Dear Wien2k users,
I am using Wien2k for a Supercell calculation but after making
Supercell the space group is shown to be undefined. But I need to know the
space group. Could anyone please tell me how can I get that space group.
Thank you.
Santu Baidya
India,
kolkata-700098
SNBNCBS
please tell me what is the problem here. Thanks .
Santu Baidya
SRF
SNBNCBS
Material Science
Kolkata-700098
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*"The happiest people do not always have the best of all,* * they simply
appreciate what they find on their way!!!" SANTU
*
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ell but I
could not find such problem. From rhombohedral cell it is mentioned that
lattice parameters should be given in hexagonal units. But is there any
such restrictions over hexagonal unit cell.
Please tell me if there is any solution of this problem.
Thanks in advance.
Santu Baidya
SRF
SNBN
ell but I
could not find such problem. From rhombohedral cell it is mentioned that
lattice parameters should be given in hexagonal units. But is there any
such restrictions over hexagonal unit cell.
Please tell me if there is any solution of this problem.
Thanks in advance.
Santu Baidya
SRF,
SNBN
.
>
> Of course, since you have opted not to provide sufficient information
> about your structure this is just a guess, and could well be wrong. If
> you want sensible responses you MUST provide more information.
>
> On Mon, Feb 11, 2013 at 8:06 AM, Santu Baidya
> wrote:
>
ail: cannot open `+2' for reading: No such file or directory
I have also verified if the error is system dependent or not by doing
calculation on other systems, but I got the same error.
Could anyone please tell me about the problem.
Thanks in advance.
Santu Baidya
SRF, CMPMS,
SNBNCBS,
orbit calculation. But this type of error never
appeared. Could any one please tell me what is the actual reason behind it.
Thanks in advance.
Santu Baidya
SRF,
Material Science Department,
SNBNCBS,
Kolkata-700098
--
*"The happiest people do not always have the best of all,* * they simply
ently asked questions
but I did not get it.
So Could any one please give me the reason for this problem. Thanks in
advance.
Santu Baidya
PhD Student
SNBNCBS
Kolkata-700098
--
*"The happiest people do not always have the best of all,* * they simply
appreciate what they find on their
e mailing list.
>
> Am 24.05.2012 19:10, schrieb Santu Baidya:
>
>> Dear Wien2k users, I am using WIEN2k_07.3 (Release 13/8/2007) for doing
>> GGA+SO calculation on a double perovskite compound A2BB'O6 with P21/n (14
>> No.) spacegroup. I first
>> did a simp
version WIEN2k_12.1 to get the
antiferromagnetic structure.
I do antiferromagnetic calculation by making Co ions inequivalent in
case.struc file.
Thanks in advamce.
Santu Baidya
SRF, CMPMS
SNBNCBS
*"The happiest people do not always have the best of all,* * they simply
appreciate what they fi
Dear Michael Sluydts,
yes I have tried it several times and during "init_lapw" I am getting the
error:
WARNING: Mult not equal. PLEASE CHECK outputnn-file
WARNING: ityp not equal. PLEASE CHECK outputnn-file
WARNING: ityp not equal. PLEASE CHECK outputnn-file
WARNING: ityp not equal. PLEASE CH
ion continued without fat-bands
SPAGH END
0.310u 0.194s 0:00.50 100.0%0+0k 0+14088io 0pf+0w
Can anyone tell me the exact procedure to calculate fatband in relativistic
basis.
Thanks in advance,
Santu Baidya
SRF, SMPMS
SNBNCBS
Kolkata
*"The happiest people do not always have the bes
MULT= 2 ISPLIT=-1
tot,d,d3/2(-3/2),,,d3/2(3/2),(d5/2)(-5/2),d5/2(5/2),
JATOM 4 MULT= 4 ISPLIT= 2
tot,s,p,px,py,pz,
JATOM 5 MULT= 4 ISPLIT= 2
tot,s,p,px,py,pz,
JATOM 6 MULT= 4 ISPLIT= 2 tot,s,p,px,py,pz,
Can any one tell me please if I am missing something.
Thanks.
Santu
.
Could any one please tell me if I have missed anything.
What I am doing is spin-orbit calculation and I want to see fatband
according to J quantum no. as we know l and s quantum no. are not good
quantum no. anymore.
That is the reason I am looking for fatband under |j> basis.
Thanks.
Santu Bai
et fatbands?
Please tell me if I did mistake.
Thanks again.
Santu Baidya
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something. Can you give some suggestion?
Thank you very much,
Santu Baidya
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0.00737
>> 0.7 0.00251 0.00113 0.00203 0.00162 0.00113
>>
>> How can it be possible!!!
>>
>> Am I missing something. Can you give some suggestion?
>>
>> Thank you very much,
>>
>> Santu Baidya
>>
>>
>>
>>
>>
>>
an I learn XMCD calculation in wien2k.
Thanks.
Santu Baidya
SRF, CMPMS
SNBNCBS
Kolkata-700098
*"The happiest people do not always have the best of all,* * they simply
appreciate what they find on their way!!!" SANTU
*
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Respected Sir,
I am using Wien2k package to do SpinOrbit calculation of a
double perovskite compound .I have spin polarised calculation.I have done
exactly same steps to do SO calculation as given in userguide. But at the
end LAPW2 is crashed. In error file it is showing the error--
are
automatically given in case.struct_st file. But I am finding the all unit
matrices in the file. So could you please suggest me anything so that I can
find out m projected density of states with local coordinates. Thanking you.
Santu Baidya
SNBNCBS, JRF
kolkata
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Santu Baidya
JRF
SNBNCBS
KOLKATA
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Dear Wien2k users,
while I am running the init_lapw I am getting an error during
selection of energy to
separate core and valence states. The error is :
SELECT ENERGY to separate core and valence states:
recommended: -6.0 Ry (check how much core charge leaks out of MT-sphere)
-9.2
ST
0.0% 0+0k 0+0io 14pf+0w}
I donot understand what is the difficulty in running if all inputs are
correct. Could u please give me any suggestion to overcome the difficulty.
Thanks.
Santu Baidya
SNBNCBS,JRF
KOLKATA
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still showing the
same error. I am really confused about the problem. Could anyone please help
me to solve the issue.Thanks in advance.
Santu Baidya
SNBNCBS,Kolkata
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Dear wien2k users,
I am using wien2k version "WIEN2k_12.1" to do spin-orbit caluclation with
GGA exchange-correlation functional. Could any one please tell me if it is
possible to get the value of "spin-orbit coupling constant" in wien2k.
Thanks in advance,
Santu Baidy
calculation for trial. But it gives me same "optic crash".
I would like to request you to help me to solve this problem in running
optic program. Is wien2k optic program is unstable for XMCD calculation ?!
Thanking you in advance,
Santu Baidya
University of Duisburg
Germany
__
So please suggest me to know the problem here and solve it.
Thankin you,
Santu Baidya
On 15 May 2015 at 11:59, Peter Blaha wrote:
> You need spin-orbit coupling for xmcd
>
> Am 14.05.2015 um 20:58 schrieb Santu Baidya:
>
>> Dear Prof. Blaha and Wien2k users,
>>
&
Dear Gavin Abo,
Thank you for your suggestions. I shall try this and see if it can remove
the error.
Thanks again,
Santu Baidya
On 15 May 2015 at 20:33, Gavin Abo wrote:
> An additional comment:
>
> I have seen that input conversion error before when IPRINT in case.inc was
&
nc and
case.inc_st files. There is a case.incup file with no data.
Thanking you ,
Santu Baidya
On 18 May 2015 at 12:33, Peter Blaha wrote:
>
> Did you set IPRINT=1 in case.inc (and rerun lcore) ??
>
> Check the content of the file CoO.corewfup
>
>
> -
Dear Prof. Blaha,
Thank you very much Prof. now it works. I did manually x lcore -dn and
now optic run.
Thank you very much for your help.
Thanking you and with regards,
Santu Baidya
On 18 May 2015 at 17:20, Peter Blaha wrote:
> If you look into your own log file, you can see t
in EMCD. As it is possible to get
EELS from telnes3 program. Can it be used for EMCD spectra determination
using wien2k.
Thanking you .
Santu Baidya
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Dear Dr. Gavin Abo,
Thanks for this information.
With regards,
Santu Baidya
On 25 May 2015 at 22:26, Gavin Abo wrote:
> EMCD calculations have been done using WIEN2k [1, 2].
>
> [1] http://arxiv.org/abs/0704.1407v1
> [2] http://www.chiraltem.physics.at/Workshop2_Rusz.pdf
&
case.inop and writes output to
case.symmatup/dn.
Thanks in advance.
Santu Baidya
On 18 May 2015 at 19:36, Peter Blaha wrote:
> I have changed the docu in the UG and do not recommend anymore usage of
> runsp -e lcore.
> Instead the actual necessry sequence of lapw1
userguide it is mentioned that the broadened and unbroadened spectra are
written in files case.xmcd and case.rawxmcd. Please tell me how can i get
these files.
Thanks,
Santu Baidya
On 5 June 2015 at 20:13, Gavin Abo wrote:
> It looks like it is reading the XMCD line in case.inop just f
,
Santu Baidya
University of Duisburg
Germany
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give me completely different results
-metal and insulator.
Please tell me which approach should I accept as solution.
I look forward to get reply.
Thanking you,
Santu Baidya
University of Duisburg-Essen
Duisburg
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Wien
+U+SOC
calculation.
Which gave me two different electronic structure for the same relaxed
structure.
So I have to take lowest energy structure.
Thanking you and regards,
Santu Baidya
On 23 November 2015 at 18:58, Peter Blaha
wrote:
> It is well know that GGA+U calculations can end up
9E-05 % 1.3122E-01 when started from scratch.
So for both cases :MVORD is less than 1% ?
Please enlighten this little more.
Thanking you and with regards,
Santu Baidya
On 23 November 2015 at 19:31, Laurence Marks
wrote:
> Let me add one small thing to what Peter said. Be care
Dear Prof. Laurence Marks,
Thank you very much for your reply. So at the end I would like to ask you
that in my cases :MVORD are less than 1%. So I have to choose lowest energy
case.
Thanking you and with regards,
Santu Baidya
On 23 November 2015 at 20:33, Laurence Marks
wrote:
> W
approx. I can get
band character at 10eV above Fermi level?
I increased the emax in case.in1 to include more bands and calculated
case.qtlup/dn. case.qtlup/dn contains band character only upto valence band
orbital, for example, d orbital.
So please suggest me some way .
Thanking you,
Santu Baidya
spin as a function of k vector information to write?
I look forward to receive your positive help in this regard.
Thanking you and with regards,
Santu Baidya
University of Duisburg-Essen
Germany
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