Hi all,
Is there any post-processing utility to extract Lowdin charges for Siesta
that anyone knows of?
Best,
Marcos
Hi all,
I'd like to use the full relativistic pseudos of Pseudo Dojo in my
calculations, but I'd also like to avoid having to compile the latest trunk
version in the cluster I'm using right now. Is there any tool to convert
the PSML pseudos from Pseudo Dojo to the old psf format?
Best regards,
M
Hi all,
I am running a geometry relaxation of a Cu2N@Cu(100) slab with a Fe atom on
top, comprising 235 atoms - fixed cell, not variable cell.
All went well until at one point during the CG optimization, I got the
following warning:
WARNING: Connected supercells may have changed: [in]/[out] 215
Dear Prof. Auluck,
This is not the case. I am referring to the total spin magnetization of all
atoms in the cell so it cannot be the case. Moreover, I have only one Fe
atom in the cell, which is responsible for almost all of the spin
magnetization.
Best,
Marcos
On Fri, May 25, 2018 at 5:08 AM,
Dear all,
I am performing my first spin-orbit calculations for a Fe atom over a
Cu2N/Cu(100) slab. By the end of the calculation, Siesta prints a table
with sqrt^2 for each of the atom in the supercell, the sum of all
sqrt^2, and at the end of the calculation, the total spin.
What I get is, for t
Hi all,
I am trying out OMM released in the 4.0 beta version, and it is really
amazing how faster it is with respect to diagonalization. However, I see
two possible issues there. (I am testing it on a phonon calculation).
1) There seems to be a small bug in one of the variables, namely
OMM.LongO
Silly, silly me! Now it works perfectly. Thanks, Nick.
Marcos
On Tue, Dec 1, 2015 at 9:14 PM, Nick Papior wrote:
> Try use the bands.WFSX file instead.
>
> 2015-12-02 0:06 GMT+01:00 Marcos Veríssimo Alves <
> marcos.verissimo.al...@gmail.com>:
>
>> Hi Nick,
>&g
Hi all,
I am a bit confused about the output of a fat bands calculation. I have
calculated the band structure for my system, with the options for
generating the necessary output for "fat".
Problem is, after using eigfat2plot, the x-axis scale is completely
different from that of the band structur
Hi all,
I have a doubt in a COOP calculation. I have performed a calculation for an
ethene molecule (C2H4), and the EIG file indicates that the Fermi level is
-4.9449 eV. According to this Fermi level, the HOMO would be at -6.41786
eV. Therefore, if I integrate the DOS up to -6.41786 eV, I should
ri, Sep 25, 2015 at 11:15 AM, Nick Papior wrote:
> I think so, I have not tested.
>
> I think none of the codes in the last couple of releases have any changes
> in the affected files.
>
> 2015-09-25 16:08 GMT+02:00 Marcos Veríssimo Alves <
> marcos.verissimo.al...@gmail.c
.
>> Any way it seems weird that it "suddenly" triggers as all memory have
>> been allocated.
>>
>> Could you also attach the fdf files?
>> --
>>
>> Kind regards Nick Papior
>> On 25 Sep 2015 02:34, "Marcos Veríssimo Alves" <
>&g
smoothly till the 19954 suggests something not directly
> related to the code? Do you have disk space?
>
> PS. Which options did you recompile with?
>
> 2015-09-24 17:20 GMT+00:00 Marcos Veríssimo Alves <
> marcos.verissimo.al...@gmail.com>:
>
>> Hi all,
>>
>>
Hi all,
I am trying to write data for a COOP analysis. I have to go to a very high
number of k-points, otherwise the curves (PDOS, for example) are rather
"noisy", with pretty wild wigglings.
The problem is, for some reason, it seems that wwave does not handle the
number of k-points I'd like to h
ble to pass the ghost state detection. I will start the process
for the LMKLL functional now, but I suspect the same will happen.
Could there be a bug in the XC library, or somewhere else?
Best regards,
Marcos
On Wed, Sep 2, 2015 at 5:05 PM, Marcos Veríssimo Alves <
marcos.verissimo.al..
On Sep 2, 2015, at 1:17 PM, I. Camps wrote:
>
> Hello,
>
> I generated the vdW pseudos with trunk-458 with the DRSLL and LMKLL
> functionals without the ghost problem for H, C, O and N. I used the INP
> files from SIESTA pseudopotentials webpage.
>
>
> []'s,
>
> @
functionals without the ghost problem for H, C, O and N. I used the INP
> files from SIESTA pseudopotentials webpage.
>
>
> []'s,
>
> @mps
>
> On Wed, Sep 2, 2015 at 4:06 PM, Marcos Veríssimo Alves <
> marcos.verissimo.al...@gmail.com> wrote:
>
>> H
Hi all,
I am trying to generate pseudos for H with the vdW functionals and use them
in vdW calculations using trunk-462 for the H2 molecule. However, I am
running into ghost states when I try running the calculation for the H2
molecule with the DRSLL, LMKLL, C09 and BH functionals.
I tried using
27;m messing up with something
here inadvertently.
Cheers,
Marcos
On Fri, Aug 21, 2015 at 5:29 AM, Emilio Artacho wrote:
> Hi Marcos
>
> The k-point sampling would in general be different. Are
> both calculations well converged in k points?
>
> Emilio
>
> On Aug 21, 2
Hi all,
I am running some calculations for a 3D structure made of carbon, using
Siesta 3.2-pl-5. The executable was compiled with
gfortran using mpif90 -O2 -g -pipe -Wall -Wp,-D_FORTIFY_SOURCE=2
-fexceptions -fstack-protector --param=ssp-buffer-size=4 -m64
-mtune=generic
however, I am running th
ld not be an
> issue.
>
>
>
> 2015-04-16 17:46 GMT+02:00 Marcos Veríssimo Alves <
> marcos.verissimo.al...@gmail.com>:
>
>> Hi all,
>>
>> I have been performing some calculations for graphene-like materials
>> using the trunk-462 version, and I have
Hi all,
I have been performing some calculations for graphene-like materials using
the trunk-462 version, and I have been obtaining some warnings at the
beginning of some SCF cycles:
Note: For starting DM, Qtot, Tr[D*S] = 10.
10.09624902
These warnings disappear as the structure
Ciao Feffe,
Siesta can print Mulliken charges - I guess it's the closest to what you
need. Just add *WriteMullikenPop 1* to your input, and it will print the
Mulliken charges at the end of every CG step.
Cheers,
Marcos
On Wed, Mar 28, 2012 at 1:54 PM, Federico Iori wrote:
> Hi all.
>
> Maybe
pack.f
>> @echo "==> Compiling dc_lapack.a in Libs..."
>> @(cd Libs ; $(MAKE) dc_lapack.a)
>> *#*
>> version:
>> @echo
>> @echo "==> Incorporating information about present compilation
>>
>> then i error was the same
>>
>>
Mohammad,
I also have the same setting as you, and didn't have any problems compiling
1.3f1, at least not in this part. I remember, though, that I also had this
problem when I first tried to compile it. It's likely that you could have
your problem solved by replacing the entries in lines 153 and 1
Natalia,
You are correct in saying that all codes do add a compensating background
to charged systems. However, without the SimulateDoping option, the
background added is homogeneous, while with the abovementioned option,
"This background charge is constant at points of the mesh near the atoms,
a
Hi Andrei,
Just one comment. If I'm not mistaken, the default spin polarization for
Siesta, when you don't specify anything, is that one atom is initialized
with spin up and the other down, in this case - an antiferro configuration.
The final spin of the system could be non zero in this case, I su
Hi all,
I am trying to do calculations for bulk (fcc) Pd using the van der Waals
functional parametrized by Klimes et al (vk in atom, KBM in siesta, as in
JPCM 22, 022201 - 2009). I have generated my own pseudo and I just can't
obtain the results for the lattice constant described in PRB 83, 19513
Guys,
If this pseudo has been used before, it most likely doesn't present ghost
states. If it did, Siesta would have stopped. So one possibility for these
ghost states is that the compiler options are such that wrong results are
being output. This is especially strong in ifort. If it is ifort, I
r
Heiko,
One comment on pseudopotentials. Usually pseudopotentials are not optimized
for a particular problem. They are created to be good for any kind of
problem. This is done by setting cutoff radii which yield the softest
possible potential with good agreement of the pseudo-eigenenergies and
loga
It should be readable by a suitable Fortran code, even if it is stored
unformatted. Check the manual for the WriteMDHistory flag:
http://www.icmab.es/siesta/manuales/manual-3.0-b/node83.html#3035 and also
the Util folder for possible utilities to read and convert the MD files to
other formats, as w
If you don't tell us what the problem is in some detail, no one will ever be
able to help you. Please state the problem in a more detailed way.
Marcos
On Mon, Oct 24, 2011 at 6:01 AM, Surjeet Chandel wrote:
> dear siesta users
> There is a problem in reading the position and velocity in .MD file
+ p*V (eV/cell) -5787.5740
> Target enthalpy (eV/cell) -5814.1462
>
> ------
>
> 22 октября 2011, 17:52 от Henrik Löfås :
>
> Dear Maxim,
>
> Another point, you set
> MaxSCFIterations 0
> I am not sure but I think this means that you just get you
Maxim,
I believe Chun has a point here, and I beg to differ from what you say.
For some materials, it is important to include special k-points, so as to
get a correct band structure and (eventually) forces - the most "famous"
case would perhaps be graphene, with its K point. Even if your material
Check the list archives... This has come up a few months ago. Look for an
answer by José Soler, more specifically.
Marcos
On Fri, Oct 14, 2011 at 10:20 AM, Yusia Rosee wrote:
> Dear All,
>
> I am quite confused about the relation about the quanbum numbers
> m(=-2,-1,0,1,2) and the d orbitals (
Hi all,
My three cents on the subject.
Graphene needs a very dense in-plane sampling for a correct description of
its physical properties. It is likely that bilayer graphene does need a high
sampling as well. Since it's an isolated bilayer, it would be fine to use
just 1 MP division in the direct
Hector, looks like you have missed this post:
http://www.mail-archive.com/siesta-l@uam.es/msg00735.html
> On Thu, 18 Mar 2010 09:58:15 -0500, Backlund, Daniel wrote
> > The forces are in eV/Ang (per iofa.f)
> >
> > Daniel J. Backlund
> > Texas Tech University - Physics
> > daniel.backl...@ttu.ed
In addition to Andrei's and Slimane's suggestions, I'd increase the mesh
cutoff. You have too few atoms to justify such a low cutoff, and a finer
mesh could help in the convergence. Keep the electronic temperature high
from the beginning, increasing it if necessary until you reach convergence
in th
Piotr,
One possible reason is that your convergence parameters are not sufficiently
strict. DM convergences of 10^-3 will give you very poor results. Ideally,
the DM convergence should be as strict as possible, and you can easily get
down to 10^-5 or even 10^-6 with systems as easy to handle as gr
Zahra,
Again Andrei's remark applies: what exactly do you understand by "wrong"?
Marcos
On Fri, Sep 2, 2011 at 8:26 AM, Zahra Talebi wrote:
> hi,
> Thanks for your answer,
> I have a question,
> YOu know puting the kgrid cutoff just affect my DOS and make its result
> wrong. but I have the cor
Ye-Fei,
Indeed there are people who say that adding U to O 2p orbitals is
meaningless. However, I remember there is a paper on the subject by Anisimov
himself (and co-authors), in http://arxiv.org/abs/cond-mat/0009107 . In this
paper, they justify the application of U to O 2p states by stating (if
Coming back to Lily's first question, it seems that a space between the word
total and the = sign was forgotten: "Total =" instead of "Total=".
Marcos
On Thu, Aug 4, 2011 at 12:26 PM, Hongyi Zhao wrote:
> On 08/04/2011 05:50 AM, apost...@uni-osnabrueck.de wrote:
>
>> This is not in the flags; t
Krishna,
Do you have the same problem for smaller systems? Most probably fdf files
are useless in this case, since it is a compiler problem. My wild guess:
check if you are using optimization O3. If you are, then lower it to O2.
Marcos
On Thu, Jul 28, 2011 at 4:45 AM, krishna Mohan Grangadhran P
Karim, I think OrderN works as long as your system has a gap. If your
nanowire doesn't have one, you'll be in trouble there. If the first system
is an isolated molecule, then it makes sense that OrderN works. If your
nanowire is known to have a gap, then OrderN should work as well.
Marcos
On Thu,
This variable sets an extrapolation of the density matrix to the new set of
coordinates in a relaxation process, after an SCF cycle ends. It is
hopefully a better starting, than just using the DM from the previous step
at the end of the SCF cycle. It is independent of variable cell or
relaxation me
Check work by Xavier Blase. It hasn't been necessarily done with Siesta, but
if I remember well, he calculates the electron-phonon coupling strength for
some superconductivity formula. From his paper, you will know what you need,
and it will be easier for people to figure out if what you need can b
The paper I've suggested before deals exactly with this question.
>
> Cheers
>
> NH
>
>
> 2011/7/18 Marcos Veríssimo Alves
>
>> As far as I remember, the first approach is used in siesta (adding a
>> neutral background). However, this only works well, in pr
As far as I remember, the first approach is used in siesta (adding a neutral
background). However, this only works well, in principle, for cubic (simple,
bc and fc), for which Madelung corrections are properly implemented. To
check this properly, run a test calculation with a net charge, just so yo
pdosxml.
On Fri, Jul 15, 2011 at 11:27 PM, lily zheng wrote:
> Thanks, It seems there is no ready-made one like eig2dosto
> handle.PDOs?
>
> Lily
>
>
> On Fri, Jul 15, 2011 at 4:11 PM, wrote:
>
>> > Dear all,
>> >
>> > How to give those parameters which show up as the head of .PDOS file?
Perhaps
%block AtomicCoordinatesAndAtomicSpecies52006 <<===
?
Marcos
On Thu, Jul 14, 2011 at 11:01 PM, lily zheng wrote:
> Dear all,
>
> I got so confused about this run. Usually if everything is okay, the last
> line is "end of run, time" .
>
> But this one is without "end of run
Should stand for Polarization. Notice it has higher angular momentum (l=3).
Marcos
On Thu, Jul 14, 2011 at 2:04 PM, Hongyi Zhao wrote:
> Hi all,
>
> I let siesta write out the wavefunction for graphene and then I use the
> readwfx utility to extract the information from graphene.WFSX.
>
> Then
You must add the 3d electrons explicitly to your basis set in the block
PAO.Basis. Check the manual and the list archives - a few years ago I have
written a rather extended email explaining these things.
Cheers,
Marcos
2011/6/27 Gregorio García Moreno
> **
> Sorry, but I have obtained the same
Hi Gao,
It is not very trivial to deduce this, and I have struggled with it a bit.
But the correspondence between orbital quantum numbers and labels is:
p: m=-1 -> x
m=0 -> z
m=1 -> y
d: m=-2 -> x^2-y^2
m=-1 -> yz
m=0 -> z^2
m=1 -> xz
m=2 -> xy
It's even good to have thi
As far as I remember, the way siesta does the division of the x-axis from
one point to the other is to calculate the length of the vector joining the
initial and final points in k-space, then divide this length by the number
of points along the direction, defining a delta_l for the direction
consid
Sorry,
I made a mistake here. It should be K=(0.5, -0.5, 0) instead.
Marcos
2011/6/14 Marcos Veríssimo Alves
> It has nothing to do with Hydrogens in the system. As a matter of fact,
> hydrogens would open the gap - it would be graphane, not graphene. The input
> seems fine to me,
It has nothing to do with Hydrogens in the system. As a matter of fact,
hydrogens would open the gap - it would be graphane, not graphene. The input
seems fine to me, and it it most likely because your specification of band
lines is incorrect. If you choose
BandLinesScale ReciprocalLatticeVector
with the code...
> Any idea of the performance hit taken by not using atlas?
>
> Thanks!
> Carlos
>
> 2011/6/10 Marcos Veríssimo Alves :
> > When it comes to energies, it seems that some of them are too different.
> Try
> > compiling without atlas (that is, no libra
When it comes to energies, it seems that some of them are too different. Try
compiling without atlas (that is, no libraries, just the siesta libs) and if
that doesn't work, try lowering the optimization level. Also, compile siesta
with the flag -DGRID_DP - that could make some difference.
Best reg
Thanks for the info, Jesús. There's no need to make any benchmark, I just
wanted to know if it was worth trying to install ifort 12 at all :)
Marcos
2011/6/9 Jesús Carrete Montaña
> On 09/06/11 16:23, Marcos Veríssimo Alves wrote:
> > Jesús,
> >
> > Thanks fo
Jesús,
Thanks for sharing. A few questions:
1) What mpi are you using? How is it compiled?
2) Do you have benchmarks to compare with previous versions of ifort (10.x,
11.x) and perhaps other compilers in the same processors?
Best regards,
Marcos
2011/6/9 Jesús Carrete Montaña
> On 09/06/11 1
d Mn basis set from the siesta website.
Best of luck,
Marcos
On Mon, Jun 6, 2011 at 4:49 PM, silvia wrote:
> Sorry,
>
> this is the correct fdf file
>
>
>
> El 06/06/2011, a las 16:17, Marcos Veríssimo Alves escribió:
>
> Silvia,
>
> There is too little information o
Silvia,
There is too little information on your problem for anyone to say anything
meaningful. But, no, in principle there are no such problems - I am doing
calculations using Siesta LDAU using semicore states and U and I get no such
error.
Marcos
On Mon, Jun 6, 2011 at 4:08 PM, silvia wrote:
Perhaps in your case the best thing to do is a COOP analysis. It could in
principle show you which states are more bonding and which are not: check
http://www.cohp.de (and the bibliography therein, of course) for more
details.
Hope this helps,
Marcos
On Mon, May 30, 2011 at 9:43 PM, Hongyi Zhao
Not necessarily. Set MD.TargetPressure to the desired value (0.01 GPa,
f.e.).
Marcos
On Thu, May 19, 2011 at 2:52 PM, akshu hans wrote:
> Dear users
> when i try to relax the technetium unit cell using MD.VariableCell T, the
> forces on atoms relax to less the 0.04ev and stress tensor is close
Indeed, these lines (the ones with ==) shouldn't be there. Or, at least,
they should have a hash (#) in the beginning, in which case Siesta would
interpret them as a comment and it would have no effect.
Marcos
On Thu, May 19, 2011 at 1:29 PM, Hongyi Zhao wrote:
> 2011/5/19 Valentin V. Karas
Make an xsf file including the translation vectors (check the XCrysDen
documentation on the website for how to do it, or use Andrei Postnikov's
tool). Then, in XCrysDen, increase the number of repetitions in the
direction you want. If yout structure appears continuous, then it is correct
(in princi
xcrysden is great. Check the xcrysden documentaiton (howto) in the xcrysden
website to see how to make a xsf file. You can use an xyz and struct_out
files to create a xsf file without much effort. You can even use xcrysden
files in Vesta fot visualization.
Marcos
On Thu, Apr 28, 2011 at 10:25 PM,
Ghous,
Forget about the .pseudos file, it just means something in the context of
running the tests in an automated way. The procedure for running siesta is
in pages 9 and 10 of the manual, and in the tutorials available on the web.
In a very simplified manner, suppose you want to run a compiled ve
Ram,
1) Discover what $MKL_ROOT is. If you're using a standard intel installation
and ifort 11 as your arch.make suggests, it should be something like
/opt/intel/Compiler/11.1/075/mkl/lib/em64t/ (check this in your system). For
the sake of example, let's suppose that this is where the mkl is insta
Yes, eV.
Marcos
On Tue, Apr 12, 2011 at 7:01 PM, Szakacs, Csaba wrote:
> Question:
>
> are the values from the .EIG file in eV ?
>
> Suggestion:
>
> somewhere it should mention the units in use.
>
>
> Thanks,
> Csaba
>
>
>
>
x: + 598 2 924 1906
> Web: http://cryssmat.fq.edu.uy/ricardo/ricardo.htm
> ---------
>
> El 06/04/2011, a las 10:27, Marcos Veríssimo Alves <
> marcos.verissimo.al...@gmail.com> escribió:
>
>
> Hi all,
>>
>> So, great to know there a
Hi all,
So, great to know there are knowledgeable people on Vesta in the mailing
list. My question is the following: I have a cubic structure, a perovskite.
I have a [sqrt(2) x sqrt(2)] cell of this structure, with relaxed positions
with rotated oxygen octahedra in the x-y plane only, out of which
Hi all,
This has nothing to do with Siesta, strictly speaking, but it could be of
general interest: supercell building.
I see many people here use and like GDIS. I have tried to download and
compile it once, but it didn't compile. With the executable version of GDIS
that came with Ubuntu, I found
That is a particular thing to gmail, I think. When my email was the academic
one, I used to get my replies. But I do get follow-ups as threads to my
posts on the list.
Marcos
On Fri, Mar 18, 2011 at 8:17 AM, Alexander Vozny wrote:
> I can only see the threads by others, and cann't see the thre
This issue has been discussed a few days ago in the list (I myself answered
it). Please check the list archives before posting a question: someone most
likely has had the same problem you have had before.
Marcos
On Thu, Mar 17, 2011 at 3:47 AM, wrote:
> Dear all,
>
> I compiled the siesta-3.0-r
This is a private implementation by the group of Stefano Sanvito, if I'm not
mistaken. You'd have to contact him directly to see if he can release you
the code, because it is not distributed in official Siesta releases.
Marcos
On Wed, Mar 16, 2011 at 5:23 PM, Alexander Vozny wrote:
>
> I rememb
My advice is that you read about pseudopotentials as they are used in DFT
calculations (especially, what their use entails). The answer to your
question lies there.
Marcos
On Mon, Mar 14, 2011 at 2:22 PM, gaohaiyuan wrote:
> Dear siesta users:
>
> I intend to use DFT simulation to verify Higgs
You forgot to include the mesh shfits. Your MP block should read
x1 y1 z1 sh1
x2 y2 z2 sh2
x3 y3 z3 sh3
Usually the shifts are 0.0 or 0.5.
Marcos
On Sun, Mar 13, 2011 at 3:04 PM, sheetal sharma wrote:
> hi,
> I am working on graphene sheet and using the following in input file
> it works
This has happened before to people using ifort 11. If this is the case,
switch to ifort 10.1, and don't forget to recompile mpi with it.
Marcos
On Fri, Mar 11, 2011 at 9:06 AM, Reza Kalantari <
rezakalantarinez...@gmail.com> wrote:
> Dear Siesta Users
>
> I have used ifort and mpich2 to compile
Juliana,
I suppose the best you can do is to fix the spin of the system as a whole
using the FixSpin and TotalSpin flags. However, there is no way to guarantee
the final state of the system, at least within SIESTA - at least, none that
I know of.
Marcos
On Fri, Mar 11, 2011 at 4:27 AM, Juliana M
It is trying to read more data than there actually is in the .bands file. I
am not sure of what you are doing exactly, but the amount of data in the
file, if you are creating it by hand (???) should be consistent with what
you tell the program to read.
Marcos
On Wed, Mar 9, 2011 at 5:48 AM, deepa
= 3 rc= 2.047986 el= 0.003178 Ekb= -1.649997 kbcos= -0.006611
>
> KBgen: Total number of Kleinman-Bylander projectors: 16
> atom:
> -
>
> atom: SANKEY-TYPE ORBITALS:
> atom: Selecte
Michael,
I'm pretty sure this issue has already been discussed before on the list,
but here goes the short version of the story.
Siesta needs infiniband or myrinet (in general, a low latency internode
connection) to work properly in parallel, otherwise you should try to run it
in parallel only on
Fen,
If your calculation was done correctly, you must have made some convergence
study for the thickness of the slab. Your slab should be thick enough so
that the lattice parameter in the center of the slab, and the electronic
structure of the center of the slab, are the same with respect to bulk.
Gao,
If you already have your O2 molecule in a box big enough so that it is
already isolated from its periodic images (10, 12 Ang should do the job),
there is no need to place the O2 molecule far from the surface, and all you
need is the isolated O2 molecule calculation and the O2+surface calculat
Bohr / Angstrom conversion?
On Thu, Feb 10, 2011 at 3:47 PM, pietro bonfa wrote:
> Dear Siesta users,
>
> I have a problem that I wasn't able to overcome despite it has been largely
> discussed in this mailing list.
> The following BandLines block is from the input file that have been given
> t
Hi Michael,
"Channel" refers to angular momentum channel (I can't quite remember why
it's called so, but you'll see it sometimes). So (n=2, l=0) is the 2s
orbital or 2s "channel"; (n=2, l=1) is the 2p "channel" and so on.
So actually, when you refer to basis sets, you should specify them,
strictl
Ian,
Are you using the PBSsol as your XC functional inside the fdf file? Ususlly
this kind of warning is trying to tell you that your pseudo has been
generated with a different XC functional than that which you are using for
your DFT calculation, which can be rather messy.
Marcos
On Sat, Feb 5,
On Mon, Jan 31, 2011 at 11:55 AM, Fen Hong wrote:
> Dear Marcos
> Thank you very much.
>
> what do you mean that "plot the complete PDOS and integrate it up to the
> Fermi level". I think the integration is the total states up to the fermi
> level not the number of electrons.
>
If I am not mista
N,
Just a remark: in principle, you can calculate transition dipole moments -
this is exactly what the optical subroutine does. The formalism is in
Harrison's books. However, for the UV-VIS spectra, not all of them will
contribute, you will have to select the appropriate ones, or perhaps
construct
Karim,
I'd say that the basis set deosn't play as much an influence on the final
symmetry of the unit cell (at least in Siesta) as much as a fine real-space
mesh. However, if you know which symmetrization operations on forces and
stresses maintain the symmetry of a cell, then you can implement the
I think for that, you'd have to determine the boundaries of each plane,
calculate the whole LDOS and then set the elements of the LDOS(x,y,z) of the
planes you don't want to zero, in case you want it just for visualization
purposes.
Marcos
On Sun, Jan 30, 2011 at 3:57 PM, mashiat alaaii wrote:
>
Fen,
Regarding the first question, this is basic Fortran90 programming stuff.
Check any good Fortran programming tutorial for how a record is constructed.
Orbid is a record which contains the relevant information about each
contribution to the PDOS in the file: n, l, m, zeta, spin, atom number in
This has to do with how polarization orbitals are determined in Siesta. The
subject has been discussed in the list before, I think, but in brief: in the
manual, you can see that they are the solutions to the perturbation problem
of an atom in a weak electric field. Now, if you look at this problem,
Menghao,
Whereas I am not sure what exactly is the setup for the angles theta and phi
(that is, if theta is measured from the z axis or from the x-y plane), it
could be that theta=90 degrees is already a possible energy minimum. In
particular, if theta is measured from the x-y plane, then you have
wrote:
> Hi, Marcos.
>
> If z refers to the zeta of the basis, now it makes sense because i'm using
> the DZP ones. So the PDOS of one orbital, 2p for example, is the sum of the
> two zeta contributions ?
>
> Thanks for your time.
>
> My bests,
>
> Weslley.
>
Weslley,
z here refers to the zetas of your basis function. If I am not mistaken,
spin is denoted by s in the .PDOS files.
Marcos
On Fri, Jan 21, 2011 at 6:10 PM, Weslley Souza Patrocinio <
wesl...@vonbraunlabs.com.br> wrote:
> Hi, all.
>
> I'm using the pdosxml util for a system without spin p
e easily.
> Please check the input and suggest me what basis set and pseudo is suitable
> for bulk Beta Sn (body centered tetragonal structure).
>
> Suman Kalyan Sahoo
>
> --- On *Wed, 19/1/11, Marcos Veríssimo Alves <
> marcos.verissimo.al...@gmail.com>* wrote:
>
>
>
Giacomo,
I see you are using a mesh cutoff of 100 Ry for your calculation. This could
be too small by itself for O, which is a hard pseudo in comparison with
other elements. I believe converged calculations for compound with O should
use at least 180 Ry (an equivalent of 45 Ry in plane waves), wh
Suman, could you give us a more precise idea of how the band structure,
lattice parameters and cohesive energy compare with the data in the
literature (that is, providing numbers and an illustration of the band
structure)?
With the very scarce information you provide I can only think of trivial
mi
Sean,
There are redirection signs ( < > ) missing in what you have typed. If you
type
/siesta/obj/siesta < /siesta/util/vibra/src/si.ifc.fdf > si.ifc.out
it should work for real. Perhaps there is some font problem somewhere -
either in Javier's file or your version of Powerpoint.
Marcos.
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