[SIESTA-L] VACF and PHONON DOS in SIESTA
Dear SIESTA user : Is there any utility program is SIESTA which can calculate the velocity autocorrelation function and the fourier transform of it, because the fourier transform of velocity autocorrelation function gives the phonon density of states which I want to calculate..
[SIESTA-L] PIEZOELECTRIC behavior
Dear all SIESTA users, Does anyone have any idea about how to study the PIEZOELECTRIC behavior of materials by using SIESTA??
Re: [SIESTA-L] Band Structure and PDOS results not matching
Again thank you so so much Prof. Nick Papior On Sun, Feb 4, 2018 at 11:44 PM, Nick Papior <nickpap...@gmail.com> wrote: > I used PDOS from siesta, just as you said you did in your original post. > > 2018-02-04 17:25 GMT+01:00 Suman Chowdhury <sumanchowdhur...@gmail.com>: > >> Just let me know how did you calculate the DOS.. >> >> On Sat, Feb 3, 2018 at 3:04 AM, Nick Papior <nickpap...@gmail.com> wrote: >> >>> Dear Suman, >>> >>> I think you should solve this yourself. >>> >>> 2018-02-02 5:56 GMT+01:00 Suman Chowdhury <sumanchowdhur...@gmail.com>: >>> >>>> Dear Nick Papior, >>>> >>>> Thank you so so much for your help. Can you help me in this regard >>>> about how I can get the correct coordinates for plotting the band >>>> structure?? >>>> >>>> On Thu, Feb 1, 2018 at 3:56 PM, Nick Papior <nickpap...@gmail.com> >>>> wrote: >>>> >>>>> If I run your system without performing cell relaxations I find the >>>>> attached eigenvalues (for the Monkhorst-Pack grid). >>>>> >>>>> In this case there is *only* a bandgab of ~0.5 eV. Provided that the >>>>> cell-relaxation does not change the spectrum drastically then this is what >>>>> you should suspect in the PDOS. >>>>> Secondly, the PDOS is *exactly* reproducing the bandgab in this >>>>> calculation. >>>>> >>>>> 1) I would highly suggest you to perform cell/coordinate relaxations >>>>> in one directory, then afterwards perform analysis on the relaxed >>>>> structure, PDOS, band-structure, optical, etc. >>>>> 2) Possibly your band-structure coordinates are wrong because when I >>>>> plot the bandstructure for this structure it does not capture the correct >>>>> band gab (this *has* to be the problem). >>>>> >>>>> 2018-01-31 16:35 GMT+01:00 Suman Chowdhury <sumanchowdhur...@gmail.com >>>>> >: >>>>> >>>>>> I have just tried to see the variation of TDOS by changing the >>>>>> smearing parameter. But I could not observe any change in it. >>>>>> >>>>>> On Wed, Jan 31, 2018 at 6:44 PM, Suman Chowdhury < >>>>>> sumanchowdhur...@gmail.com> wrote: >>>>>> >>>>>>> This is the fdf that I have used... >>>>>>> >>>>>>> On Thu, Jan 25, 2018 at 11:40 AM, Nick Papior <nickpap...@gmail.com> >>>>>>> wrote: >>>>>>> >>>>>>>> Dear Suman, >>>>>>>> >>>>>>>> Without data (plots) or fdf file it is very difficult to help you. >>>>>>>> It could be that your smearing parameter is too large. >>>>>>>> >>>>>>>> >>>>>>>> 2018-01-24 15:13 GMT+01:00 Suman Chowdhury < >>>>>>>> sumanchowdhur...@gmail.com>: >>>>>>>> >>>>>>>>> Dear SIESTA User, >>>>>>>>> >>>>>>>>> Recently I am getting some confusing results by using SIESTA. >>>>>>>>> While plotting a band structure I am getting a band gap which is quite >>>>>>>>> large. However, when I am trying to plot its corresponding total >>>>>>>>> partial >>>>>>>>> density of states (PDOS), I can clearly see that there is no >>>>>>>>> existence of >>>>>>>>> any band gap. But interestingly the component PDOS are giving the >>>>>>>>> required >>>>>>>>> band gap. The problem is with the total PDOS. Do any of you have any >>>>>>>>> idea >>>>>>>>> about these kinds of results... >>>>>>>>> >>>>>>>>> -- >>>>>>>>> *Dr. Suman Chowdhury* >>>>>>>>> >>>>>>>>> >>>>>>>>> >>>>>>>>> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- >>>>>>>>> 79, West Bengal, India.* >>>>>>>>> >>>>>>>>> >>>>>>>> >>>>>>>> >>>>>>>> -- >>>>>>>> Kind regards Nick >>>>>>>> >>>>>>> >>>>>>> >>>>>>> >>>>>>> -- >>>>>>> *Dr. Suman Chowdhury* >>>>>>> >>>>>>> >>>>>>> >>>>>>> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- >>>>>>> 79, West Bengal, India.* >>>>>>> >>>>>>> >>>>>>> >>>>>> >>>>>> >>>>>> -- >>>>>> *Dr. Suman Chowdhury* >>>>>> >>>>>> >>>>>> >>>>>> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- >>>>>> 79, West Bengal, India.* >>>>>> * Ph no-+91-9830512232 <+91%2098305%2012232>* >>>>>> >>>>>> >>>>> >>>>> >>>>> -- >>>>> Kind regards Nick >>>>> >>>> >>>> >>>> >>>> -- >>>> *Dr. Suman Chowdhury* >>>> >>>> >>>> >>>> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- >>>> 79, West Bengal, India.* >>>> * Ph no-+91-9830512232 <+91%2098305%2012232>* >>>> >>>> >>> >>> >>> -- >>> Kind regards Nick >>> >> >> >> >> -- >> *Dr. Suman Chowdhury* >> >> >> >> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, >> West Bengal, India.* >> * Ph no-+91-9830512232 <+91%2098305%2012232>* >> >> > > > -- > Kind regards Nick > -- *Dr. Suman Chowdhury* *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Band Structure and PDOS results not matching
Just let me know how did you calculate the DOS.. On Sat, Feb 3, 2018 at 3:04 AM, Nick Papior <nickpap...@gmail.com> wrote: > Dear Suman, > > I think you should solve this yourself. > > 2018-02-02 5:56 GMT+01:00 Suman Chowdhury <sumanchowdhur...@gmail.com>: > >> Dear Nick Papior, >> >> Thank you so so much for your help. Can you help me in this regard about >> how I can get the correct coordinates for plotting the band structure?? >> >> On Thu, Feb 1, 2018 at 3:56 PM, Nick Papior <nickpap...@gmail.com> wrote: >> >>> If I run your system without performing cell relaxations I find the >>> attached eigenvalues (for the Monkhorst-Pack grid). >>> >>> In this case there is *only* a bandgab of ~0.5 eV. Provided that the >>> cell-relaxation does not change the spectrum drastically then this is what >>> you should suspect in the PDOS. >>> Secondly, the PDOS is *exactly* reproducing the bandgab in this >>> calculation. >>> >>> 1) I would highly suggest you to perform cell/coordinate relaxations in >>> one directory, then afterwards perform analysis on the relaxed structure, >>> PDOS, band-structure, optical, etc. >>> 2) Possibly your band-structure coordinates are wrong because when I >>> plot the bandstructure for this structure it does not capture the correct >>> band gab (this *has* to be the problem). >>> >>> 2018-01-31 16:35 GMT+01:00 Suman Chowdhury <sumanchowdhur...@gmail.com>: >>> >>>> I have just tried to see the variation of TDOS by changing the smearing >>>> parameter. But I could not observe any change in it. >>>> >>>> On Wed, Jan 31, 2018 at 6:44 PM, Suman Chowdhury < >>>> sumanchowdhur...@gmail.com> wrote: >>>> >>>>> This is the fdf that I have used... >>>>> >>>>> On Thu, Jan 25, 2018 at 11:40 AM, Nick Papior <nickpap...@gmail.com> >>>>> wrote: >>>>> >>>>>> Dear Suman, >>>>>> >>>>>> Without data (plots) or fdf file it is very difficult to help you. >>>>>> It could be that your smearing parameter is too large. >>>>>> >>>>>> >>>>>> 2018-01-24 15:13 GMT+01:00 Suman Chowdhury < >>>>>> sumanchowdhur...@gmail.com>: >>>>>> >>>>>>> Dear SIESTA User, >>>>>>> >>>>>>> Recently I am getting some confusing results by using SIESTA. While >>>>>>> plotting a band structure I am getting a band gap which is quite large. >>>>>>> However, when I am trying to plot its corresponding total partial >>>>>>> density >>>>>>> of states (PDOS), I can clearly see that there is no existence of any >>>>>>> band >>>>>>> gap. But interestingly the component PDOS are giving the required band >>>>>>> gap. >>>>>>> The problem is with the total PDOS. Do any of you have any idea about >>>>>>> these >>>>>>> kinds of results... >>>>>>> >>>>>>> -- >>>>>>> *Dr. Suman Chowdhury* >>>>>>> >>>>>>> >>>>>>> >>>>>>> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- >>>>>>> 79, West Bengal, India.* >>>>>>> >>>>>>> >>>>>> >>>>>> >>>>>> -- >>>>>> Kind regards Nick >>>>>> >>>>> >>>>> >>>>> >>>>> -- >>>>> *Dr. Suman Chowdhury* >>>>> >>>>> >>>>> >>>>> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- >>>>> 79, West Bengal, India.* >>>>> >>>>> >>>>> >>>> >>>> >>>> -- >>>> *Dr. Suman Chowdhury* >>>> >>>> >>>> >>>> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- >>>> 79, West Bengal, India.* >>>> * Ph no-+91-9830512232 <+91%2098305%2012232>* >>>> >>>> >>> >>> >>> -- >>> Kind regards Nick >>> >> >> >> >> -- >> *Dr. Suman Chowdhury* >> >> >> >> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, >> West Bengal, India.* >> * Ph no-+91-9830512232 <+91%2098305%2012232>* >> >> > > > -- > Kind regards Nick > -- *Dr. Suman Chowdhury* *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Band Structure and PDOS results not matching
Dear Nick Papior, Thank you so so much for your help. Can you help me in this regard about how I can get the correct coordinates for plotting the band structure?? On Thu, Feb 1, 2018 at 3:56 PM, Nick Papior <nickpap...@gmail.com> wrote: > If I run your system without performing cell relaxations I find the > attached eigenvalues (for the Monkhorst-Pack grid). > > In this case there is *only* a bandgab of ~0.5 eV. Provided that the > cell-relaxation does not change the spectrum drastically then this is what > you should suspect in the PDOS. > Secondly, the PDOS is *exactly* reproducing the bandgab in this > calculation. > > 1) I would highly suggest you to perform cell/coordinate relaxations in > one directory, then afterwards perform analysis on the relaxed structure, > PDOS, band-structure, optical, etc. > 2) Possibly your band-structure coordinates are wrong because when I plot > the bandstructure for this structure it does not capture the correct band > gab (this *has* to be the problem). > > 2018-01-31 16:35 GMT+01:00 Suman Chowdhury <sumanchowdhur...@gmail.com>: > >> I have just tried to see the variation of TDOS by changing the smearing >> parameter. But I could not observe any change in it. >> >> On Wed, Jan 31, 2018 at 6:44 PM, Suman Chowdhury < >> sumanchowdhur...@gmail.com> wrote: >> >>> This is the fdf that I have used... >>> >>> On Thu, Jan 25, 2018 at 11:40 AM, Nick Papior <nickpap...@gmail.com> >>> wrote: >>> >>>> Dear Suman, >>>> >>>> Without data (plots) or fdf file it is very difficult to help you. >>>> It could be that your smearing parameter is too large. >>>> >>>> >>>> 2018-01-24 15:13 GMT+01:00 Suman Chowdhury <sumanchowdhur...@gmail.com> >>>> : >>>> >>>>> Dear SIESTA User, >>>>> >>>>> Recently I am getting some confusing results by using SIESTA. While >>>>> plotting a band structure I am getting a band gap which is quite large. >>>>> However, when I am trying to plot its corresponding total partial density >>>>> of states (PDOS), I can clearly see that there is no existence of any band >>>>> gap. But interestingly the component PDOS are giving the required band >>>>> gap. >>>>> The problem is with the total PDOS. Do any of you have any idea about >>>>> these >>>>> kinds of results... >>>>> >>>>> -- >>>>> *Dr. Suman Chowdhury* >>>>> >>>>> >>>>> >>>>> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- >>>>> 79, West Bengal, India.* >>>>> >>>>> >>>> >>>> >>>> -- >>>> Kind regards Nick >>>> >>> >>> >>> >>> -- >>> *Dr. Suman Chowdhury* >>> >>> >>> >>> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- >>> 79, West Bengal, India.* >>> >>> >>> >> >> >> -- >> *Dr. Suman Chowdhury* >> >> >> >> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, >> West Bengal, India.* >> * Ph no-+91-9830512232 <+91%2098305%2012232>* >> >> > > > -- > Kind regards Nick > -- *Dr. Suman Chowdhury* *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Band Structure and PDOS results not matching
I have just tried to see the variation of TDOS by changing the smearing parameter. But I could not observe any change in it. On Wed, Jan 31, 2018 at 6:44 PM, Suman Chowdhury <sumanchowdhur...@gmail.com > wrote: > This is the fdf that I have used... > > On Thu, Jan 25, 2018 at 11:40 AM, Nick Papior <nickpap...@gmail.com> > wrote: > >> Dear Suman, >> >> Without data (plots) or fdf file it is very difficult to help you. >> It could be that your smearing parameter is too large. >> >> >> 2018-01-24 15:13 GMT+01:00 Suman Chowdhury <sumanchowdhur...@gmail.com>: >> >>> Dear SIESTA User, >>> >>> Recently I am getting some confusing results by using SIESTA. While >>> plotting a band structure I am getting a band gap which is quite large. >>> However, when I am trying to plot its corresponding total partial density >>> of states (PDOS), I can clearly see that there is no existence of any band >>> gap. But interestingly the component PDOS are giving the required band gap. >>> The problem is with the total PDOS. Do any of you have any idea about these >>> kinds of results... >>> >>> -- >>> *Dr. Suman Chowdhury* >>> >>> >>> >>> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- >>> 700009, West Bengal, India.* >>> >>> >> >> >> -- >> Kind regards Nick >> > > > > -- > *Dr. Suman Chowdhury* > > > > *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, > West Bengal, India.* > > > -- *Dr. Suman Chowdhury* *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Band Structure and PDOS results not matching
This is the fdf that I have used... On Thu, Jan 25, 2018 at 11:40 AM, Nick Papior <nickpap...@gmail.com> wrote: > Dear Suman, > > Without data (plots) or fdf file it is very difficult to help you. > It could be that your smearing parameter is too large. > > > 2018-01-24 15:13 GMT+01:00 Suman Chowdhury <sumanchowdhur...@gmail.com>: > >> Dear SIESTA User, >> >> Recently I am getting some confusing results by using SIESTA. While >> plotting a band structure I am getting a band gap which is quite large. >> However, when I am trying to plot its corresponding total partial density >> of states (PDOS), I can clearly see that there is no existence of any band >> gap. But interestingly the component PDOS are giving the required band gap. >> The problem is with the total PDOS. Do any of you have any idea about these >> kinds of results... >> >> -- >> *Dr. Suman Chowdhury* >> >> >> >> *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, >> West Bengal, India.* >> >> > > > -- > Kind regards Nick > -- *Dr. Suman Chowdhury* *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, West Bengal, India.* SiC.fdf Description: Binary data
[SIESTA-L] Band Structure and PDOS results not matching
Dear SIESTA User, Recently I am getting some confusing results by using SIESTA. While plotting a band structure I am getting a band gap which is quite large. However, when I am trying to plot its corresponding total partial density of states (PDOS), I can clearly see that there is no existence of any band gap. But interestingly the component PDOS are giving the required band gap. The problem is with the total PDOS. Do any of you have any idea about these kinds of results... -- *Dr. Suman Chowdhury* *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Application of strain in SIESTA
Dear All, Does any one know how to introduce strain in siesta. What I know is, suppose I want to introduce strain in the x-direction. Then I have to change the x-component of the each of the lattice vector as well as the unit cell coordinate, then let it relax. Am I right or wrong?? Please explain.Should I keep the volume of the supercell constant or variable cell relaxation. Please help me. -- *Dr. Suman Chowdhury* *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Determination of Spin-Orbit strength
Dear SIESTA User, I am doing some simulation with spin-orbit coupling. Is there any way in SIESTA to determine the actual strength of the spin-orbit coupling. I have taken a material for which the spin-orbit coupling is not known, which I want to know by performing a self-consistent calculation. I can able to vary the strength of spin-orbit coupling in SIESTA. But I want to determine it. How to do that in SIESTA... From Dr. Suman Chowdhury -- *Dr. Suman Chowdhury* *Assistant Professor Dept. of Physics, Bangabasi College Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Problem in siesta parallel job
Dear Barnali, May be this is slightly an off topic but I need some help from you. As you are using the k2 cluster of IUAC, which I am also using. But Iam facing some problems while using SIESTA. While running siesta in the serial mode, the program runs but the output file is not generated. While trying to run the parallel version, the program is not even started even after waiting for 2-3 days. Have you even faced similar kind of problems?? On Thu, Mar 30, 2017 at 1:05 PM, Barnali Bhattacharya < barnalidgbh...@gmail.com> wrote: > Dear SIESTA user > > > I have installed parallel version of siesta 3.2 in k2 cluster and I am > trying to run transiesta job in all.q queue. I have found that, siesta > and transiesta successfully run on the serial.q, but In case of all.q > queue the job started successfully and goes to first MD step ‘New_DM. > Step: 1’, then stop automatically and a new file namely > ‘transiesta.80s-28515,compute-11-14.local’is generated which contain the > following error massage- > > …. > > > > transiesta:28515 terminated with signal 11 at PC=668de0 SP=7fff67d08118. > Backtrace: > > /mnt/oss/sarkar_au/install/siesta-3.2-pl3/Obj/transiesta( > zdotc_+0x70)[0x668de0] > > /opt/intel/composer_xe_2013_sp1.2.144/mkl/lib/intel64/ > libmkl_scalapack_lp64.so(zvvdotc_+0x16)[0x2b758d717a26] > > /opt/intel/composer_xe_2013_sp1.2.144/mkl/lib/intel64/ > libmkl_scalapack_lp64.so(pzdotc_+0xbe4)[0x2b758d7b3584] > > /opt/intel/composer_xe_2013_sp1.2.144/mkl/lib/intel64/ > libmkl_scalapack_lp64.so(pzlatrd_+0xdce)[0x2b758d5845ce] > > /opt/intel/composer_xe_2013_sp1.2.144/mkl/lib/intel64/ > libmkl_scalapack_lp64.so(pzhetrd_+0x721)[0x2b758d534801] > > /opt/intel/composer_xe_2013_sp1.2.144/mkl/lib/intel64/ > libmkl_scalapack_lp64.so(pzheevd_+0x7e9)[0x2b758d524d79] > > /mnt/oss/sarkar_au/install/siesta-3.2-pl3/Obj/transiesta[0x4d0eb9] > > /mnt/oss/sarkar_au/install/siesta-3.2-pl3/Obj/transiesta[0x43b51e] > > /mnt/oss/sarkar_au/install/siesta-3.2-pl3/Obj/transiesta[0x42a2af] > > /mnt/oss/sarkar_au/install/siesta-3.2-pl3/Obj/transiesta[0x4ec9f3] > > /mnt/oss/sarkar_au/install/siesta-3.2-pl3/Obj/transiesta[0x5085d5] > > /mnt/oss/sarkar_au/install/siesta-3.2-pl3/Obj/transiesta[0x508768] > > /mnt/oss/sarkar_au/install/siesta-3.2-pl3/Obj/transiesta[0x6fb60a] > > /lib64/libc.so.6(__libc_start_main+0xfd)[0x365ba1ecdd] > > /mnt/oss/sarkar_au/install/siesta-3.2-pl3/Obj/transiesta[0x404d79] > > > > …… > > *Question 1:* > > Could anyone please help me to solve this problem? Any help will be > greatfully acknowledged. > > Here I am attaching the input, output and error file for siesta > installation for detailed information. > > > Thanking you. > > > Sincerely > > > Barnali Bhattachrya > > Ph. D. student, Department of Physics > > Assam University, Silchar > > > > -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Stoner Parameter
Dear SIESTA user, does anyone know how to calculate the Stoner-Exchange parameter from SIESTA?? -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] mobility, effective mass etc..
Dear SIESTA use, Does anyone know how to calculate effective mass, mobility, thermal and electrical conductivity, Seebeck coefficient through siesta simulation??? -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] problem with gnubands
you can get them from published paper.. On Sep 10, 2016 4:25 PM, "Uttam Paliwal" <uttam...@gmail.com> wrote: > is there any resource or website from where can get the above data > > On Sat, Sep 10, 2016 at 12:30 PM, Suman Chowdhury < > sumanchowdhur...@gmail.com> wrote: > >> For that you need to provide two quantities. The lattice vectors and the >> unit cell coordinate. That is all to specify the crystal structure. >> >> On Sat, Sep 10, 2016 at 12:10 PM, Uttam Paliwal <uttam...@gmail.com> >> wrote: >> >>> then how to specify the crystal structures >>> >>> On Sat, Sep 10, 2016 at 12:00 PM, Suman Chowdhury < >>> sumanchowdhur...@gmail.com> wrote: >>> >>>> Dear Uttam, >>>> >>>> In SIESTA there is no option to provide space group number as far as I >>>> know. >>>> >>>> On Sat, Sep 10, 2016 at 11:57 AM, Uttam Paliwal <uttam...@gmail.com> >>>> wrote: >>>> >>>>> thanks prof Alberto >>>>> >>>>> Kindly clear my another small doubt. In siesta where we provide the >>>>> space group number eg for Si the space group is #216 zinc blende type >>>>> crystal structure. >>>>> >>>>> thanks and regards >>>>> >>>>> On Fri, Sep 9, 2016 at 6:16 PM, Alberto Garcia <alber...@icmab.es> >>>>> wrote: >>>>> >>>>>> Hi, >>>>>> >>>>>> Please note that the gnubands program is intended to plot band >>>>>> structures, i.e., energy values along *lines* in the BZ. The relevant >>>>>> data >>>>>> is obtained with the "BandLines" option in Siesta. If you use the >>>>>> "BandPoints" option you get information about a set of *points* in the >>>>>> BZ, >>>>>> which is not appropriate for a band structure plot. >>>>>> >>>>>> It is perhaps unfortunate that the file extension is the same for >>>>>> both cases. We make a note to change it. >>>>>> >>>>>> Regards, >>>>>> >>>>>> Alberto >>>>>> >>>>>> On 09 Sep 2016, at 12:27, Uttam Paliwal <uttam...@gmail.com> wrote: >>>>>> >>>>>> > hi >>>>>> > I am using siesta-4.1-b1 and running the si_bandpoints.bands files >>>>>> with gnubands. Then i found following error message on cygwin (windows 7) >>>>>> terminal >>>>>> > >>>>>> > >>>>>> --- >>>>>> > >>>>>> > hp@jks /cygdrive/f/siesta-4.1-b1/util/bands >>>>>> > $ ./gnubands < si_bandpoints.bands > up.dat >>>>>> > >>>>>> > At line 143 of file gnubands.f90 (unit = 5, file = 'stdin') >>>>>> > Fortran runtime error: Bad integer for item 1 in list input >>>>>> > >>>>>> > -- >>>>>> -- >>>>>> > >>>>>> > i am attetching the gnubands.f90, makefile, si_bandpoints files >>>>>> herewith. >>>>>> > >>>>>> > kindly provide suggestions >>>>>> > Uttam Paliwal >>>>>> > Assistant Professor >>>>>> > Department of Physics >>>>>> > J.N.V. University >>>>>> > Jodhpur (India) >>>>>> > Phone- 7597908441 >>>>>> > >>>>>> >>>>>> >>>>> >>>>> >>>>> -- >>>>> Uttam Paliwal >>>>> *Assistant Professor* >>>>> Department of Physics >>>>> J.N.V. University >>>>> Jodhpur (India) >>>>> Phone- 7597908441 >>>>> >>>> >>>> >>>> >>>> -- >>>> >>>> >>>> >>>> *Senior research fellow Dept. of Physics, University of >>>> Calcutta Kolkata- 79, West Bengal, India.* >>>> * Ph no-+91-9830512232* >>>> >>>> >>> >>> >>> -- >>> Uttam Paliwal >>> *Assistant Professor* >>> Department of Physics >>> J.N.V. University >>> Jodhpur (India) >>> Phone- 7597908441 >>> >> >> >> >> -- >> >> >> >> *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- >> 79, West Bengal, India.* >> * Ph no-+91-9830512232* >> >> > > > -- > Uttam Paliwal > *Assistant Professor* > Department of Physics > J.N.V. University > Jodhpur (India) > Phone- 7597908441 >
Re: [SIESTA-L] problem with gnubands
For that you need to provide two quantities. The lattice vectors and the unit cell coordinate. That is all to specify the crystal structure. On Sat, Sep 10, 2016 at 12:10 PM, Uttam Paliwal <uttam...@gmail.com> wrote: > then how to specify the crystal structures > > On Sat, Sep 10, 2016 at 12:00 PM, Suman Chowdhury < > sumanchowdhur...@gmail.com> wrote: > >> Dear Uttam, >> >> In SIESTA there is no option to provide space group number as far as I >> know. >> >> On Sat, Sep 10, 2016 at 11:57 AM, Uttam Paliwal <uttam...@gmail.com> >> wrote: >> >>> thanks prof Alberto >>> >>> Kindly clear my another small doubt. In siesta where we provide the >>> space group number eg for Si the space group is #216 zinc blende type >>> crystal structure. >>> >>> thanks and regards >>> >>> On Fri, Sep 9, 2016 at 6:16 PM, Alberto Garcia <alber...@icmab.es> >>> wrote: >>> >>>> Hi, >>>> >>>> Please note that the gnubands program is intended to plot band >>>> structures, i.e., energy values along *lines* in the BZ. The relevant data >>>> is obtained with the "BandLines" option in Siesta. If you use the >>>> "BandPoints" option you get information about a set of *points* in the BZ, >>>> which is not appropriate for a band structure plot. >>>> >>>> It is perhaps unfortunate that the file extension is the same for both >>>> cases. We make a note to change it. >>>> >>>> Regards, >>>> >>>> Alberto >>>> >>>> On 09 Sep 2016, at 12:27, Uttam Paliwal <uttam...@gmail.com> wrote: >>>> >>>> > hi >>>> > I am using siesta-4.1-b1 and running the si_bandpoints.bands files >>>> with gnubands. Then i found following error message on cygwin (windows 7) >>>> terminal >>>> > >>>> > >>>> --- >>>> > >>>> > hp@jks /cygdrive/f/siesta-4.1-b1/util/bands >>>> > $ ./gnubands < si_bandpoints.bands > up.dat >>>> > >>>> > At line 143 of file gnubands.f90 (unit = 5, file = 'stdin') >>>> > Fortran runtime error: Bad integer for item 1 in list input >>>> > >>>> > -- >>>> -- >>>> > >>>> > i am attetching the gnubands.f90, makefile, si_bandpoints files >>>> herewith. >>>> > >>>> > kindly provide suggestions >>>> > Uttam Paliwal >>>> > Assistant Professor >>>> > Department of Physics >>>> > J.N.V. University >>>> > Jodhpur (India) >>>> > Phone- 7597908441 >>>> > >>>> >>>> >>> >>> >>> -- >>> Uttam Paliwal >>> *Assistant Professor* >>> Department of Physics >>> J.N.V. University >>> Jodhpur (India) >>> Phone- 7597908441 >>> >> >> >> >> -- >> >> >> >> *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- >> 79, West Bengal, India.* >> * Ph no-+91-9830512232* >> >> > > > -- > Uttam Paliwal > *Assistant Professor* > Department of Physics > J.N.V. University > Jodhpur (India) > Phone- 7597908441 > -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] problem with gnubands
Dear Uttam, In SIESTA there is no option to provide space group number as far as I know. On Sat, Sep 10, 2016 at 11:57 AM, Uttam Paliwalwrote: > thanks prof Alberto > > Kindly clear my another small doubt. In siesta where we provide the space > group number eg for Si the space group is #216 zinc blende type crystal > structure. > > thanks and regards > > On Fri, Sep 9, 2016 at 6:16 PM, Alberto Garcia wrote: > >> Hi, >> >> Please note that the gnubands program is intended to plot band >> structures, i.e., energy values along *lines* in the BZ. The relevant data >> is obtained with the "BandLines" option in Siesta. If you use the >> "BandPoints" option you get information about a set of *points* in the BZ, >> which is not appropriate for a band structure plot. >> >> It is perhaps unfortunate that the file extension is the same for both >> cases. We make a note to change it. >> >> Regards, >> >> Alberto >> >> On 09 Sep 2016, at 12:27, Uttam Paliwal wrote: >> >> > hi >> > I am using siesta-4.1-b1 and running the si_bandpoints.bands files with >> gnubands. Then i found following error message on cygwin (windows 7) >> terminal >> > >> > --- >> > >> > hp@jks /cygdrive/f/siesta-4.1-b1/util/bands >> > $ ./gnubands < si_bandpoints.bands > up.dat >> > >> > At line 143 of file gnubands.f90 (unit = 5, file = 'stdin') >> > Fortran runtime error: Bad integer for item 1 in list input >> > >> > -- >> -- >> > >> > i am attetching the gnubands.f90, makefile, si_bandpoints files >> herewith. >> > >> > kindly provide suggestions >> > Uttam Paliwal >> > Assistant Professor >> > Department of Physics >> > J.N.V. University >> > Jodhpur (India) >> > Phone- 7597908441 >> > >> >> > > > -- > Uttam Paliwal > *Assistant Professor* > Department of Physics > J.N.V. University > Jodhpur (India) > Phone- 7597908441 > -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] interband or intraband
> Dear Users, > I am really confused about one issue. While calculating optical properties through SIESTA, what we get. Are these obtained data due to interband transition or intraband transition. In one paper I have seen they have separately calculate intraband and interband optical properties by using siesta. Can anyone please help me to clear this confusion. > > From > > Suman > > -- > Senior research fellow > Dept. of Physics, > University of Calcutta > Kolkata- 79, West Bengal, India. > Ph no-+91-9830512232 >
[SIESTA-L] interband or intraband
Dear Users, I am really confused about one issue. While calculating optical properties through SIESTA, what we get. Are these obtained data due to interband transition or intraband transition. In one paper I have seen they have separately calculate intraband and interband optical properties by using siesta. Can anyone please help me to clear this confusion. From Suman -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Real and imaginary part of the wavefunction as a function of energy
Dear Prof. Junquera, Thank you sooo much for your reply. Sir can I get your email id. Because "javier.junquera -- unican es" one is not working. I want to ask you some siesta related question and also some post doc related questions. If you do not have any problem, can you please provide me your email id.. Thanking you On Sat, Jun 4, 2016 at 4:57 PM, Javier Junquerawrote: > > Dear Suman: > > Take a look to the self-explained exercise at: > > http://personales.unican.es/junqueraj > > and follow the links: > > - A self-explained Siesta tutorial > - Set of self-explained Siesta exercises > - Computing structural and electronic properties of materials > - Exercise 2: analysis of the charge density in real space > > Pay special attention to the variables: > > WriteWaveFunctions > %block WaveFuncKPoints > > Read their meaning and other related variables in the Siesta User Guide. > > Hope this helps, > > Javier > > > > > > Dear siesta user. > > I need the real and imaginary part of the wavefunction as a function of > energy. Is it possible to retrieve separately the real and imaginary part > of the wavefucntion from siesta. Please look into the following paper for > this: > > Raymond Atta Fynn et al PRB 69 085207 (2004) > > -- > > > > *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- > 79, West Bengal, India.* > * Ph no-+91-9830512232* > > > -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Real and imaginary part of the wavefunction as a function of energy
Dear siesta user. I need the real and imaginary part of the wavefunction as a function of energy. Is it possible to retrieve separately the real and imaginary part of the wavefucntion from siesta. Please look into the following paper for this: Raymond Atta Fynn et al PRB 69 085207 (2004) -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] How to get simple stm images from plstm.f
It is very easy..it is absolutely applicable to linux...you have to download it by a software called wine... First install wine then install the .exe file thorugh wine... On Wed, Nov 11, 2015 at 2:49 PM, Sukanya Ghosh <ghosh.sukanya1...@gmail.com> wrote: > Dear Suman, > I have downloaded WSxM using the link you have sent. Can you please tell > me how to install it ? > > On Wed, Nov 11, 2015 at 2:42 PM, Sukanya Ghosh < > ghosh.sukanya1...@gmail.com> wrote: > >> Dear Suman, >> Is WSxM applicable to linux ? I thought its is useful for Windows >> >> On Wed, Nov 11, 2015 at 1:49 PM, Suman Chowdhury < >> sumanchowdhur...@gmail.com> wrote: >> >>> Dear Sukanya, >>> For this please download this software from the following link. It is >>> very easy to download and install and also very easy to visualize STM >>> images from the RHO file generated by SIESTA. >>> >>> http://www.wsxmsolutions.com/ >>> >>> On Wed, Nov 11, 2015 at 1:17 PM, Sukanya Ghosh < >>> ghosh.sukanya1...@gmail.com> wrote: >>> >>>> Dear all, >>>> >>>> I want to plot stm images using siesta. I want to plot simple stm >>>> images. Can any of you please tell me how to run the executable from >>>> plstm.f to get the out files. >>>> >>>> Any suggestion is highly appreciated. >>>> >>>> >>>> Thanking you, >>>> >>>> SUKANYA GHOSH >>>> >>> >>> >>> >>> -- >>> >>> >>> >>> *Senior research fellow Dept. of Physics, University of >>> Calcutta Kolkata- 79, West Bengal, India.* >>> * Ph no-+91-9830512232* >>> >>> >> > -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] layers is charge density plot
Dear siesta user, I am trying to plot the charge density of a monolayer system by using rho2xsf utility and then visualize by using xcrysden. I have observed that depending on the spanning vector, the layer number depends. I know the extra atoms are the mirror images of the original structure. But among all the layers, one structure is different from rest of the structures. I am now confused which one is the original. Can anyone help me... -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] MD Visualize in Linux machine
Dear SIESTA User, I want to do molecular dynamics simulation. I have found that after the simulation the program generates three files, SystemLabel.MD,SystemLabel.MDE and SystemLabel.ANI.Can you tell me how to visualize these files. I am unable to find any suitable software for this in linux... -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Problem using gnubands
Try this one ./gnubands si_bandpoints.bands si_bands.dat On Thu, Jul 23, 2015 at 1:47 PM, jv sharma jvnano...@gmail.com wrote: I get like this: jv@jv-desktop:~$ cd siesta-trunk-462/Util/Bands jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ ./gnubands si_bandpoints.bands si_bands.dat At line 27 of file gnubands.f (unit = 5, file = 'stdin') Fortran runtime error: Bad integer for item 1 in list input jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ I get like this, after trying with ./new.gnubands : jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ ./new.gnubands si_bandpoints.bands si_bands.dat At line 128 of file new.gnubands.f90 (unit = 5, file = 'stdin') Fortran runtime error: Bad integer for item 1 in list input jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ On Thu, Jul 23, 2015 at 12:55 PM, Nick Papior nickpap...@gmail.com wrote: Try ./gnubands instead of gnubands. On 23 Jul 2015 06:28, jv sharma jvnano...@gmail.com wrote: Attached here the output. Thanks for the link on basics of linux. Regards, JVN. On Thu, Jul 23, 2015 at 2:06 AM, Nick Papior nickpap...@gmail.com wrote: Do this in the Bands directory (and supply the output to us). $ ls -l $ which gnubands $ make $ which gnubands Consider using the new.gnubands executable which can do several new things. Please read this: http://www.linfo.org/path_env_var.html and the links therein to get a basic grasp of linux. As you are a basic user of unix, this might shed some light of why things goes wrong, as well as providing some basic insights. 2015-07-22 3:56 GMT+00:00 jv sharma jvnano...@gmail.com: Sorry, I could not catch your point, could you please elaborate? On Tue, Jul 21, 2015 at 11:13 PM, Nick Papior nickpap...@gmail.com wrote: It does not look like you are using the gnubands program in siesta-trunk-462, please assert you are... Line 27 is empty in siesta-trunk-462. 2015-07-21 16:52 GMT+00:00 jv sharma jvnano...@gmail.com: Dear Users and Experts, I am new to Ubuntu and Siesta. I have installed siesta-trunk-462. While trying to convert si_bandpoints.bands from the Test, I get the following Fortran runtime error: jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ gnubands si_bandpoints.bands si_bands.dat At line 27 of file gnubands.f (unit = 5, file = 'stdin') Fortran runtime error: Bad integer for item 1 in list input jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ I really don't know what to do. Could someone please suggest a working solution? Many thanks. Best regards, JVN Sarma. -- Kind regards Nick -- Kind regards Nick -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Problem using gnubands
Don't give after ./gnubands. On Thu, Jul 23, 2015 at 2:01 PM, jv sharma jvnano...@gmail.com wrote: Got like this: jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ make clean rm -f *.o *.mod new.gnubands eigfat2plot gnubands jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ make f95 -c -g -O2 -DFC_HAVE_FLUSH -DFC_HAVE_ABORT -UMPI f2kcli.F90 f95 -c -g -O2 m_getopts.f90 f95 -c -g -O2 eigfat2plot.f90 f95 -o eigfat2plot m_getopts.o f2kcli.o eigfat2plot.o f95 -c -g -O2 new.gnubands.f90 f95 -o new.gnubands m_getopts.o f2kcli.o new.gnubands.o f95 -c -g -O2 gnubands.f f95 -o gnubands gnubands.o jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ ./gnubands si_bandpoints.bands si_bands.dat At line 37 of file gnubands.f (unit = 5, file = 'stdin') Fortran runtime error: Bad integer for item 1 in list input jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ Attached here the .bands file. On Thu, Jul 23, 2015 at 1:53 PM, Nick Papior nickpap...@gmail.com wrote: Do make clean, make, retry. Attach the band file. On 23 Jul 2015 10:19, jv sharma jvnano...@gmail.com wrote: I get like this: jv@jv-desktop:~$ cd siesta-trunk-462/Util/Bands jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ ./gnubands si_bandpoints.bands si_bands.dat At line 27 of file gnubands.f (unit = 5, file = 'stdin') Fortran runtime error: Bad integer for item 1 in list input jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ I get like this, after trying with ./new.gnubands : jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ ./new.gnubands si_bandpoints.bands si_bands.dat At line 128 of file new.gnubands.f90 (unit = 5, file = 'stdin') Fortran runtime error: Bad integer for item 1 in list input jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ On Thu, Jul 23, 2015 at 12:55 PM, Nick Papior nickpap...@gmail.com wrote: Try ./gnubands instead of gnubands. On 23 Jul 2015 06:28, jv sharma jvnano...@gmail.com wrote: Attached here the output. Thanks for the link on basics of linux. Regards, JVN. On Thu, Jul 23, 2015 at 2:06 AM, Nick Papior nickpap...@gmail.com wrote: Do this in the Bands directory (and supply the output to us). $ ls -l $ which gnubands $ make $ which gnubands Consider using the new.gnubands executable which can do several new things. Please read this: http://www.linfo.org/path_env_var.html and the links therein to get a basic grasp of linux. As you are a basic user of unix, this might shed some light of why things goes wrong, as well as providing some basic insights. 2015-07-22 3:56 GMT+00:00 jv sharma jvnano...@gmail.com: Sorry, I could not catch your point, could you please elaborate? On Tue, Jul 21, 2015 at 11:13 PM, Nick Papior nickpap...@gmail.com wrote: It does not look like you are using the gnubands program in siesta-trunk-462, please assert you are... Line 27 is empty in siesta-trunk-462. 2015-07-21 16:52 GMT+00:00 jv sharma jvnano...@gmail.com: Dear Users and Experts, I am new to Ubuntu and Siesta. I have installed siesta-trunk-462. While trying to convert si_bandpoints.bands from the Test, I get the following Fortran runtime error: jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ gnubands si_bandpoints.bands si_bands.dat At line 27 of file gnubands.f (unit = 5, file = 'stdin') Fortran runtime error: Bad integer for item 1 in list input jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ I really don't know what to do. Could someone please suggest a working solution? Many thanks. Best regards, JVN Sarma. -- Kind regards Nick -- Kind regards Nick -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Problem using gnubands
Attach the file si_bands.dat On Thu, Jul 23, 2015 at 2:06 PM, jv sharma jvnano...@gmail.com wrote: Hi, After giving this, nothing happened, just the cursor starts blinking in the next line: jv@jv-desktop:~$ cd siesta-trunk-462/Util/Bands jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ ./gnubands si_bandpoints.bands si_bands.dat A blank si_bands.dat is also created in the directory. On Thu, Jul 23, 2015 at 1:56 PM, Suman Chowdhury sumanchowdhur...@gmail.com wrote: Try this one ./gnubands si_bandpoints.bands si_bands.dat On Thu, Jul 23, 2015 at 1:47 PM, jv sharma jvnano...@gmail.com wrote: I get like this: jv@jv-desktop:~$ cd siesta-trunk-462/Util/Bands jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ ./gnubands si_bandpoints.bands si_bands.dat At line 27 of file gnubands.f (unit = 5, file = 'stdin') Fortran runtime error: Bad integer for item 1 in list input jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ I get like this, after trying with ./new.gnubands : jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ ./new.gnubands si_bandpoints.bands si_bands.dat At line 128 of file new.gnubands.f90 (unit = 5, file = 'stdin') Fortran runtime error: Bad integer for item 1 in list input jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ On Thu, Jul 23, 2015 at 12:55 PM, Nick Papior nickpap...@gmail.com wrote: Try ./gnubands instead of gnubands. On 23 Jul 2015 06:28, jv sharma jvnano...@gmail.com wrote: Attached here the output. Thanks for the link on basics of linux. Regards, JVN. On Thu, Jul 23, 2015 at 2:06 AM, Nick Papior nickpap...@gmail.com wrote: Do this in the Bands directory (and supply the output to us). $ ls -l $ which gnubands $ make $ which gnubands Consider using the new.gnubands executable which can do several new things. Please read this: http://www.linfo.org/path_env_var.html and the links therein to get a basic grasp of linux. As you are a basic user of unix, this might shed some light of why things goes wrong, as well as providing some basic insights. 2015-07-22 3:56 GMT+00:00 jv sharma jvnano...@gmail.com: Sorry, I could not catch your point, could you please elaborate? On Tue, Jul 21, 2015 at 11:13 PM, Nick Papior nickpap...@gmail.com wrote: It does not look like you are using the gnubands program in siesta-trunk-462, please assert you are... Line 27 is empty in siesta-trunk-462. 2015-07-21 16:52 GMT+00:00 jv sharma jvnano...@gmail.com: Dear Users and Experts, I am new to Ubuntu and Siesta. I have installed siesta-trunk-462. While trying to convert si_bandpoints.bands from the Test, I get the following Fortran runtime error: jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ gnubands si_bandpoints.bands si_bands.dat At line 27 of file gnubands.f (unit = 5, file = 'stdin') Fortran runtime error: Bad integer for item 1 in list input jv@jv-desktop:~/siesta-trunk-462/Util/Bands$ I really don't know what to do. Could someone please suggest a working solution? Many thanks. Best regards, JVN Sarma. -- Kind regards Nick -- Kind regards Nick -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] rho2xsf not working
Denchar also is not working..Instead of having the .DIM file in the working directory the program is unable to read the .DIM file... On Mon, Jul 6, 2015 at 4:42 PM, fariborz nemati fariborz.nem...@gmail.com wrote: Need I a denchar output before use of the rho2xsf program? On 5 Jul 2015 13:01, Suman Chowdhury sumanchowdhur...@gmail.com wrote: Dear SIESTA User : Now another problem arises..While I am trying to plot the charge density using rho2xsf program it is showing Program received signal SIGFPE: Floating-point exception - erroneous arithmetic operation. Backtrace for this error: #0 0xB76B8163 #1 0xB76B8800 #2 0xB77C23FF #3 0x804CA75 in intpl04_ at intpl04.f:42 #4 0x804AEEE in rho2xsf at rho2xsf.f:216 Floating point exception Can anyone help me to solve this error.. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] rho2xsf not working
Dear SIESTA User : Now another problem arises..While I am trying to plot the charge density using rho2xsf program it is showing Program received signal SIGFPE: Floating-point exception - erroneous arithmetic operation. Backtrace for this error: #0 0xB76B8163 #1 0xB76B8800 #2 0xB77C23FF #3 0x804CA75 in intpl04_ at intpl04.f:42 #4 0x804AEEE in rho2xsf at rho2xsf.f:216 Floating point exception Can anyone help me to solve this error..
[SIESTA-L] Unable to compile denchar
Dear SIESTA user : While I am trying to compile denchar by typing make denchar it is giving me an error No rule to make target `../../../../Obj/arch.make'. Stop. . Can anyone help me in this regard to solve the problem -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Dielectric function
Dear User, I have a question. By definition the imaginary part of the dielectric function is positive and also it can be seen from its mathematical expression that at zero frequency it should be zero. Right now I am studying some structure where sometimes I am getting 0 at 0 frequency and sometimes I am not getting 0 at 0 frequency. It is coming of the order of 10. Do any of you know what is the reason behind it. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] partial band structure
Thanks a lot Prof Artacho..I will now work very hard to learn the fatband.. On Mon, Apr 27, 2015 at 1:02 PM, Emilio Artacho ea...@cam.ac.uk wrote: fatbands gives you that kind of information E On Apr 27, 2015, at 9:24 AM, Suman Chowdhury wrote: My question is, is it possible to identify the bands arising out due to transition of electron from a particular orbital..Suppose I want to identify the bands due to the pi bonded p_z orbital of graphene. Is it possible in siesta.. On Mon, Apr 27, 2015 at 12:41 PM, Emilio Artacho ea...@cam.ac.uk wrote: Not sure what you mean, maybe you are talking about the utility fatbands in the Util directory? Emilio On Apr 27, 2015, at 8:25 AM, Suman Chowdhury wrote: I am not talking about partial DOS...I want to know about partial band structure...I know how to calculate partial DOS by using fmpdos.f... On Mon, Apr 27, 2015 at 11:42 AM, fthe...@iesl.forth.gr wrote: Yes. It is easy to be done, thanks to Andrei Postnikov's utility fmpdos.f. You have to use as input the .PDOS output file of SIESTA and another file where you include details on which partial DOS you want (atom and/or orbitals). Dear User As we all know partial density of states can be calculated easily by using SIESTA...But in many papers I have seen partial band structure that is which band is due to which orbital...is there any way to do that in SIESTA.. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* * Dr Zacharias G. Fthenakis Research Associate Institute of Electronic Structure and Laser (I.E.S.L.) Foundation for Research and Technology Hellas (FO.R.T.H.) Vassilika Vouton P.O. Box 1527 71003 Heraklion Crete Greece Phone +30 2810 391824 FAX +30 2810 391305 webpage: http://esperia.iesl.forth.gr/~fthenak ** -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- Emilio Artacho CIC nanoGUNE Consolider, and Cavendish Laboratory, University of Cambridge Tolosa Hiribidea 76, E-20018 Donostia - San Sebastián, Spain, e.arta...@nanogune.eu, +34 943 574039, http://theory.nanogune.eu -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- Emilio Artacho CIC nanoGUNE Consolider, and Cavendish Laboratory, University of Cambridge Tolosa Hiribidea 76, E-20018 Donostia - San Sebastián, Spain, e.arta...@nanogune.eu, +34 943 574039, http://theory.nanogune.eu -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] partial band structure
I am not talking about partial DOS...I want to know about partial band structure...I know how to calculate partial DOS by using fmpdos.f... On Mon, Apr 27, 2015 at 11:42 AM, fthe...@iesl.forth.gr wrote: Yes. It is easy to be done, thanks to Andrei Postnikov's utility fmpdos.f. You have to use as input the .PDOS output file of SIESTA and another file where you include details on which partial DOS you want (atom and/or orbitals). Dear User As we all know partial density of states can be calculated easily by using SIESTA...But in many papers I have seen partial band structure that is which band is due to which orbital...is there any way to do that in SIESTA.. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* * Dr Zacharias G. Fthenakis Research Associate Institute of Electronic Structure and Laser (I.E.S.L.) Foundation for Research and Technology Hellas (FO.R.T.H.) Vassilika Vouton P.O. Box 1527 71003 Heraklion Crete Greece Phone +30 2810 391824 FAX +30 2810 391305 webpage: http://esperia.iesl.forth.gr/~fthenak ** -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] partial band structure
My question is, is it possible to identify the bands arising out due to transition of electron from a particular orbital..Suppose I want to identify the bands due to the pi bonded p_z orbital of graphene. Is it possible in siesta.. On Mon, Apr 27, 2015 at 12:41 PM, Emilio Artacho ea...@cam.ac.uk wrote: Not sure what you mean, maybe you are talking about the utility fatbands in the Util directory? Emilio On Apr 27, 2015, at 8:25 AM, Suman Chowdhury wrote: I am not talking about partial DOS...I want to know about partial band structure...I know how to calculate partial DOS by using fmpdos.f... On Mon, Apr 27, 2015 at 11:42 AM, fthe...@iesl.forth.gr wrote: Yes. It is easy to be done, thanks to Andrei Postnikov's utility fmpdos.f. You have to use as input the .PDOS output file of SIESTA and another file where you include details on which partial DOS you want (atom and/or orbitals). Dear User As we all know partial density of states can be calculated easily by using SIESTA...But in many papers I have seen partial band structure that is which band is due to which orbital...is there any way to do that in SIESTA.. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* * Dr Zacharias G. Fthenakis Research Associate Institute of Electronic Structure and Laser (I.E.S.L.) Foundation for Research and Technology Hellas (FO.R.T.H.) Vassilika Vouton P.O. Box 1527 71003 Heraklion Crete Greece Phone +30 2810 391824 FAX +30 2810 391305 webpage: http://esperia.iesl.forth.gr/~fthenak ** -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- Emilio Artacho CIC nanoGUNE Consolider, and Cavendish Laboratory, University of Cambridge Tolosa Hiribidea 76, E-20018 Donostia - San Sebastián, Spain, e.arta...@nanogune.eu, +34 943 574039, http://theory.nanogune.eu -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] partial band structure
Dear User As we all know partial density of states can be calculated easily by using SIESTA...But in many papers I have seen partial band structure that is which band is due to which orbital...is there any way to do that in SIESTA.. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] negative PDOS
Can you provide us any reference.. On Sun, Apr 12, 2015 at 1:23 PM, fthe...@iesl.forth.gr wrote: This is a well known problem, but has not to do with SIESTA. It has to do with the physical meaning of the decomposition of DOS to PDOS. If you decompose to orbitals with different orientation you may probably not have those problems. Zacharias Fthenakis Dear siesta users, Has any one encountered the problem of negative value of projected DOS which is calculated with the mprop utility? It seems quite unreasonable for me, any ideas how this come out? Best regards, Bing * Dr Zacharias G. Fthenakis Research Associate Institute of Electronic Structure and Laser (I.E.S.L.) Foundation for Research and Technology Hellas (FO.R.T.H.) Vassilika Vouton P.O. Box 1527 71003 Heraklion Crete Greece Phone +30 2810 391824 FAX +30 2810 391305 webpage: http://esperia.iesl.forth.gr/~fthenak ** -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] negative PDOS
I got the negative values of the PDOS while using double zeta polarized basis set implemented within the SIESTA...Are these basis sets non-orthogonal? On Sun, Apr 12, 2015 at 1:40 PM, Emilio Artacho ea...@cam.ac.uk wrote: The mentioned well-known problem is related with the use of non-orthogonal basis sets. For orthogonal ones the PDOS is definite positive, which is what people expect. But for non-orthogonal ones that is not the case (although negatve values tend to be small since the diagonal bit dominates and that one is positive) Emilio -- Emilio Artacho CIC Nanogune Consolider, and Cavendish Laboratory, University of Cambridge Tolosa Hiribidea 76, E-20018 Donostia - San Sebastián, Spain, e.arta...@nanogune.eu, +34 943 574 4000, http://theory.nanogune.eu On 12 Apr 2015, at 09:53, fthe...@iesl.forth.gr wrote: This is a well known problem, but has not to do with SIESTA. It has to do with the physical meaning of the decomposition of DOS to PDOS. If you decompose to orbitals with different orientation you may probably not have those problems. Zacharias Fthenakis Dear siesta users, Has any one encountered the problem of negative value of projected DOS which is calculated with the mprop utility? It seems quite unreasonable for me, any ideas how this come out? Best regards, Bing * Dr Zacharias G. Fthenakis Research Associate Institute of Electronic Structure and Laser (I.E.S.L.) Foundation for Research and Technology Hellas (FO.R.T.H.) Vassilika Vouton P.O. Box 1527 71003 Heraklion Crete Greece Phone +30 2810 391824 FAX +30 2810 391305 webpage: http://esperia.iesl.forth.gr/~fthenak ** -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] negative PDOS
Thanks for the post...I have also encountered the same problem...Still I don't understand what is the reason for this unreasonable PDOS... On Sun, Apr 12, 2015 at 1:01 PM, BingHuang hbdft2...@gmail.com wrote: Dear siesta users, Has any one encountered the problem of negative value of projected DOS which is calculated with the mprop utility? It seems quite unreasonable for me, any ideas how this come out? Best regards, Bing -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] negative PDOS
In this situation my question is suppose I have obtained negative PDOS for a particular structure. If I will give this values in the manuscript and send to any journal for publication and if the referee will ask about this then what should I do? On Sun, Apr 12, 2015 at 3:05 PM, fthe...@iesl.forth.gr wrote: I fully agree with Emilio. The fact that you find negative PDOS even for s orbitals has to do with the interactions between those s-orbitals with the orbitals of the other atoms, which might give small negative contributions. If you select different orientations of the atoms, you may have different contributions from the atomic orbitals (since their orientation will not change) and those negative contributions could (hopefully) absorbed by other positive contributions. Thus, the PDOS will (hopefully) not be negative. Obviously, there is not any physical meaning for a negative PDOS. The problem comes from the physical meaning assigned to the PDOS, which is exactly the same with the physical meaning assigned to the Mullicken charges. Maybe you can get some answers in Roald Hoffmann's book Solids and Surfaces. Zacharias Fthenakis The mentioned well-known problem is related with the use of non-orthogonal basis sets. For orthogonal ones the PDOS is definite positive, which is what people expect. But for non-orthogonal ones that is not the case (although negatve values tend to be small since the diagonal bit dominates and that one is positive) Emilio -- Emilio Artacho CIC Nanogune Consolider, and Cavendish Laboratory, University of Cambridge Tolosa Hiribidea 76, E-20018 Donostia - San Sebastián, Spain, e.arta...@nanogune.eu, +34 943 574 4000, http://theory.nanogune.eu On 12 Apr 2015, at 09:53, fthe...@iesl.forth.gr wrote: This is a well known problem, but has not to do with SIESTA. It has to do with the physical meaning of the decomposition of DOS to PDOS. If you decompose to orbitals with different orientation you may probably not have those problems. Zacharias Fthenakis Dear siesta users, Has any one encountered the problem of negative value of projected DOS which is calculated with the mprop utility? It seems quite unreasonable for me, any ideas how this come out? Best regards, Bing * Dr Zacharias G. Fthenakis Research Associate Institute of Electronic Structure and Laser (I.E.S.L.) Foundation for Research and Technology Hellas (FO.R.T.H.) Vassilika Vouton P.O. Box 1527 71003 Heraklion Crete Greece Phone +30 2810 391824 FAX +30 2810 391305 webpage: http://esperia.iesl.forth.gr/~fthenak ** * Dr Zacharias G. Fthenakis Research Associate Institute of Electronic Structure and Laser (I.E.S.L.) Foundation for Research and Technology Hellas (FO.R.T.H.) Vassilika Vouton P.O. Box 1527 71003 Heraklion Crete Greece Phone +30 2810 391824 FAX +30 2810 391305 webpage: http://esperia.iesl.forth.gr/~fthenak ** -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Symmetry from band structure
In siesta is it possible to identify the symmetry operations which give rise to different bands from the band structure plot... -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] atom contribution from pDOS
Dear user, In one paper, the authors have used siesta and commented such that by calculating pDOS we can conclude that the contribution to the DOS is mainly due to the edge atoms My question is how can it be calculated? Because pDOS gives us the information about orbital contribution but not atom by atom contribution. Can anyone help me in this regard... -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] [***Posible SPAM***]
As far as I am concern it is not possible to calculate raman spectroscopy by using siesta. You can calculate other DFT code such as quantum espresso or Gaussian for this. On Thu, Feb 26, 2015 at 9:51 PM, Mourad Boutahir mourad.bouta...@gmail.com wrote: helo, i m phD in morocco i start to use the code siesta for dynamic calculations i would calculate the raman spectroscopy of some structures. so please if it was possible to indicate me how i can calculate the raman polarisabity model using the code siesta. best regards -- --- *Mr. Mourad BOUTAHIR* ; Doctorant à la Faculté des sciences MEKNES ; Laboratoire d'Etude des Matériaux Avancés et Applications (LEM2A) Université Moulay Ismail GSM : +212662770697; E-mail : *mourad.bouta...@gmail.com mourad.bouta...@gmail.com** ait_ta...@yahoo.fr;* - -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Time steps in MD
Dear user, In the SIESTA manual it is written that, if I want to do molecular dynamics simulation then I need to give the initial time steps and the final time steps. The default values for initial time steps and the final time steps are given as 1. But no unit of the time is mentioned. Do you know what is the unit of time in this case, I think it should be femto-second (fs). But I want to confirm with you. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Constraint adsorption
Dear siesta user, Suppose I want to do some adsorption by using SIESTA...If I don't want to change the xyz coordinate of the lattice on which the adatom is going to adsorbed and also the x and y coordinate of the adatom only want to change the z coordinate of the adatom..Then how can it be done by using siesta... -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Spin Orbit Coupling
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 j.fer...@cinn.es wrote: My apologies. This was intended to be sent to Suman only. Jaime Ferrer El 9/12/2014, a las 18:06, Jaime Ferrer j.fer...@cinn.es 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 sumanchowdhur...@gmail.com 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 j.fer...@cinn.es 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 ica...@gmail.com 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
Re: [SIESTA-L] Spin Orbit Coupling
I want to thank Prof Ferrer and Prof Seivane for such an excellent discussion on SO effect in SIESTA... On Wed, Dec 10, 2014 at 3:13 PM, Lucas Fernandez Seivane queve...@gmail.com wrote: Dear All As Jaime said, the only drawback is the bigger memory and thus time requirements. And as you see in his link and former literature, bands can be perfectly plotted. I just want to point to you all to this reference which may be interesting in your case, where all the calculations were performed with SIESTA trying to match previous a previous ABINIT version of the calculations. While in the final paper we didn't do all the final calculations with SO, we also tested the SO in the bulk and monolayer, but it didn't affect what we were looking for in the initial calculations of the NWs in the cases we were interested, and as Prof. Ferrer said it makes the calculations slower, so we proceeded just with spin polarized. In any case, if you have problems reproducing literature I can look up the psf files we used for the MoS2. https://www.researchgate.net/publication/257247197_Atomic_and_electronic_properties_of_quasi-one-dimensional_MoS2_nanowires All the best -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Spin Orbit Coupling
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 j.fer...@cinn.es 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 ica...@gmail.com 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 sumanchowdhur...@gmail.com 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 smt...@gmail.com 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- 79, West Bengal, India.* * Ph no-+91-9830512232 %2B91-9830512232* -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] How to extract TB parameters from SIESTA
I think it cannot be done in siesta. Alternatively you can try LMTO. On Wed, Dec 3, 2014 at 2:07 PM, 邵德喜 dxshao...@gmail.com wrote: Dear everyone: I'm now interested in formulating a TB Hamilton from SIESTA. Any ideas and comments will be appreciated. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] How to extract TB parameters from SIESTA
Yes. LMTO is another ab inito software which uses tight binding hamiltonian. From where you can get the TB parameter. LMTO is completely free. On Wed, Dec 3, 2014 at 2:32 PM, 邵德喜 dxshao...@gmail.com wrote: Thanks, is LMTO here also a software about ab initial? 2014-12-03 16:42 GMT+08:00 Suman Chowdhury sumanchowdhur...@gmail.com: I think it cannot be done in siesta. Alternatively you can try LMTO. On Wed, Dec 3, 2014 at 2:07 PM, 邵德喜 dxshao...@gmail.com wrote: Dear everyone: I'm now interested in formulating a TB Hamilton from SIESTA. Any ideas and comments will be appreciated. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] electronic and magnetic properties
You have to use Eig2dos in the Utils folder. After compilation of the filename.EIG with the help of eig2dos you can have folder where there will four coloumns. The first one will be the energy in eV. The next one will be dos for spin up, then dos for spin down and the last one will be the dos for spin up + spin down. On Tue, Dec 2, 2014 at 1:03 PM, Nadia Salami nadiasala...@gmail.com wrote: I think that the density of states of spin up and down are same. On Tue, Dec 2, 2014 at 9:05 AM, Nadia Salami nadiasala...@gmail.com wrote: Dear Siesta users, I want to obtain the electronic and magnetic properties of my system. So I have used SpinPolarized true option. But after DFT calculation by Siesta code, there aren't two files for density of states for up and down spins, but there are Mulliken Atomic and Orbital Populations for all species with up and down spins in the output file. It will be highly appreciated any help and comment. Thanks in advance, Best regards. Nadia Salami PhD student -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Hybridization
If I want to study some doped structure,how can I understand from siesta data if there is some hybridization takes place or not between the dopant atoms and the substrate.. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Contribution to the magnetism
Dear siesta user, I have studied the magnetic property of some systems and found magnetism. Is it possible from the siesta data to know which atoms are contributing in this magnetism...It is very urgent... -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Unrelaxed coordinates after siesta Optimization
Can you post your full .fdf file.. On Fri, Oct 10, 2014 at 3:07 PM, Manjeet Bhatia manjeetbhati...@gmail.com wrote: Dear Siesta Users, After Siesta optimization i got forces as Tot0.0065550.016954 0.0022713 and OutCoor: Final (Unrelaxed) atomic coordinates. Is that ok with the relaxation? if not then what parameter I have to change . Look forward to your reply. Manjeet -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Unrelaxed coordinates after siesta Optimization
This .fdf file will never give relaxed structure. Because you have given number of CG steps is 50, which not at all sufficient for this structure to relax with the given relaxation criteria. Just increase the number of CG steps to 1000, hopefully it will going to converge to within this.. On Fri, Oct 10, 2014 at 4:05 PM, Manjeet Bhatia manjeetbhati...@gmail.com wrote: Attached... On Fri, Oct 10, 2014 at 3:33 PM, Suman Chowdhury sumanchowdhur...@gmail.com wrote: Can you post your full .fdf file.. On Fri, Oct 10, 2014 at 3:07 PM, Manjeet Bhatia manjeetbhati...@gmail.com wrote: Dear Siesta Users, After Siesta optimization i got forces as Tot0.0065550.016954 0.0022713 and OutCoor: Final (Unrelaxed) atomic coordinates. Is that ok with the relaxation? if not then what parameter I have to change . Look forward to your reply. Manjeet -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] fatband
Dear user, Can anyone clearly explain (step by step) how to plot fatband...I am unable to understand from the siesta manual...Suppose I want to plot the band structure of 2pz electrons...How to do that? -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Monkhorst Pack grid for structure relaxation
Dear user, I want to know if I only want to relax the structure, without calculating any other physical quantity from the siesta simulation, is it OK to define the K point sampling i.e. Monkhorst Pack grid is simply 1 0 0 0 1 0 0 0 1 Because this will accelerate the convergence...I just want to relax the structure..Will not use any data for calculation... -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Monkhorst Pack grid for structure relaxation
Thanks to all of you for your reply... On Wed, Oct 1, 2014 at 1:58 PM, Riccardo Rurali rrur...@icmab.es wrote: It depends on what your 'structure' is? If it is a non-periodic system not only you 'can', but you 'should' use only the Gamma point. If the system is periodic and the computational cell is not large enough, such a reduced sampling of the Brillouin zone could lead to an incorrect relaxed geometry. Riccardo On 10/1/14 9:53 AM, Suman Chowdhury wrote: Dear user, I want to know if I only want to relax the structure, without calculating any other physical quantity from the siesta simulation, is it OK to define the K point sampling i.e. Monkhorst Pack grid is simply 1 0 0 0 1 0 0 0 1 Because this will accelerate the convergence...I just want to relax the structure..Will not use any data for calculation... -- /*Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.*/ /* Ph no-+91-9830512232*/ /* */ -- Riccardo Rurali Institut de Cičncia de Materials de Barcelona (ICMAB-CSIC) Campus de Bellaterra 08193 Bellaterra (Barcelona) Spain tel.: +34 935801853 ext. 347 e-mail: rrur...@icmab.es http://www.researcherid.com/rid/D-3676-2011 Man, the dope's that there's still hope -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] SIESTA in FACEBOOK
Dear all SIESTA User, Those users who has facebook account are requested to join the following group for discussion: https://www.facebook.com/groups/1482411542018575/ -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Automatic Shut Down after simulation
Dear user, Is it possible to configure one's PC or laptop in such a way that the PC or laptop shut down automatically after the completion of the simulation. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Automatic Shut Down after simulation
Thanks, Can I run this command in my ubuntu PC? On Tue, Sep 30, 2014 at 6:38 PM, Nick Papior Andersen nickpap...@gmail.com wrote: Sure, Make shutdown a command exectuable by any user, (search around unix fora for this) then do: $ siesta RUN.fdf RUN.out ; shutdown -h now 2014-09-30 12:56 GMT+00:00 Suman Chowdhury sumanchowdhur...@gmail.com: Dear user, Is it possible to configure one's PC or laptop in such a way that the PC or laptop shut down automatically after the completion of the simulation. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232 %2B91-9830512232* -- Kind regards Nick -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Problem with PBE Na pseudopotential
While I am running a simulation using GGA-PBE Na pseudopotential I am getting the error. I am sure the problem is not with the .fdf file but with the Na pseudopotential. I am attaching you the .out file. I also think the problem lies in not including p shell in the pseudopotential. I don't know how to include that in the pseudopotential. Please help to solve the problem. -- *Senior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* Na1.out Description: Binary data
Re: [SIESTA-L] How to restart Siesta?
Few weeks ago I had also posted a similar question in the forum.. On Sun, Sep 21, 2014 at 6:55 AM, Julio Henrique juliohenri...@msn.com wrote: I had simulations interrupted by prolonged lack of electricity. How to restart from where it was interrupted? Is it possible? Thank's. Julio Henrique. -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Force vs Iteration
I don't understand what you are saying...Can you please it clearly step by step.. On Wed, Sep 17, 2014 at 8:50 PM, Irtaza Hassan irtazahassa...@gmail.com wrote: grep 'constrained' outputfile filename.ext use filename.ext file for plots. On Wed, Sep 17, 2014 at 8:08 PM, Suman Chowdhury sumanchowdhur...@gmail.com wrote: Dear all, I need to produce a graph Force vs MD steps.Can you please tell me how to do that. IT is very urgent.? -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232 %2B91-9830512232* -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Force vs Iteration
Dear all, I need to produce a graph Force vs MD steps.Can you please tell me how to do that. IT is very urgent.? -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Fwd: Forceful termination of the program
-- Forwarded message -- From: Suman Chowdhury sumanchowdhur...@gmail.com Date: Fri, Aug 22, 2014 at 1:30 PM Subject: Forceful termination of the program To: siesta-l@uam.es Dear user, I have a question. Suppose I have made MD.UseSaveXV, MD.UseSaveCG and DM.UseSaveDM flags true and run a simulation. Then suppose I have to stopped the program forcefully before its completion.Then I will again run the unfinished program. My question is will the program start from where I have stopped it forcefully before the completion. -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] why the result (lattice constant...etc.) of Siesta and Vasp can't compare?
Because they use different algorithm, different potential and different basis set. On Fri, Aug 22, 2014 at 11:15 AM, joyce79928cc . joyce79...@gmail.com wrote: Dear: I have asked this similar question before. why the result (lattice constant...etc.) of Siesta and Vasp can't compare? because I have use this two software to calculate the example provided by Siesta and also create the input file for Vasp. Though I have tried my best to set the same flag. but the results are just very different. why the result (lattice constant...etc.) of Siesta and Vasp can't compare? Thank you! the file attached is my input for vasp and siesta -- Best Regards 邱芳瑜 Chiu Fang Yu 國立成功大學 材料科學與工程學系碩一 MOBILE:0930287221(中華) GMAIL:joyce79...@gmail.com wisdom4...@gmail.com -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Forceful termination of the program
Dear user, I have a question. Suppose I have made MD.UseSaveXV, MD.UseSaveCG and DM.UseSaveDM flags true and run a simulation. Then suppose I have to stopped the program forcefully before its completion.Then I will again run the unfinished program. My question is will the program start from where I have stopped it forcefully before the completion. -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] lattice constant problem
No I don't think so.. On Fri, Aug 22, 2014 at 4:38 PM, Максим Арсентьев ars21031...@gmail.com wrote: I believe cartesian coordinate is orthogonal http://en.wikipedia.org/wiki/Cartesian_coordinate_system It is better to use reduced? 2014-08-22 7:23 GMT+04:00 Suman Chowdhury sumanchowdhur...@gmail.com: Yes I have corrected entered the coordinated, because when the make the supercell I am getting the structure which I want but with zero z coordinate and with much much longer lattice constant. Cartesian coordinate can be of any system not necessarily of orthogonal system. On Fri, Aug 22, 2014 at 1:28 AM, Максим Арсентьев ars21031...@gmail.com wrote: PLs give us the link of the literature. K point grid should be more dense. Did you properly entered coordinates (cartesian are for ortogonal system)? 2014-08-21 21:04 GMT+04:00 Suman Chowdhury sumanchowdhur...@gmail.com: But after optimization the 2D sheet no longer remains 2D. It must have some non -zero buckling. On Thu, Aug 21, 2014 at 9:54 PM, Sergio Ferrari lic.sergio.ferr...@gmail.com wrote: I simply notice that you said that you want to optimize a two dimensional sheet of germanium, so all atoms should be put in a plane (of your choice), of course 2 atoms are allways in a plane but I wonder if for simplicity it is preferable to write the coordinates of the atoms in the x-y plane. Also in your kgrid_Monkhorst_Pack your k points are equal en all directions, that is clearly wrong if you want to simulate a 2D sheet. 2014-08-15 5:27 GMT-03:00 Suman Chowdhury sumanchowdhur...@gmail.com : Dear siesta user, I am trying to optimize the two dimensional sheet of germanium. I am using the pp given in the siesta website. The lattice constant given in the literature is within 3.97 to 4.01 A with buckling 0.6 to 0.7 A. But each time I run the siesta program I am getting the lattice constant just the double of this and with almost zero buckling. I started with lattice constant 3.97 and buckling 0.7 A. Can anyone help to solve the problem. I am attaching the .fdf file. -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- Dr. Sergio Ferrari Depto. de Física-Fac. de Ingeniería INTECIN (UBA-CONICET) Av. Paseo Colón 850 C1063ACV-Ciudad de Buenos Aires ARGENTINA Tel: +54 (11) 4342-1396 (Directo) 4342-9184/4343-0891/4343-2775 (Int. 1021) http://intecin.fi.uba.ar -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- Best wishes, Maxim Arsent'ev, D.Sc.(Chemistry) Laboratory of research of nanostructures Institute of Silicate Chemistry of RAS -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- Best wishes, Maxim Arsent'ev, D.Sc.(Chemistry) Laboratory of research of nanostructures Institute of Silicate Chemistry of RAS -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] lattice constant problem
But after optimization the 2D sheet no longer remains 2D. It must have some non -zero buckling. On Thu, Aug 21, 2014 at 9:54 PM, Sergio Ferrari lic.sergio.ferr...@gmail.com wrote: I simply notice that you said that you want to optimize a two dimensional sheet of germanium, so all atoms should be put in a plane (of your choice), of course 2 atoms are allways in a plane but I wonder if for simplicity it is preferable to write the coordinates of the atoms in the x-y plane. Also in your kgrid_Monkhorst_Pack your k points are equal en all directions, that is clearly wrong if you want to simulate a 2D sheet. 2014-08-15 5:27 GMT-03:00 Suman Chowdhury sumanchowdhur...@gmail.com: Dear siesta user, I am trying to optimize the two dimensional sheet of germanium. I am using the pp given in the siesta website. The lattice constant given in the literature is within 3.97 to 4.01 A with buckling 0.6 to 0.7 A. But each time I run the siesta program I am getting the lattice constant just the double of this and with almost zero buckling. I started with lattice constant 3.97 and buckling 0.7 A. Can anyone help to solve the problem. I am attaching the .fdf file. -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- Dr. Sergio Ferrari Depto. de Física-Fac. de Ingeniería INTECIN (UBA-CONICET) Av. Paseo Colón 850 C1063ACV-Ciudad de Buenos Aires ARGENTINA Tel: +54 (11) 4342-1396 (Directo) 4342-9184/4343-0891/4343-2775 (Int. 1021) http://intecin.fi.uba.ar -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] lattice constant problem
Yes I have corrected entered the coordinated, because when the make the supercell I am getting the structure which I want but with zero z coordinate and with much much longer lattice constant. Cartesian coordinate can be of any system not necessarily of orthogonal system. On Fri, Aug 22, 2014 at 1:28 AM, Максим Арсентьев ars21031...@gmail.com wrote: PLs give us the link of the literature. K point grid should be more dense. Did you properly entered coordinates (cartesian are for ortogonal system)? 2014-08-21 21:04 GMT+04:00 Suman Chowdhury sumanchowdhur...@gmail.com: But after optimization the 2D sheet no longer remains 2D. It must have some non -zero buckling. On Thu, Aug 21, 2014 at 9:54 PM, Sergio Ferrari lic.sergio.ferr...@gmail.com wrote: I simply notice that you said that you want to optimize a two dimensional sheet of germanium, so all atoms should be put in a plane (of your choice), of course 2 atoms are allways in a plane but I wonder if for simplicity it is preferable to write the coordinates of the atoms in the x-y plane. Also in your kgrid_Monkhorst_Pack your k points are equal en all directions, that is clearly wrong if you want to simulate a 2D sheet. 2014-08-15 5:27 GMT-03:00 Suman Chowdhury sumanchowdhur...@gmail.com: Dear siesta user, I am trying to optimize the two dimensional sheet of germanium. I am using the pp given in the siesta website. The lattice constant given in the literature is within 3.97 to 4.01 A with buckling 0.6 to 0.7 A. But each time I run the siesta program I am getting the lattice constant just the double of this and with almost zero buckling. I started with lattice constant 3.97 and buckling 0.7 A. Can anyone help to solve the problem. I am attaching the .fdf file. -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- Dr. Sergio Ferrari Depto. de Física-Fac. de Ingeniería INTECIN (UBA-CONICET) Av. Paseo Colón 850 C1063ACV-Ciudad de Buenos Aires ARGENTINA Tel: +54 (11) 4342-1396 (Directo) 4342-9184/4343-0891/4343-2775 (Int. 1021) http://intecin.fi.uba.ar -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- Best wishes, Maxim Arsent'ev, D.Sc.(Chemistry) Laboratory of research of nanostructures Institute of Silicate Chemistry of RAS -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Charge Transfer
Thanks a lot.. On Sun, Aug 17, 2014 at 3:14 AM, I. Camps ica...@gmail.com wrote: I Dear Suman, You have two different type of charge analysis. One is simple: to get the charge distribution. The second one is to get the charge transfer from/to your system. In the first case, your system is only one. In this case, you calculate the charge distribution (using one or different schemes) and you are set. In the second case, your system has an initial conformation/configuration, them it suffers some modification giving it a final conformation/configuration. In this case, you calculate the charge distribution BEFORE the fenomenum that alter the conformation/configuration and calculate again AFTER the fenomenum, so, you calculate the charges twice. After that, you calculate the charge transfer as the difference between the two situations. An example: the water molecule. If you one to get the charges in each atom, you calculate the charge distribution for the atoms in the molecule only one time. If you want to calculate the charge modification in the O (the difference between the isolated and molecular atoms) you must do the calculation twice: one for the isolated atom and one for the molecular atom. Then, you calculate the transferred charge as Charge_O_isolated-Charge_O_molecular. Regards On 15 Aug, 2014 1:22 AM, Suman Chowdhury sumanchowdhur...@gmail.com wrote: Dear Camps, Twice means? Can you please explain clearly what should be the process. On Fri, Aug 15, 2014 at 3:23 AM, Bishal Bhattarai bishalbhattarai...@gmail.com wrote: Can we get the wave functions out from the MULIKEN charge distribution ? I want to calculate IPR( Inverse Participation Ratio ) for my 648 silica atoms Bishal On Thu, Aug 14, 2014 at 4:11 PM, I. Camps ica...@gmail.com wrote: Hello Suman, If you want to calculate charge transfer you have to do your calculation twice and then calculate the difference of charges for the two calculations. You can use the diferente charge scheme implemented in SIESTA such as Voroni, Hirsfeld or Muliken (or all at the same time). Take a look in the manual for the wright keywords. Regards, On 14 Aug, 2014 6:50 AM, Suman Chowdhury sumanchowdhur...@gmail.com wrote: Dear siesta user, How I can estimate the charge transfer from atom to atom from SIESTA? -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232 %2B91-9830512232* -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232 %2B91-9830512232* -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] lattice constant problem
Dear siesta user, I am trying to optimize the two dimensional sheet of germanium. I am using the pp given in the siesta website. The lattice constant given in the literature is within 3.97 to 4.01 A with buckling 0.6 to 0.7 A. But each time I run the siesta program I am getting the lattice constant just the double of this and with almost zero buckling. I started with lattice constant 3.97 and buckling 0.7 A. Can anyone help to solve the problem. I am attaching the .fdf file. -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* germanene.fdf Description: Binary data
[SIESTA-L] Charge Transfer
Dear siesta user, How I can estimate the charge transfer from atom to atom from SIESTA? -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Charge Transfer
Dear Camps, Twice means? Can you please explain clearly what should be the process. On Fri, Aug 15, 2014 at 3:23 AM, Bishal Bhattarai bishalbhattarai...@gmail.com wrote: Can we get the wave functions out from the MULIKEN charge distribution ? I want to calculate IPR( Inverse Participation Ratio ) for my 648 silica atoms Bishal On Thu, Aug 14, 2014 at 4:11 PM, I. Camps ica...@gmail.com wrote: Hello Suman, If you want to calculate charge transfer you have to do your calculation twice and then calculate the difference of charges for the two calculations. You can use the diferente charge scheme implemented in SIESTA such as Voroni, Hirsfeld or Muliken (or all at the same time). Take a look in the manual for the wright keywords. Regards, On 14 Aug, 2014 6:50 AM, Suman Chowdhury sumanchowdhur...@gmail.com wrote: Dear siesta user, How I can estimate the charge transfer from atom to atom from SIESTA? -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232 %2B91-9830512232* -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] unfolding formula
This paper is very interesting. In fact I have also been searching in internet for this kind of methods. But how can I implement this method in siesta. It is now not possible for me to implement your method in siesta by writing programs, because I don't have so much time left for my phd. If you can supply me your package then I can use it then definitely with proper acknowledgement or citations of your papers in our all future works...So can we collaborate.. On Tue, Aug 12, 2014 at 1:20 PM, Antonino LaMagna antonino.lama...@imm.cnr.it wrote: Dear SIESTA Users, I would like to annonce the pubblication of the manuscript Role of basis sets on the unfolding of supercell band structures: From tight-binding to density functional theory Eur. Phys. Lett. 107 27006 (2014) by I. Deretzis et al. http://iopscience.iop.org/0295-5075/107/2/27006/ Here we propose a band unfolding method for supercell calculations which can be directly applied with the SIESTA outcomes. Kind Regards Antonino La Magna -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Huge stress tensor
Dear all, After running just 1 CG step, I got the following stress-tensor-voigt (kbar) Stress-tensot-voigt (kbar) -10092.56 -61.77 5.74 -0.46 0.00 0.00.. My question is can said that the structure is relaxed after the CG step. -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] charge density
Dear user, Can anyone know how to plot charge density through siesta by using vmd visualization tool. -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Magnetism from Charge Density
Dear all, How to estimate magnetism from charge density in siesta? -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Xcrysden
Dear All, I have tried thousand times to install Xcrysden in my machine, but I failed.Can anyone tell me how to do it step by step? -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Band Structure
Dear all, How can I get a good band structure when my unit cell is large? -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Band Structure
Dear all, To plot the band structure which is to be set true, WriteBands or WriteKBands or both. -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Energy window in siesta
Dear all, When I calculate the optical properties of any system in SIESTA, the imaginary part of the di electric constant which it gives as an output, the difference between any two successive energy is always found to be constant (0.01979).How can I change this energy window. -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Nanodisks
Dear all, How do I calculate the electronic structure of graphene nano disks which do not have any boundary condition by siesta? -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
Re: [SIESTA-L] Nanodisks
Thanks to all.Can you tell me how I put fake boundary condition i.e. putting the nano disk in a large enough box.. On Fri, Feb 7, 2014 at 9:11 PM, Bailey, Steven s.bai...@lancaster.ac.ukwrote: Taking the isolated disc will give you the energy levels (flat). You need to connect the disc to periodic leads or make the discs periodic to obtain the band structure of your system. Dr S Bailey Department of Physics Lancaster University UK Email: s.bai...@lancaster.ac.uk Tel: +441524592844 *From:* siesta-l-requ...@uam.es [mailto:siesta-l-requ...@uam.es] *On Behalf Of *Suman Chowdhury *Sent:* 07 February 2014 15:19 *To:* siesta-l@uam.es *Subject:* [SIESTA-L] Nanodisks Dear all, How do I calculate the electronic structure of graphene nano disks which do not have any boundary condition by siesta? -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232* -- *Junior research fellow Dept. of Physics, University of Calcutta Kolkata- 79, West Bengal, India.* * Ph no-+91-9830512232*
[SIESTA-L] Pseudo
Dear all, How reliable are the pseudo potentials given in the siesta website?
Re: [SIESTA-L] atoms
thanks a lot On Sat, Jan 25, 2014 at 2:50 AM, Abraham Hmiel abehm...@gmail.com wrote: Suman, I think the answer you're looking for is 42. Only 42-atom simulations are considered by peer review ;) But joking aside, you should look to previously-published ab-initio results in your system of interest or something close to it. Even if such results exist, you should perform methodological checks on system size, i.e. size-convergence simulations with respect to: the number of layers in a surface slab, or supercell dimensions if you're simulating a bulk compound (perhaps with a defect or other non-homogeneity), different sizes of nanowire, etc. Some of the most important current problems in nanoscience involve quantum size-effects, and you don't really know how many atoms a good simulation requires until you try it- the physics of a particular solid-state system can vary dramatically based on small size increments! So, to answer the question you posed, no real number of atoms guideline exists. Use what is feasible and timely for your computational setup while giving trustworthy, meaningful, repeatable results! By the way, the T in siesta stands for Thousands (but this only really makes sense with the order-N functional). The number of atoms in a SIESTA simulation could be anywhere in the range {10^0, 10^4}. -- *Abraham Hmiel* Katherine Belz Groves Fellow in Nanoscience Xue Group, SUNY College of Nanoscale Science and Engineering http://abehmiel.net/about On Fri, Jan 24, 2014 at 8:21 AM, Suman Chowdhury sumanchowdhur...@gmail.com wrote: Dear all, what is the typical number of atoms one should use for publishable results using SIESTA?
[SIESTA-L] Elastic Constant
Dear all, How all the elastic constants can be calculated by using SIESTA?
[SIESTA-L] Graphene Band Lines
Dear all. Can anyone provide me the correct band lines of a hexagonal lattice (like graphene,silicene,germanene,stanene etc. sheet (not in terms of reciprocal lattice vectors)
[SIESTA-L] Spin Orbit Coupling
Can anyone provide me the SIESTA code where the Spin Orbit coupling is considered.
[SIESTA-L] Fwd: Convergence
-- Forwarded message -- From: Suman Chowdhury sumanchowdhur...@gmail.com Date: Thu, Dec 19, 2013 at 12:10 PM Subject: Convergence To: siesta-l@uam.es Dear all siesta user, How do I know if my molecular dynamics simulation is converging or not?
[SIESTA-L] Convergence
Dear all siesta user, How do I know if my molecular dynamics simulation is converging or not?