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Dept of Chemistry,
Pohang Univ of Sci Tech
Pohang, Republic of Korea
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thanks Prof. Peter Blah
On Sun, Jul 29, 2012 at 1:16 PM, Peter Blaha
pblaha at theochem.tuwien.ac.at wrote:
IR and Raman means first: phonon calculations (Gamma only).
This can be done
either by creating the corresponding displacements by hand and also
setup/diagonalize the
dynamical
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Alpa Dashora
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First: If you are unexperienced in computing, why would you use mpi at all.
Try the k-point parallel version first.
.machines:
1:arya
1:arya
1:arya
no lapw0 line !!
Am 30.07.2012 08:58, schrieb alpa dashora:
Dear Wien2k Users, Mr. Abo and Prof. Blaha,
I have edited my .machines file
://zeus.theochem.tuwien.ac.at/pipermail/wien/attachments/20120730/3f9e44f5/attachment.htm
No. For large cells you have to learn how to configure and use mpi correctly.
Am 30.07.2012 09:21, schrieb alpa dashora:
Dear Prof. Blaha,
As per your suggestion, I am able to run the k-point parallel calculation.
But in case of large systems, about 100 atoms, can I use this technique (with
When you change ISPLIT by hand in case.struct, be sure to keep the numbers in
the correct column !
Alternative: Use the qtl program to generate case.qtl for the f-orbitals.
Am 28.07.2012 02:50, schrieb Jonathan Solomon:
To WIEN2k users and developers:
I would like to print QTLs for all
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I would not bother too much about B', but B is changing by 20 %, which is too
much.
You have to analyse your data to find out where your error is. Maybe in one set
of
calculations you have not got the optimized c/a ratio (and corresponding
energy) for
each volume ???
PS: 5 points are probably
,
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Yes, I can confirm that the missing real*8 in pimach is a bug, even when it
does not show up
in optimized compilations. One should insert
IMPLICIT REAL*8 (A-H,O-Z)
in function pimach (bottom of SRC_lapw0/fftpack_helpers.f file).
As L.Marks already pointed out, the kurki.f problem is not really
Dear WIEN2k users,
This is an update to let you know that a new version (v1.3.0 r149) of
the SKEAF extremal area code for extracting quantum oscillation
information from calculated Fermi surfaces has been released. The new
version contains several important improvements and bug fixes (see the
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