during installation?
- What does the error message file of nn say?
A recommendation: As a beginner use the w2web interface! It goes a long
way to help keeping the correct sequence of tasks, setting defaults and
so on.
Good luck
---
Dr. Martin Pieper
Karl-Franzens University
Institute of
Question is, is there anything wrong? Are these parts of ERROR messages
or at least WARNINGS, or are they just echoes, your job(s) telling you
what they are doing?
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380
there I am no epert and I dont know anything about
your server anyway.
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 21.07.2016 17:40, schrieb Jing Qun:
Thanks.
These are neither ERROR messages nor
consider SO because it changes energy
differences and might split degeneracies.
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 29.10.2016 23:20, schrieb Abderrahmane Reggad:
Hello again
I am waiting for
different. A drastic example: SO
interaction may lead to non-collinear helical spin structures - which
are outside the scope of standard Wien2k.
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 30.10.2016 14
differences. Are they
reasonable?
Good luck with the calculations,
Martin Pieper
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 31.10.2016 19:53, schrieb Abderrahmane Reggad:
Thank you Dr Pieper for the detailed
sgroup (or other scripts in the initialization) does'nt change the
positions of the atoms, it changes the basis used to describe the
positions. 'Optimization' is done with respect to internal forces, or
energy, both unknown at that step.
Good luck
Martin Pieper
---
Dr. Mar
re optimization in the user guide, and perhaps the
'Optimization Notes' of L. D. Marks that you will find on the Wien2k
website. I am completely unable to improve on those.
Best luck
Martin Pieper
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz
e ingredient and the
poor scf wanders helpless around, lost in a multidimensional world ...
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 13.11.2016 19:14, schrieb Abderrahman
as to
guess an Emax that will generate a band with a band minimum above E_F.
Why not have tetra choose Emax as the minimum of the Emax input in .int
and the highest Band-MAXIMUM?
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.:
0.
.
.
.
--
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 16.11.2016 07:41, schrieb Peter Blaha:
The DOS is calculated up to a value for which we can guarantee that
the DOS is correct and complete.
Of cours
0.29294 ATOM=1
L= 2
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 16.11.2016 16:06, schrieb Peter Blaha:
The question is: what does your scf2up/dn files (and the scf1up/dn
files say ?
I
. The same argument works
for Co, and to my knowledge for Fe, though its less accurate there, and
it breaks down for Mn. So maybe fcc-Fe and fcc-Ni are other examples - I
didn't try.
Thanks again,
Martin
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplat
High Komal,
please consult the LAPWDM sections in the user guide. There calculation
of the orbital moment is explained.
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
e the
cases where the tetra's and lapw1's automatic setting of Emax might have
difficulties.
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 21.11.2016 09:48, schrieb Lyudmila Dobysheva:
17.11.201
ground state that DFT is
concerned with.
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 26.11.2016 22:30, schrieb Abderrahmane Reggad:
Thank you Prof Blaha for your quick answer.
The Ni atom is 3d
entials arising from
U or hybrids are set to zero. Not strictly what happens in the material,
but a way to improve the model significantly and keep the calculation
viable.
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)31
e wants to model.
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 28.11.2016 08:33, schrieb Fecher, Gerhard:
I hope you agree that Pt is paramagnetic
I did two calculations for Pt, one was spin polarized
some additional potential with simply is not there in
your material. And using spheres you certainely cannot avoid some
intermediate space between them.
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am
& Mermin).
Or you can take it for granted that Wien2k does its very best to model
the electronic structure correctly - especially localized and itinerant
as limiting behavior. The more difficult (and interesting) possibilities
are in between.
---
Dr. Martin Pieper
Karl-Franzens Univer
that they are not!
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 03.01.2017 11:26, schrieb Abderrahmane Reggad:
Thank you Mr delamora for your reply
You have got
a 0.003Ry/Cr difference between Cr
/ supercells /
symmetries?
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 26.01.2017 19:17, schrieb venkatesh chandragiri:
Dear Prof. Lyudmila Dobysheva
Thanks for your reply
) U MUST produce a
gap. Here the real experts might provide more useful comments.
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 28.01.2017 01:21, schrieb venkatesh
u got the units in struct right)
and start the scf only when everything went ok.
... and keep fingers crossed
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 13.02.2017 09:18, schrieb Abhilash Patra:
Dear W
/listinfo/wien
SEARCH the MAILING-LIST at:
http://www.mail-archive.com/wien@zeus.theochem.tuwien.ac.at/index.html
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
___
Wien
stion then is to specify which states he
wants to give the honor of being part of team 'topmost layer' - then to
project on them.
And my best wishes for the most difficult part: convince his audience
that the choice is convincing for the point to be made. ;-)
Martin Pieper
Am 0
but different
configuration.
Martin Pieper
Am 09.05.2017 01:55, schrieb Dr. K. C. Bhamu:
Dear Wien2k Users
I am alloying a quaternery compound: replacing Cr with Br one by one.
What I see is, the pristine compound is cubic with 225 SG. When I
replace Cl by Br one by one then lattice
Pauli spin susceptibility (see your favorite
textbook on the theory magnetism), so it is by no means safe to simply
assume its small.
Greetings,
Martin Pieper
Am 08.05.2017 20:19, schrieb Peter Blaha:
In an insulator/semiconductor you have only the orbital part of the
susceptibility. This can
mport numpy # math library
This probably will not work as shown here for my terminal, meaning that
numpy is either not installed, or in some unexpected place and you will
have to point python to that place. You will have to look into what you
did to install numpy (or a module including it,
ructural relaxations, look what changes in your (GGA-) calculations,
and keep fingers crossed that things you are interested in converge for
supercells of a size you still can handle.
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.:
.
So the general advise seems to be stiduy the UG - and if possible some
of the references therein.
Good luck
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 08.07.2017 17:08, schrieb Peng Bingrui
). If all option boxes are
left untouched it uses the last possibility in the list (I forgot which
one that is). save_lapw from the terminal works just fine.
Best regards,
Martin Pieper
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
effects of a magnetic
field.
ad 2) If you apply a magnetic field experimentally in the lab you do it
at all atoms. I suppose you want to model that situation. imho it makes
little sense to exempt one or two of your atoms from the field.
Good luck
---
Dr. Martin Pieper
Karl-Franzens University
t has no -orb and -dm switches.
I suggest you use the w2web interface and the examples in the UG to make
yourself more familiar with the package ...
Good luck
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
ot a specialized treatment
of magnetism. Personally I like the introduction to Solid State Physics
by Ashcroft and Mermin.
Good luck
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 19.07.2017 16:02, schrieb kari
r, the susceptibility
is about how the applied field couples the ground state determined by
DFT to any low lying excited states - and especially in magnetically
ordered systems these excited states might well be beyond the scope of
DFT.
---
Dr. Martin Pieper
Karl-Franzens Univer
get per Tesla field.
If you want/need anything more elaborate you will have to provide more
information on what kind of measurement in what kind of ferromagnetic
metal or semiconductor you actually are interested in (and/or read
Ashcroft & Mermin).
---
Dr. Martin Pieper
Karl-Fran
.
So, how did you determine the gap in the table? Did you plot a DOS? Is
this really an insulator, or are there in fact bands crossing E_F? You
might severly misjudge the (direct?) gap depending on where in k-space
it is and the points in your k-list.
Good luck
---
Dr. Martin Pieper
Karl-Fran
Of course! The local moments in an AF insulator can be anything. I just
saw that there is only one type of magnetic atom in the unit cell (Ir)
and did not think properly. Sorry for that one.
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 22.08.2017 12:19, schrieb Abderrahmane Reggad:
Dear wien users
I want to simulate the NiO compound in its ionic state. We know that
the Ni and O atoms hav
ESULT. The
simulation of any property one wishes to study can proceed from there.
And if the electron density of NiO does not really resemble the ionic
picture, why use the ionic model to simulate things?
Best regards,
Martin
---
Dr. Martin Pieper
Karl-Franzens University
Institute
at it says so through ETOT. ;-)
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 23.08.2017 11:16, schrieb Fecher, Gerhard:
Funny discussion,
I wonder wether iron (Z=26) knows th
n his/her
free time.
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 24.08.2017 02:23, schrieb Abderrahmane Reggad:
Thank you for all for the rich discussion
If I introduce th
e enough. There are
more complicated cases where you may have to guide the scf to the
correct symmetry by populating the density matrices accordingly - this
has been discussed in the mailing list a lot - see also option -orbc in
the UG.
Good luck
Martin Pieper
---
Dr. Martin Pieper
Karl-Fran
matrix of
the problematic orbitals by hand and let the scf cycle dig itself in in
that state by using the option -orbc. This also has been explained in
posts in this mailing list before - perhaps most detailed by prof. Tran.
Good luck with your calculations
---
Dr. Martin Pieper
Karl-Franzens Unive
w and rule of physics
is valid only within some domain more or less clearly defined by such
assumptions.
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 05.09.2017 07:45, schrieb Fecher, Gerhard:
ic field (which they - and you - don't calculate). Not a bad idea,
as far as I am concerned.
And they do give details on VS in section 3.1 - in fact, a lot more
details than you give us here about your calculations.
Best regards
---
Dr. Martin Pieper
Karl-Franzens University
Institute of
onvince us, but keep it in mind for fights
with the referees of a publication on this.
Good luck with your calculations
Martin Pieper
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 07.09.2017 00:26,
xperiment.
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 07.09.2017 11:02, schrieb E.A.Moore:
I have been following this thread and I think there is some confusion.
1. On th
echer found instead of your practically zero 0.05 mu_B? You will have
to follow his suggestions about the initial state!
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 09.09.2017 02:08, schrieb Abderra
forwarded us? Any comments on the magnetic
moment Prof. Fecher told us about?
Did you follow his advice?
Did you even read it?
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 11.09.2017 15:55, schrieb
nn labels are printed (perhaps HFF's are only
calculated?) to case.scf only during the finalizing iterations. This
makes the number of iterations larger than the number of HFFnnn values.
Maybe the module filling in the plot arrays is confused by this.
Best regards,
Martin Pieper
--
Dr. Martin Pi
to MMI's would be ok with me. Or, if you are interested, I can mail the
few python lines I use to read plot arrays for gnuplot from case.scf
files. Perl certainely can do something very similar.
Best regards,
Martin Pieper
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Ph
dline .= " -eels" if ($u);
No recompile necessary.
As I said before, I am no good around perl, so don't ask me why this
works, i.e. where $p becomes true. I don't think the browser is to
blame, since I had the misbehaviour with Firefox, Opera, and Konqueror
(KDE's own bro
s what the INSTALL file of libxc seems to say (and what
worked with me, but I am using gfortran).
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 21.09.2017 11:41, schrieb nov
hat I am unaware of?
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
___
Wien mailing list
Wien@zeus.theochem.tuwien.ac.at
Thanks a lot for the explanation. So, since my main interest is magnetic
materials moments on outer shells polarizing core s-electrons will
remain problematic ... (sigh)
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316
Hi Karima,
see e.g.
http://www.ieeemagnetics.org/index.php?option=com_content&view=article&id=118&Itemid=107
Best regards,
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 22.09.2017 15
It's as simple as you guessed, you have to convert between a molar
(number) density and a mass density:
(emu/mol) = (emu/mol)*1 = (emu/mol)*(g/g) = (emu/g)*(g/mol)
Best regards
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austri
. From there you should be able to convert to cgs and be
able to tell us what exactly the typo is ...
Best regards,
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 23.09.2017 23:55, schrieb karima Physique
on between electron
spin and field. Wether or not the electrons are localized doesn't
matter. An example might be the large spin susceptibility of
antiferromagnetic insulators.
Best regards,
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 G
4 etc.).
I hope one of the two works in your case as well
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 20.10.2017 10:25, schrieb mohamed mahdi:
i m trying to performe a calculation for ErCo4.5
ell (double the cell along basis directions ...) are sufficient.
There is no guarantee for this to be the case. You may have to work out
the fitting new shape and the positions of the atoms in the new unit
cell using additional tools.
I hope this helps,
Martin Pieper
---
Dr. Martin Pieper
Karl
again and
decide if you really want these neighbors being antiparallel, or if it's
the neighbours at some other distance.
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
along the (1,1,1) direction. Is there a 3-fold
symmetry?
I hope this helps,
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 25.10.2017 22:39, schrieb Abderrahmane Reggad:
Hello again
Here is the 3
(n_i*Z_i).
The concentration is c=N/V.
And yes, volume V as well as total number of electrons N are printed in
Wien2k's result file ...
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 01.11.2017
(the number of valence electrons, like file case.in2)
Or view case.scf in your favorite editor and search for 'UNIT CELL',
'NUCLEAR', 'VALENCE', or labels likes ':VOL', ':NOE', ':NEC', ... See
the UG for a list and an explanation
d in that package.
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 12.11.2017 23:46, schrieb delamora:
Thank you, but I think that the usersguide should have a minimal
explanat
Hamiltonian for magnetic field and quadrupole interaction.
Best regards,
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 22.11.2017 13:33, schrieb Peter Blaha:
This is a question to NMR-experimentalists
trons with Wien2k' by Elias
Assmann Wien, workshop 2013, ldau.pdf among the documentations on the
Wien2k site
[2] G. K. H. Madsen and P. Novák, Europhys. Lett. 69, 777 (2005)
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.:
case directory and restart there by modifying your
file case.struct - perhaps using programs like structgen and supercell.
Good luck
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 30.11.2017 06:12, schrieb
ct structure you are interested in,
each in fresh case directory.
---
Dr. Martin Pieper
Karl-Franzens University
Institute of Physics
Universitätsplatz 5
A-8010 Graz
Austria
Tel.: +43-(0)316-380-8564
Am 30.11.2017 20:27, schrieb chin Sabsu:
Dear Pieper Sir,
Thank you for detailed reply.
Ok
(see user guide)
...
I hope this helps. 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 18.09.2018 12:34, schrieb sandeep Kumar:
Dear Prof. Peter Blaha and WIEN2k Users,
I am
differences you observed.
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 10.10.2018 09:53, schrieb 李艳丽:
Hello,
I carried out the calculations with the external magnetic field
There is little information on what you did - my guess is a problem with
gnuplot ... is it installed?
Martin Pieper
On Mon, 5 Dec 2011 10:39:53 +0800, bakhtiar ul Haq
wrote:
> Hi Dear Wien usres!
> I am running wien version 2011 on Fedora 15. The purpose of my
calculations
> is t
++
--
++
--
vacuum spacer
chmiesorption layer
++
--
++
--
.
.
.
could easily be the result of a supercell construction - and it would NOT
be compatible with an overall AFM solution.
Best regards,
Martin Pieper
On Tue, 24 Jan 2012 21:00:58 -0600, Jianguang Wang
wrote
spin densities and HFF in case.scf? I assume they are they ok?
Or, if not, how do I get the correct values?
Best regards,
Martin Pieper
--
Dr. Martin Pieper
Karl-Franzens University
Experimentalphysik
Universit?tsplatz 5
A-8010 Graz
Austria
Tel. +43-1-58801-13132
+43-316-380-8564
ging Makefile in SRC_supercell
> changing Makefile in SRC_symmetry
> changing Makefile in SRC_symmetso
> changing Makefile in SRC_telnes3
> No Makefile.orig in SRC_templates, leaving directory.
> changing Makefile in SRC_tetra
> changing Makefile in SRC_trig
> changing Makefile in SRC_txspec
> No Makefile.orig in SRC_usersguide_html, leaving directory.
> changing Makefile in SRC_vecpratt
> No Makefile.orig in SRC_w2web, leaving directory.
>
> Press RETURN to continue
--
Dr. Martin Pieper
Karl-Franzens University
Experimentalphysik
Universitätsplatz 5
A-8010 Graz
Austria
Tel. +43-316-380-8564
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u generate case.indm? Since your case is magnetic you most probably
need case.indmc!
Do you use w2web? Did you switch on orb and dm there?
And finally: Does your ferrite structure REALLY contain 11 inequivalent Fe
atoms?
Best regards,
Martin Pieper
On Tue, 29 Jan 2013 09:46:02 -0600, Jihoon Park
wro
ochem.tuwien.ac.at
> http://zeus.theochem.tuwien.ac.at/mailman/listinfo/wien
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cessful run?
I am a little suspicious about you mentioning 'lapw2c': Is this a complex
case (magnetic or without inversion)?
Best luck,
Martin Pieper
On Thu, 18 Apr 2013 23:51:18 +0800, Muhammad Sajjad
wrote:
> Respected members
>
> Sorry, some text was missing in the first
knowledge. You only could do a (collinear!) fixed spin
moment calculation (see FSM calculation in the UG), which is WITHOUT
spin-orbit, and see what happens in an SCF with spin-orbit from there.
Best regards,
Martin Pieper
On Thu, 18 Apr 2013 14:53:27 +0530, "Ghosh SUDDHASATTWA"
wro
rors? With 4GB
on core i5 you may run into memory limits with a magnetic "transition metal
doped CdTe for 25 percent doping concentration" (see UG installation
section for memory requirements).
Best luck,
Martin Pieper
On Fri, 19 Apr 2013 12:49:06 +0800, Muhammad Sajjad
wrote:
> De
omehow the case directory got messed up. In such
a case I tend to
-create a new case,
- copy only the old .struct file into the corresponding directory
- rename this struct file to the new case name
- look with structgen if that went ok
- run the initialization and the SCF
Best luck
Martin Pieper
A
Hello, Vishal Jain,
Gavin is right, the Warnings should disappear if you accept to use the
new case_nn.struct generated by nn. Do sgroup after accepting to replace
case.struct by case_nn.struct. This will find the new space group and
symmetries (you broke some symmetries by removing the atom).
tural relaxation (if it fits in your
computer), etc. pp.
... and keep fingers crossed
Martin Pieper
Am 31.05.2013 22:20, schrieb Alex Animalu:
Dear Prof. Laurence,
Yes. Pt3 has 50% occupancy. Please, guide me on how to get the
structure file correctly.
Thanks for your help.
FROM: Laurence Mark
specific questions.
Regards,
Martin Pieper
Am 04.07.2013 14:52, schrieb Mamta Chauhan:
Dear Wien2k users,
I want to apply hubbard U correction in my calculations. Please help
me and suggest me to apply hubbard u correction.
Thanks and regards,
mamta
find
the line by line format of case.inorb (subsection 7.2.3), where you see
that especially lines 1, 3ff and 5ff are the answer to this problem.
Don't forget to adapt case.indm!
Good luck
Martin Pieper
Am 08.07.2013 08:53, schrieb Rocquefelte:
Could you clarify your question
magneton in 60 T
field in Ry units). Do you see an effect in, say, the local Ce-moment?
(grep :MMI *.scf)
Best regards
Martin Pieper
Am 10.07.2013 15:54, schrieb majid yazdani:
Dear WIEN2k authors and users
I’m trying to calculate the effect of the external magnetic filed on
the electronic
or DFT calculations? Materials
with a field induced magnetic transition?
Good luck
Martin Pieper
Am 10.07.2013 19:12, schrieb majid yazdani:
Dears Prof. Blaha and Martin Pieper
Thanks for your reply
I use the unit cell for my calculations. Is this similar to the
electric field?
When I grep the MMT
Dear Wasim,
I am far from being an expert, but when you call supercell you shift all
atoms a full 2 unit cells in (111) direction. Why? I never tried but
maybe nn has difficulties with that.
Best regards,
Martin Pieper
Am 15.07.2013 08:55, schrieb wasim raja Mondal:
Dear wien2k experts
presenting the template since it seems that
the script misses it in complex cases)
11) scf-cycle, spin-pol, k-parallel, so, dm, orb: crash in lapwso with
.dayfile:
Calculating fccniso in /home/pieper/WIEN2k/Fccni/fccniso
on tschucktschuck with PID 19259
start (Fr 5. M??r 14:39:08 CET 2010)
On Mon, 8 Mar 2010 19:49:31 -0600, Vladimir Michaelis
wrote:
> Hello,
>
>I have a paramagnetic unit cell with a Re with an electron spin of 1
>and three other non-paramagnetic ions. I have built a supercell and
>have run these calculations a few times using various number of
kpoints,
if 4 parameters per atom given"
>
>
>
>
>
> Suddhasattwa
--
Dr. Martin Pieper
Karl-Franzens University
Experimentalphysik
Universit?tsplatz 5
A-8010 Graz
Austria
Tel. +43-1-58801-13132
+43-316-380-8564
A late contribution to a closed case:
If the SDW is not a linear polarized wave but a helical one (I don't know
for Cr) you will, to my knowledge, also be unable to model it exactly using
the standard version of Wien2k, which only knows colinear spin structures.
Best regards,
Martin Piepe
Dear Irina,
I myself never really tried to calculate the MAE, so take this with a
grain of salt and take replies of people with real experience more serious
than this:
is in the SCF files. So I
>> analysed SCF-files and I saw that total Energy almost the same as one
>> in my previous calculations without external field.
>>
>> I'll be very pleased if anyone would tell me, what was wrong in my
>> actions.
>>
>> Best regards,
&
ourse, particularly important for spin-1/2 systems like
Cu2+ where the single-ion anisotropy vanishes.
Best regards,
Martin
--
Dr. Martin Pieper
Karl-Franzens University
Experimentalphysik
Universit?tsplatz 5
A-8010 Graz
Austria
Tel. +43-1-58801-13132
+43-316-380-8564
g this command I am getting the error
> stop error: the required input file case.indmc for the next step
> could
> not be found
>please give suggestion in this regards
> --
--
Dr. Martin Pieper
Karl-Franzens University
Experimentalphysik
Universit?tspl
ameters
> just help/allow the convergence, or do they change the resulting
> converged band structure.
>
> Regards,
> Lukasz
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