[Wien] MIXER runtime error + solution on Mac OS X

2014-09-03 Thread Martin Kroeker
I would expect the __APPLE__ define to come in automatically from your
compiler and/or system headers. 
The NaNs are interesting - could this be another case of uninitialized
array elements, just like the lapw0 bug you found last month ? Heap vs
stack would then just change the likelyhood of obtaining (non-)zeroed
memory on allocation...
-- 
Dr. Martin Kroekermar...@ruby.chemie.uni-freiburg.de
c/o Prof.Dr. Caroline Roehr
Institut fuer Anorganische und Analytische Chemie der Universitaet Freiburg

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[Wien] Calculation about the effect of external magnetic field

2014-09-03 Thread 李艳丽
Dear Dr. Gerhard H. Fecher,
Thank you very much for your reply. So for example, if I want to see the 
effect of external magnetic field on the properties(such as the Fermi level, 
DOS and Bandstructures) of Fe3O4(the saturated magnetic moment of Fe3O4/unit 
cell is about 8.0. mu_B ) , I am wondering whether I should  try runfsm_lapw 
-m -7.0(or other non-saturated value of magnetic moment) -orb ?
   Thank you again!
Best Regards,
Yanli___
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Re: [Wien] Calculation about the effect of external magnetic field

2014-09-03 Thread pieper

Dear Yanli,

you did not answer the crucial question:

what is the size of the field you put in your calculation?

My guess is that it simply is much too small to see any effect in, e.g. 
the DOS. You plot the DOS on energy scales of eV. Compare that to the 
energy of the moment of an electron in the field you chose - I  expect 
something like 1 T - so maybe you calculate 1 mu_B*1 T  ... then decide 
if you should be able to see the shift in energy corresponding to that 
field.


Best regards,

Martin Pieper

---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564


Am 03.09.2014 09:42, schrieb 李艳丽:

Dear Dr. Gerhard H. Fecher,
 Thank you very much for your reply. So for example, if I want to see
the effect of external magnetic field on the properties(such as the
Fermi level, DOS and Bandstructures) of Fe3O4(the saturated magnetic
moment of Fe3O4/unit cell is about 8.0. mu_B ) , I am wondering
whether I should try runfsm_lapw -m -7.0(or other non-saturated value
of magnetic moment) -orb ?
 Thank you again!
Best Regards,
Yanli


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Re: [Wien] Hard charge convergence

2014-09-03 Thread Luis Ogando
Dear Prof. Tran,

   Thank you again !
   All the best,
  Luis


2014-09-02 17:32 GMT-03:00 t...@theochem.tuwien.ac.at:

 What is important for geometry optimization is to require also force
 convergence (-fc) with a value like 0.5 or 1 (see user's guide).



 On Tue, 2 Sep 2014, Luis Ogando wrote:

  Dear Professor Tran,

Thank you for your response.
Actually, I am doing structure optimization, so energy is the most
 important parameter (and forces due to free parameters). Perhaps, I am
 being
 too strict when asking for charge convergence during structure
 optimization.
 What is your opinion ?
Thank you again.
All the best,
  Luis


 2014-09-02 16:59 GMT-03:00 t...@theochem.tuwien.ac.at:
   Hi,

   It depends on your needs. Just use the command grep to see
   if the quantity you are interested in particular (e.g., magnetic
   moment
   or band gap) seems to have reached a degree of convergence
   which satisfies you.

   F. Tran

   On Tue, 2 Sep 2014, Luis Ogando wrote:

 Dear Wien2k community,

I would like some general hints for a system with
 a difficult charge convergence.
In my case, I got the energy convergence (-ec
 0.0001), but not the charge one (-cc 0.0001).
Would it be acceptable to increase the charge
 convergence criterion to -cc 0.0005 ? I am getting
 charge changes bellow this value.
All the best,
 Luis


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[Wien] Calculation about the effect of external magnetic field

2014-09-03 Thread 李艳丽
Dear Dr. Martin Pieper,
Thank you for your help! For my calculation, I have ever tried different 
values of magnetic field ( 0.1 T, 1T, and 10T) and all of them have no effects 
on the electronic structures such as DOS, or bandstructures e.g. So you mean I 
should try a even larger magnetic field ?
   Thank you again!
Best Regards,
Yanli

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Re: [Wien] Calculation about the effect of external magnetic field

2014-09-03 Thread Gavin Abo
You did Dr. Pieper's exercise [ 
http://www.mail-archive.com/wien%40zeus.theochem.tuwien.ac.at/msg11090.html 
]?


For example:

muB = ~5.7884*10^-5 eV/T [ http://en.wikipedia.org/wiki/Bohr_magneton ]

muB*Bext = (5.7884*10^-5 eV/T)*(10 T) = 5.7884*10^-4 eV

Likely the point is, say you plot DOS with an energy range of -5 to 5 eV 
with 1 eV major increments.  Probably, you are not going to see any 
change in the DOS plot with a 10 T field.  muB*Bext would likely need to 
be on the order of about 0.1 eV (corresponding to Bext = ~1728 T) to see 
any change with that energy range scale.  If on the other hand the plot 
of your DOS was say plotted with an energy range of -10*10^-3 eV to 
10*10^-3 eV with 1*10^-3 eV increments, then the change with a 10 T 
field would probably be noticeable (unless it is overwhelmed by noise in 
the numerical calculation [ 
http://www.mail-archive.com/wien%40zeus.theochem.tuwien.ac.at/msg09466.html 
]).


So you need to either change the energy scale of your plots or increase 
the magnetic field value to see the effects.


On 9/3/2014 7:31 PM, ??? wrote:

Dear Dr. Martin Pieper,
Thank you for your help! For my calculation, I have ever tried 
different values of magnetic field ( 0.1 T, 1T, and 10T) and all of 
them have no effects on the electronic structures such as DOS, or 
bandstructures e.g. So you mean I should try a even larger magnetic 
field ?

   Thank you again!
Best Regards,
Yanli
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[Wien] Bethe-Salpeter Equition

2014-09-03 Thread Chikashi Suzuki (鈴木知史)
Dear Prof. Blaha and Wien2k users

My name is Chikashi Suzuki, from Japan Atomic Energy Agency.
I am running wien version WIEN2k 10.1.

I have tried to caclulate Cs M4,5 Xay absoprtion spectra of Cs compound.
Cs M4,5 XANES of CsCl is well reproduced
in case where the core hole is 0.6 (not 1.0),
though I cannot find this reason.

I found some studies where XANES spectra are well-repsoduced
using Bethe-Salpeter Equition with Wien2k code.
However, I cannot find how to calculate  XANES spectra using
Bethe-Salpeter Equition with Wien2k code.
(For example, what input file to use, and what to write
 in the input file)

What should I do in order to calculate XANES spectra using
Bethe-Salpeter Equition with Wien2k code.

Sincerely yours

***
Dr. Chikashi Suzuki
Research Group for Accident Progression Analysis
Nuclear Science and Engineering Center
Japan Atomic Energy Agency
Tokai-mura, Naka-gun, Ibaraki-ken 319-1195, Japan
Tel: +81-29-282-5386
E-mail:suzuki.chika...@jaea.go.jp
***
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Re: [Wien] Bethe-Salpeter Equition

2014-09-03 Thread Kevin Jorissen
Dear Chikashi,

from your question I guess that you do not know the theory behind BSE and
WIEN2k, so I will give some background information:

Bethe-Salpeter is a whole different game: it is a completely different
theory than Density Functional Theory (DFT).  BSE solves an explicit
many-body equation (the basis consists of two-particle wave functions)
while WIEN2k/DFT solves an effective single-particle equation (Kohn-Sham
equation).  WIEN2k does not include BSE calculations.

The codes that do BSE are generally harder to install and to use than
WIEN2k.  They also take much longer to calculate (you need more CPUs and
more memory).

There is a separate code based on WIEN2k that does BSE calculations.  There
are also other codes such as Exc!ting, OCEAN, and a few others that can do
the BSE calculation.   Again, these calculations are generally a bit more
difficult than WIEN2k.

The strength of the core hole (0.6 vs. 1.0) is an arbitrary parameter.
 Roughly speaking it represents the strength of the screening (i.e. how
quickly and efficiently surrounding electrons respond to the presence of
the core hole and screen it, thus modifying the interaction between the
core hole and the photoelectron resulting from the excitation).  This
approach is an approximation to the true many-body description of the
problem (such as BSE) and therefore it is justifiable to use whatever value
of the core hole gives the best results.  In most cases people use 0, 0.5,
or 1.0 because these can be conceptually understood.  But as I said,
whichever value gives the best result compared to experiment, is obviously
the best static description of the screening that you will be able to
find in a DFT calculation, so go ahead and use 0.6.  In the BSE you would
not have this parameter of core hole strength per se.  The screening will
be calculated (and is frequency dependent, not just a number).  However
there may be other somewhat ad hoc parameters in a BSE calculation, and
such calculations are less established routine than a DFT calculation.

If you get a good result from using WIEN2k with a 0.6 core hole, I'd
personally declare victory and stop there.  Just add 2 sentences about
screening to your paper and referees will make no problem of that.
 Apparently your material is sufficiently well described by a DFT
Final-State-Rule approach.


Also, you should go to wien2k.at and download a newer version of WIEN2k.
 Your version is 4 years old and has many bugs that have since been fixed,
as well as improved performance and new functionality.

Cheers,

Kevin




On Wed, Sep 3, 2014 at 9:51 PM, Chikashi Suzuki (鈴木知史) 
suzuki.chika...@jaea.go.jp wrote:

 Dear Prof. Blaha and Wien2k users

 My name is Chikashi Suzuki, from Japan Atomic Energy Agency.
 I am running wien version WIEN2k 10.1.

 I have tried to caclulate Cs M4,5 Xay absoprtion spectra of Cs compound.
 Cs M4,5 XANES of CsCl is well reproduced
 in case where the core hole is 0.6 (not 1.0),
 though I cannot find this reason.

 I found some studies where XANES spectra are well-repsoduced
 using Bethe-Salpeter Equition with Wien2k code.
 However, I cannot find how to calculate  XANES spectra using
 Bethe-Salpeter Equition with Wien2k code.
 (For example, what input file to use, and what to write
  in the input file)

 What should I do in order to calculate XANES spectra using
 Bethe-Salpeter Equition with Wien2k code.

 Sincerely yours

 ***
 Dr. Chikashi Suzuki
 Research Group for Accident Progression Analysis
 Nuclear Science and Engineering Center
 Japan Atomic Energy Agency
 Tokai-mura, Naka-gun, Ibaraki-ken 319-1195, Japan
 Tel: +81-29-282-5386
 E-mail:suzuki.chika...@jaea.go.jp
 ***
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