Re: [Wien] L'approximation MBJ

2013-07-02 Thread tran
Ce sont quelques articles sur MBJ:

http://publik.tuwien.ac.at/files/PubDat_175662.pdf
http://publik.tuwien.ac.at/files/PubDat_197196.pdf
http://publik.tuwien.ac.at/files/PubDat_207439.pdf
http://prb.aps.org/abstract/PRB/v82/i20/e205102
http://prb.aps.org/abstract/PRB/v87/i7/e075121
http://prb.aps.org/abstract/PRB/v87/i7/e075121
http://link.aip.org/link/doi/10.1063/1.4798706

et le guide de l'utilisateur:

http://www.wien2k.at/reg_user/textbooks/usersguide.pdf


On Tue, 2 Jul 2013, Sameh noui wrote:

 SVP je cherche des documents sur l'approximation MBJ
 
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Re: [Wien] Exchange functional

2013-07-02 Thread tran
Hi,

with wien2k it is possible to do calculations with a functional which
is similar (but not exactly the same) to the Sx-LDA functional of
Bylander and Kleinman [PRB 41, 7868 (1990)].

To do such calculations you have to follow the steps explained in pages
50-54 and 104-106 of the userguide:
http://www.wien2k.at/reg_user/textbooks/usersguide.pdf

In your case you have to choose:
indxc=5 in case.in0
indxc=51 in case.in0_grr
alpha=1 in case.inhf

The screening parameter lambda is calculated automatically in the Sx-LDA
functional, but not in wien2k where it is a parameter chosen by the user
(in case.inhf).

Be aware that calculations using the Hartree-Fock exchange (e.g., Sx-LDA)
are between 1 and 3 orders of magnitude more expensive than LDA/GGA
calculations.

F. Tran


On Tue, 2 Jul 2013, wasim raja Mondal wrote:

 Dear wien2k experts
 
 I want to use Sx-LDA functional for my calculation. May I know this
 functional is available in wien2k and if yes what is the number for that.
 
 Regards
 wasim
 
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Re: [Wien] How to use LDA+U

2013-07-03 Thread tran
http://prb.aps.org/abstract/PRB/v71/i3/e035105
http://prb.aps.org/abstract/PRB/v79/i3/e035103

On Tue, 2 Jul 2013, Yasir Ali wrote:

 
 
  Hi.
 
 I need to know how to use LDA+U method for exchange and correlation and when 
 it is suitable to use?
 
 
 Regards: 
 Yasir Ali___
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Re: [Wien] kinetic energy in WIEN2k

2013-07-09 Thread tran
Yes, but not by default. In the 1st line of case.in0 you have to
replace TOT by KXC. Then, in case.scf the kinetic energy corresponds to
the keyword :EKIN. Be aware that the value is wrong when LDA+U is used.

F. Tran

On Tue, 9 Jul 2013, Yundi Quan wrote:

 Does WIEN2k_12 write kinetic energy term in case.scf file?
 
 
 
 
 Yundi
 
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Re: [Wien] XCPOT = 99 is available?

2013-07-11 Thread tran
Hi,

during initialization (init_lapw), these are the functionals listed in
vxclm2.f from SRC_lstart (and not SRC_lapw0) that can be used.
But, after the initialization is finished you can select any functional
you want in case.in0 (e.g., 99) before starting scf.

F. Tran

On Thu, 11 Jul 2013, Chang-Jong Kang wrote:

 Dear Prof. Blaha and Wien2k users,
 
 I found that some exchange-correlation functionals are available but
 init_lapw dose not show them.
 
 The list of them is in the vxclm2.f source file in SRC_lapw0.
 
 Among them, IGRAD = 99 is Exc and Vxc = 0.
 
 I tried the # 99, x lstart error happened.
 
 When I again initialized it with XCPOT = 5 (LSDA) and then changed XCPOT to
 99,
 x lapw0 error happened.
 
 My question is, how to use XCPOT # 99 (Exc and Vxc = 0).
 
 Is there any trick to use it?
 
 
 Regards,
 Chang-Jong Kang
 
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Re: [Wien] XCPOT = 99 is available?

2013-07-11 Thread tran
Send us the file xcpot1.f.

On Thu, 11 Jul 2013, Chang-Jong Kang wrote:

 Dear Prof. Blaha and Tran,
 
 Thank you for replying.
 
 During initialization, I selected LSDA functional, and then I changed from
 5 to 99 in case.in0 file.
 When I started scf loop, the following error message appeared;
 
 =
 forrtl: severe (174): SIGSEGV, segmentation fault occurred
 Image  PCRoutineLineSource
 
 lapw0  00492537  xcpot1_   463  xcpot1.f
 lapw0  0044AE66  MAIN__   1865  lapw0.F
 lapw0  00403B6C  Unknown   Unknown  Unknown
 libc.so.6  0036B581ECDD  Unknown   Unknown  Unknown
 lapw0  00403A69  Unknown   Unknown  Unknown
 13.408u 8.895s 0:22.53 98.9%0+0k 184+128io 2pf+0w
 error: command   /WIEN2k_12/lapw0para lapw0.def   failed
 =
 
 As you mentioned, it ran without any error, but in my case, the above lapw0
 error always happened.
 
 How could I settle it?
 
 Many thanks,
 Chang-Jong Kang
 
 
 On Thu, Jul 11, 2013 at 5:59 PM, t...@theochem.tuwien.ac.at wrote:
 
  Hi,
 
  during initialization (init_lapw), these are the functionals listed in
  vxclm2.f from SRC_lstart (and not SRC_lapw0) that can be used.
  But, after the initialization is finished you can select any functional
  you want in case.in0 (e.g., 99) before starting scf.
 
  F. Tran
 
  On Thu, 11 Jul 2013, Chang-Jong Kang wrote:
 
   Dear Prof. Blaha and Wien2k users,
  
   I found that some exchange-correlation functionals are available but
   init_lapw dose not show them.
  
   The list of them is in the vxclm2.f source file in SRC_lapw0.
  
   Among them, IGRAD = 99 is Exc and Vxc = 0.
  
   I tried the # 99, x lstart error happened.
  
   When I again initialized it with XCPOT = 5 (LSDA) and then changed XCPOT
  to
   99,
   x lapw0 error happened.
  
   My question is, how to use XCPOT # 99 (Exc and Vxc = 0).
  
   Is there any trick to use it?
  
  
   Regards,
   Chang-Jong Kang
  
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Re: [Wien] HSE

2013-07-13 Thread tran
No, but YS-PBE0 gives very similar results:
http://prb.aps.org/abstract/PRB/v83/i23/e235118

On Fri, 12 Jul 2013, Yundi Quan wrote:

 Is it possible to use HSE functional in the latest verion?
 
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Re: [Wien] Confusion in Selecting proper value of Hubbard potential.

2013-07-19 Thread tran
Hi,

I have never heard that the proper value of U is the one when the band gap
starts to decrease. Usually the value of U is chosen such that the
calculated properties (e.g., band gap or magnetic moment) agree with
experiment.

F. Tran

On Sat, 20 Jul 2013, Zaid wrote:

 Respected Users
 
 
 I am applying GGA+U technique to considered compounds. In order to select
 proper value of U for specific material, I am changing the value of U from
 2eV to 10eV with a step of 1eV. I was expecting that on increasing U value
 in the range 2-10eV, a value of U will appear where the corresponding band
 gap will start to decrease instead of increase. That value of U where the
 band gap start to decrease instead of rising will be the proper U value in
 the range 2-10eV.
 
 I my case the, every time I am getting increasing band gap values on
 increasing U value from 2-10eV with a step of 1eV. Band gap does not
 decrease in the range 2-10eV. Should I increase the range ? May anyone
 suggest that whether my practice of finding U value is right ? If not how
 can I find proper value of U for specific compound ?
 
 Thank you very much
 
 Best Regards
 Zaid
 
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Re: [Wien] Confusion in Selecting proper value of Hubbard potential.

2013-07-20 Thread tran
You can try larger U to see what happens, but values above 10 or 12 eV
start to be unphysical in solids. Also, the more the top of the valence
band or bottom of conduction band has an important contribution not coming
from the d or f electrons (e.g., oxygen-p), the less GGA+U will be
efficient to adjust the band gap. GGA+U does not always solve problems in
stronlgy correlated systems. As mentioned by Hong Jiang, you should maybe
consider other methods.

F. Tran

On Sat, 20 Jul 2013, Zaid wrote:

 Dear Sir H. Jiang
 
 I implemented GGA+U to my considered compound, keeping in mind that GGA+U
 is valuable for compounds having strongly correlated system (like in d and
 f orbitals). But My problem is regarding the selection of U value.
 
 Experimental band gap for my compound is 2.0eV. The maximum band gap on
 increasing U value for my calculation is 1.117eV at 10 eV. So, should I
 increase U value beyond 10eV ? Untill now from my literature review, the
 value of U is less than 10 eV.
 Secondly, if suppose a compound has not been studied experimentally then
 how we choose calue of U ?
 
 Kindly guide.
 
 Best regards
 Zaid
 
 
 On Sat, Jul 20, 2013 at 2:31 PM, Hong Jiang jiang...@googlemail.com wrote:
 
   Hi,
  The Hubbard U correction in LDA/GGA+U is to correct the failure of LDA/GGA
  to describe localized d- or f-states.  Therefore LDA/GGA+U is able to give
  an accurate band gap only if the band gap of your system happens to be of
  d-d or f-f character, which, however, not the case for most systems (see,
  e.g. H. Jiang, et al. *Phys. Rev. B* *82*, 045108 
  (2010)).http://prb.aps.org/abstract/PRB/v82/i4/e045108
 
  To obtain accurate band gaps, you can try
  * modified Becke-Johnson, ( F. Tran and P. Blaha, Phys. Rev. Lett. *102*,
  226401 
  (2009)http://link.aip.org/link/?l_creator=getabs-normal1l_dir=FWDl_rel=CITESfrom_key=JCPSA60001381313411501from_keyType=CVIPSfrom_loc=AIPto_j=PRLTAOto_v=102to_p=226401to_loc=APSto_url=http%3A%2F%2Flink.aps.org%2Fabstract%2FPRL%2Fv102%2Fe226401;
  H. Jiang (J. Chem. Phys. *134*, 
  134115(2013)http://dx.doi.org/10.1063/1.4798706)
  * hybrid functionals, (F. Tran and P. Blaha, Phys. Rev. B 83, 235118
  (2011) http://dx.doi.org/10.1103/PhysRevB.83.235118)
  * GW (if your system is not very big).  (H. Jiang et al. Computer Phys.
  Commun.,*184*, 348(2013) http://dx.doi.org/10.1016/j.cpc.2012.09.018).
 
  Hong
 
 
  于 2013/7/20 14:03, Zaid 写道:
 
 Dear Sir,
 
   you are right. Experimental band gap for my compound is 2.0eV. The
  maximum band gap on increasing U value for my calculation is 1.117eV at 10
  eV. So, should I increase U value beyond 10eV ? Untill now from my
  literature review, the value of U is less than 10 eV.
   Secondly, if suppose a compound has not been studied experimentally then
  how we choose calue of U ?
 
   Thank you
   Zaid
 
 
  On Sat, Jul 20, 2013 at 1:48 PM, t...@theochem.tuwien.ac.at wrote:
 
  Hi,
 
  I have never heard that the proper value of U is the one when the band gap
  starts to decrease. Usually the value of U is chosen such that the
  calculated properties (e.g., band gap or magnetic moment) agree with
  experiment.
 
  F. Tran
 
  On Sat, 20 Jul 2013, Zaid wrote:
 
   Respected Users
  
  
   I am applying GGA+U technique to considered compounds. In order to
  select
   proper value of U for specific material, I am changing the value of U
  from
   2eV to 10eV with a step of 1eV. I was expecting that on increasing U
  value
   in the range 2-10eV, a value of U will appear where the corresponding
  band
   gap will start to decrease instead of increase. That value of U where
  the
   band gap start to decrease instead of rising will be the proper U value
  in
   the range 2-10eV.
  
   I my case the, every time I am getting increasing band gap values on
   increasing U value from 2-10eV with a step of 1eV. Band gap does not
   decrease in the range 2-10eV. Should I increase the range ? May anyone
   suggest that whether my practice of finding U value is right ? If not
  how
   can I find proper value of U for specific compound ?
  
   Thank you very much
  
   Best Regards
   Zaid
  
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Re: [Wien] Rkmax

2013-07-27 Thread tran
Hi,

When you choose RKMAX, then K is given by RKMAX/RMT, but
since K can take only some particular value (K is not a continuous
variable) then the one closest (or maybe the next larger?)
to RKMAX/RMT is used.
This value is multiplied by RMT to give :RKM.
If you are lucky then RKMAX/RMT will be equal (or very closely equal)
to an allowed value of K.

F. Tran

On Fri, 26 Jul 2013, Francisco Garcia wrote:

 Dear users,
 
 I would like to know why rkmax is sometimes slightly reduced in case.scf
 compared to the value in case.in1(c). E.g, grep :RKM in case.scf is 7.97
 but rkmax is 8 in case.in1(c). Sometimes the values match exactly.
 
 Thank you.
 
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Re: [Wien] DOS with GGA+U and SO

2013-07-29 Thread tran
If this is a complex calculation (no symmetry inversion) then you need also -c

F. Tran

On Mon, 29 Jul 2013, pl...@physics.ucdavis.edu wrote:

 Dear Wien2k experts,
 
 I have a problem calculating DOS when both GGA+U and SO are switched on. I
 tested on bulk Gd. I tried different options directly after SCF (x lapw2
 -qtl -up -so, x qtl -up -so). The position of the f-bands comes out
 different in DOS and different in band-structure calculation (which I
 perform after DOS calculation). I suspect either that SO is not on when
 calculating DOS...
 
 It would help me if an expert could list the correct sequence of programs
 after SCF to obtain the correct DOS with GGA+U and SO.
 
 Regards,
 Lukasz
 
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Re: [Wien] how to extract and plot the spin-charge density

2013-08-03 Thread tran
Hi,

You can use XCrysDen, see page 188 of the user's guide:
http://www.wien2k.at/reg_user/textbooks/usersguide.pdf

or run yourself lapw5 (see page 144 of the UG) and then use
a software to plot the data in case.rho

F. Tran

On Sat, 3 Aug 2013, Madhav Ghimire wrote:

 Dear wien experts and users,
I am interested to plot the iso-surface spin charge density using the
 wien2k calculated data.
 Using the scf file I fail to plot the iso-surface of spin-charge density.
 
 Does someone familiar on
 (i) how to  extract the information of spin-charge density and from which
 file
 (ii) how to plot the iso-surface of spin-charge density
 
 I will be very glad for your help.
 Thanks in advance
 Best regards
 Madhav Ghimire
 
 
 -- 
 MANA, Nano-System Theoretical Physics Unit
 NIMS, Tsukuba, Japan
 
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Re: [Wien] how to extract and plot the spin-charge density

2013-08-05 Thread tran
yes it's ok

On Mon, 5 Aug 2013, Madhav Ghimire wrote:

 Dear Tran,
 Thanks for your comment.
 In order to plot the spin-charge density, I still have some doubts in
 selecting the necessary appropriate file.
 After going through the userguide as you suggested,
 I have edited the corresponding files as shown below:
 
 (i) case.in5
 -1 -1 0 4 # x, y, z, divisorof origin
 -1  3 0 4 # x, y, z, divisorof x-end
  3 -1 0 4 # x, y, z, divisorof y-end
 3 2 3   # number of shells
 100 100# number of points in x and y dir, (ratio close to lenght
 ratio
 RHO #   RHO|DIFF|OVER; ADD|SUB or blank
 TOT VAL NODEBUG #   ANG|ATU; VAL|TOT; DEBUG|NODEBUG
 ORTHO   # optional: ORHO|NONORTHO plotting directions
 
 (ii) lapw5.def
 5 ,'sr2.in5c', 'old','formatted',0
 6 ,'sr2.output5',   'unknown','formatted',0
 8 ,'sr2.struct','old','formatted',0
 9 ,'sr2.clmup','old','formatted',0
 10,'sr2.tmp',   'unknown','unformatted',0
 11,'sr2.clmdn',  'unknown','formatted',0
 12,'sr2.sigma', 'unknown','formatted',0
 20,'sr2.rho_onedim','unknown','formatted',0
 21,'sr2.rho',   'unknown','formatted',0
 
 Can you please confirm if (i) RHO and TOT in line 6 and 7 of case.in5c and
 (ii) replacement of case.clmvalup/dn of unit 9(11) with case.clmup/dn of
 lapw5.def are correct for obtaining the spin-charge density.
 
 Thanks for your co-operation.
 Best regards
 Madhav
 
 On Sat, Aug 3, 2013 at 4:45 PM, t...@theochem.tuwien.ac.at wrote:
 
  Hi,
 
  You can use XCrysDen, see page 188 of the user's guide:
  http://www.wien2k.at/reg_user/textbooks/usersguide.pdf
 
  or run yourself lapw5 (see page 144 of the UG) and then use
  a software to plot the data in case.rho
 
  F. Tran
 
  On Sat, 3 Aug 2013, Madhav Ghimire wrote:
 
   Dear wien experts and users,
  I am interested to plot the iso-surface spin charge density using the
   wien2k calculated data.
   Using the scf file I fail to plot the iso-surface of spin-charge density.
  
   Does someone familiar on
   (i) how to  extract the information of spin-charge density and from which
   file
   (ii) how to plot the iso-surface of spin-charge density
  
   I will be very glad for your help.
   Thanks in advance
   Best regards
   Madhav Ghimire
  
  
   --
   MANA, Nano-System Theoretical Physics Unit
   NIMS, Tsukuba, Japan
  
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 -- 
 MANA, Nano-System Theoretical Physics Unit
 NIMS, Tsukuba, Japan
 
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[Wien] Small problem with hybrid functionals

2013-08-05 Thread tran
Dear WIEN2k users,

I mention to those who intend to use hybrid functionals with 
WIEN2k_13, that they have to modify the last line of case.in0_grr (FFT
parameters and enhancement factor) such that this line is the same as in 
case.in0. By default, in case.in0_grr the enhancement factor is 1, while
it is usually 2 in case.in0. There was no such problem with WIEN2k_12
since case.in0_grr was created manually from case.in0.

F. Tran

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Re: [Wien] run_bandplothf problem crash for HF

2013-08-07 Thread tran

Dear Martin,

Actually, I don't exactly know what is the problem since it does not
happen to me. Maybe you can try to know what the messages Bareword ...
mean. Are you using a queueing system?

F. Tran


Date: Tue, 16 Jul 2013 07:51:21 +0200
From: Martin Gmitra martin.gmi...@gmail.com
Reply-To: A Mailing list for WIEN2k users wien@zeus.theochem.tuwien.ac.at
To: A Mailing list for WIEN2k users wien@zeus.theochem.tuwien.ac.at
Subject: [Wien] run_bandplothf problem crash for HF

Dear Wien2k users,

I am running spin-polarized calculations using YS-PBE0 with the latest
Wien2k release v13. Self-consistent calculations run smooth on 4 cores. For
the band calculations I asked 10 cores (.machines modified) invoking

run_bandplothf -p -up -redklist -qtl

Here is list of :log
Mon Jul 15 21:53:14 CEST 2013 (x) lapw1 -band -up -p
Tue Jul 16 00:53:26 CEST 2013 (x) hf -band -up -p -redklist
Tue Jul 16 00:53:37 CEST 2013 (x) sumhfpara -c -up -band -d
Tue Jul 16 00:53:37 CEST 2013 (x) lapw2 -hf -band -up -qtl

After successful  lapw1 -band -up -p there is the following std output
(repeated 10 times, giving here non redundant info)

Bareword up not allowed while strict subs in use at (eval 1) line 1.
Bareword case not allowed while strict subs in use at (eval 1) line 1.
Bareword klist_band not allowed while strict subs in use at (eval 1)
line 1.
running HF in parallel mode
[1] 4791
OPEN FAILED
[1]  + Done   ( cd $PWD; $t $exe ${def}_${loop}.def; rm -f
.lock_$lockfile[$p] )   ...
 localhost ERROR IN OPENING UNIT: 16 FILENAME: case.klist_1 STATUS:
old FORM:formatted 0.0u 0.0s 0:00.00 0.0% 0+0k 0+0io 0pf+0w

. . .
 localhost ERROR IN OPENING UNIT: 16 FILENAME: case.klist_10 STATUS:
old FORM:formatted 0.0u 0.0s 0:00.00 0.0% 0+0k 0+0io 0pf+0w

Should not file id 16 uphf_*.def files (see uphf_1.def below) contain
case.klist_band_1 or x_lapw script create corresponding case.klist_* files?

4,'case.inhf',   'old','formatted',0
5,'case.in0','old','formatted',0
6,'case.outputhfup_1',  'unknown','formatted',0
7,'case.clmsum', 'old','formatted',0
8,'case.clmup','unknown','formatted',0
9,'case.in1c',  'old','formatted',0
10,'case.vectorup_1','old','unformatted',9000
11,'case.vectorhfup_old','old','unformatted',9000
12,'case.vectorhfup_1',  'unknown','unformatted',9000
14,'case.r2v_grr','old','formatted',0
15,'case.klist_fbz',  'old','formatted',0
16,'case.klist_1',  'old','formatted',0
17,'case.outputkgenhf',   'old','formatted',0
19,'case.clmcorup','old','formatted',0
20,'case.struct', 'old','formatted',0
21,'case.scfhfup_1', 'unknown','formatted',0
26,'case.weighhfup',   'old','unformatted',0
28,'case.inc','old','formatted',0
29,'case.corewfup','old','formatted',0
31,'case.energyhfup_1',   'unknown','formatted',0
32,'case.vspup',   'old','formatted',0
33,'case.vspup_old', 'old','formatted',0
40,'case.klist_band_1'   ,'unknown','formatted',0
45,'case.para' ,'unknown','formatted',0
46,'case.klist_rfbz'   ,'unknown','formatted',0


Best regards,
Martin Gmitra
Uni Regensburg

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Re: [Wien] FeO

2013-08-08 Thread tran

Hi,

If you are considering the ground-state of FeO which is antiferromagnetic
(AFII) you need a unit cell which contains two formula units.
I attached such a struct file. It would be good to try to understand it.

F. Tran

On Thu, 8 Aug 2013, Antonio Vanderlei dos Santos - Fisica wrote:



dear users
I'm working with the oxide FeO. Could someone tell me the unitary cell of this 
compound.

 

Dr Antonio
 

FeO_AFII
R   LATTICE,NONEQUIV.ATOMS:  3166_R-3m  
MODE OF CALC=RELA unit=ang 
  5.791258  5.791258 28.371255 90.00 90.00120.00
ATOM  -1: X=0. Y=0. Z=0.
  MULT= 1  ISPLIT= 8
Fe1NPT=  781  R0=0.5000 RMT=2.1600   Z: 26.0
LOCAL ROT MATRIX:1.000 0.000 0.000
 0.000 1.000 0.000
 0.000 0.000 1.000
ATOM   2: X=0.5000 Y=0.5000 Z=0.5000
  MULT= 1  ISPLIT= 8
Fe2NPT=  781  R0=0.5000 RMT=2.1600   Z: 26.0
LOCAL ROT MATRIX:0.000 0.000 0.000
 0.000 0.000 0.000
 0.000 0.000 0.000
ATOM   3: X=0.2500 Y=0.2500 Z=0.2500
  MULT= 2  ISPLIT= 8
ATOM   3:X= 0.7500 Y=0.7500 Z=0.7500
O  NPT=  781  R0=0.0001 RMT=1.9100   Z:  8.0
LOCAL ROT MATRIX:0.000 0.000 0.000
 0.000 0.000 0.000
 0.000 0.000 0.000
   0  NUMBER OF SYMMETRY OPERATIONS
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Re: [Wien] about c in TB-mBJ for open structures

2013-08-15 Thread tran

Hi,

The mBJ potential can certainly not be used for systems with infinite
vacuum (e.g., isolated molecule, surface), but for open structures the
results can (maybe) still be ok without fixing c to some value
(I have not tried myself, but maybe there is already results in the
literature on open structures). If the gaps that you obtained without
fixing c are not completely wrong, then I do not see any reason
to fix c from a previous calculation.

Also, there is no reason to fix c to the one obtained with graphite
and not another solid. The procedure you mentioned looks ok.

F. Tran

On Thu, 15 Aug 2013, Fabiana Da Pieve wrote:


Dear wien2k developers and users

I am checking the performance of Tran-Blaha mBJ with respect to GW
(non self consistent, for the moment) for some organic crystals (quite
open structures). For some of them the improvement with respect to LDA
(my starting point for G0W0) is good, for some others it is still
pretty good but I would like to have a better result. Prof. Blaha
suggested sometime ago to use the c parameter from bulk graphite,
since the scf calculation  of the c parameter of TB-mBJ in suh open
structures could have not so much sense.

I am using Wien2k_11.1. Could you please confirm that the procedure I
am going to use (reported here below) is correct ?
(I just want a confirmation of what I read in the manual for this
version at page 50,
or IF THERE IS SOMETHING MORE THAT I SHOULD DO and that I did not
catch from the manual).

I will do a bulk calculation for graphite, then take the graphite.grr
file, copy it into the orgcrystal.grr ; then I will cancel  the
orgcrystal.in0_grr file and then I will run finally the mBJ self
consistent run. The value inside the .grr file (which will be indeed
the one corresponding to bulk graphite) will be read by the scf mBJ
run.

(sorry to ask, but my contract finishes soon and I cannot allow myself
to do stupid errors...)

Thank you very much
Fabiana

VUB, Free University of Brussels
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Re: [Wien] need clarification on changes in spin magnetic moment in cell after SCF run

2013-08-16 Thread tran

If the total magnetic moment appears/disappears during geometry
optimization, it means that you are close to a non-magnetic/magnetic
phase transition.

It can happen that a functional does not give the correct magnetic
phase.

The sign of :MMTOT has no physical meaning. What is important
is to compare the signs of the magnetic moments in the spheres
(:MMI00).

F. Tran

On Thu, 15 Aug 2013, venkatesh chandragiri wrote:


Dear Sir,

I did the calculations on 225 space group compounds as regular methodology
in Wien2k such as running volume optimization and Force minimization before
going to the final SCF. I have few doubts on the results that i have obtain
as written below
1. I found that total magnetic moment of my structure is  0 uB (Bohr
magnetron) which is predicted for my case. But, whenever working with run
scf by taking Force optimized case.struct file, i got increased total
magnetic moment  to -0.00168 uB. So, why this increase in magnetic moment
happens, Is there ant correction to be done..?

2. As i already done scf calculations while doing Force minimization, can i
use this case.scf file for my further property estimations like..DOS,
magnetic moment, band structure and optical properties...etc.? (Because
this struct file have total magnetic moment same as predicted).

3. I have got negative total magnetic moments for some structures, Is that
means these structures have anti ferromagnetic ground state..?

looking forward to your responses.

thanks in advance

regards,
Ch. Venkatesh,C/o. Prof. V. Srinivas,
Department of Physics  Meteorology,
IIT Kharagpur.
ph: +919445909693

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Re: [Wien] possible bugs in kgen after SOC

2013-08-16 Thread tran

If your solid has a bcc or fcc unit cell, then it is normal,
since the k points are expressed in terms of the cubic lattice
vectors which are not the primitive ones.

F. Tran

On Thu, 15 Aug 2013, Guo-ping Zhang wrote:



Dear Peter and wien users,

I got a very strange list of k point with kgen after initso (with noaxial 
magnetization say, along (1,1,1) direction.


Here is an example. My initization was done as usual (without using 0 
division) and I also made true three divs are exactly same.


| is larger than the div
|
v
 1757   655   -3   36  4.0
 1790   653   -1   36  4.0
 1858   65   -13   36  4.0
 1891   65   -35   36  4.0
 2968   655   -1   36  4.0
 3064   65   -15   36  4.0
 1791   664   -2   36  4.0
 1824   6620   36  2.0
 1892   66   -24   36  4.0
 3000   6640   36  2.0
 1825   673   -1   36  4.0
 1893   67   -13   36  4.0
 1859   6820   36  2.0

This can not be right. When I checked the new structure file, I found 
symmetso  did not produce a correct structure file. Instead, it reduces the 
number of  symmetry operations.



I would appreciare it if you could give me some hints how to resolve this 
issue.



Thanks a lot!

Best regards,

Guoping
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Re: [Wien] need clarification on changes in spin magnetic moment in cell after SCF run

2013-08-16 Thread tran

Sir, i have seen MMI of all spheres in the given structure. It is observed that 
some of the random spheres have negative moments with different amplitudes and 
the ot
hers have positive magnetic moments of different amplitudes. what sort of 
magnetic nature this indicates...? can we call it as a Non-co-linear magnetic 
structure..?


http://phy.ntnu.edu.tw/~changmc/Teach/SS/SS_note/chap12.pdf___
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Re: [Wien] possible bugs in kgen after SOC

2013-08-16 Thread tran

The k-points in case.klist and the G-vectors in, e.g., case.clmsum are
expressed the same way (cubic). I think that there is no transformation
from cubic to primitive before doing calculations in the code.

F. Tran

On Fri, 16 Aug 2013, Guo-ping Zhang wrote:


Thank you so much, Dr. Tran!

Yes, my test case is fcc.  I also verified that this does not happen for 
orthorhombic structures.


However, do you know whether the wien code internally uses the cubic lattice 
vectors instead of primitive lattice vectors?


It worries me since the klist's division is read into the code many times.

Any comments on this?

Thanks!

Guoping




On Fri, 16 Aug 2013, t...@theochem.tuwien.ac.at wrote:


If your solid has a bcc or fcc unit cell, then it is normal,
since the k points are expressed in terms of the cubic lattice
vectors which are not the primitive ones.

F. Tran

On Thu, 15 Aug 2013, Guo-ping Zhang wrote:



Dear Peter and wien users,

I got a very strange list of k point with kgen after initso (with noaxial 
magnetization say, along (1,1,1) direction.


Here is an example. My initization was done as usual (without using 0 
division) and I also made true three divs are exactly same.


| is larger than the div
|
v
 1757   655   -3   36  4.0
 1790   653   -1   36  4.0
 1858   65   -13   36  4.0
 1891   65   -35   36  4.0
 2968   655   -1   36  4.0
 3064   65   -15   36  4.0
 1791   664   -2   36  4.0
 1824   6620   36  2.0
 1892   66   -24   36  4.0
 3000   6640   36  2.0
 1825   673   -1   36  4.0
 1893   67   -13   36  4.0
 1859   6820   36  2.0

This can not be right. When I checked the new structure file, I found 
symmetso  did not produce a correct structure file. Instead, it reduces 
the number of  symmetry operations.



I would appreciare it if you could give me some hints how to resolve this 
issue.



Thanks a lot!

Best regards,

Guoping
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Re: [Wien] Problem in Band Structue plot in wien2k

2013-08-17 Thread tran

Maybe you forgot to replace 0. by the Fermi energy (:FER in
Mn2FeSi.scf) in Mn2FeSi.insp.

On Sat, 17 Aug 2013, vivek jain wrote:



Dear Sir,


I am running wien2k version on Ubuntu system.
i am calculating for band structure of Mn2FeZ heusler alloys using PBE-GGA 96 
approximation, Rmt*Kmax = 7.0 
i give k-mesh point = 48 
X lapw1 band up  down calculation successfully run. but when using 
Commandline: x spaghetti -up following problem occured. 

Commandline: x spaghetti -up 
Program input is:  

 number of k-points read in case.vector= 111
forrtl: severe (59): list-directed I/O syntax error, unit 5, file 
/home/nrl/WIEN2k/Mn2FeZ/Mn2FeSi/Mn2FeSi.insp
Image  PCRoutineLineSource 
spaghetti  080CECCF  Unknown   Unknown  Unknown

spaghetti  080CD9C5  Unknown   Unknown  Unknown
spaghetti  080A94F1  Unknown   Unknown  Unknown
spaghetti  0809630E  Unknown   Unknown  Unknown
spaghetti  08095B92  Unknown   Unknown  Unknown
spaghetti  08076956  Unknown   Unknown  Unknown
spaghetti  08055B89  inview_32  inview.f
spaghetti  0805B6D2  MAIN__363  spag.f
spaghetti  0804A104  Unknown   Unknown  Unknown
libc.so.6  400A44D3  Unknown   Unknown  Unknown
0.0u 0.0s 0:00.02 100.0% 0+0k 0+48io 0pf+0w
error: command   /home/nrl/WIEN2k/spaghetti upspaghetti.def   failed

Continue with

[FORM]

--
Warm Regards,
Vivek Kumar Jain
09413635180

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Re: [Wien] the c parameter in TB-mBJ

2013-08-22 Thread tran

Hi,

I have not really observed a larger dependence of the mBJ results on the
atomic radii than for a normal GGA calculation.

But, just to remind you:
the more the size of the basis set is large, the less the results will
depend on the choice of the atomic radii RMT.

F. Tran

On Thu, 22 Aug 2013, Fabiana Da Pieve wrote:


Dear Wien2k developers and users

I am running several TB-mBJ calculations to be compared with some GW results 
for organic crystals. My aim is to plug the mBJ .vcould and .r2v into a code for
resonant spectroscopies (if it comes out that mBJ describes well the electronic 
structure of the systems).
The calculations are running and I see that indeed the GGA starting gap is 
*slowly* opening, very good sign. But I also would like to check what Prof. 
Blaha
suggested some time ago, i.e. to use the c parameter from graphite,  as the 
average of gradrho/rho might be ill-defined for my open structures.

Now, for my open structures, I needed to choose a certain radius for the carbon 
atoms, which is different from the one that wien2k was suggesting when I 
constructed
the .struct file from an .xsf file.

So, when I launch the calculation for graphite (in order ot use the resulting 
c parameter also for my open structures), do I have to set the same radius I 
have
chosen for the carbon atoms for my open structures, or leave it as it is chosen 
by Wien2k ?

I think that in the APW method results should be in principle independent on 
the choice of the radius (I hope I am not totally wrong here), but I guess 
somehow it
could influence gradrho/rho.

Thank you very much

Fabiana
VUB, Free University of Brussels

 

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Re: [Wien] Parallel execution of hybrid functional calculation

2013-09-01 Thread tran

I don't really know. Anyway, the execution of the hf module will take
between 1 and 3 orders of magnitude more time than lapw1 and lapw2.
Therefore, to run lapw1 and lapw2 for FBZ in parallel will barely
change the total execution time.

F. Tran

On Sun, 1 Sep 2013, t...@theochem.tuwien.ac.at wrote:


Hi,

Thank you for your quick reply.


No, with hybrid functionals the k-point parallelization is for the
k-points in case.klist_ibz only.

How about the fine-grained parallelization?
I can put the $para to the lines for case.klist_fbz calculations.
Does  this cause some problems?

Shinichi

On 2013/09/01, at 17:31, tran at theochem.tuwien.ac.at wrote:


Hi,

No, with hybrid functionals the k-point parallelization is for the
k-points in case.klist_ibz only.

Another thing:
If you start a hybrid calculation without case.vectorhf,
case.energyhf and case.weighhf in your directory, then in order to
generate these files, during the 1st iteration lapw1 and lapw2 will
be executed one additional time compared to the next iterations.

F. Tran

On Sun, 1 Sep 2013,   wrote:


Dear WIEN2k users,

I am trying to perform the hybrid functionals calculation with
-hf of option like:
$ runsp -hf -p.

The version of WIEN2k is 13.1.

With the -hf execution lapw1 and lapw2 with the FBZ-klist do not run in 

parallel mode,

while the normal runsp runs in parallel mode (MPI/k-point),
I checked the runsp script, and found that
the lines for the calculations with FBZ-klist do not have the $para 

variable.


We can not run the FBZ calculations with any parallel options?

Thanks in advance,

Shinichi Nishimura
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Re: [Wien] Error in mBJGGA

2013-09-03 Thread tran

Hi,

you have probably not selected the correct value for indxc in case.in0 or
case.in0_grr. It should be 28 in case.in0 and 50 in case.in0_grr.
I guess that you did it correctly for 0.25 doping.

F. Tran

On Tue, 3 Sep 2013, Muhammad Sajjad wrote:


Dear Wien2k users

I am am running mBJGGA calculations for ternary alloy. the super cell is of 8 
atoms and doping
is 0.75. For 0.25 doping, the mBJGGA calculations (spin is involved) have 
completed with no
error, but for 0.75 doping the following error is appearing.  


[msajjad@msajjad SCF75]$ runsp_lapw -cc 0.1 -in1new 2 -i 100 -NI
forrtl: severe (24): end-of-file during read, unit 60, file
/home/msajjad/3rdpaper/MgVTe/SCF75/SCF75.inhf
Image              PC                Routine            Line        Source      
       
lapw0              005405AD  Unknown               Unknown  Unknown
lapw0              0053F0B5  Unknown               Unknown  Unknown
lapw0              004DF760  Unknown               Unknown  Unknown
lapw0              0049E7AA  Unknown               Unknown  Unknown
lapw0              0049DFA0  Unknown               Unknown  Unknown
lapw0              004BDE9C  Unknown               Unknown  Unknown
lapw0              00441273  MAIN__                    255  lapw0.F
lapw0              00403BAC  Unknown               Unknown  Unknown
libc.so.6          0034BF01ECDD  Unknown               Unknown  Unknown
lapw0              00403AA9  Unknown               Unknown  Unknown

   stop error


Please help me to overcome this problem.

With thanks
M. Sajjad

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Re: [Wien] Why is the case.inorb file required for use in hybrid functionals

2013-09-04 Thread tran

As DFT+U, the onsite hybrid functionals are implemented in the orb module,
therefore case.inorb is necessary (to specify the fraction of Hartree-Fock
exchange and to which electrons it is applied). But, you don't need to
care about case.inorb and case.indm(c) since they are created
automatically by the script runeece_lapw from case.ineece.

F. Tran

On Wed, 4 Sep 2013, Joshua Davis wrote:


In the user-guide, it states that the case.inorb file is needed when using 
hybrid functionals. (option -eece).  If I am using a hybrid functional, I 
shouldn't need a corrective U.  Is the
case.inorb file just used as place holder to invoke case.indm, the density 
matrix.
Any help would be appreciated.
--
Joshua D. Davis

Graduate Assistant
Department of Chemistry
Michigan State University

578 S. Shaw Lane, room 432

East Lansing, MI 48824
-

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Re: [Wien] L -4

2013-09-12 Thread tran

yes

On Thu, 12 Sep 2013, John Rundgren wrote:


Dear WIEN2k team,
In case.clmsum and case.vcoul one finds designations like
  CLM(R) FOR L  4   M= 4
  CLM(R) FOR L -4   M= 4
Does the second line mean
  CLM(R) FOR L  4   M= -4 ?
John Rundgren / KTH


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Re: [Wien] L -4

2013-09-12 Thread tran

Ah yes. I answered too fast.

On Thu, 12 Sep 2013, Peter Blaha wrote:


No.

We expand the density in real spherical harmonics, which are linear 
combinations ofY_44 +/- Y_4-4  and these two combinations are labeled 
that way.


There are papers by Kurki-Suonio, or see the UG (lapw2).


On 09/12/2013 04:05 PM, John Rundgren wrote:

Dear WIEN2k team,
In case.clmsum and case.vcoul one finds designations like
CLM(R) FOR L  4   M= 4
CLM(R) FOR L -4   M= 4
Does the second line mean
CLM(R) FOR L  4   M= -4 ?
John Rundgren / KTH


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--

 P.Blaha
--
Peter BLAHA, Inst.f. Materials Chemistry, TU Vienna, A-1060 Vienna
Phone: +43-1-58801-165300 FAX: +43-1-58801-165982
Email: bl...@theochem.tuwien.ac.atWWW: http://info.tuwien.ac.at/theochem/
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Re: [Wien] GGA+U

2013-09-15 Thread tran

I can see that your file case.inorb is named Pr3Si1.25Se7.inrob instead
of Pr3Si1.25Se7.inorb. If this is not the problem, maybe you forgot
to use the option -orb when executing runsp_lapw, which means that
your 5 calculations are the same (check if the total energies are the
same or different).

Something not related: I don't understand why your files are called
Pr3Si1.25Se7. Since there are 6 Pr, 4 Si and 14 Se, shouldn't it be
Pr3Si2Se7?

F. Tran

On Sun, 15 Sep 2013, t...@theochem.tuwien.ac.at wrote:


Dear users

I run 5 tests for diffrent values of U parameters in GGA+U for Pr3Si1.25Se7 
but in all cases f state of Pr is on Fermi level and there is no shift. 
Please help me whats wrong with my files. The crystal structure is complex so 
I set two files Pr3Si1.25Se7.indm and also make a copy with name 
Pr3Si1.25Se7.indmc. My input files are given

Pr3Si1.25Se7.struct
Pr3Si1.25Se7
H6173_P63
RELA
19.892777 19.892777 11.413194 90.00 90.00120.00
ATOM  -1: X=0.23711794 Y=0.36583509 Z=0.73076334
 MULT= 6  ISPLIT= 8
 -1: X=0.87128286 Y=0.23711794 Z=0.23076334
 -1: X=0.63416491 Y=0.87128286 Z=0.73076334
 -1: X=0.76288206 Y=0.63416491 Z=0.23076334
 -1: X=0.12871714 Y=0.76288206 Z=0.73076334
 -1: X=0.36583509 Y=0.12871714 Z=0.23076334
Pr NPT=  781  R0=0.1000 RMT=2.   Z:  59.0
LOCAL ROT MATRIX:1.000 0.000 0.000
0.000 1.000 0.000
0.000 0.000 1.000
ATOM  -2: X=0. Y=0. Z=0.12656934
 MULT= 2  ISPLIT= 4
 -2: X=0. Y=0. Z=0.62656934
Si NPT=  781  R0=0.0001 RMT=2.   Z:  14.0
LOCAL ROT MATRIX:1.000 0.000 0.000
0.000 1.000 0.000
0.000 0.000 1.000
ATOM  -3: X=0. Y=0.6667 Z=0.31368149
 MULT= 2  ISPLIT= 4
 -3: X=0.6667 Y=0. Z=0.81368149
Si NPT=  781  R0=0.0001 RMT=2.   Z:  14.0
LOCAL ROT MATRIX:1.000 0.000 0.000
0.000 1.000 0.000
0.000 0.000 1.000
ATOM  -4: X=0. Y=0.6667 Z=0.93548176
 MULT= 2  ISPLIT= 4
 -4: X=0.6667 Y=0. Z=0.43548176
Se NPT=  781  R0=0.5000 RMT=2.   Z:  34.0
LOCAL ROT MATRIX:1.000 0.000 0.000
0.000 1.000 0.000
0.000 0.000 1.000
ATOM  -5: X=0.90744747 Y=0.17074225 Z=0.71763298
 MULT= 6  ISPLIT= 8
 -5: X=0.73670522 Y=0.90744747 Z=0.21763298
 -5: X=0.82925775 Y=0.73670522 Z=0.71763298
 -5: X=0.09255253 Y=0.82925775 Z=0.21763298
 -5: X=0.26329478 Y=0.09255253 Z=0.71763298
 -5: X=0.17074225 Y=0.26329478 Z=0.21763298
Se NPT=  781  R0=0.5000 RMT=2.   Z:  34.0
LOCAL ROT MATRIX:1.000 0.000 0.000
0.000 1.000 0.000
0.000 0.000 1.000
ATOM  -6: X=0.41351132 Y=0.89624471 Z=0.46473424
 MULT= 6  ISPLIT= 8
 -6: X=0.51726661 Y=0.41351132 Z=0.96473424
 -6: X=0.10375529 Y=0.51726661 Z=0.46473424
 -6: X=0.58648868 Y=0.10375529 Z=0.96473424
 -6: X=0.48273339 Y=0.58648868 Z=0.46473424
 -6: X=0.89624471 Y=0.48273339 Z=0.96473424
Se NPT=  781  R0=0.5000 RMT=2.   Z:  34.0
LOCAL ROT MATRIX:1.000 0.000 0.000
0.000 1.000 0.000
0.000 0.000 1.000
  6  NUMBER OF SYMMETRY OPERATIONS
-1 1 0 0.
-1 0 0 0.
0 0 1 0.
  1
0-1 0 0.
1-1 0 0.
0 0 1 0.
  2
1 0 0 0.
0 1 0 0.
0 0 1 0.
  3
1-1 0 0.
1 0 0 0.
0 0 1 0.5000
  4
-1 0 0 0.
0-1 0 0.
0 0 1 0.5000
  5
0 1 0 0.
-1 1 0 0.
0 0 1 0.5000
  6


Pr3Si1.25Se7.indmc
-9.  Emin cutoff energy
1   number of atoms for which density matrix is 
calculated

1  1  3  index of 1st atom, number of L's, L1
0 0   r-index, (l,s)index
Pr3Si1.25Se7.inrob
1  1  0 nmod, natorb, ipr
PRATT  1.0BROYD/PRATT, mixing
 1 1 3  iatom nlorb, lorb
 1  nsic 0..AFM, 1..SIC, 2..HFM
  0.59 0.00U J (Ry)   Note: we recommend to use U_eff = U-J and J=0


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Re: [Wien] restarting the TB-mBJ with a bigger mixing to speed up calculations

2013-09-16 Thread tran

Hi,

to stop a calculation properly you have to create a .stop file
(with touch .stop) in the directory of your calculation. Wien2k
will detect this file and stop the calculation a the end of the current
iteration. Then, modify case.inm and restart the calculation as before.

With mBJ, the energy converges very slowly, but does not diverge.
If you think that :GAP is converged (and this is the only quantity that
you need), maybe you don't really need to converge :ENE.

F. Tran

On Mon, 16 Sep 2013, Fabiana Da Pieve wrote:


Dear Wien2k developers

I have a very simple technical question on TB-mBJ calculations. I
cannot allow myself to make any error as my contract runs only until
the end of the month.

I am running TB-mBJ calculations to be compared with GW. Doing grep
GAP *scf*  inside my TB-mBJ directory, I see that the calculation is
proceeding well, the band gap is increasing, pretty going towards
convergence and pretty going towards the GW result ;
The command I am using for running such calculation is:
run_lapw -p -I -cc 0.001 -ec 0.0001 -it -i 100

I have always obtained good results with such convergence criteria
compared to experiments and to predictions from other (non
all-electron) codes using PAW.

however, if I do  grep :ENE *scf*   in such TB-mBJ directory, the
total energy does not really seems to go towards convergence, or
anyway it is too slow for the remaining time I have (but the energy
does NOT oscillate, or diverge, which is good).


From the usersguide (I am using wien2k-11), I see that it is advised

to change at a certain point from a mixing factor 0.2 (the one I am
using now) to 0.5 (which should increase the speed).

Could you please tell me the DETAILED instructions to abort the
calculation and restart it without breaking ANYTHING (i.e. restarting
safely the calculations with mixing 0.5, from the very last scf step
with mixing 0.2 completed before I kill my calculation) ??

Thank you very much in advance

Fabiana
VUB, Free University of Brussels
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Re: [Wien] restarting the TB-mBJ with a bigger mixing to speed up calculations

2013-09-16 Thread tran

It should be ok.

On Mon, 16 Sep 2013, Fabiana Da Pieve wrote:


Dear Dr. Tran

thank you very much for your answer. Well, I am not only interested in
the gap, I want to check the performance of TB-mBJ also for the width
of the valence and conduction region with respect to GW. So, I want to
calculate the TB-mBJ band structure when my TB-mBJ SCF calculations is
finished, to be compared with the GW band structure obtained by
Wannierization.

So, if I understand well, these are the things I have to do:
- inside my directory touch .stop
- I do not need to send qdel or scancel to the scheduler of my
cluster, the code will detect the .stop file and automatically stops
when the current iteration is finished. Right ?
- When it has stopped, I change the mixing in case.inm to 0.5
- I restart the calculation with my command
 run_lapw -p -I -cc 0.001 -ec 0.0001 -it -i 100

ARE YOU SURE THAT THIS COMMAND DOES NOT NEED ANY MODIFICATION ?
(sorry, but I really cannot allow myself to make any error)

Thank you very much

Fabiana





2013/9/16, t...@theochem.tuwien.ac.at t...@theochem.tuwien.ac.at:

Hi,

to stop a calculation properly you have to create a .stop file
(with touch .stop) in the directory of your calculation. Wien2k
will detect this file and stop the calculation a the end of the current
iteration. Then, modify case.inm and restart the calculation as before.

With mBJ, the energy converges very slowly, but does not diverge.
If you think that :GAP is converged (and this is the only quantity that
you need), maybe you don't really need to converge :ENE.

F. Tran

On Mon, 16 Sep 2013, Fabiana Da Pieve wrote:


Dear Wien2k developers

I have a very simple technical question on TB-mBJ calculations. I
cannot allow myself to make any error as my contract runs only until
the end of the month.

I am running TB-mBJ calculations to be compared with GW. Doing grep
GAP *scf*  inside my TB-mBJ directory, I see that the calculation is
proceeding well, the band gap is increasing, pretty going towards
convergence and pretty going towards the GW result ;
The command I am using for running such calculation is:
run_lapw -p -I -cc 0.001 -ec 0.0001 -it -i 100

I have always obtained good results with such convergence criteria
compared to experiments and to predictions from other (non
all-electron) codes using PAW.

however, if I do  grep :ENE *scf*   in such TB-mBJ directory, the
total energy does not really seems to go towards convergence, or
anyway it is too slow for the remaining time I have (but the energy
does NOT oscillate, or diverge, which is good).


From the usersguide (I am using wien2k-11), I see that it is advised

to change at a certain point from a mixing factor 0.2 (the one I am
using now) to 0.5 (which should increase the speed).

Could you please tell me the DETAILED instructions to abort the
calculation and restart it without breaking ANYTHING (i.e. restarting
safely the calculations with mixing 0.5, from the very last scf step
with mixing 0.2 completed before I kill my calculation) ??

Thank you very much in advance

Fabiana
VUB, Free University of Brussels
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Re: [Wien] gap with hybrid functional

2013-09-18 Thread tran

Hi,

For DOS calculation with full hybrid functionals you need to
execute lapw2 and tetra with -hf:
x lapw2 -qtl -hf (-up/dn)
x tetra -hf (-up/dn)

Maybe this was the problem. This is not explained in the users's guide,
but we will add a paragraph about that soon.

F. Tran

On Wed, 18 Sep 2013, abdel Mar.. wrote:


dear Wien2k community,
i'm interested on the calculation of gap for 4f materials with hybrid 
functional.
(1) with onsite B3PW91
 (2) with full hybrid  B3PW91

for (1)  the value with grep GAP  case.scf  in agreement with  difference 
betwwen (the top) VB 
and (the bottom) of CB in Total DOS plot, also in agrement with expt. value ~ 
3eV

for (2) i have 2 values
 big one with grep GAP in the scf file   ~ 3.4 eV
small from total DOS plot ~ 0.8 eV

can any one tell me please where this difference comes from for the same full 
hybrid functional
and between on site and full hybrid functional?

Regards
 
M.



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Re: [Wien] re-initialization issue with mBJ on reducing RMT

2013-09-26 Thread tran

Hi,

Yes, it is better to reinitialize and run PBEsol again before
switching to mBJ.

F. Tran

On Thu, 26 Sep 2013, Ushma Ahuja wrote:


Dear Wien 2k users,

I am working with Wien2k 12.1 for calculating electronic and optical properties 
of MoTeSe using a 1x1x2 supercell.
Scf convergence with pbe-sol gga was successful and error free (I reduced the 
RMT by 5%) so I proceeded with mBJ calculations.
While running the scf with mBJ potential, I got an error in LAPW1: Select:  No 
energy limit found for atom2, L=0 Select: Ebottom 2.97919, Etop -200.000.
Now I am trying to reduce the RMT more or change the energy between core and 
valence states to rectify this error. 
If I do that, do I need to reinitialize and run pbe sol again and then switch 
to mBJ calc? or can I directly re-initialize in some way for mBJ calc only?

rgds
Ushma Ahuja
ML Sukhadia University
Udaipur, India

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Re: [Wien] Clarification on (a) effective moment including spin-orbit coupling and (b) spin-state configuration

2013-10-02 Thread tran

(i) I don't know Sr2CoO4, but if Co1 and Co2 are inequivalent (e.g., they
have a different environment), then maybe this is not surprising.

(ii) SPIN MAGNETIC MOMENT IN CELL is the number of up-electrons minus the
number of down-electrons.

(iii) You can use instgen_lapw -ask to generate case.inst. Don't
forget, before runsp_lapw - ..., to generate the electron density:
x lstart
x dstart
x dstart -up
x dstart -dn


On Wed, 2 Oct 2013, Kalpana wrote:


Dear wien-users,
   
Using runsp_lapw -so I obtain the converged results for Sr2CoO4 doped with La 
to Sr-site:

With U=4 eV for Co1 and Co2, I obtain their spin-moment as:
:MMI001: MAGNETIC MOMENT IN SPHERE   1    =    1.83531
:MMI002: MAGNETIC MOMENT IN SPHERE   2    =    2.60958

orbital moment as:
:ORB001:  ORBITAL MOMENT:  0.0  0.0  0.81759 PROJECTION ON M  0.81759
:ORB002:  ORBITAL MOMENT:  0.0  0.0  0.76033 PROJECTION ON M  0.76033

total spin-moment in a cell is:
:MMTOT: SPIN MAGNETIC MOMENT IN CELL   = 4.72942


My question here are:

(i) Why Co1 having less spin-moment have larger orbital moment compared to Co2
(ii) When considering the GGA+U+SOC (spin-orbit coupling), I find that the 
results on spin-magnetic moment in a cell
significantly changes with respect to GGA+U.
For example,
With GGA+U  :MMTOT: SPIN MAGNETIC MOMENT IN CELL   = 5.00042
With GGA+U+SOC   :MMTOT: SPIN MAGNETIC MOMENT IN CELL   = 4.72942

Could you please clarify if the SPIN MAGNETIC MOMENT IN CELL with GGA+U+SOC 
calculations is the effective moment or something
else because if we add.

(iii) I also could not understand how to create:
   (a) High-spin configuration
   (b) Intermediate spin configuration
   (c) Low-spin configuration
from the given case.inst for Co atoms. Please help to generate this 
spin-configurations!
For my studied system, the case.inst file of Co atoms looks like:
Co
Ar 3
3, 2,2.0  N
3, 2,2.0  N
3,-3,3.0  N
3,-3,0.0  N
4,-1,1.0  N
4,-1,1.0  N
Co
Ar 3
3, 2,2.0  N
3, 2,2.0  N
3,-3,3.0  N
3,-3,0.0  N
4,-1,1.0  N
4,-1,1.0  N


I need your assistance to resolve these issues...
Thanks
Kalpana

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Re: [Wien] how to start an mBJ after a GGA calculation of the band structure and an unexplicable error

2013-10-02 Thread tran

I don't know what can be the problem in your low parameters
directory, but maybe a clean_lapw or running on another machine
can help.

In your high parameters directory, if case.klist is the proper
file then you can do the preparatory steps for the mBJ as usual.

F. Tran

On Wed, 2 Oct 2013, Fabiana Da Pieve wrote:


Dear Wien2k developers

I am continuing my Tran-Blaha mBJ studies on a series of crystals, and
most of them are proceeding fine (one has finished and compares well
with GW).
However, for one of them, I have a problem. I have two different sets
of calculations for it:

1) one is done with quite high parameters (only at the GGA level) and
it worked fine, I did the usual things (SCF,DOS and band structure).

2) Then I wanted to do the TB-mBJ, and I decided to RE-run (in a
different directory) the preparatory GGA SCF cycle with lower
parameters with respect to case 1). I do not know why, but this time
the GGA runs fails, with the messages in the dayfile and in the error
file that I report below. I have tried to re-initialize the
calculation and re-run the calculation several times, but it always
fails. Why it fails and why before it was working is unexplicable to
me !!

So: I said to myself, ok, let's forget about this low parameters
calculation and let's run the mBJ on the very initial GGA run (with
high parameters). However, in this directory I have calculated, as I
said before, the GGA DOS and the GGA band structure, exactly in this
order. The GGA band structure is done on a different number of k
points with respect to the initial GGA SCF run.

How can I start now an mBJ calculation in this directory ?
Do I have to regenerate the klist file, as it was for the initial GGA
run, and then maybe relaunch lapw1, before doing all the preparatory
steps for the mBJ (i.e. create case.inm_vresp, set r2v in case.in0 and
do run_lapw -NI -i 1) ???
(if you could explain things step by step it would be very helpful for me)

Thank you very much for your help and patience
Fabiana

These are the errors I get for the low parameters GGA SCF run:

in thedayfile:


  lapw2 -p(02:59:27) running LAPW2 in parallel mode

**  LAPW2 crashed!
error: command   /data/home/lamoen/wien2k-11/lapw2para lapw2.def   failed

  stop error


and the message in the error file:

cp: cannot stat `.in.tmp': No such file or directory
rm: cannot remove `.in.tmp': No such file or directory
rm: cannot remove `.in.tmp1': No such file or directory
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Re: [Wien] Clarification on (a) effective moment including spin-orbit coupling and (b) spin-state configuration

2013-10-02 Thread tran

As I said, :MMTOT is the number of up-electrons minus the number of
down-electrons, which obviously means that orbital(L) is not included.

If your system is an insulator, then :MMTOT is an integer
(e.g., :MMTOT=23-18=5), but if it is a metal, then :MMTOT can be
a non-integer (e.g., :MMTOT=22.8-18.2=4.6) because some bands are
only partially filled.


On Wed, 2 Oct 2013, Kalpana wrote:


Dear Prof. Blaha and Tran,    Thanks for your nice comment.
Your reply to my first and third questions in clear now.
However, I am still not clear to my first question.

While performing the calculations for GGA+U and GGA+U+SOC, I obtained solutions 
of total spin-magnetic moemnts as below:
  With GGA+U              :MMTOT: SPIN MAGNETIC MOMENT IN CELL   = 
5.00042
  With GGA+U+SOC   :MMTOT: SPIN MAGNETIC MOMENT IN CELL   =     4.72942

(i) The MMTOT (Spin-magnetic moment) from GGA+U+SOC is 4.72942 not 5.00, which 
I suppose to be same or nearly equal because both
are spin-magnetic moment in cell [without including spin-orbit coupling]. 
So, I am interested to know whether the SPIN MAGNETIC MOMENT in CELL for 
GGA+U+SOC should be read as an effective moment [i.e.
spin(S) + orbital (L)] or something else.
Additionally, if they are the actual SPIN MOMENT in GGA+U+SOC, why are their 
magnitude different with GGA+U because
orbital-moment is not included. 
Can you please clarify my doubt again.
Thanks
Kalpana






On Wed, Oct 2, 2013 at 9:36 PM, Peter Blaha pbl...@theochem.tuwien.ac.at 
wrote:
(ii) When considering the GGA+U+SOC (spin-orbit coupling), I find 
that
the results on spin-magnetic moment in a cell significantly changes 
with
respect to GGA+U.
For example,
With GGA+U              :MMTOT: SPIN MAGNETIC MOMENT IN CELL   =
5.00042
With GGA+U+SOC   :MMTOT: SPIN MAGNETIC MOMENT IN CELL   =     
4.72942


If you did not make any other mistake, it means that without SO you have 
probably an insulating state, while with SO you
got a metal.

  Co
  Ar 3
  3, 2,2.0  N
3, 2,2.0  N   intermediate spin:    low spin
3,-3,3.0  N      2.0                  1.5
3,-3,0.0  N      1.0                  1.5
4,-1,1.0  N
4,-1,1.0  N--


But there is NO guarantee, that these starting configurations yield the desired 
states.

Evendually, you can manually modify the case.dmatup/dn files and run
-orbc   or for a FM you can use runfsm

Peter Blaha
Inst.Materials Chemistry
TU Vienna
Getreidemarkt 9
A-1060 Vienna
Austria
+43-1-5880115671
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Re: [Wien] Error during mBJ calculation

2013-10-10 Thread tran

Hi,

The value in case.grr is the average of (grad rho)/rho in the unit cell.
Apparently some nonsense large value is obtained. Using a smaller mixing
factor in case.inm (e.g., 0.05) may help.

F. Tran

On Thu, 10 Oct 2013, Dileep Krishnan wrote:


Dear users and developers,

I am using mBJ calculation for NiCo2O4 with a mixed spinel and inverse spinel 
structure. The calculation is running fine for more than 20 cycles ( i have 
tried twice) and the stops with the lapw0 error

Error in LAPW0  'LAPW0' - case.grr file not present, which is requred for mBJ

The case.grr file actually is present but without any values but a line of 
asterics! I tried manually creating .grr file by inputting the grr28 value from 
the previous cycle. But when i run scf the line of asterics reappears and the 
program stops. lapw0 runs fine when i type the command 'x lapw0' without 
running 'lapw0 -grr'. I think 'lapw0 -grr' is writing the line of asterics 
corrupting the .grr file which lapw0 cannot read. If anyone knows a solution 
kindly help.

- Dileep Krishnan
 c/o Dr. Ranjan Datta
 JNCASR,
 Jakkur
 Bangalore, India.
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Re: [Wien] RMT

2013-10-15 Thread tran

Hi,

In general, the more the basis set (RMT_min*K_max) is large, the more the
results should be independent of the RMT. But in any case it is strongly
recommended to compare results only when they were obtained with same
parameters (e.g, RMT).

For you case, you can use either the original RMT for the relaxed
structure or the new RMT for the unrelaxed structure.

On Tue, 15 Oct 2013, Salman Zarrini wrote:



Dear Wien2k user,

I would be appreciated if anybody could answer two below questions concerning 
to the muffin-tin radius(RMT):


1. The RMT should be usually reduced for some percent in surface 
relaxation(MSR1a) as we know, however, for a correct comparison of some 
physical properties(surface energy, work function...) between a relaxed and 
unrelaxed surface(to see the relaxation effects), if a new scf should be 
again done for the relaxed one with original RMT?


2. I was wonering if the physical properties (surface energy ...) of two 
different surfaces of a solid, let say Ni3B(110) and Ni3B(101), are 
comparable if different RMT have been used in their calculation?


Best regards,

Salman

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Re: [Wien] charged cell in screened hybrid (YS-PBE0)

2013-10-16 Thread tran

Hi,

Because of the way some loops are constructed it is not possible to
calculate :EXC (exchange-correlation energy) or :AEXSL (exchange-only for
hybrid multiplied by alpha (lapw0 -grr)) when the cell is charged.
Some changes (not extensive) in the code would be necessary. In general it
would be obviously better to have the possibility to run charged cell with
hybrid. I will think about it.

Concerning total energy versus N, in this article it is mentioned (if 
I'm not wrong) that for solids also semilocal functionals show piecewise

linearity:
http://dx.doi.org/10.1103/PhysRevLett.100.146401

F. Tran

On Fri, 11 Oct 2013, Martin Gmitra wrote:


Dear Wien2k users,

I would like to perform charged cell calculations using YS-PBE0 hybrid
functional.
The lapw0 stoped with the message in case.output0_grr file:
Charged cells AND E-tot decomposition not possible

Is there a way to have charged cell calculations? The idea might be not correct,
but I would like to check self-interaction error i.e. plotting total
energy as a function
of charged cell for different portion of Hartree-Fock in order to get
straight lines
connecting N-1, N and N+1 cases (N is the number of valence electrons).
Could you please comment on the idea?

Best regards,
Martin Gmitra
Uni Regensburg
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Re: [Wien] lapw0 hang with mbj calculation for slab

2013-10-18 Thread tran

Hi,

Most likely the problem is due to the Newton iteration procedure in brj.f
which does not stop. Replace this subroutine by the one that I attached
(it is based on an analytical representation of the solution).

By the way, it is nonsense to calculate the average of grad rho/rho when
there is vacuum. So, fix the value of c to the one obtained for the bulk.

F. Tran

On Fri, 18 Oct 2013, alpa dashora wrote:


Dear Prof. Blaha and Wien2k users,
I am trying to run mbj calculation for MoS2 10 layer slab. After few cycles 
lapw0 hanged. I have seen the earlier posts discussed on the same topics. I 
have used the vxclm2.f file as
provided by Prof. Blaha and removed case.in0_grr file. I have also increased 
the Rmt*Kmax up to 9 but still I am not able to solve my problem.

Please suggest any other solution for this error or any other method to 
calculate the correct band gap.

Thanks in advance.

With kind regards,
 
--
Alpa Dashora

  subroutine brj(rho,grho,g2rho,tau,vxbrj,ir)

!A. D. Becke and M. R. Roussel, Phys. Rev. A 39, 3761 (1989).
!A. D. Becke and E. R. Johnson, J. Chem. Phys. 124, 221101 (2006).
!E. Proynov, Z. Gan, and J. Kong, Chem. Phys. Lett. 455, 103 (2008).

  use xcparam 

  implicit real*8(a-h,o-z)

  real*8 :: a(1:3), b(0:5), c(0:5), d(0:5), e(0:5), yp(0:5)

  save iint,isphere
  data iint/0/,isphere/0/
  pi = 4d0*atan(1d0)

  vxbrj = 0d0

  if (rho .gt. 1d-18) then

 tautf = (3d0/10d0)*(3d0*pi**2)**(2d0/3d0)*(2d0*rho)**(5d0/3d0)
 tauw = 0.125d0*grho*grho*2.d0/rho

 if (tau.lt.tauw) then
tau_falsch=tau
tau=tauw
 endif

 if (tau.eq.tauw .and. rho.lt.10.d0.and.ir.lt.900.and.isphere.eq.0) then
print*,'sphere:rho,tauw,grho,g2rho',rho,tau,grho,g2rho,'tauwrong=',tau_falsch
isphere=1
 endif

 if (tau.eq.tauw .and. ir.gt.900.and.iint.lt.10) then
print*,'int:rho,tauw,grho,g2rho',rho,tau,grho,g2rho,'tauwrong=',tau_falsch
iint=iint+1
 endif

 a(1) = 1.5255251812009530d0
 a(2) = 0.4576575543602858d0
 a(3) = 0.4292036732051034d0

 c(0) =   0.7566445420735584d0
 c(1) =  -2.6363977871370960d0
 c(2) =   5.4745159964232880d0
 c(3) = -12.657308127108290d0
 c(4) =   4.1250584725121360d0
 c(5) = -30.425133957163840d0

 b(0) =   0.4771976183772063d0
 b(1) =  -1.7799813494556270d0
 b(2) =   3.8433841862302150d0
 b(3) =  -9.5912050880518490d0
 b(4) =   2.1730180285916720d0
 b(5) = -30.425133851603660d0

 d(0) =0.4435009886795587d0
 d(1) =0.58128653604457910d0
 d(2) =   66.742764515940610d0
 d(3) =  434.26780897229770d0
 d(4) =  824.7765766052239000d0
 d(5) = 1657.9652731582120d0

 e(0) =0.3347285060926091d0
 e(1) =0.47917931023971350d0
 e(2) =   62.392268338574240d0
 e(3) =  463.14816427938120d0
 e(4) =  785.2360350104029000d0
 e(5) = 1657.96296822327300d0

 dd = tau - 0.25d0*grho**2/rho
 q = (g2rho - 1.6d0*dd)/6d0

 if (abs(q) .gt. 1d-18) then

y = (2d0/3d0)*pi**(2d0/3d0)*rho**(5d0/3d0)/q
do i=0, 5
   yp(i) = y**i
enddo

if (y .le. 0d0) then
   g = -atan(a(1)*y + a(2)) + a(3)
   p1 = sum(c(0:5)*yp(0:5))
   p2 = sum(b(0:5)*yp(0:5))
elseif (y .gt. 0d0) then
   z = 2.085749716493756d0*y
   g = log(sqrt(1d0 + 1d0/z**2) + 1d0/z) + 2d0
   p1 = sum(d(0:5)*yp(0:5))
   p2 = sum(e(0:5)*yp(0:5))
endif

if (abs(p2) .gt. 1d-18) then

   x = g*p1/p2

   if (abs(x) .gt. 1d-18) then

  vxbrj = -2d0*pi**(1d0/3d0)*rho**(1d0/3d0)*exp(x/3d0)/x*(1d0 - exp(-x) - 0.5d0*x*exp(-x))

  if (tau .ge. 0d0) then
 vxbrj = xcconst*vxbrj + (3d0*xcconst-2d0)*sqrt(5d0/12d0)/pi*sqrt(tau/rho)
  else
 vxbrj = xcconst*vxbrj - (3d0*xcconst-2d0)*sqrt(5d0/12d0)/pi*sqrt(abs(tau/rho))
  endif

   endif
endif
 endif
  endif

  return
  end
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Re: [Wien] error in mbj

2013-10-21 Thread tran

Hi,

There are one or two reasons why this can happen. Some explanations
are given in pages 207-208 of the user's guide. Maybe they will help
you:
www.wien2k.at/reg_user/textbooks/usersguide.pdf‎

F. Tran

On Sun, 20 Oct 2013, Amine Slassi wrote:


hi,
I made a calcule scf with mbj for a systeme with doping. but i found a
problem in lapw1. the error appears when the scf close to converge.

lapw1.error
'select' - no energy limits found for atom 5 L=1
'select' -E- bottom  -2.32207 E-top -200.000


please help me

cordialy

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Re: [Wien] MPI setup on a multicore maschine

2013-10-22 Thread tran

Hi,

I don't know what is the problem, but I can just say that
in .machines there is no line specific for the HF module.
If lapw1 and lapw2 are run in parallel, then this will be the same for hf.

F. Tran

On Tue, 22 Oct 2013, Martin Gmitra wrote:


Dear Wien2k users,

We are running recent version of Wien2k v13.1 in k-point
parallelization. To perform
screened HF we believe that MPI parallelization would speed up our calculations.
The calculations are intended for test reasons to be run on a local
multicore maschine.

Our .machines file looks like:
lapw0:localhost:4
1:localhost:4
2:localhost:4
hf:localhost:4
granularity:1

Invoking x lapw0 -p
starting parallel lapw0 at Tue Oct 22 09:15:48 CEST 2013
 .machine0 : 4 processors
LAPW0 END
LAPW0 END
LAPW0 END
LAPW0 END
58.2u 0.6s 0:16.92 348.4% 0+0k 0+37528io 21pf+0w

run lapw0 in parallel while
x lapw1 -up -c -p
starting parallel lapw1 at Tue Oct 22 09:18:30 CEST 2013
-  starting parallel LAPW1 jobs at Tue Oct 22 09:18:30 CEST 2013
running LAPW1 in parallel mode (using .machines)
Granularity set to 1
Extrafine unset
@: Expression Syntax.
0.0u 0.0s 0:00.10 10.0% 0+0k 0+64io 0pf+0w
error: command   /temp_local/CODES/WIEN2k_v13_mpi/lapw1cpara -up -c
uplapw1.def   failed

The parallel_options file looks like:
setenv TASKSET no
setenv USE_REMOTE 0
setenv MPI_REMOTE 0
setenv WIEN_GRANULARITY 1

Before starting the tests we load all libs from intel compiler sets WIENROOT and
   export TASKSET=no
   export USE_REMOTE=0
   export MPI_REMOTE=0
   export WIEN_GRANULARITY=1
   export WIEN_MPIRUN=mpirun -np _NP_ -machinefile _HOSTS_ _EXEC_

Do you have any idea while lapw1 does not start?
Many thanks in advance,

Martin Gmitra
Uni Regensburg
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Re: [Wien] Basic question about mbj potential

2013-10-25 Thread tran

Hi,

It has been shown that MBJ yields (very often) band gaps which are in
better agreement with experiment than LDA/PBE for many types of
semiconductors/insulators (sp, Mott-Hubbard, rare gases, ionic), but there
are also a few cases where MBJ does not improve over LDA/PBE.
There is no reason to think that MBJ would not work for systems with
mixed Mott-Hubbard/charge-transfer band gaps. For instance, NiO (whose gap
contains a non-negligible charge-transfer character) is a system for which
MBJ works well. If you look at the papers citing our PRL [Phys. Rev.
Lett. 102, 226401 (2009)], maybe you will find something useful.

F. Tran

On Fri, 25 Oct 2013, shamik chakrabarti wrote:


Dear wien2k users,

     I have a basic question regarding mbj potential. As GGA+U is an useful 
scheme for mott-hubbard type
insulator, similarly, whether acquiring mbj potential is an good approach for 
any types of insulator?.

specifically, whether it is useful for both mott-hubbard and charge-transfer 
type insulator?also if an
insulator/semiconductor posses both mott-hubbard and charge transfer type band 
gaps...whether still mbj is an
useful option?

Please, pardon me, as I have not gone through the basics of mbj yet through any 
lit. survey.

.  
with regards,

--
Shamik Chakrabarti
Senior Research Fellow
Dept. of Physics  Meteorology
Material Processing  Solid State Ionics Lab
IIT Kharagpur
Kharagpur 721302
INDIA

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Re: [Wien] how to derive at interstitial DOS for crystals?

2013-10-27 Thread tran

In case.int you need to add the line
n1   interstitial
where n is the number of inequivalent atoms + 1.

Below this is an example for MoS2:
MoS2
 -0.50 0.002 1.500 0.003  # EMIN, DE, EMAX, Gauss-broadening(de)
 22N   0.000  # NUMBER OF DOS-CASES below, G/L/B broadening (Ry)
01   total# atom, case=column in qtl-header, label
11   Mo-tot
12   Mo-s
13   Mo-p
14   Mo-pz
15   Mo-px+py
16   Mo-d
17   Mo-dz2
18   Mo-dx2y2+dxy
19   Mo-dxz+dyz
1   10   Mo-f
21   S-tot
22   S-s
23   S-p
24   S-pz
25   S-px+py
26   S-d
27   S-dz2
28   S-dx2y2+dxy
29   S-dxz+dyz
2   10   S-f
31   interstitial


On Sun, 27 Oct 2013, Bing Zhou wrote:


Dear all,
Could you please let me know how to get the interstitial DOS map for crystals?
Thank you in advance!
Bing
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Re: [Wien] Refenence for LSDA functional

2013-11-02 Thread tran

indxc=5 corresponds to LSDA with Dirac for exchange and
PW92 [J. P. Perdew and Y. Wang, Phys. Rev. B 45, 13244 (1992)] for
correlation.


On Sat, 2 Nov 2013, sonusha...@iitmandi.ac.in wrote:


Respected Sir
I am using the latest version of WIEN2k_13.1 code. There are different
option for exchange correlation functional. I want to know the reference
for the LSDA functional implemented in this code.

Thanks and regards.
Dr. Sonu Sharma
IIT Mandi (H.P.)
India

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Re: [Wien] band in Hybrid functunal sumhfpara'

2013-11-13 Thread tran

I suppose that it's because there are more atoms in the unit cell for
nanoribbon than for bulk. How many atoms do contain these unit cells?

In general, since hybrid functionals are very expensive it is
recommended to do some tests to search for the lowest values of
the parameters in case.inhf which still leads to the desired accuracy.

On Wed, 13 Nov 2013, ali ghafari wrote:


Dear Tran
Thank you very much for reply.
I'm using 50 K-point for ploting band structure of ZrSe2 bulk
 and nanoribbon. But in the bulk structure run bandplothf lapw is more than 
100 times faster than nanoribbon. the question is why?
Best Regards
Ali


On Wednesday, November 13, 2013 5:00 PM, t...@theochem.tuwien.ac.at 
t...@theochem.tuwien.ac.at wrote:
sumhfpara does not run in parallel simply because this is the program
which merges the vector files case.vectorhf_1, case.vectorhf_2,
etc. created by hf on processors 1, 2, etc.
Anyway, sumhfpara is very fast (a few seconds). This is hf which is very
expensive. How many k-points are you using for plotting band structure?
Maybe you should choose less k-points.

F. Tran

On Tue, 12 Nov 2013, ali ghafari wrote:

 Dear Prof. Blaha
 I'm calculating the band structure by hybrid functional B3LYP. for polting 
band structure as
 discussed on page 53 of UG, we should run run_bandplothf_lapw -p which will 
takes about two weeks
 for a structure with 2 atoms.
  I see,
   lapw1 -band -p
   hf -band -p
   sumhfpara -band -d

 my question is: why 'sumhfpara' can not run on parallel? 
 Best Regards
 Ali



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[Wien] Bug in hybrid functionals with -redklist for metals

2013-11-15 Thread tran

Dear WIEN2k users,

Concerning hybrid functionals (-hf), do not use the option -redklist
for metals since there is a bug in this case. For systems with gap it
is ok.

FT
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Re: [Wien] Exchange-correlation energy

2013-11-26 Thread tran

Hi,

For 1 there is IGRAD.EQ.33 in vxclm2.f which is for exchange-only PBE
(then correlation c is c=xc-x). For such thing the correct procedure is to
plug the PBE orbitals (obtained from an usual PBE calculation) into the
exchange-only PBE:
1) replace 13 by 33 in case.in0
2) x lapw0

I' m not really sure to understand for 2.

For 3 there is the contributions from the spheres and interstitial
in case.output0. This is the 3rd column when you grep for TOTAL=
(the values are in Hartree). This is not really possible to get easily
the contrbution from an arbitrary region of space. A solution
would be to use lapw5 to write on a file the values of exc on a
regaular 3d grid an then integrate yourself. But then the integration
close to the nuclei will be very inaccurate.

One thing: It is dangerous and not recommended to compare two values
of Exc when they were obtained from two different electron densities.

F. Tran


On Tue, 26 Nov 2013, Martin Gmitra wrote:


Dear Wien2k users,

Some time ago there was discussed topic about xc energy
http://www.mail-archive.com/wien@zeus.theochem.tuwien.ac.at/msg01719.html.
Since then Wien2k has KVC flag allowing to print :EXC contribution to
the total energy. Could you please navigate me how:

1. one gets separate exchange and correlation contributions?

2. to get the separate contributions orbital resolved for each atom in the cell?

3. to get the xc contributions in a particular region (say cylinder =
including part of interstitial and muffin-tins) of the cell?

I would like to do it for PBE (option 13).
Thanks in advance for help.
Martin Gmitra
Uni Regensburg
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Re: [Wien] Fixed spin calculations with antiferromagnetic order

2013-11-30 Thread tran

No, it is not possible to fix the spin moment in a sphere. Only the total
spin moment in the unit cell can be fixed.

On Sat, 30 Nov 2013, Alaska Subedi wrote:


Dear Prof. Blaha and others,

Is it possible to do fixed spin moment calculations for
antiferromagnetic order in Wien2k?

Thanks,
Alaska
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Re: [Wien] Fixed spin calculations with antiferromagnetic order

2013-12-01 Thread tran

Related to your question, recently a severe bug in the
script runfsm_lapw was fixed:

The following line has to be removed or commented
if ( $orb2 == -orb ) goto lcore1

F. Tran

On Sat, 30 Nov 2013, Alaska Subedi wrote:


Dear Prof. Blaha and others,

Is it possible to do fixed spin moment calculations for
antiferromagnetic order in Wien2k?

Thanks,
Alaska
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Re: [Wien] Fixed spin calculations with antiferromagnetic order

2013-12-01 Thread tran

Yes, apparently it's only recently (in version 13) that the line was
introduced.


On Sun, 1 Dec 2013, Zhu, Jianxin wrote:


There is no such a line in the runfsm_lapw with version up to 12.1.
Which version are you referring to, 13.1?

Thanks,

Jianxin


On 12/1/13 2:00 AM, t...@theochem.tuwien.ac.at
t...@theochem.tuwien.ac.at wrote:


Related to your question, recently a severe bug in the
script runfsm_lapw was fixed:

The following line has to be removed or commented
if ( $orb2 == -orb ) goto lcore1

F. Tran

On Sat, 30 Nov 2013, Alaska Subedi wrote:


Dear Prof. Blaha and others,

Is it possible to do fixed spin moment calculations for
antiferromagnetic order in Wien2k?

Thanks,
Alaska
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[Wien] Fixed spin calculations with antiferromagnetic order

2013-12-02 Thread tran

Hello all,

Sorry, in a previous e-mail I made a mistake. In fact, this is the line 499

if ( $orb2 == -orb ) goto lcore

which must be deleted. The following line (606) is ok and should NOT be
deleted

if ( $orb2 == -orb ) goto lcore1

Note the difference (lcore versus lcore1). I attached a corrected
script runfsm_lapw. The bug was affecting runfsm_lapw -orb such that the
results were wrong.

F. Tran#!/bin/csh -f
hup
unalias rm

set name  = $0
set bin   = $name:h #directory of WIEN-executables
if !(-d $bin) set bin = .
set name  = $name:t #name of this script-file
set logfile = :log
set tmp   = (:$name)#temporary files

set scratch =   # set directory for vectors and help files
set scratchstring =
if ($?SCRATCH) then  #if envronment SCRATCH is set
 set scratch=`echo $SCRATCH  | sed -e 's/\/$//'`/ #set $scratch to that value  
endif  

#--- functions  subroutines
alias   testinput   'set errin=\!:1;if (! -e \!:1 || -z \!:1) goto \!:2'
alias   teststatus  'if ($status) goto error'
alias   testerror   'if ( -e \!:1.error  ! -z \!:1.error) goto error'
alias   teststop'if (\!:1 == $stopafter ) goto stop'
alias   cleandayfile'grep -v \[ $dayfile .tmp;'\
'mv .tmp $dayfile'
alias   output  'set date = `date +(%T)`;'\
'printf%s\t%s  \!:* $date  $dayfile'

alias   exec'($bin/x  \!:*)  $dayfile;'\
'teststatus'

alias   total_exec  'output \!:*;'\
'exec \!:*;'\
'cleandayfile;'\
'testerror \!:1;'\
'testerror up\!:1;'\
'testerror dn\!:1;'\
'teststop \!:1'
alias   TOTtoFOR'sed s/TOT/FOR/ \!:1  $tmp;'\
'mv $tmp \!:1'
alias   FORtoTOT'sed s/FOR/TOT/ \!:1  $tmp;'\
'mv $tmp \!:1'

#--- default parameters
set ccut= 0.#upper limit for charge convergence
set fcut= 0 #upper limit for force convergence
set ecut= 0.0001#upper limit for energy convergence
unset ec_conv
set cc_conv
set fc_conv
set ec_test
unset ec_test1
unset cc_test
unset fc_test
set iter= 40#maximum number of iterations
set riter   = 99#restart after $riter iterations
set stopafter   #stop after $stopafter
set next#set - start cycle with $next
set qlimit = 0.05   #set - writes E-L in new in1 when qlimit is fulfilled
set in1new = 999
set write_all = -ef # new default: -in1ef is activated (version 10.1)
set para
set nohns
set nohns1 = 0
set it
set readHinv
unset vec2pratt
set it0
set itnum=0
set itnum1=0
set so
set orb
set orb2
set broyd
set eece1
unset eece
unset orbc
unset orbdu
unset dm
set ctest=(0 0 0)
set etest=(0 0 0)

#--- default flags
unset renorm
set   in1orig
unset force #set - force-calculation after self-consistency
unset f_not_conv
unset help  #set - help output
unset complex   #set - complex calculation
unset init  #set - switches initially set to total energy calc.

#--- handling of input options
echo($name) options: $argv$logfile
set commandline=`echo $name $argv  `
alias sb 'shift; breaksw'   #definition used in switch
while ($#argv)
  switch ($1)
  case -[M|m]:
shift; set m = $1; sb
echo $m
  case -[H|h]:
set help; sb
  case -so:
echo 'so not supported with FSM calculations'
exit 3
set so = -so; sb
  case -nohns:
set nohns = -nohns; shift; set nohns1 = $1;sb
  case -dm:
set dm; sb
  case -orb:
set orb2 = -orb
set orb = -orb; sb
  case -orbc:
set orbc
set orb = -orb; sb
  case -hf:
echo '-hf not yet supported with FSM calculations'
exit 3
  case -eece:
echo '-eece not yet supported with FSM calculations'
exit 3
set eece
set eece1 = -eece
set orbc
set orb = -orb; sb
  case -orbdu:
set orbdu
set orb = -orb; sb
  case -it:
set itnum = 99; set it = -it; set it0 = -it; sb
  case -it1:
set itnum = 99; set it = -it; set it0 = -it; touch .noHinv; sb
  case -it2:
set itnum = 99; set it = -it; set it0 = -it; touch .fulldiag; sb
  case -noHinv:
set itnum = 99; set it = -it; set it0 = -it; set readHinv = -noHinv; sb
  case -vec2pratt:
set vec2pratt; sb
  case -p:
set para = -p; sb
  case -I:
set init; sb
  case -NI:
unset broyd; sb
  case -e: 
shift; set stopafter = $1; sb
  case -cc: 
shift; set ccut = $1; set cc_test;unset cc_conv; sb
  case -ec: 
shift; set ecut = $1; set ec_test1;unset ec_conv; sb
  case -fc: 
shift; set f_not_conv; set fcut = $1; set fc_test;unset fc_conv; sb
  case -ql: 
shift; set qlimit = $1;  sb
  case -in1ef: 
set in1new = -1;set write_all = -ef;  sb
  case -in1new: 
shift; set in1new = $1;set

Re: [Wien] Fixed spin calculations with antiferromagnetic order

2013-12-02 Thread tran

No, line 499:
if ( $orb2 == -orb ) goto lcore
which was anyway introduced only recently in WIEN2k_13


On Mon, 2 Dec 2013, Zhu, Jianxin wrote:


Are you meaning the line 489?

Thanks,

Jianxin

-Original Message-

From: t...@theochem.tuwien.ac.at t...@theochem.tuwien.ac.at
Reply-To: A Mailing list for WIEN2k users wien@zeus.theochem.tuwien.ac.at
Date: Monday, December 2, 2013 3:26 AM
To: wien@zeus.theochem.tuwien.ac.at wien@zeus.theochem.tuwien.ac.at
Subject: [Wien]  Fixed spin calculations with antiferromagnetic order


Hello all,

Sorry, in a previous e-mail I made a mistake. In fact, this is the line
499

if ( $orb2 == -orb ) goto lcore

which must be deleted. The following line (606) is ok and should NOT be
deleted

if ( $orb2 == -orb ) goto lcore1

Note the difference (lcore versus lcore1). I attached a corrected
script runfsm_lapw. The bug was affecting runfsm_lapw -orb such that the
results were wrong.

F. Tran


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[Wien] Fixed spin calculations with antiferromagnetic order

2013-12-02 Thread tran

Yes, sorry this is probably line 489 in the version of runfsm_lapw that
you have.


Are you meaning the line 489?

Thanks,

Jianxin

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Re: [Wien] semicore band ranges too large error

2013-12-04 Thread tran

This check was introduced recently to detect ghost bands.
If this problem appears at the very beginning of the SCF iteration
for a new geometry then there is probably no problem of ghost bands.
This is just the starting density which is not good.

To avoid the stop of the calculation, in case.in2 set the value of
iqtlsave to 0.

F. Tran


On Wed, 4 Dec 2013, Torsten Weissbach wrote:


Dear all,

after switching to Wien2k_13, I frequently get the semicore band ranges
too large error, often during relaxation. Though I can understand why
that should not happen, can you explain what could have gone wrong that
it appears and how the source of this error can be traced?

Best regards,
Torsten

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Re: [Wien] RKMAX reduced due to NMATMAX

2013-12-06 Thread tran

grep for :RKM in case.scf

On Fri, 6 Dec 2013, Parker, David S. wrote:


Dear all: I am running a large calculation and got the above error message in 
case.scf, which I presume is due to a limit in param.inc
on the size of the matrix to be diagonalized in lapw1.  Does anyone know where 
I can find the actual RKmax lapw1 used (not the value specified in case.in1)? 
Thanks in advance, David Parker

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Re: [Wien] lapwdm program with B3Pw91 functional

2013-12-07 Thread tran

Hi,

Any value between 0 and 1 for alpha in case.ineece can be chosen.
For your problem with lapwdm I don't really know, but you have to make
sure that:
1) you are running the two SCF calculations with the same and proper
case.indmc
2) you modified case.indmc and not case.indm since apparently your
calculation is complex (-c), which means that this is case.indmc
which is read by WIEN2k

In brief, make sure that case.indmc is always correct.

F. Tran

On Sat, 7 Dec 2013, Majid Yazdani wrote:


 Dear WIEN2k developers and  users
I'm studying a  magnetic case by B3Pw91 hybrid functional.

In the UG B3PW91 is defined as follows:
B3PW91: indxc=18 in case.in0. mode = HYBR and fraction = 0.2 in case.ineece
So I change the indxc to 18 in the case.in0 file
[yazdani@cm6 ]$ cat case.in0
TOT   18    (5:LDA, 13:PBE, 11:WC, 19:PBEsol, 28:mBJ, 29:revTPSS, 46:HTBS)
NR2V  IFFT  (R2V)
  90  90  90    2.00  1    min IFFT-parameters, enhancement factor, iprint
[yazdani@cm6 ]$
and at the first I use alpha=0.2 in my calculations.
[yazdani@cm6 ]$ cat case.ineece
-9.0  2   emin natom
1 1 3 iatom nlorb lorb
2 1 3 iatom nlorb lorb
HYBR  HYBR / EECE mode
0.2  amount of exact exchange
[yazdani@cm6 ]$
then run the program with this command:
runsp_lapw -p -i 900 -so -eece -in1ef -cc 0.1
this is a section of the log
Sat Aug 31 09:26:38 IRDT 2013 (x) lapw0 -p
Sat Aug 31 09:27:58 IRDT 2013 (x) lapw1 -up -p
Sat Aug 31 09:32:24 IRDT 2013 (x) lapw1 -dn -p
Sat Aug 31 09:35:36 IRDT 2013 (x) lapwso -up -orb -p
Sat Aug 31 09:40:09 IRDT 2013 (x) lapw2 -up -p -c -so
Sat Aug 31 09:43:41 IRDT 2013 (x) sumpara -up -d
Sat Aug 31 09:43:42 IRDT 2013 (x) lapw2 -dn -p -c -so
Sat Aug 31 09:46:28 IRDT 2013 (x) sumpara -dn -d
Sat Aug 31 09:46:29 IRDT 2013 (x) lcore -up
Sat Aug 31 09:46:29 IRDT 2013 (x) lcore -dn
   (runeece_lapw) options: -so -p
Sat Aug 31 09:46:29 IRDT 2013 (x) lapwdm -up -p -so -c
Sat Aug 31 09:46:46 IRDT 2013 (x) sumpara -du -d
Sat Aug 31 09:46:46 IRDT 2013 (x) lapw2 -c -up -so -p -eece
Sat Aug 31 09:47:43 IRDT 2013 (x) sumpara -up -eece -d
Sat Aug 31 09:47:43 IRDT 2013 (x) lapw2 -c -dn -so -p -eece
Sat Aug 31 09:48:43 IRDT 2013 (x) sumpara -dn -eece -d
Sat Aug 31 09:48:43 IRDT 2013 (x) lapw0 -p -eece
Sat Aug 31 09:50:23 IRDT 2013 (x) orb -up -p
Sat Aug 31 09:50:24 IRDT 2013 (x) orb -dn -p
Sat Aug 31 09:50:24 IRDT 2013 (x) mixer -eece -orb

after doing calculations with this  alpha parameter I  determine the magnetic 
moment and cotibution of each orbital in it.
so I set the case.indmc as follows with r-index=1 and (l,s)-index=2 for spin 
and (l,s)-index=3 for orbital moment respectively.
then run lapwdm with this command:
 x lapwdm -up -p -so -c
after doing the lapwdm program i extract the results from case.scfdmup

then in order to reduce the HF energy contribution I use alpha=0.1 in the 
case.ineece
[yazdani@cm6 ]$ cat case.ineece
-9.0  2   emin natom
1 1 3 iatom nlorb lorb
2 1 3 iatom nlorb lorb
HYBR  HYBR / EECE mode
0.1  amount of exact exchange
[yazdani@cm6 ]$

and performed calculations with this alpha parameter
runsp_lapw -p -i 900 -so -eece -in1ef -cc 0.1
 this is the log file
Sat Nov 16 15:02:16 IRST 2013 (x) lapw0 -p
Sat Nov 16 15:05:34 IRST 2013 (x) lapw1 -up -p
Sat Nov 16 15:10:02 IRST 2013 (x) lapw1 -dn -p
Sat Nov 16 15:14:28 IRST 2013 (x) lapwso -up -orb -p
Sat Nov 16 15:17:38 IRST 2013 (x) lapw2 -up -p -c -so
Sat Nov 16 15:20:58 IRST 2013 (x) sumpara -up -d
Sat Nov 16 15:20:59 IRST 2013 (x) lapw2 -dn -p -c -so
Sat Nov 16 15:24:17 IRST 2013 (x) sumpara -dn -d
Sat Nov 16 15:24:18 IRST 2013 (x) lcore -up
Sat Nov 16 15:24:18 IRST 2013 (x) lcore -dn
   (runeece_lapw) options: -so -p
Sat Nov 16 15:24:18 IRST 2013 (x) lapwdm -up -p -so -c
Sat Nov 16 15:24:34 IRST 2013 (x) sumpara -du -d
Sat Nov 16 15:24:34 IRST 2013 (x) lapw2 -c -up -so -p -eece
Sat Nov 16 15:27:45 IRST 2013 (x) sumpara -up -eece -d
Sat Nov 16 15:27:45 IRST 2013 (x) lapw2 -c -dn -so -p -eece
Sat Nov 16 15:30:54 IRST 2013 (x) sumpara -dn -eece -d
Sat Nov 16 15:30:54 IRST 2013 (x) lapw0 -p -eece
Sat Nov 16 15:33:58 IRST 2013 (x) orb -up -p
Sat Nov 16 15:33:58 IRST 2013 (x) orb -dn -p
Sat Nov 16 15:33:59 IRST 2013 (x) mixer -eece -orb
Sat Nov 16 15:33:59 IRST 2013 (x) lapw0 -p
 
then I try to drive the orbital contributions in the magnetic moment with 
lapwdm program, similar to previuos calculations.
So  change the case.indmc as follows for orbital moment
[yazdani@cm6 ]$ cat case.indmc
-9.0
1
1 4 0,1,2,3
1 3
[yazdani@cm6 ]$

 But when i open the case.scfdmup see that the portion of all orbitals is zero
[yazdani@cm6 ]$ cat case.scfdmup
 Spin-polarized + s-o calculation, M||  1.000  1.000  1.000
  Calculation of X, X=c*Xr(r)*Xls(l,s)
  Xr(r)    =   I
  Xls(l,s) = L(dzeta)
  c=  1.0
  atom   L    up  dn total
:XOP001  0 0.0 0.0 0.0 0.0
:XOP001  1 0.0 0.0 0.0 0.0
:XOP001  2 0.0

Re: [Wien] hf calculations

2013-12-13 Thread tran

Hi,

For hf calculations the scratch directory needs to be the same as the
working directory. You have to set your SCRATCH as ./

We will change that in the next release of WIEN2k such that hf works also
with another directory for scratch.

F. Tran

On Fri, 13 Dec 2013, Sebastien Petit wrote:


Dear,

I try to use Wien2k + hybrid calculation  on a very simple compound MgO
(obviously, this is a test).

The version of wien2k is : WIEN2k_13.1 (Release 17/6/2013).

i) The DFT calculation seems ok.
 My batch is
#!/bin/bash
 init_lapw -vxc 13 -ecut -6.0  -numk 1000 -b
 run_lapw -ec 0.0001 -NI
exit
 The calculation gives a GAP of 4.764 eV (as in exercice 13 of
http://www.wien2k.at/reg_user/textbooks/WIEN2k_lecture-notes_2013/Exercises_13.pdf)

ii) After a save_lapw, i use the programs init_hf_lapw (with NBAND=12 and a 
4x4x4 k-point mesh without reduction)
and run_lapw -hf -ec 0.0001 -NI and ...
The message are :
LAPW0 END
 LAPW0 END
 LAPW1 END
mv: ne peut évaluer `MgO.vector': Aucun fichier ou répertoire de ce type
 LAPW1 END
mv: ne peut évaluer `MgO.vectorhf_old': Aucun fichier ou répertoire de ce type
FOURIR2 - Error

   stop error


iii) In the log file, I can read :

 (x) lapw0 -grr
 (x) lapw0
 (x) lapw1
 (x) lapw1
 (x) lapw2

In the scratch disk, I find the file  called MgO.vector (generated by the first 
 lapw1). But, i don't
have the MgO.vectorhf file (generated by the second lapw1, yes ? no ?)...


I think it is a very simple mistake, but i can not find it ... --))

Thanks  for your help

Sebastien Petit



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Re: [Wien] NN error

2013-12-21 Thread tran

This is because the atomic spheres overlap. So, you have to choose smaller
spheres radii.

On Sun, 22 Dec 2013, Muhammad Sajjad wrote:


Dear all
I am running optimization with wien2k 12 version. I am facing the following 
error


ERROR status in OPTF123_vol__-5.0
   stop error

NN - Error
 LAPW0 Kindlyhelp me to solve this propblem.

Kind Regards



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Re: [Wien] NN error

2013-12-21 Thread tran

At the beginning of the initiatlization (init_lapw) you are asked to
enter a reduction in %. Choose a larger value than you did before.

More informations here:
http://www.wien2k.at/reg_user/textbooks/usersguide.pdf

On Sat, 21 Dec 2013, Muhammad Sajjad wrote:


Dear Tran,
Thank you so much for your kind response. Please let me know in which file i 
can do the mentioned job? I mean how can i choose smaller spheres readii?


True Regards
Sajjad


On Sat, Dec 21, 2013 at 10:16 PM, t...@theochem.tuwien.ac.at wrote:
  This is because the atomic spheres overlap. So, you have to choose smaller
  spheres radii.

  On Sun, 22 Dec 2013, Muhammad Sajjad wrote:

Dear all
I am running optimization with wien2k 12 version. I am facing the 
following error


ERROR status in OPTF123_vol__-5.0
   stop error

NN - Error
 LAPW0 Kindlyhelp me to solve this propblem.

Kind Regards


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Re: [Wien] Electronic Structure of CoP3

2013-12-31 Thread tran

Hi,
If you can not see in the DOS that your system is metallic, it is probably
because your k-mesh is not dense enough to catch the regions in the
Brillouin zone where the valence and conduction bands overlap.
So, choose more k-points.

F. Tran

On Tue, 31 Dec 2013, Banaras Khan wrote:


Dear WIEN2k Members

I am working on CoP3 skutterudute compound and tried to get the electronic
structure by minimizing the internal parameters.

Bandgap is clearly seen in density of states and from the grep command
but the Bandgap is not there in the Electronic Band

Structure. Please guide me..

   Thanks
   
   Banaras Khan
   University of Malakand, Chakdara, Pakistan. 

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Re: [Wien] band in Hybrid functunal sumhfpara'

2014-01-08 Thread tran

Hi,

Is it really sumhfpara which is not finishing? If this is the case
I don't understand why. Can you send me the files :log and case.dayfile.

Beside this, there is a problem that I am aware of since very recently:
In this article
http://prb.aps.org/abstract/PRB/v87/i16/e165122
it is shown that the method used in WIEN2k to treat the Coulomb
singularity in the unscreened Hartree-Fock exchange (the spherical
truncated method) does not work for cells whose lattice constants are very
different from each other (1 or 2 dimensional systems are the extrem
cases). Look at the green x in Figs. 7 and 8 in this article.
So, I suspect that this problem concerns your calculation on
nanoribbon. In this case it would be better to use a screened hybrid
functional for which there is no problem.

One last thing: Is it necessary to use a 16x16x1 k-mesh for the scf
calculations? I would say that less k-points is probably enough
(and less expensive),

F. Tran

On Wed, 8 Jan 2014, ali ghafari wrote:


Dear Tran
Thank you very much for your advice.
I finish the calculations by B3LYP on Nanoribbon with 16 16 1 k-points. But for 
band structure calculation I have used 20 kpoints at
the in-plane of BZ (i.e. M--Gamma---K---Gamma). now after 2 months the 
'sumhfpara' hasn't finished yet! Which is very surprising
because for SCF it just took about less than one week (on a pc with cpu i7 
930). In the following, you will see the case.outputhf_
which is for scf.
I think, cpu time for scf should be to much more that cpu time for 
run_bandplothf_lapw -p. is it right?
what is your advice?
Best Regards
Ali


cpu time (in sec.) for calc_h:
--
total   :  3812
all before loop ik1 : 0    0%
FFT 1   : 0    0%
alm, blm, clm   : 0    0%
ftmp3a, ftmp3b, ftmp3c  :    17    0%
FFT 2   :    33    1%
qlm, tdd    :    12    0%
FFT 3   :   592   16%
pseudocharge, potential :   552   14%
FFT 4   :   624   16%
Hamiltonian in interstitial :   165    4%
Hamiltonian in spheres 1    : 2    0%
Hamiltonian in spheres 2    :   139    4%
diagonalization and other things    : 0    0%
 
wall time (in sec.) for calc_h:
---
total   :  3986
all before loop ik1 : 0    0%
FFT 1   : 0    0%
alm, blm, clm   : 0    0%
ftmp3a, ftmp3b, ftmp3c  :    18    0%
FFT 2   :    34    1%
qlm, tdd    :    13    0%
FFT 3   :   621   16%
pseudocharge, potential :   577   14%
FFT 4   :   653   16%
Hamiltonian in interstitial :   173    4%
Hamiltonian in spheres 1    : 2    0%
Hamiltonian in spheres 2    :   145    4%
diagonalization and other things    : 0    0%
 
cpu time (in sec.) for hf:
--
total   :  3821
Hamiltonian (calc_h)    :  3812  100%
 
wall time (in sec.) for hf:
---
total   :  3995
Hamiltonian (calc_h)    :  3986  100%


On Thursday, November 14, 2013 8:54 AM, t...@theochem.tuwien.ac.at 
t...@theochem.tuwien.ac.at wrote:
So, I suppose these are the FFTs which take most of the time because of the
large unit cell used for the vacuum. At the end of the files case.outputhf_*
the timing is shown and the values for FFT 3 and FFT 4 should be
much larger than the others.

On Wed, 13 Nov 2013, ali ghafari wrote:

 both structures have 3 atoms. Furthermore, I have selected the same values
 in case.inhf for both structures.



 On Wednesday, November 13, 2013 8:27 PM, t...@theochem.tuwien.ac.at
 t...@theochem.tuwien.ac.at wrote:
 I suppose that it's because there are more atoms in the unit cell for
 nanoribbon than for bulk. How many atoms do contain these unit cells?

 In general, since hybrid functionals are very expensive it is
 recommended to do some tests to search for the lowest values of
 the parameters in case.inhf which still leads to the desired accuracy.

 On Wed, 13 Nov 2013, ali ghafari wrote:

  Dear Tran
  Thank you very much for reply.
  I'm using 50 K-point for ploting band structure of ZrSe2 bulk
   and nanoribbon. But in the bulk structure run bandplothf lapw is more
 than 100

Re: [Wien] pseudo convergence

2014-01-23 Thread tran

If you used the PRATT method with a very small mixing factor, then
the convergence maybe fake. To be sure it's not the case, restart
(after save_lapw) the calculation with the usual (default)
case.inm file.

F. Tran

On Thu, 23 Jan 2014, Lawal Mohammed wrote:


Dear Developers and Users,

Please, how can I know that the mBJ cycle stops at fake convergence?
Any response is appreciated.

With regards
Mohammed Lawal



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Re: [Wien] Not able to stop charge leakage. Tried Reduced RMT/seperation energy

2014-02-03 Thread tran

Hi,

charge leakage means that the radius RMT of the Te atom is not large
enough to accomodate the electron density of the core electrons. So,
you have to increase (and not decrease) RMT to reduce charge leakage.

F. Tran

On Mon, 3 Feb 2014, Naseem Hassan wrote:



Dear Users
I tried to stop the charge leakage although I changed the seperation energy up 
to -10Ry

and also reduced the RMT upto 5%. Both of the actions was not able to prevent 
charge density. Kindly have a look on the information below to understand the 
problem.


 SELECT XCPOT:
  recommended: 13: PBE-GGA (Perdew-Burke-Ernzerhof 96)
5: LSDA
   11: WC-GGA (Wu-Cohen 2006)
   19: PBEsol-GGA (Perdew etal. 2008)
  SELECT ENERGY to separate core and valence states:
  recommended: -6.0 Ry (check how much core charge leaks out of MT-sphere)
  ALTERNATIVELY: specify charge localization
  (between 0.97 and 1.0) to select core state

:WARNING: 0.965  Te   CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy 
:WARNING: ORBITAL:  4P*-8.883-8.883

:WARNING: ORBITAL:  4P -8.169-8.169

:WARNING: 0.965  Te   CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy 
:WARNING: ORBITAL:  4P*-8.883-8.883

:WARNING: ORBITAL:  4P -8.169-8.169
LSTART ENDS
0.167u 0.008s 0:00.17 94.1% 0+0k 0+960io 0pf+0w

Best Reagrds

Naseem 

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Re: [Wien] request

2014-02-06 Thread tran

Hi,

For a parallel calculation (-p), the orbitals energies are printed
in case.energyup_1, case.energyup_2, etc. (the same for dn).


On Thu, 6 Feb 2014, Saleem Ayaz wrote:


Dear users 
 I run the scf for spin polarize calculation of Nd3Si1.25Se7 using GGA+U. 
I used the command runsp_lapw -p -ec 0.1 -orb and converged the energy. The 
calculations
are completed but Nd3Si1.25Se7.energyup and  Nd3Si1.25Se7.energydn are empty. 
Please help me what is the problem.

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Re: [Wien] mBJ calculation stops after 2 cycles

2014-02-06 Thread tran

Hi,

are you sure that the executable wien2k_13/lcore is present?

F

On Thu, 6 Feb 2014, Pascal BOULET wrote:



I forgot to mention that I tried twice the calculation and I got the same 
result. So, it does not seem to be an accidental failure.

Second, I checked the lcore.def file: all the files mentioned in there exist 
and are not empty. It contains the following:

5,'MS.inc', 'old','formatted',0
6,'MS.outputc','unknown','formatted',0
8,'MS.vsp','old','formatted',0
9,'MS.clmcor', 'unknown','formatted',0
19,'MS.vns','unknown','formatted',0
20,'MS.struct',  'old','formatted',0 
21,'MS.scfc',   'unknown','formatted',0

28,'MS.vrespcor',   'unknown','formatted',0
29,'MS.corewf',   'unknown','formatted',0
83,'MS.rsplcore',   'unknown','formatted',0

and the listing of the files returns:

-rw-r--r-- 1 paboulet pmc6881 2.4K 2014-02-05 18:43 MS.struct
-rw-r--r-- 1 paboulet pmc6881  825 2014-02-05 18:45 MS.inc
-rw--- 1 paboulet pmc6881  62K 2014-02-05 23:13 MS.vsp
-rw--- 1 paboulet pmc6881 977K 2014-02-05 23:13 MS.vns
-rw--- 1 paboulet pmc6881  62K 2014-02-05 23:14 MS.vrespcor
-rw--- 1 paboulet pmc6881 1.1K 2014-02-05 23:14 MS.scfc
-rw--- 1 paboulet pmc6881  73K 2014-02-05 23:14 MS.rsplcore
-rw--- 1 paboulet pmc6881 8.6K 2014-02-05 23:14 MS.outputc
-rw--- 1 paboulet pmc6881  160 2014-02-05 23:14 MS.corewf
-rw--- 1 paboulet pmc6881  62K 2014-02-05 23:14 MS.clmcor




From: Lyudmila Dobysheva lyuk...@mail.ru
Sent: Thu Feb 06 07:19:02 CET 2014
To: A Mailing list for WIEN2k users wien@zeus.theochem.tuwien.ac.at
Subject: Re: [Wien] mBJ calculation stops after 2 cycles


On 06.02.2014 03:25, pascal boulet wrote:
 After 2 cycles the job
 stops when starting the lcore program. The dayfile file reads:
 error: command   wien2k_13/lcore lcore.def failed
 The lcore.error file is empty.

Is there an lcore.def file? What it contains?
Make again:
  run_lapw -p -ec 0.0001 -cc 0.01 -i 200 -NI
Does the error repeat in the first or other cycle? If no - that was some 
aсcidental failure, for example, problem with disk, or the like.


If repeats, make in terminal:
x lcore
and see the results.

Best wishes
   Lyudmila Dobysheva
--
Phys.-Techn. Institute of Ural Br. of Russian Ac. of Sci.
426001 Izhevsk, ul.Kirova 132
RUSSIA
--
Tel.:7(3412) 218988(office), 722529(Fax)
E-mail: l...@ftiudm.ru, lyuk...@mail.ru (office)
 lyuk...@gmail.com (home)
Skype:  lyuka17 (home), lyuka18 (office)
http://fti.udm.ru/content/view/25/103/lang,english/
--
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-

Pascal Boulet
Aix-Marseille University 
MADIREL Laboratory

Avenue Normandie-Niemen
13397 Marseille Cedex 20
Email: pascal.bou...@univ-amu.fr
Tel. +33 413 55 18 10
Fax  +33 413 55 18 50
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Re: [Wien] Please help me

2014-02-06 Thread tran

There is no GW module officially included in WIEN2k, but a separate
GW code being developed by Mr. Hong Jiang:
http://www.chem.pku.edu.cn/jianghgroup/codes/fhi-gap.html

Be aware that GW calculations require important computational ressources.

F. Tran

On Thu, 6 Feb 2014, kalsoom Khan wrote:


Dear All
Please some one help me that can i do calculation using GW method in Wien2k.
If yes then how please help me.
with best regards
Kalsoom



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Re: [Wien] electron density plot

2014-02-08 Thread tran

Maybe you need to select an appropriate range of values
for the electron density.

On Sat, 8 Feb 2014, mohamadreza sahmani wrote:


Dear Wien2k developers and users
I want to plot electron density (2D) of a structure by XCrysDen.
After following the procedure given in wien2k user guide, just a
Thermometer Box appears. I want a plot like those depicted in Koller
et al. (2011) [Merits and limits of mBJ exchange potential]
Thanks
Reza Sahmani, University of Mohaghegh, Iran
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Re: [Wien] Hello

2014-02-08 Thread tran

Your question is not very clear. What you have to do is just
1 iteration (-i 1) to generate case.r2v and case.vresp. Then,
when this single iteration is finished follow these steps
1) Save the calculation
2) Make the appropriate changes in case.in0 and case.in0_grr
3) Do the mBJ calculation with, e.g.,  run_lapw -ec 0.0001 -cc 0.0001 -NI

Usually, a mBJ calculation requires many more iterations than conventional
functionals to converge.

On Sat, 8 Feb 2014, moufdi hadjab wrote:



Mr. Moufdi HADJAB
Applied Materials laboratory, departement of Electronic
Universty Djillali Liabes of Sidi Bel Abbes, 22000 Algeria.
Mob: +213 778307600
(E-mail: moufd...@yahoo.fr).
--

Hello dears, I have a problem with mBJ approximation, exactelly in the step of: 
 run one more iteration (use run lapw -NI -i 1) to generate the required
case.r2v and case.vresp files., my question is, how many iterations can I 
start my cycles calculation. 
Best regardless
 


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Re: [Wien] AFM

2014-02-08 Thread tran

Usually, the file case.inso does not need to be changed, except
if you want to choose a particular direction for the magnetization axis,
which is probably not your case.

On Sat, 8 Feb 2014, Karima Karim wrote:


Dear all
I study to get Dos with GGA+U+SO of rare earth métal  ( f orbital) of AmO2  the 
phase Antiferromgnetic  space groupe 221-Pm3m my probleme is I dont' know
complete fichie AmO2.inso 
so , I have ( Am1 , Am2 , O )


WFFIL
 4  1  0  llmax,ipr,kpot
 -10.   1.5   emin,emax (output energy window)
   0.  0.  1. direction of magnetization (lattice vectors)
 NX   number of atoms for which RLO is added
 NX1   -4.97  0.005   atom number,e-lo,de (case.in1), repeat NX times
 0 0 0 0 0    number of atoms for which SO is switch off; atoms
please help me

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Re: [Wien] Avoid leak out of MT sphere with lower RMT values???

2014-02-14 Thread tran

Hi,

during initialization, choose a lower (more negative) core-valence energy
separation such that, eventually, more states will be treated as valence
states. The standard value is -6 Ry, but you can go down to -12 Ry.

F. Tran

On Fri, 14 Feb 2014, Kondaiah Samudrala wrote:


Dear all,
It is known and essential to keep RMTs constant within a series of 
calculations. In the present case, I am doing
mBJ calculations (optimized structures from CASTEP) for AB2 type compound with 
set of pressures ranging from 0
to 100 GPa,  and my A-B distance decreasing drastically. How can I avoid RMT 
problem???

The other thing is, how to avoid leak out of MT sphere with lower RMT values???

Please suggest me some references for choosing RMT's from lower mass to higher 
mass.

Thanks in advance..

with regards
S. Appalakondaiah

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Re: [Wien] orbital occupancy

2014-02-20 Thread tran

In case.scf2 the partial charges are printed (:QTL001, :QTL002, etc.).
These are the number of s, p, etc. electrons inside the atomic sphere
1, 2, etc. But, be aware that in solids, the valence s-electrons are
mainly in the interstitial region.

On Thu, 20 Feb 2014, ali ghafari wrote:


Dear Prof.Blaha and users
I have found out that the number of occupied band can be find in case.scf2.
while I would like to find out orbital occupancy of each atom in the
structure at the end of SCF.  For instance, Cu is 3d9 4s0 or 3d7 4s2. 
I'm using Wien2k_13.1 but I couldn't find such an information in the output
files.
I really appreciate any suggestion.
Best Regards
Ali

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Re: [Wien] band structure error

2014-03-04 Thread tran

It seems that your input file case.insp is not ok.

On Wed, 5 Mar 2014, berber mo wrote:



Dear wien2k community,

I try to calculate band structure with mBJ model installed in wien2K 13.1
with 64 atoms supercell
when I execute x_spaghetti appear this error:
At line 300 of file spag.f (unit = 30, file = 'case.insp')
Fortran runtime error: Bad value during integer read
error:../wien/spaghetti spaghetti.def failed
 best regards,

 
---
---
Berber Mohamed
Applied Materials Laboratory
Research Center
Djillali Liabes University
Sidi Bel Abbes, 22000
Algeria
E-mail:berbermoha...@yahoo.fr
---
-

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Re: [Wien] Need Help please

2014-03-10 Thread tran

Look at page 117 of the UG:
http://www.wien2k.at/reg_user/textbooks/usersguide.pdf

Usually, we don't need to care about Gmax since 12 is good enough in
most cases.

On Mon, 10 Mar 2014, kalsoom Khan wrote:


Dear All
Why we use Gmax=12 in our calculation, Please explain me what it means,
(i.e. i don't know the Gmax)
With regards
kalsoom



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Re: [Wien] Need your help

2014-03-10 Thread tran

yes

On Mon, 10 Mar 2014, kalsoom Khan wrote:


Dear all Please help me
Can we do Spin Orbit Coupling with out spin polarization.
With regards
Kalsoom

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Re: [Wien] something about mbj

2014-03-12 Thread tran

Hi,

In the vast majority of cases, the mBJ potential increases the band gap
with respect to LDA/PBE, and FeO is a case which is metallic with LDA/PBE
but insulator with mBJ. Concerning the band structure in general, it
depends on the case. In many papers you can find comparisons
between LDA/PBE and mBJ band structures. For instance here:

http://journals.aps.org/prb/abstract/10.1103/PhysRevB.82.205102
http://journals.aps.org/prb/abstract/10.1103/PhysRevB.83.195134

F. Tran

On Wed, 12 Mar 2014, nju...@sina.com wrote:



Dear all

I have use the mbj to make the better band gap. The results are consistent with 
experiment.  And my question is that how mbj reform the band structure. whether
it change the hybridization between the band or not? Can mbj change a metal 
into insulator? 

thank you very much! 

best wishes!


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Re: [Wien] mBJ parameters

2014-03-26 Thread tran

Hi,

The parameters A, B and e have to be specified at lines 1, 2 and 3 of
case.in0abp, respectively. If they are present, then they are read
(in free format) and used. If case.in0abp is empty, then the values
a=-0.012, b=1.023, p=0.5 (original mBJ) are used.

F. Tran

On Wed, 26 Mar 2014, nju...@sina.com wrote:



Dear all

I read the paper of David Koller (PRB 85, 155109(2012)), in which he mentioned
that one can set some other mBJ parameters. However, I find, in the user's
guide, that one can define them in case.in0abp. Just put 3 values A,B,e. My
question is that what is the format of the case.in0abp? When I do the mBJ
calculation follow the step in user's guide, I find the empty case.in0abp has
been created. If I add the 3 parameters in the case.in0abp before the mBJ scf
calculation then I is using the new parameters?


best wishes!




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Re: [Wien] so interaction

2014-03-26 Thread tran

Hi,

It is not very clear what you want to do.
The correct procedure is to create case.inorb and case.indm(c) for orb
and execute the script initso_lapw which will create/modify some files.
Then, for spin-polarized systems the calculation is started with
runsp_lapw -orb -so ...


On Wed, 26 Mar 2014, Hemza Kouarta wrote:


Hi ,

I am running wien2k 11 ,i tried tu run so with orb+dm .
i fellow the instruction : i run sp ,then so,then orb , but ,
when i switching to -orb it give me an error in uporb after lapw0 as : 
lapw0 stop error

my struct is hexagonal 2H-NbSe2 doped with Fe,  


2014-03-25 20:17 GMT+01:00 Hemza Kouarta hemzakouarta@gmail.com:
  Hi,

I have qst about sp calculation with so interaction :

If we are able to run sp with so ,and calculating all v element matrix by chanching 
kpot to 1 in case.inso ,why we dont'n have x lapwso -dn ?



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Re: [Wien] Reg; Percentage of hybridization

2014-03-27 Thread tran

Yes, with band-character plotting. The size of a circle is
proportional to the percentage of state of an atom (see Sec. 8.18
in the user's guide).

On Thu, 27 Mar 2014, vijaykumar gudelli wrote:


Dear WIen2k Users,
 Is it possible to calculate the amount (percentage) of hybridization of the
atoms in the band structure?
Specifically, as shown in these paper
https://journals.aps.org/prb/pdf/10.1103/PhysRevB.81.155103

Thanks in advance.

--
-- Regards


VIJAY KUMAR GUDELLI



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Re: [Wien] (no subject)

2014-03-27 Thread tran

Apparently, there is a problem with the file case.dmatup/dn which
contains the density matrix. The 1st thing to do is to check that your
input files case.indm and case.inorb are ok and consistent with each
other.


On Thu, 27 Mar 2014, kalsoom Khan wrote:


Dear All
Please help me
i am doing calculation by using GGA+U, but i get this problem
forrtl: severe (24): end-of-file during read, unit 10, file
/auto/scratch/azam/job_4443022.arien.ics.muni.cz/case/case.dmatup
Image              PC                Routine            Line        Source
orb                004A123A  Unknown               Unknown  Unknown
orb                0049FD36  Unknown               Unknown  Unknown
orb                004540C0  Unknown               Unknown  Unknown
orb                0041C7AF  Unknown               Unknown  Unknown
orb                0041BCB7  Unknown               Unknown  Unknown
orb                0043946E  Unknown               Unknown  Unknown
orb                0040B2C5  init_                     294  init.f
orb                004039F1  MAIN__                    103  main.f
orb                004033DC  Unknown               Unknown  Unknown
libc.so.6          7F2B8AA96C8D  Unknown               Unknown  Unknown
orb                004032D9  Unknown               Unknown  Unknown

Please help me
with regards
kkhan

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Re: [Wien] program for configuration of case.indm and case.inorb

2014-03-27 Thread tran

Hi,

If you want help you need to explain in more details what are your
problems.

F. Tran

On Thu, 27 Mar 2014, paul ivanovich wrote:



Dear Prof. Blaha, 


I have somme problemes regarding my configuration of .inorb and .indm files.

are there a program for that 


many thanks.



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Re: [Wien] Reg; Percentage of hybridization

2014-03-27 Thread tran

You can find this kind of information in case.qtl, where for each
k-point and band, the s, p, d etc. decomposition is written.

On Thu, 27 Mar 2014, vijaykumar gudelli wrote:


Dear Prof. Tran sir,
   Thanks for your kind response sir. Now I got the
relation for the percentage of the hybridization.
   But still I have a small query, how we can
estimate the actual size of the radius, it means the exact percentage of
hybridization?


On Thu, Mar 27, 2014 at 6:03 PM, t...@theochem.tuwien.ac.at wrote:
  Yes, with band-character plotting. The size of a circle is
  proportional to the percentage of state of an atom (see Sec.
  8.18
  in the user's guide).

  On Thu, 27 Mar 2014, vijaykumar gudelli wrote:

Dear WIen2k Users,
 Is it possible to calculate the amount (percentage)
of hybridization of the
atoms in the band structure?
Specifically, as shown in these paper
https://journals.aps.org/prb/pdf/10.1103/PhysRevB.81.155103

Thanks in advance.

--
-- Regards


VIJAY KUMAR GUDELLI




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--
-- Regards


VIJAY KUMAR GUDELLI



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Re: [Wien] Reg: Fixed spin moment calculations

2014-03-29 Thread tran

Yes, this is the correct procedure.

On Sat, 29 Mar 2014, Peram sreenivasa reddy wrote:


Dear WIEN2k,

    I am working on magnetic compound. For my system i got 
total magnetic moment
1.95 bohr magneton. Now i want to do fixed spin moment calculations.

  My quires are
1). To do fixed spin moment calculations, first i have to initiate the 
calculations in spin
polarized case after that i have to give the run command like runfsm_lapw -m 1.95 
-ec 0.01.
Is it correct way or give any suggestions?

2). To check weather this magnetic moment is correct or not i have to take 
different magnetic moment
values like 0.5, 1.0, 1.5, 2.0, 2.5, 3.0. For all the values i have to run scf 
and check the total
energy for each fsm value. After this i have to plot total energy verses 
magnetic moment values. In
this plot where i get the minimum energy for a particular fsm value, that 
magnetic moment value i
should have to consider.
Is this correct procedure?

Please suggest me further.

Thank you very much in advance.




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Re: [Wien] Spin-Orbit

2014-04-14 Thread tran

Hi,

The procedures to apply SOC for spin-polarized and spin-unpolarized
systems are similar:

initso_lapw (initialization)
run(sp)_lapw -so ... (run the calculation)

F. Tran

On Tue, 15 Apr 2014, Riemann Derakhshan wrote:


Dear Wien2k user

I hope You are fine

I want to calculate the Band-structure of Monolayer  silicene in presence of
Spin orbit coupling, But since silicene is not spin polarized material, I want 
to know how
I should run this. You do favour If You give me any detailed guidance.

Sincerely Yours

Riemann

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Re: [Wien] Spin-Orbit

2014-04-14 Thread tran

Now, I understand that your question was about band-structure and not
SCF calculation.

On Mon, 14 Apr 2014, t...@theochem.tuwien.ac.at wrote:


Hi,

The procedures to apply SOC for spin-polarized and spin-unpolarized
systems are similar:

initso_lapw (initialization)
run(sp)_lapw -so ... (run the calculation)

F. Tran

On Tue, 15 Apr 2014, Riemann Derakhshan wrote:


Dear Wien2k user

I hope You are fine

I want to calculate the Band-structure of Monolayer  silicene in presence 
of
Spin orbit coupling, But since silicene is not spin polarized material, I 
want to know how

I should run this. You do favour If You give me any detailed guidance.

Sincerely Yours

Riemann

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Re: [Wien] mBJ gap GaAs

2014-04-15 Thread tran

Hi,

yes, 1.63 eV is the value that you should obtained with mBJ. This value is
in much better agreement with experiment than LDA or PBE, but you should
not expect perfect agreement with experiment. However, by varying
manually the value of c [Eq. (3) of PRL 102, 226401 (2009)] you can get
more or less any value of the band gap that you want (an increase of
c leads to an increase of the band gap). For this, you have
to specify yourself the values of alpha, beta and e in case.in0abp
(c=alpha and choose 0 and 1 for beta and e, respectively).
You can find some explanations at the very end of Sec. 4.5.9 in the user's
guide.

F. Tran

On Tue, 15 Apr 2014, sollebac wrote:


Dear wien2k users, 
Im trying to calculate the gap mBJ  of GaAs as an example following the
user-guide. Everything finished ok  but the value that  I got is 1.63 eV  at 
Gamma,  while the experimental value are  ~1.52 (300K)  and ~1.42 (0K).  How 
can i
get close value to experimental?  i mean how can i converge the value (1.63)  
to get the best value close to experimental?  the k-points are 560 IBZ and is
not-spin-polarized. 
thank in advance. 
Jose Luis              

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Re: [Wien] Need help

2014-04-29 Thread tran

Hi,

Maybe. 34 atoms with WIEN2k is not a cheap calculation. To eventually
speed up the calculation, you have to consider two things:

1) Are you not using parameters (e.g., size of basis set, k-mesh, etc.)
which are set to values that are more than what you really need?
I'm thinking about the k-mesh in particular.

2) The possibility to run your calculation in parallel (with -p).

F. Tran

On Tue, 29 Apr 2014, Ahmed Subhi wrote:


Dear Developers and users,
I am a new user of wien2k, I got a problem, I am running SCF calculation for
7 days, but only four cycles was achieved. Where my compound have 34 atoms.
My question is this normal?
Any response is appreciated.

With regards

    Ahmed Subhi Jbara
   Physics Department
   Science College
 Al-Muthanna University
   Samawah - Iraq


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Re: [Wien] mBJ run stops w/o error message in lapw0

2014-04-29 Thread tran

Hello,

In case you don't know, the mBJ potential can not be applied as such
to systems with infinite vacuum (e.g., isolated molecule, surfaces),
because the average of |grad(rho)|/rho (and therefore the parameter c
in mBJ) is infinite in this case. You have to fix the parameter c
(to the value of bulk ZnO for instance) to avoid this problem
(you can do it by creating manually case.in0abp, see the UG).

For your problem, lapw0 is probably hanging in the brj.f subroutine
because of Newton method. In the next WIEN2k release, brj.f will be
replaced by a new one (attached to this email) without such problem.

So, replace brj.f in SRC_lapw0 and recompile to have new executables
lapw0 and lapw0_mpi. Also, fix the parameter c.

F. Tran


On Tue, 29 Apr 2014, Kamil Klier wrote:

Dear Colleagues,

I am seeking your advice for solving the following problem exemplified
on a model of a Cu-ZnO slab (40 ZnO with one Cu(0) on the slab surface):

After a successful completion of parallel sp -so -orb, the subsequent
mBJ run stops in the lapw0 step within (after completing lapw0_grr
with *.output0_grr completed with no error) which is frozen at the
stage listed below between asterisks:

**
  lapw0 -grr -p   (12:24:46) starting parallel lapw0 at Tue Apr 29
12:24:46 EDT 2014
 .machine0 : processors
running lapw0 in single mode
404.681u 60.392s 7:45.39 99.9%  0+0k 0+0io 0pf+0w

  lapw0 -p(12:32:31) starting parallel lapw0 at Tue Apr 29
12:32:32 EDT 2014

 .machine0 : processors
running lapw0 in single mode
  int:rho,tauw,grho,g2rho  2.824350877551655E-002  6.103772359501373E-004
   8.304021873750874E-003 -5.082098170048767E-002 tauwrong=
  -4.495911213141860E-003
  int:rho,tauw,grho,g2rho  2.825356952954721E-002  6.095285785363750E-004
   8.299724832528738E-003 -5.083964511044604E-002 tauwrong=
  -4.491001032794553E-003
  int:rho,tauw,grho,g2rho  2.706250413726011E-002  1.941298184091310E-003
   1.449639819246514E-002 -4.116294968078159E-002 tauwrong=
  -5.376820894514224E-003
  int:rho,tauw,grho,g2rho  2.707222807780667E-002  1.940275366823992E-003
   1.449518227059034E-002 -4.118138094334088E-002 tauwrong=
  -5.374249039619829E-003
  int:rho,tauw,grho,g2rho  2.509516009055439E-002  3.708033157499589E-003
   1.929286766746054E-002 -2.311418448605970E-002 tauwrong=
  -9.069682710427986E-004
  int:rho,tauw,grho,g2rho  2.510432669330462E-002  3.706885067692818E-003
   1.929340340674948E-002 -2.313235104252417E-002 tauwrong=
  -9.063351511093207E-004
  int:rho,tauw,grho,g2rho  8.029845099838655E-004  5.176735132921631E-004
   1.289470918481737E-003  1.548234958760512E-003 tauwrong=
   4.963361214083710E-004
  int:rho,tauw,grho,g2rho  8.026535824516776E-004  5.174160846724353E-004
   1.24593717297E-003  1.547070346152785E-003 tauwrong=
   4.958243436286073E-004
  int:rho,tauw,grho,g2rho  6.726180563432650E-004  4.323545213751433E-004
   1.078535039428152E-003  1.083803658602449E-003 tauwrong=
   3.060876913841199E-004
  int:rho,tauw,grho,g2rho  6.723607160887903E-004  4.321348107839394E-004
   1.078054675469817E-003  1.082698790040087E-003 tauwrong=
   3.055804491221129E-004
055804491221129E-004


There is no error message - the job just hangs in this state, sometime
in the first mBJ scf cycle, but other times in the n-th mBJ scf cycle
(e.g. n = 7, or even 21).

I have tried to alleviate possible linearization error by adding 1.0
Ry LOs for Cu3d, but with no success.

I am using Wien2k-13.1, running the job at the Brookhaven National Lab
CFN cluster, where we installed and successfully ran many Wien2k jobs,
and can supply additional files for your analysis as needed.  Previous
successful completion of this job prior to mBJ indicates no problem
within the CFN cluster and with our installation parameters. Our use
of -orb is based on experience with pure ZnO, but the present problem
persists with or without running LDA+U.

Any hint/advice/experience would be highly appreciated.

Regards,

Kamil Klier
Lehigh University
e-mail k...@lehigh.edu  subroutine brj(rho,grho,g2rho,tau,vxbrj,ir)

!A. D. Becke and M. R. Roussel, Phys. Rev. A 39, 3761 (1989).
!A. D. Becke and E. R. Johnson, J. Chem. Phys. 124, 221101 (2006).
!E. Proynov, Z. Gan, and J. Kong, Chem. Phys. Lett. 455, 103 (2008).

  use xcparam 

  implicit real*8(a-h,o-z)

  real*8 :: a(1:3), b(0:5), c(0:5), d(0:5), e(0:5), yp(0:5)

  save iint,isphere
  data iint/0/,isphere/0/
  pi = 4d0*atan(1d0)

  vxbrj = 0d0

  if (rho .gt. 1d-18) then

 tautf = (3d0/10d0)*(3d0*pi**2)**(2d0/3d0)*(2d0*rho)**(5d0/3d0)
 tauw = 0.125d0*grho*grho*2.d0/rho

 if (tau.lt.tauw) then
tau_falsch=tau
tau=tauw
 endif

 if (tau.eq.tauw .and. rho.lt.10.d0.and.ir.lt.900

Re: [Wien] (no subject)

2014-05-02 Thread tran

Hi,

the file AmO2.joint is created by the joint package and then used by the
kram package. Did you execute x joint before x kram?

F. Tran

On Fri, 2 May 2014, Karima Karim wrote:


Dear user

I want to calculate the opticle properties of the tetragonal  but I have the
probleme

Invalid null command.
 AmO2.joint

   could not be opened - check def-file
0.0u 0.0s 0:00.00 0.0% 0+0k 0+0io 0pf+0w

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Re: [Wien] file case.klist_band

2014-05-19 Thread tran

In the file inilpw.f (lapw1), case.klist* are read with
 5100 FORMAT(A10,4I5,3F5.2,A3)
for the old format and
 5101 FORMAT(A10,4I10,3F5.2,A3)
for the new format.
So, it means at least 5 digits are allowed.

On Mon, 19 May 2014, Parker, David S. wrote:


Does anyone know if it is possible in the case.klist_band file to include
k vectors consisting of 3 digit numbers, not 1 or 2 (the physical k-point
is divided of course by the overall number, for which 3 digits seems OK)?
I am trying to plot an off-symmetry point feature and need to use a
3-digit k-point identifier. Thanks, David Parker

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Re: [Wien] PW91 exchange-correlation functional indxc in case.in0-reg

2014-05-23 Thread tran

Hi,

As indicated in Sec. 4.5.9 of the user's guide, the purpose of the
LDA or GGA calculation before mBJ is just to create case.r2v and case.vresp
which are necessary for mBJ. It does not matter how converged (in terms
of scf iterations) is this LDA/GGA calculation and which LDA or GGA was
used.

The indices of the functionals are in this file:
$WIENROOT/SRC_lapw0/vxclm2.f

F. Tran

On Fri, 23 May 2014, Yedu Kondalu wrote:


Dear users and experts,

   We are doing electronic structure calculations using Wien2k. In order to get
reliable energy bands for semiconductors/insulators, we are using TB-mBJ 
functional.
To perform TB-mBJ calculations first one has to do scf with standard LDA/GGA
functional and then to continue with TB-mBJ potential. However, GGA consists of
various kinds of parametrization such as PBE (13), PBESol (19), WC (11),  PW91, 
etc.
Now, what is the index number of PW91 in case.in0 file same as other mentioned ?
Shall we do scf calculation with PW91 and continue with TB-mBJ calculations ?

Thanks in advance

Regards
KONDAL

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Re: [Wien] How to get exact 25% doping ?

2014-05-24 Thread tran

It's not possible to get 31 atoms in a 2*2*2 supercell,
unless you manually removed one. I guess it should be 32 in your case.

On Sun, 25 May 2014, Naseem Hassan wrote:


Dear community Fellows

I created a 2*2*2 supercell and got 31 Cd atoms. I want to replace Cd atoms
by Zn atoms so that to get 25% of doping. 25% of 31 atoms is 7.75 which is
not a whole number. How to obtain whole number to get exact 25% of doping ?.

Thank You All
Naseem



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Re: [Wien] warning: !!! Bravais lattice has changed.

2014-05-29 Thread tran

Hi,

you can find some informations in the answers to this question (at the
very bottom of the page):
https://www.mail-archive.com/wien@zeus.theochem.tuwien.ac.at/msg09208.html

On Thu, 29 May 2014, sonusha...@iitmandi.ac.in wrote:


Dear all

In doing the initialization of As element in the trigonal symmetry, space
group number is 166 with
a=b= 3.76 and c=10.5480
alpha and beta = 90 and gamma = 120 (Information from WWW-MINCRYST)
atomic positions are 0.0   0.0   0.226
I am getting warning: !!! Bravais lattice has changed.
Space group has changed to 12 (C 2/m), while I have used 166 (R-3m) space
group.
Why I am getting this error.



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Re: [Wien] Dear Wien2k users and developers

2014-05-29 Thread tran

The problem is that spheres overlap which is forbidden.
I don't think that your case.struct file is ok.
Be aware that the values for a, b and c in case.struct are always in bohr.
unit=ang in case.struct is only for the w2web interface.


On Thu, 29 May 2014, Mian Fayyaz Ahmad wrote:


I am making structure file  of BiFeO3 space group R3 with lattice parameters 
a=b =5.5805 and  c= 13.8763 (Angstrom) with angles alpha= beta = 90 gamma = 120 
(
degree) during initialization i got an error. if i accept gmax value reduces to 
gmin in LSTAR. please help me how can strucure file can be made with above said
space group.

ERROR !!!
 RMT(  3)=2.0 AND RMT(  5)=2.0
 SUMS TO 4.0 GT NNN-DIST= 2.26055

   ERROR !!!
 RMT(  3)=2.0 AND RMT(  3)=2.0
 SUMS TO 4.0 GT NNN-DIST= 2.32636

   ERROR !!!
 RMT(  3)=2.0 AND RMT(  1)=2.0
 SUMS TO 4.0 GT NNN-DIST= 2.34990

   ERROR !!!
 RMT(  3)=2.0 AND RMT(  2)=2.0
 SUMS TO 4.0 GT NNN-DIST= 2.97626

   ERROR !!!
 RMT(  3)=2.0 AND RMT(  6)=2.0
 SUMS TO 4.0 GT NNN-DIST= 3.96941

   ERROR !!!
 RMT(  4)=2.0 AND RMT(  2)=2.0
 SUMS TO 4.0 GT NNN-DIST= 2.34990

   ERROR !!!
 RMT(  4)=2.0 AND RMT(  4)=2.0
 SUMS TO 4.0 GT NNN-DIST= 2.94645

   ERROR !!!
 RMT(  4)=2.0 AND RMT(  1)=2.0
 SUMS TO 4.0 GT NNN-DIST= 2.97626

   ERROR !!!
 RMT(  4)=2.0 AND RMT(  5)=2.0
 SUMS TO 4.0 GT NNN-DIST= 3.13382

   ERROR !!!
 RMT(  5)=2.0 AND RMT(  2)=2.0
 SUMS TO 4.0 GT NNN-DIST= 0.86519

   ERROR !!!
 RMT(  6)=2.0 AND RMT(  3)=2.0
 SUMS TO 4.0 GT NNN-DIST= 3.96941
NN ENDS
0.1u 0.0s 0:00.13 100.0% 0+0k 0+320io 0pf+0w
atom  Z   RMT-max   RMT
 1  83.0  1.20   0.47 
 2  83.0  0.47   0.47 
 3  26.0  1.14   1.14 
 4  26.0  1.14   1.14 
 5   8.0  0.39   0.39 
 6   8.0  1.82   0.39 
Do you want to accept these radii; discard them; or rerun setRmt (a/d/r):

Best Regards Mian Fayyaz AhmadPhD Research Scholar
Magnetophotonics Research Lab.
Department of Physics
Sungkyunkwan University
Suwon,440-746
 Republic of Korea
Cell# +821059295956

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Re: [Wien] (no subject)

2014-05-29 Thread tran

Your RMT spheres are too small, such that there is quite big
core leakage. If possible, choose larger RMT spheres.

On Thu, 29 May 2014, sikandar azam wrote:


Dear ALl
I am doing the initialization and got this problem
13
  SELECT ENERGY to separate core and valence states:
  recommended: -6.0 Ry (check how much core charge leaks out of MT-sphere)
  ALTERNATIVELY: specify charge localization
  (between 0.97 and 1.0) to select core state
-9.8

:WARNING: 0.111  Sr   CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.111  Sr   CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.648  Ce   CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.648  Ce   CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy

:WARNING: 0.021  N    CORE electrons leak out of MT-sphere 
:WARNING: touch .lcore and run scf-cycle with core density superposition
:WARNING: Or: rerun lstart with lower E-core separation energy
LSTART ENDS
1.448u 0.044s 0:07.05 20.9% 0+0k 0+16064io 0pf+0w
ERROR !!! nstop,iter,tets,test 28 1 9.99939225290E-009 nstop,iter,tets,test 
28 1 9.99939225290E-009 nstop,iter,tets,test 28 1 9.99939225290E-009
nstop,iter,tets,test 28 1 9.99939225290E-009 nstop,iter,tets,test 28 1 
9.99939225290E-009 nstop,iter,tets,test 28 1 9.99939225290E-009
nstop,iter,tets,test 28 1 9.99939225290E-009 nstop,iter,tets,test 28 1 
9.99939225290E-009 nstop,iter,tets,test 28 1 9.99939225290E-009
nstop,iter,tets,test 28 1 9.99939225290E-009 nstop,iter,tets,test 28 1 
9.99939225290E-009 nstop,iter,tets,test 28 1 9.99939225290E-009
nstop,iter,tets,test 28 1 9.99939225290E-009 

Re: [Wien] SO coupling and mBJ

2014-05-30 Thread tran

Maybe hybrid functionals, but the problem is that at the moment
SOC can not be used with hybrid functionals.

On Fri, 30 May 2014, Luis Ogando wrote:


Dear Wien2k community,
   I have successfully optimized GaN in the zinc blend phase using LSDA.
After that, I got the band structure using LSDA and mBJ (P-semiconductor
parameters : A=0.267, B=0.656 and e=1).
   I noticed that mBJ significantly improves the band gap, but the SO
splitting goes down from 12meV (LSDA) to 3 meV (mBJ). The experimental value
is about 16 meV.
   Well, I would like to know if there is some way to keep both quantities
well described.
   All the best,
                Luis


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Re: [Wien] SO coupling and mBJ

2014-05-30 Thread tran

Usually the effect does not consist of a rigid shift and in fact, mBJ
does not seem that good for effective masses as shwon in these articles:

http://journals.aps.org/prb/abstract/10.1103/PhysRevB.82.205212
http://iopscience.iop.org/0953-8984/24/20/205503/
http://scitation.aip.org/content/aip/journal/jap/114/18/10.1063/1.4829674


On Fri, 30 May 2014, Luis Ogando wrote:


Dear Tran,
   Thank you for your comment.
   I am interested in extracting kp parameters (effective masses, ...) from
the calculated band structure. Do you believe that the bands can be
significantly deformed in theses results or the main effect should be a
rigid displacement of the bands ?
   All the best,
                    Luis


2014-05-30 13:45 GMT-03:00 t...@theochem.tuwien.ac.at:
  Maybe hybrid functionals, but the problem is that at the moment
  SOC can not be used with hybrid functionals.

  On Fri, 30 May 2014, Luis Ogando wrote:

Dear Wien2k community,
   I have successfully optimized GaN in the zinc
blend phase using LSDA.
After that, I got the band structure using LSDA and
mBJ (P-semiconductor
parameters : A=0.267, B=0.656 and e=1).
   I noticed that mBJ significantly improves the
band gap, but the SO
splitting goes down from 12meV (LSDA) to 3 meV
(mBJ). The experimental value
is about 16 meV.
   Well, I would like to know if there is some way
to keep both quantities
well described.
   All the best,
                Luis



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Re: [Wien] why there is no case.in1c and case.in2c ?

2014-06-06 Thread tran

Hi,

according to my understanding, the box complex calculation (no inversion)
is useless and misleading. One should never select it even if there is no
inversion in the solid. So, do everything without selecting complex 
During initialization, WIEN2k will automatically determine if there is
inversion or not, and create case.in1c and case.in2c if there is no
inversion.

F. Tran

On Fri, 6 Jun 2014, lin chensheng wrote:


Dear users:

       I want to do a no inversion caculation, and I select the complex calculation 
(no inversion)   
 function at the begining session. 
       Then I follow the w2web step by step until to the x dstart function, 
But there is no case.in1c and
case.in2c produced, then the x dstart crashed saying that
       can not found the case.in1c and case.2c files.

      What is wrong? May I simply copy the case.in1_st to case.in1c, and copy 
cast.in2_st to case.in2c. When
I do this and refresh the web,
       it shows the words  complex selected   just under the  x dstart button, and 
the x dstart
calculation can run smoothly.  

       Is it right to do this? How can I produce the case.in1c and case.in2c 
automatically?


Best regards
Chensheng Lin



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Re: [Wien] SCF doesn't run after initso_lap

2014-06-23 Thread tran

Hi,

what do you mean by but it doesn't run? Did the calculation crash?
You have to give more details.

F. Tran

On Mon, 23 Jun 2014, hüsnü kara wrote:


Dear Wien Users,

I did structure optimization and I got regular initialization. I runned the SCF 
calculation for spin poarized case.(runsp_lapw -ec 0.1 -cc 0.1 -Nl -i
50)  I saved the results. Then I used initso_lapw command in terminal:

For large spin orbit effects it might be necessary to include many more
eigenstates from lapw1 by increasing EMAX in case.in1(c).
 
Please enter EMAX(default 5.0 Ryd):
 
The radial basis set for heavy atoms with p-semicore states is very
limited. One can improve this by adding RLOs. Note: you MUST NOT add
RLOs for atoms like oxygen, therefore the default is set to NONE
Add RLO for NONE, ALL, CHOOSE elements? (N/a/c) : c
p-Energy parameters for Sr atom is :
 1   -1.35  0.002 CONT 1
 1    0.30  0.000 CONT 1
 
Would you like to add RLO? (Y/n)Y
p-Energy parameters for Ti atom is :
 1   -2.58  0.002 CONT 1
 1    0.30  0.000 CONT 1
 
Would you like to add RLO? (Y/n)Y
 Check the generated a3.inso file (RLOs,...)
 Check the generated a3.in1 file (Emax at the bottom of the file)

In spinpolarized case SO may reduce symmetry.

The program symmetso dedects the proper symmetry and creates new struct and
input files. (Note, equivalent atoms could become inequivalent in some cases).

Do you have a spinpolarized case (and want to run symmetso) ? (y/N)y
   90.0    90.0    1.57079632679490  T
   1.00   0.000E+000  0.000E+000
  6.123233995736766E-017   1.00   0.000E+000
  6.123233995736766E-017  6.123233995736766E-017   1.00
0.0u 0.0s 0:00.11 81.8% 0+0k 2224+4208io 8pf+0w
 A new structure for SO calculations has been created (_so).
 If you commit it will create new  a3.struct, in1(c), in2c, inc,
 clmsum/up/dn, vspup/dn and vnsup/dn files. (Please SAVE any previous
 calculations)

NOTE: Files for -orb (a3.indm(c),inorb,dmatup/dn) must be adapted manually
Do you want to use the new structure for SO calculations ? (y/N)y

 We run KGEN to generate a new kmesh for the SO calculation:
 
Number of Kpoint in a3.klist is : 1000

Please enter Number of k-points in full BZ (default: 1000):

  NUMBER OF K-POINTS IN WHOLE CELL: (0 allows to specify 3 divisions of G)
 length of reciprocal lattice vectors:   0.843   0.843   0.843  10.000  10.000  
10.000
  Shift of k-mesh allowed. Do you want to shift: (0=no, 1=shift)
  75  k-points generated, ndiv=  10  10  10
KGEN ENDS
Do you want to rerun kgen ? (y/N)N

Spinorbit is now ready to run.

And then I runned the SCF calculation(runsp_lapw -so -ec 0.1 -cc 0.1 
-NI ), but it doesn't run.

Please can you help me?

With regards,

 





--

Hüsnü Kara

Doktora Öğrencisi/ PhD Candidate
Yıldız Teknik Üniversitesi/ Yildiz Technical University
İstanbul / Turkey


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Re: [Wien] got error when use mbj

2014-07-04 Thread tran

Hi,

it is difficult to answer without more information. Is there a message
in lapw0.error?

F. Tran

On Fri, 4 Jul 2014, Tuan Vu wrote:


Hello
I make step by step in user's guide about mbj for zns and got error (last 
command run_lapw -i 80)

start   (Fri Jul  4 15:03:08 MSK 2014) with lapw0 (40/99 to go)

cycle 1 (Fri Jul  4 15:03:08 MSK 2014)  (40/99 to go)

   lapw0 -grr -p(15:03:08) starting parallel lapw0 at Fri Jul  4 15:03:08 
MSK 2014
 .machine0 : processors
running lapw0 in single mode
2.3u 0.0s 0:02.39 99.5% 0+0k 0+1760io 0pf+0w
   lapw0 -p (15:03:11) starting parallel lapw0 at Fri Jul  4 15:03:11 MSK 2014
 .machine0 : processors
running lapw0 in single mode
0.1u 0.0s 0:00.14 92.8% 0+0k 0+472io 0pf+0w
error: command   /home/vutuan/WIEN_13K/lapw0para -c lapw0.def   failed

   stop error
Please help.



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