[Wien] band strucuture for spin polarized case with spin-orbital coupling
stargmoon
stargmoon at yahoo.com
Fri Nov 28 15:14:23 CET 2003
Dear Torsten, Peter, and Andrei,
Thanks a lot for your kindly reply.
Best,
Stargmoon
Torsten Andersen <thor at physik.uni-kl.de> wrote:
Dear Stargmoon,
you can do that by modifying the source code of spaghetti, but you will
have to define what you mean by majority- and minority spin (e.g., 80%
or 90% of the modulus of the wavefunction has spin-up or spin-dn
character) - I do not think it is a well-defined quantity, though,
although it may make some sense in the understanding of the band
structure with spin-orbit interaction.
Best regards,
Torsten Andersen.
stargmoon wrote:
> Dear Wien2k user,
>
> Have you ever used Wien2k to calculate the band structure for spin
> polarized case with spin-orbital coupling?
>
> I did it by following procedure:
> x lapw1 -up
> x lapw1 -dn
> x lapwso -up
> x lapw2 -c -so -qtl -up
> x lapw2 -c -so -qtl -dn
> x spaghetti -up -so
> x spaghetti -dn -so
> Now the problem is, after lapwso, the eigenvalues are stored in file
> "/case.outputso/", because of spin-orbital coupling, we can't
> distinguish up and down spin. How can I get the band structure for up
> and down spin ( or majority and minority spin)?
> By the way, when I tried to run "x spaghetti -up/dn -so", the
> /case.outputsoup/dn /file is required.
>
> How can I do such band structure calculations? Thanks in advance.
>
> Best,
>
> Stargmoon
>
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--
Dr. Torsten Andersen TA-web: http://deep.at/myspace/
AG H#40666;ner, Department of Physics, Kaiserslautern University, and
Condensed Matter Theory Group, Department of Physics, Uppsala University
Web: http://www.fysik4.fysik.uu.se/ http://www.physik.uni-kl.de/
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