d, silver, chromium, titanium, and aluminum in the visible
> bandwidth":
>
> https://doi.org/10.1117/1.JNP.8.083097
>
> On 1/15/2021 6:26 PM, karima Physique wrote:
> > Dear WIEN2k users,
> > for intraband contribution, where can I find the value of Gamma for
>
Dear WIEN2k users,
for intraband contribution, where can I find the value of Gamma for Drude
term
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Dear WIEN2k users,
How to find the optimized structure after an optimization using option 7 (a
b c and gamma) for monoclinic case?
Thank you in advance
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Dear wien2k users,
When I run the x w2w -p command, I see that there is a one core occupied
(non-parallel) despite the presence of the machine file
Any suggestions?
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.ac.at>> a écrit :
> >
> > Clearly, omp_global:12 is NOT efficient for lapw1. The
> > diagonalization
> > does not scale for so many cores.
> >
> > Otherwise it means that your mpi-installation (what are you using ?
> >
pw1. The diagonalization
> does not scale for so many cores.
>
> Otherwise it means that your mpi-installation (what are you using ?
> ifort, gfortran, which mpi, blas, scalapack, elpa, ...) is VERY bad.
>
>
> On 8/27/20 1:44 PM, karima Physique wrote:
> > Dear Wien2k users,
Dear Wien2k users,
A calculation with 38 equivalent atoms (96 inequivalent ), we found that
using lapw1 with omp_global is very faster than lapw1_mpi
machine file 1
omp_global: 12
1: node1
machine file 2
1: node1:12
Have you any comment on this?
___
Dear Prof. P Blaha and F. Tran
if I understand correctly, for the different parts of the susceptibility, I
can use the induced field of each part and I can use the equation 5.1 of
the userguide
Is this correct?
Le lun. 13 mai 2019 à 22:41, karima Physique a
écrit :
> Thank you prof. F. T
22:22, a écrit :
> Some guidance here:
>
> https://www.bc.edu/content/dam/bc1/schools/mcas/physics/pdf/wien2k/Hyperfine_NMR.pdf
>
>
> On Monday 2019-05-13 22:19, karima Physique wrote:
>
> >Date: Mon, 13 May 2019 22:19:28
> >From: karima Physique
> >Re
ields in our workshop notes).
>
>
> Am 11.05.2019 um 18:15 schrieb karima Physique:
> > Dear Prof. P. Blaha and Wien2k users;
> >
> > 1) how to calculate the orbital part of susceptibility for spinpolarized
> > case using
> > x nmr lapw -mode in1
> > do I ha
Dear Wien2k users;
how to calculate the dielectric function for spin-up only? or for spin-dn
only?
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hwestern.edu
>
> On Thu, Nov 22, 2018, 5:18 PM karima Physique
> wrote:
>
>> Dear Prof. Laurence Marks
>>
>> do you mean that I have to be content with -ec 0.001 as a convergence
>> criterion?
>>
>> Le jeu. 22 nov. 2018 à 23:58, Laurence Marks
&g
stern.edu
>
> On Thu, Nov 22, 2018, 3:33 PM karima Physique
> wrote:
>
>> Dear Dr. Gavin Abo;
>>
>> I use WIEN2k_18.2 and I have already tried this method on a material
>> based on Iron and it works very well but for another material based on Mn,
>> the calcu
the d energy value in
> case.in1 shown in Constraint_U.pdf but it worked after following the "[3]
> Usually it is better to just set the d energy 2-4 Ry above the Fermi
> level..." in that same file [
> https://www.mail-archive.com/wien@zeus.theochem.tuwien.ac.at/msg15599.html
> ].
Dear Wien2k user;
Using cLDA method , I modified case.in2 according to the example in
http://susi.theochem.tuwien.ac.at/reg_user/textbooks/Constraint_U.pdf by
replacing
TETRA 0.000 by GAUSS 0.006 but after more than 500 cycle, calculation does
not converge (the convergence does not exceed 0.001)
inimization has been done. In addition, MSR1a
> often works better when started from a partial minimization where the
> density and pseudo-charges are somewhat converged. For a large problem add
> "-noHinv", I have had problems with -min and -it in the past.
>
> On Mon, Oct
Dear Wien2k user;
According to user guide, after a SCF cycle with runsp -fc 1 we continue
with run runsp -min
I want to know which of these two methods is the correct one:
1)
runsp -fc 1
runsp -min
runsp -min -fc 0.5 -ec 0.0001 -cc 0.001
or
2)
runsp -fc 1
runsp -min -fc 0.5 -ec 0.0001 -cc 0.001
/scatter-plot-with-different-size-for-each-point
> , http://gnuplot.sourceforge.net/docs_4.2/node100.html ] or Indexed Size
> (Bubble) and Color Map Graph in Origin [
> https://www.originlab.com/doc/Origin-Help/2DSym-Graph ].
> On 8/28/2018 11:40 AM, karima Physique wrote:
>
> Dear dr. Oleg
Dear dr. Oleg Rubel and Wien2k users:
1- do you have any idea to how to plot the band strcture using gnuplot or
Originlab (transform F2B file to dataplot file with X:Y columns).
2- the unit of energy is it eV or Ry in F2B file
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most appropriate one to reach one of the Intel company's experts for
> the Intel Parallel Studio Cluster Edition.
> On 7/19/2018 10:57 AM, Laurence Marks wrote:
>
> As I said, this is in your IB (or similar) fabric.
>
> On Thu, Jul 19, 2018 at 11:54 AM, karima Physique <
> p
, Laurence Marks a
écrit :
> See
>
> https://www.google.com/search?q=no+hfi+units+are+available+(err%3D23)=no+hfi+units+are+available+(err%3D23)=chrome..69i57.481j0j4=chrome=UTF-8
>
> This appears to be an issue with your local mpi/fabric.
>
> On Thu, Jul 19, 2018 at 8:0
her possible cause of
> the problem.
>
> Unfortunately, since I don't have access to a system having that exact
> same error, it is hard to see why those errors are happening as there seems
> to be many possible causes of that problem and not a single one.
>
> Kind Regards,
>
> G
hosts file if that happens to be the
> source of the problem.
> On 7/18/2018 6:07 PM, karima Physique wrote:
>
> Dear wien2k users:
>
> Using the folowing machines files :
> lapw0:master:12
> dstart:master:12
> 1:master:12
> 1:node1:12
> 1:node2:12
> ..
> the calculat
Dear wien2k users:
Using the folowing machines files :
lapw0:master:12
dstart:master:12
1:master:12
1:node1:12
1:node2:12
..
the calculation works very well, but using the following machines file:
lapw0:master:12 node1:12 node2:12
dstart:master:12 node1:12 node2:12
1:master:12
1:node1:12
> calculate-u-parameter-in-nickel.html
> [2] http://susi.theochem.tuwien.ac.at/reg_user/textbooks/Constraint_U.pdf
>
>
> On 3/5/2018 4:00 PM, karima Physique wrote:
>
> Dear wien2k users:
>
> According to Georg K. H. Madsen and Pavel Novak method for the estimation
> of U
Dear wien2k users:
According to Georg K. H. Madsen and Pavel Novak method for the estimation
of Ueff, they use the penultimate eigenvalue of d orbital d (head -2 | tail
-1), I would be grateful if you can explain to me why they did not take the
last value (tail -1)?
Thank you in advance
-archive.com/wien@zeus.theochem.tuwien.ac.at/msg05054.html
>
> On 3/3/2018 6:00 AM, karima Physique wrote:
>
> Thank you very much Prof. Gavin Abo
> I have another question about this query
> case.inst file also contains the occupations with their spins, if we
> remove electrons from
ulate-u-parameter-in-nickel.html
>
> [3] https://www.mail-archive.com/wien@zeus.theochem.tuwien.ac.
> at/msg14460.html
> On 3/2/2018 6:35 PM, karima Physique wrote:
>
> Dear Prof. P. Blaha and Wien2k users:
>
> When using the method described by Georg K. H. Madsen and Pa
Dear Prof. P. Blaha and Wien2k users:
When using the method described by Georg K. H. Madsen and Pavel Novak for
the calculation of Ueff, should we add the electrons of d-orbital in
case.inst file that we removed from the case.incup/dn file or we only
modify case.incup/dn .?.
l-archive.com/wien@zeus.theochem.tuwien.ac.at/msg15118.html
>
> or maybe a newer version of Wien2Wannier is needed:
>
> https://www.mail-archive.com/wien@zeus.theochem.tuwien.ac.at/msg16099.html
>
>
> On 12/26/2017 9:08 AM, karima Physique wrote:
>
>> Dear Prof. P. BLAHA and WIEN2k use
Dear Prof. P. BLAHA and WIEN2k users:
I got this error "write_inwf: error: unrecognized arguments: -up "
when launching the command ""init_w2w -up""
how to solve it please
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Dear prof. P. Blaha and wien2k users :
I am still waiting for your answers and I thank you in advance.
my question was :
Does Ueff=U-J or Ueff=U- 1/2 J? how to estimate J using constrained DFT.?
Thank you in advance
2017-11-27 12:05 GMT+01:00 karima Physique <physique.kar...@gmail.
Dear Wien2k users:
Does Ueff=U-J or Ueff=U- 1/2 J? how to estimate J using constrained DFT.?
Thank you in advance
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ination_language=http://www.slab.phys.nagoya-u.ac.jp/
> ai/pukiwiki/index.php?wien2wannier
>
> [2] http://susi.theochem.tuwien.ac.at/events/ws2017/notes/
> tutorial-Wannier.pdf (slide 6)
>
> On 11/24/2017 4:43 PM, karima Physique wrote:
>
> Dear Prof. P. Blaha and Wien2k users;
>
Dear Prof. P. Blaha and Wien2k users;
how to fix this error with write_win command
Input parameter hr_plot is no longer used. Please use write_hr instead.
Error: examine the output/error file for details
0.012u 0.007s 0:00.02 50.0% 0+0k 0+8io 0pf+0w
orthwestern.edu
>
> On Nov 24, 2017 8:28 AM, "karima Physique" <physique.kar...@gmail.com>
> wrote:
>
>> Dear wien2k users:
>>
>> how can i determine the energy range (minimum and maximum) of 4f orbital
>> (bands) after a SCF calcu
Dear wien2k users:
how can i determine the energy range (minimum and maximum) of 4f orbital
(bands) after a SCF calculation.
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Dear Prof. Laurence Marks
Thank you very much
2017-11-24 14:44 GMT+01:00 Laurence Marks <l-ma...@northwestern.edu>:
> I think this is right, but I have not checked the notes on the web site.
>
> Note: be careful about spin.
>
> On Fri, Nov 24, 2017 at 7:24 AM, karima Phys
-ma...@northwestern.edu>:
> In my experience, yes.
>
> On Nov 23, 2017 6:13 PM, "karima Physique" <physique.kar...@gmail.com>
> wrote:
>
>> Dear wien2k users;
>>
>> can we use the method described by G. K. H. Madsen and P. No
Dear wien2k users;
can we use the method described by G. K. H. Madsen and P. Novák to estimate
the hubbard term for the 4f elements.?
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arge spin susceptibility of antiferromagnetic
> insulators.
>
> Best regards,
>
> ---
> Dr. Martin Pieper
> Karl-Franzens University
> Institute of Physics
> Universitätsplatz 5
> <https://maps.google.com/?q=Universit%C3%A4tsplatz+5=gmail=g>
> A-8010 Graz
>
ty, i.e. itinerant electrons near the Fermi level. But I
> might be wrong.
>
>
>
>
>
> On Sat, Sep 30, 2017 at 8:40 AM, karima Physique <
> physique.kar...@gmail.com> wrote:
>
>> Dear Prof. P. Blaha and Wien2k user;
>>
>>
>> Is the spin pa
Dear Prof. P. Blaha and Wien2k user;
Is the spin part of the magnetic susceptibility due to the contribution of
delocalized electrons only?
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Dear Prof. P. Blaha and wien2k users;
what the meaning of the number 6.258116 in the expression of spin
susceptibility?
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Dear Prof P. Blaha and Wien2k users;
The unit of the spin susceptibility in the userguide is indicated in (10^6
cm^3 / mol*cell) but when I calculate it I find a value of the order of
10-6 which seems to me that the unit is (cm^3 / mol*cell) and not (10^6
cm^3 / mol*cell).
I just want to know
gt; you want to convert it to the mass susceptibility in cm3/g? If so you
> need to divide by the relative molecular mass.
>
>
>
> Should you not use SI rather than cgs units?
>
>
>
>
>
> Elaine A. Moore
>
>
>
> *From:* Wien [mailto:wien-boun...@zeus.theochem.tu
> Universitätsplatz 5
> <https://maps.google.com/?q=Universit%C3%A4tsplatz+5=gmail=g>
> A-8010 Graz
> Austria
> Tel.: +43-(0)316-380-8564
>
>
> Am 22.09.2017 15:16, schrieb karima Physique:
>
>> Dear Wien2k users:
>>
>> how to convert the magnetic sus
In this message you find the correction of this error:
http://www.mail-archive.com/wien@zeus.theochem.tuwien.ac.at/msg16069.html
2017-07-22 13:18 GMT+02:00 Dürrschnabel, Michael <
duerrschna...@geo.tu-darmstadt.de>:
> Dear Wien2k users,
>
>
> I am running Wien2k version 17.1 on a Dual Core
If you run a parallel calculation, you must first lunch the command:
gather_energy.pl
2017-07-21 3:35 GMT+02:00 Lagoun brahim :
> hallo every one
>
> i am doing a transport properties calculation with (wien2k14.2+BoltzTraP
> 1.2.5) code but when i execute: x_trans
Prof. Fecher
> and read up on the subject of magnetism in solids. Perhaps start with
> something on solid state physics in general, not a specialized treatment of
> magnetism. Personally I like the introduction to Solid State Physics by
> Ashcroft and Mermin.
>
> Good luck
&g
>From what I have understood from userguide and Prof P Blaha's replies; For
semiconductor and insulator; there is the orbital part of the magnetic
susceptibility only but for the metals there is also the spin part and I
ask Prof. P Blaha and Prof Gerhard Fecher to confirm this answer or to
Dear Wien2k users;
I am still waiting for your answers and I thank you in advance.
I have 2 questions concerning the use of the FHI-gap code
1- How to determine the term of Hubbard using FHI-gap code.
2- how to lunch a GW and G0W0 calculation
2017-06-13 4:46 GMT+02:00 karima Physique
Dear Wien2k users,
I have 2 questions concerning the use of the FHI-gap code
1- How to determine the term of Hubbard using FHI-gap code.
2- how to lunch a GW and G0W0 calculation.
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Thank you very much
2017-06-11 8:43 GMT+02:00 <t...@theochem.tuwien.ac.at>:
> LDA+U, onsite hybrid, and full hybrid are all supposed to be
> better than normal LDA/GGA for correlated systems.
> It would not really make sense to mix them together.
>
> On Sunday 2017-06-11 0
Dear wien2k users;
Are the full hybrid funtional sufficient for the treatment of highly
correlated systems (use of full hybrid functional without the need to add
the hubbard term).
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p (bigger than just 5 mRy), you don't need the -metal
> switch, otherwise use it (and select TEMP 0.00x; x=2-6)
>
>
> On 05/29/2017 07:09 PM, karima Physique wrote:
>
>> Dear Wien2k users;
>>
>> I want to run an NMR calculation for a semimeta
Dear Wien2k users;
I want to run an NMR calculation for a semimetal compound so is I using
x_nmr only or x_nmr -metal?
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(with wien2k_16.1).
>
>
> On 05/15/2017 11:20 PM, karima Physique wrote:
>
>> Dear Prof P. Blaha
>>
>> Thank you for your answer
>> I did the calculation again but I had the same error but when I used
>> wien2k_14, the calculation ended without
ase.in2(c).
>
> On 05/15/2017 10:31 AM, karima Physique wrote:
>
>> Sorry but I work on a material of which it is diamagnetic and this is
>> already verified experimentally so I want an answer to my question
>>
>> 2017-05-15 8:57 GMT+02:00 Fecher, Gerhard <fec..
_________
> Von: Wien [wien-boun...@zeus.theochem.tuwien.ac.at] im Auftrag von karima
> Physique [physique.kar...@gmail.com]
> Gesendet: Montag, 15. Mai 2017 00:31
> An: A Mailing list for WIEN2k users
> Betreff: [Wien] Error with NMR calculation
>
> I launched the fo
I launched the following commands :
run_lapw
x_nmr -mode in1
x_nmr -metal
for NMR calculation of a diamagnetic material (metal)
And I got the following error;
EXECUTING: /home/Work/Wien2k/nmrc -case Dia -mode current-green
-scratch ./ -noco-metal
forrtl:
Thank you very much for you answers
Is there a difference between trace of magnetic susceptibility in the file
case.xim and :NMRXIM in the file case.outputnmr_integ because they have two
different values?
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;> force (very high field, very much k-points etc.)
>>>>> If a ferro- or other "magnetic" solution is close, then the
>>>>> application of the field may break the symmetry in such a way that
>>>>> you run into this state instead of staying in t
is that you have never actually known what the question is."
>>
>> ====
>> Dr. Gerhard H. Fecher
>> Institut of Inorganic and Analytical Chemistry
>> Johannes Gutenberg - University
>> 55099 Mainz
>> and
>> Max Planck Institute for
Gutenberg - University
> 55099 Mainz
> and
> Max Planck Institute for Chemical Physics of Solids
> 01187 Dresden
> ________
> Von: Wien [wien-boun...@zeus.theochem.tuwien.ac.at] im Auftrag von karima
> Physique [physique.kar...@gmail.com]
> Ge
Dear Wien2k users:
How I can know if the material is paramagnetic or diamagnetic with a
calculation.?
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quot;
>
> On Saturday 2017-04-22 02:38, karima Physique wrote:
>
> Date: Sat, 22 Apr 2017 02:38:36
>> From: karima Physique <physique.kar...@gmail.com>
>> Reply-To: A Mailing list for WIEN2k users <w...@zeus.theochem.tuwien.ac.
>> at>
>> To: A Mailing list
Dear wien2k users;
I had this error when executing the following command (x lapw2 -qtl -up -hf
-p -redklist) for calculating dos with hybrid funcional:
The error:
scp: /HFvectorup_1: No such file or directory
scp: /HFvectorup_2: No such file or directory
scp: /HFvectorup_3: No such file or
thank you very much
2017-04-21 23:00 GMT+02:00 <t...@theochem.tuwien.ac.at>:
> This is the value next to the last :FER in case.scf
>
> On Friday 2017-04-21 22:57, karima Physique wrote:
>
> Date: Fri, 21 Apr 2017 22:57:19
>> From: karima Physique <physi
Dear Wien2k users;
I calculated the band structure of a magnetic material with hybrid
functional and I want to know where I can find the value of Fermi level to
insert it in the file case.insp.
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Dear Wien2k users,
I want to calculate Ueff of a chalcopyrite material XFeY2 using G. K. H.
Madsen and P. Novak but I have 8 atoms of which (4 inequivalents) therefore
must I take 1 atom (2 equivalent atoms) or else I have to split the 4
inequivalent atoms into 8 atoms and I Take one only?
Dear Wien2k users,
I want to calculate Ueff of a chalcopyrite material XFeY2 using G. K. H.
Madsen and P. Novak but I have 8 atoms of which (4 inequivalents) therefore
must I take 1 atom (2 equivalent atoms) or else I have to split the 4
inequivalent atoms into 8 atoms and I Take one only?
Dear Wien2k users,
I want to calculate Ueff of a chalcopyrite material XFeY2 using G. K. H.
Madsen and P. Novak but I have 8 atoms of which (4 inequivalents) therefore
must I take 1 atom (2 equivalent atoms) or else I have to split the 4
inequivalent atoms into 8 atoms and I Take one only?
rchive.com/wien%40zeus.theochem.tuwien.
> ac.at/msg01700.html
> [12] http://www.mail-archive.com/wien%40zeus.theochem.tuwien.
> ac.at/msg08186.html
>
> On 3/27/2017 9:50 AM, karima Physique wrote:
>
> Thank you for your answer but i I noticed that Ueff is very sensitive with
> th
> Dr. Gerhard H. Fecher
> Institut of Inorganic and Analytical Chemistry
> Johannes Gutenberg - University
> 55099 Mainz
> and
> Max Planck Institute for Chemical Physics of Solids
> 01187 Dresden
> ________
nd
> Max Planck Institute for Chemical Physics of Solids
> 01187 Dresden
> ____
> Von: Wien [wien-boun...@zeus.theochem.tuwien.ac.at] im Auftrag von karima
> Physique [physique.kar...@gmail.com]
> Gesendet: Montag, 27. März 2017 02:09
> An: wien@z
Dear Wien2k users,
I used the method described by G. K. H. Madsen and P. Novak but I found two
different values of Ueff when I changed the number of K-point and RKmax
For K=1 Point and RKmax 5 i found Ueff=3.6 eV
but For K=100 Points and RKmax 8.5 i found Ueff=5.4 eV
Do I use one point only ?
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