Dear Prof Ferrer,
You have written that the drawback of the serial version is that it cannot
 plot the SOC band, but you have also mentioned that it can be easily
done..Sir I am asking you can we do that..Because suppose I have done some
work and send it to a journal for publication, now suppose the referee ask
me to plot the band structure including the SOC effect, then I cannot do
anything. So I am requesting you if you do this easy task then I will
surely give your name as an author in my work..Hope to get a response from
you soon...

On Tue, Dec 9, 2014 at 10:49 PM, Jaime Ferrer <[email protected]> wrote:

> My apologies.
> This was intended to be sent to Suman only.
> Jaime Ferrer
>
> El 9/12/2014, a las 18:06, Jaime Ferrer <[email protected]> escribió:
>
> Sure. There goes, together with an afdf file. Cheers,
> Jaime
> <Reservoir-18-Septiembre-2007.zip>
> <Ir copia.fdf>
>
> El 9/12/2014, a las 17:54, Suman Chowdhury <[email protected]>
> escribió:
>
> Dear Prof. Ferrer,
> Can you share your serial version code with me..I am very much interested.
>
> On Tue, Dec 9, 2014 at 10:00 PM, Jaime Ferrer <[email protected]> wrote:
>
>> Dear all,
>>
>> I guess that this string of emails calls for some clarification.
>>
>> The SIESTA team together with myself worked for some time to have the SOC
>> facility implemented
>> into the main trunk, but for a variety of reasons the project never
>> reached the desired end.
>>
>> As a consequence, I have two private versions of SIESTA+SOC that I am
>> happy to share
>> with anyone having a SIESTA license. This comes under an old agreement
>> between
>> the SIESTA authors and me. I believe that perhaps these versions could be
>> made publicly
>> available in the SIESTA Web site, provided that there is a critical mass
>> of plausible users,
>> but this decision is beyond my reach.
>>
>> The two versions have each advantages and disadvantages, that I summarize:
>>
>> 1. Serial version, based on siesta-1.4. This one is fully tested, and
>> works with LDA and GGA,
>> either non-magnetic, collinear magnetic and non-collinear magnetic. It
>> also computes orbital moments.
>> However, as far as I remember, it does not output SOC bands - although it
>> would be easy to fix this.
>>
>> 2. Parallel version, based on a beta release of siesta-3.0. This one is
>> fully tested for LDA: non-magnetic
>> and any sort of collinear and non-collinear magnetic systems. For GGA, it
>> works only for
>> non-magnetic systems. It provides wrong results for non-collinear
>> magnetic systems. This version
>> outputs also bands, DOS and I kind of remember that also wave-functions.
>> Again orbital moments are
>> computed and written.
>>
>> Two warnings are in order now:
>>
>> 1. The SIESTA-SOC version converges slowly, and swallows more RAM
>> resources than
>> conventional simulations.
>>
>> 2. You have to test carefully your pseudopotential parameters, because
>> ghost states may appear.
>>
>> However, a new open-access paper has just appeared where Pablo Rivero,
>> Salvador Barraza-Lopez, myself
>> and collaborators have tested thoroughly the pseudo potentials of 20
>> elements with focus on
>> those having strong SOC -having in mind topological insulators -. We have
>> used for testing the parallel
>> SOC version. We have benchmarked the SIESTA results against VASP and in
>> quite a few cases
>> against an all-electrons code, and the pseudos work quite well.
>>
>> I would advise those interested in SOC to use any of the above two
>> flavors together with the pseudos
>> written down in the paper. The reference to the paper is:
>>
>>  http://www.sciencedirect.com/science/article/pii/S0927025614007940#
>>
>> A last warning: I am no longer maintaining the SIESTA-SOC. What I can
>> hand is what I wrote up to 2009.
>>
>> OK. I guess that this is all for now.
>>
>> With kind regards,
>>
>> Jaime Ferrer
>>
>>
>>
>> El 8/12/2014, a las 18:05, I. Camps <[email protected]> escribió:
>>
>> Hello,
>>
>> Since 2006, in the paper bellow there is an implementation of the
>> spin-orbit coupling in SIESTA. Unfortunately, until now, I didn´t see this
>> implemented in any version of the code.
>>
>> Paper: On-site approximation for spin–orbit coupling in linear
>> combination of atomic orbitals density functional methods, L
>> Fernandez-Seivane, M A Oliveira, S Sanvito and J Ferrer, J. Phys.: Condens.
>> Matter 18 (2006) 7999–8013
>>
>> *Abstract*
>> We propose a computational method that drastically simplifies the
>> inclusion
>> of the spin–orbit interaction in density functional theory when
>> implemented
>> over localized basis sets. Our method is based on a well-known procedure
>> for obtaining pseudopotentials from atomic relativistic *ab initio *
>> calculations
>> and on an on-site approximation for the spin–orbit matrix elements.
>> We have implemented the technique in the SIESTA (Soler J M *et al *2002
>> *J. Phys.: Condens. Matter **14 *2745–79) code, and show that it
>> provides accurate
>> results for the overall band-structure and splittings of group IV and
>> III–IV
>> semiconductors as well as for 5d metals.
>>
>> DOI: http://dx.doi.org/10.1088/0953-8984/18/34/012
>>
>>
>> []'s,
>>
>> @mps
>>
>> On Mon, Dec 8, 2014 at 2:52 PM, Suman Chowdhury <
>> [email protected]> wrote:
>>
>>> Yes, I completely agree with you. As far as I know, spin-orbit coupling
>>> is not included in siesta code. Even I posted about this issue in past in
>>> siesta forum.
>>>
>>> On Mon, Dec 8, 2014 at 10:01 PM, Seyed Mohammad Tabatabaei <
>>> [email protected]> wrote:
>>>
>>>> Dear SIESTA Users,
>>>>
>>>> I want to implement spin orbit coupling for mono-layer MoS2 but as far
>>>> as I know this is not implemented directly in the code. Any help or ideas
>>>> in this regard is appreciated.
>>>>
>>>> Kind regards,
>>>> Mohammad,
>>>>
>>>
>>>
>>>
>>> --
>>>
>>>
>>>
>>> *Senior research fellow Dept. of Physics, University of
>>> Calcutta Kolkata- 700009, West Bengal, India.*
>>> * Ph no-+91-9830512232 <%2B91-9830512232>*
>>>
>>>
>>
>>
>
>
> --
>
>
>
> *Senior research fellow Dept. of Physics, University of Calcutta Kolkata-
> 700009, West Bengal, India.*
> * Ph no-+91-9830512232*
>
>
>
>


-- 



*Senior research fellow Dept. of Physics, University of Calcutta Kolkata-
700009, West Bengal, India.*
* Ph no-+91-9830512232*

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