax) is rediculous small than it migth not find
   such a plane wave (You should it, when you have more LOs than PWs ???)
   ii) When your struct file is wrong (e.g it contains one atom twice) than
   it cannot find a "symmetry-adapted" plane-wave and the message
       "LOPW' - Plane waves exhausted" appears. This is the "common" problem.


> because I had used before even Rmt*Kmax=2 successfully.

What is "successfully" ??? This is completely rediculous and I'm tempted to
insert some code which definitely prevents such calculations !!!!

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Fri, 6 Dec 2002 14:52:37 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: 'LOPW' - Plane waves exhausted

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> a) I don't believe that we have changed anything or introduced anything
> preventing a small RKMax in newer WIEN2k versions.
Please trust one more!!!

> b) There could be a difference between WIEN97 and WIEN2k
> > because I had used before even Rmt*Kmax=2 successfully.
I would paste below something submitted from you in August 22, 2002, when we
were using wien2k code and not wien97 code in an e-mail with the subject of
"large system with hydrogens".
"With 84 DIFFICULT atoms (because of small spheres) it is certainly
a big calculation, but should be feasable eventually (start with RKmax=2.5)"

> What is "successfully" ???
Doing one cycle or more with no LOPW error emploing EKmax<4.45 is
successfully perfomed, whcih does not men a successfull caculation!!!
> This is completely rediculous and I'm tempted to
> insert some code which definitely prevents such calculations !!!!
As one now is tempted to believe that it is prevented.
        Your,
        S. Jalali.

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------------------------------

Date: Fri, 6 Dec 2002 12:16:44 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: hello

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear Dr. Stefaan

       thanx and I very much appreciate your  help.

1) your suggested .machine file , 

1:longhorn1
1:longhorn1
1:longhorn1
1:longhorn1
1:longhorn1
1:longhorn1
1:longhorn1
1:longhorn1
granularity:1

is for k-point parallaization run if I wish to use only 8 processors 
out of 16 processors availble on longhorn1 and leaving 8 others idle. 
am I right?

for launching such runs, do I have to include in the batch job script

poe ./run(sp) -p .machines or some different command to run k-point 
parallization.

2) I do wish to use "mpi" executable.  I do wish to use all the 16 
machines for 8  k-points for example. Then according to your suggestion, I 
should include in the job script(given below), the following:
_______________________________________________________________
setenv kortenaam `hostname`
setenv langenaam $kortenaam'.cc.kuleuven.ac.be'(here .cc.kuleuven.ac.be 
would be replaced by appropriate address)
setenv lijn1 '14:'$langenaam
setenv lijn2 '14:'$langenaam
setenv lijn3 '14:'$langenaam
setenv gran  'granularity:1'
echo $lijn1 > .machines
echo $lijn2 >> .machines
echo $lijn3 >> .machines
echo $gran  >> .machines
cat .machines
____________________________________________________________________________ 

what does "granularity" does? if I change
the granularity value to some other values how does it affect the 
the code?

_____________________________________________________________
2) The job script for submitting the MPI parallel jobs on our SP4 looks 
like:
#!/usr/bin/csh
#@ job_name = gamo-nonmag
#@ output =$(job_name).o$(jobid)
#@ error = $(job_name).o$(jobid)
#@ initialdir = /gpfs/utexas/ph/phaa406/GaMo
#@ job_type = parallel
#@ environment = COPY_ALL; MP_SHARED_MEMORY=yes;
#@ resources = ConsumableCpus(1) ConsumableMemory(1gb)
#@ notify_user = sahu@matter3.ph.utexas.edu
#@ node = 1
#@ tasks_per_node = 16
#@ class = normal
#@ notification=error
#@ wall_clock_limit = 24:00:00
#@ notification=error
#@ notification = complete
#@ queue
poe ./(WIEN2k  executable)
____________________________________

while compiling the code, I selected  the MPI command to be:

 poe _EXEC_ -shared_memory yes -procs _NP_ -hfile _HOSTS_

then in the above job script file, what should come after poe ./(WIEN2k
executable)? for launching WIEN2k MPI jobs on SP$?  Do I need to put "-p"  
with the "WIEN executable" for MPI parallel jobs?

Pl. let me know If I am not clear this time.

regards
sahu


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------------------------------

Date: Fri, 6 Dec 2002 13:15:13 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: hello

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear Dr. Stefaan

1) K-point parallelization is now clear and the run is successful. I 
played with differnet k-points with different no. of processors with
the .machines file you suggested and it works fine. I used in the
batch script just ./run(sp) -p. No "poe". thanx

2) pl. let me know about my query about "mpi" run.

regards
sahu

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------------------------------

Date: Fri, 06 Dec 2002 08:43:18 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: 'LOPW' - Plane waves exhausted

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Sorry, Saeid, but I have to correct you on this one. I have a 
calculation with CO_2 where I use rmt*kmax=4 to speed things up in the 
beginning, and there are no problems running it. It affects the quality 
of the total energy convergence, but I can live with that.

Best regards,
Torsten Andersen.

Saeid Jalali wrote:

>====
>"Saeid Jalali" <sjalali@cc.iut.ac.ir>
>submitted the following contribution:
>====
>
>>>We miss a strange error in a tetrahedral structure.
>>>It stop at the lapw1 of first cycle.
>>>We get a error message in uplapw1.error:
>>> 'LOPW' - Plane waves exhausted
>>>
>>This means your struct file is wrong!
>>
>In addition to the Peter's comment, this error occurs in lapw1 (up/dn) if
>Rmt*Kmax<4.45 in case.in1. One can check the above given condition selecting
>Rmt*Kmax=4.44 or less than this value even for every simple case, e.g. fcc
>structure containing one atom! The version of the code had been nicely
>touched by Torsten, which in this point I did agree and remember that old
>versions of wien2k code worked even employing cutoff less than 4.45 for the
>plane waves. In the mailing list, as it was mentioned by Torsten, there is a
>discussion between us in this respect. At that time I used Rmt*Kmax<3 to
>just speed up to perform some tests due to many atoms in the structure we
>were struggling with it. But, the "LOPW' - Plane waves exhausted" error did
>not allow me to conquer the problem. I said this story, since I would
>emphasis on this point that I allowed myself to use such an small Rmt*Kmax,
>because I had used before even Rmt*Kmax=2 successfully. This would be
>considered as a telltale to show that old versions of wien2k worked for
>small cutoff's. It will be great if the authors fix this problem, so that we
>can use again small cutoff's for doing test to run one cycle or more  to
>just see what is going on in the cases containing many atoms per their cells
>before going through them within well-converged SCF's.
>        Your,
>        S. Jalali.
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Sat, 7 Dec 2002 02:49:19 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: 'LOPW' - Plane waves exhausted

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

Thank you Torsten. According to the valuable comment of Peter the lowest
value of RKmax depends on the number of LO's.  I have checked this fact and
found that it is 2.8 for C or O with the same no. of LO's, and thus for your
CO_2 case, while this is 4.45 for Yb. You will see LOPW error using 2.7
instead of 4. Now everything is clear, and confirms the fact indicated by
Peter that nothing has been changed or introduced preventing a small RKMax
in newer WIEN2k versions (at least up to now!). At that time, when I
exploited a ridiculously small value 2, I had to work on H systems with no
LO's.
        Your,
        S. Jalali.
> Sorry, Saeid, but I have to correct you on this one. I have a
> calculation with CO_2 where I use rmt*kmax=4 to speed things up in the
> beginning, and there are no problems running it. It affects the quality
> of the total energy convergence, but I can live with that.
>
> Best regards,
> Torsten Andersen.
>
> Saeid Jalali wrote:
>
> >====
> >"Saeid Jalali" <sjalali@cc.iut.ac.ir>
> >submitted the following contribution:
> >====
> >
> >>>We miss a strange error in a tetrahedral structure.
> >>>It stop at the lapw1 of first cycle.
> >>>We get a error message in uplapw1.error:
> >>> 'LOPW' - Plane waves exhausted
> >>>
> >>This means your struct file is wrong!
> >>
> >In addition to the Peter's comment, this error occurs in lapw1 (up/dn) if
> >Rmt*Kmax<4.45 in case.in1. One can check the above given condition
selecting
> >Rmt*Kmax=4.44 or less than this value even for every simple case, e.g.
fcc
> >structure containing one atom! The version of the code had been nicely
> >touched by Torsten, which in this point I did agree and remember that old
> >versions of wien2k code worked even employing cutoff less than 4.45 for
the
> >plane waves. In the mailing list, as it was mentioned by Torsten, there
is a
> >discussion between us in this respect. At that time I used Rmt*Kmax<3 to
> >just speed up to perform some tests due to many atoms in the structure we
> >were struggling with it. But, the "LOPW' - Plane waves exhausted" error
did
> >not allow me to conquer the problem. I said this story, since I would
> >emphasis on this point that I allowed myself to use such an small
Rmt*Kmax,
> >because I had used before even Rmt*Kmax=2 successfully. This would be
> >considered as a telltale to show that old versions of wien2k worked for
> >small cutoff's. It will be great if the authors fix this problem, so that
we
> >can use again small cutoff's for doing test to run one cycle or more  to
> >just see what is going on in the cases containing many atoms per their
cells
> >before going through them within well-converged SCF's.
> >        Your,
> >        S. Jalali.
> >
> >====
> >WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> >To (un)subscribe send mail to
> >majordomo@zeus.theochem.tuwien.ac.at
> >====
> >
> >
>
> --
> Dr. Torsten Andersen
> Department of Physics, Condensed Matter Theory Group, Uppsala University
> UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
> News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics
>
>
>
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====

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------------------------------

Date: Sat,  7 Dec 2002 09:24:52 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: hello

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
> submitted the following contribution:
> ====
> 
> 1) your suggested .machine file , 
> 
> 1:longhorn1
> 1:longhorn1
> 1:longhorn1
> 1:longhorn1
> 1:longhorn1
> 1:longhorn1
> 1:longhorn1
> 1:longhorn1
> granularity:1
> 
> is for k-point parallaization run if I wish to use only 8 processors 
> out of 16 processors availble on longhorn1 and leaving 8 others idle. 
> am I right?

Yes.

> for launching such runs, do I have to include in the batch job script
> 
> poe ./run(sp) -p .machines or some different command to run k-point 
> parallization.

Assume you are starting a serial run by e.g. 'run_lapw -i 30 -cc 0.00001'. For 
a parallel run, you use exactly the same command, with the -p added : 'run_lapw 
- -i 30 -cc 0.00001 -p'. (this is only an example, use the command you have been 
using before, just add -p)

> 2) I do wish to use "mpi" executable.  I do wish to use all the 16 
> machines for 8  k-points for example. Then according to your suggestion, I 
> should include in the job script(given below), the following:
> _______________________________________________________________
> setenv kortenaam `hostname`
> setenv langenaam $kortenaam'.cc.kuleuven.ac.be'(here .cc.kuleuven.ac.be 
> would be replaced by appropriate address)
> setenv lijn1 '14:'$langenaam
> setenv lijn2 '14:'$langenaam
> setenv lijn3 '14:'$langenaam
> setenv gran  'granularity:1'
> echo $lijn1 > .machines
> echo $lijn2 >> .machines
> echo $lijn3 >> .machines
> echo $gran  >> .machines
> cat .machines
> ____________________________________________________________________________
> 

No. This script was only for k-point parallelization on an SP whit a queing 
system that doesn't allow you to know before on which machine a job will run.

> what does "granularity" does? if I change
> the granularity value to some other values how does it affect the 
> the code?

It determines how the k-points are distributed. If you have 4 k-points and 2 
nodes, you can distribute them as 2+2 or 2x(1+1). When you have as many 
k-points as nodes, granularity:1 is fine (see UG for a more detailed 
explanation, or experiment yourself by using testpara_lapw)

> _____________________________________________________________
> 2) The job script for submitting the MPI parallel jobs on our SP4 looks 
> like:
> #!/usr/bin/csh
> #@ job_name = gamo-nonmag
> #@ output =$(job_name).o$(jobid)
> #@ error = $(job_name).o$(jobid)
> #@ initialdir = /gpfs/utexas/ph/phaa406/GaMo
> #@ job_type = parallel
> #@ environment = COPY_ALL; MP_SHARED_MEMORY=yes;
> #@ resources = ConsumableCpus(1) ConsumableMemory(1gb)
> #@ notify_user = sahu@matter3.ph.utexas.edu
> #@ node = 1
> #@ tasks_per_node = 16
> #@ class = normal
> #@ notification=error
> #@ wall_clock_limit = 24:00:00
> #@ notification=error
> #@ notification = complete
> #@ queue
> poe ./(WIEN2k  executable)
> ____________________________________
> 
> while compiling the code, I selected  the MPI command to be:
> 
>  poe _EXEC_ -shared_memory yes -procs _NP_ -hfile _HOSTS_
> 
> then in the above job script file, what should come after poe ./(WIEN2k
> executable)? for launching WIEN2k MPI jobs on SP$?  Do I need to put "-p"  
> with the "WIEN executable" for MPI parallel jobs?

I never used the mpi option so far, and never looked at it in detail, maybe 
somebody else can help you here.

Stefaan
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Date: Sat, 7 Dec 2002 21:25:46 +0800 (CST)
From: music@theory.issp.ac.cn
Subject: [WIEN]: DSTART ERROR

====
music@theory.issp.ac.cn
submitted the following contribution:
====

Dear wien users,
  I want to calculate the supercell of tio2 in 2a*2b*c, and substiute A Ti 
atom with other atom. And when doing dstart, error occurs  in 
dstart.error file :
 'ROTDEF' - no symmetry operation found.
 'ROTDEF' - for jatom, index 1 2
 'ROTDEF' - atomposition of jatom   0.0000000   0.0000000   0.0000000
 'ROTDEF' - atomposition of index   0.0000000   0.5000000   0.0000000
~
I think the struct file  is right but I dont know why dstart cant do.
Could anyone help me ? 
 THANKS IN ADVANCE!A 
- --
sincerely yours 

Ying.X


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Date: Sat, 07 Dec 2002 16:47:38 +0200
From: "B. Yanchitsky" <yan@im.imag.kiev.ua>
Subject: Re: [WIEN]: DSTART ERROR

====
"B. Yanchitsky" <yan@im.imag.kiev.ua>
submitted the following contribution:
====

Most probably your struct file is incorrect. This looks that positions
(0,0,0) and (0,0.5,0) are connected by a lattice translation. Use sgroup
to check the struct file, or check atomic positions using Intern. Tables
if space group is known and the unit cell has been chosen properly.

Regards,
Bogdan

> 
> Dear wien users,
>   I want to calculate the supercell of tio2 in 2a*2b*c, and substiute A Ti
> atom with other atom. And when doing dstart, error occurs  in
> dstart.error file :
>  'ROTDEF' - no symmetry operation found.
>  'ROTDEF' - for jatom, index 1 2
>  'ROTDEF' - atomposition of jatom   0.0000000   0.0000000   0.0000000
>  'ROTDEF' - atomposition of index   0.0000000   0.5000000   0.0000000
> ~
> I think the struct file  is right but I dont know why dstart cant do.
> Could anyone help me ?
>  THANKS IN ADVANCE!A
> --
> sincerely yours
> 
> Ying.X
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
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Date: Sun, 8 Dec 2002 01:29:03 +0800 (HKT)
From: Ma Chi Chiu <martin@yangtze.hku.hk>
Subject: Re: [WIEN]: Question

====
Ma Chi Chiu <martin@yangtze.hku.hk>
submitted the following contribution:
====

Dear Prof. Blaha,


Actually, I would like to consult the procedure for register for WIEN2K.

We have bought WIEN97 and now we would like to upgrade to WIEN2K. What 
is the procedure for register for WIEN2K? Thank you very much

Martin



On Mon, 4 Nov 2002, Peter Blaha wrote:

> 
> WIEN2k has no problems with your structure.
> 
> I suggest you register for WIEN2k.
> 
> 
> 
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
> 

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------------------------------

Date: Sun, 08 Dec 2002 01:52:26 +0800
From: =?gb2312?B?1dQg1r684Q==?= <zzj_fd@hotmail.com>
Subject: [none]

====
=?gb2312?B?1dQg1r684Q==?= <zzj_fd@hotmail.com>
submitted the following contribution:
====

Dear sir:
   I have a question, when I execute lapw2 in parallel model.
 I have 8 nodes together, and my .machines file like this:
granularity:3
1:node0
1:node1
1:node2
1:node3
1:node4
1:node5
1:node6
1:node7
I have 68 irreducibal k-points,so the case.klist file like this:
#####################################################
#                     TESTPARA                      #
#####################################################
Test: LAPW1 in parallel mode (using .machines)
Granularity set to 3
Extrafine unset
    klist:       68
    machines:    node0 node1 node2 node3 node4 node5 node6 node7
    procs:       8
    weigh(old):  1 1 1 1 1 1 1 1
    sumw:        8
    granularity: 3
    weigh(new):  2 2 2 2 2 2 2 2

Distribution of k-point (under ideal conditions)
will be:

1 : node0(2) 2k
2 : node1(2) 2k
3 : node2(2) 2k
4 : node3(2) 2k
5 : node4(2) 2k
6 : node5(2) 2k
7 : node6(2) 2k
8 : node7(2) 2k
9 : node0(2) 2k
10 : node1(2) 2k
11 : node2(2) 2k
12 : node3(2) 2k
13 : node4(2) 2k
14 : node5(2) 2k
15 : node6(2) 2k
16 : node7(2) 2k
17 : node0(2) 2k
18 : node1(2) 2k
19 : node2(2) 2k
20 : node3(2) 2k
21 : node4(2) 2k
22 : node5(2) 2k
23 : node6(2) 2k
24 : node7(2) 2k
25 : node0(2) 2k
26 : node1(2) 2k
27 : node2(2) 2k
28 : node3(2) 2k
29 : node4(2) 2k
30 : node5(2) 2k
31 : node6(2) 2k
32 : node7(2) 2k
33 : node0(2) 2k
34 : node1(2) 2k

Firstly, I type the command: run_lapw -p,
then, I run the program: testpara2,
I find the file like this:
#####################################################
#                     TESTPARA2                     #
#####################################################

Sun Dec  8 01:38:03 CST 2002

     lapw2para is running

27 of 34 (79%) junks distributed

machines(processors) in calling order are:
        node0   node0   node0   node0
        node0   node0   node0   node0
        node0   node0   node0   node0
        node0   node0   node0   node0
        node0   node0   node0   node0
        node0   node0   node0   node0
        node0   node0   node0   node0
wait a minute,I again run testpara2,finding like this:

#####################################################
#                     TESTPARA2                     #
#####################################################

Sun Dec  8 01:39:00 CST 2002

    lapw2para has finished

The question is I want to know whether the performance of "lapw2 -p"  is 
correct according to the above information. If it is wrong,what should I 
do? Thank you very much.
Best regards. 
                                                          J.Zhao 
                                                          12/8/2002



_________________________________________________________________
ÏíÓÃÊÀ½çÉÏ×î´óµÄµç×ÓÓÊ¼þÏµÍ³¡ª MSN Hotmail¡£ http://www.hotmail.com 

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------------------------------

Date: Sun, 8 Dec 2002 00:46:21 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: DSTART ERROR

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Dear mr. Ying,

it would really be easier to help you if had sent the struct-file.
When you create a supercell and add an impurity, you reduce the symmetry of
your system.  Thus, atoms that were (crystallographically) equivalent before
will now become inequivalent, and you may have to change your lattice type,
and enter more atom coordinates (eg. if you have to go from F to P-lattice).
So it's best to do the whole initialization from scratch.  Start with a
struct-file where all atoms of the same kind are equivalent, run nn, and
sgroup, and symmetry, and by the time you get there, wien will provide you
with a struct-file that looks totally different.  Check this file to see
whether it looks reasonable (eg. equivalent atoms should at least be of the
same kind and at equal distances to the impurity; also, they should be
connected by one of the 48 'legal' symmetry operations).  Usually it's
errors in the struct-file related to atom equivalency that produce the kind
of messages that you get.
If you keep having problems, please send the struct-file.

kind regards,
Kevin Jorissen.

PS These are the WIEN criteria for equivalency :
- - atoms must have the same atomic number  (nn)
- - atoms must have the same environment, i.e. for equivalent atoms, the same
number of atoms of the same atomic number have to be found at the same
distances of these equivalent atoms, and this up to a certain distance
determined by the input you give to nn (for super cells, it may be safer to
check with a higher value than the default '2')     (nn)
- - the coordinates of equivalent atoms in the global coordinate system must
transform into one another by application of one symmetry operations of your
structure (these are the ones out of the 48 known operations that can be
applied to every atom in the unit cell)    (symmetry)


- ----- Original Message -----
From: <music@theory.issp.ac.cn>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Saturday, December 07, 2002 2:25 PM
Subject: [WIEN]: DSTART ERROR


> ====
> music@theory.issp.ac.cn
> submitted the following contribution:
> ====
>
> Dear wien users,
>   I want to calculate the supercell of tio2 in 2a*2b*c, and substiute A Ti
> atom with other atom. And when doing dstart, error occurs  in
> dstart.error file :
>  'ROTDEF' - no symmetry operation found.
>  'ROTDEF' - for jatom, index 1 2
>  'ROTDEF' - atomposition of jatom   0.0000000   0.0000000   0.0000000
>  'ROTDEF' - atomposition of index   0.0000000   0.5000000   0.0000000
> ~
> I think the struct file  is right but I dont know why dstart cant do.
> Could anyone help me ?
>  THANKS IN ADVANCE!A
> --
> sincerely yours
>
> Ying.X
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

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------------------------------

Date: Sun, 8 Dec 2002 14:29:42 +0800 (CST)
From: music@theory.issp.ac.cn
Subject: Re: [WIEN]: DSTART ERROR

====
music@theory.issp.ac.cn
submitted the following contribution:
====


Dear Mr Jorissen,
 Thank you very much for your instructive advise!
 I did not notice  that  a new struct was out after sgroup. NN produce a 
new struct refer to the distance of atoms, and sgroup brings out new 
inequivalent atoms.  So now it's ok.
 
> ====
> "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
> submitted the following contribution:
> ====
> 
> Dear mr. Ying,
> 
> it would really be easier to help you if had sent the struct-file.
> When you create a supercell and add an impurity, you reduce the symmetry of
> your system.  Thus, atoms that were (crystallographically) equivalent before
> will now become inequivalent, and you may have to change your lattice type,
> and enter more atom coordinates (eg. if you have to go from F to P-lattice).
> So it's best to do the whole initialization from scratch.  Start with a
> struct-file where all atoms of the same kind are equivalent, run nn, and
> sgroup, and symmetry, and by the time you get there, wien will provide you
> with a struct-file that looks totally different.  Check this file to see
> whether it looks reasonable (eg. equivalent atoms should at least be of the
> same kind and at equal distances to the impurity; also, they should be
> connected by one of the 48 'legal' symmetry operations).  Usually it's
> errors in the struct-file related to atom equivalency that produce the kind
> of messages that you get.
> If you keep having problems, please send the struct-file.
> 
> kind regards,
> Kevin Jorissen.
> 
> PS These are the WIEN criteria for equivalency :
> - atoms must have the same atomic number  (nn)
> - atoms must have the same environment, i.e. for equivalent atoms, the same
> number of atoms of the same atomic number have to be found at the same
> distances of these equivalent atoms, and this up to a certain distance
> determined by the input you give to nn (for super cells, it may be safer to
> check with a higher value than the default '2')     (nn)
> - the coordinates of equivalent atoms in the global coordinate system must
> transform into one another by application of one symmetry operations of your
> structure (these are the ones out of the 48 known operations that can be
> applied to every atom in the unit cell)    (symmetry)
> 
> 
> ----- Original Message -----
> From: <music@theory.issp.ac.cn>
> To: <wien@zeus.theochem.tuwien.ac.at>
> Sent: Saturday, December 07, 2002 2:25 PM
> Subject: [WIEN]: DSTART ERROR
> 
> 
> > ====
> > music@theory.issp.ac.cn
> > submitted the following contribution:
> > ====
> >
> > Dear wien users,
> >   I want to calculate the supercell of tio2 in 2a*2b*c, and substiute A Ti
> > atom with other atom. And when doing dstart, error occurs  in
> > dstart.error file :
> >  'ROTDEF' - no symmetry operation found.
> >  'ROTDEF' - for jatom, index 1 2
> >  'ROTDEF' - atomposition of jatom   0.0000000   0.0000000   0.0000000
> >  'ROTDEF' - atomposition of index   0.0000000   0.5000000   0.0000000
> > ~
> > I think the struct file  is right but I dont know why dstart cant do.
> > Could anyone help me ?
> >  THANKS IN ADVANCE!A
> > --
> > sincerely yours
> >
> > Ying.X
> >
> >
> > ====
> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> > To (un)subscribe send mail to
> > majordomo@zeus.theochem.tuwien.ac.at
> > ====
> >
> 
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 

- -- 





sincerely yours 

Ying.X


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------------------------------

Date: Sun,  8 Dec 2002 10:09:45 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: [WIEN]: Re: 

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

>    I have a question, when I execute lapw2 in parallel model.
>  I have 8 nodes together, and my .machines file like this:
> granularity:3
> 1:node0
> 1:node1
> 1:node2
> 1:node3
> 1:node4
> 1:node5
> 1:node6
> 1:node7
> I have 68 irreducibal k-points,so the case.klist file like this:

If you don't have to share these 8 nodes with other users during the execution 
of your job, you can use also

9:node0
9:node1
9:node2
9:node3
9:node4
9:node5
9:node6
5:node7
granularity:1

This will give 8x1=8 jobs to each node (node 7 is occupied somewhat less).

> Firstly, I type the command: run_lapw -p,

Do 'run_lapw -p -i 1'. This will execute 1 iteration in parallel. Then check 
*.dayfile, to see how much time each of the sub-jobs took, and whether they 
used the processors efficiently.

Stefaan
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Date: Sun, 8 Dec 2002 23:3:42 +0800
From: "Wenhui Xie" <xiewh@sun20.iphy.ac.cn>
Subject: [WIEN]: Symmetry operation of Group No. 119 and No. 139

====
"Wenhui Xie" <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear Sir£¬


The symmetry operation of Group No.119 and No. 139 given by 
Wien2k are 8 and 16, respectively. However, someone claim that
the operation is 16 and 32, respectively, like this website: 
http://autodep.ebi.ac.uk/sgtable.html  

I am puzzle about it. I would appreciate if someone 
could give a hint about what and why.

Your Sincerely 				
Wenhui Xie
xiewh@sun20.iphy.ac.cn
2002-12-08



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Date: Sun, 8 Dec 2002 23:9:41 +0800
From: "Wenhui Xie" <xiewh@sun20.iphy.ac.cn>
Subject: Re: Re: [WIEN]: 'LOPW' - Plane waves exhausted

====
"Wenhui Xie" <xiewh@sun20.iphy.ac.cn>
submitted the following contribution:
====

Dear Peter Blaha,


We check the struct file and find that the beta angle is wrong.
Now, everything is OK.
Thank the instructive advise of Prof. Plaha and other people in here.

		
Yours Sincerely 
Wenhui Xie
xiewh@sun20.iphy.ac.cn
2002-12-08




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------------------------------

Date: Mon, 9 Dec 2002 12:55:53 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: [WIEN]: Re: your mail

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>    I have a question, when I execute lapw2 in parallel model.
>     lapw2para has finished
>
> The question is I want to know whether the performance of "lapw2 -p"  is
> correct according to the above information. If it is wrong,what should I
> do? Thank you very much.
> Best regards.

It seems to be ok.   Just make a run with and without -p and compare.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Mon, 9 Dec 2002 13:45:00 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: hello

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

Parallel calculations:

You really need to read the UG (at least section about parallelization!!!!)

In all circumstances you use only     run_lapw -p    for parallel execution.

When you have configured WIEN2k properly during siteconfig, the rest is done
by the .machines file.

> 1:longhorn1
> 1:longhorn1
> granularity:1

This does k-point parallelization (with two processors)

If you want to use the fine-grain mpi parallelization (NOTE: this works only
reasonably well when you have a large case (matrix sizes of 5000 and more), It
is absolutely nonsense to use this for smaller matrices and may even run
slower than on 1 processor).

To select mpi parallelization your machines file should contain lines like:

lapw0:longhorn1:1 longhorn1:1
1:longhorn1:1 longhorn1:1
1:longhorn1:1 longhorn1:1

This runs lapw0 on 2 processors   and 2-k-point parallel lapw1_mpi jobs, where
each lapw1_mpi runs on 2 processors in parallel.


Please note: You were saying you are using an IBM with the "loadleveler".
At least on our IBM-SP3 a loadleveler script with a line:
> #@ tasks_per_node = 16
will always use 16 processors for an mpi-executable, and completely ignore
any values for _NP_ in the actual  "poe" command line (which is called
internally in lapw1para).
  poe _EXEC_ -shared_memory yes -procs _NP_ -hfile _HOSTS_

Thus on our IBM we cannot use the loadleveler and use k-point and
mpi-parallelization at once. (We run it in background and this works nicely,
but you may have to negotioate with your computing center to operate in this
mode).

PS: If anybody knows how to override the "tasks_per_node" value in the
actual job, please let me know).

If you have to use the loadleveler, I strongly recommend to use the k-parallel
version only (and start a second project on the other 8 processors), unless
you have a really big case with just 1-2 k-points.

If you run a queuing system, you may have to create the .machines file
"on the fly" with the script decribed by Stefaan. (Although on a cluster
of shared memory machines it is not really necessary).

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Mon, 9 Dec 2002 14:18:06 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Symmetry operation of Group No. 119 and No. 139

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> The symmetry operation of Group No.119 and No. 139 given by
> Wien2k are 8 and 16, respectively. However, someone claim that
> the operation is 16 and 32, respectively, like this website:
> http://autodep.ebi.ac.uk/sgtable.html
>
> I am puzzle about it. I would appreciate if someone
> could give a hint about what and why.

Because they do not use the primitive cell ! There is a difference
of 2 (or 4) for I or F centered cells.


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 9 Dec 2002 20:48:59 +0400 (SAMT)
From: Lyudmila Dobysheva <lyu@otf.fti.udmurtia.su>
Subject: [WIEN]: BROYD mixing parameter

====
Lyudmila Dobysheva <lyu@otf.fti.udmurtia.su>
submitted the following contribution:
====

Dear WIEN-users,

How the BROYD mixing scheme works? 
I have made an scf-cycle, it gave such charge distances:
:DIS  :  CHARGE DISTANCE       0.0005600
:DIS  :  CHARGE DISTANCE       0.0004390
:DIS  :  CHARGE DISTANCE       0.0004751
:DIS  :  CHARGE DISTANCE       0.0004486
:DIS  :  CHARGE DISTANCE       0.0002515
:DIS  :  CHARGE DISTANCE       0.0002113
:DIS  :  CHARGE DISTANCE       0.0001803
:DIS  :  CHARGE DISTANCE       0.0001699
:DIS  :  CHARGE DISTANCE       0.0001136
:DIS  :  CHARGE DISTANCE       0.0000699

When I looked at mixing parameter used, I saw that it's rather low 
as compared to the parameter given in case.inm (0.40) and equal in all
cycles: 
       BROYD MIXING SCHEME WITH 0.182
       BROYD MIXING SCHEME WITH 0.182
       BROYD MIXING SCHEME WITH 0.182

Another scf-cycle gave such a convergency:
:DIS  :  CHARGE DISTANCE       0.0489381
:DIS  :  CHARGE DISTANCE       0.0888596
:DIS  :  CHARGE DISTANCE       0.0172118
:DIS  :  CHARGE DISTANCE       0.0090646
:DIS  :  CHARGE DISTANCE       0.0182707
:DIS  :  CHARGE DISTANCE       0.0022858
:DIS  :  CHARGE DISTANCE       0.0018873
:DIS  :  CHARGE DISTANCE       0.0015986
:DIS  :  CHARGE DISTANCE       0.0011595
:DIS  :  CHARGE DISTANCE       0.0008809
:DIS  :  CHARGE DISTANCE       0.0006736
:DIS  :  CHARGE DISTANCE       0.0005523
:DIS  :  CHARGE DISTANCE       0.0004370
:DIS  :  CHARGE DISTANCE       0.0003596
:DIS  :  CHARGE DISTANCE       0.0003257

And again, the mixing parameter from the scf file was in all cycles:
       BROYD MIXING SCHEME WITH 0.182

Why it is not larger, especially in the first case? And why it has the 
same magnitude in both cases? I thought it should depend on the :DIS value.

Best regards,
  Lyudmila Dobysheva 
- ------------------------------------------------------------------------
Phys.-Techn. Institute of            |   Tel.(home):   7 (3412) 442118
Ural Branch of Russian Ac. of Sci.   |   Tel.(office): 7 (3412) 218988
426001 Izhevsk, ul.Kirova 132        |   Fax:          7 (3412) 250614
RUSSIA                               |   E-mail: lyu@otf.fti.udmurtia.su
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------------------------------

Date: Mon, 9 Dec 2002 15:03:50 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: MPI run

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear Peter (and other w2k users)

 thanx.

1) k-point parallelization works fine with the load leveler.

2) with the help of the loadleveler on SP4, the job is always put in the 
background using the batch job script :

#!/usr/bin/csh
#@ job_name = test
#@ output =$(job_name).o$(jobid)
#@ error = $(job_name).o$(jobid)
#@ initialdir = /gpfs/utexas/ph/phaa406/gaas
#@ job_type = parallel
#@ environment = COPY_ALL; MP_SHARED_MEMORY=yes;
#@ resources = ConsumableCpus(1) ConsumableMemory(1gb)
#@ notify_user = sahu@matter3.ph.utexas.edu
#@ node = 1
#@ tasks_per_node = 16
#@ class = normal
#@ notification=error
#@ wall_clock_limit = 24:00:00
#@ notification=error
#@ notification = complete
#@ queue
poe executable

________________________________________________

in this case poe will use number of processors(here 16) for the run and
the loadleveler assigns the next available node depending upon the info in
the jobscript(tested for MPI parallel codes like VASP, CPMD etc where
other parallelization strategies might have been used)

now, if I have a system say 60 atoms with 1-2 k-pt, then as per the 
userguide and your suggestion, mpi parallel jobs are preferable.
but 

in this case can 

poe ./wien_executables(run(sp)_lapw -p)

in the above jobscript work without

- -shared_memory yes -procs _NP_ -hfile _HOSTS_ explicitly specified?
(by assuming that "poe" picks up lapw0_mpi, lapw1_mpi etc instead of
lapw1_para, lapw2_para )

your example of the .machines file for the mpi parallel run has
2 processors and 2 k-point. However, if I wish to use all the 16 
processors available in the given node(here longhorn1) with 2 k-points
then the machine file can be:

lapw0: longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 
longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 
longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
(where I wish to use all 16 processors for lapw0)
1:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 
longhorn1:1 longhorn1:1 
1:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 
longhorn1:1 longhorn1:1 

where I have distributed 2 kpoints over 8 processors each(in total 16 
processors).

is this correct?
do we need "granularity" here too?

2) If I wish to calculate the orbital magnetic moment on a particular atom
in the unit cell by adding SOC nonselfconsistently, hen will -so switch in
run(sp)_lapw -so calulates it with the proper case.inso file generated by
initso_lapw(where I have the results of previous scf cycle without -so
i.e. run(sp)_lapw -p). I dont have to use -p switch for adding SOC by 
non-scf. only for adding SOC selfconsistently, I need to use 
from the begining run(sp)_lapw -so -p.
am I right?

3) If I understand correctly, for volume or internal parameter
optimization, the userguide says, we need to "renormalize" the charge
density using 'MIXER'(with -renorm).  what does the switch "-renorm"
exactly do and why it is necessary to renormalize the charge density for a
new calculation with different lattice parameters(as done in vol.
optimization procedure).If I have a situation where I am using a shell
script(optimize.job) for vol optimization after every scf cycle for each
lattice paramter I do save_lapw -d "directory" then anyway *broydX files
are deleted then what does the -renorm parameter do for the next scf
cycle for the next lattice parameter?

regards
sahu

 





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------------------------------

Date: Mon, 9 Dec 2002 15:58:34 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: hi

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear w2kusers

       Is there an article, where the "orbital polarization" method is 
described in detail including the self-consistent calculation of OP 
parameters. Userguide gives Eriksson et.al ref( J.Phys:Cond. Matter vol 1 
pg 4005(1989) and Brooks Physica B130 pg 6 1985) where these authors
used OP method to describe magnetic properties of Uranium ternary alloys 
the method itself is not described in detail.In Eriksson et.al's paper
there is reference to OP method but in the reference list it is 
"unpublished"

regards
sahu

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------------------------------

Date: Tue, 10 Dec 2002 08:03:31 +0800
From: gyguo <gyguo@phys.ntu.edu.tw>
Subject: Re: [WIEN]: hi

====
gyguo <gyguo@phys.ntu.edu.tw>
submitted the following contribution:
====


Hi,

It might be helpful to take a look at a paper of mine
and references therein [PRB 55, 11619 (1997)].

Cheers, Guang-Yu

"Dr. B.R.Sahu" ¼g¹D¡G

> ====
> "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
> submitted the following contribution:
> ====
>
> Dear w2kusers
>
>        Is there an article, where the "orbital polarization" method is
> described in detail including the self-consistent calculation of OP
> parameters. Userguide gives Eriksson et.al ref( J.Phys:Cond. Matter vol 1
> pg 4005(1989) and Brooks Physica B130 pg 6 1985) where these authors
> used OP method to describe magnetic properties of Uranium ternary alloys
> the method itself is not described in detail.In Eriksson et.al's paper
> there is reference to OP method but in the reference list it is
> "unpublished"
>
> regards
> sahu
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====

- --
Dr. G.Y. Guo
Professor
Department of Physics
National Taiwan University
1 Roosevelt Road, Sec. 4
Taipei 106, Taiwan, R.O.C.
Tel. ++886-2-33665180
Fax. ++886-2-23639984
E-mail: gyguo@phys.ntu.edu.tw


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------------------------------

Date: Mon, 9 Dec 2002 23:02:35 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [none]

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---559023410-1804928587-1039496555=:16285
Content-Type: TEXT/PLAIN; charset=US-ASCII

Dear All:

I don't know my case.struct failed to be run with "init_lapw", could you
please take a look of the attached file and give me some ideas about how
to fix my case.struct file?

Thanks!

Pacholite (Hawthorne)
P   LATTICE,NONEQUIV. ATOMS:13                       15 C2/c
MODE OF CALC=RELA
 18.778216 19.679616 29.630917 90.000000142.442600 90.000000
Atom= -1: X=0.17281000 Y=0.12590000 Z=0.71803000
          MULT= 1          ISPLIT= 8
Al         NPT=  781  R0=0.00010000 RMT=    1.8000   Z: 13.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -2: X=0.18750000 Y=0.17360000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Ca         NPT=  781  R0=0.00005000 RMT=    1.8000   Z: 20.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -3: X=0.18750000 Y=0.56940000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Ca         NPT=  781  R0=0.00005000 RMT=    1.8000   Z: 20.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -4: X=0.31460000 Y=0.12740000 Z=0.62520000
          MULT= 1          ISPLIT= 8
Na         NPT=  781  R0=0.00010000 RMT=    1.8000   Z: 11.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -5: X=0.02710000 Y=0.99910000 Z=0.19380000
          MULT= 1          ISPLIT= 8
F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -6: X=0.12995000 Y=0.99070000 Z=0.36130000
          MULT= 1          ISPLIT= 8
F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -7: X=0.15725000 Y=0.11380000 Z=0.57470000
          MULT= 1          ISPLIT= 8
F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -8: X=0.18960000 Y=0.14300000 Z=0.86440000
          MULT= 1          ISPLIT= 8
F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -9: X=0.09910000 Y=0.25050000 Z=0.30210000
          MULT= 1          ISPLIT= 8
F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom=-10: X=0.99540000 Y=0.25300000 Z=0.12490000
          MULT= 1          ISPLIT= 8
F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom=-11: X=0.19650000 Y=0.37530000 Z=0.42790000
          MULT= 1          ISPLIT= 8
O          NPT=  781  R0=0.00010000 RMT=    1.5000   Z:  8.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom=-12: X=0.17550000 Y=0.37100000 Z=0.35100000
          MULT= 1          ISPLIT= 8
H          NPT=  781  R0=0.00010000 RMT=    1.1000   Z:  1.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom=-13: X=0.23050000 Y=0.36000000 Z=0.48800000
          MULT= 1          ISPLIT= 8
H          NPT=  781  R0=0.00010000 RMT=    1.1000   Z:  1.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
   0 SYMMETRY OPERATIONS:


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- ---559023410-1804928587-1039496555=:16285--
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------------------------------

Date: Tue, 10 Dec 2002 09:53:41 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: MPI run

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> 2) with the help of the loadleveler on SP4, the job is always put in the
> background using the batch job script :
>
> #!/usr/bin/csh
> #@ job_name = test
> #@ output =$(job_name).o$(jobid)
> #@ error = $(job_name).o$(jobid)
> #@ initialdir = /gpfs/utexas/ph/phaa406/gaas
> #@ job_type = parallel
> #@ environment = COPY_ALL; MP_SHARED_MEMORY=yes;
> #@ resources = ConsumableCpus(1) ConsumableMemory(1gb)
> #@ notify_user = sahu@matter3.ph.utexas.edu
> #@ node = 1
> #@ tasks_per_node = 16
> #@ class = normal
> #@ notification=error
> #@ wall_clock_limit = 24:00:00
> #@ notification=error
> #@ notification = complete
> #@ queue
> poe executable
>
> ________________________________________________
>
> in this case poe will use number of processors(here 16) for the run and
> the loadleveler assigns the next available node depending upon the info in
> the jobscript(tested for MPI parallel codes like VASP, CPMD etc where
> other parallelization strategies might have been used)
>
> now, if I have a system say 60 atoms with 1-2 k-pt, then as per the
> userguide and your suggestion, mpi parallel jobs are preferable.
> but
>
> in this case can
>
> poe ./wien_executables(run(sp)_lapw -p)
>
> in the above jobscript work without
>
> -shared_memory yes -procs _NP_ -hfile _HOSTS_ explicitly specified?
> (by assuming that "poe" picks up lapw0_mpi, lapw1_mpi etc instead of
> lapw1_para, lapw2_para )

No, just use    run_lapw -p

This script calls internally lapw0/1/2para   and those scripts will then
issue the  necessary poe commands.




>
> your example of the .machines file for the mpi parallel run has
> 2 processors and 2 k-point. However, if I wish to use all the 16
> processors available in the given node(here longhorn1) with 2 k-points
> then the machine file can be:
>
> lapw0: longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
> longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
> longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
> (where I wish to use all 16 processors for lapw0)
> 1:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
> longhorn1:1 longhorn1:1
> 1:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
> longhorn1:1 longhorn1:1
>
> where I have distributed 2 kpoints over 8 processors each(in total 16
> processors).

Yes, this would be the suggested .machines file. The idea is to span two jobs,
one for the first k-point using 8 mpi-parallel processors and another for the
second k-point (again with 8 mpi-processors.
However, remember my previous email:
On our SP3 the loadleveler ignores the NP command and takes always 16
processors (when tasks_per_nodes=16) and then crashes with the second
k-point (since he has already used 16 processors for the first k-point.)

I know only 2 ways out (and if somebody could provide a better solution?!):
a) Do not use the loadleveler (if you are allowed to do so)
b) Remove the last line from .machines. This will use all 16 processors
for the first k-point and AFTER this has finished, it will do the second
k-point again with 16 processors. (This is less efficient, but maybe the
only way you can do it)

> do we need "granularity" here too?

You don't need "granularity" here (When you have 30 k-points, a larger
granularity will submit not 15 and 15 k-points, but first eg. 5 and 5 and
once one of these jobs has finished, the next junk is submitted. This allows
for some loadballancing on clusters, but on shared memory machines always use
granularity=1 (and for 2k points it has no effect at all).

>
> 2) If I wish to calculate the orbital magnetic moment on a particular atom
> in the unit cell by adding SOC nonselfconsistently, hen will -so switch in
> run(sp)_lapw -so calulates it with the proper case.inso file generated by
> initso_lapw(where I have the results of previous scf cycle without -so
> i.e. run(sp)_lapw -p). I dont have to use -p switch for adding SOC by
> non-scf. only for adding SOC selfconsistently, I need to use
> from the begining run(sp)_lapw -so -p.
> am I right?

You can do it with or without "-p" (k-point parallel only for lapwso)

> 3) If I understand correctly, for volume or internal parameter
> optimization, the userguide says, we need to "renormalize" the charge
> density using 'MIXER'(with -renorm).  what does the switch "-renorm"
> exactly do and why it is necessary to renormalize the charge density for a
> new calculation with different lattice parameters(as done in vol.
> optimization procedure).If I have a situation where I am using a shell
> script(optimize.job) for vol optimization after every scf cycle for each
> lattice paramter I do save_lapw -d "directory" then anyway *broydX files
> are deleted then what does the -renorm parameter do for the next scf
> cycle for the next lattice parameter?

If you change the lattice parameters, the planewave charge density in the
interstital does not give the correct number of electrons when you integrate
it. Renormalization just fixes this problem.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

====
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------------------------------

Date: Tue, 10 Dec 2002 09:58:45 +0100
From: Georg Madsen <georg@chem.au.dk>
Subject: [WIEN]: Re: 

====
Georg Madsen <georg@chem.au.dk>
submitted the following contribution:
====

You have typed in your C centered lattice as primitive. This could be a good
idea because you want sgroup to convert it to B2/b. But then you have to type in
all your atoms. This means also the atoms from the (1/2,1/2,0) translation.

Quoting Bing Zhou <umbingz@cc.UManitoba.CA>:

> Dear All:
> 
> I don't know my case.struct failed to be run with "init_lapw", could you
> please take a look of the attached file and give me some ideas about how
> to fix my case.struct file?
> 
> Thanks!
> 
> Pacholite (Hawthorne)
> P   LATTICE,NONEQUIV. ATOMS:13                       15 C2/c
> MODE OF CALC=RELA
>  18.778216 19.679616 29.630917 90.000000142.442600 90.000000
> Atom= -1: X=0.17281000 Y=0.12590000 Z=0.71803000
>           MULT= 1          ISPLIT= 8
> Al         NPT=  781  R0=0.00010000 RMT=    1.8000   Z: 13.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -2: X=0.18750000 Y=0.17360000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Ca         NPT=  781  R0=0.00005000 RMT=    1.8000   Z: 20.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -3: X=0.18750000 Y=0.56940000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Ca         NPT=  781  R0=0.00005000 RMT=    1.8000   Z: 20.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -4: X=0.31460000 Y=0.12740000 Z=0.62520000
>           MULT= 1          ISPLIT= 8
> Na         NPT=  781  R0=0.00010000 RMT=    1.8000   Z: 11.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -5: X=0.02710000 Y=0.99910000 Z=0.19380000
>           MULT= 1          ISPLIT= 8
> F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -6: X=0.12995000 Y=0.99070000 Z=0.36130000
>           MULT= 1          ISPLIT= 8
> F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -7: X=0.15725000 Y=0.11380000 Z=0.57470000
>           MULT= 1          ISPLIT= 8
> F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -8: X=0.18960000 Y=0.14300000 Z=0.86440000
>           MULT= 1          ISPLIT= 8
> F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -9: X=0.09910000 Y=0.25050000 Z=0.30210000
>           MULT= 1          ISPLIT= 8
> F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom=-10: X=0.99540000 Y=0.25300000 Z=0.12490000
>           MULT= 1          ISPLIT= 8
> F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom=-11: X=0.19650000 Y=0.37530000 Z=0.42790000
>           MULT= 1          ISPLIT= 8
> O          NPT=  781  R0=0.00010000 RMT=    1.5000   Z:  8.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom=-12: X=0.17550000 Y=0.37100000 Z=0.35100000
>           MULT= 1          ISPLIT= 8
> H          NPT=  781  R0=0.00010000 RMT=    1.1000   Z:  1.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom=-13: X=0.23050000 Y=0.36000000 Z=0.48800000
>           MULT= 1          ISPLIT= 8
> H          NPT=  781  R0=0.00010000 RMT=    1.1000   Z:  1.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
>    0 SYMMETRY OPERATIONS:
> 
> 


- ----------------------------
Georg Madsen
Dept. of Inorganic Chemistry
University of Aarhus
DK-8000 Århus C
Denmark
- ----------------------------
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------------------------------

Date: Tue, 10 Dec 2002 11:05:48 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: BROYD mixing parameter

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> How the BROYD mixing scheme works?
> I have made an scf-cycle, it gave such charge distances:
> :DIS  :  CHARGE DISTANCE       0.0005600
>
> When I looked at mixing parameter used, I saw that it's rather low
> as compared to the parameter given in case.inm (0.40) and equal in all
> cycles:
>        BROYD MIXING SCHEME WITH 0.182
> Why it is not larger, especially in the first case? And why it has the
> same magnitude in both cases? I thought it should depend on the :DIS value.

Yes, it depends on :DIS, but your :DIS values are too small to have any effect.
Besides that, the mixing depends on the number of (heavier) atoms in your
cell and is reduced automatically the more atoms you have.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

====
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------------------------------

Date: Tue, 10 Dec 2002 08:39:45 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: case.struct file

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---559023410-1804928587-1039496555=:16285
Content-Type: TEXT/PLAIN; CHARSET=US-ASCII
Content-ID: <Pine.GSO.4.40.0212100838102.16546@antares.cc.umanitoba.ca>

Dear All:

I don't know my case.struct failed to be run with "init_lapw", could you
please take a look of the attached file and give me some ideas about how
to fix my case.struct file?

Thanks!

Pacholite (Hawthorne)
P   LATTICE,NONEQUIV. ATOMS:13                       15 C2/c
MODE OF CALC=RELA
 18.778216 19.679616 29.630917 90.000000142.442600 90.000000
Atom= -1: X=0.17281000 Y=0.12590000 Z=0.71803000
          MULT= 1          ISPLIT= 8
Al         NPT=  781  R0=0.00010000 RMT=    1.8000   Z: 13.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -2: X=0.18750000 Y=0.17360000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Ca         NPT=  781  R0=0.00005000 RMT=    1.8000   Z: 20.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -3: X=0.18750000 Y=0.56940000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Ca         NPT=  781  R0=0.00005000 RMT=    1.8000   Z: 20.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -4: X=0.31460000 Y=0.12740000 Z=0.62520000
          MULT= 1          ISPLIT= 8
Na         NPT=  781  R0=0.00010000 RMT=    1.8000   Z: 11.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -5: X=0.02710000 Y=0.99910000 Z=0.19380000
          MULT= 1          ISPLIT= 8
F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -6: X=0.12995000 Y=0.99070000 Z=0.36130000
          MULT= 1          ISPLIT= 8
F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -7: X=0.15725000 Y=0.11380000 Z=0.57470000
          MULT= 1          ISPLIT= 8
F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -8: X=0.18960000 Y=0.14300000 Z=0.86440000
          MULT= 1          ISPLIT= 8
F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom= -9: X=0.09910000 Y=0.25050000 Z=0.30210000
          MULT= 1          ISPLIT= 8
F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom=-10: X=0.99540000 Y=0.25300000 Z=0.12490000
          MULT= 1          ISPLIT= 8
F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom=-11: X=0.19650000 Y=0.37530000 Z=0.42790000
          MULT= 1          ISPLIT= 8
O          NPT=  781  R0=0.00010000 RMT=    1.5000   Z:  8.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom=-12: X=0.17550000 Y=0.37100000 Z=0.35100000
          MULT= 1          ISPLIT= 8
H          NPT=  781  R0=0.00010000 RMT=    1.1000   Z:  1.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
Atom=-13: X=0.23050000 Y=0.36000000 Z=0.48800000
          MULT= 1          ISPLIT= 8
H          NPT=  781  R0=0.00010000 RMT=    1.1000   Z:  1.0
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
   0 SYMMETRY OPERATIONS:


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Date: Tue, 10 Dec 2002 16:27:22 +0100 (CET)
From: =?iso-8859-1?q?sham=20fred?= <sham_f2002@yahoo.fr>
Subject: [WIEN]: question about electron density input?

====
=?iso-8859-1?q?sham=20fred?= <sham_f2002@yahoo.fr>
submitted the following contribution:
====

- --0-1159391477-1039534042=:538
Content-Type: text/plain; charset=iso-8859-1
Content-Transfer-Encoding: 8bit


Dear All:

Actually, I would like to consult the procedure for 

Edit TiC.in5 choose the offered template input file. To select the (100) plane for plotting specify the following input: 

- -1 -1 0 4     # origin of plot (x,y,z,denominator)-1  3 0 4     # x-end of plot 3 -1 0 4     # y-end of plot3 2 3         # x,y,z number of shells100 100       # number of x and y points, ratio should be                # similar to x,y length RHO               ANG VAL NODEBUGORTHO

for why this choose ,and what is solution for other direction ? and  is possible with xcrysden for get input of electron density properties?

any suggestions or helps are welcome!

thanks

 



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<P>Dear All:<BR><BR>Actually, I would like to consult the procedure for </P>
<P>Edit <TT><B>TiC.in5</B></TT> choose the offered template input file. To select the (100) plane for plotting specify the following input: </P>
<BLOCKQUOTE><FONT size=-1></FONT></BLOCKQUOTE><PRE>-1 -1 0 4     # origin of plot (x,y,z,denominator)
- -1  3 0 4     # x-end of plot
 3 -1 0 4     # y-end of plot
3 2 3         # x,y,z number of shells
100 100       # number of x and y points, ratio should be  
              # similar to x,y length 
RHO               
ANG VAL NODEBUG
ORTHO
</PRE>
<P>for why this choose ,and what is solution for other direction ? and&nbsp; is possible with xcrysden for get input of electron density properties?</P>
<P>any suggestions or helps are welcome!<BR><BR>thanks</P>
<P>&nbsp;</P><p><br><hr size=1>Soyez solidaire soutenez l’action du Téléthon avec Yahoo! France.<br>
<a href=http://www1.telethon.fr/030-Espace-Relais-Dons/webtirelire1.asp?hebergeur_id=1309>Cliquez ici pour faire un don !</a>
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Date: Tue, 10 Dec 2002 17:01:59 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: question about electron density input?

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====


> Actually, I would like to consult the procedure for
>
> Edit TiC.in5 choose the offered template input file. To select the (100)
> plane for plotting specify the following input:
>
> -1 -1 0 4     # origin of plot (x,y,z,denominator)-1  3 0 4     # x-end of
> plot 3 -1 0 4     # y-end of plot3 2 3         # x,y,z number of shells100
> 100       # number of x and y points, ratio should be                #
> similar to x,y length RHO               ANG VAL NODEBUGORTHO
>
> for why this choose ,and what is solution for other direction ? and  is
> possible with xcrysden for get input of electron density properties?


I think you better read the section 8.6 on lapw5 in the usersguide first.

Stefaan
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Date: Tue, 10 Dec 2002 19:05:13 +0200
From: "B. Yanchitsky" <yan@im.imag.kiev.ua>
Subject: Re: [WIEN]: case.struct file

====
"B. Yanchitsky" <yan@im.imag.kiev.ua>
submitted the following contribution:
====

Dear Bing,

This seems to be a bug in symmetry. Because your structure is triclinic
(not monoclinic!) and symmetry is unable to determine point groups
for atoms. Note also, that there exists an overlap of MT's.

ps
Georg gave you some trick how to convert monoclinic C-base centered
with unique axis b to monoclinic B-base centered with unique axis c.
But it seems that the problem is not related to this
point, because the structure is triclinic.
 
Regards,
Bogdan Yanchitsky

Bing Zhou wrote:
> 
> Dear All:
> 
> I don't know my case.struct failed to be run with "init_lapw", could you
> please take a look of the attached file and give me some ideas about how
> to fix my case.struct file?
> 
> Thanks!
> 
> Pacholite (Hawthorne)
> P   LATTICE,NONEQUIV. ATOMS:13                       15 C2/c
> MODE OF CALC=RELA
>  18.778216 19.679616 29.630917 90.000000142.442600 90.000000
> Atom= -1: X=0.17281000 Y=0.12590000 Z=0.71803000
>           MULT= 1          ISPLIT= 8
> Al         NPT=  781  R0=0.00010000 RMT=    1.8000   Z: 13.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -2: X=0.18750000 Y=0.17360000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Ca         NPT=  781  R0=0.00005000 RMT=    1.8000   Z: 20.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -3: X=0.18750000 Y=0.56940000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Ca         NPT=  781  R0=0.00005000 RMT=    1.8000   Z: 20.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -4: X=0.31460000 Y=0.12740000 Z=0.62520000
>           MULT= 1          ISPLIT= 8
> Na         NPT=  781  R0=0.00010000 RMT=    1.8000   Z: 11.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -5: X=0.02710000 Y=0.99910000 Z=0.19380000
>           MULT= 1          ISPLIT= 8
> F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -6: X=0.12995000 Y=0.99070000 Z=0.36130000
>           MULT= 1          ISPLIT= 8
> F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -7: X=0.15725000 Y=0.11380000 Z=0.57470000
>           MULT= 1          ISPLIT= 8
> F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -8: X=0.18960000 Y=0.14300000 Z=0.86440000
>           MULT= 1          ISPLIT= 8
> F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom= -9: X=0.09910000 Y=0.25050000 Z=0.30210000
>           MULT= 1          ISPLIT= 8
> F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom=-10: X=0.99540000 Y=0.25300000 Z=0.12490000
>           MULT= 1          ISPLIT= 8
> F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom=-11: X=0.19650000 Y=0.37530000 Z=0.42790000
>           MULT= 1          ISPLIT= 8
> O          NPT=  781  R0=0.00010000 RMT=    1.5000   Z:  8.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom=-12: X=0.17550000 Y=0.37100000 Z=0.35100000
>           MULT= 1          ISPLIT= 8
> H          NPT=  781  R0=0.00010000 RMT=    1.1000   Z:  1.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> Atom=-13: X=0.23050000 Y=0.36000000 Z=0.48800000
>           MULT= 1          ISPLIT= 8
> H          NPT=  781  R0=0.00010000 RMT=    1.1000   Z:  1.0
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
>    0 SYMMETRY OPERATIONS:
> 
>   --------------------------------------------------------------------------------------------------------------------------------
>                             Name: pachnolite-new.struct
>    pachnolite-new.struct    Type: Plain Text (TEXT/PLAIN)
>                         Encoding: BASE64
> 
>                           Name: pachnolite-new.inst
>    pachnolite-new.inst    Type: Plain Text (TEXT/PLAIN)
>                       Encoding: BASE64
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Date: Tue, 10 Dec 2002 12:48:28 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: MPI

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear peter
      
        thanx

1) If I understand your suggestion correctly, to use the lapw0/1/2_mpi 
scripts for large systems(having large number of atoms but small 
number of k-points say 1 or 2 ), I need to 
use run(sp)_lapw -p in the batch job script.

but this is the same command used for k-point parallelization batch job
run. how does the run(sp)_lapw -p command knows which script to call
whether lapw0/1/2_mpi OR lapw0/1/2_para?

In short, what could be the command for running mpi scripts (and not
para scripts) in the batch job script using load leveler?

2) Here on SP4, the batch queue jobs are always scheduled using
loadleveler, so one can not avoid using loadleveler for batch queue jobs.
Your second suggestion seems to be promising(although less efficient)  
until some other w2k users sugget a way out of this problem. With your
second suggestion it means, If I have 2 k-point then I put only 
1 k-point in the .machines file and once for this k-point(with 
tasks_per_node = number of processors) has finished the job, it will
automatically go for the 2nd k-point with the same number of processors.
am I right?

3) about volume/internal parameter optimization:

If I have set of case.struct files for volume optimization generated by
the script opitmize and wish to run these struct files using optimize.job
shell-script without having any previous scf results to start with, then
for the first struct file, and first iterataion would be calling "MIXER"
and from second iteration onwards, the scf cycle starts and it would be
same procedure for all struct files, ie the first iteration for each
struct file would be calling the "MIXER" and renormalizing the
interstitial charge density (if it is available from the previous run).

am I right?

Also Is the order of switches important in the following:

ie

run(sp)_lapw -p -ec 0.0000001 -renorm

OR

run(sp)_lapw -ec 0.00000001 -renorm -p

do the same job?

regards
sahu

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Date: Tue, 10 Dec 2002 14:54:19 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: case.struct file

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear Bogdan:

Good to hear from you agian and thank for your kind help!

Originally I used the structure data from Hawthorne (F. Hawthorne et al,
1983, Canadian Mineralogist, p.561-566) for pachnolite, however, WIEN2k and
WIEN97 could not recognize the space group F2/d (a=12.117, b=10.414,
c=15.690, beta=90.37).

Both the papers of Hawthorne (F. Hawthorn et al., 1983) and Adhikesavalu
(D. Adhikesavalu et al., Canadian Journal of Chemistry, Vol.63, 1985,
p.3322-3327) argued pachnolite was in monoclinic symmetry. Adhikesavalu et
al. (1985, p.3325) expressed that Hawthorne et al (1983) adopted for its
description the F2/d setting of C2/c by the following relationship:
	a(F)=2a(C)+c(C)
	b(F)=b(C)
	C(F)=c(C)

Therefore, I transformed the F2/d space group to C2/c for pachnolite. I
calculated the new a, b, c and beta for C2/c space group from the geometry
as 9.939, 10.414, 15.68 and 142.4426. I also transformed all the atom
coordinates in the F2/d unit cell to C2/c using the following matrix:

	2    0   1
	0    1   0
	0    0   1

That is how I got the pachnolite.struct file. I list the original F2/d
unit cell data from Hawthorne (F. Hawthorne, 1983) as following:

Space Group: F2/d
a=12.117, b=10.414, c=15.68, beta=90.37

Atoms	x	y	z

Al	0.34562	0.1259	0.37421
Ca1	3/8	0.1736	1/8
Ca2	3/8	0.5694	1/8
Na	0.6292	0.1274	-0.0040
F1	0.0542	-0.0009	0.1396
F2	0.2599	-0.0093	0.1014
F3	0.3145	0.1138	0.2602
F4	0.3792	0.1430	0.4852
F5	0.1982	0.2505	0.1039
F6	-0.0092	0.2530	0.134
O	0.3930	0.3753	0.0349
H1	0.351	0.371	-0.000
H2	0.461	0.360	0.027

As the result, I got the structure data for new C2/c group as the
following:

Space Group: C2/c
a=9.939, b=10.414, c=16.680, beta=142.4426

Atoms 	x	y	z

Al	0.17281	0.1259	0.91803
Ca1	0.1875	0.1376	0.5
Ca2	0.1875	0.5694	0.5
Na	0.3146	0.1274	0.6252
F1	0.0271	-0.0009	0.1938
F2	0.12995	-0.0093	0.3613
F3	0.15725	0.1138	0.5747
F4	0.1896	0.1430	0.8644
F5	0.0991	0.2505	0.3021
F6	-0.0046	0.2530	0.1249
O	0.1965	0.3753	0.4279
H1	0.1755	0.371	0.351
H2	0.2305	0.360	0.488


So, could you please help me out and let me know how to work out the
proper pachnolite.struct file from the original F2/d data?

Looking forward to hearing from you, thanks!

Best wishes!


On Tue, 10 Dec 2002, B. Yanchitsky wrote:

> ====
> "B. Yanchitsky" <yan@im.imag.kiev.ua>
> submitted the following contribution:
> ====
>
> Dear Bing,
>
> This seems to be a bug in symmetry. Because your structure is triclinic
> (not monoclinic!) and symmetry is unable to determine point groups
> for atoms. Note also, that there exists an overlap of MT's.
>
> ps
> Georg gave you some trick how to convert monoclinic C-base centered
> with unique axis b to monoclinic B-base centered with unique axis c.
> But it seems that the problem is not related to this
> point, because the structure is triclinic.
>
> Regards,
> Bogdan Yanchitsky
>
> Bing Zhou wrote:
> >
> > Dear All:
> >
> > I don't know my case.struct failed to be run with "init_lapw", could you
> > please take a look of the attached file and give me some ideas about how
> > to fix my case.struct file?
> >
> > Thanks!
> >
> > Pacholite (Hawthorne)
> > P   LATTICE,NONEQUIV. ATOMS:13                       15 C2/c
> > MODE OF CALC=RELA
> >  18.778216 19.679616 29.630917 90.000000142.442600 90.000000
> > Atom= -1: X=0.17281000 Y=0.12590000 Z=0.71803000
> >           MULT= 1          ISPLIT= 8
> > Al         NPT=  781  R0=0.00010000 RMT=    1.8000   Z: 13.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom= -2: X=0.18750000 Y=0.17360000 Z=0.50000000
> >           MULT= 1          ISPLIT= 8
> > Ca         NPT=  781  R0=0.00005000 RMT=    1.8000   Z: 20.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom= -3: X=0.18750000 Y=0.56940000 Z=0.50000000
> >           MULT= 1          ISPLIT= 8
> > Ca         NPT=  781  R0=0.00005000 RMT=    1.8000   Z: 20.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom= -4: X=0.31460000 Y=0.12740000 Z=0.62520000
> >           MULT= 1          ISPLIT= 8
> > Na         NPT=  781  R0=0.00010000 RMT=    1.8000   Z: 11.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom= -5: X=0.02710000 Y=0.99910000 Z=0.19380000
> >           MULT= 1          ISPLIT= 8
> > F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom= -6: X=0.12995000 Y=0.99070000 Z=0.36130000
> >           MULT= 1          ISPLIT= 8
> > F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom= -7: X=0.15725000 Y=0.11380000 Z=0.57470000
> >           MULT= 1          ISPLIT= 8
> > F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom= -8: X=0.18960000 Y=0.14300000 Z=0.86440000
> >           MULT= 1          ISPLIT= 8
> > F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom= -9: X=0.09910000 Y=0.25050000 Z=0.30210000
> >           MULT= 1          ISPLIT= 8
> > F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom=-10: X=0.99540000 Y=0.25300000 Z=0.12490000
> >           MULT= 1          ISPLIT= 8
> > F          NPT=  781  R0=0.00010000 RMT=    1.3000   Z:  9.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom=-11: X=0.19650000 Y=0.37530000 Z=0.42790000
> >           MULT= 1          ISPLIT= 8
> > O          NPT=  781  R0=0.00010000 RMT=    1.5000   Z:  8.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom=-12: X=0.17550000 Y=0.37100000 Z=0.35100000
> >           MULT= 1          ISPLIT= 8
> > H          NPT=  781  R0=0.00010000 RMT=    1.1000   Z:  1.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > Atom=-13: X=0.23050000 Y=0.36000000 Z=0.48800000
> >           MULT= 1          ISPLIT= 8
> > H          NPT=  781  R0=0.00010000 RMT=    1.1000   Z:  1.0
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> >    0 SYMMETRY OPERATIONS:
> >
> >   --------------------------------------------------------------------------------------------------------------------------------
> >                             Name: pachnolite-new.struct
> >    pachnolite-new.struct    Type: Plain Text (TEXT/PLAIN)
> >                         Encoding: BASE64
> >
> >                           Name: pachnolite-new.inst
> >    pachnolite-new.inst    Type: Plain Text (TEXT/PLAIN)
> >                       Encoding: BASE64
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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Date: Tue, 10 Dec 2002 20:58:40 -0800 (PST)
From: hamid salehi <salehihamid@yahoo.com>
Subject: Re: [WIEN]: question about electron density input?

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear sir
You have  select the (100) plane  for plotting of
Flowing.
0 0 0 1
0 1 0 1
0 0 1 1
   best wishes

- --- sham fred <sham_f2002@yahoo.fr> wrote:
> 
> Dear All:
> 
> Actually, I would like to consult the procedure for 
> 
> Edit TiC.in5 choose the offered template input file.
> To select the (100) plane for plotting specify the
> following input: 
> 
> -1 -1 0 4     # origin of plot (x,y,z,denominator)-1
>  3 0 4     # x-end of plot 3 -1 0 4     # y-end of
> plot3 2 3         # x,y,z number of shells100 100   
>    # number of x and y points, ratio should be      
>          # similar to x,y length RHO              
> ANG VAL NODEBUGORTHO
> 
> for why this choose ,and what is solution for other
> direction ? and  is possible with xcrysden for get
> input of electron density properties?
> 
> any suggestions or helps are welcome!
> 
> thanks
> 
>  
> 
> 
> 
> ---------------------------------
> Soyez solidaire soutenez l’action du Téléthon avec
> Yahoo! France.
> Cliquez ici pour faire un don !


=====
Hamdollah Salehi
Dept of Physics
Ferdowsi University
Mashhad IRAN
Post boxs 1436
Post code 91775
faxs

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Date: Wed, 11 Dec 2002 10:28:22 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: MPI

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> 1) If I understand your suggestion correctly, to use the lapw0/1/2_mpi
> scripts for large systems(having large number of atoms but small
> number of k-points say 1 or 2 ), I need to
> use run(sp)_lapw -p in the batch job script.
>
> but this is the same command used for k-point parallelization batch job
> run. how does the run(sp)_lapw -p command knows which script to call
> whether lapw0/1/2_mpi OR lapw0/1/2_para?

from the .machines file!!!  If it has lines
1:host
1:host      it does k-point parallelization, but with

1:host:1 host:1       it does mpi-parallelization and calls the poe command
                      automatically.


> 2) Here on SP4, the batch queue jobs are always scheduled using
> loadleveler, so one can not avoid using loadleveler for batch queue jobs.
> Your second suggestion seems to be promising(although less efficient)
> until some other w2k users sugget a way out of this problem. With your
> second suggestion it means, If I have 2 k-point then I put only
> 1 k-point in the .machines file and once for this k-point(with
> tasks_per_node = number of processors) has finished the job, it will
> automatically go for the 2nd k-point with the same number of processors.
> am I right?

Yes you are right.

>
> 3) about volume/internal parameter optimization:
>
> If I have set of case.struct files for volume optimization generated by
> the script opitmize and wish to run these struct files using optimize.job
> shell-script without having any previous scf results to start with, then
> for the first struct file, and first iterataion would be calling "MIXER"
> and from second iteration onwards, the scf cycle starts and it would be
> same procedure for all struct files, ie the first iteration for each
> struct file would be calling the "MIXER" and renormalizing the
> interstitial charge density (if it is available from the previous run).
> am I right?

One cannot give a unique answer to this. Sometimes it is better to start
with an existing clmsum file (and renormalize it, although this does not help
too much in some cases), while sometimes it is better to start with a clmsum
file generated by   x dstart (-c) for the actual struct file.


> Also Is the order of switches important in the following:
>
> ie
>
> run(sp)_lapw -p -ec 0.0000001 -renorm
>
> OR
>
> run(sp)_lapw -ec 0.00000001 -renorm -p
>
> do the same job?

Yes it does the same job,  BUT:

- -ec 0.00000001 !!!!   We calculate E-total only up to 6 figures after the
comma!!! Even   -ec 0.000001 is usually not possible (for large cells) and
not at all necessary.

E.g.: A volume optimization changes E-tot by several 10 or even 100 mRy, so
convergence up to 0.0001 or maybe 0.00001 is completely sufficient.
Usually you can rely on the WIEN2k default parameters unless you are
getting more experienced.

PS: Your question about volume optimization brings me to another point:
It is by far more efficient to run each volume using "k-parallel" instead of
"mpi-parallel" and do all volumes simultaneously!!! (Each one in a different
subdirectory!! but for convenience having the same name: i.e.:
vol1/case
vol2/case
vol3/case    and so on.

Only a "force"-minimization (internal coordinates) needs to be done
sequentially.



                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Wed, 11 Dec 2002 10:44:18 +0000
From: Paula <pauhar@chem.gla.ac.uk>
Subject: [WIEN]: segmentation fault

====
Paula <pauhar@chem.gla.ac.uk>
submitted the following contribution:
====

- --=====================_6349963==_
Content-Type: text/plain; charset="us-ascii"; format=flowed

Dear wienusers,

I get a segmentation fault during lapw2 whenever l increase Emax value to 
4.0. If l leave it at the default value of 1.5 then lapw2 runs okay. 
However when l try to run ELNES, specifically the x tetra part, then l get 
another segmentation fault. This occurs even when l leave the original 
default values. I have previously run the same .struct file on wien97 and 
found good results. Does anyone know why a segmentation fault is occurring now?

Thanks for your advice,
Paula



Paula Harkins
   Room A3-31C - Materials Chemistry Group
   Department of Chemistry
   University of Glasgow
   Glasgow
   G12 8QQ
   Scotland, UK
   0141 330 4941 
- --=====================_6349963==_
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Date: Wed, 11 Dec 2002 07:43:00 -0800 (PST)
From: xin gao <stargmoon@yahoo.com>
Subject: [WIEN]: about k-point parallel

====
xin gao <stargmoon@yahoo.com>
submitted the following contribution:
====

- --0-1045039590-1039621380=:11706
Content-Type: text/plain; charset=us-ascii


Dear wien2k user,

The following total energy of the same system was calculated with the same parameters (RKmax, Gmax, et.al) by using k-point parallelization version and serial version of WIEN2k respectively.

for k-point parallelization version: 

:ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486870
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129313
:ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486873
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129309
:ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486869
:ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486871
:ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486871
:ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486873
:ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486873
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129311
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129312
:ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486874
:ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486874
:ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486882
:ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486874


for serial version:

:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129306
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129299
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129307
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129296
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129295
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129297
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129295
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129314
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129313
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129316
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129306
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129316
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129316
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129313
:ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129316


I had checked all the energies outputed in case.scf (there seems no double count term), i.e., the sum of eigenvalues, energies of core states, both of them are nearly equal, but I don't know why the total energies are not equal. 

Had you ever met this problem, and how did you deal with it? I am looking forward for your kindly replying. Thank you very much.

Best regards,



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- --0-1045039590-1039621380=:11706
Content-Type: text/html; charset=us-ascii

<P>Dear wien2k user,</P>
<P>The following total energy of the same system was calculated with the same parameters (RKmax, Gmax, et.al) by using k-point parallelization version and serial&nbsp;version of WIEN2k respectively.</P>
<P>for k-point parallelization version:&nbsp;</P>
<P>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -3848.486870<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129313<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -3848.486873<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129309<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -3848.486869<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -3848.486871<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -3848.486871<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -3848.486873<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -3848.486873<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nb!
sp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129311<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129312<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -3848.486874<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -3848.486874<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -3848.486882<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -3848.486874<BR></P>
<P>for serial version:</P>
<P>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129306<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129299<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129307<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129296<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129295<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129297<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129295<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129314<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129313<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nb!
sp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129316<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129306<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129316<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129316<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129313<BR>:ENE&nbsp; : ********** TOTAL ENERGY IN Ry =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; -6828.129316<BR></P>
<P>I had checked all the energies outputed in case.scf (there seems no double count term), i.e., the sum of eigenvalues, energies of core states, both of them are nearly equal, but I don't know why the total energies are not equal. </P>
<P>Had you ever met this problem, and how did you deal with it? I am looking forward for your kindly replying. Thank you very much.</P>
<P>Best regards,</P><p><br><hr size=1>Do you Yahoo!?<br>
<a href="http://rd.yahoo.com/mail/mailsig/*http://mailplus.yahoo.com">Yahoo! Mail Plus</a> - Powerful. Affordable. <a href="http://rd.yahoo.com/mail/mailsig/*http://mailplus.yahoo.com">Sign up now</a>
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Date: Wed, 11 Dec 2002 15:40:12 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: SELECT error

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear all:

When I run "run_lapw" for my mineral of pachnolite (in monoclinic
symmetry), the calcualtion was crashed in the first lapw1 with message
"SELECT error", and the lapw1.error contains the following information:

'SELECT' - no energy limits found for L= 0
'SELECT' - E-bottom   -5.97500   E-top -200.00000

How can I fix it?

Looking forward to hearing from you, thank you in advance!

Best wishes!



Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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Date: Wed, 11 Dec 2002 15:17:03 -0800 (PST)
From: yanming Ma <ymma66@yahoo.com>
Subject: [WIEN]: QTL-B = 1220.43

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-2095760556-1039648623=:24630
Content-Type: text/plain; charset=us-ascii


Dear WIEN2k  users,

When I do the calculation for CsBiTe including SO coupling, I try to follow the following procedure

init_lapw--runsp_lapw--initso_lapw--runsp_lapw -so

But When I do runsp_lapw, the warning of OTL-B=1220.43 occurred.
There are two possibility for this warning as in userguide:

(1)atoms with very different atomic sphere radii. 
In my case, the atomic sphere radii are 2.8, 2.8 ,and 3.2 for Te, Bi, and Cs respectively.
I choose the energy cut off to seperate the core and valance electrons as -7 Ryd. 
I have already checked the charge leakage for Te, Bi, and Cs. 
They are 0.0002, 0.0006, 0.0000002, respectively.

(2)one doesn't use a proper set of local orbitals.
In my case, the case.in1 file is as follows
WFFIL        (WFPRI, SUPWF)
7.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT )

0.30    5  0   (Bi)
2   -1.54     0.010 CONT 1
2    0.30      0.000 CONT 1
0   -0.73      0.010 CONT 1
0    0.30      0.000 CONT 1
1    0.30      0.000 CONT 1

0.30    5  0   (Cs)
2    0.30      0.000 CONT 1
2   -5.08      0.005 STOP 1
0   -1.66      0.010 CONT 1
0    0.30      0.000 CONT 1
1    0.30      0.000 CONT 1

0.30    5  0   (Te)
2   -2.70      0.010 CONT 1
2    0.30      0.000 CONT 1
0   -0.84      0.010 CONT 1
0    0.30      0.000 CONT 1
1    0.30      0.000 CONT 1
K-VECTORS FROM UNIT:4   -7.0       1.5      emin/emax window

I know I can use "run_lapw -in1new 1" to choose the proper local orbitals. 
But, in my such big case (one iteration will cost 4 days using 9 cpus), 
it is difficult to do many tries. So can you kindly help me to analyz what is the possible reason for the large QTL-B values? Any comments are welcom.

Thanks in advance.


Yanming Ma Ph.D
Steacie Institute for Molecular Sciences,
National Research Councils of Canada,
Ottawa, Ontario
K1A 0R6
Canada


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<P><FONT face="Times New Roman" size=3>Dear WIEN2k&nbsp; users,</FONT></P>
<P><FONT face="Times New Roman" size=3>When I do the calculation for CsBiTe including SO coupling, I try to follow the following procedure</FONT></P>
<P><FONT face="Times New Roman" size=3>init_lapw--runsp_lapw--initso_lapw--runsp_lapw -so</FONT></P>
<P><FONT face="Times New Roman" size=3>But When I do runsp_lapw, the warning of OTL-B=1220.43 occurred.<BR>There are two possibility for this warning as in userguide:</FONT></P>
<P><FONT face="Times New Roman" size=3>(1)atoms with very different atomic sphere radii. <BR>In my case, the atomic sphere radii are 2.8, 2.8 ,and 3.2 for Te, Bi, and Cs respectively.<BR>I choose the energy cut off to seperate the core and valance electrons as -7 Ryd. <BR>I have already checked the charge leakage for Te, Bi, and Cs. <BR>They are 0.0002, 0.0006, 0.0000002, respectively.</FONT></P>
<P><FONT face="Times New Roman" size=3>(2)one doesn't use a proper set of local orbitals.<BR>In my case, the case.in1 file is as follows<BR>WFFIL&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; (WFPRI, SUPWF)<BR>7.00&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 10&nbsp;&nbsp;&nbsp; 4 (R-MT*K-MAX; MAX L IN WF, V-NMT )</FONT></P>
<P><FONT face="Times New Roman" size=3>0.30&nbsp;&nbsp;&nbsp; 5&nbsp; 0&nbsp;&nbsp; (Bi)<BR>2&nbsp;&nbsp; -1.54&nbsp;&nbsp;&nbsp;&nbsp; 0.010 CONT 1<BR>2&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT 1<BR>0&nbsp;&nbsp; -0.73&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010 CONT 1<BR>0&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT 1<BR>1&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT 1</FONT></P>
<P><FONT face="Times New Roman" size=3>0.30&nbsp;&nbsp;&nbsp; 5&nbsp; 0&nbsp;&nbsp; (Cs)<BR>2&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT 1<BR>2&nbsp;&nbsp; -5.08&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.005 STOP 1<BR>0&nbsp;&nbsp; -1.66&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010 CONT 1<BR>0&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT 1<BR>1&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT 1</FONT></P>
<P><FONT face="Times New Roman" size=3>0.30&nbsp;&nbsp;&nbsp; 5&nbsp; 0&nbsp;&nbsp; (Te)<BR>2&nbsp;&nbsp; -2.70&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010 CONT 1<BR>2&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT 1<BR>0&nbsp;&nbsp; -0.84&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010 CONT 1<BR>0&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT 1<BR>1&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000 CONT 1<BR>K-VECTORS FROM UNIT:4&nbsp;&nbsp; -7.0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 1.5&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; emin/emax window</FONT></P>
<P><FONT face="Times New Roman" size=3>I know I can use "run_lapw -in1new 1" to choose the proper local orbitals. <BR>But, in my such big case (one iteration will cost 4 days using 9 cpus), <BR>it is difficult to do many tries. So can you kindly help me to analyz what is the possible reason for the large QTL-B values? Any comments are welcom.</FONT></P>
<P><FONT face="Times New Roman" size=3>Thanks in advance.</FONT></P><BR><BR>Yanming Ma Ph.D<br>Steacie Institute for Molecular Sciences,<br>National Research Councils of Canada,<br>Ottawa, Ontario<br>K1A 0R6<br>Canada<p><br><hr size=1>Do you Yahoo!?<br>
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------------------------------

Date: Wed, 11 Dec 2002 18:36:03 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: MPI

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear Peter
       
        thanx

1) I try your suggestion for MPI-parallel run and get back to you  by 
tomorrow.

2)about spin-orbit run: 

what could be the run command to get 
 an orbital moment on an atom with SOC when it is included

a) non-selfconsistently i.e after a spinpolarized scf run without SOC, and
assuming that proper case.inso file is created using initso_lapw script.

OR

b) selfconsistenly with spin polarization, ie from scratch(assuming that
proper case.inso file is already  created using initso_lapw script).


Your reply in the mailing list on 4th Nov 2002 says
lapwdm calculates orbital moments but it is not called during runsp 
- -so.one needs the updated version to use the switch -dm for this.
I downloaded the entire w2k code on Nov 19(which is much after 4th 
Nov).does it include -dm switch then?

if yes,

is runsp -so -dm  for including the SOC selfconsistently? 

using this for nonselfconsistent inclusion will do by default 20 
iteration? so one need to force it to have only one iteration ie 
runsp -so -dm -i 1 . am I right? 


3) I am not clear about doing volume optimization simultaneously using 
k-point parallelization. can you be little more descriptive?

for a given volume, scf cycle is performed and then it is repeated for
all volumes in optimized.job script ie volume optimization is done
sequentially with scf cycle in k-point parallelization for each volume.

how to launch simultaneous volume optimization using the same optimization 
file? is not we need as many machines files as there are subdirectories
ie vol1 vol2 etc.


regards
sahu

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Date: Thu, 12 Dec 2002 08:09:09 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: SELECT error

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Bing,

this is a FAQ. Read the website documentation, please. And scan the 
mailing list digest if the FAQ does not help you. This you can do by 
downloading the digest and use an editor (or grep) to search it. There 
are tons of mail with this subject.

Best regards,
Torsten.

Bing Zhou wrote:

>====
>Bing Zhou <umbingz@cc.UManitoba.CA>
>submitted the following contribution:
>====
>
>Dear all:
>
>When I run "run_lapw" for my mineral of pachnolite (in monoclinic
>symmetry), the calcualtion was crashed in the first lapw1 with message
>"SELECT error", and the lapw1.error contains the following information:
>
>'SELECT' - no energy limits found for L= 0
>'SELECT' - E-bottom   -5.97500   E-top -200.00000
>
>How can I fix it?
>
>Looking forward to hearing from you, thank you in advance!
>
>Best wishes!
>
>
>
>Bing Zhou
>Dept. of Geological Sc.
>The Univ. of Manitoba
>Canada R3T 2N2
>Tel: (204)474-8395
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Thu, 12 Dec 2002 09:17:03 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: about k-point parallel

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> The following total energy of the same system was calculated with the same parameters (RKmax, Gmax, et.al) by using k-point parallelization version and serial version of WIEN2k respectively.
>
> for k-point parallelization version:
>
> :ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486870   <---
> :ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129313   <---
> :ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486873   <---
> :ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129309
> :ENE  : ********** TOTAL ENERGY IN Ry =        -3848.486869

>
> for serial version:
>
> :ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129306
> :ENE  : ********** TOTAL ENERGY IN Ry =        -6828.129299

If you see jumps like this the problem is always the same:
You must    save_lapw  save_name    your calculations before you start/continue
with the next one.
If in the scf file an iteration number xx appears twice, the calculated E-tot
will be wrong.

PS: In the last version of WIEN2k, a warning should be printed if this occurs.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 12 Dec 2002 10:31:12 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: QTL-B = 1220.43

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====


> But When I do runsp_lapw, the warning of OTL-B=1220.43 occurred.

When you see this warning, have a look into case.output2.  For instance
search for 1220   and find out for which atom/state these QTL-Bs occur.

> In my case, the atomic sphere radii are 2.8, 2.8 ,and 3.2 for Te, Bi, and Cs respectively.

I would not have chosen 3.2 for Cs, but kept it also at 2.8

> 0.30    5  0   (Cs)
> 2    0.30      0.000 CONT 1
> 2   -5.08      0.005 STOP 1
> 0   -1.66      0.010 CONT 1
> 0    0.30      0.000 CONT 1
> 1    0.30      0.000 CONT 1

Is it really the default input ? I would have guessed that Cs has p-semicore
states and thus has also an lo for l=1  (But I hav'n't checked it myself)?

So my guess is that Cs p states produce this QTL-B (but I could be wrong)

Also: Where is your EF ? Only than one can estimate if the energy parameters
are ok or need to be changed about 0.2 Ry below EF

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Thu, 12 Dec 2002 10:42:11 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: segmentation fault

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I get a segmentation fault during lapw2 whenever l increase Emax value to
> 4.0. If l leave it at the default value of 1.5 then lapw2 runs okay.

Enough memory and swap space configured ?
Check the *help* files for '****'. Maybe for those high energies some ghost
states appear?

> However when l try to run ELNES, specifically the x tetra part, then l get
> another segmentation fault. This occurs even when l leave the original
> default values. I have previously run the same .struct file on wien97 and
> found good results. Does anyone know why a segmentation fault is occurring now?

DO you use the latest version of lapw2 ? We had some problems for elnes
calculations, but they have been fixed some weeks ago (see www.wien2k.at).

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu, 12 Dec 2002 16:54:00 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: SELECT error

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> When I run "run_lapw" for my mineral of pachnolite (in monoclinic
> symmetry), the calcualtion was crashed in the first lapw1 with message
> "SELECT error", and the lapw1.error contains the following information:
>
> 'SELECT' - no energy limits found for L= 0
> 'SELECT' - E-bottom   -5.97500   E-top -200.00000
This error in FIRST cycle is not described in FAQ so that reducing mixing
factor from 0.4 is not a cure. Also one cannot get a chance to check
linearization, as it needs at least one preformed cycle. In addition no
heavy elements are there in the struct file of  Pachnolite with the formula
NaCaAlF6·(H2O), in order to one can be convinced about changing the default
E-paparemetr.
> How can I fix it?
I think your struct file is wrong. The output of sgroup program is empty
employing your structure file, which is an indication that they are not
consistent. The space group of Pachnolite is  F2/d. This space group can be
converted to  B2/b or C2/c with the # of 15. Only B2/b is included in the
struct generator of WIEN2K. Thus, one possible way is to convert F2/d to
B2/b and then use the facility of WIEN2K, which the conversion would be done
carefully.

Another (more suitable) way was described by Madsen, which appears that one
needs more description for more realization.

I see you claim that, your struct file works well employing wien97 code! I
don't access to wien97, but I am interested to know how it is possible.

        Your,

        S. Jalali.







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Date: Thu, 12 Dec 2002 22:50:31 +0800
From: =?gb2312?B?1dQg1r684Q==?= <zzj_fd@hotmail.com>
Subject: [none]

====
=?gb2312?B?1dQg1r684Q==?= <zzj_fd@hotmail.com>
submitted the following contribution:
====







Dear sir:
   I have a question when I do "runsp_lapw -p".I want to calculate the 
magnetic moment of W(tungsten) bulk. So I select the "spin polarize"  model 
during  "init_lapw".
  I use 3000 k-points(there are 100 irreducible k-points), and have 5 
nodes. My 
.machines like this :

20:node13
20:node14
20:node15
20:node16
20:node17
granularity:1

After "runsp_lapw -p", I do "testpara", and get the following information:
              

####################################################
#                     TESTPARA                      #
#####################################################
 
Test: LAPW1 in parallel mode (using .machines)
Granularity set to 1
Extrafine unset
 
    klist:       100
    machines:    node13 node14 node15 node16 node17
    procs:       5
    weigh(old):  20 20 20 20 20
    sumw:        100
    granularity: 1
    weigh(new):  20 20 20 20 20
 
Distribution of k-point (under ideal conditions)
will be:
 
1 : node13(20) 20k
2 : node14(20) 20k
3 : node15(20) 20k
4 : node16(20) 20k
5 : node17(20) 20k                                      
 
furthermore run "testpara1" and get the information like this:

#####################################################
#                     TESTPARA1                     #
#####################################################
 
Thu Dec 12 21:43:42 CST 2002
 
     lapw1para is running
 
100 of 100 (100%) k-points distributed
 
  node13: running
  node14: running
  node15: running
  node16: running
  node17: running

But unfortunately when I rlogin to every node(node13,node14,etc),
I find these nodes' CPUs are doing noting really! because of the command 
"top" giving the information like this: 

CPU states:  0.0% user,  0.1% system,  0.0% nice, 99.8% idle

And I get the *.dayfile like this :

Calculating wbulk in /home/d0/jzhao/wien/work/wbulk
on node0
 
    start       (Thu Dec 12 21:24:36 CST 2002) with lapw0 (2/20 to go)
>   lapw0 -p    (21:24:36) starting parallel lapw0 at Thu Dec 12 21:24:36 
CST 2002
- --------
running lapw0 in single mode
3.660u 0.090s 0:04.05 92.5%     0+0k 0+0io 2321pf+0w
>   lapw1  -up -p       (21:24:40) starting parallel lapw1 at Thu Dec 12 
21:24:41 CST 2002
- ->  starting parallel LAPW1 jobs at Thu Dec 12 21:24:41 CST 2002
running LAPW1 in parallel mode (using .machines)
5 number_of_parallel_jobs
     node13(20)      node14(20)      node15(20)      node16(20)      
node17(20)    Summary of lapw1para:
   node13        k=20    user=0  wallclock=20
   node14        k=20    user=0  wallclock=20
   node15        k=20    user=0  wallclock=20
   node16        k=20    user=0  wallclock=20
   node17        k=20    user=0  wallclock=20
0.220u 0.320s 0:08.12 6.6%      0+0k 0+0io 22048pf+0w
>   lapw1  -dn -p       (21:24:49) starting parallel lapw1 at Thu Dec 12 
21:24:49 CST 2002
- ->  starting parallel LAPW1 jobs at Thu Dec 12 21:24:49 CST 2002
running LAPW1 in parallel mode (using .machines.help)
5 number_of_parallel_jobs
[1] 9780
[2] 9796
[3] 9811
[1]    Done                          ( $remote $machine[$p]  ...
[4] 9826
[2]    Done                          ( $remote $machine[$p]  ...
[5] 9841
[3]    Done                          ( $remote $machine[$p]  ...
[4]  - Done                          ( $remote $machine[$p]  ...
[5]  + Done                          ( $remote $machine[$p]  ...    

After 10 hours, I find the *.dayfile has nothing different compared with 
the  file 10 hours before!  
So, I want to know :
1.why it takes me so long time to do "runsp_lapw -p", but get nothing 
result.
2.during the calculation of "runsp_lapw -p", WIEN2K gave me a information:

GETARG: argument index (2) out of range  
 whether it is harmful?
 Thank you very much in advance.

Best regards.
                                             J.Zhao
                                             12/12/2002
                                


























































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Date: Thu, 12 Dec 2002 16:36:56 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: [WIEN]: Re:

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====


> 1.why it takes me so long time to do "runsp_lapw -p", but get nothing
> result.

Perform this command : 'rlogin node13'. Does it ask you for a password? If 
yes, then put in your home directory af file with the name .rhosts that 
contains the lines

node13
node14
node15
node16
node17

Now you should be able to rlogin to all of these nodes without a password. I 
guess that your calculation just is waiting for a password that will never 
come.

Stefaan

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wien-digest       Thursday, December 19 2002       Volume 2002 : Number 048




----------------------------------------------------------------------

Date: Thu, 12 Dec 2002 07:59:56 -0800 (PST)
From: yanming Ma <ymma66@yahoo.com>
Subject: Re: [WIEN]: QTL-B = 1220.43

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-850918627-1039708796=:71525
Content-Type: text/plain; charset=us-ascii


Dear Peter,
Thanks very much for your reply.
>> 0.30 5 0 (Cs)
>> 2 0.30 0.000 CONT 1
>>2 -5.08 0.005 STOP 1
>> 0 -1.66 0.010 CONT 1
>> 0 0.30 0.000 CONT 1
>> 1 0.30 0.000 CONT 1

>Is it really the default input ? I would have guessed that Cs has p-semicore
>states and thus has also an lo for l=1 (But I hav'n't checked it myself)?


Yes, it is the default input. No semicore is chosen in Cs by default.


>So my guess is that Cs p states produce this QTL-B (but I could be wrong)
I aslo doubt about Cs, there are 36 electrons in core states 1s2s2p3s3p3d4s4p, while the other 19 electrons 4d5s5p6s are treated as valence electrons, no seimcore states. 


>Also: Where is your EF ? Only than one can estimate if the energy parameters
>are ok or need to be changed about 0.2 Ry below EF


The EF is around 0.32 Ryd in my case. So do you mean I should change the energy parameters for s, p, d orbitals from 0.3 to 0.12, But how about the energy values for local orbital?

When I check the case.scf file, I also find the following messages

6 eighvalues below the energy -7.0 ( energy cut off in Lstart)

From this message, do I need to increase the energy cut off in Lstart?


Yanming Ma Ph.D
Steacie Institute for Molecular Sciences,
National Research Councils of Canada,
Ottawa, Ontario
K1A 0R6
Canada


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<P><FONT face="Times New Roman" size=3>Dear Peter,</FONT>
<P><FONT face="Times New Roman" size=3>Thanks very much for your reply.</FONT>
<P><FONT face="Times New Roman" size=3>&gt;&gt; 0.30 5 0 (Cs)<BR>&gt;&gt; 2 0.30 0.000 CONT 1<BR>&gt;&gt;2 -5.08 0.005 STOP 1<BR>&gt;&gt; 0 -1.66 0.010 CONT 1<BR>&gt;&gt; 0 0.30 0.000 CONT 1<BR>&gt;&gt; 1 0.30 0.000 CONT 1<BR><BR>&gt;Is it really the default input ? I would have guessed that Cs has p-semicore<BR>&gt;states and thus has also an lo for l=1 (But I hav'n't checked it myself)?<BR></FONT></P>
<P><FONT face="Times New Roman" size=3>Yes, it is the default input. No semicore is chosen in Cs by default.</FONT></P>
<P><BR><FONT face="Times New Roman" size=3>&gt;So my guess is that Cs p states produce this QTL-B (but I could be wrong)<BR>I aslo doubt about Cs, there are 36 electrons in core states 1s2s2p3s3p3d4s4p, while&nbsp;the&nbsp;other&nbsp;19 electrons 4d5s5p6s are treated as valence electrons, no seimcore states.&nbsp;</FONT></P>
<P><FONT face="Times New Roman" size=3><BR>&gt;Also: Where is your EF ? Only than one can estimate if the energy parameters<BR>&gt;are ok or need to be changed about 0.2 Ry below EF<BR></P></FONT><FONT face="Times New Roman" size=3></FONT>
<P><FONT face="Times New Roman" size=3>The EF is around&nbsp;0.32 Ryd in my case. So do you mean I should change the energy parameters for s, p, d orbitals from 0.3 to 0.12, But how about the energy values for local orbital?</FONT></P>
<P><FONT face="Times New Roman" size=3>When I check the case.scf file, I also find the following messages</FONT></P>
<P><FONT face="Times New Roman" size=3><EM>6 eighvalues below the energy -7.0 ( energy cut off in Lstart)</EM></FONT></P>
<P><FONT face="Times New Roman" size=3>From this message, do I need to increase the energy cut off in Lstart?</FONT></P><BR><BR>Yanming Ma Ph.D<br>Steacie Institute for Molecular Sciences,<br>National Research Councils of Canada,<br>Ottawa, Ontario<br>K1A 0R6<br>Canada<p><br><hr size=1>Do you Yahoo!?<br>
<a href="http://rd.yahoo.com/mail/mailsig/*http://mailplus.yahoo.com">Yahoo! Mail Plus</a> - Powerful. Affordable. <a href="http://rd.yahoo.com/mail/mailsig/*http://mailplus.yahoo.com">Sign up now</a>
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------------------------------

Date: Thu, 12 Dec 2002 16:15:36 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: MPI

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear Peter and other Wieners
        

1) I tested a unit cell containing 13 atoms with 1 k-point for MPI run. 
my .machines file:

lapw0:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 
longhorn1:1 longhorn1:1 longhorn1:1
1:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 
longhorn1:1 longhorn1:1
(where lapw0 is assigned 8 processor and the 1 k-point 8 processors)

in the job script for for load leveler the run command was:

../w2k/runsp_lapw -p

the  case.dayfile is:
______________________________________________________________________________
Calculating GaMo1 in /gpfs/utexas/ph/phaa406/GaMo1
on longhorn5.tacc.utexas.edu

    start       (Thu Dec 12 14:58:23 CST 2002) with lapw0 (20/20 to go)
>   lapw0 -p    (14:58:23) starting parallel lapw0 at Thu Dec 12 14:58:24 
CST 2002
- -------- .machine1 : 8 processors
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1
- --------
0.0u 0.1s 0:28 0% 106+682k 0+0io 0pf+0w
>   lapw1  -c -up -p    (14:58:52) starting parallel lapw1 at Thu Dec 12 
14:58:52 CST 2002
- ->  starting parallel LAPW1 jobs at Thu Dec 12 14:58:52 CST 2002
running LAPW1 in parallel mode (using .machines)
1 number_of_parallel_jobs
[1] 38132
___________________

as you can see, it does not pick up lapw0_mpi(although it runs lapw0 on 8 
processors in parallel) and lapw1_mpi(instead it picks lapw1) and says
1 number_of_parallel_jobs?

My idea was If MPI-script works for 13 atom unit cell with 1 
k-point(although the scf output will not be correct), there will not be
any problem for doing a cell with very large number of atoms and 1-2 
kpoints(ie small BZ).

Is it the correct message in the case.dayfile?  is lapw1_mpi is running on
8 processors in parallel using mpi scripts?
Pl. let me know.

2) Pl. let me know about my yesterday's query about SOC and simultaneous 
optimization in k-point parallelization?


Regards
sahu 




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------------------------------

Date: Fri, 13 Dec 2002 14:15:37 +0900
From: Li Wang <lwang@hrc.toyama-u.ac.jp>
Subject: [WIEN]: Dstart error

====
Li Wang <lwang@hrc.toyama-u.ac.jp>
submitted the following contribution:
====

This is a multi-part message in MIME format.
- --------------020002030808090606030205
Content-Type: text/plain; charset=us-ascii; format=flowed
Content-Transfer-Encoding: 7bit

Dear all,
  I am calculating a slab with H2 molecule.  A error file is created 
when begining running "x start" in a "Initialize calculation" progress, 
which only contaion "Error in Dstart" message.
The process (dstart) will finish in 1~2 hours.  Can you tell me the 
reason and if I can ignore it?


Li Wang
Hydrogen Isotope Research Center,
Toyama University,
3190 Gofuku,
Toyama 930-8555
Japan

- --------------020002030808090606030205
Content-Type: text/plain;
 name="dstart.error"
Content-Transfer-Encoding: 7bit
Content-Disposition: inline;
 filename="dstart.error"


- --------------020002030808090606030205
Content-Type: text/plain;
 name="test6.struct"
Content-Transfer-Encoding: 7bit
Content-Disposition: inline;
 filename="test6.struct"

Wien2k struct file generated by XCrySDen program                               
CXY LATTICE,NONEQUIV. ATOMS  935_Cmm2                                          
MODE OF CALC=NREL unit=bohr                                                    
 11.451745 16.195213105.000000 90.000000 90.000000 90.000000                   
ATOM  -1: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT= 8
V 1        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM  -2: X=0.25000000 Y=0.25000000 Z=0.00000000
          MULT= 2          ISPLIT= 8
      -2: X=0.75000000 Y=0.25000000 Z=0.00000000
V 2        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM  -3: X=0.00000000 Y=0.50000000 Z=0.00000000
          MULT= 1          ISPLIT= 8
V 3        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM  -4: X=0.25000000 Y=0.50000000 Z=0.95161951
          MULT= 2          ISPLIT= 8
      -4: X=0.75000000 Y=0.50000000 Z=0.95161951
V 4        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
LOCAL ROT MATRIX:    0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
                     1.0000000 0.0000000 0.0000000
ATOM  -5: X=0.00000000 Y=0.25000000 Z=0.95161951
          MULT= 2          ISPLIT= 8
      -5: X=0.00000000 Y=0.75000000 Z=0.95161951
V 5        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
LOCAL ROT MATRIX:    0.0000000 0.0000000 1.0000000
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
ATOM  -6: X=0.00000000 Y=0.50000000 Z=0.90323901
          MULT= 1          ISPLIT= 8
V 6        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM  -7: X=0.25000000 Y=0.75000000 Z=0.90323901
          MULT= 2          ISPLIT= 8
      -7: X=0.75000000 Y=0.75000000 Z=0.90323901
V 7        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM  -8: X=0.00000000 Y=0.00000000 Z=0.90323901
          MULT= 1          ISPLIT= 8
V 8        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM  -9: X=0.00000000 Y=0.90000000 Z=0.00000000
          MULT= 2          ISPLIT= 8
      -9: X=0.00000000 Y=0.10000000 Z=0.00000000
H 1        NPT=  781  R0=0.00010000 RMT=    0.4561   Z:  1.0                   
LOCAL ROT MATRIX:    0.0000000 0.0000000 1.0000000
                     1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
   4      NUMBER OF SYMMETRY OPERATIONS
 1 0 0 0.0000000
 0 1 0 0.0000000
 0 0 1 0.0000000
       1
- -1 0 0 0.0000000
 0-1 0 0.0000000
 0 0 1 0.0000000
       2
 1 0 0 0.0000000
 0-1 0 0.0000000
 0 0 1 0.0000000
       3
- -1 0 0 0.0000000
 0 1 0 0.0000000
 0 0 1 0.0000000
       4

- --------------020002030808090606030205--

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------------------------------

Date: Fri, 13 Dec 2002 08:18:59 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Dstart error

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

If the file is still there when dstart finishes (and containing some 
error message) you can usually not ignore it. But in case.outbutd or 
case.dayfile, or on your screen there may be further hints as to what 
went wrong.

Best regards,
Torsten Andersen.

Li Wang wrote:

> Dear all,
>  I am calculating a slab with H2 molecule.  A error file is created 
> when begining running "x start" in a "Initialize calculation" 
> progress, which only contaion "Error in Dstart" message.
> The process (dstart) will finish in 1~2 hours.  Can you tell me the 
> reason and if I can ignore it?
>
>
> Li Wang
> Hydrogen Isotope Research Center,
> Toyama University,
> 3190 Gofuku,
> Toyama 930-8555
> Japan
>
>
>------------------------------------------------------------------------
>
>Wien2k struct file generated by XCrySDen program                               
>CXY LATTICE,NONEQUIV. ATOMS  935_Cmm2                                          
>MODE OF CALC=NREL unit=bohr                                                    
> 11.451745 16.195213105.000000 90.000000 90.000000 90.000000                   
>ATOM  -1: X=0.00000000 Y=0.00000000 Z=0.00000000
>          MULT= 1          ISPLIT= 8
>V 1        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
>LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                     0.0000000 1.0000000 0.0000000
>                     0.0000000 0.0000000 1.0000000
>ATOM  -2: X=0.25000000 Y=0.25000000 Z=0.00000000
>          MULT= 2          ISPLIT= 8
>      -2: X=0.75000000 Y=0.25000000 Z=0.00000000
>V 2        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
>LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                     0.0000000 1.0000000 0.0000000
>                     0.0000000 0.0000000 1.0000000
>ATOM  -3: X=0.00000000 Y=0.50000000 Z=0.00000000
>          MULT= 1          ISPLIT= 8
>V 3        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
>LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                     0.0000000 1.0000000 0.0000000
>                     0.0000000 0.0000000 1.0000000
>ATOM  -4: X=0.25000000 Y=0.50000000 Z=0.95161951
>          MULT= 2          ISPLIT= 8
>      -4: X=0.75000000 Y=0.50000000 Z=0.95161951
>V 4        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
>LOCAL ROT MATRIX:    0.0000000 1.0000000 0.0000000
>                     0.0000000 0.0000000 1.0000000
>                     1.0000000 0.0000000 0.0000000
>ATOM  -5: X=0.00000000 Y=0.25000000 Z=0.95161951
>          MULT= 2          ISPLIT= 8
>      -5: X=0.00000000 Y=0.75000000 Z=0.95161951
>V 5        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
>LOCAL ROT MATRIX:    0.0000000 0.0000000 1.0000000
>                     1.0000000 0.0000000 0.0000000
>                     0.0000000 1.0000000 0.0000000
>ATOM  -6: X=0.00000000 Y=0.50000000 Z=0.90323901
>          MULT= 1          ISPLIT= 8
>V 6        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
>LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                     0.0000000 1.0000000 0.0000000
>                     0.0000000 0.0000000 1.0000000
>ATOM  -7: X=0.25000000 Y=0.75000000 Z=0.90323901
>          MULT= 2          ISPLIT= 8
>      -7: X=0.75000000 Y=0.75000000 Z=0.90323901
>V 7        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
>LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                     0.0000000 1.0000000 0.0000000
>                     0.0000000 0.0000000 1.0000000
>ATOM  -8: X=0.00000000 Y=0.00000000 Z=0.90323901
>          MULT= 1          ISPLIT= 8
>V 8        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0                   
>LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                     0.0000000 1.0000000 0.0000000
>                     0.0000000 0.0000000 1.0000000
>ATOM  -9: X=0.00000000 Y=0.90000000 Z=0.00000000
>          MULT= 2          ISPLIT= 8
>      -9: X=0.00000000 Y=0.10000000 Z=0.00000000
>H 1        NPT=  781  R0=0.00010000 RMT=    0.4561   Z:  1.0                   
>LOCAL ROT MATRIX:    0.0000000 0.0000000 1.0000000
>                     1.0000000 0.0000000 0.0000000
>                     0.0000000 1.0000000 0.0000000
>   4      NUMBER OF SYMMETRY OPERATIONS
> 1 0 0 0.0000000
> 0 1 0 0.0000000
> 0 0 1 0.0000000
>       1
>-1 0 0 0.0000000
> 0-1 0 0.0000000
> 0 0 1 0.0000000
>       2
> 1 0 0 0.0000000
> 0-1 0 0.0000000
> 0 0 1 0.0000000
>       3
>-1 0 0 0.0000000
> 0 1 0 0.0000000
> 0 0 1 0.0000000
>       4
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Fri, 13 Dec 2002 11:54:36 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: Dstart error

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

>   I am calculating a slab with H2 molecule.  A error file is created
> when begining running "x start" in a "Initialize calculation" progress,
> which only contaion "Error in Dstart" message.
> The process (dstart) will finish in 1~2 hours.  Can you tell me the
> reason and if I can ignore it?
I noticed that the size of your sent dstart.error file is zero byte. This
means that x dstart -c  was performed with no error.
        Your,
        S. Jalali.


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------------------------------

Date: Fri, 13 Dec 2002 09:38:23 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: QTL-B = 1220.43

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> The EF is around 0.32 Ryd in my case. So do you mean I should change the energy parameters for s, p, d orbitals from 0.3 to 0.12, But how about the energy values for local orbital?

No, not necessary.

>
> When I check the case.scf file, I also find the following messages
>
> 6 eighvalues below the energy -7.0 ( energy cut off in Lstart)

Ah !!!! As I expected, you got ghostbands. Increasing of the energy cutoff
will not help. Reduce the Cs sphere and start all over again.

(You might need to put a Cs-p LO by hand (e.g. at -0.6 Ry) and for security
set the p-LAPW to e.g. 1.0 Ry). I checked it, the default input does
not give a l=1 LO, because the semicore 5p level is at -0.95 and thus just
above the -1.0 Ry criteria).



                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Fri, 13 Dec 2002 10:07:19 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Dstart error

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>   I am calculating a slab with H2 molecule.  A error file is created
> when begining running "x start" in a "Initialize calculation" progress,
> which only contaion "Error in Dstart" message.
> The process (dstart) will finish in 1~2 hours.  Can you tell me the
> reason and if I can ignore it?

As long as dstart is running, the file  dstart.error contains the message
you mentioned above. As soon as dstart finishes, this file still exists, but
must be empty. If it is NOT empty, you cannot ignore it.

H2 with it's small sphere is a difficult task for WIEN.

Are you sure your structure is what you want to calculate??

H is in exactly the same surface hight as V ? and leads to exceptional small
distances between H and V ?   At least your structure is NOT an H2-molecule!!

If you really want to do such a structure, you will need to reduce RKMAX from
the default (7) to 3-4 (test it?). You also may need a higher GMAX (20-24 ?)
for correct forces!

If you correct the positions, use larger spheres for both, H and V (if
possible).

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Fri, 13 Dec 2002 10:23:24 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: Dstart error

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

This is just the way wien handles its error files.  At the beginning of each
program (eg dstart), an error file is created containing the line 'error in
program'.  When the program is able to end succesfully, the file is emptied.
But during the execution of the program, there is a non-empty error file.
The advantage of this is simple : even if the program crashes in the most
spectacular way and has no chance whatsoever to give you any message, there
will still be an error message.  On the other hand, if the machine would
only write an error file in case something does go wrong, it might not be
able to do this after all, and you would not know there's something wrong
with your calculation.

Don't worry, the errorfile will be empty at the end of dstart.

Good luck with the calculations.

Kevin Jorissen
kevin.jorissen@ua.ac.be

- ----- Original Message -----
From: "Li Wang" <lwang@hrc.toyama-u.ac.jp>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Friday, December 13, 2002 6:15 AM
Subject: [WIEN]: Dstart error


> Dear all,
>   I am calculating a slab with H2 molecule.  A error file is created
> when begining running "x start" in a "Initialize calculation" progress,
> which only contaion "Error in Dstart" message.
> The process (dstart) will finish in 1~2 hours.  Can you tell me the
> reason and if I can ignore it?
>
>
> Li Wang
> Hydrogen Isotope Research Center,
> Toyama University,
> 3190 Gofuku,
> Toyama 930-8555
> Japan
>


- ----------------------------------------------------------------------------
- ----


>


- ----------------------------------------------------------------------------
- ----


> Wien2k struct file generated by XCrySDen program
> CXY LATTICE,NONEQUIV. ATOMS  935_Cmm2
> MODE OF CALC=NREL unit=bohr
>  11.451745 16.195213105.000000 90.000000 90.000000 90.000000
> ATOM  -1: X=0.00000000 Y=0.00000000 Z=0.00000000
>           MULT= 1          ISPLIT= 8
> V 1        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM  -2: X=0.25000000 Y=0.25000000 Z=0.00000000
>           MULT= 2          ISPLIT= 8
>       -2: X=0.75000000 Y=0.25000000 Z=0.00000000
> V 2        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM  -3: X=0.00000000 Y=0.50000000 Z=0.00000000
>           MULT= 1          ISPLIT= 8
> V 3        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM  -4: X=0.25000000 Y=0.50000000 Z=0.95161951
>           MULT= 2          ISPLIT= 8
>       -4: X=0.75000000 Y=0.50000000 Z=0.95161951
> V 4        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> LOCAL ROT MATRIX:    0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
>                      1.0000000 0.0000000 0.0000000
> ATOM  -5: X=0.00000000 Y=0.25000000 Z=0.95161951
>           MULT= 2          ISPLIT= 8
>       -5: X=0.00000000 Y=0.75000000 Z=0.95161951
> V 5        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> LOCAL ROT MATRIX:    0.0000000 0.0000000 1.0000000
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
> ATOM  -6: X=0.00000000 Y=0.50000000 Z=0.90323901
>           MULT= 1          ISPLIT= 8
> V 6        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM  -7: X=0.25000000 Y=0.75000000 Z=0.90323901
>           MULT= 2          ISPLIT= 8
>       -7: X=0.75000000 Y=0.75000000 Z=0.90323901
> V 7        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM  -8: X=0.00000000 Y=0.00000000 Z=0.90323901
>           MULT= 1          ISPLIT= 8
> V 8        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM  -9: X=0.00000000 Y=0.90000000 Z=0.00000000
>           MULT= 2          ISPLIT= 8
>       -9: X=0.00000000 Y=0.10000000 Z=0.00000000
> H 1        NPT=  781  R0=0.00010000 RMT=    0.4561   Z:  1.0
> LOCAL ROT MATRIX:    0.0000000 0.0000000 1.0000000
>                      1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>    4      NUMBER OF SYMMETRY OPERATIONS
>  1 0 0 0.0000000
>  0 1 0 0.0000000
>  0 0 1 0.0000000
>        1
> -1 0 0 0.0000000
>  0-1 0 0.0000000
>  0 0 1 0.0000000
>        2
>  1 0 0 0.0000000
>  0-1 0 0.0000000
>  0 0 1 0.0000000
>        3
> -1 0 0 0.0000000
>  0 1 0 0.0000000
>  0 0 1 0.0000000
>        4
>

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------------------------------

Date: 13 Dec 2002 21:34:36 +0900
From: Li Wang <lwang@hrc.toyama-u.ac.jp>
Subject: Re: [WIEN]: Dstart error

====
Li Wang <lwang@hrc.toyama-u.ac.jp>
submitted the following contribution:
====

Dear Prof. P.Blaha,
  Thank you for your reply. The structure file is not a correct, and it
is only a test. Now I am studying  absorption of Hydrogen molecule on 
metal surface with Wien2k and other package. As you said, it is a
difficult task for Wien.
  
Li wang
 
 
  
ÔÚ 2002-12-13 Îå µÄ 18:07£¬ Peter Blaha Ð´µÀ£º
> ====
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> ====
> 
> >   I am calculating a slab with H2 molecule.  A error file is created
> > when begining running "x start" in a "Initialize calculation" progress,
> > which only contaion "Error in Dstart" message.
> > The process (dstart) will finish in 1~2 hours.  Can you tell me the
> > reason and if I can ignore it?
> 
> As long as dstart is running, the file  dstart.error contains the message
> you mentioned above. As soon as dstart finishes, this file still exists, but
> must be empty. If it is NOT empty, you cannot ignore it.
> 
> H2 with it's small sphere is a difficult task for WIEN.
> 
> Are you sure your structure is what you want to calculate??
> 
> H is in exactly the same surface hight as V ? and leads to exceptional small
> distances between H and V ?   At least your structure is NOT an H2-molecule!!
> 
> If you really want to do such a structure, you will need to reduce RKMAX from
> the default (7) to 3-4 (test it?). You also may need a higher GMAX (20-24 ?)
> for correct forces!
> 
> If you correct the positions, use larger spheres for both, H and V (if
> possible).
> 
>                                       P.Blaha
> --------------------------------------------------------------------------
> Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
> Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
> Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
> --------------------------------------------------------------------------
> 
> ====
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> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 


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------------------------------

Date: 13 Dec 2002 21:38:17 +0900
From: Li Wang <lwang@hrc.toyama-u.ac.jp>
Subject: Re: [WIEN]: Dstart error

====
Li Wang <lwang@hrc.toyama-u.ac.jp>
submitted the following contribution:
====

Dear Jalali,
   Thank you for your reply.

Sincerely, yous
Li Wang
 
ÔÚ 2002-12-13 Îå µÄ 17:24£¬ Saeid Jalali Ð´µÀ£º
> ====
> "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> submitted the following contribution:
> ====
> 
> >   I am calculating a slab with H2 molecule.  A error file is created
> > when begining running "x start" in a "Initialize calculation" progress,
> > which only contaion "Error in Dstart" message.
> > The process (dstart) will finish in 1~2 hours.  Can you tell me the
> > reason and if I can ignore it?
> I noticed that the size of your sent dstart.error file is zero byte. This
> means that x dstart -c  was performed with no error.
>         Your,
>         S. Jalali.
> 
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 


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------------------------------

Date: 13 Dec 2002 21:39:48 +0900
From: Li Wang <lwang@hrc.toyama-u.ac.jp>
Subject: Re: [WIEN]: Dstart error

====
Li Wang <lwang@hrc.toyama-u.ac.jp>
submitted the following contribution:
====

Dear Jorissen,
  Thank you for your reply.

Sincerely,yous
Li Wang

ÔÚ 2002-12-13 Îå µÄ 18:23£¬ Kevin Jorissen Ð´µÀ£º
> ====
> "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
> submitted the following contribution:
> ====
> 
> This is just the way wien handles its error files.  At the beginning of each
> program (eg dstart), an error file is created containing the line 'error in
> program'.  When the program is able to end succesfully, the file is emptied.
> But during the execution of the program, there is a non-empty error file.
> The advantage of this is simple : even if the program crashes in the most
> spectacular way and has no chance whatsoever to give you any message, there
> will still be an error message.  On the other hand, if the machine would
> only write an error file in case something does go wrong, it might not be
> able to do this after all, and you would not know there's something wrong
> with your calculation.
> 
> Don't worry, the errorfile will be empty at the end of dstart.
> 
> Good luck with the calculations.
> 
> Kevin Jorissen
> kevin.jorissen@ua.ac.be
> 
> ----- Original Message -----
> From: "Li Wang" <lwang@hrc.toyama-u.ac.jp>
> To: <wien@zeus.theochem.tuwien.ac.at>
> Sent: Friday, December 13, 2002 6:15 AM
> Subject: [WIEN]: Dstart error
> 
> 
> > Dear all,
> >   I am calculating a slab with H2 molecule.  A error file is created
> > when begining running "x start" in a "Initialize calculation" progress,
> > which only contaion "Error in Dstart" message.
> > The process (dstart) will finish in 1~2 hours.  Can you tell me the
> > reason and if I can ignore it?
> >
> >
> > Li Wang
> > Hydrogen Isotope Research Center,
> > Toyama University,
> > 3190 Gofuku,
> > Toyama 930-8555
> > Japan
> >
> 
> 
> ----------------------------------------------------------------------------
> ----
> 
> 
> >
> 
> 
> ----------------------------------------------------------------------------
> ----
> 
> 
> > Wien2k struct file generated by XCrySDen program
> > CXY LATTICE,NONEQUIV. ATOMS  935_Cmm2
> > MODE OF CALC=NREL unit=bohr
> >  11.451745 16.195213105.000000 90.000000 90.000000 90.000000
> > ATOM  -1: X=0.00000000 Y=0.00000000 Z=0.00000000
> >           MULT= 1          ISPLIT= 8
> > V 1        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> > LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > ATOM  -2: X=0.25000000 Y=0.25000000 Z=0.00000000
> >           MULT= 2          ISPLIT= 8
> >       -2: X=0.75000000 Y=0.25000000 Z=0.00000000
> > V 2        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> > LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > ATOM  -3: X=0.00000000 Y=0.50000000 Z=0.00000000
> >           MULT= 1          ISPLIT= 8
> > V 3        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> > LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > ATOM  -4: X=0.25000000 Y=0.50000000 Z=0.95161951
> >           MULT= 2          ISPLIT= 8
> >       -4: X=0.75000000 Y=0.50000000 Z=0.95161951
> > V 4        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> > LOCAL ROT MATRIX:    0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> >                      1.0000000 0.0000000 0.0000000
> > ATOM  -5: X=0.00000000 Y=0.25000000 Z=0.95161951
> >           MULT= 2          ISPLIT= 8
> >       -5: X=0.00000000 Y=0.75000000 Z=0.95161951
> > V 5        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> > LOCAL ROT MATRIX:    0.0000000 0.0000000 1.0000000
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> > ATOM  -6: X=0.00000000 Y=0.50000000 Z=0.90323901
> >           MULT= 1          ISPLIT= 8
> > V 6        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> > LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > ATOM  -7: X=0.25000000 Y=0.75000000 Z=0.90323901
> >           MULT= 2          ISPLIT= 8
> >       -7: X=0.75000000 Y=0.75000000 Z=0.90323901
> > V 7        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> > LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > ATOM  -8: X=0.00000000 Y=0.00000000 Z=0.90323901
> >           MULT= 1          ISPLIT= 8
> > V 8        NPT=  781  R0=0.00005000 RMT=    1.0634   Z: 23.0
> > LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >                      0.0000000 0.0000000 1.0000000
> > ATOM  -9: X=0.00000000 Y=0.90000000 Z=0.00000000
> >           MULT= 2          ISPLIT= 8
> >       -9: X=0.00000000 Y=0.10000000 Z=0.00000000
> > H 1        NPT=  781  R0=0.00010000 RMT=    0.4561   Z:  1.0
> > LOCAL ROT MATRIX:    0.0000000 0.0000000 1.0000000
> >                      1.0000000 0.0000000 0.0000000
> >                      0.0000000 1.0000000 0.0000000
> >    4      NUMBER OF SYMMETRY OPERATIONS
> >  1 0 0 0.0000000
> >  0 1 0 0.0000000
> >  0 0 1 0.0000000
> >        1
> > -1 0 0 0.0000000
> >  0-1 0 0.0000000
> >  0 0 1 0.0000000
> >        2
> >  1 0 0 0.0000000
> >  0-1 0 0.0000000
> >  0 0 1 0.0000000
> >        3
> > -1 0 0 0.0000000
> >  0 1 0 0.0000000
> >  0 0 1 0.0000000
> >        4
> >
> 
> ====
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------------------------------

Date: Fri, 13 Dec 2002 06:36:00 -0800 (PST)
From: Wenqing ZHANG <dft_flapw@yahoo.com>
Subject: [WIEN]: MPI lib for intel/linux fortran

====
Wenqing ZHANG <dft_flapw@yahoo.com>
submitted the following contribution:
====

Hi,

Can anyone tell me what is the best MPI lib for
intel/Fortran? Where can download the package? I am
currently trying to run WIEN on xeon machine.

Thanks for help.

Yours -- Wenqing

=====
Wenqing ZHANG
1970 Crystal Lake Dr. Apt#E79
Shelby Twp., MI 48316
Tel: (810)254-9931(h), (810)323-1551(o)
Fax: (810)323-9898

__________________________________________________
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------------------------------

Date: Fri, 13 Dec 2002 06:47:36 -0800 (PST)
From: yanming Ma <ymma66@yahoo.com>
Subject: Re: [WIEN]: QTL-B = 1220.43

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-288855027-1039790856=:77978
Content-Type: text/plain; charset=us-ascii


Dear Peter,
Thanks for your answers. I will try under your suggestion and let you know the results. But due to the long computing time, I may reply you a little bit later.
Best Regards.
Yanming Ma
 Peter Blaha <pblaha@theochem.tuwien.ac.at> wrote:====
Peter Blaha 

submitted the following contribution:
====

> The EF is around 0.32 Ryd in my case. So do you mean I should change the energy parameters for s, p, d orbitals from 0.3 to 0.12, But how about the energy values for local orbital?

No, not necessary.

>
> When I check the case.scf file, I also find the following messages
>
> 6 eighvalues below the energy -7.0 ( energy cut off in Lstart)

Ah !!!! As I expected, you got ghostbands. Increasing of the energy cutoff
will not help. Reduce the Cs sphere and start all over again.

(You might need to put a Cs-p LO by hand (e.g. at -0.6 Ry) and for security
set the p-LAPW to e.g. 1.0 Ry). I checked it, the default input does
not give a l=1 LO, because the semicore 5p level is at -0.95 and thus just
above the -1.0 Ry criteria).



P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671 FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

====
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Yanming Ma Ph.D
Steacie Institute for Molecular Sciences,
National Research Councils of Canada,
Ottawa, Ontario
K1A 0R6
Canada


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- --0-288855027-1039790856=:77978
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<P>Dear Peter,
<P>Thanks for your answers. I will try&nbsp;under your suggestion and let you know the results. But due to the long computing time, I may reply you&nbsp;a little bit later.
<P>Best Regards.
<P>Yanming Ma
<P>&nbsp;<B><I>Peter Blaha &lt;pblaha@theochem.tuwien.ac.at&gt;</I></B> wrote:
<BLOCKQUOTE style="PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #1010ff 2px solid">====<BR>Peter Blaha <PBLAHA@THEOCHEM.TUWIEN.AC.AT><BR>submitted the following contribution:<BR>====<BR><BR>&gt; The EF is around 0.32 Ryd in my case. So do you mean I should change the energy parameters for s, p, d orbitals from 0.3 to 0.12, But how about the energy values for local orbital?<BR><BR>No, not necessary.<BR><BR>&gt;<BR>&gt; When I check the case.scf file, I also find the following messages<BR>&gt;<BR>&gt; 6 eighvalues below the energy -7.0 ( energy cut off in Lstart)<BR><BR>Ah !!!! As I expected, you got ghostbands. Increasing of the energy cutoff<BR>will not help. Reduce the Cs sphere and start all over again.<BR><BR>(You might need to put a Cs-p LO by hand (e.g. at -0.6 Ry) and for security<BR>set the p-LAPW to e.g. 1.0 Ry). I checked it, the default input does<BR>not give a l=1 LO, because the semicore 5p level is at -0.95 and thus just<BR>above the -1.0 Ry criteria).<BR><!
BR><BR><BR>P.Blaha<BR>--------------------------------------------------------------------------<BR>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna<BR>Phone: +43-1-58801-15671 FAX: +43-1-58801-15698<BR>Email: blaha@theochem.tuwien.ac.at WWW: http://info.tuwien.ac.at/theochem/<BR>--------------------------------------------------------------------------<BR><BR>====<BR>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at<BR>To (un)subscribe send mail to<BR>majordomo@zeus.theochem.tuwien.ac.at<BR>====</BLOCKQUOTE><BR><BR>Yanming Ma Ph.D<br>Steacie Institute for Molecular Sciences,<br>National Research Councils of Canada,<br>Ottawa, Ontario<br>K1A 0R6<br>Canada<p><br><hr size=1>Do you Yahoo!?<br>
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------------------------------

Date: Fri, 13 Dec 2002 19:23:11 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: meta-GGA

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear W2kusers

1) From the Peter's reply in the mailing list,it seems that
meta-gga(perdew et.al 2000) is possible with w2k. However in the
userguide, script "lstart" gives only three options of XC-potentials (LSDA
and two GGA). In the description of "case.in0" file, it is said option
12(meta-GGA) is possible. That means one has to put manually(by hand)
number 12 for meta-GGA case in 'case.in0' before starting the scf cycle.
am I right? the procedure would be(from Peter's reply in the mailing list)

1) run atleast one iteration with GGA option( number 13).
 
2) copy case.inm to case.inm_vresp.
3) set NORM = NO in case.inm_vresp and change GMAX to 24 in case.in2.
4) start the scf cycle.

Have any user tested this option for bulk systems say for optimized
lattice parameters?any problems encountered? any special precautions?

2) In case.inso (for SO run), one needs to specify the number of atoms for
which RLO's should be added(if one wish to) and in case.indm file , we
need to specify number of atoms for which DM should be calculated.If I
have a test case in which there are two inequivalant atoms in the
structure each having multiplicity two ie total four atoms in the cell.
and if I wish to add a RLO and calcualte the DM for only the 1st
inequivalant atom then number of atoms in the case.inso and case.indm
should be 1 or 2. Suppose I wish to switch-off SOC for the 2nd
inequivalant atom(multiplicity two) then the last line in case.inso look
like:
 
1 2 ----> assuming we have to put only the inequivalant atom and '2' is 
inequivalant atom number 2 ie ATOM 2 in the case.struct file.

In short, do we have to put the number of atom of inequivalant type or 
include its multiplicity also in case.inso and case.indm.

3)  I use run(sp)_lapw -so -dm available with the recent update to add the
spin-orbit coupling after non-SOC spinpolarized scf run or from the
begining. It calculates the orbital moments on the atom specified in the
case.inso and case.indm(in the file case.scfdmup). So the query about the
running procedure for SOC is now clear which I posed in my last mail to
the list. 

Please let me know about the MPI run query.


Regards
sahu

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------------------------------

Date: Sat, 14 Dec 2002 08:49:05 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: meta-GGA

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> 1) From the Peter's reply in the mailing list,it seems that
> meta-gga(perdew et.al 2000) is possible with w2k. However in the
> userguide, script "lstart" gives only three options of XC-potentials (LSDA
> and two GGA). In the description of "case.in0" file, it is said option
> 12(meta-GGA) is possible. That means one has to put manually(by hand)
> number 12 for meta-GGA case in 'case.in0' before starting the scf cycle.
> am I right?

Yes, you are right.

> the procedure would be(from Peter's reply in the mailing list)
>
> 1) run atleast one iteration with GGA option( number 13).
>
> 2) copy case.inm to case.inm_vresp.
> 3) set NORM = NO in case.inm_vresp and change GMAX to 24 in case.in2.
> 4) start the scf cycle.

Required large Gmax is due to the fact that Meta-GGA also requires the
orbital kinetic energy density, which is byond (meta) of  GGA, where in GGA
only local density and its first gradient are required.

> Have any user tested this option for bulk systems say for optimized
> lattice parameters?any problems encountered? any special precautions?

I have not tested it yet, but it is reported that:
1) such schemes are not yet self-consistent (user guied).
2) Molecular atomization energies and metal surface energies are
significantly improved (PRL 82, 2544 (1999)).
3) Lattice constants are little changed (PRL 82, 2544 (1999)).
        Your,
        S. Jalali.

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Date: Sat, 14 Dec 2002 18:23:00 +0800 (CST)
From: music@theory.issp.ac.cn
Subject: [WIEN]: LAPW and APW

====
music@theory.issp.ac.cn
submitted the following contribution:
====


Dear wien users,
  When we modify the case.in1 file, How to determine the selecting 
of LAPW or APW ?  Does the appearance of ghost band have relation  to 
to the selecting  ?
  Could anyone could help me ? THANKS IN ADVANCE!
- -- 





sincerely yours 

Ying.X


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Date: Sat, 14 Dec 2002 19:08:33 +0800 (CST)
From: yshzhang@theory.issp.ac.cn
Subject: Re: [WIEN]: LAPW and APW

====
yshzhang@theory.issp.ac.cn
submitted the following contribution:
====

Hi

>   When we modify the case.in1 file, How to determine the selecting 
> of LAPW or APW ?  

Please read the UG page 79. For example: 
WFFIL        (WFPRI, SUPWF)
  7.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  0.30    6  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global 
APW/LAPW)
In this case.in1, it use LAPW. 

Change the file as the following:
WFFIL        (WFPRI, SUPWF)
  7.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  0.30    6  1
the APW is using.      

Does the appearance of ghost band have relation  to 
> to the selecting  ?

Yes, I think the 0(LAPW) is better than 1 (APW) if ghost bands exist.

- -- 
Best Regards
YS Zhang

- ------------------------------------------------------------------------
 Address: Institute of Solid State Physics
          Chinese Academy of Sciences
          P.O.BOX 1129,230031 Hefei 
          P.R~China
 Tel:     086-551-5591464(Office)
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 Fax:     086-551-5591434
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Date: Sat, 14 Dec 2002 10:05:54 -0500
From: "michel certier" <mcertier@mail.com>
Subject: [WIEN]: test

====
"michel certier" <mcertier@mail.com>
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====

sorry this is just test !!!


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Date: Sat, 14 Dec 2002 10:22:40 -0500
From: "michel certier" <mcertier@mail.com>
Subject: [WIEN]: about kgen

====
"michel certier" <mcertier@mail.com>
submitted the following contribution:
====

Hi, I am novice so excuse me if my question appear some stupid. I am doing some test on orthorhombic system (62_Pnm) when I run x kgen it ask me Number of k-points:, so I choose 8, if I use Shift k-mesh (if applicable) its give me 4 kpoint in the irreducible part of Brillouin zone otherwise its give me 2 kpoint. Cans some one explain me the scheme used here and the difference between the two choice. Thanks

Michele 

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Date: Sat, 14 Dec 2002 10:26:08 -0500
From: "michel certier" <mcertier@mail.com>
Subject: [WIEN]: question

====
"michel certier" <mcertier@mail.com>
submitted the following contribution:
====

Hi, Its against me :-). Whene I read somme paper of electronic band structute (ab initio) for exampel for the semi conductor usally the authors says ...we have shift the fermi level to the top of band valence ( in principal in sc the fermi level lie at the half of Ec-Eg) So can somme explain me this ....
Thanks once more
Michele 

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Date: Sat, 14 Dec 2002 16:30:02 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: about kgen

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Michele,

If you had read the manual (Sec. 6.5, I think), it would be clear to 
you. Shifting the k-mesh shifts it away from high-symmetry points, thus 
giving more k-points. The k-points are generated according to the paper 
of Bloechl et. al. cited in the manual.

Best regards,
Torsten Andersen.

michel certier wrote:

>====
>"michel certier" <mcertier@mail.com>
>submitted the following contribution:
>====
>
>Hi, I am novice so excuse me if my question appear some stupid. I am doing some test on orthorhombic system (62_Pnm) when I run x kgen it ask me Number of k-points:, so I choose 8, if I use Shift k-mesh (if applicable) its give me 4 kpoint in the irreducible part of Brillouin zone otherwise its give me 2 kpoint. Cans some one explain me the scheme used here and the difference between the two choice. Thanks
>
>Michele 
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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Date: Sat, 14 Dec 2002 16:34:41 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: question

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

I'll bet this is one of the variants of the "scissors operator"... 
because the calculated band structure is wrong, one adjusts the bandgap 
by cutting, moving, etc. the spaghetties (which are Kohn-Sham 
eigenvalues, and in principle unphysical, but "works very well in 
practice" as people usually say). Alternatively, it is referred to 
because these methods do not calculate the Fermi energy explicitly. The 
Wien code calculates the Fermi energy for you.

Best regards,
Torsten Andersen.

michel certier wrote:

>====
>"michel certier" <mcertier@mail.com>
>submitted the following contribution:
>====
>
>Hi, Its against me :-). Whene I read somme paper of electronic band structute (ab initio) for exampel for the semi conductor usally the authors says ...we have shift the fermi level to the top of band valence ( in principal in sc the fermi level lie at the half of Ec-Eg) So can somme explain me this ....
>Thanks once more
>Michele 
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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Date: Sun, 15 Dec 2002 18:44:58 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: question

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Hi, Its against me :-). Whene I read somme paper of electronic band structute (ab initio) for exampel for the semi conductor usally the authors says ...we have shift the fermi level to the top of band valence ( in principal in sc the fermi level lie at the half of Ec-Eg) So can somme explain me this ....

In theory the Fermi level is the highest occupied state and this is (for
our idealized semiconductor) the top of the valence band.

Also remember: Usually the energy gap comes out 50% too small in theory.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Mon, 16 Dec 2002 13:35:00 +0100 (CET)
From: =?iso-8859-1?q?amm=E9=20marcel?= <marcel_sig@yahoo.fr>
Subject: [WIEN]: need to help

====
=?iso-8859-1?q?amm=E9=20marcel?= <marcel_sig@yahoo.fr>
submitted the following contribution:
====

- --0-2051491089-1040042100=:56799
Content-Type: text/plain; charset=iso-8859-1
Content-Transfer-Encoding: 8bit


Dear Wien users

H!

Please, could you explain to me what is the origin of this message in lapw1.error file :

'DPHTRF'  -  DPHTR4  aborded unsuccessfully

Thank you

best ragrds

Marcel



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- --0-2051491089-1040042100=:56799
Content-Type: text/html; charset=iso-8859-1
Content-Transfer-Encoding: 8bit

<P>Dear Wien users</P>
<P>H!</P>
<P>Please, could you explain to me what is the origin of this message in lapw1.error file&nbsp;:</P>
<P>'DPHTRF'&nbsp; -&nbsp; DPHTR4&nbsp; aborded unsuccessfully</P>
<P>Thank you</P>
<P>best ragrds</P>
<P>Marcel</P><p><br><hr size=1>Do You Yahoo!? -- Une adresse @yahoo.fr gratuite et en français !<br>
<a href=http://fr.mail.yahoo.com>Testez le nouveau Yahoo! Mail</a>
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Date: Mon, 16 Dec 2002 13:56:46 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: need to help

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

It probably means that your struct file is wrong. It is from BLAS, I think.

Best regards,
Torsten Andersen.

ammé marcel wrote:

> Dear Wien users
>
> H!
>
> Please, could you explain to me what is the origin of this message in 
> lapw1.error file :
>
> 'DPHTRF'  -  DPHTR4  aborded unsuccessfully
>
> Thank you
>
> best ragrds
>
> Marcel
>
>
> ------------------------------------------------------------------------
> Do You Yahoo!? -- Une adresse @yahoo.fr gratuite et en français !
> Testez le nouveau Yahoo! Mail <http://fr.mail.yahoo.com> 


- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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Date: Mon, 16 Dec 2002 11:08:02 -0800 (PST)
From: yanming Ma <ymma66@yahoo.com>
Subject: Re: [WIEN]: QTL-B = 1220.43

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-532721984-1040065682=:6778
Content-Type: text/plain; charset=us-ascii


Dear Peter,


>Ah !!!! As I expected, you got ghostbands. Increasing of the energy cutoff
>will not help. Reduce the Cs sphere and start all over again.

I reduced the Cs sphere from 3.2 to 2.8. Bi and Te sphere are also set as 2.8. 
I restart the calculation and use the default values for Case.in1. 
But I still got the ghostbands as indicated by warnings of 
QTL- B = 1922. and 6 eighnvectors are below -7.0 Ryd.

>(You might need to put a Cs-p LO by hand (e.g. at -0.6 Ry) and for security
>set the p-LAPW to e.g. 1.0 Ry). I checked it, the default input does
>not give a l=1 LO, because the semicore 5p level is at -0.95 and thus just
>above the -1.0 Ry criteria).

The default energy parameters in Case.in1 are 

0.3     5      0
2      0.30        0.000    CONT 1
2     -5.08        0.005    STOP  1
0     -1.66        0.010    CONT 1
0      0.30        0.000    CONT 1
1      0.30        0.000    CONT 1

I changed  to the following

0.3     5      0
2      0.30        0.000    CONT 1
2     -5.08        0.005    STOP  1
0     -1.66        0.010    CONT 1
0      0.30        0.000    CONT 1
1      0.30        0.000    CONT 1
1     -0.60        0.010    CONT 1    ------   added line for p lo

Using this changed Case.in1 file, the lapw1 crashed. I also tried in this way,
 
0.3     5      0
2      0.30        0.000    CONT 1
2     -5.08        0.005    STOP  1
0     -1.66        0.010    CONT 1
0      0.30        0.000    CONT 1
1      1.00        0.000    CONT 1   ------- changed line
1     -0.60        0.010    CONT 1   ------- added line for p lo

The lapw1 still crashed.

So any other ideas?

Best Regards




Yanming Ma Ph.D
Steacie Institute for Molecular Sciences,
National Research Councils of Canada,
Ottawa, Ontario
K1A 0R6
Canada


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- --0-532721984-1040065682=:6778
Content-Type: text/html; charset=us-ascii

<P>Dear Peter,</P>
<P><BR>&gt;Ah !!!! As I expected, you got ghostbands. Increasing of the energy cutoff<BR>&gt;will not help. Reduce the Cs sphere and start all over again.</P>
<P>I reduced the Cs sphere from 3.2 to 2.8. Bi and Te sphere are also set as 2.8. <BR>I restart the calculation and use the default values for Case.in1. <BR>But I still got the ghostbands as indicated by warnings of <BR>QTL- B = 1922. and 6 eighnvectors are below -7.0 Ryd.</P>
<P>&gt;(You might need to put a Cs-p LO by hand (e.g. at -0.6 Ry) and for security<BR>&gt;set the p-LAPW to e.g. 1.0 Ry). I checked it, the default input does<BR>&gt;not give a l=1 LO, because the semicore 5p level is at -0.95 and thus just<BR>&gt;above the -1.0 Ry criteria).</P>
<P>The default energy parameters in Case.in1 are </P>
<P>0.3&nbsp;&nbsp;&nbsp;&nbsp; 5&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0<BR>2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>2&nbsp;&nbsp;&nbsp;&nbsp; -5.08&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.005&nbsp;&nbsp;&nbsp; STOP&nbsp; 1<BR>0&nbsp;&nbsp;&nbsp;&nbsp; -1.66&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010&nbsp;&nbsp;&nbsp; CONT 1<BR>0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>1&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1</P>
<P>I changed&nbsp; to the following</P>
<P>0.3&nbsp;&nbsp;&nbsp;&nbsp; 5&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0<BR>2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>2&nbsp;&nbsp;&nbsp;&nbsp; -5.08&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.005&nbsp;&nbsp;&nbsp; STOP&nbsp; 1<BR>0&nbsp;&nbsp;&nbsp;&nbsp; -1.66&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010&nbsp;&nbsp;&nbsp; CONT 1<BR>0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>1&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>1&nbsp;&nbsp;&nbsp;&nbsp; -0.60&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010&nbsp;&nbsp;&nbsp; CONT 1&nbsp;&nbsp;&nbsp; ------&nbsp;&nbsp; added line for p lo</P>
<P>Using this changed Case.in1 file, <STRONG>the lapw1 crashed</STRONG>. I also tried in this way,<BR>&nbsp;<BR>0.3&nbsp;&nbsp;&nbsp;&nbsp; 5&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0<BR>2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>2&nbsp;&nbsp;&nbsp;&nbsp; -5.08&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.005&nbsp;&nbsp;&nbsp; STOP&nbsp; 1<BR>0&nbsp;&nbsp;&nbsp;&nbsp; -1.66&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010&nbsp;&nbsp;&nbsp; CONT 1<BR>0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>1&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 1.00&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1&nbsp;&nbsp; ------- changed line<BR>1&nbsp;&nbsp;&nbsp;&nbsp; -0.60&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010&nbsp;&nbsp;&nbsp; CONT 1&nbsp;&nbsp; ------- added line for p lo</P>
<P><STRONG>The lapw1 still crashed.</STRONG></P>
<P>So any other ideas?</P>
<P>Best Regards<BR><BR></P><BR><BR>Yanming Ma Ph.D<br>Steacie Institute for Molecular Sciences,<br>National Research Councils of Canada,<br>Ottawa, Ontario<br>K1A 0R6<br>Canada<p><br><hr size=1>Do you Yahoo!?<br>
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Date: Tue, 17 Dec 2002 08:42:33 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: QTL-B = 1220.43

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I changed  to the following
>
> 0.3     5      0                          <======================
> 2      0.30        0.000    CONT 1
> 2     -5.08        0.005    STOP  1
> 0     -1.66        0.010    CONT 1
> 0      0.30        0.000    CONT 1
> 1      0.30        0.000    CONT 1
> 1     -0.60        0.010    CONT 1    ------   added line for p lo
>
> Using this changed Case.in1 file, the lapw1 crashed.

Of course!!!   You must change the 5 to 6 in the first line!

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
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Date: Tue, 17 Dec 2002 12:20:27 -0500
From: "michel certier" <mcertier@mail.com>
Subject: [WIEN]: Wien2K instalation on dual PIV

====
"michel certier" <mcertier@mail.com>
submitted the following contribution:
====

Dear wien users. Can some one explain me how ti install WIEN2K in Dual Pentium Machime I have some problem to this task (do I need mpi for ex etc ...)

Thank you once More

Michel  
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Date: Tue, 17 Dec 2002 18:30:12 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Wien2K instalation on dual PIV

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

If you want to distribute one k-point over the two processors, you need 
MPI. If you want to distribute two or more, you don't need it.

Best regards,
Torsten.

michel certier wrote:

>====
>"michel certier" <mcertier@mail.com>
>submitted the following contribution:
>====
>
>Dear wien users. Can some one explain me how ti install WIEN2K in Dual Pentium Machime I have some problem to this task (do I need mpi for ex etc ...)
>
>Thank you once More
>
>Michel  
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
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Date: Wed, 18 Dec 2002 09:01:14 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Wien2K instalation on dual PIV

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Dear wien users. Can some one explain me how ti install WIEN2K in Dual Pentium Machime I have some problem to this task (do I need mpi for ex etc ...)

All you need is a f90 compiler. We recommend the free Intel ifc 6.0 together
with the mkl 5.2 (also from www.intel.com).

Then follow the instructions from the download page and finally run
siteconfig and userconfig. It should be quite easy.

If you want to run WIEN2k just on ONE dual Pentium machine, select "shared
memory", if you have more usable PCs on your network, say no.
If you want to use parallelization over more PCs make sure you configure
your machines such that you have a common NFS-filesystem (Your files
must be accessible on all machines under the same path) and that you can
logon with rsh or ssh without a password.

It depends what you want to study, but for "regular" cases you don't need mpi.
Only for very large cases with just one k-point (usually more than 50
atoms/cell) the mpi-parallel version is a valuable option.
It is clearly an "expert" option.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
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Date: Wed, 18 Dec 2002 20:44:01 +0900
From: Li Wang <lwang@hrc.toyama-u.ac.jp>
Subject: [WIEN]: Allocate error

====
Li Wang <lwang@hrc.toyama-u.ac.jp>
submitted the following contribution:
====

Dear all ,
 
  The lapw1 crashed when I run "x lapw -c".  The message is:
"Allocate error 494: Allocation of Array with extent of 143952004 failed
End of diagnostics",
Can some one can tell me the possible reason.

Thanks.

Li Wang



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------------------------------

Date: Wed, 18 Dec 2002 12:44:40 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: Allocate error

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Out of memory (virtual memory). The program requests a chunk of data 
(roughly 137MB) from the system main memory, and it is not available. 
Try to increase the swap size.

Best regards,
Torsten Andersen.

Li Wang wrote:

> ====
> Li Wang <lwang@hrc.toyama-u.ac.jp>
> submitted the following contribution:
> ====
>
> Dear all ,
>
>  The lapw1 crashed when I run "x lapw -c".  The message is:
> "Allocate error 494: Allocation of Array with extent of 143952004 failed
> End of diagnostics",
> Can some one can tell me the possible reason.
>
> Thanks.
>
> Li Wang
>
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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Date: Thu, 19 Dec 2002 10:00:32 +0900
From: Li Wang <lwang@hrc.toyama-u.ac.jp>
Subject: Re: [WIEN]: Allocate error

====
Li Wang <lwang@hrc.toyama-u.ac.jp>
submitted the following contribution:
====

Torsten Andersen wrote:

> ====
> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
> submitted the following contribution:
> ====
>
> Out of memory (virtual memory). The program requests a chunk of data 
> (roughly 137MB) from the system main memory, and it is not available. 
> Try to increase the swap size.
>
> Best regards,
> Torsten Andersen.
>
> Li Wang wrote:
>
>> ====
>> Li Wang <lwang@hrc.toyama-u.ac.jp>
>> submitted the following contribution:
>> ====
>>
>> Dear all ,
>>
>> The lapw1 crashed when I run "x lapw -c". The message is:
>> "Allocate error 494: Allocation of Array with extent of 143952004 failed
>> End of diagnostics",
>> Can some one can tell me the possible reason.
>>
>> Thanks.
>>
>> Li Wang
>>
>>
>>
>> ====
>> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>> To (un)subscribe send mail to
>> majordomo@zeus.theochem.tuwien.ac.at
>> ====
>>
>>
>
Dear Dr. Andersen,
Thank you for your reply. But I have 2G memory and 2G swap space. I 
think that there should be another reason.

Best regrads,

Li Wang

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------------------------------

Date: Wed, 18 Dec 2002 12:20:02 +0100
From: Peer Kruse <kruse@lem.uni-karlsruhe.de>
Subject: Re: [WIEN]: Allocate error

====
Peer Kruse <kruse@lem.uni-karlsruhe.de>
submitted the following contribution:
====

Have you checked your ulimits? It's not enough to have the memory but 
you have to be allowed to use it.
Try a
"ulimit -a" if you have Linux, often data seg size and stack size are 
critical points, unlimited is somtimes good value
but be aware not to write too big core files.

regards

Peer

Li Wang wrote:

> ====
> Li Wang <lwang@hrc.toyama-u.ac.jp>
> submitted the following contribution:
> ====
>
> Torsten Andersen wrote:
>
>> ====
>> Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
>> submitted the following contribution:
>> ====
>>
>> Out of memory (virtual memory). The program requests a chunk of data 
>> (roughly 137MB) from the system main memory, and it is not available. 
>> Try to increase the swap size.
>>
>> Best regards,
>> Torsten Andersen.
>>
>> Li Wang wrote:
>>
>>> ====
>>> Li Wang <lwang@hrc.toyama-u.ac.jp>
>>> submitted the following contribution:
>>> ====
>>>
>>> Dear all ,
>>>
>>> The lapw1 crashed when I run "x lapw -c". The message is:
>>> "Allocate error 494: Allocation of Array with extent of 143952004 
>>> failed
>>> End of diagnostics",
>>> Can some one can tell me the possible reason.
>>>
>>> Thanks.
>>>
>>> Li Wang
>>>
>>>
>>>
>>> ====
>>> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>>> To (un)subscribe send mail to
>>> majordomo@zeus.theochem.tuwien.ac.at
>>> ====
>>>
>>>
>>
> Dear Dr. Andersen,
> Thank you for your reply. But I have 2G memory and 2G swap space. I 
> think that there should be another reason.
>
> Best regrads,
>
> Li Wang
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====




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------------------------------

Date: Thu, 19 Dec 2002 08:22:26 -0800 (PST)
From: Claudio Lee <claudio_lee1@yahoo.com>
Subject: [WIEN]: error in .dayfile

====
Claudio Lee <claudio_lee1@yahoo.com>
submitted the following contribution:
====

Dear all,
Is there anyone there knows this problem please help
me out.
My problem is: In the case.dayfile  I got something
like this:
 
>   lapw0       (18:55:26)  ABBRUCH: DIE EFG-MATRIX
IST DIE NULLMATRIX !
 ABBRUCH: DIE EFG-MATRIX IST DIE NULLMATRIX !
19.0u 0.0s 0:19 96% 0+0k 0+0io 0pf+0w
>   lapw1  -c -up       (18:55:46) 1199.0u 7.0s 20:18
98% 0+0k 0+0io 0pf+0w
>   lapw1  -c -dn       (19:16:05) 1198.0u 8.0s 20:22
98% 0+0k 0+0io 0pf+0w
>   lapwso -up -c       (19:36:27) 8986.0u 17.0s
2:31:23 99% 0+0k 0+0io 0pf+0w
>   lapw2 -c -up -so    (22:07:51) 632.0u 41.0s 11:16
99% 0+0k 0+0io 0pf+0w
>   lapw2 -c -dn -so    (22:19:07) 633.0u 46.0s 11:21
99% 0+0k 0+0io 0pf+0w
>   lcore -up   (22:30:29) 0.0u 0.0s 0:00 0% 0+0k
0+0io 0pf+0w
>   lcore -dn   (22:30:30) 0.0u 0.0s 0:00 0% 0+0k
0+0io 0pf+0w
>   mixer       (22:30:30)  INFO: LM-LIST in CLMSUM
changed in MIXER
 INFO: LM-LIST in CLMSUM changed in MIXER
 INFO: LM-LIST in CLMSUM changed in MIXER
 INFO: LM-LIST in CLMSUM changed in MIXER
 INFO: LM-LIST in CLMSUM changed in MIXER
 INFO: K-LIST in CLMSUM changed in MIXER 3
 INFO: K-LIST in CLMSUM changed in MIXER 4
 INFO: K-LIST in CLMSUM changed in MIXER 5
 INFO: K-LIST in CLMSUM changed in MIXER 6
...
...
For next iterations everything seems going well.
What does that mean as K-LIST and LM-LIST changed in
MIXER?

Thank you in advance.

Sincerely,
Claudio.


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------------------------------

End of wien-digest V2002 #48
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #49
Reply-To: wien
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wien-digest        Friday, December 27 2002        Volume 2002 : Number 049




----------------------------------------------------------------------

Date: Thu, 19 Dec 2002 15:51:25 -0500 (EST)
From: Neme Nnolim <non6886@alizarin.njit.edu>
Subject: [WIEN]: Symmetry decomposed electron density plots?

====
Neme Nnolim <non6886@alizarin.njit.edu>
submitted the following contribution:
====


Dear WIEN users,

I am interested in calculating symmetry decomposed (for example
d-eg, d-t2g) valence electron density plots. How do I go about it?
I think this question has been asked before on this mailing list,
although my search keywords do not seem to be bringing them up.


Thanks and regards,


Neme



- ------------------------------------------------------------------------------
Neme Okechukwu Nnolim
Department of Applied Physics, Material Science Program
New Jersey Institute of Technology
Room 302, Tiernan Hall, 161 Warren Street, University Heights
Newark, New Jersey 07102-1982
Tel: (973) 596-8283, FAX: (973) 596-5794
- -------------------------------------------------------------------------------


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------------------------------

Date: Fri, 20 Dec 2002 09:12:58 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Symmetry decomposed electron density plots?

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I am interested in calculating symmetry decomposed (for example
> d-eg, d-t2g) valence electron density plots. How do I go about it?
> I think this question has been asked before on this mailing list,
> although my search keywords do not seem to be bringing them up.

This is not possible. All you can do is select a specific energy range in
case.in2 and plot the density only for states in this range. And when you
analyse the partial DOS first, you might be able to separate such states
approximately.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Fri, 20 Dec 2002 09:18:29 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: error in .dayfile

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> Is there anyone there knows this problem please help
> me out.
> My problem is: In the case.dayfile  I got something
> like this:
>
> >   lapw0       (18:55:26)  ABBRUCH: DIE EFG-MATRIX
> IST DIE NULLMATRIX !
>  ABBRUCH: DIE EFG-MATRIX IST DIE NULLMATRIX !
> 19.0u 0.0s 0:19 96% 0+0k 0+0io 0pf+0w
> >   mixer       (22:30:30)  INFO: LM-LIST in CLMSUM
> changed in MIXER
>  INFO: LM-LIST in CLMSUM changed in MIXER
>  INFO: LM-LIST in CLMSUM changed in MIXER
>  INFO: LM-LIST in CLMSUM changed in MIXER
>  INFO: LM-LIST in CLMSUM changed in MIXER
>  INFO: K-LIST in CLMSUM changed in MIXER 3
>  INFO: K-LIST in CLMSUM changed in MIXER 4
>  INFO: K-LIST in CLMSUM changed in MIXER 5
>  INFO: K-LIST in CLMSUM changed in MIXER 6
> ...
> ...
> For next iterations everything seems going well.
> What does that mean as K-LIST and LM-LIST changed in
> MIXER?

You must have done something one should never do in WIEN2k:

In the directory "case" you have initialized a certain case and run scf.

After that you have changed the symmetry of your case (either by putting
different lattice parameters or by putting atoms in positions which
breaks symmetry. After that you must have "initialized" again leading
to a new LM list in case.in2, new symmetry operations in case.struct,...

But you still had an "old" clmsum file (with LMs and a K-list for the old
symmetry) and you tried to "mix" this old list with the new one.
Most likely mixer took care of that and it is ok.

Nevertheless: my recommendation is: never mix different symmetries in ONE
case.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Fri, 20 Dec 2002 19:38:34 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: supercell error

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====



Dear Prof. Blaha and W2k users

I generated using recently added utility to w2k "supercell", 3x3x3 cell of
Na(starting from 2 atom bcc cell).The target lattice chosen was P. It
generated a supercell struct file in which there are 54 Na atoms which
are all inequivalant.
and I replaced one of sodium at (1/2a, 1/2a, 1/2a) by a transition metal 
say Ti.Total 54 atoms(53 Na+ one TM). 

 using the supercell struct file, 

1) " sgroup" gave a struct file where the number of inequivalant atoms
changed from 54 to 8 due to Ti. I copied case.struct_sgroup to
case.struct.  
2)" symmetry"  struct file is also same.  
3) using "instgen_lapw" generated "case.inst" file.  
4) and continued with lstart, kgen, dstart [-up/dn]
 NO ERROR anywhere, NO WARNINGS. 
checked case.in0,case.in1, case.in2 etc. All are generated properly.

1 k-point chosen and .machines file in MPI parallel format, 4 processor 
for lapw0 and 1 kpt distribued on 4 processors.  

however, I get error:

case.dayfile:
________________________________________________________________________
    start       (Fri Dec 20 15:11:43 CST 2002) with lapw0 (20/20 to go)
>   lapw0 -p    (15:11:43) starting parallel lapw0 at Fri Dec 20 15:11:43 
CST 2002
- -------- .machine1 : 4 processors
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1
- --------
**  lapw0 crashed!
0.0u 0.2s 0:03 7% 65+461k 0+0io 0pf+0w

>   stop error
_____________________________


I checked the four case.output000* files generated it has some important 
message while generating multipole moments (in all four files)
______________________________________________________________
                              M U L T I P O L M O M E N T S
                              ------------------------------


   ATOM= 1   Ti           Z=22.00   LM= 5     POSITION=  0.500  0.500  
0.500

   L= 0   M= 0   SPHERE MM =   0.720283455  0.000000000
   L= 4   M= 0   SPHERE MM =   0.000662637  0.000000000
   L= 4   M= 4   SPHERE MM =   0.000396001  0.000000000
   L= 6   M= 0   SPHERE MM =  -0.000160274  0.000000000
   L= 6   M= 4   SPHERE MM =   0.000299845  0.000000000


   ATOM= 2   Na1          Z=11.00   LM=10     POSITION=  0.833  0.500  
0.500

 UNCORRECT LM LIST FOR CUBIC STRUCTURE
 MULTSU.F
L=   1 M=   0
_____________________________________

this error is from  SRC_lapw0/multsu.f.

the terminal output error:
_________________________________________________________________
hup: Command not found.
ERROR: 0032-184 MPI was not finalized  in routine unknown, task 1
ERROR: 0032-184 MPI was not finalized  in routine unknown, task 2
ERROR: 0032-184 MPI was not finalized  in routine unknown, task 3
ERROR: 0032-184 MPI was not finalized  in routine unknown, task 0
No match
_________________________________________________________________

I checked while compiling the code there were no complilation error and
linking error message in SRC_lapw0/compile.msg etc(SCALAPACK and BLACS
linking are then OK).

lapw0_mpi, lapw1_mpi, law2_mpi are indeed created. 

If any w2k have experience in running MPI parallel job 
with huge supercell have clue as to where I have gone wrong in the
procedure, pl. let me know.

thanx in advance

Regards
sahu

PS: If you would like to check struct and any other files, pl. let me know

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Date: Sat, 21 Dec 2002 10:31:18 +0800
From: gyguo <gyguo@phys.ntu.edu.tw>
Subject: [WIEN]: AFM calculations

====
gyguo <gyguo@phys.ntu.edu.tw>
submitted the following contribution:
====


Dear Dr. Blaha and WIEN users,

I tried to do AFM calculations for bcc Cr using runafm_lapw.
I followed the procedure in UG. However, the run was stuck after
lapw1. The run kept copying case.vectorup to case.vectordn till
the whole disc space was full, and in this way, the file "case.vectordn"
is far much large than case.vectorup.

Can anyone help to solve this problem?

Guang-Yu Guo

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------------------------------

Date: Sat, 21 Dec 2002 08:12:53 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: AFM calculations

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> I tried to do AFM calculations for bcc Cr using runafm_lapw.
> I followed the procedure in UG. However, the run was stuck after
> lapw1. The run kept copying case.vectorup to case.vectordn till
> the whole disc space was full, and in this way, the file "case.vectordn"
> is far much large than case.vectorup.
>
> Can anyone help to solve this problem?
One can after labeling the two Cr's (Cr1, Cr2) and flipping the spins also
use the runsp_lapw script: runafm_lapw script just saves the time
calculating only spin up, which for this bcc-Cr with no impurity may not be
serious.
        Your,
        S. Jalali.

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------------------------------

Date: Sat, 21 Dec 2002 17:10:35 -0800 (PST)
From: yanming Ma <ymma66@yahoo.com>
Subject: Re: [WIEN]: QTL-B = 1220.43

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-2106486406-1040519435=:79981
Content-Type: text/plain; charset=us-ascii


Dear Peter, 
> >I changed to the following
> > 0.3     5      0                          <======================
> 2      0.30        0.000    CONT 1
> 2     -5.08        0.005    STOP  1
> 0     -1.66        0.010    CONT 1
> 0      0.30        0.000    CONT 1
> 1      0.30        0.000    CONT 1
> 1     -0.60        0.010    CONT 1    ------   added line for p lo
>>
>> Using this changed Case.in1 file, the lapw1 crashed.

>Of course!!! You must change the 5 to 6 in the first line!

I changed the 5 to 6 in the first line. The lapw1 works fine. But When the runsp_lapw -up finish, I still found the warning "8 Eignvalue below the -8.0 Ry" in Case.scfup file. I aslo tried to using the following energy parameters. 

 0.3     6      0                          <======================
> 2      0.30        0.000    CONT 1
> 2     -5.08        0.005    STOP  1
> 0     -1.66        0.010    CONT 1
> 0      0.30        0.000    CONT 1
> 1      1.00        0.000    CONT 1
> 1     -0.60        0.010    CONT 1    ------   added line for p lo


I also got the similar warning in Case.scfup files.

Are there other possible reasons for this ghost band problem?

Best Wishes

 


Yanming Ma Ph.D
Steacie Institute for Molecular Sciences,
National Research Councils of Canada,
Ottawa, Ontario
K1A 0R6
Canada


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- --0-2106486406-1040519435=:79981
Content-Type: text/html; charset=us-ascii

<P>Dear Peter, 
<P>&gt; &gt;I changed to the following<BR>&gt; &gt; 0.3&nbsp;&nbsp;&nbsp;&nbsp; 5&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; &lt;======================<BR>&gt; 2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>&gt; 2&nbsp;&nbsp;&nbsp;&nbsp; -5.08&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.005&nbsp;&nbsp;&nbsp; STOP&nbsp; 1<BR>&gt; 0&nbsp;&nbsp;&nbsp;&nbsp; -1.66&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010&nbsp;&nbsp;&nbsp; CONT 1<BR>&gt; 0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>&gt; 1&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>&gt; 1&nbsp;&nbsp;&nbsp;&nbsp; -0.60&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010&nbsp;&nbsp;&nbsp; CONT 1!
&nbsp;&nbsp;&nbsp; ------&nbsp;&nbsp; added line for p lo<BR>&gt;&gt;<BR>&gt;&gt; Using this changed Case.in1 file, the lapw1 crashed.<BR><BR>&gt;Of course!!! You must change the 5 to 6 in the first line!<BR><BR>I changed the 5 to 6 in the first line. The lapw1 works fine. But When the runsp_lapw -up finish, I&nbsp;still found the warning "8 Eignvalue below the -8.0 Ry" in Case.scfup file.&nbsp;I aslo tried to using the following energy parameters.&nbsp;</P>
<P>&nbsp;0.3&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;6&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; &lt;======================<BR>&gt; 2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>&gt; 2&nbsp;&nbsp;&nbsp;&nbsp; -5.08&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.005&nbsp;&nbsp;&nbsp; STOP&nbsp; 1<BR>&gt; 0&nbsp;&nbsp;&nbsp;&nbsp; -1.66&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010&nbsp;&nbsp;&nbsp; CONT 1<BR>&gt; 0&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.30&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>&gt; 1&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;1.00&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.000&nbsp;&nbsp;&nbsp; CONT 1<BR>&gt; 1&nbsp;&nbsp;&nbsp;&nbsp; -0.60&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 0.010&nbsp;&nbsp;&nbsp; CONT 1&nbsp;&nbsp;&nbsp; ------&nbsp;&n!
bsp; added line for p lo<BR></P>
<P>I also got the similar warning in Case.scfup files.</P>
<P>Are there other possible reasons for this ghost band problem?</P>
<P>Best Wishes</P>
<P>&nbsp;</P><BR><BR>Yanming Ma Ph.D<br>Steacie Institute for Molecular Sciences,<br>National Research Councils of Canada,<br>Ottawa, Ontario<br>K1A 0R6<br>Canada<p><br><hr size=1>Do you Yahoo!?<br>
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------------------------------

Date: Sun, 22 Dec 2002 16:48:18 +0800
From: "liu wan" <wien97wan@hotmail.com>
Subject: [WIEN]: question about "iterative diagonalization"

====
"liu wan" <wien97wan@hotmail.com>
submitted the following contribution:
====

Dear WIEN users,

In order to save time, I tired to use iterative diagonalization. I run
"run_lapw -it". But after LAPW2, the program exit and report "Arguments
too long". If I run "run_lapw", everything is OK, and I can get
self-consistent.

Can anyone help me to solve this problem?

Thanks.

Liu






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Date: Sun, 22 Dec 2002 16:49:29 +0800
From: "liu wan" <wien97wan@hotmail.com>
Subject: [WIEN]: question about reference

====
"liu wan" <wien97wan@hotmail.com>
submitted the following contribution:
====


Dear all,

For the exchange-correlation potential, I had set 5 in the case.in0

which reference correspond to this choice?

Thank you in advance. Sincerely,

Liu





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Date: Mon, 23 Dec 2002 09:29:49 +0800
From: gyguo <gyguo@phys.ntu.edu.tw>
Subject: Re: [WIEN]: AFM calculations

====
gyguo <gyguo@phys.ntu.edu.tw>
submitted the following contribution:
====



Saeid Jalali ¼g¹D¡G

> ====
> "Saeid Jalali" <sjalali@cc.iut.ac.ir>
> submitted the following contribution:
> ====
>
> > I tried to do AFM calculations for bcc Cr using runafm_lapw.
> > I followed the procedure in UG. However, the run was stuck after
> > lapw1. The run kept copying case.vectorup to case.vectordn till
> > the whole disc space was full, and in this way, the file "case.vectordn"
> > is far much large than case.vectorup.
> >
> > Can anyone help to solve this problem?
> One can after labeling the two Cr's (Cr1, Cr2) and flipping the spins also
> use the runsp_lapw script: runafm_lapw script just saves the time
> calculating only spin up, which for this bcc-Cr with no impurity may not be
> serious.
>         Your,
>         S. Jalali.

Dear Dr. Jalali,

Thanks for your e-mail. I have done AF calculations for bcc Cr using
"runsp_lapw" before [PRB 62,5136 (2000)]. Here, I just wanted to see
whether "runafm_lapw" works or not since it will save substantial CPU
time. It obviously does not work for me here.

Cheers, Guang-Yu Guo

>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
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------------------------------

Date: Mon, 23 Dec 2002 08:15:14 +0330
From: "Saeid Jalali" <sjalali@cc.iut.ac.ir>
Subject: Re: [WIEN]: AFM calculations

====
"Saeid Jalali" <sjalali@cc.iut.ac.ir>
submitted the following contribution:
====

> > > I tried to do AFM calculations for bcc Cr using runafm_lapw.
> > > I followed the procedure in UG. However, the run was stuck after
> > > lapw1. The run kept copying case.vectorup to case.vectordn till
> > > the whole disc space was full, and in this way, the file
"case.vectordn"
> > > is far much large than case.vectorup.
> > > Can anyone help to solve this problem?

> > One can after labeling the two Cr's (Cr1, Cr2) and flipping the spins
also
> > use the runsp_lapw script: runafm_lapw script just saves the time
> > calculating only spin up, which for this bcc-Cr with no impurity may not
be
> > serious.

> Thanks for your e-mail. I have done AF calculations for bcc Cr using
> "runsp_lapw" before [PRB 62,5136 (2000)]. Here, I just wanted to see
> whether "runafm_lapw" works or not since it will save substantial CPU
> time. It obviously does not work for me here.

Then, did you also copy case.struct of nonmagnetic bcc-Cr (with B symmetry
and one Cr at 0 0 0) to case.struct_supergroup, where you have the
antiferromagnetic bcc-Cr (with P symmetry and two Cr's)?
        your,
        S. Jalali.

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------------------------------

Date: Mon, 23 Dec 2002 10:18:56 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: question about reference

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> For the exchange-correlation potential, I had set 5 in the case.in0
>
> which reference correspond to this choice?

Look into the Userguide!

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 23 Dec 2002 10:31:46 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: supercell error

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>    ATOM= 1   Ti           Z=22.00   LM= 5     POSITION=  0.500  0.500
> 0.500
>
>    L= 0   M= 0   SPHERE MM =   0.720283455  0.000000000
>    L= 4   M= 0   SPHERE MM =   0.000662637  0.000000000
>    L= 4   M= 4   SPHERE MM =   0.000396001  0.000000000
>    L= 6   M= 0   SPHERE MM =  -0.000160274  0.000000000
>    L= 6   M= 4   SPHERE MM =   0.000299845  0.000000000
>
>
>    ATOM= 2   Na1          Z=11.00   LM=10     POSITION=  0.833  0.500
> 0.500
>
>  UNCORRECT LM LIST FOR CUBIC STRUCTURE
>  MULTSU.F
> L=   1 M=   0

Please have a look into your struct file. It could be that sgroup has made
an error:

Compare your struct file with the output of outputs:
There it tells you for each atom the "pointgroup" and selects the LM list.
If it is a "non-cubic" atom (see UG for explanation), this atom should have
a "negative atomnumber", while if it is cubic, it should be positive.

For your output above I can see that the first atom is "cubic", i.e. in the
struct file it should have a positive counter, while the second should be
non-cubic, i.e. have a negative number.

My suggestion: Put the "number of symmetry operations" to zero (w2web)
and reinitialize starting with symmetry.

In case that my analysis is correct (and you have not made any other mistake?)
please send (to my private email) the struct file generated by
"supercell"+the replaced TM ion.

Regards


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 23 Dec 2002 18:27:23 +0800
From: "liu wan" <wien97wan@hotmail.com>
Subject: Re: [WIEN]: question about reference

====
"liu wan" <wien97wan@hotmail.com>
submitted the following contribution:
====

Dear Dr. Peter Blaha

Thank you very much for your reply.

The reference corresponding to "5" in case.in0 is "Perdew J.P. and Wang Y. 
1992, Phys.Rev. B45, 13244"?

Could you please help me to solve another problem?

In order to save time, I tired to use iterative diagonalization. I run
"run_lapw -it". But after LAPW2, the program exit and report "Arguments
too long". If I run "run_lapw", everything is OK, and I can get
self-consistent.

Thank you

Liu


>From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: <wien@zeus.theochem.tuwien.ac.at>
>Subject: Re: [WIEN]: question about reference
>Date: Mon, 23 Dec 2002 10:18:56 +0100 (MET)
>
>====
>Peter Blaha <pblaha@theochem.tuwien.ac.at>
>submitted the following contribution:
>====
>
> > For the exchange-correlation potential, I had set 5 in the case.in0
> >
> > which reference correspond to this choice?
>
>Look into the Userguide!
>
>                                       P.Blaha
>--------------------------------------------------------------------------
>Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
>Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
>Email: blaha@theochem.tuwien.ac.at    WWW: 
>http://info.tuwien.ac.at/theochem/
>--------------------------------------------------------------------------
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====


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------------------------------

Date: Mon, 23 Dec 2002 11:50:54 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: question about reference

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> In order to save time, I tired to use iterative diagonalization. I run
> "run_lapw -it". But after LAPW2, the program exit and report "Arguments
> too long". If I run "run_lapw", everything is OK, and I can get
> self-consistent.

I don't know what to do with this.

Maybe change  in run_lapw   the first line to -xf   to get
more debugging output.

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 23 Dec 2002 11:28:20 -0500
From: "Dadi Dai" <dai@unity.ncsu.edu>
Subject: [WIEN]: Error message in Bandstructure in w2web

====
"Dadi Dai" <dai@unity.ncsu.edu>
submitted the following contribution:
====

I met an error message when I was using w2web to generate
bandstructure.  I click "x lapw1 -band -up", and then an
error appears:

if - Malformed file inquiry

I don't know where this error comes from.  The wien2k
package that I am using was downloaded on Nov. 5.  I haven't
seen any update on lapw1 on the update info list since then.

As I remembered, the previous versions of wien2k doesn't
have such problem.  Unfortunately, however, I haven't kept
the old versions.

Could anyone help me?

Thank you very much!

Dadi Dai

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------------------------------

Date: Tue, 24 Dec 2002 14:07:29 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: MPI parallel

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear W2k users

I have a problem in running MPI parallel job(54 atom cell, 1 k-point, 
.machines file in MPI parallel format). initialization is correct(ie 
correct struct and other files).

the Machine is SP4 with 4 nodes each node having 16 POWER4 
processors(shared memory machine).

With 1 k-point, .machines file in MPI parallel format

lapw0:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
longhorn1:1 longhorn1:1 longhorn1:1
1:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
longhorn1:1 longhorn1:1
granularity:1
(8 processors for laow0 and 8 processors for 1 k-point MPI parallel) 

I launched the job on SP4.

the dayfile:

    start       (Tue Dec 24 12:06:03 CST 2002) with lapw0 (20/20 to go) 
>   lapw0 -p    (12:06:03) starting parallel lapw0 at Tue Dec 24 12:06:03
CST 2002
- -------- .machine1 : 8 processors
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1  
longhorn1:1
longhorn1:1
- --------
0.0u 0.1s 0:50 0% 101+829k 0+0io 0pf+0w
>   lapw1  -up -p       (12:06:53) starting parallel lapw1 at Tue Dec 24
12:06:54 CST 2002
- ->  starting parallel LAPW1 jobs at Tue Dec 24 12:06:54 CST 2002
running LAPW1 in parallel mode (using .machines)
1 number_of_parallel_jobs
[1] 52146
________________________

As you can see lapw0 now passes smoothly. I checked the case.output000*
files. No error message like I was getting before. BUT at lapw1 -up it
spends enormous amount of time. I waited for 24 hours but nothing is
written to Na.output1_up and does not stop with any error. It seems it
stuck at lapw1 -up.

What it is waiting for?It should not take so much time in my opinion to
complete even a subpart of 1st iteration. I have the executables
lapw0_mpi, lapw1_mpi etc. On such fast machine(I have tested 54 atom using
VASP, another MPI parallel code and very efficiently), the on-node(ie I am 
using only 1 node
with 8 processors here longhorn1 is 1 node with 8 processors)
 communication is done by high performance dual-plane SP switch 2
interconnect rather than ethernet GigE networks. so communication between
the processors on the given node(here longhorn1) is really very fast and
may not be cause of the problem. lapw0_mpi, lapw1_mpi,lapw2_mpi etc
are created properly without any error in compile.msg during compilation 
and linking.

I suspected whether it is waiting for passwd on longhorn1(It should not as
it is a shared memory machine). so I put .rhosts file with the longhorn1
node in it. but no success.

I have done 13 atoms cell with different k-point mesh in k-point parallel
mode on the same machine. there is no problem.

thank you in advance for your suggestion/s.


Regards
sahu

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------------------------------

Date: Tue, 24 Dec 2002 16:01:13 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: MPI parallel 

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear W2k users

I have a problem in running MPI parallel job(54 atom cell, 1 k-point, 
.machines file in MPI parallel format). initialization is correct(ie 
correct struct and other files).

the Machine is SP4 with 4 nodes each node having 16 POWER4 
processors(shared memory machine).

With 1 k-point, .machines file in MPI parallel format

lapw0:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
longhorn1:1 longhorn1:1 longhorn1:1
1:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
longhorn1:1 longhorn1:1
granularity:1
(8 processors for laow0 and 8 processors for 1 k-point MPI parallel) 

I launched the job on SP4.

the dayfile:

    start       (Tue Dec 24 12:06:03 CST 2002) with lapw0 (20/20 to go) 
>   lapw0 -p    (12:06:03) starting parallel lapw0 at Tue Dec 24 12:06:03
CST 2002
- -------- .machine1 : 8 processors
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1  
longhorn1:1
longhorn1:1
- --------
0.0u 0.1s 0:50 0% 101+829k 0+0io 0pf+0w
>   lapw1  -up -p       (12:06:53) starting parallel lapw1 at Tue Dec 24
12:06:54 CST 2002
- ->  starting parallel LAPW1 jobs at Tue Dec 24 12:06:54 CST 2002
running LAPW1 in parallel mode (using .machines)
1 number_of_parallel_jobs
[1] 52146
________________________

As you can see lapw0 now passes smoothly. I checked the case.output000*
files. No error message like I was getting before. BUT at lapw1 -up it
spends enormous amount of time. I waited for 24 hours but nothing is
written to Na.output1_up and does not stop with any error. It seems it
stuck at lapw1 -up.

What it is waiting for?It should not take so much time in my opinion to
complete even a subpart of 1st iteration. I have the executables
lapw0_mpi, lapw1_mpi etc. On such fast machine(I have tested 54 atom using
VASP, another MPI parallel code and very efficiently), the on-node(ie I am 
using only 1 node
with 8 processors here longhorn1 is 1 node with 8 processors)
 communication is done by high performance dual-plane SP switch 2
interconnect rather than ethernet GigE networks. so communication between
the processors on the given node(here longhorn1) is really very fast and
may not be cause of the problem. lapw0_mpi, lapw1_mpi,lapw2_mpi etc
are created properly without any error in compile.msg during compilation 
and linking.

I suspected whether it is waiting for passwd on longhorn1(It should not as
it is a shared memory machine). so I put .rhosts file with the longhorn1
node in it. but no success.

I have done 13 atoms cell with different k-point mesh in k-point parallel
mode on the same machine. there is no problem.

thank you in advance for your suggestion/s.


Regards
sahu


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------------------------------

Date: Wed, 25 Dec 2002 04:16:44 -0800 (PST)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: instal 

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====

Dear wien Users
I  want instal the WIEN2k_02-executables.tar.gz
Package.
would you please Write step by step  with details of
installing WIEN2k_02-executables.tar.gz 
  best wishes


=====
Hamdollah Salehi
Dept of Physics
Ferdowsi University
Mashhad IRAN
Post boxs 1436
Post code 91775
faxs

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------------------------------

Date: Wed, 25 Dec 2002 05:52:03 -0800 (PST)
From: hamid salehi <salehihamid@yahoo.com>
Subject: [WIEN]: install

====
hamid salehi <salehihamid@yahoo.com>
submitted the following contribution:
====


 Dear wien Users
 I  want instal the WIEN2k_02-executables.tar.gz
 Package.
 would you please Write step by step  with details of
 installing WIEN2k_02-executables.tar.gz 
   best wishes
 
 
 =====
 Hamdollah Salehi
 Dept of Physics
 Ferdowsi University
 Mashhad IRAN
 Post boxs 1436
 Post code 91775
 faxs
 
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- --------DreamInTech.nfra21WAS2.Mail.Engine3e09ace042433--


=====
Hamdollah Salehi
Dept of Physics
Ferdowsi University
Mashhad IRAN
Post boxs 1436
Post code 91775
faxs

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------------------------------

Date: Thu, 26 Dec 2002 01:56:06 +0000
From: ecat@nfrn-mail.org.uk
Subject: [WIEN]: The problem about Etop and Ebottom

====
ecat@nfrn-mail.org.uk
submitted the following contribution:
====

Dear friends,

I have some difficulty in running Wien2k.Could you please give 
any help? The problem is:

In uplapw1.error,there is something like:
 'SELECT' - no energy limits found for L= 1
 'SELECT' - E-bottom    1.97000   E-top -200.00000

In my case.in1,there are lines like:
WFFIL        (WFPRI, SUPWF)
  7.00       10    4 (R-MT*K-MAX; MAX L IN WF, V-NMT
  0.30    4  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, 
global APW/LAPW)
 0    0.30      0.000 CONT 1
 0   -5.57      0.005 CONT 1
 1    0.30      0.000 CONT 1
 1   -3.12      0.005 STOP 1
  0.30    5  0      (GLOBAL E-PARAMETER WITH n OTHER CHOICES, 
global APW/LAPW)
 0    0.30      0.000 CONT 1
 0   -7.93      0.005 CONT 1
 1    0.30      0.000 CONT 1
 1   -4.96      0.005 STOP 1
 2    0.30      0.010 CONT 1
K-VECTORS FROM UNIT:4  -10.0       1.5      emin/emax window

If the Etop or the Ebottom for l=1 cannot be found,the scf cycle 
will stop. How to solve this problem? If the Etop or the Ebottom 
cannot be found,how to make the scf program run well?

Thanks a lot!

Yours,
Ecat


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------------------------------

Date: Wed, 25 Dec 2002 21:18:23 -0800
From: "aparna chakrabarti" <chakrabarti@lycos.com>
Subject: [WIEN]: (No Subject)

====
"aparna chakrabarti" <chakrabarti@lycos.com>
submitted the following contribution:
====

Has anyone simulated the NiAs phase for some
binary semiconductors? I get the wurtzite phase 
right, lattice constant and bulk modulus. For 
NiAs lattice constant is fine but bulk modulus 
is almost doubled. Does anyone have an answer?!
Thanks in advance. Regards
Aparna


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------------------------------

Date: Thu, 26 Dec 2002 08:54:23 -0500
From: "Dadi Dai" <dai@unity.ncsu.edu>
Subject: [WIEN]: w2web, Bandstructure, Error Message

====
"Dadi Dai" <dai@unity.ncsu.edu>
submitted the following contribution:
====

I met an error message when I was using w2web to generate
bandstructure.  I click "x lapw1 -band -up", and then an
error appears:

if - Malformed file inquiry

I don't know where this error comes from.  The wien2k
package that I am using was downloaded on Nov. 5.  I haven't
seen any update on lapw1 on the update info list since then.

As I remembered, the previous versions of wien2k doesn't
have such problem.  Unfortunately, however, I haven't kept
the old versions.

Could anyone help me?

Thank you very much!

Dadi Dai


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------------------------------

Date: Thu, 26 Dec 2002 21:52:50 +0800
From: "liu wan" <wien97wan@hotmail.com>
Subject: [WIEN]: question about c/a in "OPTIMIZE"

====
"liu wan" <wien97wan@hotmail.com>
submitted the following contribution:
====

Dear all,

Merry X'mas & Happy new year!

I try to use "OPTIMIZE" to change c/a. By runing "OPTIMIZE" I get several 
file.

D-V=-12_initial.struct
10.836754  9.571427 17.740615 93.069000 90.000000 90.000000

D-V=-12_coa___1.5.struct
10.345935 10.345935 17.191161 93.069000 90.000000 90.000000

D-V=-12_coa___3.0.struct
10.295466 10.295466 17.360118 93.069000 90.000000 90.000000

I am very surprised that, in the initial structure lattice parameter a is 
not equal to b, but in the other two file a is equal to b! Another question 
is: when I run optimize, I input c/a increase 3%, then I get 
D-V=-12_coa___3.0.struct. But the c/a in D-V=-12_initial.struct is 1.637, 
the c/a in D-V=-12_initial.struct is 1.686!

Who can tell me the rule about changing c/a in "OPTIMIZE"?

Thank you in advance. Sincerely,

Liu


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------------------------------

Date: Thu, 26 Dec 2002 22:40:13 +0530
From: "R.K.Thapa" <rktt@sancharnet.in>
Subject: [WIEN]: greetings

====
"R.K.Thapa" <rktt@sancharnet.in>
submitted the following contribution:
====

To all WIEN users, Happy XMAS and New Year.
R.K.Thapa
=============
Condensed Matter Theory Research Group
Department of Physics
Pachhunga University College
Mizoram University
Aizawl 796 001 Mizroam
India
Ph. No. 0091-0389-2328044
FAX : 0091-0389-2323491
E-mails : rktt@sancharnet.in
              ramkumar_thapa@yahoo.com



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------------------------------

Date: Thu, 26 Dec 2002 12:55:07 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: MPI parallel 

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear W2k users

I have a problem in running MPI parallel job(54 atom cell, 1 k-point, 
.machines file in MPI parallel format). initialization is correct(ie 
correct struct and other files).

the Machine is SP4 with 4 nodes each node having 16 POWER4 
processors(shared memory machine).

With 1 k-point, .machines file in MPI parallel format

lapw0:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
longhorn1:1 longhorn1:1 longhorn1:1
1:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
longhorn1:1 longhorn1:1
granularity:1
(8 processors for laow0 and 8 processors for 1 k-point MPI parallel) 

I launched the job on SP4.

the dayfile:

    start       (Tue Dec 24 12:06:03 CST 2002) with lapw0 (20/20 to go) 
>   lapw0 -p    (12:06:03) starting parallel lapw0 at Tue Dec 24 12:06:03
CST 2002
- -------- .machine1 : 8 processors
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1
longhorn1:1  
longhorn1:1
longhorn1:1
- --------
0.0u 0.1s 0:50 0% 101+829k 0+0io 0pf+0w
>   lapw1  -up -p       (12:06:53) starting parallel lapw1 at Tue Dec 24
12:06:54 CST 2002
- ->  starting parallel LAPW1 jobs at Tue Dec 24 12:06:54 CST 2002
running LAPW1 in parallel mode (using .machines)
1 number_of_parallel_jobs
[1] 52146
________________________

As you can see lapw0 now passes smoothly. I checked the case.output000*
files. No error message like I was getting before. BUT at lapw1 -up it
spends enormous amount of time. I waited for 24 hours but nothing is
written to Na.output1_up and does not stop with any error. It seems it
stuck at lapw1 -up.

What it is waiting for?It should not take so much time in my opinion to
complete even a subpart of 1st iteration. I have the executables
lapw0_mpi, lapw1_mpi etc. On such fast machine(I have tested 54 atom using
VASP, another MPI parallel code and very efficiently), the on-node(ie I am 
using only 1 node
with 8 processors here longhorn1 is 1 node with 8 processors)
 communication is done by high performance dual-plane SP switch 2
interconnect rather than ethernet GigE networks. so communication between
the processors on the given node(here longhorn1) is really very fast and
may not be cause of the problem. lapw0_mpi, lapw1_mpi,lapw2_mpi etc
are created properly without any error in compile.msg during compilation 
and linking.

I suspected whether it is waiting for passwd on longhorn1(It should not as
it is a shared memory machine). so I put .rhosts file with the longhorn1
node in it. but no success.

I have tested 13 atoms cell with 1 k-point mesh MPI mode on the same
machine.but the same problem. it stucks at lapw1. However, it 
doesnot give any problem wiht k-point parallel mode.

thank you in advance for your suggestion/s.


Regards
sahu


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------------------------------

Date: Thu, 26 Dec 2002 20:08:24 +0100 (MET)
From: Gilles Hug <hug@onera.fr>
Subject: Re: [WIEN]: question about c/a in "OPTIMIZE"

====
Gilles Hug <hug@onera.fr>
submitted the following contribution:
====

Hi,
Happy New Year Wienners.

I think the script optimize uses the cell parameters of the
case_initial.struct file to compute a change from this value by the
percentage you specify. It doesn't use the case.struct file. So if you
want to make several c/a variation with several starting volume you have
to copy the case.struct file to the case_initial.struct file.
And, of course, you need to keep trace of what you are doing! :)
Best
Gilles


On Thu, 26 Dec 2002, liu wan wrote:

> ====
> "liu wan" <wien97wan@hotmail.com>
> submitted the following contribution:
> ====
>
> Dear all,
>
> Merry X'mas & Happy new year!
>
> I try to use "OPTIMIZE" to change c/a. By runing "OPTIMIZE" I get several
> file.
>
> D-V=-12_initial.struct
> 10.836754  9.571427 17.740615 93.069000 90.000000 90.000000
>
> D-V=-12_coa___1.5.struct
> 10.345935 10.345935 17.191161 93.069000 90.000000 90.000000
>
> D-V=-12_coa___3.0.struct
> 10.295466 10.295466 17.360118 93.069000 90.000000 90.000000
>
> I am very surprised that, in the initial structure lattice parameter a is
> not equal to b, but in the other two file a is equal to b! Another question
> is: when I run optimize, I input c/a increase 3%, then I get
> D-V=-12_coa___3.0.struct. But the c/a in D-V=-12_initial.struct is 1.637,
> the c/a in D-V=-12_initial.struct is 1.686!
>
> Who can tell me the rule about changing c/a in "OPTIMIZE"?
>
> Thank you in advance. Sincerely,
>
> Liu
>
>
> _________________________________________________________________
> MSN 8 limited-time offer: Join now and get 3 months FREE*.
> http://join.msn.com/?page=dept/dialup&xAPID=42&PS=47575&PI=7324&DI=7474&SU=
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------------------------------

Date: Fri, 27 Dec 2002 10:15:07 +0800
From: "liu wan" <wien97wan@hotmail.com>
Subject: Re: [WIEN]: question about c/a in "OPTIMIZE"

====
"liu wan" <wien97wan@hotmail.com>
submitted the following contribution:
====

Dear Dr. Gilles Hug

Thank you very much for your reply!

Yes, the program use the initial.struct as the origin file. My initial file 
has a=10.836754, b=9.571427l and c=17.740615, and I set the change of c/a is 
1.5% and 3.0%, but from the file coa___1.5.struct, and coa___3.0.struct, I 
found that a=b in these two file!!! And the c/a=1.637 in inital.struct, but 
is 1.661 in coa___1.5.struct and c/a is 1.686 in coa___3.0.struct! I want to 
know the rule of changing c/a in "OPTIMIZE".

Best wish

liu

>From: Gilles Hug <hug@onera.fr>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: <wien@zeus.theochem.tuwien.ac.at>
>Subject: Re: [WIEN]: question about c/a in "OPTIMIZE"
>Date: Thu, 26 Dec 2002 20:08:24 +0100 (MET)
>
>====
>Gilles Hug <hug@onera.fr>
>submitted the following contribution:
>====
>
>Hi,
>Happy New Year Wienners.
>
>I think the script optimize uses the cell parameters of the
>case_initial.struct file to compute a change from this value by the
>percentage you specify. It doesn't use the case.struct file. So if you
>want to make several c/a variation with several starting volume you have
>to copy the case.struct file to the case_initial.struct file.
>And, of course, you need to keep trace of what you are doing! :)
>Best
>Gilles
>
>
>On Thu, 26 Dec 2002, liu wan wrote:
>
> > ====
> > "liu wan" <wien97wan@hotmail.com>
> > submitted the following contribution:
> > ====
> >
> > Dear all,
> >
> > Merry X'mas & Happy new year!
> >
> > I try to use "OPTIMIZE" to change c/a. By runing "OPTIMIZE" I get 
>several
> > file.
> >
> > D-V=-12_initial.struct
> > 10.836754  9.571427 17.740615 93.069000 90.000000 90.000000
> >
> > D-V=-12_coa___1.5.struct
> > 10.345935 10.345935 17.191161 93.069000 90.000000 90.000000
> >
> > D-V=-12_coa___3.0.struct
> > 10.295466 10.295466 17.360118 93.069000 90.000000 90.000000
> >
> > I am very surprised that, in the initial structure lattice parameter a 
>is
> > not equal to b, but in the other two file a is equal to b! Another 
>question
> > is: when I run optimize, I input c/a increase 3%, then I get
> > D-V=-12_coa___3.0.struct. But the c/a in D-V=-12_initial.struct is 
>1.637,
> > the c/a in D-V=-12_initial.struct is 1.686!
> >
> > Who can tell me the rule about changing c/a in "OPTIMIZE"?
> >
> > Thank you in advance. Sincerely,
> >
> > Liu
> >
> >
> > _________________________________________________________________
> > MSN 8 limited-time offer: Join now and get 3 months FREE*.
> > 
>http://join.msn.com/?page=dept/dialup&xAPID=42&PS=47575&PI=7324&DI=7474&SU=
> > 
>http://www.hotmail.msn.com/cgi-bin/getmsg&HL=1216hotmailtaglines_newmsn8ishere_3mf
> >
> > ====
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> > To (un)subscribe send mail to
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> > ====
> >
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------------------------------

End of wien-digest V2002 #49
****************************

From: owner-wien-digest@theochem.tuwien.ac.at (wien-digest)
To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #50
Reply-To: wien
Sender: owner-wien-digest@theochem.tuwien.ac.at
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Precedence: bulk


wien-digest         Friday, January 3 2003         Volume 2002 : Number 050




----------------------------------------------------------------------

Date: Fri, 27 Dec 2002 23:27:58 +0800
From: "liu wan" <wien97wan@hotmail.com>
Subject: Re: [WIEN]: question about c/a in "OPTIMIZE"

====
"liu wan" <wien97wan@hotmail.com>
submitted the following contribution:
====

Dear all,

Who can tell me the rule of of changing c/a in "OPTIMIZE"?

Set 3% means the the c/a ratio will increase 3%, it is right? When c/a 
change, the b/a will also change???

When lattice constant a is not equal to b in the initial structure file, if 
I change c/a ratio using "OPTIMIZE", the a will equal to b!

Who can tell me? Thank you.

Liu


>From: "liu wan" <wien97wan@hotmail.com>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: wien@zeus.theochem.tuwien.ac.at
>Subject: Re: [WIEN]: question about c/a in "OPTIMIZE"
>Date: Fri, 27 Dec 2002 10:15:07 +0800
>
>====
>"liu wan" <wien97wan@hotmail.com>
>submitted the following contribution:
>====
>
>Dear Dr. Gilles Hug
>
>Thank you very much for your reply!
>
>Yes, the program use the initial.struct as the origin file. My initial file 
>has a=10.836754, b=9.571427l and c=17.740615, and I set the change of c/a 
>is 1.5% and 3.0%, but from the file coa___1.5.struct, and coa___3.0.struct, 
>I found that a=b in these two file!!! And the c/a=1.637 in inital.struct, 
>but is 1.661 in coa___1.5.struct and c/a is 1.686 in coa___3.0.struct! I 
>want to know the rule of changing c/a in "OPTIMIZE".
>
>Best wish
>
>liu
>
>>From: Gilles Hug <hug@onera.fr>
>>Reply-To: wien@zeus.theochem.tuwien.ac.at
>>To: <wien@zeus.theochem.tuwien.ac.at>
>>Subject: Re: [WIEN]: question about c/a in "OPTIMIZE"
>>Date: Thu, 26 Dec 2002 20:08:24 +0100 (MET)
>>
>>====
>>Gilles Hug <hug@onera.fr>
>>submitted the following contribution:
>>====
>>
>>Hi,
>>Happy New Year Wienners.
>>
>>I think the script optimize uses the cell parameters of the
>>case_initial.struct file to compute a change from this value by the
>>percentage you specify. It doesn't use the case.struct file. So if you
>>want to make several c/a variation with several starting volume you have
>>to copy the case.struct file to the case_initial.struct file.
>>And, of course, you need to keep trace of what you are doing! :)
>>Best
>>Gilles
>>
>>
>>On Thu, 26 Dec 2002, liu wan wrote:
>>
>> > ====
>> > "liu wan" <wien97wan@hotmail.com>
>> > submitted the following contribution:
>> > ====
>> >
>> > Dear all,
>> >
>> > Merry X'mas & Happy new year!
>> >
>> > I try to use "OPTIMIZE" to change c/a. By runing "OPTIMIZE" I get 
>>several
>> > file.
>> >
>> > D-V=-12_initial.struct
>> > 10.836754  9.571427 17.740615 93.069000 90.000000 90.000000
>> >
>> > D-V=-12_coa___1.5.struct
>> > 10.345935 10.345935 17.191161 93.069000 90.000000 90.000000
>> >
>> > D-V=-12_coa___3.0.struct
>> > 10.295466 10.295466 17.360118 93.069000 90.000000 90.000000
>> >
>> > I am very surprised that, in the initial structure lattice parameter a 
>>is
>> > not equal to b, but in the other two file a is equal to b! Another 
>>question
>> > is: when I run optimize, I input c/a increase 3%, then I get
>> > D-V=-12_coa___3.0.struct. But the c/a in D-V=-12_initial.struct is 
>>1.637,
>> > the c/a in D-V=-12_initial.struct is 1.686!
>> >
>> > Who can tell me the rule about changing c/a in "OPTIMIZE"?
>> >
>> > Thank you in advance. Sincerely,
>> >
>> > Liu
>> >
>> >
>> > _________________________________________________________________
>> > MSN 8 limited-time offer: Join now and get 3 months FREE*.
>> > 
>>http://join.msn.com/?page=dept/dialup&xAPID=42&PS=47575&PI=7324&DI=7474&SU=
>> > 
>>http://www.hotmail.msn.com/cgi-bin/getmsg&HL=1216hotmailtaglines_newmsn8ishere_3mf
>> >
>> > ====
>> > WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>> > To (un)subscribe send mail to
>> > majordomo@zeus.theochem.tuwien.ac.at
>> > ====
>> >
>>
>>====
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------------------------------

Date: Fri, 27 Dec 2002 17:35:45 +0100 (MEZ)
From: "A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
Subject: Re: [WIEN]: question about c/a in "OPTIMIZE"

====
"A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
submitted the following contribution:
====

Addressing the "mistery" of changing C/A in "optimize":

Without a fresh look into the "optimize" script - that used to be
quite straightforward - I'd guess that the option of changing
C/A assumes you have tetragonal (or, hex or rhombo) structure,
i.e., lattice parameters A A C, that's why the script forces
B=A in your case. This makes sense because
if your structure is orthorhombic the script doesn't know
what you want to do with the third parameter - keep it fixed?
Scale along with A? Or with C? That is an example of situation
where the user has better to understand what he/she is doing.
For optimizing the structure you'd need to vary all three
parameters in some way, for each trial volume, that makes
TWO independent parameters to vary, and not just C/A.
A foolproof advice: prepare a sequence of struct files
by hand, varying the parameters in a way (and within limits)
that make sense for your structure, for example changing
A and B independently so as to keep A*B*C=const,
then fit the total energy as function of these two variables to find
the local minimum for the given volume, refine if necessary, etc.
And don't forget, if you have internal coordinates you must
in principle vary them simultaneously...

Hopefully it helps,

Andrei Postnikov
 +----------  Dr. habil. Andrei Postnikov  -----  apostnik@uos.de  ----------+
 | Universitaet Osnabrueck - Fachbereich Physik, D-49069 Osnabrueck, Germany |
 +----------  Tel. +49-541-9692377  -------  Fax  +49-541-9692351  ----------+

> ====
> "liu wan" <wien97wan@hotmail.com>
> submitted the following contribution:
> ====
>
> Dear Dr. Gilles Hug
>
> Thank you very much for your reply!
>
> Yes, the program use the initial.struct as the origin file. My initial file
> has a=10.836754, b=9.571427l and c=17.740615, and I set the change of c/a is
> 1.5% and 3.0%, but from the file coa___1.5.struct, and coa___3.0.struct, I
> found that a=b in these two file!!! And the c/a=1.637 in inital.struct, but
> is 1.661 in coa___1.5.struct and c/a is 1.686 in coa___3.0.struct! I want to
> know the rule of changing c/a in "OPTIMIZE".
>
> Best wish
>
> liu
>

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------------------------------

Date: Fri, 27 Dec 2002 12:31:58 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: "orb" error

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear W2k users

         I have a magnetic system containing Mo atoms where orbital
potentials are important for the correct physics. So first I did scf LSDA
calculation without SO. Then initso_lapw step produced the proper files
with case.inso. I have case.indmc(the system dont have inversion symmetry)
and case.inorb file(the mode is LDA+U). I used "runsp_lapw -so -orb" to
introduce the orbital potential selfconsistencly with SO into the
system.It always stops at second iteration WITHOUT any errors. There are
no errors in any step in the first iteration.I checked all case.error
files.  the dayfile is:

____________________________________________________________________________________
the first iteration is OK as :log file shows:

19/19 to go

>   lapw0 -p    (19:25:14) starting parallel lapw0 at Thu Dec 26 19:25:14 
CST 2002
- --------
running lapw0 in single mode
33.9u 0.3s 0:34 98% 371+51469k 0+0io 0pf+0w
>   orb -up -p  (19:25:49) 0.0u 0.0s 0:00 0% 0+0k 0+0io 19pf+0w
>   orb -dn -p  (19:25:49) 0.0u 0.0s 0:00 10% 0+0k 0+0io 0pf+0w
__________________________________________________________________________________________

the :log file:

>   (runsp_lapw) options: -so -orb -p
Thu Dec 26 18:50:49 CST 2002> (x) lapw0 -p
Thu Dec 26 18:51:15 CST 2002> (x) lapw1 -c -up -p
Thu Dec 26 19:01:57 CST 2002> (x) lapw1 -c -dn -p
Thu Dec 26 19:12:35 CST 2002> (x) lapwso -up -c -orb -p
Thu Dec 26 19:19:59 CST 2002> (x) lapw2 -c -up -so -p
Thu Dec 26 19:22:06 CST 2002> (x) sumpara -up -d
Thu Dec 26 19:22:08 CST 2002> (x) sumpara_vresp -up -d
Thu Dec 26 19:22:09 CST 2002> (x) lapw2 -c -dn -so -p
Thu Dec 26 19:24:17 CST 2002> (x) sumpara -dn -d
Thu Dec 26 19:24:19 CST 2002> (x) sumpara_vresp -dn -d
Thu Dec 26 19:24:20 CST 2002> (x) lapwdm -up -p -so -c
Thu Dec 26 19:25:06 CST 2002> (x) sumpara -du -d
Thu Dec 26 19:25:07 CST 2002> (x) lcore -up
Thu Dec 26 19:25:07 CST 2002> (x) lcore -dn
Thu Dec 26 19:25:09 CST 2002> (x) mixer
Thu Dec 26 19:25:14 CST 2002> (x) lapw0 -p
Thu Dec 26 19:25:49 CST 2002> (x) orb -up -p
Thu Dec 26 19:25:49 CST 2002> (x) orb -dn -p
_________________________________________________________


the terminal output is:
___________________________________________________________________
in cycle 2    ETEST: 106.6573260000000000   CTEST: 1.8484003
hup: Command not found.
STOP  LAPW0 END
STOP  ORB   END
STOP  ORB   END
if: Badly formed number.---> it stops here
_____________________________________________________________

While initializing the system for SO using initso_lapw, at somepoint
of the procedure, it asks whether

Do you want to rerun kgen ? (y/N)

If I say yes, with the same k-point info as in the previous step then
it runs x kgen -so and again asks

Do you want to rerun kgen ? (y/N)

this time If I say 'No' then it stops with

if: Badly formed number

if I say again it continues again, and again, and again. How to get out of 
the loop?

surprisingly the same message "if: Badly formed number" appears in the
terminal output file above before the execution stops!!

If any W2k user have experienced simillar problem/ have suggestions, Pl. 
let me know.

thanking you in advance.

Regards
sahu

PS: If any W2k user wish to see the struct or any other file pl. let me 
know.



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------------------------------

Date: Sat, 28 Dec 2002 14:06:02 +0800
From: "liu wan" <wien97wan@hotmail.com>
Subject: Re: [WIEN]: question about c/a in "OPTIMIZE"

====
"liu wan" <wien97wan@hotmail.com>
submitted the following contribution:
====

Dear Dr. A. Postnikov

Thank you

Liu

>From: "A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
>Reply-To: wien@zeus.theochem.tuwien.ac.at
>To: wien@zeus.theochem.tuwien.ac.at
>Subject: Re: [WIEN]: question about c/a in "OPTIMIZE"
>Date: Fri, 27 Dec 2002 17:35:45 +0100 (MEZ)
>
>====
>"A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
>submitted the following contribution:
>====
>
>Addressing the "mistery" of changing C/A in "optimize":
>
>Without a fresh look into the "optimize" script - that used to be
>quite straightforward - I'd guess that the option of changing
>C/A assumes you have tetragonal (or, hex or rhombo) structure,
>i.e., lattice parameters A A C, that's why the script forces
>B=A in your case. This makes sense because
>if your structure is orthorhombic the script doesn't know
>what you want to do with the third parameter - keep it fixed?
>Scale along with A? Or with C? That is an example of situation
>where the user has better to understand what he/she is doing.
>For optimizing the structure you'd need to vary all three
>parameters in some way, for each trial volume, that makes
>TWO independent parameters to vary, and not just C/A.
>A foolproof advice: prepare a sequence of struct files
>by hand, varying the parameters in a way (and within limits)
>that make sense for your structure, for example changing
>A and B independently so as to keep A*B*C=const,
>then fit the total energy as function of these two variables to find
>the local minimum for the given volume, refine if necessary, etc.
>And don't forget, if you have internal coordinates you must
>in principle vary them simultaneously...
>
>Hopefully it helps,
>
>Andrei Postnikov
>  +----------  Dr. habil. Andrei Postnikov  -----  apostnik@uos.de  
>----------+
>  | Universitaet Osnabrueck - Fachbereich Physik, D-49069 Osnabrueck, 
>Germany |
>  +----------  Tel. +49-541-9692377  -------  Fax  +49-541-9692351  
>----------+
>
> > ====
> > "liu wan" <wien97wan@hotmail.com>
> > submitted the following contribution:
> > ====
> >
> > Dear Dr. Gilles Hug
> >
> > Thank you very much for your reply!
> >
> > Yes, the program use the initial.struct as the origin file. My initial 
>file
> > has a=10.836754, b=9.571427l and c=17.740615, and I set the change of 
>c/a is
> > 1.5% and 3.0%, but from the file coa___1.5.struct, and coa___3.0.struct, 
>I
> > found that a=b in these two file!!! And the c/a=1.637 in inital.struct, 
>but
> > is 1.661 in coa___1.5.struct and c/a is 1.686 in coa___3.0.struct! I 
>want to
> > know the rule of changing c/a in "OPTIMIZE".
> >
> > Best wish
> >
> > liu
> >
>
>====
>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====


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------------------------------

Date: Sat, 28 Dec 2002 19:08:55 +0800
From: =?gb2312?B?1dQg1r684Q==?= <zzj_fd@hotmail.com>
Subject: [none]

====
=?gb2312?B?1dQg1r684Q==?= <zzj_fd@hotmail.com>
submitted the following contribution:
====



Dear sir:
   I want to know the detail choices in the "init_lapw" of TiO2, which 
supplied 
by WIEN2k. Because I can't get the same result that supported by the 
TiO2.scf file of the example TiO2.
   In addition, can you give me a ferromagnetic surface calculation example 
which includes the main file and detail choice in initialization, such as 
Fe(100) or (110) surface.
   Thank you very much in advance.
Best regards.
                                                       J.Zhao
                                                       28/12/2002/


_________________________________________________________________
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------------------------------

Date: Sat, 28 Dec 2002 07:08:01 -0800 (PST)
From: sayede adlane <dft22000@yahoo.fr>
Subject: Re: [WIEN]: question about c/a in "OPTIMIZE"

====
sayede adlane <dft22000@yahoo.fr>
submitted the following contribution:
====

Hi, I guess that you have to update your optimize and
w2web.  Doing that you can use the "new" optimize
script to vary c/a or b/a with v=cst for orthorhombic
structure.

Adlane
Best wish

 
 
- --- liu wan <wien97wan@hotmail.com> wrote:
> ====
> "liu wan" <wien97wan@hotmail.com>
> submitted the following contribution:
> ====
> 
> Dear Dr. A. Postnikov
> 
> Thank you
> 
> Liu
> 
> >From: "A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
> >Reply-To: wien@zeus.theochem.tuwien.ac.at
> >To: wien@zeus.theochem.tuwien.ac.at
> >Subject: Re: [WIEN]: question about c/a in
> "OPTIMIZE"
> >Date: Fri, 27 Dec 2002 17:35:45 +0100 (MEZ)
> >
> >====
> >"A. Postnikov" <postnik@thp.Uni-Duisburg.DE>
> >submitted the following contribution:
> >====
> >
> >Addressing the "mistery" of changing C/A in
> "optimize":
> >
> >Without a fresh look into the "optimize" script -
> that used to be
> >quite straightforward - I'd guess that the option
> of changing
> >C/A assumes you have tetragonal (or, hex or rhombo)
> structure,
> >i.e., lattice parameters A A C, that's why the
> script forces
> >B=A in your case. This makes sense because
> >if your structure is orthorhombic the script
> doesn't know
> >what you want to do with the third parameter - keep
> it fixed?
> >Scale along with A? Or with C? That is an example
> of situation
> >where the user has better to understand what he/she
> is doing.
> >For optimizing the structure you'd need to vary all
> three
> >parameters in some way, for each trial volume, that
> makes
> >TWO independent parameters to vary, and not just
> C/A.
> >A foolproof advice: prepare a sequence of struct
> files
> >by hand, varying the parameters in a way (and
> within limits)
> >that make sense for your structure, for example
> changing
> >A and B independently so as to keep A*B*C=const,
> >then fit the total energy as function of these two
> variables to find
> >the local minimum for the given volume, refine if
> necessary, etc.
> >And don't forget, if you have internal coordinates
> you must
> >in principle vary them simultaneously...
> >
> >Hopefully it helps,
> >
> >Andrei Postnikov
> >  +----------  Dr. habil. Andrei Postnikov  ----- 
> apostnik@uos.de  
> >----------+
> >  | Universitaet Osnabrueck - Fachbereich Physik,
> D-49069 Osnabrueck, 
> >Germany |
> >  +----------  Tel. +49-541-9692377  -------  Fax 
> +49-541-9692351  
> >----------+
> >
> > > ====
> > > "liu wan" <wien97wan@hotmail.com>
> > > submitted the following contribution:
> > > ====
> > >
> > > Dear Dr. Gilles Hug
> > >
> > > Thank you very much for your reply!
> > >
> > > Yes, the program use the initial.struct as the
> origin file. My initial 
> >file
> > > has a=10.836754, b=9.571427l and c=17.740615,
> and I set the change of 
> >c/a is
> > > 1.5% and 3.0%, but from the file
> coa___1.5.struct, and coa___3.0.struct, 
> >I
> > > found that a=b in these two file!!! And the
> c/a=1.637 in inital.struct, 
> >but
> > > is 1.661 in coa___1.5.struct and c/a is 1.686 in
> coa___3.0.struct! I 
> >want to
> > > know the rule of changing c/a in "OPTIMIZE".
> > >
> > > Best wish
> > >
> > > liu
> > >
> >
> >====
> >WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> >To (un)subscribe send mail to
> >majordomo@zeus.theochem.tuwien.ac.at
> >====
> 
> 
>
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------------------------------

Date: Mon, 30 Dec 2002 16:04:08 +0800
From: =?gb2312?B?1dQg1r684Q==?= <zzj_fd@hotmail.com>
Subject: [none]

====
=?gb2312?B?1dQg1r684Q==?= <zzj_fd@hotmail.com>
submitted the following contribution:
====



Dear sir: 
  I want to know the detail choices in the "init_lapw" of TiO2, which 
supplied by WIEN2k. Because I can't get the same result that supported by 
the TiO2.scf file of the example TiO2. 
  In addition, can you give me a ferromagnetic surface calculation example 
which includes the main file and detail choice in initialization, such as 
Fe(100) or (110) surface. 
  Thank you very much in advance. 
Best regards. 
                                                      J.Zhao 
                                                      28/12/2002/ 






_________________________________________________________________
ÏíÓÃÊÀ½çÉÏ×î´óµÄµç×ÓÓÊ¼þÏµÍ³¡ª MSN Hotmail¡£ http://www.hotmail.com 

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------------------------------

Date: Mon, 30 Dec 2002 10:03:35 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: [WIEN]: Re: your mail

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- ---2105530234-832121234-1041239015=:19613
Content-Type: TEXT/PLAIN; charset=US-ASCII

>    I want to know the detail choices in the "init_lapw" of TiO2, which
> supplied
> by WIEN2k. Because I can't get the same result that supported by the
> TiO2.scf file of the example TiO2.

What means "not the same results" ?? Small differences are possible since
the code (and some input-defaults) have changed.


>    In addition, can you give me a ferromagnetic surface calculation example
> which includes the main file and detail choice in initialization, such as
> Fe(100) or (110) surface.

For Fe(100) try the new "supercell" program.
Fe(110) you must create yourself, but I include a 5-layer W(110) struct file
for you.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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- ---2105530234-832121234-1041239015=:19613--
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------------------------------

Date: Mon, 30 Dec 2002 10:24:24 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: The problem about Etop and Ebottom

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> In uplapw1.error,there is something like:
>  'SELECT' - no energy limits found for L= 1
>  'SELECT' - E-bottom    1.97000   E-top -200.00000

Read the "faq" pages at www.wien2k.at


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

====
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------------------------------

Date: Mon, 30 Dec 2002 11:26:05 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: MPI parallel

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I have a problem in running MPI parallel job(54 atom cell, 1 k-point,
> .machines file in MPI parallel format). initialization is correct(ie
> correct struct and other files).

The struct file seems to be correct, but it is still not well set up.
You left all RMT values at the default of 2.0, but your Na crystal has
very large distances. It will save an order of magnitude when you increase RMT
from 2.0 to e.g. 2.8 bohr
(see the faq page about setting RMTs at www.wien2k.at).


> lapw0:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
> longhorn1:1 longhorn1:1 longhorn1:1
> 1:longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1 longhorn1:1
> longhorn1:1 longhorn1:1
> granularity:1
> (8 processors for laow0 and 8 processors for 1 k-point MPI parallel)
>
> I launched the job on SP4.

I don't know what you are doing and it is impossible to say much.

If you specified "shared memory machine" during siteconfig,
it does not use "rsh" and a .rhosts file is not necessary. If you did not,
maybe your system does not allow rsh at all ??

When using poe it does not really use the .machines file. I.e. the details
of how many machines are used do not come from .machines, but from the
number of processors specified for this poe job. Right? Only to tell WIEN2k
that it should use mpi-parallel jobs you must specify the "mpi-syntax" in the
.machines file.

> files. No error message like I was getting before. BUT at lapw1 -up it
> spends enormous amount of time. I waited for 24 hours but nothing is
> written to Na.output1_up and does not stop with any error. It seems it

It should write to Na.output1up_1 !???

Reduce RKmax (Na.in1) and run

x lapw1 -up

and

x lapw1 -up -p

in two different batch jobs. It should create
Na.output1up and Na.output1up_1.
You get an idea of the timing from the 1-processor
job and the parallel job should be faster.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 30 Dec 2002 15:40:02 -0500
From: "Dadi Dai" <dai@unity.ncsu.edu>
Subject: [WIEN]: Bandstructure, Error Message

====
"Dadi Dai" <dai@unity.ncsu.edu>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0121_01C2B019.B7A3C6F0
Content-Type: text/plain;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

I used the program "spaghetti" as a step toward generating =
bandstructure.  But I met an error message as shown at the end of this =
email.  The version of "spaghett" was downloaded on Nov. 5, which seems =
to be the latest version.

Could anyone help me figure out where the problem is?

Thank you very much!

Dadi Dai

Attached: the message that the "spaghett" gave:

x spaghetti -up <return>

 number of k-points read in case.vector=3D 101
 k-point nr  41  not treated with irrep
 k-point nr  42  not treated with irrep
 k-point nr  43  not treated with irrep
 k-point nr  44  not treated with irrep
 k-point nr  45  not treated with irrep
 k-point nr  46  not treated with irrep
 k-point nr  47  not treated with irrep
 k-point nr  48  not treated with irrep
 k-point nr  49  not treated with irrep
 k-point nr  50  not treated with irrep
 k-point nr  51  not treated with irrep
 k-point nr  52  not treated with irrep
 k-point nr  53  not treated with irrep
 k-point nr  54  not treated with irrep
 k-point nr  55  not treated with irrep
 k-point nr  56  not treated with irrep
 k-point nr  57  not treated with irrep
 k-point nr  58  not treated with irrep
 k-point nr  59  not treated with irrep
 k-point nr  60  not treated with irrep
 k-point nr  61  not treated with irrep
 k-point nr  101  not treated with irrep
  band 8   char-min/max: 1.00000000000000002E-2,  5.98699999999999996E-2
  band 9   char-min/max: 1.00000000000000002E-2,  5.98680000000000045E-2
  band 10   char-min/max: 1.00000000000000002E-2,  =
5.98680000000000045E-2
  band 11   char-min/max: 1.00000000000000002E-2,  =
5.98680000000000045E-2
  band 12   char-min/max: 1.00000000000000002E-2,  =
5.98700000000000065E-2
  band 13   char-min/max: 5.98419999999999994E-2,  =
5.98580000000000084E-2
  band 14   char-min/max: 5.98419999999999994E-2,  =
5.98580000000000084E-2
  band 15   char-min/max: 5.98500000000000074E-2,  =
5.98700000000000065E-2
  band 16   char-min/max: 5.98500000000000074E-2,  =
5.98700000000000065E-2
  band 17   char-min/max: 5.98600000000000035E-2,  =
5.98660000000000095E-2
  band 18   char-min/max: 5.98600000000000035E-2,  =
5.98660000000000095E-2
  band 19   char-min/max: 5.98600000000000035E-2,  =
5.98660000000000095E-2
  band 20   char-min/max: 5.98620000000000055E-2,  =
5.98680000000000045E-2

lib-4212 : UNRECOVERABLE library error
  An internal WRITE tried to write beyond the end of an internal file.

Encountered during a sequential formatted WRITE to an internal file =
(character v
ariable)
IOT Trap
Abort (core dumped)
0.5u 0.9s 0:01 98% 0+0k 2+0io 0pf+0w

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Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2722.900" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD><FONT face=3DArial><FONT size=3D2>
<BODY>
<DIV>I used the program "spaghetti" as a step toward generating=20
bandstructure.&nbsp; But I met an error message as shown at the end of =
this=20
email.&nbsp; The version of "spaghett" was downloaded on Nov. 5, which =
seems to=20
be the latest version.</DIV>
<DIV>&nbsp;</DIV>
<DIV>Could anyone help me figure out where the problem is?</DIV>
<DIV>&nbsp;</DIV>
<DIV>Thank you very much!</DIV>
<DIV>&nbsp;</DIV>
<DIV>Dadi Dai</DIV>
<DIV>&nbsp;</DIV>
<DIV>Attached: the message that the "spaghett" gave:</DIV>
<DIV>&nbsp;</DIV>
<DIV>x spaghetti -up &lt;return&gt;</DIV>
<DIV><BR>&nbsp;number of k-points read in case.vector=3D =
101<BR>&nbsp;k-point=20
nr&nbsp; 41&nbsp; not treated with irrep<BR>&nbsp;k-point nr&nbsp; =
42&nbsp; not=20
treated with irrep<BR>&nbsp;k-point nr&nbsp; 43&nbsp; not treated with=20
irrep<BR>&nbsp;k-point nr&nbsp; 44&nbsp; not treated with =
irrep<BR>&nbsp;k-point=20
nr&nbsp; 45&nbsp; not treated with irrep<BR>&nbsp;k-point nr&nbsp; =
46&nbsp; not=20
treated with irrep<BR>&nbsp;k-point nr&nbsp; 47&nbsp; not treated with=20
irrep<BR>&nbsp;k-point nr&nbsp; 48&nbsp; not treated with =
irrep<BR>&nbsp;k-point=20
nr&nbsp; 49&nbsp; not treated with irrep<BR>&nbsp;k-point nr&nbsp; =
50&nbsp; not=20
treated with irrep<BR>&nbsp;k-point nr&nbsp; 51&nbsp; not treated with=20
irrep<BR>&nbsp;k-point nr&nbsp; 52&nbsp; not treated with =
irrep<BR>&nbsp;k-point=20
nr&nbsp; 53&nbsp; not treated with irrep<BR>&nbsp;k-point nr&nbsp; =
54&nbsp; not=20
treated with irrep<BR>&nbsp;k-point nr&nbsp; 55&nbsp; not treated with=20
irrep<BR>&nbsp;k-point nr&nbsp; 56&nbsp; not treated with =
irrep<BR>&nbsp;k-point=20
nr&nbsp; 57&nbsp; not treated with irrep<BR>&nbsp;k-point nr&nbsp; =
58&nbsp; not=20
treated with irrep<BR>&nbsp;k-point nr&nbsp; 59&nbsp; not treated with=20
irrep<BR>&nbsp;k-point nr&nbsp; 60&nbsp; not treated with =
irrep<BR>&nbsp;k-point=20
nr&nbsp; 61&nbsp; not treated with irrep<BR>&nbsp;k-point nr&nbsp; =
101&nbsp; not=20
treated with irrep<BR>&nbsp; band 8&nbsp;&nbsp; char-min/max:=20
1.00000000000000002E-2,&nbsp; 5.98699999999999996E-2<BR>&nbsp; band=20
9&nbsp;&nbsp; char-min/max: 1.00000000000000002E-2,&nbsp;=20
5.98680000000000045E-2<BR>&nbsp; band 10&nbsp;&nbsp; char-min/max:=20
1.00000000000000002E-2,&nbsp; 5.98680000000000045E-2<BR>&nbsp; band=20
11&nbsp;&nbsp; char-min/max: 1.00000000000000002E-2,&nbsp;=20
5.98680000000000045E-2<BR>&nbsp; band 12&nbsp;&nbsp; char-min/max:=20
1.00000000000000002E-2,&nbsp; 5.98700000000000065E-2<BR>&nbsp; band=20
13&nbsp;&nbsp; char-min/max: 5.98419999999999994E-2,&nbsp;=20
5.98580000000000084E-2<BR>&nbsp; band 14&nbsp;&nbsp; char-min/max:=20
5.98419999999999994E-2,&nbsp; 5.98580000000000084E-2<BR>&nbsp; band=20
15&nbsp;&nbsp; char-min/max: 5.98500000000000074E-2,&nbsp;=20
5.98700000000000065E-2<BR>&nbsp; band 16&nbsp;&nbsp; char-min/max:=20
5.98500000000000074E-2,&nbsp; 5.98700000000000065E-2<BR>&nbsp; band=20
17&nbsp;&nbsp; char-min/max: 5.98600000000000035E-2,&nbsp;=20
5.98660000000000095E-2<BR>&nbsp; band 18&nbsp;&nbsp; char-min/max:=20
5.98600000000000035E-2,&nbsp; 5.98660000000000095E-2<BR>&nbsp; band=20
19&nbsp;&nbsp; char-min/max: 5.98600000000000035E-2,&nbsp;=20
5.98660000000000095E-2<BR>&nbsp; band 20&nbsp;&nbsp; char-min/max:=20
5.98620000000000055E-2,&nbsp; 5.98680000000000045E-2</DIV>
<DIV>&nbsp;</DIV>
<DIV>lib-4212 : UNRECOVERABLE library error<BR>&nbsp; An internal WRITE =
tried to=20
write beyond the end of an internal file.</DIV>
<DIV>&nbsp;</DIV>
<DIV>Encountered during a sequential formatted WRITE to an internal file =

(character v<BR>ariable)<BR>IOT Trap<BR>Abort (core dumped)<BR>0.5u 0.9s =
0:01=20
98% 0+0k 2+0io 0pf+0w</DIV></BODY></HTML></FONT></FONT>

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------------------------------

Date: Mon, 30 Dec 2002 23:42:59 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Bandstructure, Error Message

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I used the program "spaghetti" as a step toward generating bandstructure.
But I met an error message as shown at the end of this email.
>
> x spaghetti -up <return>
>
>  number of k-points read in case.vector= 101
>  k-point nr  41  not treated with irrep
>   band 20   char-min/max: 5.98620000000000055E-2,  5.98680000000000045E-2
>
> lib-4212 : UNRECOVERABLE library error
>   An internal WRITE tried to write beyond the end of an internal file.
>
> Encountered during a sequential formatted WRITE to an internal file (character v
> ariable)

I'm not sure about this, but it seems you have run irrep and/or lapw2 -qtl
with a different k-mesh before.

Remove all *irrep* files (and maybe also case.qtlup/dn) before running
spaghetti (or rerun x irrep -up/dn )

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 30 Dec 2002 17:56:00 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: test

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


testing....


sorry for inconvience.

Regards
sahu

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------------------------------

Date: Tue, 31 Dec 2002 10:14:40 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: [WIEN]: Re: MPI

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> 2) I tried the 54 atom supercell with " x lapw1 -up -p" using the
> jobscript(1 processor)
>
> _______________________________________________________________
> #!/usr/bin/csh
> #@ job_name = na
> #@ output =$(job_name).o$(jobid)
> #@ error = $(job_name).o$(jobid)
> #@ initialdir = /gpfs/utexas/ph/phaa406/Na.mpi
> #@ job_type = parallel
> #@ environment = COPY_ALL; MP_SHARED_MEMORY=yes;
> #@ resources = ConsumableCpus(1) ConsumableMemory(1gb)
> #@ notify_user = sahu@matter3.ph.utexas.edu
> #@ node = 1
> #@ tasks_per_node = 1
> #@ class = interactive
> #@ notification=error
> #@ wall_clock_limit = 1:15:00
> #@ notification=error
> #@ notification = complete
> #@ queue
> ../w2k/x lapw1 -up -p
> _________________________________________________~
>
> and .machines file
>
> 1:longhorn1:1
> granularity:1
>
> It does produce Na.mpi.output1up_1 in 16 seconds.

With this machines file it will use the sequential lapw1.

But you could keep task_per_node=1, but in .machines use:
1:longhorn1:1 longhorn1:1

This machines file will force lapw1para to use the poe command and the
lapw1_mpi executable, but since the loadleveler ignores any -p xx
directives and just uses "task_per_node", it will run the mpi-executable
on just one processor.

llsubmit produces output and error file *.out and *.err. Is there any
message?

Another test:
For those short runtimes try to run interactively, i.e. execute at the
commandline:

x lapw1 -up
x lapw1 -up -p (with a 2-processor "mpi" .machines file)
Any system messages ?


> 54 atom supercell atom works fine with k-point parallel mode. No problem.
> But in this case I need to choose some finite number of k-points(instead
> of 1 k-point) But its the efficiency compared to MPI scripts need to be
> checked for the supercell case(with same number of k-points).

You can trust me, that for a metallic supercell like yours with such short
runtimes the k-point parallel version is by orders of magnitude more
efficient!!!! And metallic Na requires many k-points!!!!

> If I remember correctly, on SP3 you could run the MPI script without any
> problem.am I right?

Yes of course. We use wien2k on our SP3 regularely, but I also know that
it is used on SP4 in mpi-parallel mode (for matrixsizes up to 15000 !!!)

> On SP4, normally the "poe" command preceeds the executables for example
> "poe ./wien2k_executable". "poe" calls proper parallel environment
> like mpirun, communication routines used during compilation etc.
> but in the above I did not use "poe" command and just
> ./wien2k_executables -p.
>
> For checking I tried with poe preceeding ./wien_executables.
> ie  poe ../w2k/x lapw1 -up -p

I guess I explained before: Using    x lapw1 -p
will call a shell script "lapw1para" which analyses .machines and then
issues a "poe lapw1 lapw1.def ...  " command. So you must not use poe
together with "x", but you could in principle (for testing) use poe with a
WIEN-executable. To learn more about that edit lapw1para and put -xf in
the first line. This will log all its actions and you will also see the
required poe command.

Regards
                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 31 Dec 2002 18:31:07 +0300 (MSK)
From: Alexander Korlyukov <alex@xrlab.ineos.ac.ru>
Subject: [WIEN]: plots of laplacian of electron density

====
Alexander Korlyukov <alex@xrlab.ineos.ac.ru>
submitted the following contribution:
====

Dear Wien2k users.
May I obtain plots of laplacian using aim program?
In userguide this possibility is not mentioned.
Hovewer, when I saw the documentation concerning aim I found file titled
"ToDo" (unfortunately in Spanish) in which is spoken (as I understood
spanish text) that aim program can produce plots of laplacian. Details of
such procedure is not clear for me because my knowledge of Spanish is bad.

Sincerely,
A. A. Korlyukov


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------------------------------

Date: Tue, 31 Dec 2002 10:38:20 -0500
From: "Dadi Dai" <dai@unity.ncsu.edu>
Subject: Re: [WIEN]: Bandstructure, Error Message

====
"Dadi Dai" <dai@unity.ncsu.edu>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_00A0_01C2B0B8.BC86B110
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	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

Dear Dr. Blaha,

Thanks for your reply!  I have tried all of your suggestions, but I =
still have the same error message.  Could you please give me any futher =
comments on how to solve this problem?

Thank you!

Dadi Dai

- ----- Original Message -----=20
From: "Peter Blaha" <pblaha@theochem.tuwien.ac.at>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Monday, December 30, 2002 5:42 PM
Subject: Re: [WIEN]: Bandstructure, Error Message


> =3D=3D=3D=3D
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> =3D=3D=3D=3D
>=20
> > I used the program "spaghetti" as a step toward generating =
bandstructure.
> But I met an error message as shown at the end of this email.
> >
> > x spaghetti -up <return>
> >
> >  number of k-points read in case.vector=3D 101
> >  k-point nr  41  not treated with irrep
> >   band 20   char-min/max: 5.98620000000000055E-2,  =
5.98680000000000045E-2
> >
> > lib-4212 : UNRECOVERABLE library error
> >   An internal WRITE tried to write beyond the end of an internal =
file.
> >
> > Encountered during a sequential formatted WRITE to an internal file =
(character v
> > ariable)
>=20
> I'm not sure about this, but it seems you have run irrep and/or lapw2 =
- -qtl
> with a different k-mesh before.
>=20
> Remove all *irrep* files (and maybe also case.qtlup/dn) before running
> spaghetti (or rerun x irrep -up/dn )
>=20
> Regards
>=20
>                                       P.Blaha


- ------=_NextPart_000_00A0_01C2B0B8.BC86B110
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	charset="iso-8859-1"
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2722.900" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY>
<DIV><FONT face=3DArial size=3D2></FONT><FONT face=3DArial size=3D2>Dear =
Dr.=20
Blaha,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Thanks for your reply!&nbsp; I have =
tried all of=20
your suggestions, but I still have the same error message.&nbsp; Could =
you=20
please give me any futher comments on how to solve this =
problem?</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Thank you!</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Dadi Dai</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>----- Original Message ----- </FONT>
<DIV><FONT face=3DArial size=3D2>From: "Peter Blaha" &lt;</FONT><A=20
href=3D"mailto:pblaha@theochem.tuwien.ac.at"><FONT face=3DArial=20
size=3D2>pblaha@theochem.tuwien.ac.at</FONT></A><FONT face=3DArial=20
size=3D2>&gt;</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>To: &lt;</FONT><A=20
href=3D"mailto:wien@zeus.theochem.tuwien.ac.at"><FONT face=3DArial=20
size=3D2>wien@zeus.theochem.tuwien.ac.at</FONT></A><FONT face=3DArial=20
size=3D2>&gt;</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Sent: Monday, December 30, 2002 5:42=20
PM</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Subject: Re: [WIEN]: Bandstructure, =
Error=20
Message</FONT></DIV></DIV>
<DIV><FONT face=3DArial><BR><FONT size=3D2></FONT></FONT></DIV><FONT =
face=3DArial=20
size=3D2>&gt; =3D=3D=3D=3D<BR>&gt; Peter Blaha &lt;</FONT><A=20
href=3D"mailto:pblaha@theochem.tuwien.ac.at"><FONT face=3DArial=20
size=3D2>pblaha@theochem.tuwien.ac.at</FONT></A><FONT face=3DArial=20
size=3D2>&gt;<BR>&gt; submitted the following contribution:<BR>&gt; =
=3D=3D=3D=3D<BR>&gt;=20
<BR>&gt; &gt; I used the program "spaghetti" as a step toward generating =

bandstructure.<BR>&gt; But I met an error message as shown at the end of =
this=20
email.<BR>&gt; &gt;<BR>&gt; &gt; x spaghetti -up &lt;return&gt;<BR>&gt;=20
&gt;<BR>&gt; &gt;&nbsp; number of k-points read in case.vector=3D =
101<BR>&gt;=20
&gt;&nbsp; k-point nr&nbsp; 41&nbsp; not treated with irrep<BR>&gt;=20
&gt;&nbsp;&nbsp; band 20&nbsp;&nbsp; char-min/max: =
5.98620000000000055E-2,&nbsp;=20
5.98680000000000045E-2<BR>&gt; &gt;<BR>&gt; &gt; lib-4212 : =
UNRECOVERABLE=20
library error<BR>&gt; &gt;&nbsp;&nbsp; An internal WRITE tried to write =
beyond=20
the end of an internal file.<BR>&gt; &gt;<BR>&gt; &gt; Encountered =
during a=20
sequential formatted WRITE to an internal file (character v<BR>&gt; &gt; =

ariable)<BR>&gt; <BR>&gt; I'm not sure about this, but it seems you have =
run=20
irrep and/or lapw2 -qtl<BR>&gt; with a different k-mesh before.<BR>&gt; =
<BR>&gt;=20
Remove all *irrep* files (and maybe also case.qtlup/dn) before =
running<BR>&gt;=20
spaghetti (or rerun x irrep -up/dn )<BR>&gt; <BR>&gt; Regards<BR>&gt; =
<BR>&gt;=20
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&=
nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&n=
bsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nb=
sp;=20
P.Blaha<BR></FONT></BODY></HTML>

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------------------------------

Date: Tue, 31 Dec 2002 17:16:06 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: plots of laplacian of electron density

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> May I obtain plots of laplacian using aim program?
> In userguide this possibility is not mentioned.
> Hovewer, when I saw the documentation concerning aim I found file titled
> "ToDo" (unfortunately in Spanish) in which is spoken (as I understood
> spanish text) that aim program can produce plots of laplacian. Details of
> such procedure is not clear for me because my knowledge of Spanish is bad.

I suggest you use lapw0: Put "potential option"= 36 and R2V in case.in0.
x lapw0
case.r2v contains in the "XC-potential" the laplacian of rho.

Use lapw5 for plotting (replace clmval by r2v file).

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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Date: Tue, 31 Dec 2002 13:10:55 -0500
From: "Dadi Dai" <dai@unity.ncsu.edu>
Subject: Re: [WIEN]: Bandstructure, Error Message

====
"Dadi Dai" <dai@unity.ncsu.edu>
submitted the following contribution:
====

This is a multi-part message in MIME format.

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	charset="iso-8859-1"
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Dear Dr. Blaha,

In the file SRC_spaghetti/spag.f

Line 431:
write(label,878) (jatom_list(j),j=3D1,jatom)

where "label" is defined as character*12 in the line 23 of the same =
file.

I guess the trouble comes here, because "write" should be followed by a =
file unit number instead of a string.

Could you please let me know how this line should be revised?

Thanks!

Dadi Dai

- ----- Original Message -----=20
From: "Peter Blaha" <pblaha@theochem.tuwien.ac.at>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Monday, December 30, 2002 5:42 PM
Subject: Re: [WIEN]: Bandstructure, Error Message


> =3D=3D=3D=3D
> Peter Blaha <pblaha@theochem.tuwien.ac.at>
> submitted the following contribution:
> =3D=3D=3D=3D
>=20
> > I used the program "spaghetti" as a step toward generating =
bandstructure.
> But I met an error message as shown at the end of this email.
> >
> > x spaghetti -up <return>
> >
> >  number of k-points read in case.vector=3D 101
> >  k-point nr  41  not treated with irrep
> >   band 20   char-min/max: 5.98620000000000055E-2,  =
5.98680000000000045E-2
> >
> > lib-4212 : UNRECOVERABLE library error
> >   An internal WRITE tried to write beyond the end of an internal =
file.
> >
> > Encountered during a sequential formatted WRITE to an internal file =
(character v
> > ariable)
>=20
> I'm not sure about this, but it seems you have run irrep and/or lapw2 =
- -qtl
> with a different k-mesh before.
>=20
> Remove all *irrep* files (and maybe also case.qtlup/dn) before running
> spaghetti (or rerun x irrep -up/dn )
>=20
> Regards
>=20
>                                       P.Blaha


- ------=_NextPart_000_0124_01C2B0CE.0D30D1D0
Content-Type: text/html;
	charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2722.900" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY>
<DIV><FONT face=3DArial size=3D2>Dear Dr. Blaha,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>In the file =
SRC_spaghetti/spag.f</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Line 431:</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>write(label,878)=20
(jatom_list(j),j=3D1,jatom)</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>where "label" is defined as =
character*12 in the=20
line 23 of the same file.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>I guess the trouble comes here, because =
"write"=20
should be followed by a file unit number instead of a =
string.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Could you please let me know how this =
line should=20
be revised?</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Thanks!</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Dadi Dai</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>----- Original Message ----- </FONT>
<DIV><FONT face=3DArial size=3D2>From: "Peter Blaha" &lt;</FONT><A=20
href=3D"mailto:pblaha@theochem.tuwien.ac.at"><FONT face=3DArial=20
size=3D2>pblaha@theochem.tuwien.ac.at</FONT></A><FONT face=3DArial=20
size=3D2>&gt;</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>To: &lt;</FONT><A=20
href=3D"mailto:wien@zeus.theochem.tuwien.ac.at"><FONT face=3DArial=20
size=3D2>wien@zeus.theochem.tuwien.ac.at</FONT></A><FONT face=3DArial=20
size=3D2>&gt;</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Sent: Monday, December 30, 2002 5:42=20
PM</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Subject: Re: [WIEN]: Bandstructure, =
Error=20
Message</FONT></DIV></DIV>
<DIV><FONT face=3DArial><BR><FONT size=3D2></FONT></FONT></DIV><FONT =
face=3DArial=20
size=3D2>&gt; =3D=3D=3D=3D<BR>&gt; Peter Blaha &lt;</FONT><A=20
href=3D"mailto:pblaha@theochem.tuwien.ac.at"><FONT face=3DArial=20
size=3D2>pblaha@theochem.tuwien.ac.at</FONT></A><FONT face=3DArial=20
size=3D2>&gt;<BR>&gt; submitted the following contribution:<BR>&gt; =
=3D=3D=3D=3D<BR>&gt;=20
<BR>&gt; &gt; I used the program "spaghetti" as a step toward generating =

bandstructure.<BR>&gt; But I met an error message as shown at the end of =
this=20
email.<BR>&gt; &gt;<BR>&gt; &gt; x spaghetti -up &lt;return&gt;<BR>&gt;=20
&gt;<BR>&gt; &gt;&nbsp; number of k-points read in case.vector=3D =
101<BR>&gt;=20
&gt;&nbsp; k-point nr&nbsp; 41&nbsp; not treated with irrep<BR>&gt;=20
&gt;&nbsp;&nbsp; band 20&nbsp;&nbsp; char-min/max: =
5.98620000000000055E-2,&nbsp;=20
5.98680000000000045E-2<BR>&gt; &gt;<BR>&gt; &gt; lib-4212 : =
UNRECOVERABLE=20
library error<BR>&gt; &gt;&nbsp;&nbsp; An internal WRITE tried to write =
beyond=20
the end of an internal file.<BR>&gt; &gt;<BR>&gt; &gt; Encountered =
during a=20
sequential formatted WRITE to an internal file (character v<BR>&gt; &gt; =

ariable)<BR>&gt; <BR>&gt; I'm not sure about this, but it seems you have =
run=20
irrep and/or lapw2 -qtl<BR>&gt; with a different k-mesh before.<BR>&gt; =
<BR>&gt;=20
Remove all *irrep* files (and maybe also case.qtlup/dn) before =
running<BR>&gt;=20
spaghetti (or rerun x irrep -up/dn )<BR>&gt; <BR>&gt; Regards<BR>&gt; =
<BR>&gt;=20
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&=
nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&n=
bsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nb=
sp;=20
P.Blaha<BR></FONT></BODY></HTML>

- ------=_NextPart_000_0124_01C2B0CE.0D30D1D0--

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------------------------------

Date: Tue, 31 Dec 2002 19:47:05 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: MINI

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear W2kusers

         I wish use the "min_lapw" script for internal parameter 
optimization. I browsed through the mail-digest for previous queries.
and also gone through the usersguide and FAQ on minimization of forces.

A] I found the following command:

min_lapw -I -s 1 -i 30 -j run(sp)_lapw -I -fc 1 -p

The meaning of -I and/or -fc is clear in runsp_lapw command.
 -i 30 is to do maximum 30 geometry optimization steps(defalut is 50). and
by default, 20 iteration scf steps will be done (in parallel due to -p
switch) for a particular geometry optimization step ie for each geometry
optimization step(maximum 30 above),20 scf cycles will be done. At the
last step of geometry optimization, -I in runsp_lapw switch "TOT" to "FOR"
in case.in2(c) (to take into account the incomplete basis set correction
or pulay force correction).Is the interpretation correct? But what does -I
- -s 1 infront of min_lapw means.

B] In the case.inM file :

NEWT 1.0           #(NOSE, NEWT, BFGS, MOLD, tolf (a4,f5.2))
5.0 5.0 5.0 0.8    # Atom1   (NOSE, MOLD:Masse, delta t, T, 
nose-frequency) 
5.0 5.0 5.0 0.8    # Atom2   (NEWT: 1,2,3:delta, 4:eta(1=MOLD))
5.0 5.0 5.0 0.8    # Atom3   (BFGS, NEWT: [ 1 || 2 || 3 ] = 0 constraint)

the number of atoms for which one wish to perform geometry optimization
is total number of atoms in the case.struct file OR just number of
inequivalant atoms?

If BFGS scheme is used for optimization instead of damped Newton scheme 
then  

a) friction parameter "eta" should be = 1 ie no friction. is it correct? 
Or we always have some friction in both schemes.

b) tolf determines when geometry optimization stops but -fc 1(ie 1
mRy/bohr) also means geometry optimization stops when this condition is 
met. 

Is -fc 1mRy/bohr means when individual component of force on a given atom
is less than this value then geometry optimizatin stops OR the total(sum
of components) force on a given atom should be less than this value for
stopping the geometry optimization criteria?

then what does tolf in case.inM does since we already have -fc? is the
value -fc 1 overrides the value specified by tolf in case.inM?am I
missing something here?

c) delta(i) (i =x, y, z) are small increments to the coordinates of each
atom(taken from case.struct or case.struct_mini file). that means for each
geometry optimizatinon step, these increments are added to the coordinates
from the case.strut file in 1st geometry iteration (or case.struct_mini 
in subsequent iterations)  and  a chosen  optimization scheme
is then used for finding the forces and resultant new coordinates. Is it
correct?

thanking you in advance for answers/suggestions. 

Regards
sahu

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------------------------------

Date: Wed, 1 Jan 2003 10:35:42 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Bandstructure, Error Message

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> In the file SRC_spaghetti/spag.f
>
> Line 431:
> write(label,878) (jatom_list(j),j=1,jatom)
>
> where "label" is defined as character*12 in the line 23 of the same file.
>
> I guess the trouble comes here, because "write" should be followed by a file unit number instead of a string.
>
> Could you please let me know how this line should be revised?

This line is ok. One can do a "write" to a character variable.

I guess your insp file is wrong (last lines where eventually some fat-band
parameters are specified).

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Thu,  2 Jan 2003 12:42:29 +0100
From: Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: MINI

====
Stefaan Cottenier <Stefaan.Cottenier@fys.kuleuven.ac.be>
submitted the following contribution:
====

> ====
> "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
> submitted the following contribution:
> ====
> 
> A] I found the following command:
> 
> min_lapw -I -s 1 -i 30 -j run(sp)_lapw -I -fc 1 -p
> 
>(...)
>
> Is the interpretation correct? 

Yes.

> But what does -I -s 1 infront of min_lapw means.

The -I tells that mini should forget the history of previous changes of the
internal parameters. It should be used when you start mini for the first time,
or when you have changed your case.inM and want to restart with these other
values. Use -NI instead when you want to continue the minimization if it has
stopped too early (e.g. because -i 30 was reached) but has no errors or problems
otherwise. The -s 1 tells that it should save the clm* and scf file at every
change of positions, with -s 5 this is only after each 5th change of position, etc.

> B] In the case.inM file :
> 
> NEWT 1.0           #(NOSE, NEWT, BFGS, MOLD, tolf (a4,f5.2))
> 5.0 5.0 5.0 0.8    # Atom1   (NOSE, MOLD:Masse, delta t, T, 
> nose-frequency) 
> 5.0 5.0 5.0 0.8    # Atom2   (NEWT: 1,2,3:delta, 4:eta(1=MOLD))
> 5.0 5.0 5.0 0.8    # Atom3   (BFGS, NEWT: [ 1 || 2 || 3 ] = 0 constraint)
> 
> the number of atoms for which one wish to perform geometry optimization
> is total number of atoms in the case.struct file OR just number of
> inequivalant atoms?

The number of inequivalent ones.

> If BFGS scheme is used for optimization instead of damped Newton scheme 
> then  
> 
> a) friction parameter "eta" should be = 1 ie no friction. is it correct? 
> Or we always have some friction in both schemes.

Eta=1 is no friction. This is useless for minimization, as the atoms will
continue to oscillate forever. The MOLD keyword for molecular dynamics is
effictively NEWT with zero friction.

> b) tolf determines when geometry optimization stops but -fc 1(ie 1
> mRy/bohr) also means geometry optimization stops when this condition is 
> met. 
> 
> Is -fc 1mRy/bohr means when individual component of force on a given atom
> is less than this value then geometry optimizatin stops OR the total(sum
> of components) force on a given atom should be less than this value for
> stopping the geometry optimization criteria?

I'm not sure, but it should be easy to test.
 
> then what does tolf in case.inM does since we already have -fc? is the
> value -fc 1 overrides the value specified by tolf in case.inM?am I
> missing something here?

tolf in case.inM tells when the mini scf cycle should stop, i.e. when the forces
on all atoms are close enough to zero. -fc tells when the regular electronic scf
cycle should stop, i.e. when all forces are sufficiently stable (but not
necessarily zero).

> c) delta(i) (i =x, y, z) are small increments to the coordinates of each
> atom(taken from case.struct or case.struct_mini file). that means for each
> geometry optimizatinon step, these increments are added to the coordinates
> from the case.strut file in 1st geometry iteration (or case.struct_mini 
> in subsequent iterations)  and  a chosen  optimization scheme
> is then used for finding the forces and resultant new coordinates. Is it
> correct?

Almost. The forces are determined by a regular electronic scf calculation, the
minimization scheme determines the new positions from the the forces and the old
positions.

Stefaan
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------------------------------

Date: Thu, 2 Jan 2003 14:33:37 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: MINI

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

.
>
> > b) tolf determines when geometry optimization stops but -fc 1(ie 1
> > mRy/bohr) also means geometry optimization stops when this condition is
> > met.
> >
> > Is -fc 1mRy/bohr means when individual component of force on a given
atom
> > is less than this value then geometry optimizatin stops OR the total(sum
> > of components) force on a given atom should be less than this value for
> > stopping the geometry optimization criteria?


Tolf is compared to the total force on an atom in a converged calculation.
(given in case.scfm (and copied to case.scf)).  So optimization stops when
all atoms have total forces smaller than tolf mRy.
fc is used only within one step of the optimization, as already explained by
Stefaan Cottenier (it is the equivalent of -ec 0.0001, eg.).  fc 1  does not
mean that SCF runs until the force is smaller than 1 mRy, but until the size
of the force is converged to within 1.  (I don't know whether total or
separate components are compared to determine force convergence.  Components
seem to be more logical?).


[By the way, you may have noticed that in the last cycle of an
scf-calculation, the force is a lot different from the previous cycles -
even though the calculation is said to be converged w.r.t. forces.  This is
because a certain contribution to the forces which is not important for the
convergence is calculated only in the last iteration.  Nothing to worry
about.]


Kevin Jorissen
kevin.jorissen@ua.ac.be

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------------------------------

Date: Thu, 2 Jan 2003 13:52:09 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: initso script

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear W2kusers

 thanks to Prof. Cottenier and Kevin Jorissen for clarifying MINI queries.

Is it possible for me to know as how to come out of k-point generation
cycle while initializing the run for SO using initso_lapw script?b'cause
once the number of k-points is chosen, and kgen -so is run by the script,
it asks again

Do you want to rerun kgen ? (y/N)

If I say, No or N or n, It stops with the error

if: Badly formed number

and If I say yes or Y or y, it continues and again asks the same thing.

Does the initialization script initso_lapw needs modification?

 thanks for your attention/s.

Regards
sahu 


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------------------------------

Date: Thu, 2 Jan 2003 14:27:22 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: runsp_script 

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear W2kusers,

1)  While running SO+ORB for a spin-polarized system using runsp_lapw
- -orb -so, I encountered an error in the 2nd scf cycle:

____________________________________________________________
in cycle 2    ETEST: 106.6573260000000000   CTEST: 1.8484003
hup: Command not found.
STOP  LAPW0 END
STOP  ORB   END
STOP  ORB   END
if: Badly formed number.---> it stops here with this message.

I checked the "runsp_script". The end of the section orb: 
____________________________________________----

orb:
foreach i (dmatup dmatdn dmatud )
  if (-e $file.$i"_old" ) rm $file.$i"_old"
  if (-e $file.$i ) cp $file.$i $file.$i"_old"          #save this cycle 
for next
end

if ( -e $file.scforbup ) rm $file.scforbup
if ( -e $file.scforbdn ) rm $file.scforbdn
if ( -e $file.scforbdu ) rm $file.scforbdu
if ( "$orb" != "-orb" ) goto lapw1
if ( $?orbc ) goto lapw1
if (! -e $file.dmatup || -z $file.dmatup ) goto lapw1
#foreach i ( vorbup vorbdn vorbdu )
#  if (-e $file.$i ) \
#  cp $file.$i $file.$i"_old"           #save last cycle
#end
testinput       $file.inorb error_input
total_exec      orb -up $para
total_exec      orb -dn $para
if ( "$so" == "-so" && -s $file.dmatud ) then
total_exec      orb -du $para
endif
______________________________________

It is trying to calculate orb -du $para if -so switch and case.dmatud 
exists. I checked that file case.dmatud is created in the first iteration 
by x lapwdm in addition to case.dmatup and case.dmatdn  and also it is SO 
calculation. but as soon as the control goes to

if ( "$so" == "-so" && -s $file.dmatud ) 

it stops with the message:

if: Badly formed number.

The procedure I followed is:
_________________________________________________________________
I first did the spinpolarized scf calculation without SO and orbital
potentials ie just runsp_lapw.proper convergence achieved.

To add SO and orbital potential starting with this:

a) initso_lapw --> it created a the case.inso and other case.*_so files
including proper struct file(the case.*_so files and case.struct_so are
copied to corresponding case.* files)

b) prepared the proper case.indmc and case.inorb file.

c) finally "runsp_lapw -orb -so.
______________________________________

I contacted Prof. Novak regarding this(I couldnot put this qurey that time
on w2k mailing list due to problem in accessing w2k server. All my mails
to w2k mailing list that time returned but it is workig now!!) and thanks
to him he suggested that the problem might be connected with the
nondiagonal term of the orbital potential (<spin up|V|spin down>)and there
seems to be some bug there.

He gave me his own shell script "joborb"(equivalant to runsp_lapw -so
- -orb) and suggested me to first do 1 iteration only without -orb switch in
lapwso(so that case.vorbup and case.vorbdn is first produced in -orb
- -up/dn later in the one iteration cycle) and then add again -orb switch to
lapwso run the cycle for required number of iterations(say 40).Now since
case.vorbup/dn files are there these will be used by lapwso -orb. I didnot
encounter any problem so far.

However the convergnce conditions(:DIS, :ENE, :FOR, :MMI0XX etc) are 
to be monitered manually now!!

Also he mentioned that Prof. Peter Blaha removed this term from the
scripts running WIEN some time ago, but perhaps some remnant remained.

I downloaded the latest w2k and the above error is from this latest
download. but I dont know whether It is taken care of now.

2) If I have a completed run (but not converged, say with 20 iteration)
with PRATT mixing scheme, then can I switch to BROYD mixing scheme(by
changing PRATT to BROYD and FACTOR to say 0.4 in case.inm file) without
deleting any files from the PRATT mixing scheme run and continuing with
BROYD for convergence?

thanks in advance for your attention and suggestion/s.

Regards
sahu

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------------------------------

Date: Fri, 3 Jan 2003 13:37:29 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: MIXER

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear W2k users

1)     Yesterday I sent an qurey regaring change from PRATT to BROYD 
scheme. 
If any w2kuser had a simillar situation and has an answer, pl. let me 
know.

I also had an query about intiso_lapw and runsp_lapw script.
 
I repeat the mixing qurery only.

If I have a completed run (but not converged, say with 20 iteration) with
PRATT mixing scheme, then if I wish to switch to BROYD mixing scheme(by
changing PRATT to BROYD and FACTOR to say 0.4 in case.inm file) 
do I have to delete/save any file before I start the run again with
BROYD mixing scheme.


2) I observed the following:

When I have a run , spin-polarized, SO+ORB starting from scratch, even if 
the case.inm and case.inorb file both has BROYD scheme with FACTOR 0.4,
the case.scf file has the written "PRATT MIXING SCHEME WITH 0.400"!!!
I monitored it for few iteration, BROYD is not used at all.

However, for just spinpolarized(runsp) run OR spinpolarized with 
spin-orbit(runsp -so), it correctly picks up BROYD from case.inm file.

Does this mean there is some problem with -orb while calling MIXER? so
even if BROYD is specified in case.inm/case.inorb, PRATT will be picked up
by default?

thanking you in advance for your suggestion/s.

Regards
sahu

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------------------------------

End of wien-digest V2002 #50
****************************

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To: wien-digest@theochem.tuwien.ac.at
Subject: wien-digest V2002 #51
Reply-To: wien
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wien-digest         Sunday, January 12 2003         Volume 2002 : Number 051




----------------------------------------------------------------------

Date: Fri, 03 Jan 2003 19:22:44 -0300
From: Gabriela Fernanda Cabeza <gcabeza@criba.edu.ar>
Subject: [WIEN]: Compiling TELNES

====
Gabriela Fernanda Cabeza <gcabeza@criba.edu.ar>
submitted the following contribution:
====

Dear Wien users,

When recompiling TELNES on a Linux box with g77 (recommended) i got the 
following
error file (compile.msg) at SRC_telnes directory:

- ---------------------------------------------------------------------------

g77 -O -c telnes.f
telnes.f: In subroutine `firstcase':
telnes.f:2080:
+ REAL(Factor1*Factor2*Factor3*Factor4)
^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:2085:
+ REAL(Factor1*Factor2*Factor3*Factor4)
^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f: In subroutine `secondcase':
telnes.f:2143:
+ REAL(Factor1*Factor2*Factor3*Factor4)
^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:2148:
+ REAL(Factor1*Factor2*Factor3*Factor4)
^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
make: *** [telnes.o] Error 1

- ---------------------------------------------------------------------------

Has anybody had the same errors?

Thank you very much in advance for every hint.
Kind regards




Dra. Gabriela F. Cabeza
Profesora Adjunta
Dpto. de Física - Universidad Nacional del Sur
Avda. Alem 1253, (B8000CPB) Bahía Blanca - Argentina
tel: 54-291- 4595141- 54-291-4595101, int. 2821
fax: 54-291-4595142
e-mail: gcabeza@criba.edu.ar

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Date: Fri, 3 Jan 2003 19:51:35 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: MINI

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear W2kusers

      while using case.inM file for min_lapw, Is there any guideline
for choosing delta(i) valuesfor say BFGS or NEW scheme and not molecular 
dynamics?

does it depend upon the type of atoms which are to be moved? or anything 
else?b'cause we may achieve the the chosen "tolf" value in smallar number
of geometry optimization steps by tuning the values of delta(i) numbers
in case.inM before starting the min_lapw.

thanking you in advance for suggestion/s.

Regards
sahu



 

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Date: Sat, 4 Jan 2003 08:40:49 -0800 (PST)
From: Hadi Arabi <arabi_h@yahoo.com>
Subject: [WIEN]: force minimizung

====
Hadi Arabi <arabi_h@yahoo.com>
submitted the following contribution:
====

Dear wien user
I work on Re-123 high temperature superconductor
materials which has 13 atoms in unit cell.In order to
start analysise we have to minimize the forces upon
the atoms which end up with the following amount of
forces in Z-direction:
Force on atom No.2 =0.239
Force on atom No.4 =0.495
Force on atom No.5=-0.241
Force on atom No.6=0.54
force on atom No.7 = 0.34
The forces on the rest of the atoms are zero.
My question is:
Can I start analysis with this kind of forces on atom?
Because I tried to change the positions of the atoms
to reduce the forces, but some of them reduce and some
other again increase. What can I do for this problem?
Best regard
Hadi 


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Date: Sat, 4 Jan 2003 20:49:34 -0500 (EST)
From: Dadi Dai <dai@unity.ncsu.edu>
Subject: [WIEN]: Why does LDA+U stop at the second cycle?

====
Dadi Dai <dai@unity.ncsu.edu>
submitted the following contribution:
====

I wish to do LDA+U calculation for Cu4O3.  I used "runsp -orb", and the
calculation stopped at the beginning of the second cycle.  I don't know
why and hope to get some help.

The error message is:
....................cycle 1...................
STOP  LAPW0 END
STOP  LAPW1 END
STOP  LAPW1 END
STOP  LAPW2 END
STOP  LAPW2 END
STOP  lapwdm END
STOP  lapwdm END
STOP  CORE  END
STOP  CORE  END
STOP  MIXER END
..............cycle 2..................
STOP  LAPW0 END
1525-001 The READ statement on the file Cu4O3.dmatup cannot be completed
because the end of the file was reached.  The program will stop.

I found the file "uporb.error" that shows "Error in Vorb".  The :log file
shows:
>   (runsp) options: -orb -i 40 -cc 0.0001
Fri Jan  3 15:56:23 EST 2003> (x) lapw0
Fri Jan  3 15:57:02 EST 2003> (x) lapw1 -up -orb
Fri Jan  3 16:11:31 EST 2003> (x) lapw1 -dn -orb
Fri Jan  3 16:25:58 EST 2003> (x) lapw2 -up
Fri Jan  3 16:27:31 EST 2003> (x) lapw2 -dn
Fri Jan  3 16:29:00 EST 2003> (x) lapwdm -up
Fri Jan  3 16:29:05 EST 2003> (x) lapwdm -dn
Fri Jan  3 16:29:09 EST 2003> (x) lcore -up
Fri Jan  3 16:29:10 EST 2003> (x) lcore -dn
Fri Jan  3 16:29:11 EST 2003> (x) mixer
Fri Jan  3 16:29:16 EST 2003> (x) lapw0
Fri Jan  3 16:29:57 EST 2003> (x) orb -up


The Cu4O3.inorb that I used is:
1  2  0
BROYD 0.25
1 1 2
2 1 2
1
0.55127 0.055127   U,J
0.55127 0.055127   U,J

The Cu4O3.indm that I used is:
- -9.0
2
1 1 2
1 1 2
0 0

I wonder if the inputs are correct.  Could anyone help me?

Thank you very much!

Dadi Dai

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------------------------------

Date: Mon, 6 Jan 2003 12:42:45 +0800
From: "yulihua" <yulihua-wuhan@sohu.com>
Subject: [WIEN]: case.in2 for electron density plots

====
"yulihua" <yulihua-wuhan@sohu.com>
submitted the following contribution:
====

This is a multi-part message in MIME format.

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Date: Mon, 6 Jan 2003 09:12:42 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: force minimizung

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Your forces are very small.  You should be able to analyze  your system this
way.

kind regards,

Kevin Jorissen.

- ----- Original Message -----
From: "Hadi Arabi" <arabi_h@yahoo.com>
To: <wien@zeus.theochem.tuwien.ac.at>
Cc: <arabi_h@yahoo.com>
Sent: Saturday, January 04, 2003 5:40 PM
Subject: [WIEN]: force minimizung


> ====
> Hadi Arabi <arabi_h@yahoo.com>
> submitted the following contribution:
> ====
>
> Dear wien user
> I work on Re-123 high temperature superconductor
> materials which has 13 atoms in unit cell.In order to
> start analysise we have to minimize the forces upon
> the atoms which end up with the following amount of
> forces in Z-direction:
> Force on atom No.2 =0.239
> Force on atom No.4 =0.495
> Force on atom No.5=-0.241
> Force on atom No.6=0.54
> force on atom No.7 = 0.34
> The forces on the rest of the atoms are zero.
> My question is:
> Can I start analysis with this kind of forces on atom?
> Because I tried to change the positions of the atoms
> to reduce the forces, but some of them reduce and some
> other again increase. What can I do for this problem?
> Best regard
> Hadi
>
>
> __________________________________________________
> Do you Yahoo!?
> Yahoo! Mail Plus - Powerful. Affordable. Sign up now.
> http://mailplus.yahoo.com
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

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------------------------------

Date: Mon, 06 Jan 2003 16:49:23 +0800
From: "liu wan" <wien97wan@hotmail.com>
Subject: [WIEN]: question about how to use OPTIC

====
"liu wan" <wien97wan@hotmail.com>
submitted the following contribution:
====

Dear All

I try to calculated the optical properties of a semi-conductor. But I find 
that the reult in the case.joint is: Some position is very large and the 
other position is zero. What is wrong?

2
   Energy  [eV]     Im_eps_xx          Im_eps_zz

      0.00000     0.84051298E+89     0.00000000E+00
      0.01361     0.17131700E-07     0.00000000E+00
      0.02721     0.10498127+277     0.00000000E+00
      0.04082     0.22762560E-16     0.00000000E+00
      0.05442     0.66295283E-08     0.00000000E+00
      0.06803     0.15973640+272     0.00000000E+00
      0.08163     0.21894908E-16     0.00000000E+00
      0.09524     0.21233672-152     0.00000000E+00
      0.10885     0.44776644+218     0.00000000E+00
      0.12245     0.51962383E+46     0.00000000E+00
      0.13606     0.46566129E-09     0.00000000E+00
      0.14966     0.00000000E+00     0.00000000E+00
      0.16327     0.00000000E+00     0.00000000E+00
      0.17687     0.00000000E+00     0.00000000E+00

Best wish

Liu

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Date: Mon, 6 Jan 2003 10:47:36 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: Compiling TELNES

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

People have had problems like this before (though I think it's been a long
time since I read about it, maybe there's more in the mail digest).
Try replacing all the real statements by double precisions, i.e.
DBLE(blabla) instead of REAL(blabla).  You will probably be able to compile
the program afterwards.

kind regards,

Kevin Jorissen
kevin.jorissen@ua.ac.be

- ----- Original Message -----
From: "Gabriela Fernanda Cabeza" <gcabeza@criba.edu.ar>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Friday, January 03, 2003 11:22 PM
Subject: [WIEN]: Compiling TELNES


> ====
> Gabriela Fernanda Cabeza <gcabeza@criba.edu.ar>
> submitted the following contribution:
> ====
>
> Dear Wien users,
>
> When recompiling TELNES on a Linux box with g77 (recommended) i got the
> following
> error file (compile.msg) at SRC_telnes directory:
>
> --------------------------------------------------------------------------
- -
>
> g77 -O -c telnes.f
> telnes.f: In subroutine `firstcase':
> telnes.f:2080:
> + REAL(Factor1*Factor2*Factor3*Factor4)
> ^
> Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
> telnes.f:2085:
> + REAL(Factor1*Factor2*Factor3*Factor4)
> ^
> Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
> telnes.f: In subroutine `secondcase':
> telnes.f:2143:
> + REAL(Factor1*Factor2*Factor3*Factor4)
> ^
> Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
> telnes.f:2148:
> + REAL(Factor1*Factor2*Factor3*Factor4)
> ^
> Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
> make: *** [telnes.o] Error 1
>
> --------------------------------------------------------------------------
- -
>
> Has anybody had the same errors?
>
> Thank you very much in advance for every hint.
> Kind regards
>
>
>
>
> Dra. Gabriela F. Cabeza
> Profesora Adjunta
> Dpto. de Física - Universidad Nacional del Sur
> Avda. Alem 1253, (B8000CPB) Bahía Blanca - Argentina
> tel: 54-291- 4595141- 54-291-4595101, int. 2821
> fax: 54-291-4595142
> e-mail: gcabeza@criba.edu.ar
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

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------------------------------

Date: Mon, 6 Jan 2003 10:56:04 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: Compiling TELNES

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Hello again,

I found this in the archives, first a question by Nitya Nath Shukla, a reply
by Joachim Luitz, and a comment by some guy named Andrew.

In case you are using an old wien version, why not upgrade to WIEN2k?  It's
faster, has more features, and you'll get the hang of it in no time.  The
telnes part is still the same as in wien97.

good luck!

Kevin Jorissen
kevin.jorissen@ua.ac.be


Date: Mon, 19 Jun 2000 17:13:27 +0530 (IST)
From: Nitya Nath Shukla phd phy <nitya@iitk.ac.in>
Subject: [WIEN]: Errors in compilation

====
Nitya Nath Shukla phd phy <nitya@iitk.ac.in>
submitted the following contribution:
====

Respected Sir,

I am getting this error in compilation.
I am using Linux Redhat 6.1 OS.


g77  -O -c kram.f
kram.f: In program `kram':
kram.f:233:
         write(12,113) xe(i),(real(eps(i,j)),imag(eps(i,j)),j=1,ncol)
                              ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
kram.f:234:
         write(13,113) xe(i),(real(sig(i,j)),imag(sig(i,j)),j=1,ncol)
                              ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
kram.f:235:
         write(14,113) xe(i),(real(sig(i,j))*sigf1/sigf,j=1,ncol),
                              ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
make: *** [kram.o] Error 1


g77  -O -c telnes.f
telnes.f: In subroutine `cspech':
telnes.f:1857:
        +                                      + REAL (Factor3 * Factor4)
                                                 ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:1869:
        +          REAL (Factor3 * Factor4)
                   ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:1875:
        +          REAL (Factor3 * Factor4)
                   ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:1878:
        +          REAL (Factor3 * Factor4)
                   ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:1881:
        +          REAL (Factor3 * Factor4)
                   ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:1890:
        +          REAL (Factor3 * Factor4)
                   ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:1893:
        +          REAL (Factor3 * Factor4)
                   ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:1900:
        +          REAL (Factor3 * Factor4)
                   ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:1903:
        +          REAL (Factor3 * Factor4)
                   ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:1907:
        +            REAL (Factor3 * Factor4)
                     ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:1910:
        +            REAL (Factor3 * Factor4)
                     ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:1915:
        +            REAL (Factor3 * Factor4)
                     ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:1918:
        +            REAL (Factor3 * Factor4)
                     ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f: In subroutine `firstcase':
telnes.f:2080:
        +                     REAL(Factor1*Factor2*Factor3*Factor4)
                              ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:2085:
        +           REAL(Factor1*Factor2*Factor3*Factor4)
                    ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f: In subroutine `secondcase':
telnes.f:2143:
        +                     REAL(Factor1*Factor2*Factor3*Factor4)
                              ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:2148:
        +           REAL(Factor1*Factor2*Factor3*Factor4)
                    ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
make: *** [telnes.o] Error 1

Is this problem of compiles or somthing else...
 With regards..
  Nitya Nath

**************************************************************

 Nitya Nath Shukla                  HOSTEL: C-209,Hall - 5,
                                            I.I.T. KANPUR-208016
 Physics Deptt.                     Phone : 0512 - 597115
 Indian Institute Of Technology             0512 - 597315
 Kanpur - UP.                       Email- nitsu@mailcity.com
 INDIA                                   - nitya@iitk.ac.in
 Pin - 208016
                      Resi: 1313,Ratan Lal Nagar
                 Kanpur - 208022
               Phone:(0512)-280445
 ************************************************************

ANSWER

I guess you are using an older version of WIEN. In WIEN97.9 these
statements have been changed to DBLE, which should compile on all F77
compilers.

You can also change the REAL(...) statements to DBLE(...) by hand in the
routines kram.f and telnes.f

> Is this problem of compiles or somthing else...

Compilation, indeed.


Best regards

Joachim Luitz

"Recursion n.: See Recursion. -- Random Shack Data Processing Dictionary "

- - --
 ---------------------------------------------------------------------
| Dipl.-Ing. Joachim Luitz        | j.luitz@tuwien.ac.at              |
| Vienna University of Technology | http://www.tuwien.ac.at/theochem  |
| Inst. of Physical and           | Tel: +43 1 58801-15679            |
|          Theoretical Chemistry  | Fax: +43 1 58801-15698            |
| Getreidemarkt 9/156             |                                   |
| A-1060 Wien/AUSTRIA             | private: jluitz@music.at          |
 ---------------------------------------------------------------------


COMMENT

telnes.f: In subroutine `firstcase':
telnes.f:2080:
        +                     REAL(Factor1*Factor2*Factor3*Factor4)
                              ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f:2085:
        +           REAL(Factor1*Factor2*Factor3*Factor4)
                    ^
Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
telnes.f: In subroutine `secondcase':
telnes.f:2143:
        +                     REAL(Factor1*Factor2*Factor3*Factor4)
                              ^
- - --------------------------------------------------------------------------
- --

Changing these explicitely to DREAL seems to solve this problem.

Sorry about the trouble!

Cheers,

Andrew



- ----- Original Message -----
From: "Gabriela Fernanda Cabeza" <gcabeza@criba.edu.ar>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Friday, January 03, 2003 11:22 PM
Subject: [WIEN]: Compiling TELNES


> ====
> Gabriela Fernanda Cabeza <gcabeza@criba.edu.ar>
> submitted the following contribution:
> ====
>
> Dear Wien users,
>
> When recompiling TELNES on a Linux box with g77 (recommended) i got the
> following
> error file (compile.msg) at SRC_telnes directory:
>
> --------------------------------------------------------------------------
- -
>
> g77 -O -c telnes.f
> telnes.f: In subroutine `firstcase':
> telnes.f:2080:
> + REAL(Factor1*Factor2*Factor3*Factor4)
> ^
> Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
> telnes.f:2085:
> + REAL(Factor1*Factor2*Factor3*Factor4)
> ^
> Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
> telnes.f: In subroutine `secondcase':
> telnes.f:2143:
> + REAL(Factor1*Factor2*Factor3*Factor4)
> ^
> Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
> telnes.f:2148:
> + REAL(Factor1*Factor2*Factor3*Factor4)
> ^
> Ambiguous use of intrinsic `REAL' at (^) [info -f g77 M CMPAMBIG]
> make: *** [telnes.o] Error 1
>
> --------------------------------------------------------------------------
- -
>
> Has anybody had the same errors?
>
> Thank you very much in advance for every hint.
> Kind regards
>
>
>
>
> Dra. Gabriela F. Cabeza
> Profesora Adjunta
> Dpto. de Física - Universidad Nacional del Sur
> Avda. Alem 1253, (B8000CPB) Bahía Blanca - Argentina
> tel: 54-291- 4595141- 54-291-4595101, int. 2821
> fax: 54-291-4595142
> e-mail: gcabeza@criba.edu.ar
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

====
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------------------------------

Date: Mon, 06 Jan 2003 05:16:26 -0500
From: "michel certier" <mcertier@mail.com>
Subject: [WIEN]: parallel execution problem in dual PIV

====
"michel certier" <mcertier@mail.com>
submitted the following contribution:
====

Dear wien users Happy New year !!!
I met somme problem to execut a parallel job for cubic system with 35 k-point on dual machine, after 1 iteration the program stop and I get the following message:
 
LAPW0 END
 LAPW1 END
 LAPW1 END
LAPW2 - FERMI; weighs written
 LAPW2 END
 LAPW2 END
 SUMPARA END
 SUMPARA END
 CORE  END
 MIXER END
in cycle 2    ETEST: 0   CTEST: 0
PGFIO-F-231/formatted read/unit=8/error on data conversion.
 File name = test.clmsum    formatted, sequential access   record = 2223
 In source file lapw0.F, at line number 404
cat: No match.
My .machines files is :

granularity:1
17:localhost
18:localhost
The program run well in serial mode.
Can some one give me a solution to this problem.
Thank's 

- -- 
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------------------------------

Date: Mon, 6 Jan 2003 13:20:47 +0100
From: Veerle Vanhoof <Veerle.Vanhoof@fys.kuleuven.ac.be>
Subject: [WIEN]: Problems with crystalstructure

====
Veerle Vanhoof <Veerle.Vanhoof@fys.kuleuven.ac.be>
submitted the following contribution:
====


- --------------Boundary-00=_NYKADNVGGDOGX0XT3IVL
Content-Type: text/plain;
  charset="us-ascii"
Content-Transfer-Encoding: quoted-printable

Dear wien2k user,

When I try to make a crystalstructure consisting of 29 Ag-atoms and 3=20
Co-atoms, all positioned in a supercell (8 fcc-cubes placed to form a=20
supercube with as latticeconstantes twice the ones of Ag-fcc) and the Co'=
s=20
positioned at coordinates (0, 0, 0), (0.25, 0.25, 0), (0.5, 0, 0.5), or o=
n=20
equivalent positions, sgroup suggests a "better" struct-file. But when I=20
accept this new struct-file there appears to be an inconsistency in the=20
suggested structure.=20
*.outputsgroup starts with the following warningmessage:
"warning: !!! Struct file is not consistent with space group found."

Ignoring this inconsistency and using an RK_max of 5.0 runs but ends up w=
ith=20
forces that diverge rather than converge for almost all inequivalent atom=
s.
A typical example of this divergence:

atom 1 x-component: 5.597 / 5.925 / 6.614 / 7.687 / 8.836 / 10.310 / 11.8=
68 /=20
13.518 / 15.612 / 12.750 / 21.586 / 24.271 / 28.551 / 31.127 / 44.334

Almost all the other atoms behave like atom 1, the exceptions (1 or 2 ato=
ms)=20
had already very low forces to start with:

atom 23 x-component: 0.383 / 0.374 / 0.405 / 0.462 / 0.462 / 0.478 / 0.55=
4 /=20
0.541 / 0.564 / 1.728 / 0.695 / 0.442 / 0.891 / 0.961 / 0.897=20
          z-component: 0.303 / 0.294 / 0.328 / 0.378 / 0.396 / 0.422 / 0.=
513 /=20
0.522 / 0.591 / 1.680 / 0.545 / 0.166 / 0.574 / 0.544 / 0.247

But the components that, more or less, converge are already fixed (veloci=
ty 0)=20
in name.inM.

I have made 7 other calculations with the 3th Co on a different=20
(nonequivalent) position without any problems at all. It's only this=20
configuration that gives these problems.

The used *.struct-, *.inst-file, *.outputsgroup and *.inM-file are in=20
attachement.

Does somebody know what the problem can be?=20

Thanks a lot!

Veerle Vanhoof
Institute for nuclear and radiation fysics
Department of Physics
Catholic University of Leuven
Belgium


- --------------Boundary-00=_NYKADNVGGDOGX0XT3IVL
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  charset="us-ascii";
  name="agcork5.inst"
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Co 1       
Ar 3 5
3, 2,2.0  N
3, 2,2.0  N
3,-3,3.0  N
3,-3,0.0  N
4,-1,1.0  N
4,-1,1.0  N
Co 1       
Ar 3 5
3, 2,2.0  N
3, 2,2.0  N
3,-3,3.0  N
3,-3,0.0  N
4,-1,1.0  N
4,-1,1.0  N
Co 1       
Ar 3 5
3, 2,2.0  N
3, 2,2.0  N
3,-3,3.0  N
3,-3,0.0  N
4,-1,1.0  N
4,-1,1.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
Ag 1       
Kr 3 5
4, 2,2.0  N
4, 2,2.0  N
4,-3,3.0  N
4,-3,3.0  N
5,-1,1.0  N
5,-1,0.0  N
****     End of Input
****     End of Input

- --------------Boundary-00=_NYKADNVGGDOGX0XT3IVL
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  charset="us-ascii";
  name="agcork5.inM"
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NEWT 1.0           #(NOSE, NEWT, BFGS, MOLD, tolf (a4,f5.2))
1.0 1.0 0.0 0.8    # Atom1   (NOSE, MOLD:Masse, delta t, T, nose-frequency)
1.0 1.0 0.0 0.8    # Atom2   (NEWT: 1,2,3:delta, 4:eta(1=MOLD))
0.0 0.0 0.0 0.8    # Atom3   (BFGS, NEWT: [ 1 || 2 || 3 ] = 0 constraint)
1.0 1.0 0.0 0.8    # Atom4
1.0 1.0 0.0 0.8    # Atom5
0.0 0.0 0.0 0.8    # Atom6
1.0 1.0 0.0 0.8    # Atom7
0.0 0.0 0.0 0.8    # Atom8
1.0 1.0 1.0 0.8    # Atom9
1.0 0.0 1.0 0.8    # Atom10
1.0 1.0 0.0 0.8    # Atom11
1.0 1.0 0.0 0.8    # Atom12
1.0 0.0 1.0 0.8    # Atom13
0.0 0.0 0.0 0.8    # Atom14
1.0 1.0 0.0 0.8    # Atom15
1.0 1.0 0.0 0.8    # Atom16
1.0 1.0 0.0 0.8    # Atom17
1.0 1.0 0.0 0.8    # Atom18
1.0 1.0 0.0 0.8    # Atom19
1.0 1.0 0.0 0.8    # Atom20
1.0 0.0 1.0 0.8    # Atom21
1.0 0.0 1.0 0.8    # Atom22
0.0 0.0 0.0 0.8    # Atom23
0.0 0.0 0.0 0.8    # Atom24


- --------------Boundary-00=_NYKADNVGGDOGX0XT3IVL
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AgCo                                                                           
P   LATTICE,NONEQUIV. ATOMS:24 6 Pm                                            
             RELA                                                              
 22.024507 22.024507 22.024507 90.000000 90.000000 90.000000                   
ATOM= -1: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT= 8
Co1        NPT=  781  R0=0.00010000 RMT=    2.2500   Z: 27.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -2: X=0.25000000 Y=0.25000000 Z=0.00000000
          MULT= 1          ISPLIT= 8
Co2        NPT=  781  R0=0.00010000 RMT=    2.2500   Z: 27.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -3: X=0.00000000 Y=0.50000000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Co3        NPT=  781  R0=0.00010000 RMT=    2.2500   Z: 27.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -4: X=0.50000000 Y=0.00000000 Z=0.00000000
          MULT= 1          ISPLIT= 8
Ag1        NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -5: X=0.00000000 Y=0.50000000 Z=0.00000000
          MULT= 1          ISPLIT= 8
Ag2        NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -6: X=0.00000000 Y=0.00000000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Ag3        NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -7: X=0.50000000 Y=0.50000000 Z=0.00000000
          MULT= 1          ISPLIT= 8
Ag4        NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -8: X=0.50000000 Y=0.00000000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Ag5        NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -9: X=0.25000000 Y=0.00000000 Z=0.25000000
          MULT= 2          ISPLIT= 8
      -9: X=0.25000000 Y=0.00000000 Z=0.75000000
Ag6        NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-10: X=0.75000000 Y=0.00000000 Z=0.25000000
          MULT= 2          ISPLIT= 8
     -10: X=0.75000000 Y=0.00000000 Z=0.75000000
Ag7        NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-11: X=0.75000000 Y=0.25000000 Z=0.00000000
          MULT= 1          ISPLIT= 8
Ag8        NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-12: X=0.25000000 Y=0.75000000 Z=0.00000000
          MULT= 1          ISPLIT= 8
Ag9        NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-13: X=0.00000000 Y=0.25000000 Z=0.25000000
          MULT= 2          ISPLIT= 8
     -13: X=0.00000000 Y=0.25000000 Z=0.75000000
Ag10       NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-14: X=0.00000000 Y=0.75000000 Z=0.25000000
          MULT= 2          ISPLIT= 8
     -14: X=0.00000000 Y=0.75000000 Z=0.75000000
Ag11       NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-15: X=0.75000000 Y=0.75000000 Z=0.00000000
          MULT= 1          ISPLIT= 8
Ag12       NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-16: X=0.25000000 Y=0.25000000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Ag13       NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-17: X=0.25000000 Y=0.75000000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Ag14       NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-18: X=0.75000000 Y=0.25000000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Ag15       NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-19: X=0.75000000 Y=0.75000000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Ag16       NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-20: X=0.25000000 Y=0.50000000 Z=0.25000000
          MULT= 2          ISPLIT= 8
     -20: X=0.25000000 Y=0.50000000 Z=0.75000000
Ag17       NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-21: X=0.75000000 Y=0.50000000 Z=0.25000000
          MULT= 2          ISPLIT= 8
     -21: X=0.75000000 Y=0.50000000 Z=0.75000000
Ag18       NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-22: X=0.50000000 Y=0.25000000 Z=0.25000000
          MULT= 2          ISPLIT= 8
     -22: X=0.50000000 Y=0.25000000 Z=0.75000000
Ag19       NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-23: X=0.50000000 Y=0.75000000 Z=0.25000000
          MULT= 2          ISPLIT= 8
     -23: X=0.50000000 Y=0.75000000 Z=0.75000000
Ag20       NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM=-24: X=0.50000000 Y=0.50000000 Z=0.50000000
          MULT= 1          ISPLIT= 8
Ag21       NPT=  781  R0=0.00010000 RMT=    2.4000   Z: 47.0                   
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
   2      NUMBER OF SYMMETRY OPERATIONS
 1 0 0 0.0000000
 0 1 0 0.0000000
 0 0 1 0.0000000
       1
 1 0 0 0.0000000
 0 1 0 0.0000000
 0 0-1 0.0000000
       2

- --------------Boundary-00=_NYKADNVGGDOGX0XT3IVL
Content-Type: text/plain;
  charset="us-ascii";
  name="agcork5.outputsgroup"
Content-Transfer-Encoding: 7bit
Content-Disposition: attachment; filename="agcork5.outputsgroup"

warning: !!! Struct file is not consistent with space group found.

- ----------------------------------------------------------------------

Bravais lattice: Monoclinic primitive

     a             b            c
 22.02450700    22.02450700   22.02450700
     alpha         beta         gamma
 90.00000000    90.00000000   90.00000000


===== Decomposition of new basis vectors over input basis =====
 1.000000   0.000000  0.000000  <--- 1
 0.000000   1.000000  0.000000  <--- 2
 0.000000   0.000000  1.000000  <--- 3

==== Number of atoms in cell: 32
==== Atom positions:

 0.00000000   0.00000000  0.00000000
 Co1

 0.25000000   0.25000000  0.00000000
 Co2

 0.00000000   0.50000000  0.50000000
 Co3

 0.50000000   0.00000000  0.00000000
 Ag1

 0.00000000   0.50000000  0.00000000
 Ag2

 0.00000000   0.00000000  0.50000000
 Ag3

 0.50000000   0.50000000  0.00000000
 Ag4

 0.50000000   0.00000000  0.50000000
 Ag5

 0.25000000   0.00000000  0.25000000
 Ag6
 0.25000000   0.00000000  0.75000000
 Ag6

 0.75000000   0.00000000  0.25000000
 Ag7
 0.75000000   0.00000000  0.75000000
 Ag7

 0.75000000   0.25000000  0.00000000
 Ag8

 0.25000000   0.75000000  0.00000000
 Ag9

 0.00000000   0.25000000  0.25000000
 Ag10
 0.00000000   0.25000000  0.75000000
 Ag10

 0.00000000   0.75000000  0.25000000
 Ag11
 0.00000000   0.75000000  0.75000000
 Ag11

 0.75000000   0.75000000  0.00000000
 Ag12

 0.25000000   0.25000000  0.50000000
 Ag13

 0.25000000   0.75000000  0.50000000
 Ag14

 0.75000000   0.25000000  0.50000000
 Ag15

 0.75000000   0.75000000  0.50000000
 Ag16

 0.25000000   0.50000000  0.25000000
 Ag17
 0.25000000   0.50000000  0.75000000
 Ag17

 0.75000000   0.50000000  0.25000000
 Ag18
 0.75000000   0.50000000  0.75000000
 Ag18

 0.50000000   0.25000000  0.25000000
 Ag19
 0.50000000   0.25000000  0.75000000
 Ag19

 0.50000000   0.75000000  0.25000000
 Ag20
 0.50000000   0.75000000  0.75000000
 Ag20

 0.50000000   0.50000000  0.50000000
 Ag21

==== Number of nonequivalent sorts: 24
==== Nonequivalent atoms, point group for each sort: ====

Sort number: 1
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.00000000   0.00000000  0.00000000
   Co1

Sort number: 2
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.25000000   0.25000000  0.00000000
   Co2

Sort number: 3
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.00000000   0.50000000  0.50000000
   Co3

Sort number: 4
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.50000000   0.00000000  0.00000000
   Ag1

Sort number: 5
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.00000000   0.50000000  0.00000000
   Ag2

Sort number: 6
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.00000000   0.00000000  0.50000000
   Ag3

Sort number: 7
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.50000000   0.50000000  0.00000000
   Ag4

Sort number: 8
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.50000000   0.00000000  0.50000000
   Ag5

Sort number: 9
  Names of point group: 1      1      C1
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 2
   0.25000000   0.00000000  0.25000000
   Ag6
   0.25000000   0.00000000  0.75000000
   Ag6

Sort number: 10
  Names of point group: 1      1      C1
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 2
   0.75000000   0.00000000  0.25000000
   Ag7
   0.75000000   0.00000000  0.75000000
   Ag7

Sort number: 11
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.75000000   0.25000000  0.00000000
   Ag8

Sort number: 12
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.25000000   0.75000000  0.00000000
   Ag9

Sort number: 13
  Names of point group: 1      1      C1
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 2
   0.00000000   0.25000000  0.25000000
   Ag10
   0.00000000   0.25000000  0.75000000
   Ag10

Sort number: 14
  Names of point group: 1      1      C1
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 2
   0.00000000   0.75000000  0.25000000
   Ag11
   0.00000000   0.75000000  0.75000000
   Ag11

Sort number: 15
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.75000000   0.75000000  0.00000000
   Ag12

Sort number: 16
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.25000000   0.25000000  0.50000000
   Ag13

Sort number: 17
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.25000000   0.75000000  0.50000000
   Ag14

Sort number: 18
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.75000000   0.25000000  0.50000000
   Ag15

Sort number: 19
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.75000000   0.75000000  0.50000000
   Ag16

Sort number: 20
  Names of point group: 1      1      C1
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 2
   0.25000000   0.50000000  0.25000000
   Ag17
   0.25000000   0.50000000  0.75000000
   Ag17

Sort number: 21
  Names of point group: 1      1      C1
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 2
   0.75000000   0.50000000  0.25000000
   Ag18
   0.75000000   0.50000000  0.75000000
   Ag18

Sort number: 22
  Names of point group: 1      1      C1
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 2
   0.50000000   0.25000000  0.25000000
   Ag19
   0.50000000   0.25000000  0.75000000
   Ag19

Sort number: 23
  Names of point group: 1      1      C1
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 2
   0.50000000   0.75000000  0.25000000
   Ag20
   0.50000000   0.75000000  0.75000000
   Ag20

Sort number: 24
  Names of point group: m      m      Cs
  New basis vectors for this point group:
    1.0000   0.0000  0.0000  <--- 1
    0.0000   1.0000  0.0000  <--- 2
    0.0000   0.0000  1.0000  <--- 3

  Atom positions: 1
   0.50000000   0.50000000  0.50000000
   Ag21

======================================================================

Number and name of space group: 6 (P m) [unique axis c]
- - Short - Full - Schoenflies - names of point group:
 m      m      Cs

Number of symmetry operations: 2
Operation: 1
 1.0   0.0   0.0  0.000
 0.0   1.0   0.0  0.000
 0.0   0.0   1.0  0.000

Operation: 2
 1.0   0.0   0.0  0.000
 0.0   1.0   0.0  0.000
 0.0   0.0  -1.0  0.000

============================================================
Note that shift vectors for this space group are defined
only up to the vector { X, Y, 0 }.
Here X and Y can take any values.

===== Number of possible shift vectors: 2 =====
===== List of shift vectors:
 0.0000   0.0000   0.0000
 0.0000   0.0000   0.5000

List of shifted cells:

Cell #1 
  Shift vector:  0.0000   0.0000   0.5000
  Nonequivalent atoms :

 0.00000000   0.00000000  0.50000000
 Co1

 0.25000000   0.25000000  0.50000000
 Co2

 0.00000000   0.50000000  0.00000000
 Co3

 0.50000000   0.00000000  0.50000000
 Ag1

 0.00000000   0.50000000  0.50000000
 Ag2

 0.00000000   0.00000000  0.00000000
 Ag3

 0.50000000   0.50000000  0.50000000
 Ag4

 0.50000000   0.00000000  0.00000000
 Ag5

 0.25000000   0.00000000  0.75000000
 Ag6
 0.25000000   0.00000000  0.25000000
 Ag6

 0.75000000   0.00000000  0.75000000
 Ag7
 0.75000000   0.00000000  0.25000000
 Ag7

 0.75000000   0.25000000  0.50000000
 Ag8

 0.25000000   0.75000000  0.50000000
 Ag9

 0.00000000   0.25000000  0.75000000
 Ag10
 0.00000000   0.25000000  0.25000000
 Ag10

 0.00000000   0.75000000  0.75000000
 Ag11
 0.00000000   0.75000000  0.25000000
 Ag11

 0.75000000   0.75000000  0.50000000
 Ag12

 0.25000000   0.25000000  0.00000000
 Ag13

 0.25000000   0.75000000  0.00000000
 Ag14

 0.75000000   0.25000000  0.00000000
 Ag15

 0.75000000   0.75000000  0.00000000
 Ag16

 0.25000000   0.50000000  0.75000000
 Ag17
 0.25000000   0.50000000  0.25000000
 Ag17

 0.75000000   0.50000000  0.75000000
 Ag18
 0.75000000   0.50000000  0.25000000
 Ag18

 0.50000000   0.25000000  0.75000000
 Ag19
 0.50000000   0.25000000  0.25000000
 Ag19

 0.50000000   0.75000000  0.75000000
 Ag20
 0.50000000   0.75000000  0.25000000
 Ag20

 0.50000000   0.50000000  0.00000000
 Ag21

- --------------Boundary-00=_NYKADNVGGDOGX0XT3IVL--

====
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------------------------------

Date: Mon, 6 Jan 2003 05:20:08 -0800 (PST)
From: romdhani hedi <hedi_romdhani2002@yahoo.com>
Subject: Re: [WIEN]: Compiling TELNES

====
romdhani hedi <hedi_romdhani2002@yahoo.com>
submitted the following contribution:
====


- --- Gabriela Fernanda Cabeza <gcabeza@criba.edu.ar>
wrote:
> ====
> Gabriela Fernanda Cabeza <gcabeza@criba.edu.ar>
> submitted the following contribution:
> ====
> 
> Dear Wien users,
> 
> When recompiling TELNES on a Linux box with g77
> (recommended) i got the 
> following
> error file (compile.msg) at SRC_telnes directory:
> 
>
- ---------------------------------------------------------------------------
> 
> g77 -O -c telnes.f
> telnes.f: In subroutine `firstcase':
> telnes.f:2080:
> + REAL(Factor1*Factor2*Factor3*Factor4)
> ^
> Ambiguous use of intrinsic `REAL' at (^) [info -f
> g77 M CMPAMBIG]
> telnes.f:2085:
> + REAL(Factor1*Factor2*Factor3*Factor4)
> ^
> Ambiguous use of intrinsic `REAL' at (^) [info -f
> g77 M CMPAMBIG]
> telnes.f: In subroutine `secondcase':
> telnes.f:2143:
> + REAL(Factor1*Factor2*Factor3*Factor4)
> ^
> Ambiguous use of intrinsic `REAL' at (^) [info -f
> g77 M CMPAMBIG]
> telnes.f:2148:
> + REAL(Factor1*Factor2*Factor3*Factor4)
> ^
> Ambiguous use of intrinsic `REAL' at (^) [info -f
> g77 M CMPAMBIG]
> make: *** [telnes.o] Error 1
> 
>
- ---------------------------------------------------------------------------
> 
> Has anybody had the same errors?
> 
> Thank you very much in advance for every hint.
> Kind regards
> 
> 
> 
> 
> Dra. Gabriela F. Cabeza
> Profesora Adjunta
> Dpto. de Física - Universidad Nacional del Sur
> Avda. Alem 1253, (B8000CPB) Bahía Blanca - Argentina
> tel: 54-291- 4595141- 54-291-4595101, int. 2821
> fax: 54-291-4595142
> e-mail: gcabeza@criba.edu.ar
> 
> ====
Dear Gabriela, 
 please replace "real" with "dreal" in kram.f and
telnes.f subroutines.
With best regards.

__________________________________________________
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====
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------------------------------

Date: Mon, 6 Jan 2003 05:43:10 -0800 (PST)
From: romdhani hedi <hedi_romdhani2002@yahoo.com>
Subject: Re: [WIEN]: Problems with crystalstructure

====
romdhani hedi <hedi_romdhani2002@yahoo.com>
submitted the following contribution:
====


- --- Veerle Vanhoof <Veerle.Vanhoof@fys.kuleuven.ac.be>
wrote:
> Dear wien2k user,
> 
> When I try to make a crystalstructure consisting of
> 29 Ag-atoms and 3 
> Co-atoms, all positioned in a supercell (8 fcc-cubes
> placed to form a 
> supercube with as latticeconstantes twice the ones
> of Ag-fcc) and the Co's 
> positioned at coordinates (0, 0, 0), (0.25, 0.25,
> 0), (0.5, 0, 0.5), or on 
> equivalent positions, sgroup suggests a "better"
> struct-file. But when I 
> accept this new struct-file there appears to be an
> inconsistency in the 
> suggested structure. 
> *.outputsgroup starts with the following
> warningmessage:
> "warning: !!! Struct file is not consistent with
> space group found."
> 
> Ignoring this inconsistency and using an RK_max of
> 5.0 runs but ends up with 
> forces that diverge rather than converge for almost
> all inequivalent atoms.
> A typical example of this divergence:
> 
> atom 1 x-component: 5.597 / 5.925 / 6.614 / 7.687 /
> 8.836 / 10.310 / 11.868 / 
> 13.518 / 15.612 / 12.750 / 21.586 / 24.271 / 28.551
> / 31.127 / 44.334
> 
> Almost all the other atoms behave like atom 1, the
> exceptions (1 or 2 atoms) 
> had already very low forces to start with:
> 
> atom 23 x-component: 0.383 / 0.374 / 0.405 / 0.462 /
> 0.462 / 0.478 / 0.554 / 
> 0.541 / 0.564 / 1.728 / 0.695 / 0.442 / 0.891 /
> 0.961 / 0.897 
>           z-component: 0.303 / 0.294 / 0.328 / 0.378
> / 0.396 / 0.422 / 0.513 / 
> 0.522 / 0.591 / 1.680 / 0.545 / 0.166 / 0.574 /
> 0.544 / 0.247
> 
> But the components that, more or less, converge are
> already fixed (velocity 0) 
> in name.inM.
> 
> I have made 7 other calculations with the 3th Co on
> a different 
> (nonequivalent) position without any problems at
> all. It's only this 
> configuration that gives these problems.
> 
> The used *.struct-, *.inst-file, *.outputsgroup and
> *.inM-file are in 
> attachement.
> 
> Does somebody know what the problem can be? 
> 
> Thanks a lot!
> 
> Veerle Vanhoof
> Institute for nuclear and radiation fysics
> Department of Physics
> Catholic University of Leuven
> Belgium
> 
> > Co 1       
> Ar 3 5
> 3, 2,2.0  N
> 3, 2,2.0  N
> 3,-3,3.0  N
> 3,-3,0.0  N
> 4,-1,1.0  N
> 4,-1,1.0  N
> Co 1       
> Ar 3 5
> 3, 2,2.0  N
> 3, 2,2.0  N
> 3,-3,3.0  N
> 3,-3,0.0  N
> 4,-1,1.0  N
> 4,-1,1.0  N
> Co 1       
> Ar 3 5
> 3, 2,2.0  N
> 3, 2,2.0  N
> 3,-3,3.0  N
> 3,-3,0.0  N
> 4,-1,1.0  N
> 4,-1,1.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> Ag 1       
> Kr 3 5
> 4, 2,2.0  N
> 4, 2,2.0  N
> 4,-3,3.0  N
> 4,-3,3.0  N
> 5,-1,1.0  N
> 5,-1,0.0  N
> ****     End of Input
> ****     End of Input
> > NEWT 1.0           #(NOSE, NEWT, BFGS, MOLD, tolf
> (a4,f5.2))
> 1.0 1.0 0.0 0.8    # Atom1   (NOSE, MOLD:Masse,
> delta t, T, nose-frequency)
> 1.0 1.0 0.0 0.8    # Atom2   (NEWT: 1,2,3:delta,
> 4:eta(1=MOLD))
> 0.0 0.0 0.0 0.8    # Atom3   (BFGS, NEWT: [ 1 || 2
> || 3 ] = 0 constraint)
> 1.0 1.0 0.0 0.8    # Atom4
> 1.0 1.0 0.0 0.8    # Atom5
> 0.0 0.0 0.0 0.8    # Atom6
> 1.0 1.0 0.0 0.8    # Atom7
> 0.0 0.0 0.0 0.8    # Atom8
> 1.0 1.0 1.0 0.8    # Atom9
> 1.0 0.0 1.0 0.8    # Atom10
> 1.0 1.0 0.0 0.8    # Atom11
> 1.0 1.0 0.0 0.8    # Atom12
> 1.0 0.0 1.0 0.8    # Atom13
> 0.0 0.0 0.0 0.8    # Atom14
> 1.0 1.0 0.0 0.8    # Atom15
> 1.0 1.0 0.0 0.8    # Atom16
> 1.0 1.0 0.0 0.8    # Atom17
> 1.0 1.0 0.0 0.8    # Atom18
> 1.0 1.0 0.0 0.8    # Atom19
> 1.0 1.0 0.0 0.8    # Atom20
> 1.0 0.0 1.0 0.8    # Atom21
> 1.0 0.0 1.0 0.8    # Atom22
> 0.0 0.0 0.0 0.8    # Atom23
> 0.0 0.0 0.0 0.8    # Atom24
> 
> > AgCo                                              
 
>                           
> P   LATTICE,NONEQUIV. ATOMS:24 6 Pm                 
>                           
>              RELA                                   
>                           
>  22.024507 22.024507 22.024507 90.000000 90.000000
> 90.000000                   
> ATOM= -1: X=0.00000000 Y=0.00000000 Z=0.00000000
>           MULT= 1          ISPLIT= 8
> Co1        NPT=  781  R0=0.00010000 RMT=    2.2500  
> Z: 27.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM= -2: X=0.25000000 Y=0.25000000 Z=0.00000000
>           MULT= 1          ISPLIT= 8
> Co2        NPT=  781  R0=0.00010000 RMT=    2.2500  
> Z: 27.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM= -3: X=0.00000000 Y=0.50000000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Co3        NPT=  781  R0=0.00010000 RMT=    2.2500  
> Z: 27.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM= -4: X=0.50000000 Y=0.00000000 Z=0.00000000
>           MULT= 1          ISPLIT= 8
> Ag1        NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM= -5: X=0.00000000 Y=0.50000000 Z=0.00000000
>           MULT= 1          ISPLIT= 8
> Ag2        NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM= -6: X=0.00000000 Y=0.00000000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Ag3        NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM= -7: X=0.50000000 Y=0.50000000 Z=0.00000000
>           MULT= 1          ISPLIT= 8
> Ag4        NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM= -8: X=0.50000000 Y=0.00000000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Ag5        NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM= -9: X=0.25000000 Y=0.00000000 Z=0.25000000
>           MULT= 2          ISPLIT= 8
>       -9: X=0.25000000 Y=0.00000000 Z=0.75000000
> Ag6        NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-10: X=0.75000000 Y=0.00000000 Z=0.25000000
>           MULT= 2          ISPLIT= 8
>      -10: X=0.75000000 Y=0.00000000 Z=0.75000000
> Ag7        NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-11: X=0.75000000 Y=0.25000000 Z=0.00000000
>           MULT= 1          ISPLIT= 8
> Ag8        NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-12: X=0.25000000 Y=0.75000000 Z=0.00000000
>           MULT= 1          ISPLIT= 8
> Ag9        NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-13: X=0.00000000 Y=0.25000000 Z=0.25000000
>           MULT= 2          ISPLIT= 8
>      -13: X=0.00000000 Y=0.25000000 Z=0.75000000
> Ag10       NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-14: X=0.00000000 Y=0.75000000 Z=0.25000000
>           MULT= 2          ISPLIT= 8
>      -14: X=0.00000000 Y=0.75000000 Z=0.75000000
> Ag11       NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-15: X=0.75000000 Y=0.75000000 Z=0.00000000
>           MULT= 1          ISPLIT= 8
> Ag12       NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-16: X=0.25000000 Y=0.25000000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Ag13       NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-17: X=0.25000000 Y=0.75000000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Ag14       NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-18: X=0.75000000 Y=0.25000000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Ag15       NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-19: X=0.75000000 Y=0.75000000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Ag16       NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-20: X=0.25000000 Y=0.50000000 Z=0.25000000
>           MULT= 2          ISPLIT= 8
>      -20: X=0.25000000 Y=0.50000000 Z=0.75000000
> Ag17       NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-21: X=0.75000000 Y=0.50000000 Z=0.25000000
>           MULT= 2          ISPLIT= 8
>      -21: X=0.75000000 Y=0.50000000 Z=0.75000000
> Ag18       NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-22: X=0.50000000 Y=0.25000000 Z=0.25000000
>           MULT= 2          ISPLIT= 8
>      -22: X=0.50000000 Y=0.25000000 Z=0.75000000
> Ag19       NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-23: X=0.50000000 Y=0.75000000 Z=0.25000000
>           MULT= 2          ISPLIT= 8
>      -23: X=0.50000000 Y=0.75000000 Z=0.75000000
> Ag20       NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
> ATOM=-24: X=0.50000000 Y=0.50000000 Z=0.50000000
>           MULT= 1          ISPLIT= 8
> Ag21       NPT=  781  R0=0.00010000 RMT=    2.4000  
> Z: 47.0                   
> LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
>                      0.0000000 1.0000000 0.0000000
>                      0.0000000 0.0000000 1.0000000
>    2      NUMBER OF SYMMETRY OPERATIONS
>  1 0 0 0.0000000
>  0 1 0 0.0000000
>  0 0 1 0.0000000
>        1
>  1 0 0 0.0000000
>  0 1 0 0.0000000
>  0 0-1 0.0000000
>        2
> > warning: !!! Struct file is not consistent with
> space group found.
> 
>
- ----------------------------------------------------------------------
> 
> Bravais lattice: Monoclinic primitive
> 
>      a             b            c
>  22.02450700    22.02450700   22.02450700
>      alpha         beta         gamma
>  90.00000000    90.00000000   90.00000000
> 
> 
> ===== Decomposition of new basis vectors over input
> basis =====
>  1.000000   0.000000  0.000000  <--- 1
>  0.000000   1.000000  0.000000  <--- 2
>  0.000000   0.000000  1.000000  <--- 3
> 
> ==== Number of atoms in cell: 32
> ==== Atom positions:
> 
>  0.00000000   0.00000000  0.00000000
>  Co1
> 
>  0.25000000   0.25000000  0.00000000
>  Co2
> 
>  0.00000000   0.50000000  0.50000000
>  Co3
> 
>  0.50000000   0.00000000  0.00000000
>  Ag1
> 
>  0.00000000   0.50000000  0.00000000
>  Ag2
> 
>  0.00000000   0.00000000  0.50000000
>  Ag3
> 
>  0.50000000   0.50000000  0.00000000
>  Ag4
> 
>  0.50000000   0.00000000  0.50000000
>  Ag5
> 
>  0.25000000   0.00000000  0.25000000
>  Ag6
>  0.25000000   0.00000000  0.75000000
>  Ag6
> 
>  0.75000000   0.00000000  0.25000000
>  Ag7
>  0.75000000   0.00000000  0.75000000
>  Ag7
> 
>  0.75000000   0.25000000  0.00000000
>  Ag8
> 
>  0.25000000   0.75000000  0.00000000
>  Ag9
> 
>  0.00000000   0.25000000  0.25000000
>  Ag10
>  0.00000000   0.25000000  0.75000000
>  Ag10
> 
>  0.00000000   0.75000000  0.25000000
>  Ag11
>  0.00000000   0.75000000  0.75000000
>  Ag11
> 
>  0.75000000   0.75000000  0.00000000
>  Ag12
> 
>  0.25000000   0.25000000  0.50000000
>  Ag13
> 
>  0.25000000   0.75000000  0.50000000
>  Ag14
> 
>  0.75000000   0.25000000  0.50000000
>  Ag15
> 
>  0.75000000   0.75000000  0.50000000
>  Ag16
> 
>  0.25000000   0.50000000  0.25000000
>  Ag17
>  0.25000000   0.50000000  0.75000000
>  Ag17
> 
>  0.75000000   0.50000000  0.25000000
>  Ag18
>  0.75000000   0.50000000  0.75000000
>  Ag18
> 
>  0.50000000   0.25000000  0.25000000
>  Ag19
>  0.50000000   0.25000000  0.75000000
>  Ag19
> 
>  0.50000000   0.75000000  0.25000000
>  Ag20
>  0.50000000   0.75000000  0.75000000
>  Ag20
> 
>  0.50000000   0.50000000  0.50000000
>  Ag21
> 
> ==== Number of nonequivalent sorts: 24
> ==== Nonequivalent atoms, point group for each sort:
> ====
> 
> Sort number: 1
>   Names of point group: m      m      Cs
>   New basis vectors for this point group:
>     1.0000   0.0000  0.0000  <--- 1
>     0.0000   1.0000  0.0000  <--- 2
>     0.0000   0.0000  1.0000  <--- 3
> 
>   Atom positions: 1
>    0.00000000   0.00000000  0.00000000
>    Co1
> 
> Sort number: 2
>   Names of point group: m      m      Cs
>   New basis vectors for this point group:
>     1.0000   0.0000  0.0000  <--- 1
>     0.0000   1.0000  0.0000  <--- 2
>     0.0000   0.0000  1.0000  <--- 3
> 
>   Atom positions: 1
>    0.25000000   0.25000000  0.00000000
>    Co2
> 
> Sort number: 3
>   Names of point group: m      m      Cs
>   New basis vectors for this point group:
>     1.0000   0.0000  0.0000  <--- 1
>     0.0000   1.0000  0.0000  <--- 2
>     0.0000   0.0000  1.0000  <--- 3
> 
>   Atom positions: 1
>    0.00000000   0.50000000  0.50000000
>    Co3
> 
> Sort number: 4
>   Names of point group: m      m      Cs
>   New basis vectors for this point group:
>     1.0000   0.0000  0.0000  <--- 1
>     0.0000   1.0000  0.0000  <--- 2
>     0.0000   0.0000  1.0000  <--- 3
> 
>   Atom positions: 1
>    0.50000000   0.00000000  0.00000000
>    Ag1
> 
> Sort number: 5
>   Names of point group: m      m      Cs
>   New basis vectors for this point group:
>     1.0000   0.0000  0.0000  <--- 1
>     0.0000   1.0000  0.0000  <--- 2
>     0.0000   0.0000  1.0000  <--- 3
> 
>   Atom positions: 1
>    0.00000000   0.50000000  0.00000000
>    Ag2
> 
> Sort number: 6
>   Names of point group: m      m      Cs
>   New basis vectors for this point group:
>     1.0000   0.0000  0.0000  <--- 1
>     0.0000   1.0000  0.0000  <--- 2
>     0.0000   0.0000  1.0000  <--- 3
> 
>   Atom positions: 1
>    0.00000000   0.00000000  0.50000000
>    Ag3
> 
> Sort number: 7
>   Names of point group: m      m      Cs
>   New basis vectors for this point group:
>     1.0000   0.0000  0.0000  <--- 1
>     0.0000   1.0000  0.0000  <--- 2
>     0.0000   0.0000  1.0000  <--- 3
> 
>   Atom positions: 1
>    0.50000000   0.50000000  0.00000000
>    Ag4
> 
> Sort number: 8
>   Names of point group: m      m      Cs
>   New basis vectors for this point group:
>     1.0000   0.0000  0.0000  <--- 1
>     0.0000   1.0000  0.0000  <--- 2
>     0.0000   0.0000  1.0000  <--- 3
> 
>   Atom positions: 1
>    0.50000000   0.00000000  0.50000000
>    Ag5
> 
=== message truncate
 Dear Veerle,
your atoms are equivalent in *.inst but inequivalent
in *.struct, why ?
Thanks

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------------------------------

Date: Mon, 6 Jan 2003 22:31:31 +0800
From: joshua xie <joshuaxie@etang.com>
Subject: [WIEN]: a problem

====
joshua xie <joshuaxie@etang.com>
submitted the following contribution:
====

the scf scycle stop when excuting lapw1 with following error:


**  Error in Parallel LAPW1
**  LAPW1 STOPPED at Mon Jan 6 22:10:26 CST 2003
**  check ERROR FILES!
 'SELECT' - no energy limits found for L= 1
 'SELECT' - E-bottom   -2.99000   E-top -200.00000
 'SELECT' - no energy limits found for L= 1
 'SELECT' - E-bottom   -2.99000   E-top -200.00000


I hope someone would give me some hints to solve the problem.

Thank you all in advance!

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------------------------------

Date: Mon, 6 Jan 2003 15:44:40 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: Problems with crystalstructure

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

>  Dear Veerle,
> your atoms are equivalent in *.inst but inequivalent
> in *.struct, why ?
> Thanks
> 

There are 24 atoms in her struct and 24 in her inst, what do you mean?

kind regards,

Kevin Jorissen


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------------------------------

Date: Mon, 6 Jan 2003 10:13:00 -0500
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: question about how to use OPTIC

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====


Liu,

It is difficult (impossible?) to diagnose your error.  What semiconductor is 
this, and what is its calculated bandgap?  What was your procedure after
the SCF calculation?  Did you produce a bandstructure also?  It helps if you
can produce a proper bandstructure, as a check on your scf calculation.

On January 6, 2003 03:49 am, liu wan wrote:
> ====
> "liu wan" <wien97wan@hotmail.com>
> submitted the following contribution:
> ====
>
> Dear All
>
> I try to calculated the optical properties of a semi-conductor. But I find
> that the reult in the case.joint is: Some position is very large and the
> other position is zero. What is wrong?
>
> 2
>    Energy  [eV]     Im_eps_xx          Im_eps_zz
>
>       0.00000     0.84051298E+89     0.00000000E+00
>       0.01361     0.17131700E-07     0.00000000E+00
>       0.02721     0.10498127+277     0.00000000E+00
>       0.04082     0.22762560E-16     0.00000000E+00
>       0.05442     0.66295283E-08     0.00000000E+00
>       0.06803     0.15973640+272     0.00000000E+00
>       0.08163     0.21894908E-16     0.00000000E+00
>       0.09524     0.21233672-152     0.00000000E+00
>       0.10885     0.44776644+218     0.00000000E+00
>       0.12245     0.51962383E+46     0.00000000E+00
>       0.13606     0.46566129E-09     0.00000000E+00
>       0.14966     0.00000000E+00     0.00000000E+00
>       0.16327     0.00000000E+00     0.00000000E+00
>       0.17687     0.00000000E+00     0.00000000E+00
>
> Best wish
>
> Liu
>
> _________________________________________________________________
> MSN 8 helps eliminate e-mail viruses. Get 2 months FREE*
> http://join.msn.com/?page=features/virus
>
> ====
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------------------------------

Date: Mon, 06 Jan 2003 17:13:37 +0200
From: "B. Yanchitsky" <yan@im.imag.kiev.ua>
Subject: Re: [WIEN]: Problems with crystalstructure

====
"B. Yanchitsky" <yan@im.imag.kiev.ua>
submitted the following contribution:
====

> When I try to make a crystalstructure consisting of 29 Ag-atoms and 3
> Co-atoms, all positioned in a supercell (8 fcc-cubes placed to form a
> supercube with as latticeconstantes twice the ones of Ag-fcc) and the Co's
> positioned at coordinates (0, 0, 0), (0.25, 0.25, 0), (0.5, 0, 0.5), or on
> equivalent positions, sgroup suggests a "better" struct-file. But when I
> accept this new struct-file there appears to be an inconsistency in the
> suggested structure.
> *.outputsgroup starts with the following warningmessage:
> "warning: !!! Struct file is not consistent with space group found."
> 
> Ignoring this inconsistency and using an RK_max of 5.0 runs but ends up with
> forces that diverge rather than converge for almost all inequivalent atoms.
> A typical example of this divergence:

Dear Veerle,

This is a bug in sgroup and the warning is incorrect. sgroup must not generate any warnings treating any struct file which is a
result of sgroup
output. After a quick look, it seems that your struct file is correct. The problem
is that sgroup believes (incorrectly) that your input structure is specified as unique axis b setting (alpha=gamma=90) and this
is a reason for the incorrect warning.

Thank you for this report,

Best regards,

Bogdan Yanchitsky
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Date: Mon, 6 Jan 2003 16:14:54 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: a problem

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====


- ----- Original Message -----
From: "joshua xie" <joshuaxie@etang.com>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Monday, January 06, 2003 3:31 PM
Subject: [WIEN]: a problem


> ====
> joshua xie <joshuaxie@etang.com>
> submitted the following contribution:
> ====
>
> the scf scycle stop when excuting lapw1 with following error:
>
>
> **  Error in Parallel LAPW1
> **  LAPW1 STOPPED at Mon Jan 6 22:10:26 CST 2003
> **  check ERROR FILES!
>  'SELECT' - no energy limits found for L= 1
>  'SELECT' - E-bottom   -2.99000   E-top -200.00000
>  'SELECT' - no energy limits found for L= 1
>  'SELECT' - E-bottom   -2.99000   E-top -200.00000
>
>
> I hope someone would give me some hints to solve the problem.

Have you read the users guide?  There's useful information in the section
describing the program LAPW1 and its input.
I believe there's also faq on the wien2k-website, and the mailing list
digests might be helpful, too.

If you have exhausted these sources, please provide us with more detailed
information concerning your calculation and we will try to help you to the
best of our abilities.

kind regards,

Kevin Jorissen
kevin.jorissen@ua.ac.be




> Thank you all in advance!
>
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> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
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------------------------------

Date: Mon, 6 Jan 2003 16:49:05 +0100
From: Veerle Vanhoof <Veerle.Vanhoof@fys.kuleuven.ac.be>
Subject: Re: [WIEN]: Problems with crystalstructure

====
Veerle Vanhoof <Veerle.Vanhoof@fys.kuleuven.ac.be>
submitted the following contribution:
====


> > When I try to make a crystalstructure consisting of 29 Ag-atoms and 3
> > Co-atoms, all positioned in a supercell (8 fcc-cubes placed to form a
> > supercube with as latticeconstantes twice the ones of Ag-fcc) and the
> > Co's positioned at coordinates (0, 0, 0), (0.25, 0.25, 0), (0.5, 0, 0.5),
> > or on equivalent positions, sgroup suggests a "better" struct-file. But
> > when I accept this new struct-file there appears to be an inconsistency
> > in the suggested structure.
> > *.outputsgroup starts with the following warningmessage:
> > "warning: !!! Struct file is not consistent with space group found."
> >
> > Ignoring this inconsistency and using an RK_max of 5.0 runs but ends up
> > with forces that diverge rather than converge for almost all inequivalent
> > atoms. A typical example of this divergence:
>
> Dear Veerle,
>
> This is a bug in sgroup and the warning is incorrect. sgroup must not
> generate any warnings treating any struct file which is a result of sgroup
> output. After a quick look, it seems that your struct file is correct. The
> problem is that sgroup believes (incorrectly) that your input structure is
> specified as unique axis b setting (alpha=gamma=90) and this is a reason
> for the incorrect warning.


So the inconsistency sgroup mentions can't be the reason for the divergence of 
the forces.
What can then be the cause of it?

Thanks

Veerle Vanhoof



- -- 
Veerle Vanhoof
  IKS - KULeuven
  Celestijnenlaan 200 D
  B-3001 Leuven
  BELGIUM
  Phone: +32 (0)16 32 71 45
  Fax: +32 (0)16 32 79 85
  email: Veerle.Vanhoof@fys.kuleuven.ac.be

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------------------------------

Date: Mon, 6 Jan 2003 11:07:51 -0500
From: "Dadi Dai" <dai@unity.ncsu.edu>
Subject: [WIEN]: Why does LDA+U stop at the second cycle?

====
"Dadi Dai" <dai@unity.ncsu.edu>
submitted the following contribution:
====

I wish to do LDA+U calculation for Cu4O3.  I used
"runsp -orb", and the calculation stopped at the beginning
of the second cycle.  I don't know why and hope to get some
help.

The error message is:
....................cycle 1...................
STOP  LAPW0 END
STOP  LAPW1 END
STOP  LAPW1 END
STOP  LAPW2 END
STOP  LAPW2 END
STOP  lapwdm END
STOP  lapwdm END
STOP  CORE  END
STOP  CORE  END
STOP  MIXER END
..............cycle 2..................
STOP  LAPW0 END
1525-001 The READ statement on the file Cu4O3.dmatup cannot
be completed because the end of the file was reached.  The
program will stop.

I found the file "uporb.error" that shows "Error in Vorb".
The :log file shows:
>   (runsp) options: -orb -i 40 -cc 0.0001
Fri Jan  3 15:56:23 EST 2003> (x) lapw0
Fri Jan  3 15:57:02 EST 2003> (x) lapw1 -up -orb
Fri Jan  3 16:11:31 EST 2003> (x) lapw1 -dn -orb
Fri Jan  3 16:25:58 EST 2003> (x) lapw2 -up
Fri Jan  3 16:27:31 EST 2003> (x) lapw2 -dn
Fri Jan  3 16:29:00 EST 2003> (x) lapwdm -up
Fri Jan  3 16:29:05 EST 2003> (x) lapwdm -dn
Fri Jan  3 16:29:09 EST 2003> (x) lcore -up
Fri Jan  3 16:29:10 EST 2003> (x) lcore -dn
Fri Jan  3 16:29:11 EST 2003> (x) mixer
Fri Jan  3 16:29:16 EST 2003> (x) lapw0
Fri Jan  3 16:29:57 EST 2003> (x) orb -up


The Cu4O3.inorb that I used is:
1  2  0
BROYD 0.25
1 1 2
2 1 2
1
0.55127 0.055127   U,J
0.55127 0.055127   U,J

The Cu4O3.indm that I used is:
- -9.0
2
1 1 2
1 1 2
0 0

I wonder if the inputs are correct.  Could anyone help me?

Thank you very much!

Dadi Dai



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------------------------------

Date: Mon, 6 Jan 2003 11:10:27 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: hello

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear W2kusers

       Last time, I had sent queries regarding the scripts "runsp_lapw", 
"initso_lapw" and  MIXER & MINI.

If you have an suggestions/can answer pl. let me know.

thanking in advance for your help.

Regards
sahu

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------------------------------

Date: Mon, 6 Jan 2003 08:45:12 -0800 (PST)
From: romdhani hedi <hedi_romdhani2002@yahoo.com>
Subject: Re: [WIEN]: Problems with crystalstructure

====
romdhani hedi <hedi_romdhani2002@yahoo.com>
submitted the following contribution:
====


- --- Kevin Jorissen <kevin.jorissen@ua.ac.be> wrote:
> ====
> "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
> submitted the following contribution:
> ====
> 
> >  Dear Veerle,
> > your atoms are equivalent in *.inst but
> inequivalent
> > in *.struct, why ?
> > Thanks
> > 
> 
> There are 24 atoms in her struct and 24 in her inst,
> what do you mean?
> 
> kind regards,
> 
> Kevin Jorissen
> 
> 
> > __________________________________________________
******************************************************
there are 24 atoms in both files. In *.inst for
example all Ag atoms are indexed by Ag1, but in
*.struct they are indexed by Ag1, Ag2,....which make
inequivalent.
Thanks


__________________________________________________
Do you Yahoo!?
Yahoo! Mail Plus - Powerful. Affordable. Sign up now.
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------------------------------

Date: Mon, 06 Jan 2003 18:48:45 +0200
From: "B. Yanchitsky" <yan@im.imag.kiev.ua>
Subject: Re: [WIEN]: Problems with crystalstructure

====
"B. Yanchitsky" <yan@im.imag.kiev.ua>
submitted the following contribution:
====

> So the inconsistency sgroup mentions can't be the reason for the divergence of
> the forces.
> What can then be the cause of it?
> 

Yes, i think that the warning message can't be 
responsible for the divergence.
But unfortunately i don't know actually where may be a reason for this
instability. In any case, one thing is quite clear - 
it's necessary to make sure that you have well calculated forces
(small Rkmax, or a small number of k-points may result in bad forces).

Best regards,

Bogdan
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------------------------------

Date: Mon, 6 Jan 2003 18:41:26 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: Why does LDA+U stop at the second cycle?

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> I wish to do LDA+U calculation for Cu4O3.  I used "runsp -orb", and the
> calculation stopped at the beginning of the second cycle.  I don't know
> why and hope to get some help.
> The Cu4O3.inorb that I used is:
> 1  2  0
> BROYD 0.25
> 1 1 2
> 2 1 2
> 1
> 0.55127 0.055127   U,J
> 0.55127 0.055127   U,J

Do you have the latest versions ?
Use PRATT   1.0  (the defaults) and not BROYD.

Did you remove the case.vorbdu file in the runsp_lapw script as was
discussed in the mailing list some weeks ago.

Regards

                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Mon, 6 Jan 2003 15:16:36 -0300 (ART)
From: RUBEN WEHT <ruweht@cnea.gov.ar>
Subject: Re: [WIEN]: Why does LDA+U stop at the second cycle?

====
RUBEN WEHT <ruweht@cnea.gov.ar>
submitted the following contribution:
====

Dear Dadi Dai,

Please note you have an error in the *.indm file

> The Cu4O3.indm that I used is:
> -9.0
> 2
> 1 1 2
> 1 1 2   <<<<<<<<<---------
> 0 0

You are calculating the density matrix for the same orbital twice.
Also consider the suggestion given by Peter regarding case.vorbdu file.
(I think the same is valid for a question posted by Dr. Sahu same weeks
ago...).

Best,

		Ruben

*====================================================================*
|  Ruben Weht                             |  ruweht@cnea.gov.ar      |
|  Departmento de Fisica - CNEA           |  Tel: (54-11) 4754-7104  |
|  Avda. General Paz y Constituyentes     |  Fax: (54-11) 4754-7121  |
|  1650 - San Martin - ARGENTINA          |                          |
*====================================================================*



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------------------------------

Date: Mon, 6 Jan 2003 15:26:36 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: runsp_lapw

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear Prof Blaha
      In connection with your answer to the qurey on w2k-list "Why does
LDA+U stop at .....", does it answer my qurey on runsp_lapw -so -orb which
I put last week?

In the runsp_script(latest download, 3rd week of Dec 2002). 

the case.vorbdu is already commented:


#foreach i ( vorbup vorbdn vorbdu )
#  if (-e $file.$i ) \
#  cp $file.$i $file.$i"_old"           #save last cycle
#end


but slightly below there is 


if ( "$so" == "-so" && -s $file.dmatud ) then
total_exec      orb -du $para

do you mean to say we have to comment these two lines also?

PRATT in case.inorb means
BROYD doesnot work for -orb.

If case.inm contain BROYD but case.inorb contain PRATT, orbital charge
densities will be mixed using PRATT scheme (mixer is invoked during -orb
run) but the final charge densities at the end of cycle will be done by
BROYD scheme  and case.scf file should contain BROYD instead of PRATT. is
it right?

Regards
sahu

 

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------------------------------

Date: Tue, 7 Jan 2003 01:41:41 -0300 (ART)
From: RUBEN WEHT <ruweht@cnea.gov.ar>
Subject: Re: [WIEN]: runsp_lapw

====
RUBEN WEHT <ruweht@cnea.gov.ar>
submitted the following contribution:
====

  This message is in MIME format.  The first part should be readable text,
  while the remaining parts are likely unreadable without MIME-aware tools.
  Send mail to mime@docserver.cac.washington.edu for more info.

- --1621681473-1344807548-1041914453=:18432
Content-Type: TEXT/PLAIN; CHARSET=US-ASCII
Content-ID: <Pine.LNX.4.33.0301070141111.18574@cnea.gov.ar>

Dr. Sahu,
please try with the runsp_lapw file I have attached.
It has the lines that calculated vorbdu cancelled.

Best,

		Ruben


> Dear Prof Blaha
>       In connection with your answer to the qurey on w2k-list "Why does
> LDA+U stop at .....", does it answer my qurey on runsp_lapw -so -orb which
> I put last week?
>
> In the runsp_script(latest download, 3rd week of Dec 2002).
>
> the case.vorbdu is already commented:
>
> #foreach i ( vorbup vorbdn vorbdu )
> #  if (-e $file.$i ) \
> #  cp $file.$i $file.$i"_old"           #save last cycle
> #end
>
> but slightly below there is
>
> if ( "$so" == "-so" && -s $file.dmatud ) then
> total_exec      orb -du $para
>
> do you mean to say we have to comment these two lines also?
>
> PRATT in case.inorb means
> BROYD doesnot work for -orb.
>
> If case.inm contain BROYD but case.inorb contain PRATT, orbital charge
> densities will be mixed using PRATT scheme (mixer is invoked during -orb
> run) but the final charge densities at the end of cycle will be done by
> BROYD scheme  and case.scf file should contain BROYD instead of PRATT. is
> it right?
>
> Regards
> sahu
>
>
>
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- -- 
*====================================================================*
|  Ruben Weht                             |  ruweht@cnea.gov.ar      |
|  Departmento de Fisica - CNEA           |  Tel: (54-11) 4754-7104  |
|  Avda. General Paz y Constituyentes     |  Fax: (54-11) 4754-7121  |
|  1650 - San Martin - ARGENTINA          |                          |
*====================================================================*

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------------------------------

Date: Tue, 7 Jan 2003 08:23:06 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: runsp_lapw

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

>       In connection with your answer to the qurey on w2k-list "Why does
> LDA+U stop at .....", does it answer my qurey on runsp_lapw -so -orb which
> I put last week?

Maybe.

> if ( "$so" == "-so" && -s $file.dmatud ) then
> total_exec      orb -du $para
>
> do you mean to say we have to comment these two lines also?

Should not be necessary, but does not harm.

> PRATT in case.inorb means
> BROYD doesnot work for -orb.
>
> If case.inm contain BROYD but case.inorb contain PRATT, orbital charge
> densities will be mixed using PRATT scheme (mixer is invoked during -orb
> run) but the final charge densities at the end of cycle will be done by
> BROYD scheme  and case.scf file should contain BROYD instead of PRATT. is
> it right?

It means that the density matrices (*dmat*) are now also mixed in "mixer"
and thus must not be mixed at all in "orb". This is achieved by
PRATT 1.0  in case.inorb (which is the default).

Regards
                                     P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
- --------------------------------------------------------------------------

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------------------------------

Date: Tue, 7 Jan 2003 10:13:27 +0100
From: "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
Subject: Re: [WIEN]: Problems with crystalstructure

====
"Kevin Jorissen" <kevin.jorissen@ua.ac.be>
submitted the following contribution:
====

Only inequivalent atoms are listed in the inst-file.  There is only one
entry for each class of equivalent atoms!

kind regards,

Kevin Jorissen.

- ----- Original Message -----
From: "romdhani hedi" <hedi_romdhani2002@yahoo.com>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Monday, January 06, 2003 5:45 PM
Subject: Re: [WIEN]: Problems with crystalstructure


> ====
> romdhani hedi <hedi_romdhani2002@yahoo.com>
> submitted the following contribution:
> ====
>
>
> --- Kevin Jorissen <kevin.jorissen@ua.ac.be> wrote:
> > ====
> > "Kevin Jorissen" <kevin.jorissen@ua.ac.be>
> > submitted the following contribution:
> > ====
> >
> > >  Dear Veerle,
> > > your atoms are equivalent in *.inst but
> > inequivalent
> > > in *.struct, why ?
> > > Thanks
> > >
> >
> > There are 24 atoms in her struct and 24 in her inst,
> > what do you mean?
> >
> > kind regards,
> >
> > Kevin Jorissen
> >
> >
> > > __________________________________________________
> ******************************************************
> there are 24 atoms in both files. In *.inst for
> example all Ag atoms are indexed by Ag1, but in
> *.struct they are indexed by Ag1, Ag2,....which make
> inequivalent.
> Thanks
>
>
> __________________________________________________
> Do you Yahoo!?
> Yahoo! Mail Plus - Powerful. Affordable. Sign up now.
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> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
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> ====
>

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------------------------------

Date: Tue, 07 Jan 2003 06:02:07 -0500
From: "michel certier" <mcertier@mail.com>
Subject: Re: [WIEN]: parallel execution problem in dual PIV

====
"michel certier" <mcertier@mail.com>
submitted the following contribution:
====

dear wien users i posted a message about a problem of parallel execution in dual PIV with 2 proc :
"> Dear wien users Happy New year !!!
> I met somme problem to execut a parallel job for cubic system with 35 k-point on dual machine, after 1 iteration the program stop and I get the following message:
>  
> LAPW0 END
>  LAPW1 END
>  LAPW1 END
> LAPW2 - FERMI; weighs written
>  LAPW2 END
>  LAPW2 END
>  SUMPARA END
>  SUMPARA END
>  CORE  END
>  MIXER END
> in cycle 2    ETEST: 0   CTEST: 0
> PGFIO-F-231/formatted read/unit=8/error on data conversion.
>  File name = test.clmsum    formatted, sequential access   record = 2223
>  In source file lapw0.F, at line number 404
> cat: No match.
> My .machines files is :
> 
> granularity:1
> 17:localhost
> 18:localhost
> The program run well in serial mode.
> Can some one give me a solution to this problem.
> Thank's "
I have change my number of kpoint to 56-k to have an homogen number of k-point in each proc and its run but I get many warning in my scf files with a big fluctuation in energy until a convergence. Have any one an idea !!! 
Thanks one more

- -- 
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------------------------------

Date: Tue, 7 Jan 2003 11:42:05 -0800 (PST)
From: yanming Ma <ymma66@yahoo.com>
Subject: [WIEN]: For help

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-997329679-1041968525=:94367
Content-Type: text/plain; charset=us-ascii


Dear Wien2k users,

I am trying to calculate the electric momentum density. But I do not know which code I should use. Does someone know which code can calculate electric momentum density? please let me know.  Thanks very much.

Best Wishes!


Yanming Ma Ph.D
Steacie Institute for Molecular Sciences,
National Research Councils of Canada,
Ottawa, Ontario
K1A 0R6
Canada


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- --0-997329679-1041968525=:94367
Content-Type: text/html; charset=us-ascii

<P>Dear Wien2k users,</P>
<P>I am trying to calculate the electric momentum density. But I do not know which code I should use. Does someone know which code&nbsp;can calculate electric momentum density? please let me know.&nbsp; Thanks very much.</P>
<P>Best Wishes!</P><BR><BR>Yanming Ma Ph.D<br>Steacie Institute for Molecular Sciences,<br>National Research Councils of Canada,<br>Ottawa, Ontario<br>K1A 0R6<br>Canada<p><br><hr size=1>Do you Yahoo!?<br>
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------------------------------

Date: Wed, 8 Jan 2003 08:43:18 +0100 (MET)
From: Peter Blaha <pblaha@theochem.tuwien.ac.at>
Subject: Re: [WIEN]: parallel execution problem in dual PIV

====
Peter Blaha <pblaha@theochem.tuwien.ac.at>
submitted the following contribution:
====

> "> Dear wien users Happy New year !!!
> > I met somme problem to execut a parallel job for cubic system with 35 k-point on dual machine, after 1 iteration the program stop and I get the following message:
> >
> > LAPW0 END
> >  LAPW1 END
> >  LAPW1 END
> > LAPW2 - FERMI; weighs written
> >  LAPW2 END
> >  LAPW2 END
> >  SUMPARA END
> >  SUMPARA END
> >  CORE  END
> >  MIXER END
> > in cycle 2    ETEST: 0   CTEST: 0
> > PGFIO-F-231/formatted read/unit=8/error on data conversion.
> >  File name = test.clmsum    formatted, sequential access   record = 2223
> >  In source file lapw0.F, at line number 404
> > cat: No match.
> > My .machines files is :
> >
> > granularity:1
> > 17:localhost
> > 18:localhost
> > The program run well in serial mode.
> > Can some one give me a solution to this problem.
> > Thank's "
> I have change my number of kpoint to 56-k to have an homogen number of k-point in each proc and its run but I get many warning in my scf files with a big fluctuation in energy until a convergence. Have any one an idea !!!

Most likely you did not "save_lapw" your first calculations, before you
restarted the job again.
Old *broyd* files can lead to wrong clmsum files,
an old scf file to large total energy fluctuations.


                                      P.Blaha
- --------------------------------------------------------------------------
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-15671             FAX: +43-1-58801-15698
Email: blaha@theochem.tuwien.ac.at    WWW: http://info.tuwien.ac.at/theochem/
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Date: Wed, 08 Jan 2003 12:10:59 +0100
From: marc <marc@FHI-Berlin.MPG.DE>
Subject: [WIEN]: SRC_supercell

====
marc <marc@FHI-Berlin.mpg.de>
submitted the following contribution:
====

Dear Wien2k users,

I had a problem in compiling wien2k on SGI.
The following error occured:

SRC_supercell/compile.msg:make: file `Makefile' line 72: Syntax error

Any idea?

Best regards,

Marc.



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Date: Wed, 8 Jan 2003 11:51:08 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: [WIEN]: hello

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear W2k users

I donot know whether I was clear or not in my queries about  MINI,
MIXER and initso_lapw which I put last week to w2k mailing list.

my query about runsp_lapw -so -orb is not yet clear. however,I am trying
the "runsp_lapw"  script provided by Reuben Weht yesterday in which
"vorbdu" commands are either modified or taken out altogether. 
It is assured, everything is correct(ie the input files, procedure etc.)

I put other queries briefly again:

a) about MIXER: If say 20 iterations are done with PRATT scheme and I wish
to switch to BROYD then what files to be saved/deleted before I start to
continue the scf with BROYD so that MIXER use now BROYD and not PRATT for 
mixing OR start  straightaway start the run with BROYD without 
saving/deleting any files.

b)about MINI: how to select delta(i) values in case.inM file while doing
geometry minimization with BFGS or NEWT? I feel, by properly tuning these
values, one can save the number of gemoetry optimization steps and
convergence will be faster as the atoms are moved by this increment using
the forces calculated in the scf run. Is there any guidelines OR it's 
simply a guess and luck.

c) about initso_lapw: during initializing the run for SOC, one need to'
select the number of k-point. But the "number of k-point selection"  
prompt is never ending!! If I say "no" to the selection again, it stops
with "if:bad number" message. do we need to modify initso_lapw script?
and I then have to copy all the case.*_so files 'by hand' to corresponding
case.* files before starting the scf cycle with SOC.

Thanking you in advance dor suggestion/s.

Regards
sahu

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Date: Thu, 9 Jan 2003 07:47:27 +0400
From: "Mohamed Elzain" <elzain@squ.edu.om>
Subject: Re: [WIEN]: SRC_supercell

====
"Mohamed Elzain" <elzain@squ.edu.om>
submitted the following contribution:
====

Sir
I am not sure if the error you encountered is similar to the one I had. I
had an error in the [read(*,*), vac(i)] in the main file.  There shouldn't
be a coma between read and var.

- ----- Original Message -----
From: "marc" <marc@FHI-Berlin.MPG.DE>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Wednesday, January 08, 2003 3:10 PM
Subject: [WIEN]: SRC_supercell


> ====
> marc <marc@FHI-Berlin.mpg.de>
> submitted the following contribution:
> ====
>
> Dear Wien2k users,
>
> I had a problem in compiling wien2k on SGI.
> The following error occured:
>
> SRC_supercell/compile.msg:make: file `Makefile' line 72: Syntax error
>
> Any idea?
>
> Best regards,
>
> Marc.
>
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

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------------------------------

Date: Thu, 09 Jan 2003 09:29:01 +0100
From: Ad Ettema <ettema@tn.tudelft.nl>
Subject: [WIEN]: Spin orbit interaction

====
Ad Ettema <ettema@tn.tudelft.nl>
submitted the following contribution:
====

L.S.,


Has any one experience with the spin orbit interaction parameters in 
file case.inso ?
I am calculating the case of Cu2O which has a spin orbit split valence 
band maximum in gamma. An attempt to put in the appropriate parameters 
in the case.inso file did not lead to this fundamental splitting.
Does anyone know a listing of so parameters published somewhere?




- -- 
Dr A.R.H.F. Ettema
Delft University of Technology
Department of Physics
Lorentzweg 1
2628 CJ Delft
Tel : +31 15 2782481
Fax : +31 15 2781413
Email: ettema@tn.tudelft.nl
Web: http://www.em.tudelft.nl/ad_ettema.htm


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Date: Thu, 9 Jan 2003 14:35:08 +0100
From: "Marc Willinger" <marc@FHI-Berlin.MPG.DE>
Subject: AW: [WIEN]: SRC_supercell

====
"Marc Willinger" <marc@FHI-Berlin.mpg.de>
submitted the following contribution:
====

Thank's very much!

I removed the commas, but additionally I had to deleted the following
command
in the Makefile, in line 72:

$(PREOBJS): Makefile

Honestly, I don't know if deleting that line was wise - but it seems to work
now.

regards,

Marc Willinger

====
"Mohamed Elzain" <elzain@squ.edu.om>
submitted the following contribution:
====

Sir
I am not sure if the error you encountered is similar to the one I had. I
had an error in the [read(*,*), vac(i)] in the main file.  There shouldn't
be a coma between read and var.

> Dear Wien2k users,
>
> I had a problem in compiling wien2k on SGI.
> The following error occured:
>
> SRC_supercell/compile.msg:make: file `Makefile' line 72: Syntax error
>
> Any idea?
>
> Best regards,
>
> Marc.
>
>
>
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
>

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------------------------------

Date: Thu, 09 Jan 2003 21:59:27 +0800
From: "liu wan" <wien97wan@hotmail.com>
Subject: [WIEN]: Question about how to use "XCrySDen" software

====
"liu wan" <wien97wan@hotmail.com>
submitted the following contribution:
====

Dear All

I want using the XCrySDen to creat the k-list for the energy bandstructure 
plots. But I has some questions about how to use XCrySDen.

(1) There are primitive Brillouin Zone and conventional Brillouin Zone, 
which one I will use?

(2) How to set the "ISS" value? Use the default one? Would you please 
explain the means of ISS?


CXZ LATTICE,NONEQUIV. ATOMS: 6                       12 B2/m
MODE OF CALC=RELA
32.888800 19.759000  7.704420 90.000000 90.000000104.440000


When I try to get the k-path of above-file, I get following k-list file:

X0            0    0    0*****  2.0-7.00 1.50    k-list generated by 
XCrySDen
          *****    0    0*****  2.0
          *****    0    0*****  2.0
          *****    0    0*****  2.0
          *****    0    0*****  2.0
          *****    0    0*****  2.0
          *****    0    0*****  2.0
          *****    0    0*****  2.0
X1        *****    0    0*****  2.0
          *****    0**********  2.0
          *****    0**********  2.0
          *****    0**********  2.0
          *****    0**********  2.0
          *****    0**********  2.0
          *****    0**********  2.0
          *****    0**********  2.0
          *****    0**********  2.0
          *****    0**********  2.0
          *****    0**********  2.0
          *****    0**********  2.0

I don't know what is wrong?

Best wish

Liu

Best wish


Liu


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Date: Thu, 9 Jan 2003 10:33:25 -0500
From: Fred Nastos <nastos@physics.utoronto.ca>
Subject: Re: [WIEN]: Spin orbit interaction

====
Fred Nastos <nastos@physics.utoronto.ca>
submitted the following contribution:
====

> I am calculating the case of Cu2O which has a spin orbit split valence
> band maximum in gamma. An attempt to put in the appropriate parameters
> in the case.inso file did not lead to this fundamental splitting.
> Does anyone know a listing of so parameters published somewhere?

Being a first-principles code, there aren't really any parameters to play with
(I'm not talking about LDA+U of course).  In every system (only about five 
simple ones mind you) te WIEN code has given the split-off band due to
spin-orbit interaction, and when there is no-inversion symmetry there
is also spin-spin splitting.  Since the spin-orbit interaction is strongly 
influenced by the symmetry, are you sure your structure file is correct?
If you are looking into the case.output files for the band energies, the
spin-orbit energies are in case.outputso.

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Date: Thu, 9 Jan 2003 08:22:54 -0800 (PST)
From: yanming Ma <ymma66@yahoo.com>
Subject: [WIEN]: Question about the parallelization

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-1892235412-1042129374=:30847
Content-Type: text/plain; charset=us-ascii


Dear Wien2k Users,

I was puzzled by the K point and fine grained parallelization in Wien2k. As I know, for some small cases, I should use K-point parallel, while for some extremely large cases, I should use fine grained parallel.  
When I compile the  wien2k code in SGI tp0 machine  if i chose the fine grained parallelization option, does that mean all my parallel calculation should be in fine grained parallelization? Or it depends on how to make the .machines file.
(1) .machine file as the following should be k_point parallelization if i try to use 4 CPUs.
1:tp0:1
1:tp0:1
1:tp0:1
1:tp0:1
(2).machine file as the following should be fine grained parallelization if i try to use 4 CPUs.
lapw0:tp0:4
1:tp0:4

Are the described aboves correct?

I will appreciate highly your answer.

 


Yanming Ma Ph.D
Steacie Institute for Molecular Sciences,
National Research Councils of Canada,
Ottawa, Ontario
K1A 0R6
Canada


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<P>Dear Wien2k Users,</P>
<P>I was puzzled by the K point and fine grained parallelization in Wien2k. As I know, for some small cases, I should use K-point parallel, while for some extremely large cases, I should use fine grained parallel.&nbsp; <BR>When I compile the&nbsp; wien2k code in SGI tp0 machine&nbsp; if i chose the fine grained parallelization option, does that mean all my parallel calculation should be in fine grained parallelization? Or it depends on how to make the .machines file.<BR>(1) .machine file as the following should be k_point parallelization if i try to use 4 CPUs.<BR>1:tp0:1<BR>1:tp0:1<BR>1:tp0:1<BR>1:tp0:1<BR>(2).machine file as the following should be fine grained parallelization if i try to use 4 CPUs.<BR>lapw0:tp0:4<BR>1:tp0:4</P>
<P>Are the described aboves correct?</P>
<P>I will appreciate highly your answer.</P>
<P>&nbsp;</P><BR><BR>Yanming Ma Ph.D<br>Steacie Institute for Molecular Sciences,<br>National Research Councils of Canada,<br>Ottawa, Ontario<br>K1A 0R6<br>Canada<p><br><hr size=1>Do you Yahoo!?<br>
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Date: Thu, 9 Jan 2003 12:08:22 -0800 (PST)
From: Ting Su <hwlib@yahoo.com>
Subject: [WIEN]: compiling errors

====
Ting Su <hwlib@yahoo.com>
submitted the following contribution:
====

- --0-1163648082-1042142902=:30008
Content-Type: text/plain; charset=us-ascii


Dear WIENers,

I would strongly appreciate for any advice on the following compiling errors:

make PARALLEL='-DParallel' lapw0_mpi \
  FORT=pgf90 FFLAGS=' -Mfreeform -fast -Kieee '-DParallel''
make[1]: Entering directory `/net/hulk/home4/hbsu/WIEN2k/SRC_lapw0'
pgf90 -Mfreeform -fast -Kieee -DParallel -c modules.F
PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 20)
  0 inform,   0 warnings,   1 severes, 0 fatal for init_parallel
PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 43)
  0 inform,   0 warnings,   1 severes, 0 fatal for begend
make[1]: *** [modules.o] Error 1


make PARALLEL='-DParallel' TYPE='COMPLEX' TYPE_COMMENT='\!_COMPLEX' \
  ./lapw1c_mpi FORT=pgf90 FFLAGS=' -Mfreeform -fast -Kieee '-DParallel''
make[1]: Entering directory `/net/hulk/home4/hbsu/WIEN2k/SRC_lapw1'
modules.F: COMPLEX version extracted
pgf90 -Mfreeform -fast -Kieee -DParallel -c modules_tmp_.F
PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 33)
  0 inform,   0 warnings,   1 severes, 0 fatal for init_parallel
PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 51)
  0 inform,   0 warnings,   1 severes, 0 fatal for init_parallelmatrices
PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 119)
  0 inform,   0 warnings,   1 severes, 0 fatal for barrier
PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 129)
  0 inform,   0 warnings,   1 severes, 0 fatal for close_parallel
make[1]: *** [modules.o] Error 1


make PARALLEL='-DParallel' TYPE='COMPLEX' TYPE_COMMENT='\!_COMPLEX' \
  ./lapw2c_mpi FORT=pgf90 FFLAGS=' -Mfreeform -fast -Kieee '-DParallel''
make[1]: Entering directory `/net/hulk/home4/hbsu/WIEN2k/SRC_lapw2'
pgf90 -Mfreeform -fast -Kieee -DParallel -c reallocate.f
modules.F: COMPLEX version extracted
pgf90 -Mfreeform -fast -Kieee -DParallel -c modules_tmp_.F
PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 41)
  0 inform,   0 warnings,   1 severes, 0 fatal for init_parallel
make[1]: *** [modules.o] Error 1


Thank you very much!

Tony



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<P>Dear WIENers,</P>
<P>I would strongly appreciate&nbsp;for any advice on the following compiling errors:</P>
<P>make PARALLEL='-DParallel' lapw0_mpi \<BR>&nbsp; FORT=pgf90 FFLAGS=' -Mfreeform -fast -Kieee '-DParallel''<BR>make[1]: Entering directory `/net/hulk/home4/hbsu/WIEN2k/SRC_lapw0'<BR>pgf90 -Mfreeform -fast -Kieee -DParallel -c modules.F<BR>PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 20)<BR>&nbsp; 0 inform,&nbsp;&nbsp; 0 warnings,&nbsp;&nbsp; 1 severes, 0 fatal for init_parallel<BR>PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 43)<BR>&nbsp; 0 inform,&nbsp;&nbsp; 0 warnings,&nbsp;&nbsp; 1 severes, 0 fatal for begend<BR>make[1]: *** [modules.o] Error 1<BR></P>
<P>make PARALLEL='-DParallel' TYPE='COMPLEX' TYPE_COMMENT='\!_COMPLEX' \<BR>&nbsp; ./lapw1c_mpi FORT=pgf90 FFLAGS=' -Mfreeform -fast -Kieee '-DParallel''<BR>make[1]: Entering directory `/net/hulk/home4/hbsu/WIEN2k/SRC_lapw1'<BR>modules.F: COMPLEX version extracted<BR>pgf90 -Mfreeform -fast -Kieee -DParallel -c modules_tmp_.F<BR>PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 33)<BR>&nbsp; 0 inform,&nbsp;&nbsp; 0 warnings,&nbsp;&nbsp; 1 severes, 0 fatal for init_parallel<BR>PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 51)<BR>&nbsp; 0 inform,&nbsp;&nbsp; 0 warnings,&nbsp;&nbsp; 1 severes, 0 fatal for init_parallelmatrices<BR>PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 119)<BR>&nbsp; 0 inform,&nbsp;&nbsp; 0 warnings,&nbsp;&nbsp; 1 severes, 0 fatal for barrier<BR>PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 129)<BR>&nbsp; 0 inform,&nbsp;&nbsp; 0 warnings,&nbsp;&nbsp; 1 severes, 0 fatal for close_pa!
rallel<BR>make[1]: *** [modules.o] Error 1<BR></P>
<P>make PARALLEL='-DParallel' TYPE='COMPLEX' TYPE_COMMENT='\!_COMPLEX' \<BR>&nbsp; ./lapw2c_mpi FORT=pgf90 FFLAGS=' -Mfreeform -fast -Kieee '-DParallel''<BR>make[1]: Entering directory `/net/hulk/home4/hbsu/WIEN2k/SRC_lapw2'<BR>pgf90 -Mfreeform -fast -Kieee -DParallel -c reallocate.f<BR>modules.F: COMPLEX version extracted<BR>pgf90 -Mfreeform -fast -Kieee -DParallel -c modules_tmp_.F<BR>PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 41)<BR>&nbsp; 0 inform,&nbsp;&nbsp; 0 warnings,&nbsp;&nbsp; 1 severes, 0 fatal for init_parallel<BR>make[1]: *** [modules.o] Error 1<BR></P>
<P>Thank you very much!</P>
<P>Tony</P><p><br><hr size=1>Do you Yahoo!?<br>
<a href="http://rd.yahoo.com/mail/mailsig/*http://mailplus.yahoo.com">Yahoo! Mail Plus</a> - Powerful. Affordable. <a href="http://rd.yahoo.com/mail/mailsig/*http://mailplus.yahoo.com">Sign up now</a>
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Date: Thu, 9 Jan 2003 19:05:13 -0600 (CST)
From: "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
Subject: Re: [WIEN]: Question about the parallelization

====
"Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu>
submitted the following contribution:
====


Dear Ma
 
     During compilation, if you dont choose the option for fine grained
parallalization, it will create only files for single processor(ie lapw0,
lapw1(c), lapw2 etc)  and script for k-pt parallelization run lapw0para,
lapw1para etc. If you choose the optiion for fine grained paralleliztion
then in addition to the above files, the files for MPI parallel run like
lapw0_mpi, lapw1_mpi and lapw2_mpi will be created.

Now, whether the scripts run(sp)_lapw and other script pick up lapw*para
or lapw*_mpi during the run depends on the structure of the .machines 
file as you mentioned.

1) the format of your k-point parallelization file is correct provided you
have 4 k-points to distribute over four cpus(in your case tp0) and the
cpu's have all same speed.For efficiency, only if we have more k-points
then the processors or cpus then only we use k-point parallelization. but
imagine a case where you have a very large system say a supercell
containing large number of atoms say more than 40 and you expect it to be
metallic, for example.
 In such cases, you need large number k-points to sample
the BZ so k-point parallelization is again useful.

2) fine grained parallelization file is to be slightly modified:

lapw0:tp0:1 tp0:1 tp0:1 tp0:1
1:tp0:1 tp0:1 tp0:1 tp0:1

it means lapw0_mpi will use 4 processors each having same speed and your 
sysetm has 1 k-point and lapw1_mpi runs on 4 processors in parallel.

Fine grained parallel will be computationally efficient if you have large
system(ie large number of atoms) and small number of k-points(1 or 2).
that's what UG says.

I myself have not tested so far the MPI parallel code, as it is giving
some problem. I am already in contact with Prof. Blaha regarding this.



Regards
sahu  



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Date: Thu, 9 Jan 2003 20:43:58 -0600 (CST)
From: Bing Zhou <umbingz@cc.UManitoba.CA>
Subject: [WIEN]: SCF stopped at lapw2

====
Bing Zhou <umbingz@cc.UManitoba.CA>
submitted the following contribution:
====

Dear All:

My calculation was stopped at the lapw2 of the fouth SCF cycle, the
following information is in the file lapw2.error:

'LAPW2' - can't open unit:  5
'LAPW2' -        filename: tug-new.in2
'LAPW2' -          status: old          form: formatted

Could you please help me with that?

Thanks!


Bing Zhou
Dept. of Geological Sc.
The Univ. of Manitoba
Canada R3T 2N2
Tel: (204)474-8395

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Date: Fri, 10 Jan 2003 09:15:05 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: compiling errors

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Ting Su,

install MPI... and make the compiler aware of where it is - it can't 
find the header file.

Best regards,
Torsten Andersen.

Ting Su wrote:

> Dear WIENers,
>
> I would strongly appreciate for any advice on the following compiling 
> errors:
>
> make PARALLEL='-DParallel' lapw0_mpi \
>   FORT=pgf90 FFLAGS=' -Mfreeform -fast -Kieee '-DParallel''
> make[1]: Entering directory `/net/hulk/home4/hbsu/WIEN2k/SRC_lapw0'
> pgf90 -Mfreeform -fast -Kieee -DParallel -c modules.F
> PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 20)
>   0 inform,   0 warnings,   1 severes, 0 fatal for init_parallel
> PGF90-S-0017-Unable to open include file: mpif.h (modules.F: 43)
>   0 inform,   0 warnings,   1 severes, 0 fatal for begend
> make[1]: *** [modules.o] Error 1
>
> make PARALLEL='-DParallel' TYPE='COMPLEX' TYPE_COMMENT='\!_COMPLEX' \
>   ./lapw1c_mpi FORT=pgf90 FFLAGS=' -Mfreeform -fast -Kieee '-DParallel''
> make[1]: Entering directory `/net/hulk/home4/hbsu/WIEN2k/SRC_lapw1'
> modules.F: COMPLEX version extracted
> pgf90 -Mfreeform -fast -Kieee -DParallel -c modules_tmp_.F
> PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 33)
>   0 inform,   0 warnings,   1 severes, 0 fatal for init_parallel
> PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 51)
>   0 inform,   0 warnings,   1 severes, 0 fatal for init_parallelmatrices
> PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 119)
>   0 inform,   0 warnings,   1 severes, 0 fatal for barrier
> PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 129)
>   0 inform,   0 warnings,   1 severes, 0 fatal for close_pa! rallel
> make[1]: *** [modules.o] Error 1
>
> make PARALLEL='-DParallel' TYPE='COMPLEX' TYPE_COMMENT='\!_COMPLEX' \
>   ./lapw2c_mpi FORT=pgf90 FFLAGS=' -Mfreeform -fast -Kieee '-DParallel''
> make[1]: Entering directory `/net/hulk/home4/hbsu/WIEN2k/SRC_lapw2'
> pgf90 -Mfreeform -fast -Kieee -DParallel -c reallocate.f
> modules.F: COMPLEX version extracted
> pgf90 -Mfreeform -fast -Kieee -DParallel -c modules_tmp_.F
> PGF90-S-0017-Unable to open include file: mpif.h (modules_tmp_.F: 41)
>   0 inform,   0 warnings,   1 severes, 0 fatal for init_parallel
> make[1]: *** [modules.o] Error 1
>
> Thank you very much!
>
> Tony
>
>
> ------------------------------------------------------------------------
> Do you Yahoo!?
> Yahoo! Mail Plus 
> <http://rd.yahoo.com/mail/mailsig/*http://mailplus.yahoo.com> - 
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- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Fri, 10 Jan 2003 09:12:54 +0100
From: Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
Subject: Re: [WIEN]: SCF stopped at lapw2

====
Torsten Andersen <Torsten.Andersen@Fysik.UU.se>
submitted the following contribution:
====

Dear Bing,

probably either the initialisation failed - no case.in2 or case.in2c 
exist, or inversion symmetry is not present - in which case you should 
have a case.in2c and run the complex version. If you are sure that what 
you do is correct, you can copy case.in2c to case.in2 and run it again.

Best regards,
Torsten.

Bing Zhou wrote:

>====
>Bing Zhou <umbingz@cc.UManitoba.CA>
>submitted the following contribution:
>====
>
>Dear All:
>
>My calculation was stopped at the lapw2 of the fouth SCF cycle, the
>following information is in the file lapw2.error:
>
>'LAPW2' - can't open unit:  5
>'LAPW2' -        filename: tug-new.in2
>'LAPW2' -          status: old          form: formatted
>
>Could you please help me with that?
>
>Thanks!
>
>
>Bing Zhou
>Dept. of Geological Sc.
>The Univ. of Manitoba
>Canada R3T 2N2
>Tel: (204)474-8395
>
>====
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>To (un)subscribe send mail to
>majordomo@zeus.theochem.tuwien.ac.at
>====
>
>

- -- 
Dr. Torsten Andersen
Department of Physics, Condensed Matter Theory Group, Uppsala University
UU-WWW: http://www.fysik4.fysik.uu.se/    TA-WWW: http://deep.at/myspace
News on TA-WWW: Two publ. articles on ab initio nonlinear magneto-optics



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------------------------------

Date: Fri, 10 Jan 2003 11:15:30 +0100
From: Ad Ettema <ettema@tn.tudelft.nl>
Subject: Re: [WIEN]: Spin orbit interaction

====
Ad Ettema <ettema@tn.tudelft.nl>
submitted the following contribution:
====

Dear Fred thanks for helping me here. I think you gave the right hints.

Ad

Fred Nastos wrote:

> ====
> Fred Nastos <nastos@physics.utoronto.ca>
> submitted the following contribution:
> ====
> 
> 
>>I am calculating the case of Cu2O which has a spin orbit split valence
>>band maximum in gamma. An attempt to put in the appropriate parameters
>>in the case.inso file did not lead to this fundamental splitting.
>>Does anyone know a listing of so parameters published somewhere?
>>
> 
> Being a first-principles code, there aren't really any parameters to play with
> (I'm not talking about LDA+U of course).  In every system (only about five 
> simple ones mind you) te WIEN code has given the split-off band due to
> spin-orbit interaction, and when there is no-inversion symmetry there
> is also spin-spin splitting.  Since the spin-orbit interaction is strongly 
> influenced by the symmetry, are you sure your structure file is correct?
> If you are looking into the case.output files for the band energies, the
> spin-orbit energies are in case.outputso.
> 
> ====
> WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at
> To (un)subscribe send mail to
> majordomo@zeus.theochem.tuwien.ac.at
> ====
> 
> 


- -- 
Dr A.R.H.F. Ettema
Delft University of Technology
Department of Physics
Lorentzweg 1
2628 CJ Delft
Tel : +31 15 2782481
Fax : +31 15 2781413
Email: ettema@tn.tudelft.nl
Web: http://www.em.tudelft.nl/ad_ettema.htm


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------------------------------

Date: Fri, 10 Jan 2003 08:43:00 -0500
From: "Dadi Dai" <dai@unity.ncsu.edu>
Subject: [WIEN]: Why bandstructure is not consistent with DOS?

====
"Dadi Dai" <dai@unity.ncsu.edu>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_004E_01C2B884.481980E0
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	charset="iso-8859-1"
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I was studying the bandstructure of Cu4O3.  I used w2web to generate the =
bandstructure and DOS.  In DOS figure, no DOS at E(F) level.  In =
bandstructure figure, however, a few bands cross the E(F) level.  I have =
inserted the E(F) value in case.insp file.

Could anyone help me figure out where the problem might be?

Thank you very much!

Dadi Dai

P.S.=20

Long time ago, when I was using old version of wien2k, I didn't have =
such a problem as long as I entered the correct E(F) in the case.insp =
file.  Now, I checked the data carefully and has given the correct E(F) =
in the case.insp file, but I still have the problem.


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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2722.900" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD><FONT face=3DArial><FONT size=3D2>
<BODY>
<DIV>
<DIV><FONT face=3DArial size=3D2>I was studying the bandstructure of =
Cu4O3.&nbsp; I=20
used w2web to generate the bandstructure and DOS.&nbsp; In DOS figure, =
no DOS at=20
E(F) level.&nbsp; In bandstructure figure, however, a few bands cross =
the E(F)=20
level.&nbsp; I have inserted the E(F) value in case.insp =
file.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Could anyone help me figure out where =
the problem=20
might be?</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Thank you very much!</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Dadi Dai</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>P.S. </FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Long time ago, when I was using old =
version of=20
wien2k, I didn't have such a problem as long as I entered the correct =
E(F) in=20
the case.insp file.&nbsp; Now, I checked the data carefully and has =
given the=20
correct E(F) in the case.insp file, but I still have the =
problem.</FONT></DIV>
<DIV>&nbsp;</DIV></DIV></BODY></HTML></FONT></FONT>

- ------=_NextPart_000_004E_01C2B884.481980E0--

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------------------------------

Date: Fri, 10 Jan 2003 14:55:05 +0100
From: Georg Madsen <georg@chem.au.dk>
Subject: Re: [WIEN]: Why bandstructure is not consistent with DOS?

====
Georg Madsen <georg@chem.au.dk>
submitted the following contribution:
====

It could be you are using a bad k-mesh for the DOS. Try a non-shifted k-mesh
with more points.

Also, ghostwiev displays the figures from spaghetti slightly wrong. I have no
idea why, but try printing it.

 Georg

Quoting Dadi Dai <dai@unity.ncsu.edu>:

> I was studying the bandstructure of Cu4O3.  I used w2web to generate the
> bandstructure and DOS.  In DOS figure, no DOS at E(F) level.  In
> bandstructure figure, however, a few bands cross the E(F) level.  I have
> inserted the E(F) value in case.insp file.
> 
> Could anyone help me figure out where the problem might be?
> 
> Thank you very much!
> 
> Dadi Dai
> 
> P.S. 
> 
> Long time ago, when I was using old version of wien2k, I didn't have such a
> problem as long as I entered the correct E(F) in the case.insp file.  Now, I
> checked the data carefully and has given the correct E(F) in the case.insp
> file, but I still have the problem.
> 
> 


- ----------------------------
Georg Madsen
Dept. of Inorganic Chemistry
University of Aarhus
DK-8000 Århus C
Denmark
Tlf: +45 8942 3880
Fax: +45 8619 6199
- ----------------------------
====
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------------------------------

Date: Fri, 10 Jan 2003 09:37:45 -0500
From: "Dadi Dai" <dai@unity.ncsu.edu>
Subject: Re: [WIEN]: Why bandstructure is not consistent with DOS?

====
"Dadi Dai" <dai@unity.ncsu.edu>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_0067_01C2B88B.EE58D800
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	charset="iso-8859-1"
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Dear Georg Madsen,

Thank you very much for your reply.  Actually DOS figure may be more =
reasonable, because no DOS appears at E(f) and experimentally the system =
is insulating. =20

I tried to print out the bandstructure, and the print-out is same as =
what I saw on the screen.=20

So, could you or anyone else give me further helps?

Thank you very much!

Dadi Dai

P.S.  I have attached the two figures with my questions in my email sent =
to wien2k mailing list yesterday, but I don't know why I haven't seen my =
post so far.  So I resent my questions today, without attaching the =
figures.

- ----- Original Message -----=20
From: "Georg Madsen" <georg@chem.au.dk>
To: <wien@zeus.theochem.tuwien.ac.at>
Sent: Friday, January 10, 2003 8:55 AM
Subject: Re: [WIEN]: Why bandstructure is not consistent with DOS?


> =3D=3D=3D=3D
> Georg Madsen <georg@chem.au.dk>
> submitted the following contribution:
> =3D=3D=3D=3D
>=20
> It could be you are using a bad k-mesh for the DOS. Try a non-shifted =
k-mesh
> with more points.
>=20
> Also, ghostwiev displays the figures from spaghetti slightly wrong. I =
have no
> idea why, but try printing it.
>=20
>  Georg
>=20
> Quoting Dadi Dai <dai@unity.ncsu.edu>:
>=20
> > I was studying the bandstructure of Cu4O3.  I used w2web to generate =
the
> > bandstructure and DOS.  In DOS figure, no DOS at E(F) level.  In
> > bandstructure figure, however, a few bands cross the E(F) level.  I =
have
> > inserted the E(F) value in case.insp file.
> >=20
> > Could anyone help me figure out where the problem might be?
> >=20
> > Thank you very much!
> >=20
> > Dadi Dai
> >=20
> > P.S.=20
> >=20
> > Long time ago, when I was using old version of wien2k, I didn't have =
such a
> > problem as long as I entered the correct E(F) in the case.insp file. =
 Now, I
> > checked the data carefully and has given the correct E(F) in the =
case.insp
> > file, but I still have the problem.
> >=20
> >=20
>=20
>=20
> ----------------------------
> Georg Madsen
> Dept. of Inorganic Chemistry
> University of Aarhus
> DK-8000 =C5rhus C
> Denmark
> Tlf: +45 8942 3880
> Fax: +45 8619 6199
> ----------------------------


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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Diso-8859-1">
<META content=3D"MSHTML 6.00.2722.900" name=3DGENERATOR>
<STYLE></STYLE>
</HEAD>
<BODY>
<DIV><FONT face=3DArial size=3D2></FONT><FONT face=3DArial size=3D2>Dear =
Georg=20
Madsen,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Thank you very much for your =
reply.&nbsp; Actually=20
DOS figure may be more reasonable, because no DOS appears at E(f) and=20
experimentally the system is insulating.&nbsp; </FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>I tried to print out the bandstructure, =
and the=20
print-out is same as what I saw on the screen.&nbsp;</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>So, could you&nbsp;or anyone else give =
me further=20
helps?</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Thank you very much!</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>Dadi Dai</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>P.S.&nbsp; </FONT><FONT face=3DArial =
size=3D2>I have=20
attached the two figures with my questions&nbsp;in my email sent to =
wien2k=20
mailing list yesterday, but I don't know why I haven't seen my post so=20
far.&nbsp; So I resent my questions today, without attaching the=20
figures.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV>
<DIV><FONT face=3DArial size=3D2>----- Original Message ----- </FONT>
<DIV><FONT face=3DArial size=3D2>From: "Georg Madsen" &lt;</FONT><A=20
href=3D"mailto:georg@chem.au.dk"><FONT face=3DArial=20
size=3D2>georg@chem.au.dk</FONT></A><FONT face=3DArial =
size=3D2>&gt;</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>To: &lt;</FONT><A=20
href=3D"mailto:wien@zeus.theochem.tuwien.ac.at"><FONT face=3DArial=20
size=3D2>wien@zeus.theochem.tuwien.ac.at</FONT></A><FONT face=3DArial=20
size=3D2>&gt;</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Sent: Friday, January 10, 2003 8:55 =
AM</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Subject: Re: [WIEN]: Why bandstructure =
is not=20
consistent with DOS?</FONT></DIV></DIV>
<DIV><FONT face=3DArial><BR><FONT size=3D2></FONT></FONT></DIV><FONT =
face=3DArial=20
size=3D2>&gt; =3D=3D=3D=3D<BR>&gt; Georg Madsen &lt;</FONT><A=20
href=3D"mailto:georg@chem.au.dk"><FONT face=3DArial=20
size=3D2>georg@chem.au.dk</FONT></A><FONT face=3DArial =
size=3D2>&gt;<BR>&gt; submitted=20
the following contribution:<BR>&gt; =3D=3D=3D=3D<BR>&gt; <BR>&gt; It =
could be you are=20
using a bad k-mesh for the DOS. Try a non-shifted k-mesh<BR>&gt; with =
more=20
points.<BR>&gt; <BR>&gt; Also, ghostwiev displays the figures from =
spaghetti=20
slightly wrong. I have no<BR>&gt; idea why, but try printing it.<BR>&gt; =

<BR>&gt; &nbsp;Georg<BR>&gt; <BR>&gt; Quoting Dadi Dai &lt;</FONT><A=20
href=3D"mailto:dai@unity.ncsu.edu"><FONT face=3DArial=20
size=3D2>dai@unity.ncsu.edu</FONT></A><FONT face=3DArial =
size=3D2>&gt;:<BR>&gt;=20
<BR>&gt; &gt; I was studying the bandstructure of Cu4O3.&nbsp; I used =
w2web to=20
generate the<BR>&gt; &gt; bandstructure and DOS.&nbsp; In DOS figure, no =
DOS at=20
E(F) level.&nbsp; In<BR>&gt; &gt; bandstructure figure, however, a few =
bands=20
cross the E(F) level.&nbsp; I have<BR>&gt; &gt; inserted the E(F) value =
in=20
case.insp file.<BR>&gt; &gt; <BR>&gt; &gt; Could anyone help me figure =
out where=20
the problem might be?<BR>&gt; &gt; <BR>&gt; &gt; Thank you very =
much!<BR>&gt;=20
&gt; <BR>&gt; &gt; Dadi Dai<BR>&gt; &gt; <BR>&gt; &gt; P.S. <BR>&gt; =
&gt;=20
<BR>&gt; &gt; Long time ago, when I was using old version of wien2k, I =
didn't=20
have such a<BR>&gt; &gt; problem as long as I entered the correct E(F) =
in the=20
case.insp file.&nbsp; Now, I<BR>&gt; &gt; checked the data carefully and =
has=20
given the correct E(F) in the case.insp<BR>&gt; &gt; file, but I still =
have the=20
problem.<BR>&gt; &gt; <BR>&gt; &gt; <BR>&gt; <BR>&gt; <BR>&gt;=20
- ----------------------------<BR>&gt; Georg Madsen<BR>&gt; Dept. of =
Inorganic=20
Chemistry<BR>&gt; University of Aarhus<BR>&gt; DK-8000 =C5rhus C<BR>&gt; =

Denmark<BR>&gt; Tlf: +45 8942 3880<BR>&gt; Fax: +45 8619 6199<BR>&gt;=20
- ----------------------------<BR></FONT></BODY></HTML>

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------------------------------

Date: Fri, 10 Jan 2003 07:00:52 -0800 (PST)
From: yanming Ma <ymma66@yahoo.com>
Subject: Re: [WIEN]: Question about the parallelization

====
yanming Ma <ymma66@yahoo.com>
submitted the following contribution:
====

- --0-186897195-1042210852=:37002
Content-Type: text/plain; charset=us-ascii


Dear Dr. B.R. Sahu,
Thanks very much for your reply. I got the point. Thanks again.
Yanming Ma
 "Dr. B.R.Sahu" <sahu@matter3.ph.utexas.edu> wrote:====
"Dr. B.R.Sahu" 
submitted the following contribution:
====


Dear Ma

During compilation, if you dont choose the option for fine grained
parallalization, it will create only files for single processor(ie lapw0,
lapw1(c), lapw2 etc) and script for k-pt parallelization run lapw0para,
lapw1para etc. If you choose the optiion for fine grained paralleliztion
then in addition to the above files, the files for MPI parallel run like
lapw0_mpi, lapw1_mpi and lapw2_mpi will be created.

Now, whether the scripts run(sp)_lapw and other script pick up lapw*para
or lapw*_mpi during the run depends on the structure of the .machines 
file as you mentioned.

1) the format of your k-point parallelization file is correct provided you
have 4 k-points to distribute over four cpus(in your case tp0) and the
cpu's have all same speed.For efficiency, only if we have more k-points
then the processors or cpus then only we use k-point parallelization. but
imagine a case where you have a very large system say a supercell
containing large number of atoms say more than 40 and you expect it to be
metallic, for example.
In such cases, you need large number k-points to sample
the BZ so k-point parallelization is again useful.

2) fine grained parallelization file is to be slightly modified:

lapw0:tp0:1 tp0:1 tp0:1 tp0:1
1:tp0:1 tp0:1 tp0:1 tp0:1

it means lapw0_mpi will use 4 processors each having same speed and your 
sysetm has 1 k-point and lapw1_mpi runs on 4 processors in parallel.

Fine grained parallel will be computationally efficient if you have large
system(ie large number of atoms) and small number of k-points(1 or 2).
that's what UG says.

I myself have not tested so far the MPI parallel code, as it is giving
some problem. I am already in contact with Prof. Blaha regarding this.



Regards
sahu 



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- --0-186897195-1042210852=:37002
Content-Type: text/html; charset=us-ascii

<P>Dear Dr. B.R. Sahu,
<P>Thanks very much for your reply.&nbsp;I got&nbsp;the point. Thanks again.
<P>Yanming Ma
<P>&nbsp;<B><I>"Dr. B.R.Sahu" &lt;sahu@matter3.ph.utexas.edu&gt;</I></B> wrote:
<BLOCKQUOTE style="PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #1010ff 2px solid">====<BR>"Dr. B.R.Sahu" <SAHU@MATTER3.PH.UTEXAS.EDU><BR>submitted the following contribution:<BR>====<BR><BR><BR>Dear Ma<BR><BR>During compilation, if you dont choose the option for fine grained<BR>parallalization, it will create only files for single processor(ie lapw0,<BR>lapw1(c), lapw2 etc) and script for k-pt parallelization run lapw0para,<BR>lapw1para etc. If you choose the optiion for fine grained paralleliztion<BR>then in addition to the above files, the files for MPI parallel run like<BR>lapw0_mpi, lapw1_mpi and lapw2_mpi will be created.<BR><BR>Now, whether the scripts run(sp)_lapw and other script pick up lapw*para<BR>or lapw*_mpi during the run depends on the structure of the .machines <BR>file as you mentioned.<BR><BR>1) the format of your k-point parallelization file is correct provided you<BR>have 4 k-points to distribute over four cpus(in your case tp0) and the<BR>cpu's hav!
e all same speed.For efficiency, only if we have more k-points<BR>then the processors or cpus then only we use k-point parallelization. but<BR>imagine a case where you have a very large system say a supercell<BR>containing large number of atoms say more than 40 and you expect it to be<BR>metallic, for example.<BR>In such cases, you need large number k-points to sample<BR>the BZ so k-point parallelization is again useful.<BR><BR>2) fine grained parallelization file is to be slightly modified:<BR><BR>lapw0:tp0:1 tp0:1 tp0:1 tp0:1<BR>1:tp0:1 tp0:1 tp0:1 tp0:1<BR><BR>it means lapw0_mpi will use 4 processors each having same speed and your <BR>sysetm has 1 k-point and lapw1_mpi runs on 4 processors in parallel.<BR><BR>Fine grained parallel will be computationally efficient if you have large<BR>system(ie large number of atoms) and small number of k-points(1 or 2).<BR>that's what UG says.<BR><BR>I myself have not tested so far the MPI parallel code, as it is giving<BR>some problem.!
 I am already in contact with Prof. Blaha regarding this.<BR><BR><BR><BR>Regards<BR>sahu <BR><BR><BR><BR>====<BR>WIEN Mailing list: wien@zeus.theochem.tuwien.ac.at<BR>To (un)subscribe send mail to<BR>majordomo@zeus.theochem.tuwien.ac.at<BR>====</BLOCKQUOTE><p><br><hr size=1>Do you Yahoo!?<br>
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Date: Fri, 10 Jan 2003 12:05:01 -0500
From: "michel certier" <mcertier@mail.com>
Subject: [WIEN]: spin-orbit

====
"michel certier" <mcertier@mail.com>
submitted the following contribution:
====

Dear wien users. I am looking for some sampel of spi-orbit calculation.
And I am wondering if it's possible (true !!) to do optimization with normal scf and run the final (optimized structure) calulation with spin-orbit option.

Thank's
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------------------------------

Date: Fri, 10 Jan 2003 12:04:46 -0500
From: "michel certier" <mcertier@mail.com>
Subject: [WIEN]: spin-orbit

====
"michel certier" <mcertier@mail.com>
submitted the following contribution:
====

Dear wien users. I am looking for some sampel of spi-orbit calculation.
And I am wondering if it's possible (true !!) to do optimization with normal scf and run the final (optimized structure) calulation with spin-orbit option.

Thank's
- -- 
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------------------------------

Date: Sun, 12 Jan 2003 11:44:04 +0800
From: "liu wan" <wien97wan@hotmail.com>
Subject: [WIEN]: Question about lapw1

====
"liu wan" <wien97wan@hotmail.com>
submitted the following contribution:
====

This is a multi-part message in MIME format.

- ------=_NextPart_000_4015_3003_2e6f
Content-Type: text/plain; format=flowed

Dear All

I try to calculate the electronic structure of ZrMoO. The lapw1 is OK, print 
"STOP LAPW1 END statement executed", and the lapw1.error is empty. But the 
ZrMoO.vector file is also empty! Why the lapw1 had been execute, but the 
vector file had not been written?

Best wish

Liu




_________________________________________________________________
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- ------=_NextPart_000_4015_3003_2e6f
Content-Type: text/plain; name="ZrMoO.inst"; format=flowed
Content-Transfer-Encoding: 8bit
Content-Disposition: attachment; filename="ZrMoO.inst"

Zr
Kr 2 5
4, 2,2.0  N
4, 2,0.0  N
5,-1,1.0  N
5,-1,1.0  N
Zr
Kr 2 5
4, 2,2.0  N
4, 2,0.0  N
5,-1,1.0  N
5,-1,1.0  N
Mo
Kr 3 5
4, 2,2.0  N
4, 2,1.0  N
4,-3,2.0  N
4,-3,0.0  N
5,-1,1.0  N
5,-1,0.0  N
O
He 3 5
2,-1,1.0  N
2,-1,1.0  N
2, 1,1.0  N
2, 1,1.0  N
2,-2,2.0  N
2,-2,0.0  N
O
He 3 5
2,-1,1.0  N
2,-1,1.0  N
2, 1,1.0  N
2, 1,1.0  N
2,-2,2.0  N
2,-2,0.0  N
O
He 3 5
2,-1,1.0  N
2,-1,1.0  N
2, 1,1.0  N
2, 1,1.0  N
2,-2,2.0  N
2,-2,0.0  N
O
He 3 5
2,-1,1.0  N
2,-1,1.0  N
2, 1,1.0  N
2, 1,1.0  N
2,-2,2.0  N
2,-2,0.0  N
****     End of Input
****     End of Input


- ------=_NextPart_000_4015_3003_2e6f
Content-Type: text/plain; name="ZrMoO.struct"; format=flowed
Content-Transfer-Encoding: 8bit
Content-Disposition: attachment; filename="ZrMoO.struct"

ZrMo2O8-alpha
H   LATTICE,NONEQUIV. ATOMS: 7                     163 P-31c
MODE OF CALC=RELA
18.857703 18.857703 21.701365 90.000000 90.000000120.000000
ATOM= -1: X=0.00000000 Y=0.00000000 Z=0.00000000
          MULT= 2          ISPLIT= 4
      -1: X=0.00000000 Y=0.00000000 Z=0.50000000
Zr         NPT=  781  R0=0.00001000 RMT=    2.0000   Z: 40.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -2: X=0.33333300 Y=0.66666700 Z=0.97520000
          MULT= 4          ISPLIT= 4
      -2: X=0.66666700 Y=0.33333300 Z=0.02480000
      -2: X=0.66666700 Y=0.33333300 Z=0.47520000
      -2: X=0.33333300 Y=0.66666700 Z=0.52480000
Zr         NPT=  781  R0=0.00001000 RMT=    2.0000   Z: 40.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -3: X=0.32980000 Y=0.33750000 Z=0.14778000
          MULT=12          ISPLIT= 8
      -3: X=0.67020000 Y=0.66250000 Z=0.85222000
      -3: X=0.66250000 Y=0.99230000 Z=0.14778000
      -3: X=0.33750000 Y=0.00770000 Z=0.85222000
      -3: X=0.33750000 Y=0.32980000 Z=0.64778000
      -3: X=0.66250000 Y=0.67020000 Z=0.35222000
      -3: X=0.00770000 Y=0.67020000 Z=0.14778000
      -3: X=0.99230000 Y=0.32980000 Z=0.85222000
      -3: X=0.67020000 Y=0.00770000 Z=0.64778000
      -3: X=0.32980000 Y=0.99230000 Z=0.35222000
      -3: X=0.99230000 Y=0.66250000 Z=0.64778000
      -3: X=0.00770000 Y=0.33750000 Z=0.35222000
Mo         NPT=  781  R0=0.00001000 RMT=    1.6000   Z: 42.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -4: X=0.16000000 Y=0.15000000 Z=0.09700000
          MULT=12          ISPLIT= 8
      -4: X=0.84000000 Y=0.85000000 Z=0.90300000
      -4: X=0.85000000 Y=0.01000000 Z=0.09700000
      -4: X=0.15000000 Y=0.99000000 Z=0.90300000
      -4: X=0.15000000 Y=0.16000000 Z=0.59700000
      -4: X=0.85000000 Y=0.84000000 Z=0.40300000
      -4: X=0.99000000 Y=0.84000000 Z=0.09700000
      -4: X=0.01000000 Y=0.16000000 Z=0.90300000
      -4: X=0.84000000 Y=0.99000000 Z=0.59700000
      -4: X=0.16000000 Y=0.01000000 Z=0.40300000
      -4: X=0.01000000 Y=0.85000000 Z=0.59700000
      -4: X=0.99000000 Y=0.15000000 Z=0.40300000
O          NPT=  781  R0=0.00010000 RMT=    1.3500   Z:  8.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -5: X=0.33400000 Y=0.50600000 Z=0.09230000
          MULT=12          ISPLIT= 8
      -5: X=0.66600000 Y=0.49400000 Z=0.90770000
      -5: X=0.49400000 Y=0.82800000 Z=0.09230000
      -5: X=0.50600000 Y=0.17200000 Z=0.90770000
      -5: X=0.50600000 Y=0.33400000 Z=0.59230000
      -5: X=0.49400000 Y=0.66600000 Z=0.40770000
      -5: X=0.17200000 Y=0.66600000 Z=0.09230000
      -5: X=0.82800000 Y=0.33400000 Z=0.90770000
      -5: X=0.66600000 Y=0.17200000 Z=0.59230000
      -5: X=0.33400000 Y=0.82800000 Z=0.40770000
      -5: X=0.82800000 Y=0.49400000 Z=0.59230000
      -5: X=0.17200000 Y=0.50600000 Z=0.40770000
O          NPT=  781  R0=0.00010000 RMT=    1.3500   Z:  8.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -6: X=0.52300000 Y=0.35200000 Z=0.12990000
          MULT=12          ISPLIT= 8
      -6: X=0.47700000 Y=0.64800000 Z=0.87010000
      -6: X=0.64800000 Y=0.17100000 Z=0.12990000
      -6: X=0.35200000 Y=0.82900000 Z=0.87010000
      -6: X=0.35200000 Y=0.52300000 Z=0.62990000
      -6: X=0.64800000 Y=0.47700000 Z=0.37010000
      -6: X=0.82900000 Y=0.47700000 Z=0.12990000
      -6: X=0.17100000 Y=0.52300000 Z=0.87010000
      -6: X=0.47700000 Y=0.82900000 Z=0.62990000
      -6: X=0.52300000 Y=0.17100000 Z=0.37010000
      -6: X=0.17100000 Y=0.64800000 Z=0.62990000
      -6: X=0.82900000 Y=0.35200000 Z=0.37010000
O          NPT=  781  R0=0.00010000 RMT=    1.3500   Z:  8.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
ATOM= -7: X=0.31700000 Y=0.34500000 Z=0.29090000
          MULT=12          ISPLIT= 8
      -7: X=0.68300000 Y=0.65500000 Z=0.70910000
      -7: X=0.65500000 Y=0.97200000 Z=0.29090000
      -7: X=0.34500000 Y=0.02800000 Z=0.70910000
      -7: X=0.34500000 Y=0.31700000 Z=0.79090000
      -7: X=0.65500000 Y=0.68300000 Z=0.20910000
      -7: X=0.02800000 Y=0.68300000 Z=0.29090000
      -7: X=0.97200000 Y=0.31700000 Z=0.70910000
      -7: X=0.68300000 Y=0.02800000 Z=0.79090000
      -7: X=0.31700000 Y=0.97200000 Z=0.20910000
      -7: X=0.97200000 Y=0.65500000 Z=0.79090000
      -7: X=0.02800000 Y=0.34500000 Z=0.20910000
O          NPT=  781  R0=0.00010000 RMT=    1.3500   Z:  8.0
LOCAL ROT MATRIX:    1.0000000 0.0000000 0.0000000
                     0.0000000 1.0000000 0.0000000
                     0.0000000 0.0000000 1.0000000
  12      NUMBER OF SYMMETRY OPERATIONS
- -1 1 0 0.0000000
- -1 0 0 0.0000000
0 0 1 0.0000000
       1
- -1 0 0 0.0000000
0-1 0 0.0000000
0 0-1 0.0000000
       2
0 1 0 0.0000000
- -1 1 0 0.0000000
0 0-1 0.0000000
       3
0-1 0 0.0000000
1-1 0 0.0000000
0 0 1 0.0000000
       4
1 0 0 0.0000000
0 1 0 0.0000000
0 0 1 0.0000000
       5
1-1 0 0.0000000
1 0 0 0.0000000
0 0-1 0.0000000
       6
1 0 0 0.0000000
1-1 0 0.0000000
0 0-1 0.5000000
       7
- -1 1 0 0.0000000
0 1 0 0.0000000
0 0-1 0.5000000
       8
0 1 0 0.0000000
1 0 0 0.0000000
0 0 1 0.5000000
       9
1-1 0 0.0000000
0-1 0 0.0000000
0 0 1 0.5000000
      10
0-1 0 0.0000000
- -1 0 0 0.0000000
0 0-1 0.5000000
      11
- -1 0 0 0.0000000
- -1 1 0 0.0000000
0 0 1 0.5000000
      12


- ------=_NextPart_000_4015_3003_2e6f--
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End of wien-digest V2002 #51
****************************

