[Wien] Comparing Total Energies

2012-07-11 Thread David Tompsett
Dear Fabien,

Thanks for the response. It is probably my k-mesh that is making it
inaccurate to compare.

David.

On Tue, Jul 10, 2012 at 3:48 PM, tran at theochem.tuwien.ac.at wrote:

 Hi,

 When comparing two total energies obtained from different unit cells, one
 has to be always very careful.

 First, if you did the calculation on the
 small unit cell with a k-mesh (n1,n2,n3), then the calculation on the
 large unit cell should be done with the corresponding k-mesh
 (n1/m1,n2/m2,n3/m3), where m1, m2, and m3 indicate by how many times
 (along the lattice vectors a, b and c) is the large unit cell larger than
 the small one. You can have problems if If n1/m1, n2/m2 or n3/m3 is not
 an integer. But this not a problem if you
 are using very good k-meshes such that the energies are well converged.

 It can also happen that the orientation of the lattice vectors are
 completely different in the small and large unit cells. In this case
 some numerical noise (e.g., from the FFTs) can introduce some errors.

 But actually, what do you mean by I can't compare?

 My recommendation: use the same unit cell.

 F. Tran

 On Tue, 10 Jul 2012, David Tompsett wrote:

  Dear All,
 
  I have what is probably a very basic question about comparing total
  energies. I have been considering a system that undergoes a charge
 density
  wave transition from a high to low symmetry structure. I have been
  comparing the total energy of the high and low symmetry structures. The
  unit cell of the high symmetry structure has half as many atoms as does
 the
  low symmetry one.
 
  In my calculations it seems I can't compare 2x(total energy of high
  symmetry cell) with 1x(total energy of low symmetry cell). Instead I have
  to perform the high symmetry calculation in the same size unit cell and
  symmetry as for the low symmetry. Why is this the case? What is the
 effect
  of having different sized unit cells?
 
  Thank you,
  David Tompsett.
 
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[Wien] Comparing Total Energies

2012-07-10 Thread David Tompsett
Dear All,

I have what is probably a very basic question about comparing total
energies. I have been considering a system that undergoes a charge density
wave transition from a high to low symmetry structure. I have been
comparing the total energy of the high and low symmetry structures. The
unit cell of the high symmetry structure has half as many atoms as does the
low symmetry one.

In my calculations it seems I can't compare 2x(total energy of high
symmetry cell) with 1x(total energy of low symmetry cell). Instead I have
to perform the high symmetry calculation in the same size unit cell and
symmetry as for the low symmetry. Why is this the case? What is the effect
of having different sized unit cells?

Thank you,
David Tompsett.
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[Wien] How to make Root3xRoot3 supercell

2012-06-30 Thread David Tompsett
VESTA (http://jp-minerals.org/vesta/en/) also has good utilities for
letting you redefine the unit cell vectors via a matrix transformation.

David.

On Sat, Jun 30, 2012 at 5:59 AM, Laurence Marks L-marks at 
northwestern.eduwrote:

 Try cryscon (http://www.shapesoftware.com), perhaps also crystalmaker
 or similar.

 On Fri, Jun 29, 2012 at 3:41 PM, H M Sohail sohail.ifm at gmail.com wrote:
  Simple Question:
 
  How to make Root3xRoot3 supercell, since it only excepts integers..
 
  Ge(111)1x1 to Ge(111)R3xR3 is required..
 
  Help is required..
 
  Regards
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 Department of Materials Science and Engineering
 Northwestern University
 www.numis.northwestern.edu 1-847-491-3996
 Research is to see what everybody else has seen, and to think what
 nobody else has thought
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[Wien] Strange results lapwdm

2012-06-07 Thread David Tompsett
Hi Peter,

Thanks for the response. The option r-index = 11 is not in the UG, but is
documented in Pavel Novak's technical report on the Hyperfine Field
calculation so other users may strike it in future.

Hopefully he will have some input.

Thanks,
David.

On Thu, Jun 7, 2012 at 7:47 AM, Peter Blaha pblaha at 
theochem.tuwien.ac.atwrote:

 You have to check directly in the code. Without looking in the code I do
 not know what r-index = 11  should do ? I guess this is not a documented
 option, but Pavel Novak migth have put in something 

 Am 06.06.2012 14:11, schrieb David Tompsett:

 Dear All,

 I have been attempting to use lapwdm to obtain the expectation value of
 the radial distribution of orbitals i.e. r.

 I have attempted the simplest case that I could think of, the hydrogen
 atom in a large cell. I used an RMT of 4.5 au so that a fraction 0.99 of
 the charge lies inside the muffin tin. Then after converged SCF cycles I
 ran x lapwdm -up with input:

 -9. Emin cutoff energy
 1   number of atoms for which density matrix is calculated
 1 1 0  index of 1st atom, number of L?s, L1
 11 1   r-index, (l,s)-index

  From the solution of the Schroedinger equation for a Hydrogen atom, the
 result should be r = 1.5 au.
 However the result from :XOP in the output of lapwdm is 104670.12. I do
 not know what the units are. Also, the value of this result seems to
 vary strongly with the RMT.

 Can anyone help me understand this behaviour or if there is a problem
 with lapwdm? I looked through the source code, but could not follow it.

 Many thanks,
 David.


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 Getreidemarkt 9
 A-1060 Vienna
 Austria
 +43-1-5880115671
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[Wien] Strange results lapwdm

2012-06-07 Thread David Tompsett
Hi Gavin,

That is a good idea, with RINDEX= -11 we obtain:
WEIGHTS READ
 Calculation of X, X=1/r**1
  atom   Lup  dn total
  product Usym*Coupl after densmat
 0.98974
 Density matrix, imag part
 0.0

:XOP  1  0 0.98974 0.0 0.98974

This looks healthier, the answer should formally be 1/r_0 if we neglect
relativistic effects.

So perhaps the problem is just for krad  10?

Many thanks,
David.

On Thu, Jun 7, 2012 at 2:53 PM, Gavin Abo gsabo at crimson.ua.edu wrote:

  May or may not help:

 RINDEX = 11 = r**krad for krad  10 = :XOP 104670.12 (large number)

 Adding a negative sign will change the calculation:

 RINDEX = -11 = 1/r**krad for krad  10 = :XOP ? (small number)

 File of reference: $WIENROOT/SRC_lapwdm/radint.f


 On 6/7/2012 7:08 AM, David Tompsett wrote:

 Hi Peter,

 Thanks for the response. The option r-index = 11 is not in the UG, but is
 documented in Pavel Novak's technical report on the Hyperfine Field
 calculation so other users may strike it in future.

 Hopefully he will have some input.

 Thanks,
 David.

 On Thu, Jun 7, 2012 at 7:47 AM, Peter Blaha pblaha at 
 theochem.tuwien.ac.atwrote:

 You have to check directly in the code. Without looking in the code I do
 not know what r-index = 11  should do ? I guess this is not a documented
 option, but Pavel Novak migth have put in something 

 Am 06.06.2012 14:11, schrieb David Tompsett:

  Dear All,

 I have been attempting to use lapwdm to obtain the expectation value of
 the radial distribution of orbitals i.e. r.

 I have attempted the simplest case that I could think of, the hydrogen
 atom in a large cell. I used an RMT of 4.5 au so that a fraction 0.99 of
 the charge lies inside the muffin tin. Then after converged SCF cycles I
 ran x lapwdm -up with input:

 -9. Emin cutoff energy
 1   number of atoms for which density matrix is calculated
 1 1 0  index of 1st atom, number of L?s, L1
 11 1   r-index, (l,s)-index

  From the solution of the Schroedinger equation for a Hydrogen atom, the
 result should be r = 1.5 au.
 However the result from :XOP in the output of lapwdm is 104670.12. I do
 not know what the units are. Also, the value of this result seems to
 vary strongly with the RMT.

 Can anyone help me understand this behaviour or if there is a problem
 with lapwdm? I looked through the source code, but could not follow it.

 Many thanks,
 David.


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 Wien at zeus.theochem.tuwien.ac.at
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 --
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 Inst.Materials Chemistry
 TU Vienna
 Getreidemarkt 9
 A-1060 Vienna
 Austria
 +43-1-5880115671
 ___
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[Wien] Strange results lapwdm

2012-06-06 Thread David Tompsett
Dear All,

I have been attempting to use lapwdm to obtain the expectation value of the
radial distribution of orbitals i.e. r.

I have attempted the simplest case that I could think of, the hydrogen atom
in a large cell. I used an RMT of 4.5 au so that a fraction 0.99 of the
charge lies inside the muffin tin. Then after converged SCF cycles I ran x
lapwdm -up with input:

-9. Emin cutoff energy
1   number of atoms for which density matrix is calculated
1 1 0  index of 1st atom, number of L?s, L1
11 1   r-index, (l,s)-index


[Wien] Radial expectation lapwdm

2012-05-30 Thread David Tompsett
Dear All,

I need a little help with the program lapwdm.

I am trying to quantify the radial extent of d-orbitals of manganese ions.
I wanted to use the expectation value r calculated by lapwdm using
RINDEX=11, LSINDEX=1.

I am not using SO-coupling and am using the latest release of Wien2k.

A few questions:
1) Is RINDEX=11, LSINDEX=1 the correct setting?
2) For spin up I have :XOP  1  2   360.97696 0.0   360.97696
For spin dn I have :XOP  1  2   166.01005 0.0   166.01005
a)   What units is r in?
b)  Also,  should I divide these numbers by the occupation n_s for each
spin to get the expectation?
c)   Even after dividing by the occupations, the values for spin up and
spin down are quite different by nearly a factor of three. Seems strange to
me, am I comparing the right things?
3) Is it possible to calculate the expectations for particular l,m for
instance for just t_2g orbitals?

Many thanks,
David.
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[Wien] Questions on the quantitative understanding of DOS and partial DOS

2012-03-22 Thread David Tompsett
Dear Balamurugan,

Some answers below and many previous postings:

On Thu, Mar 22, 2012 at 4:24 PM, J. K. Balamurugan
albertbalagan at gmail.comwrote:

 Dear WIEN2k developers and users,

 I have some problem in quantitative understanding the DOS and partial DOS
 plots/data. I post the question with a case assumption of room temperature
 (RT) structure of BaTiO3. As it is well known BaTiO3 has tetragonal
 structure at RT. Now, Ba and Ti has one site and O has two sites. If the
 DOS  partial DOS are calculated for BaTiO3, I will get total DOS for the
 unit cell which contains one formula unit of BaTiO3. I will also get
 partial DOS of Ba, Ti and O1 and O2 (in terms of total and from individual
 orbital contribution like s, p and d whichever are applicable.) Here are my
 questions:

 1. Will the sum of total DOS individual atoms [i.e., total DOS of (Ba + Ti
 + O1 + O2)] be exactly equal to total DOS of the unit cell? If the answer
 is No, why?

No, the interstitial states contribution is missing. Only the area inside
the muffin tin is included in the partial DOS.


 2. Will the total DOS of any specific atom, say Ti, will be exactly equal
 to the sum of orbital contributions [i.e., partial DOS of (Ti-s + Ti-p +
 Ti-d)]?  If the answer is No, why?

Yes, but I think even further depending on how many l-values are in the
basis set.


 Another related question: Let us assume a hypothetical structure where in
 I have two formula units of BaTiO3 in a unit cell. That is the unit cell
 has Ba2Ti2O6. Now the question is the following:
 3. Should I need to multiply 2 to the total DOS of individual atoms {i.e.,
 2*[total DOS of (Ba + Ti + O1 + O2)]} to get the total DOS of the unit cell
 with two formula unit? Will this sum be exactly equal to the actual total
 DOS of the unit cell which we get as it is from the calculations?

Yes. Then no not total DOS of cell, see point 1.


 Please explain me to clear these my questions. I wish also to get into
 reading any material/user guide/article/document which could help me to
 have a complete understanding on this issue.

 Thanks.

 With kind regards,
 K. Balamurugan.


 David Tompsett.



 --
 *K. Balamurugan
 Pittsburgh, USA.
 +1 412 961 5055*

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[Wien] B_lat hyperfine field NMR

2012-03-01 Thread David Tompsett
Dear All,

Has anyone implemented a way to calculate the hyperfine field due to
dipolar interactions between the nuclear spin and the electron spin density
outside the muffin tin sphere? This is referred to as B_lat in Pavel
Novak's notes on hyperfine calculations in Wien2k.

Many thanks,
David Tompsett.
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[Wien] Suggestion for LOPW error

2012-02-09 Thread David Tompsett
Dear All,

There have been several discussions over the past year regarding errors of
LOPW plane waves exhausted in high symmetry cells. I have recently come
across the same problems in a cubic (space group 212) cell. I could only
avoid them by taking RKmax up to 9.5. This however, seems to be nearing the
point of overcompleteness in the basis set?


[Wien] Installation question

2012-01-30 Thread David Tompsett
Dear All,

I have recently attempted to recompile Wien2k version 11 and am having some
problems with the MPI parallel binary lapw1_mpi. I used a GNU reference
implementation of Scalapack and libsci. Unfortunately my cluster does not
have inter libraries.

The compile completes with no errors, but upon running lapw1_mpi does not
print any eigenvalues, yet throws no errors:
EIGENVALUES ARE:

0 EIGENVALUES BELOW THE ENERGY  -10.0
   

There is simply nothing printed in case.output1up or case.energyup where
the eigenvalues should be. Has anyone seen such a problem before? Also,
which part of the source code should print these eigenvalues? I would like
to check if the problem is with IO by trying to flush the stream.

Many thanks,
David Tompsett.
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[Wien] Calculation for Heavy atom

2011-11-07 Thread David Tompsett
Dear All,

Is it possible to perform a calculation in Wien2k for the charge density of
a very heavy atom eg. #116 or 120? Also, would the answers be sensible?

Eg. for #116 I tried this case.inst:

Up
Rn 5
5, 3,3.0  N
5, 3,3.0  N
5,-4,4.0  N
5,-4,4.0  N
6, 2,1.0  N
6, 2,0.0  N
7,-1,1.0  N
7,-1,1.0  N
7, 1,1.0  N
7, 1,1.0  N

 END of input (instgen_lapw)

And case.struct
Title
P   LATTICE,NONEQUIV.ATOMS:  1
MODE OF CALC=RELA unit=ang
 18.897269 18.897269 18.897269 90.00 90.00 90.00
ATOM   1: X=0. Y=0. Z=0.
  MULT= 1  ISPLIT= 2
Up NPT=  781  R0=0.0100 RMT=3.5000   Z:116.0
LOCAL ROT MATRIX:1.000 0.000 0.000
 0.000 1.000 0.000
 0.000 0.000 1.000

But I receive errors after trying to run lstart:
error: Elemant120.inst not consistent with Z
edit Elemant120.inst and rerun lstart afterwards or change Z in StructGen!

If I try to put 5g states into case.inst (for element #120) lstart stops
with a format error.

Thank you,
David Tompsett.
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[Wien] Magnetic order with hybrids and DFT+U

2011-10-05 Thread David Tompsett
Dear All,

I am considering calculations of magnetic order in transition metal anion
compounds. Is anyone aware of cases where DFT+U predicts the wrong magnetic
order compared to experiment, but where hybrids predict correctly?

Thank you,
David Tompsett.
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[Wien] Forces using Tetra

2011-07-28 Thread David Tompsett
Dear All,

I have a question about the forces obtained when using TETRA in metallic
systems. I read in the 1994 Blochl paper that the Blochl Tetra method is not
variational with respect to partial occupancies. Does this mean that the
total energy from Tetra is not smoothly variational wrt. to partial
occupancies?

Therefore, can I trust the calculated forces in a metallic system?

Can I use the total energy from Tetra for metals reliably?

Many thanks for any help,
David Tompsett.
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[Wien] Forces using Tetra

2011-07-28 Thread David Tompsett
Hi Laurence,

Is there any explanation or reference as to why they are OK? The Bloch paper
suggests that they won't be.

Cheers,
David.

2011/7/28 Laurence Marks L-marks at northwestern.edu

 The forces are fine.
 On Jul 28, 2011 4:55 AM, David Tompsett dat36 at cam.ac.uk wrote:
  Dear All,
 
  I have a question about the forces obtained when using TETRA in metallic
  systems. I read in the 1994 Blochl paper that the Blochl Tetra method is
 not
  variational with respect to partial occupancies. Does this mean that the
  total energy from Tetra is not smoothly variational wrt. to partial
  occupancies?
 
  Therefore, can I trust the calculated forces in a metallic system?
 
  Can I use the total energy from Tetra for metals reliably?
 
  Many thanks for any help,
  David Tompsett.

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[Wien] Stress

2011-07-22 Thread David Tompsett
Dear All,

Has anyone ever tried to implement the calculation of the stress tensor into
Wien? Is there something in the method that prevents its calculation?

I read the Nielsen PRB 32, 3780 (1985) where stress calculation is described
for local functionals. There are 5 contributions in equation 30 of that
paper. Is any in particular difficult for LAPW methods?

Many thanks,
David Tompsett.
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[Wien] Treating d and f states of Eu using SIC

2011-07-19 Thread David Tompsett
Dear Alay,

DFT+U is more than just a SIC correction method. It corrects some
self-interaction, but also incorporates Hartree-Fock effects via a Coulomb
matrix. See PHYSICAL REVIEW B 79, 035103 (2009).

To tread both d and f electrons try:
EuTe.inorb
1 1 0nmod, natorb, ipr
PRATT,1.0  mixmod, amix
1 2 2  3  iatom nlorb, lorb   # treating d electrons with Ueff =
0.5000, How to treat f electrons as well?
1  nsic (LDA+U(SIC) used)
0.500 0.0 U J
0.500 0.0 U J

Cheers,
David.

2011/7/19 Muhammad Alay-e-Abbas alayabbas at googlemail.com

 Dear All,

 I am running wien version 11.1 on a Core 2 duo Laptop with
 Fedora 8 operating system, ifort compiler and mkl math libraries. The
 purpose of my calculations is to get band structures of Eu chalcogenides. I
 want to treat both d and f electrons of Eu atom with the additional U
 potential using the SIC approach.
 How shall i modify the case.inorb file if Eu is atom number 1 in the
 following?

 EuTe.inorb
 1 1 0nmod, natorb, ipr
 PRATT,1.0  mixmod, amix
 1 1 2iatom nlorb, lorb   # treating d electrons with Ueff =
 0.5000, How to treat f electrons as well?
 1  nsic (LDA+U(SIC) used)
 0.500 0.0 U J
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[Wien] how to find Stoner parameter using wien2k

2011-07-07 Thread David Tompsett
Hi Shamik,

Sayed's advice is good. There are also some procedures based on Fixed spin
moment calculations. You will have to think carefully about whether your
system is metallic or locaised type. The links in the appendix to this paper
should help:

Ylvisaker and Pickett, PHYSICAL REVIEW B 79, 035103 2009

Best,
David.

2011/7/6 Seyed Javad Hashemifar hashemifar at cc.iut.ac.ir

 I have no experience on calculation of stoner parameter and interesting to
 learn it. However, by doing a simple spin polarized calculations with
 nonzero and parallel initial moments on your system, you may easily find
 whether your system prefers ferromagnetism or not. The initial magnetic
 moments are controlled in case.inst file.
 SJ Hashemifar
 ==
 Seyed Javad  Hashemifar
 Physics Department, Isfahan University of Technology
 84156-83111 Isfahan, Iran
 Tel: +98 311 391 2375 Fax:+98 311 3912376
 Email:  hashemifar at cc.iut.ac.ir
 Homepage:  http://hashemifar.iut.ac.ir
 ---


 2011/7/6 Shamik Chakrabarti shamikiitkgp at gmail.com


 Dear wien2k users,

 According to the Stoner band theory of magnetism, one can able to predict
 the magnetic ground state of the material as it is paramagnetic or
 ferromagnetic using product of the non magnetic density of states around the
 Fermi level (N(E)) and the Stoner parameter (I). As given in some of the
 literature, the Stoner parameter  can be described as the exchange integral
 and it could be found using LSDA and LMTO methods. see the fallowing
 literature...

 1. http://prb.aps.org/pdf/PRB/v16/i1/p255_1

 2. http://jap.aip.org/resource/1/japiau/v89/i11/p6889_s1

 We are doing our calculations in Wein2K package using the GGA
 approximation and we want to know how the stoner parameter could be found
 according to the my calculations. As non magnetic calculations gives the
 total density of states at around the Fermi level, it is very helpful for us
 to predict the material is magnetic or not using the Stoner parameter.
 therefore, please suggest us how to find the Stoner parameter using wein2k
 package.
  --
 Shamik Chakrabarti
 Research Scholar
 Dept. of Physics  Meteorology
 Material Processing  Solid State Ionics Lab
 IIT Kharagpur
 Kharagpur 721302
 INDIA

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[Wien] K-point parallel with MPI

2011-06-09 Thread David Tompsett
Dear All,

I have a general question about installing Wien2k 11 without being able to
use remote passwordless ssh.

In the installation that I have my sysadmin chose yes to the shared memory
question in siteconfig. I then have attempted running mixed k-parallel/MPI
jobs. What I have found happens is that the mpirun calls for each group of
k-points are issued sequentially rather than in parallel, even though I have
my .machines file set up correctly.

Can anyone advise me as to how I can alter my installation setup so that the
MPI calls for each k-point group will be called at the same time?

Many thanks,
David Tompsett.
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[Wien] Warning in lapw1

2011-06-03 Thread David Tompsett
Dear All,

I have recently compiled the latest Wien2k 11 release, but have come across
an unusual warning in case.output1 when running some larger cases (30 atoms
or more):

:WARN :  WARNING: Not all eigenvectors are orthogonal
 Eigenvalue clusters in eigensolver = 7032153
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
 Gap in eigensolver =  1.05489827340396041E-004  -1.
-1.\
   -1.   -1.
-1.   -1.00\
00   -1.   -1.
-1.   -1.\
   -1.   -1.
-1.   -1.00\
00   -1.   -1.
-1.  \
 -1.   -1.
-1.   -1.\
   -1.   -1.
   Increase CLUSTERSIZE in SECLR4
 Seclr4(Cholesky complete (CPU)) :  17.200112001.02 Mflops
 Seclr4(Cholesky complete (WALL)) : 17.251111672.48 Mflops
 Seclr4(Transform to eig.problem (CPU)) :   84.490 68401.62 Mflops
 Seclr4(Transform to eig.problem (WALL)) :  85.192 67837.83 Mflops
 Seclr4(Compute eigenvalues (CPU)) :   213.210 36141.22 Mflops
 Seclr4(Compute eigenvalues (WALL)) :  213.585 36077.74 Mflops
 Seclr4(Backtransform (CPU)) :   9.500 28964.20 Mflops

This warning appeared in the first iteration of the SCF cycle. I note that
the CLUSTERSIZE  is set to 600 in SECLR4, but don't understand why I see the
warning here. Does anyone know what the cause is? I am running using MPI
parallel over 24 cores. Will the parallelisation setup affect this cluster
size problem?

Thank you,
David Tompsett.
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[Wien] Interesting effect of RLO's with Spin Orbit

2011-04-21 Thread David Tompsett
Dear All,

I have been performing calculations with GGA+U with spin-orbit on an Fe and
oxygen based material. I have noticed an unusual effect when using RLO's (
the relativistic local orbitals) for the oxygen p-states. I applied the +U
orbital potential only to the Fe ion and then applied spin-orbit coupling
inside the Fe and oxide spheres.

Without using RLO's for the oxygen p-orbitals the DOS shows a good band gap
(~3eV). However, when I add RLO's for the oxygen p-states I find that there
are states inside the band gap (significant ~0.1 states/eV/FU). The states
have the d-character of the Fe ions. It appears that the flexibility
introduced by the RLO's on the oxygen are changing the description of the
potential such that the groud state has d-orbital character inside the gap.

Does anyone have experience with such an effect? I am unsure as to whether
the effect is real. The oxygen atoms are light, so I expected the RLO's
would have little effect.

I did sensible things like converge with respect to the emax in case.in1,
k-points, IFFT factor=4.

Many thanks for your help,
David Tompsett.
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[Wien] MPI Strategy

2011-04-01 Thread David Tompsett
Dear All,

I have recently moved my Wien2k calculations to a new machine (Hector in the
UK). This machine does not allow passwordless ssh and therefore disables the
k-point parallel part of Wien2k. I therefore want to clarify some points
about how MPI (chiefly lapw1_mpi) works in Wien2k.

If I run a calculation with say 5 k-points using 5 nodes that each have 24
cores, then will the MPI call of lapw1_mpi split the 5 k-points over the 5
nodes? Or will it simply run the k-points one at a time, using all 120 cores
for each one?

Is there any documentation I can read about the MPI parallel strategy more
generally?

Many thanks,
David Tompsett.
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[Wien] Runtime problem with lapw1_mpi

2011-03-14 Thread David Tompsett
Dear All,

I have recently been attempting to compile the MPI parallel version of the
latest Wien2k. I have successfully generated binaries using ifort (MPI)
comiler, linking with MKL 10.2 and FFTW 2. My system uses QLogic MPI.

I started some small tests. My lapw0 runs well in parallel, but when lapw1
starts I receive the following error:
MPIRUN.node-h18: node-h18:0 node program unexpectedly quit: Exiting.
sh: line 39:  5927 Segmentation fault  $F_PROG lapw1_1.def

Can someone tell me what this $F_PROG variable is? Any hints on what may be
causing the issue are welcome.

My .machines file looks like:

lapw0: node-h18.storage.cluster node-h18.storage.cluster
node-h18.storage.cluster node-h18.storage.cluster node-h17.storage.cluster
node-h17.storage.cluster node-h17.storage.cluster node-h17.storage.cluster
1:node-h18.storage.cluster node-h18.storage.cluster
1:node-h18.storage.cluster node-h18.storage.cluster
1:node-h17.storage.cluster node-h17.storage.cluster
1:node-h17.storage.cluster node-h17.storage.cluster
granularity:1
extrafine:1
lapw2_vector_split:1

Many thanks,
David Tompsett.
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[Wien] Linearization of Low-lying s-state

2011-03-07 Thread David Tompsett
Dear All,

I am performing calculations on slabs of the material LiFePO4 using GGA+U in
the latest Wien2k release.

To perform min_lapw internal parameter optimisation I reduce the RMT's and
use R=1.06 for Phosphorus. This results in a need to reduce the default for
energy separation of core states to -9.2Ry during lstart. As a result
Phosphorus 2p states become part of the valence and need to be treated by a
LO. I am having trouble with large QTL-B values regarding the L=0 states
though.

The energy parameters for phosphorus from case.outputst are:

P   RHFS

 OCCUPANCYENERGY(RYD) (R4)
(R2)  (R)   (R-1) (R-3)

  1S  1.000-1.5314154E+02 5.4020520E-04 1.4448157E-02
1.0359168E-01 1.4648276E+01
  1S  1.000-1.5311976E+02 5.3994095E-04 1.579E-02
1.0357948E-01 1.4649640E+01
  2S  1.000-1.2760822E+01 1.9082408E-01 3.2223815E-01
5.1970457E-01 2.8247951E+00
  2S  1.000-1.2738260E+01 1.8994048E-01 3.2198220E-01
5.1963797E-01 2.8236582E+00
  2P* 1.000-9.1715513E+00 1.9086915E-01 2.9430623E-01
4.8389989E-01 2.7216785E+00
  2P* 1.000-9.1408359E+00 1.8923948E-01 2.9388805E-01
4.8380643E-01 2.7206626E+00
  2P  2.000-9.1041258E+00 1.9405529E-01 2.9690219E-01
4.8614968E-01 2.7052889E+00 6.2902446E+01
  2P  2.000-9.0735022E+00 1.9234866E-01 2.9645480E-01
4.8603999E-01 2.7043227E+00 6.2822412E+01
  3S  1.000-1.0878541E+00 2.9229783E+01 4.1553776E+00
1.8919617E+00 7.2068651E-01
  3S  1.000-8.8775170E-01 3.1604015E+01 4.2438626E+00
1.9036101E+00 7.2402079E-01
  3P* 1.000-4.6442261E-01 7.9415784E+01 6.4475288E+00
2.3215625E+00 5.8248088E-01
  3P* 0.000-2.7621315E-01 1.1443191E+02 7.4136855E+00
2.4614687E+00 5.6064252E-01
  3P  2.000-4.6042138E-01 8.0649286E+01 6.4959005E+00
2.3301759E+00 5.8005227E-01 3.7773200E+00
  3P  0.000-2.7242986E-01 1.1708022E+02 7.4892061E+00
2.4735418E+00 5.5768379E-01 3.5655831E+00

Examples of the low lying states I find in case.output1up and case.output1dn
are:


[Wien] problem with DOS calculations

2010-02-25 Thread David Tompsett
Dear Fhokrul,

With only one k-point you should only have a discrete set of energies. 
Therefore I think the DOS would be a set of delta functions. Your energy 
resolution in case.int is unlikely to capture them.

Best,
David.

Md. Fhokrul Islam wrote:
 Dear Wien2k users,

 I am trying to calculate DOS for a surface supercell but I am not 
 sure why case.dos1evup file
 shows only zeros in the columns for density of states. I have 
 calculated DOS many times before
 without any problem for bulk system. In my surface calculation I have 
 used MPI version of wien2k
 and have only one k-point. I have used the following steps as usual,

 x lapw2 -c -qtl -p -up
 x lapw2 -c -qtl -p -dn

 edited case.int file

 x tetra -up
 x tetra -dn

 I have tried different range of energies in case.int file but couldn't 
 make it work. I would appreciate
 if anyone can tell me how to solve this problem or whether there is a 
 problem in calculating DOS
 for only one k-point.

 Thanks,
 Fhokrul

 
 Hotmail: Trusted email with powerful SPAM protection. Sign up now. 
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 ___
 Wien mailing list
 Wien at zeus.theochem.tuwien.ac.at
 http://zeus.theochem.tuwien.ac.at/mailman/listinfo/wien
   

-- 
David A. Tompsett
Quantum Matter Group
Cavendish Laboratory
J. J. Thomson Avenue
Cambridge CB3 0HE
U.K.
Tel: +44 7907 566351 (mobile)
Fax: +44 1223 768140
http://www-qm.phy.cam.ac.uk/



[Wien] Fermi surface in XCrySDen with data from wien2k parallel calculations

2010-01-15 Thread David Tompsett
Dear Jian-Xin,

The Fermi surface can not be plotted from a parallel calculation because 
XCrysden needs the eigenvalues from a single case.output1* file. From a 
parallel calculation a separate case.output1* file is produced for each cpu.

So to solve the problem you need to write a small script (eg. using awk) 
that combines the separate case.output1* files into one file. Let me 
know if you have problems with it.

Best,
David.

Jian-Xin Zhu wrote:
 Dear Prof. Blaha and Wien2k users,

 I am trying to plot the Fermi surface in XCrySDen for a system with 
 spin-orbit coupling.
 After I finish the self-consistency calculations by
 run_lapw -so -cc 0.0001 -i 40 -p

 I save the data and start the following to prepare the data for Fermi 
 surface plotting with XCrySDen (k points have been prepared without 
 shift as
 required by XCrySDen) ---

 x lapw1 -p
 x lapwso -p
 x lapw2 -so -fermi -p

 I then start the XCrySDEN and select
 File --- Open WIEN2k --- Fermi Surface  (hit OK) --- Render Fermi 
 Surface
 I then got error in reading the  data.
 Note the panel of XCrySDen: Fermi Surface Preparation does not provide 
 the case to run the calculations with spin-orbit coupling, that is,
 x lapw2 -so -fermi

 If I take off the -p option above, and I can plot the Fermi surface 
 successfully.
 It makes me wonder whether I have missed some steps when -p option is 
 used.
 I do notice that the file case.energy is empty when x lapw1 -p is 
 executed.
 So I try running x  sumpara -d after finishing x lapw2 -so -fermi 
 -p, to no avail.

 I searched through the Wien2k archive and could not  find a discussion 
 on this issue.

 Your help/advice is appreciated.

 Jianxin












 ___
 Wien mailing list
 Wien at zeus.theochem.tuwien.ac.at
 http://zeus.theochem.tuwien.ac.at/mailman/listinfo/wien

-- 
David A. Tompsett
Quantum Matter Group
Cavendish Laboratory
J. J. Thomson Avenue
Cambridge CB3 0HE
U.K.
Tel: +44 7907 566351 (mobile)
Fax: +44 1223 768140
http://www-qm.phy.cam.ac.uk/



[Wien] Missing lapwdmc

2009-12-21 Thread David Tompsett
Dear All,

After recently updating to the latest version of Wien2k I found that the 
lapwdmc executable had not been produced, but the real version had been. 
I copy the compile.msg below from SRC_lapwdm/. Does anyone know how I 
can fix this problem?

Thank you,
David.

-- 
David A. Tompsett
Quantum Matter Group
Cavendish Laboratory
J. J. Thomson Avenue
Cambridge CB3 0HE
U.K.
Tel: +44 7907 566351 (mobile)
Fax: +44 1223 768140
http://www-qm.phy.cam.ac.uk/



[Wien] Problem Energy Sep LAPW2 ACTUALLY MKL PROBLEM

2009-12-11 Thread David Tompsett
Dear All,

I recently wrote to the list facing problems with strange eigenvalues 
leading to errors in lapw2. I have solved the issue and thought I would 
write to the list as the actual cause is due to errors in MKL 10.1 and 
early 10.2 documented at:

http://software.intel.com/en-us/articles/dgemm-and-sgemm-accuracy/

I am not sure if these problems have been mentioned on the list before, 
but may affect anyone who has built Wien2k with any of the affected 
versions of Intel MKL. The errors only occur when the system size is 
such that the matrix sizes in lapw1 satisfy the criteria listed at the 
link above. Thus it may appear that one's code is working well and then 
odd errors will occur for particular cases.

After rebuilding my Wien2k with either old MKL 9.1 or the latest 
10.2.2.025 the problems disappeared.

Best wishes,
David Tompsett.

-- 
David A. Tompsett
Quantum Matter Group
Cavendish Laboratory
J. J. Thomson Avenue
Cambridge CB3 0HE
U.K.
Tel: +44 7907 566351 (mobile)
Fax: +44 1223 768140
http://www-qm.phy.cam.ac.uk/


Peter Blaha wrote:
 You said, this happens already in the first iteration ?

 What are your RMT values of all atoms ?   RKmax ?

 Are you sure, your structure is correct ?

 The message 15 eigenvalues below -9. indicates that much more is 
 incorrect than just the energy parameters of atom 24.

 I don't think you should put the E-parameters to -8 Ry. Probably you 
 do not expect eigenvalues in this range.

 Hard to guess what you could have made wrong.

 David Tompsett schrieb:
 Dear Peter and All,

 Thank you for the help. From the case.output2 files it seems that the 
 problem is with very low lying p-states:
  QTL-B VALUE .EQ. 1876.88467   in Band of energy   -8.53431   ATOM=   
 24   L=  1
Check for ghostbands or EIGENVALUES BELOW XX messages
Adjust your Energy-parameters or use -in1new switch, check RMTs  !!!

 My linearization energies for this atom are:
 0.605  0  (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global 
 APW/LAPW)
 00.60  0.000 CONT 1
 0   -4.00  0.005 STOP 1
 1   -2.21  0.010 CONT 1
 10.60  0.000 CONT 1
 20.60  0.010 CONT 1

 My first thought is to alter -2.21 to -8.00 for the p-state LO, but I 
 am concerned that since -8.53431 is so low that somehow my 
 calculation window is including multiple p-states ie. more than two 
 sets of p-states.
 Also, the case.output1 file says that there are:
   15 EIGENVALUES BELOW THE ENERGY   -9.0
   

 Please advise me as to how to proceed.

 Thank you,
 David.

 Peter Blaha wrote:
 You are doing k-parallel calc !

 What says lse   ?
 Check the individual case.output2_xx files !

 David Tompsett schrieb:
 Dear Peter and All,

 the end of my case.output2 looks as follows and confirms that there 
 is some error in finding the separation of semi-core and valence 
 states, though from the userguide it seems that this should not be 
 a major issue without using -in1new.

 eseper below EF  0.500eseper minimum gap  
 5.000E-002
 Energy to separate semicore and valence states:  -999.  
 :NOE  : NUMBER OF ELECTRONS  =1313.000

 :FER  : F E R M I - ENERGY(TETRAH.M.)=   0.94199
 NbFe2Super222NM.weigh  
 




 8
 writing
 NbFe2Super222NM.weigh_1
 




 writing
 NbFe2Super222NM.weigh_2
 




 writing
 NbFe2Super222NM.weigh_3
 




 writing
 NbFe2Super222NM.weigh_4
 




 writing
 NbFe2Super222NM.weigh_5
 




 writing
 NbFe2Super222NM.weigh_6
 




 writing
 NbFe2Super222NM.weigh_7
 




 writing
 NbFe2Super222NM.weigh_8

[Wien] Problem with Energy Separation in LAPW2

2009-12-09 Thread David Tompsett
10351.96425840761.9977970344  0.00D+00
band10361.96677832661.9948459103  0.00D+00
band10371.97010746941.9964735701  0.00D+00
band10381.97142902331.9942832855  0.00D+00
band10391.97191115251.9950427054  0.00D+00
band10401.97382520671.9990564146  0.00D+00
band10411.97673260211.9980496124  0.00D+00
band10421.98318581341.9831858134  0.00D+00
band10431.98793378881.9879337888  0.00D+00
band10441.99082813551.9908281355  0.00D+00
band10451.99389282781.9938928278  0.00D+00

eseper below EF  0.500eseper minimum gap  
5.000E-002
Energy to separate semicore and valence states:  -999.   

:NOE  : NUMBER OF ELECTRONS  =1313.000

:FER  : F E R M I - ENERGY(TETRAH.M.)=   0.94199
NbFe2Super222NM.weigh  

   

 8
writing
NbFe2Super222NM.weigh_1

   

 writing
NbFe2Super222NM.weigh_2

   

 writing
NbFe2Super222NM.weigh_3

   

 writing
NbFe2Super222NM.weigh_4

   

 writing
NbFe2Super222NM.weigh_5

   

 writing
NbFe2Super222NM.weigh_6

   

 writing
NbFe2Super222NM.weigh_7

   

 writing
NbFe2Super222NM.weigh_8

   

 NK   8


Peter Blaha wrote:
 Please check case.output2

 D.A. Tompsett schrieb:
 Dear All,

 I am trying to run a supercell calculation of transition metals in a 
 Laves AB2 type phase. The supercell contains 96 atoms and one atom of 
 type B doped onto the site of an A atom.

 My calculation is repeatedly failing in LAPW2 and the stderr shows a 
 QTL-B error. My case.scf2 looks like:

 Can anyone suggest to me how I might fix this problem or where I 
 should look to solve it?

 Many thanks,
 David Tompsett.






Peter Blaha wrote:
 Please check case.output2

 D.A. Tompsett schrieb:
 Dear All,

 I am trying to run a supercell calculation of transition metals in a 
 Laves AB2 type phase. The supercell contains 96 atoms and one atom of 
 type B doped onto the site of an A atom.

 My calculation is repeatedly failing in LAPW2 and the stderr shows a 
 QTL-B error. My case.scf2 looks like:

 Can anyone suggest to me how I might fix this problem or where I 
 should look to solve it?

 Many thanks,
 David Tompsett.



-- 
David A. Tompsett
Quantum Matter Group
Cavendish Laboratory
J. J. Thomson Avenue
Cambridge CB3 0HE
U.K.
Tel: +44 7907 566351 (mobile)
Fax: +44 1223 768140
http://www-qm.phy.cam.ac.uk/



[Wien] Problem with Energy Separation in LAPW2

2009-12-09 Thread David Tompsett
Dear Peter and All,

Thank you for the help. From the case.output2 files it seems that the 
problem is with very low lying p-states:
  QTL-B VALUE .EQ. 1876.88467   in Band of energy   -8.53431   ATOM=   
24   L=  1
Check for ghostbands or EIGENVALUES BELOW XX messages
Adjust your Energy-parameters or use -in1new switch, check RMTs  !!!

My linearization energies for this atom are:
 0.605  0  (GLOBAL E-PARAMETER WITH n OTHER CHOICES, global 
APW/LAPW)
 00.60  0.000 CONT 1
 0   -4.00  0.005 STOP 1
 1   -2.21  0.010 CONT 1
 10.60  0.000 CONT 1
 20.60  0.010 CONT 1

My first thought is to alter -2.21 to -8.00 for the p-state LO, but I am 
concerned that since -8.53431 is so low that somehow my calculation 
window is including multiple p-states ie. more than two sets of p-states.
Also, the case.output1 file says that there are:
   15 EIGENVALUES BELOW THE ENERGY   -9.0
   

Please advise me as to how to proceed.

Thank you,
David.

Peter Blaha wrote:
 You are doing k-parallel calc !

 What says lse   ?
 Check the individual case.output2_xx files !

 David Tompsett schrieb:
 Dear Peter and All,

 the end of my case.output2 looks as follows and confirms that there 
 is some error in finding the separation of semi-core and valence 
 states, though from the userguide it seems that this should not be a 
 major issue without using -in1new.

 eseper below EF  0.500eseper minimum gap  
 5.000E-002
 Energy to separate semicore and valence states:  -999.  
 :NOE  : NUMBER OF ELECTRONS  =1313.000

 :FER  : F E R M I - ENERGY(TETRAH.M.)=   0.94199
 NbFe2Super222NM.weigh
   

  
  

 8
 writing
 NbFe2Super222NM.weigh_1  
   

  
  

 writing
 NbFe2Super222NM.weigh_2  
   

  
  

 writing
 NbFe2Super222NM.weigh_3  
   

  
  

 writing
 NbFe2Super222NM.weigh_4  
   

  
  

 writing
 NbFe2Super222NM.weigh_5  
   

  
  

 writing
 NbFe2Super222NM.weigh_6  
   

  
  

 writing
 NbFe2Super222NM.weigh_7  
   

  
  

 writing
 NbFe2Super222NM.weigh_8  
   

  
  

 NK   8

 Otherwise the file seems OK and I copy the rest of it below 
 (excluding the KVEC list). The error is occurring on the very first 
 SCF cycle each time.

 Many thanks for any more help,
 David.



-- 
David A. Tompsett
Quantum Matter Group
Cavendish Laboratory
J. J. Thomson Avenue
Cambridge CB3 0HE
U.K.
Tel: +44 7907 566351 (mobile)
Fax: +44 1223 768140
http://www-qm.phy.cam.ac.uk/



[Wien] lcore Stops

2009-09-28 Thread David Tompsett
Dear All,

I am having a problem while attempting an scf calculation of Ag5Pb2O6.

In setting up the calculation the default RMT's mean that there is core 
charge leakage from the large Pb atom if one uses the default separation 
energy of 6.0Ry.
I have tried to get around this in two ways:
1) Set the separation to 8.0Ry. The lstart indicates no leakage.
2) Increase the RMT of Pb (and decrease that of O to compensate) so that 
even with 6.0Ry separation input to lstart there is no charge leakage.

In both cases lcore fails in the same way. The program lcore fails right 
after it is called leaving no output or error file that I can find.

lapw2 seems to have produced all of its output files successfully.

In case (2) above I also attempted to reduce RKmax to adjust for the 
smaller value of RMTmin, but the same type of error occurs.

Is there something else that I should be doing in the setup? Or does 
anyone know where I should look to find the relevant error?

Thank you,
David.

-- 
David A. Tompsett
Quantum Matter Group
Cavendish Laboratory
J. J. Thomson Avenue
Cambridge CB3 0HE
U.K.
Tel: +44 7907 566351 (mobile)
Fax: +44 1223 768140
http://www-qm.phy.cam.ac.uk/



[Wien] Checking L,M Basis for new Local Rotation Matrix

2009-06-09 Thread David Tompsett
Dear All,

I have changed the local rotation matrix for an atom in my system from 
the default found by program SYMMETRY. I have determined what I think 
the new L,M basis should be according to the prescription in reference 
Kara and Kurki-Suonio 81.

In the UG it says Perform a run of LAPW1 and LAPW2 using the 
GAMMA-point only (or a complete star of
another k point). In such a case, ?wrong? LM combinations must vanish.
I want to check my new basis by this method. In what sense would the 
wrong LM vanish? Which output file would I look at?

Thank you for any help,
David.

-- 
David A. Tompsett
Quantum Matter Group
Cavendish Laboratory
J. J. Thomson Avenue
Cambridge CB3 0HE
U.K.
Tel: +44 7907 566351 (mobile)
Fax: +44 1223 768140
http://www-qm.phy.cam.ac.uk/