You compiler (gnu 4.8.5) is *very* old. Please upgrade to a modern version.
Best regards,
Alberto
- El 6 de Junio de 2024, a las 19:09, Boubacar Traore
escribió:
| I finally sorted out the issue of scalapack linking by adding its path to
| LIBRARY_PATH instead of LD_LIBRARY_PATH
ink to the hydrogen one,
e.g. H.psf.
I hope this helps.
Alberto
- El 16 de Noviembre de 2023, a las 04:17, Francisco Garcia
escribió:
| Dear Prof. Garcia
| Many thanks for your response.
| I looked up the MM.Potentials block but I couldn't figure out how to apply the
| harmon
a harmonic potential.
Best regards,
Alberto
- El 11 de Noviembre de 2023, a las 09:13, Francisco Garcia
escribió:
Dear Users,
The constraint subroutine takes the form: subroutine constr( cell, na, isa,
amass, xa, stress, fa, ntcon ). It doesn't contain information about energy.
_build stands for the CMake build
directory and for the appropriate subdirectory in the Util hierarchy.
The build_all.sh script is a fossil we forgot to remove…
If you used an old version of ‘fat’, the format of the HSX file might have
changed. Please use the latest version.
Alberto
d building steps.
Thank you for your feedback.
Alberto
- El 28 de Septiembre de 2023, a las 21:33, Reza Behjatmanesh-Ardakani
escribió:
| Hi
| I used following command for compiling siesta-master:
|
| cmake -S. -B_bui
to check that you reach a flat region in the vacuum.
Alberto
- El 15 de Marzo de 2023, a las 11:41, yh46 escribió:
| Hello Dear SIESTA Users,
| I am trying to do a work function calculation of Au 111 surface. The
| work function I get if 3.5 eV, which is quite different from
| experimenta
Hi,
This is something that we are planning to implement.
For now, if file space is a problem, you could use symbolic links from a
central location to each execution directory.
Best regards,
Alberto
- El 3 de Feb de 2023, a las 19:33, Daniel Bennett
escribió:
| Hi all,
| I was
Hi,
For some reason, you are using commas (",") instead of dots (".") as decimal
separators. In fortran,
a comma in an input line separates items. This confuses the program. You should
check your 'locale' settings.
Alberto
- El 7 de Noviembre de
Hi,
You should remove the comment character from:
#%endblock LatticeVectors
Alberto
- El 21 de Septiembre de 2022, a las 12:23, Amal Yassin
escribió:
| Dear Siesta Users
| I make run to carbone nanotube armchair, but i find an error, can anyone helle
| me to solve this error? ( I
Dear Rajesh,
I quote from (the source of) the Siesta manual:
\item The default perturbative scheme for polarization orbitals
can fail in very specific cases. When the polarization orbital
has to have a node due to the presence of a lower-lying orbital
with the same $l$, the program can (if e
ra conditions on the pseudopotential of the
alchemical species.
Best regards,
Alberto
- El 28 de Junio de 2022, a las 14:09, RCP pasia...@cnea.gov.ar escribió:
| Dear developers,
|
| I'd like to know if there is a specific reference for the method
| of mixing pseudopotentials implemented
if [ $rank -lt $limit0 ]
then
export CUDA_VISIBLE_DEVICES=0
elif [ $rank -lt $limit1 ]
then
export CUDA_VISIBLE_DEVICES=1
elif [ $rank -lt $limit2 ]
then
export CUDA_VISIBLE_DEVICES=2
else
export CUDA_VISIBLE_DEVICES=3
fi
$@
I
Hello,
You seem to be missing the BLAS library in your link statement. It could be as
simple as adding -lblas to your link line, but it would depend
on your installation.
Best regards,
Alberto
- El 22 de Junio de 2022, a las 23:14, Ghazanfari, Sarah
sarah.ghazanf...@ndsu.edu escribió
setup. Radii (standard, H): 1.000 0.600
dhscf: Vacuum level (max, mean) =0.636991 -0.068255 eV
cite: Please see "h2o.bib" for an exhaustive BiBTeX file.
[...]
in which one gets two blocks, one for Voronoi and another one for Hirshfeld
populations.
Alberto
- El 14 de Jun
Hi,
As the error message suggests, you can try the non-perturbative options (see
manual).
I hope this helps.
Regards,
Alberto
- El 13 de Junio de 2022, a las 12:22, Reza Behjatmanesh-Ardakani
reza.b@gmail.com escribió:
| Hi,
| I used following fdf file for Li unit cell
-tune the automatic split-valence options.
I hope this helps.
Alberto
- El 27 de Mayo de 2022, a las 00:01, Andres Tellez Mora
at00...@mix.wvu.edu escribió:
| Dear SIESTA users.
|
| I am trying to run a calculation with a SmNiO3 structure. I am using the
pseudo
| potentials from the
Hi,
There must be some issue with your input. Could you share it?
Regards,
Alberto
- El 28 de Marzo de 2022, a las 02:52, Francisco Garcia
garcia.ff@gmail.com escribió:
| Dear Users
|
| I performed a series of single point energy calculations on an FCC crystal by
| varying the
Hi Francisco,
You need to run a new (SOC) calculation, but you can re-use the DM file
(density matrix) from the previous run to initialize the SOC calculation, thus
typically reducing the number of steps needed for convergence.
Regards,
Alberto
- El 27 de Marzo de 2022, a las 09:34
Hi,
The units are indeed Bohr^-1. But in the .bands file (assuming you are using
the 'bandlines' option), what is printed is
the cumulative path length in reciprocal space.
I hope this helps.
Alberto
- El 10 de Feb de 2022, a las 04:39, Pasan Henadeera henadeer...@gmail.com
relatively straightforward, with basic help in the page:
https://gitlab.com/siesta-project/siesta/-/wikis/How-to-build-the-master-version-of-Siesta
We are planning a beta release of Siesta 5.X in the next few weeks.
Best regards,
Alberto
- El 6 de Feb de 2022, a las 08:50, Daniel
Hi,
You have a number of errors in your input file:
-- The atomic number of C is 6, not 12
-- For C and N, the d orbital should have n=3
-- For H the p orbital should have n=2
I hope this helps. You must have made changes to Simune's files...
Alberto
- El 2 de Feb de 2022, a las
Hi,
As explained in
https://gitlab.com/siesta-project/siesta/-/wikis/Guide-to-Siesta-versions
you need to use the rel-MaX-1 branch, which contains both PSML support and the
ELSI interface.
Best regards,
Alberto
- El 17 de Ene de 2022, a las 02:50, Chong Wang ch-w...@outlook.com
t what
is sent through the interface. What do other codes send through the interface?
Best regards,
Alberto
[1] Kresse, G., and J. Furthmüller. 1996. “Efficiency of Ab-Initio Total Energy
Calculations for Metals and Semiconductors Using a Plane-Wave Basis Set.”
Computational Materials Science
at the end of the page:
https://docs.siesta-project.org/projects/siesta/tutorials/basic/structure-optimization/index.html
Alberto
- El 5 de Octubre de 2021, a las 14:54, Ziba Torkashvand
zi.torkashv...@gmail.com escribió:
| Dear all siesta users,
| I'm trying to relax my structure
-Siesta-versions
I hope this helps.
Alberto
- El 17 de Septiembre de 2021, a las 13:44, alokkarn0 alokka...@gmail.com
escribió:
| I tried so many times in the SIESTA_psml version, I don't know where I did
make
| mistakes, that every time "file.bands.WFSX" did not work for a p
use 'make'.
Alberto
- El 12 de Jul de 2021, a las 09:32, Jimenez Alfaro, Jorge (NASERTIC)
jjime...@nasertic.es escribió:
| Hello,
|
| Any help will be really appreciated. Many thanks in advance
|
| I have modified line 33 of Makefile regarding a recipe that used to work for
|
e function are written to standard output.
c Other information is written to standard error.
Best regards,
Alberto
- El 13 de Junio de 2021, a las 19:54, Jyotirmoy Deb
deb.jyotirmo...@gmail.com escribió:
| I want to get the numerical value of electron density rho (x,y,z) along X, Y,
Hi,
For this simple kind of constraint, you should not need to write your own
constr.f file. You can use the constraint-specification options described in
the manual.
Best regards,
Alberto
- El 20 de Mayo de 2021, a las 10:40, Pablo Álvarez Rodríguez
pablo96carnic...@gmail.com
option dm-use-save-dm.
Alberto
- El 31 de Marzo de 2021, a las 18:56, El-abed Haidar
ehai2...@uni.sydney.edu.au escribió:
| Good evening,
|
|1. I was wondering for a large SIESTA calculation, if I forgot the
commands in
|the fdf file to do a fat band calculation and do not want to
do-H atoms. You could use directly the 'atom' program, or use the utilities
in Util/VCA to generate pseudos for "fractionally-charged" H atoms.
Alberto
- El 22 de Feb de 2021, a las 17:02, Mochena, Mogus D.
mogus.moch...@famu.edu escribió:
| Dear siesta users:
|
Hola,
Soy co-administrador de la lista 'siesta-l' que usa el servidor de listas
'sympa' de la UAM.
Desde hace unos días, aparecen en la lista mensajes como el que sigue a
continuación. Saben qué puede estar pasando?
Muchas gracias.
Saludos,
Alberto García
ICMAB-C
Hi,
You do not give details, but you must be using a very old version...
Try downloading a new one from the psml-support branch in Gitlab.
I hope this helps,
Alberto
- El 3 de Feb de 2021, a las 15:30, I. Camps ica...@gmail.com escribió:
| Hello SIESTers,
|
| I am trying to compile
Hi,
Since you are using a recent 'master' version, you might want to look into the
Obj/ARCH-EXPERIMENTAL directory.
There you will find a more structured way of organizing the building.
Alberto
- El 16 de Dic de 2020, a las 10:15, Tamas Karpati tkarp...@gmail.com
escri
(WFSX) file.
Alberto
- El 16 de Dic de 2020, a las 04:19, El-abed Haidar
ehai2...@uni.sydney.edu.au escribió:
| I will have to agree with Alberto because other systems worked when i did not
| specify the energy levels.
| My question then is when i used
| WFS.Energy.Min -5 eV
In the absence of more information (you might want to enable debugging symbols
to see where the error occurs):
- It might be that the energy range you specified does not contain any
wavefunctions (the program should anyway not crash... You might check this with
the Util/WFS/readwfx program).
in:
http://max-centre.eu/webinar/new-developments-siesta-high-performance-materials-simulations
Information on past and future MaX webinars can be found in:
http://max-centre.eu/webinar/
Best regards,
Alberto Garcia
for the Siesta developers
--
SIESTA is supported by the Spanish
of Siesta (including the latest along the rel-4.1 branch in
Gitlab) have an updated Util/readwfx utility with more options and a simpler
interface.
Alberto
- El 4 de Jul de 2020, a las 20:02, Medondjio Linda lindamedond...@yahoo.fr
escribió:
| Dear Siesta user,
|
| I would like to
overview of the Siesta versions available, and where to find them,
please see:
[ https://gitlab.com/siesta-project/siesta/-/wikis/Guide-to-Siesta-versions |
https://gitlab.com/siesta-project/siesta/-/wikis/Guide-to-Siesta-versions ]
Best regards,
Alberto
- El 6 de Mayo de 2020, a las 11
/tree/master
Best regards,
Alberto
- El 3 de Mayo de 2020, a las 11:12, Pablo Aguado
escribió:
| Hi everyone,
| The writing of the WFSX file is not currently implemented in the case of a
| calculation including spin-orbit. Is there any other straightforward way to
| extract the wave
Dear Dr. Popov,
Your unit cell is cubic, and the coordinates show a highly symmetric pattern.
If your
atoms happen to be in centrosymmetric positions, the forces must be zero.
- El 26 de Feb de 2020, a las 19:14, popov po...@ipb.ac.rs escribió:
| Dear Siesta users,
|
| I have got all for
bookeeping artifact, and will not "fold" your phonon
band structure. That is a concept that only applies to electronic band
structures.
So please do use a supercell...
Alberto
- El 4 de Dic de 2019, a las 22:11, popov po...@ipb.ac.rs escribió:
| Hi,
|
| My Siesta calcula
Dear Azadeh,
No, the current Grimme-D method in Siesta is the one using only two-body
potentials. See:
J Comput Chem 25: 1463–1473, 2004 and J Comput Chem 27: 1787–1799, 2006.
Alberto
- El 22 de Septiembre de 2019, a las 07:34, Azadeh Ayatollahie
azadeh.ayatolla...@gmail.com escribió
PI-enabled version of libGridXC.
Alberto
- El 7 de Junio de 2019, a las 16:29, Pablo Aguado pagu...@gmail.com
escribió:
| Hi everyone,
| I'm trying to compile the PSML-compatible version of siesta, but I get the
| error:
|
| siesta_init.F(397): error #6631: A non-optional actual argument mu
of COOP/COHP curves, for example), will not work properly if the
matrix elements of S and H have been "folded". In this case you can use the
'ForceAuxCell' option (see the manual).
Alberto
- El 27 de Feb de 2019, a las 04:15, Mina Sedighi msedi...@uwaterloo.ca
escr
forthcoming version the pool will be made dynamically resizable.
Best regards,
Alberto
> On 12 Feb 2019, at 11:57, Alejandro Martín wrote:
>
> Dear siesta users,
>
> I am struggling with a "Overflow in registry" message in siesta/4.1-b3
> version
> when I try to ru
Hi,
You are using the C++ compiler ('g++') instead of 'gcc' (C compiler). This
causes some
extra name mangling in 'sockets.o' that confuses the linking stage.
Best regards,
Alberto
- El 20 de Noviembre de 2018, a las 04:30, Zhiping Xu x...@tsinghua.ed
/blacsCinit_MPI-ppc64-0.a
/apps/scalapack/64/lib/blacs_MPI-ppc64-0.a -L/apps/scalapack/64/lib -lscalapack
Alberto
- El 22 de Septiembre de 2018, a las 22:00, SPT saravp...@googlemail.com
escribió:
| Hi
|
| Issue is : siesta 4.1-b3 MPI" Installation. I found the following issue and
|
Dear Saif,
There is no difference, really. You compute the forces with ab-initio methods,
and evolve
the ions using Newton's equations with those forces. You had bad luck with the
referee.
Alberto
- El 10 de Jul 2018, a las 23:46, sullah sul...@fisica.ufjf.br escribió:
| Dear Al
To clarify, what Siesta and all the other mentioned packages do is really
“ab-initio molecular dynamics”, as opposed to “molecular dynamics with
classical or effective potentials”.
Alberto
> On 3 Jul 2018, at 01:24, sullah wrote:
>
> Dear Najmeh.
>
> In SIESTA, you ca
Hi,
This is because the .ion file only contains the PAOs and the “scalar” KB
projectors. The extra information
in the .psf file (SO-part of the semilocal pseudopotentials) is needed to build
the spin-orbit contribution
to the Hamiltonian.
Best regards,
Alberto
> On 15 Mar 2018, at 02
Siesta is quite efficient.
For very large systems, if you have access to a large computer, the PEXSI
method (available in version 4.1-b3) might
be suitable.
Or you might want to try the new O(N) CheSS solver, available in the trunk
version in Launchpad.
Best regards,
Alberto
> On 25
lack of SCF convergence, but it
would be harmless (assuming that you
are using the correct DM…)
I hope this helps.
Alberto
> On 24 Jul 2017, at 04:28, Nicolas Duchêne wrote:
>
> Hi all,
>
> I was wondering if there was a way to restart a “calculation” without
>
, whereas your
mesh-cutoff might be on the small side.
Best regards,
Alberto
> On 11 May 2017, at 00:59, nicolas.duch...@polymtl.ca wrote:
>
> Greetings SIESTA users,
>
> I’m a new user, and have made attempts at modelling a silver nanocluster of
> 13 atoms (ic
Hi Ian,
Please make sure that you are using GNU make. We use the VPATH feature to find
source files in other directories.
Also, try to do a “make clean” in case there is some previous corruption.
Best regards,
Alberto
> On 24 Apr 2017, at 13:46, Ian Shuttleworth wrote:
>
>
,
Alberto
> On 2 Mar 2017, at 10:35, Mark Iron wrote:
>
> Dear all,
>
> I need to run some calculations for CaCO3 crystals. Because of the nature of
> the problem (I need the vibrational frequencies of large unit cells) I need
> an order(N) method, which is available in
Hi,
In your arch.make, replace -DNCDF by -DCDF, type “make clean” and “make”.
Alberto
> On 30 Jan 2017, at 11:33, RAJAN SINGH wrote:
>
> Dear Siesta users
>
> I am facing following errors while trying to install 4.1-b1 in parallel mode
> with NETCDF:
>
> Fatal
to preserve the coordinates, use the SystemLabel.STRUCT_OUT file,
renaming it to SystemLabel.STRUCT_IN, and use
the option
Use.Struct.File T
Alberto
> On 27 Jan 2017, at 02:25, Seyed Mohammad Tabatabaei wrote:
>
> Dear all,
>
> I have a converged .DM file from a previous c
The files are of the form SystemLabel.Extension.
In your case, input-ok-og.DIM, etc.
Alberto
On 24 Oct 2016, at 08:14, Marco Fronzi wrote:
> Dear Siesta Users,
>
> I am trying to plot charge density and wavefunction using denchar.
> In the working directory I put the followin
Hi,
Indeed, the CONTIGUOUS keyword is a F2008 feature, not implemented yet in all
compilers.
For now you can apply the patch attached to
https://bugs.launchpad.net/siesta/+bug/1619437
to fix this problem, or simply delete the CONTIGUOUS keyword.
Best regards,
Alberto
On 14 Sep 2016
at the file
Src/Sys/DOCUMENTED-TEMPLATE.make and at other examples in Src/Sys. You have
probably done that to find out about FC_SERIAL.
Best regards,
Alberto
On 14 Sep 2016, at 09:00, Mersad Mostaghimi wrote:
>
> Dear developers,
> In compiling siesta-4.0.0 with mpiifort there i
Hi,
Thank you for the report.
There is indeed a bug in the implementation of the -DSIESTA__NO_MRRR option.
A patch is available. See: https://bugs.launchpad.net/siesta/+bug/1622526
Regards,
Alberto
On 09 Sep 2016, at 17:03, Jariyanee Prasongkit
wrote:
> Dear Siesta team,
>
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
We are pleased to announce the release of Siesta-4.0.
This version should be the default choice for production for most users.
You can read the Release Notes and obtain the tarball in the release page:
http://launchpad.net/siesta/4.0/4.0
Note in particular the BACKWARD COMPATIBILITY ISSUES an
beta very soon.
Best regards,
Alberto, for the Siesta developers.
On 20 May 2016, at 16:51, Grigory Shamov wrote:
> Dear Alberto,
>
> Is this retroactive? I.e., do we still protect older SIESTA versions,
> asking users to agree to the old Academic access licenses?
>
> --
Dear Grigory,
That is good question... and I am not sure yet what the best answer is.
We are having a developers meeting at the end of the week. I will raise the
issue then and will let you know.
Best regards,
Alberto
On 20 May 2016, at 16:51, Grigory Shamov wrote:
> Dear Albe
-structure calculation in the same run. Since
the
k-point coordinates for the band-structure calculation are computed at the
beginning of the run, they would be appropriate for the initial cell, not the
final one. This can be considered a bug or a feature...
Alberto
On 19 May 2016, at 03:13, Zhang
-relaxation run, as the k-points would be appropriate for the original
cell.
Regards,
Alberto
On 18 May 2016, at 12:18, Zhang Aihua wrote:
> Dear All,
>
> I have noticed that if I do a single-point band structure calculation with
>
> UseStructFile true
>
> and simul
The SIESTA developers have decided to change the licensing conditions for the
code. From now on, SIESTA will be released under the GPL open-source license
(https://en.wikipedia.org/wiki/GNU_General_Public_License).
In the past SIESTA had always been free for academic use, but re-distribution
w
budget is tight you can
get the free Gfortran compiler.
Alberto
On 06 Apr 2016, at 09:33, Nick Papior wrote:
> Please try and update your compiler.
> You should use a 2003 compliant compiler.
>
> 2016-04-06 7:30 GMT+02:00 Suman deep :
>> sir,
>> i m getting the following
format,
using the tools in Util.
As of now there is no direct output of the "partial density matrix" in an
energy-window, so Denchar (which need a DM) cannot be used. If you are
interested you could modify the code yourself to insert a call to the routine
that outputs density matrices
by that of
the vdW functional to be used.
This note will be added to the Siesta documentation as soon as possible.
Best regards,
Alberto
On 17 Feb 2016, at 00:56, I. Camps wrote:
> Hello Ticu,
>
> You have to generate your own vdW-DFT pseudos.
>
> What I did:
> - Downlo
Hi,
The spin-orbit interaction is not yet included in the released version of
Siesta. It will be in the next few months.
Regards,
Alberto
On 10 Feb 2016, at 09:32, Abdullahi Lawal wrote:
> Dear Siesta user.
> Please some body should help me, i want to calculate the stru
newer siesta-4.0b version.
There is no point in using trunk-462. You should download siesta-4.0b.
Alberto
On 08 Feb 2016, at 10:33, RAJAN SINGH wrote:
> Actually I am getting same errors as one person face when installing Siesta
> 4.0 version. (http://www.mail-archive.com/siesta-l%40
Hi,
1. Please copy Src/Sys/nolibs.make to Obj/arch.make.
2. Change the name of your compiler if needed in arch.make.
3. In Obj, type "make clean" and then "make"
Regards,
Alberto
On 04 Feb 2016, at 10:50, Zaw Myo Win wrote:
> Dear Alberto,
>
If you are not using an external lapack+blas library, you should use
COMP_LIBS=linalg.a
in the arch.make file to compile all the linear-algebra code in Src/Libs.
Version 4.0 needs extra code that is not in the file Src/Libs/lapack.f.
See Src/Sys/nolibs.make.
Regards,
Alberto
On 04
Please see the "Local Density of States" section of the manual.
On 30 Jan 2016, at 11:35, Anju Saroha wrote:
> Hi to all,
>
> I am having a doubt in plotting charge density in 3D mode. I tried using
> DENCHAR utility program. I want to know how one can plot charge density in
> some specific e
Dear Jin,
The 'STRUCT' file must be in a special format produced by Siesta. Every run
produces by default a .STRUCT_OUT file. This is
the one you need to use. The xyz format is not supported by g2c_ng.
Alberto
On 02 Jan 2016, at 03:08, Jingxian Yu wrote:
> Dear Alberto
Hi,
In the new version siesta-4.0b available at the Siesta website there is an
updated grid2cube (named g2c_ng)
in the Util/Grid directory that can handle non-orthorhombic cells.
Regards,
Alberto
On 31 Dec 2015, at 11:20, Nick Papior wrote:
> I have created a small utility in pyt
We are happy to announce the availability of a beta version of the
upcoming Siesta 4.0 release.
This version includes the van der Waals functionals, the new
load-balancing code for real-space grid operations, a Wannier90
interface, a new Orbital-Minimization-Method solver, and other
improvements a
This is a semi-automatic periodic posting to the Siesta mailing list.
The mailing list can be a good resource for everybody, provided that we can
abide by a few common-sense guidelines:
* Before posting, make sure that you have made a fair effort at learning about
the issue in the documentatio
Hi,
You want the 'prefix.bands' file. The .BONDS file contains bond-length
information...
By the way, if you use the 'pi/a' option for the k-point scale, make sure that
you
have a
LatticeConstant XX.XX
line in your input file.
Regards,
Alberto
On 16 Jul 20
Hi Mike,
The FoX library does not contain any MPI calls, so it does not need mpif90 for
compilation. However, if you link it with a code (such as Siesta) with MPI
calls, then you do need to link it with mpif90.
Regards,
Alberto
On 11 Jul 2014, at 22:10, Michael R. C. Williams
wrote
version, the manual found under the
"Documentation" hierarchy of pages might not be in sync with the latest
released snapshot. These manuals are provided for the convenience of quick
lookup of standard options.
Best regards,
Alberto
On 08 Jul 2014, at 21:08, Michael R. C. Willia
(e.artacho _at_
nanogune.edu)
Alberto Garcia, Institut de Ciencia de Materials de Barcelona (ICMAB-CSIC)
(albertog _at_ icmab.es)
* Instructors:
Jose Soler, Universidad Autonoma de Madrid
Georg Huhs, Barcelona Supercomputing Center
Javier Junquera, Universidad de Cantabria
Emilio Artacho, CIC
Organizers:
Emilio Artacho, CIC NanoGUNE Consolider, Donostia-San Sebastian (e.artacho _at_
nanogune.edu)
Alberto García, Institut de Ciencia de Materials de Barcelona (ICMAB-CSIC)
(albertog _at_ icmab.es)
* Instructors:
Jose Soler, Universidad Autonoma de Madrid
Georg Huhs, Barcelona Supercomput
the fix to the development version will follow soon.
My apologies to Alexander Vozny for missing his earlier report about the
problem.
Best regards,
Alberto
d10
they are not adequate. But do you really need the spin polarization? Note that
the original source you quote used a relativistic pseudo, which is the standard
practice, even for calculations in which you are later going to consider spin.
Regards,
Alberto
On Nov 28, 2013, at 7:33 PM, I
Hi Herbert,
Siesta is also able (as of 3.2) to do Hirshfeld and Voronoi charge
partitioning analyses.
Alberto
On Thu, Jun 20, 2013 at 3:21 PM, Herbert Fruchtl <
herbert.fruc...@st-andrews.ac.uk> wrote:
> Just to add to the discussion that started with the question about PDOS
>
Hi Benedikt,
SIESTA does not need projections, as the basis orbitals are localized on
the atoms. You get naturally the "chemical" information one is used to.
Plane-wave codes such as vasp do need projections to get some kind of
"local" information from the delocalized basis.
better than what you get with 3.X. If you spend a significant fraction of the
CPU time of your runs in dhscf, this will make a difference. If not, you could
increase the mesh cutoff or the size of your box to be able to use more
processors for the diagonalization part.
Best regards,
Alberto
We have released a new Siesta development snapshot (trunk-433) which includes:
- The implementation (by Fabiano Corsetti) of an orbital-minimization
method without localization that can be used as an alternative to
diagonalization.
- The JobList suite of utilities (by Jose Soler) to organize,
We are happy to announce the release of Siesta 3.2.
Users are encouraged to use this version for production runs.
You can find the Siesta 3.2 release in the "Access
to the code" section of the Siesta website.
To report any remaining issues, see Docs/REPORTING_BUGS
Thanks for your patience and c
Dear Siesta users,
We have corrected several bugs and inconsistencies in the development version,
and released a new snapshot (trunk-427).
Some of the improvements affect the new TranSiesta and TBTrans code contributed
recently by Nick Papior Andersen, of the Technical Univ. of Denkmark.
The
Liu,
You should upgrade to the latest versions, both along the 3.X branch
and the development ("trunk") branch.
Alberto
On Thu, Nov 8, 2012 at 7:42 AM, liuyunlong0902 wrote:
> Thanks for your suggestion. Here I include the input and output file, which
> is just an example
NETCDF_INCLUDE
seems to be a fossil used by the old configure mechanism.
Please see Src/Sys/DOCUMENTED-TEMPLATE.make for a full explanation of
the variables used.
Best regards,
Alberto
On Wed, Oct 31, 2012 at 5:42 PM, Guangping Zhang wrote:
> Dear users and developers:
>
> I have encout
things to watch out
for and explore in the new version.
To report any remaining issues, see Docs/REPORTING_BUGS
Thanks for your patience and continuous support.
The Siesta team
October 31, 2012
Dr. Alberto Garcia -- Email: alber...@icmab.es
Institut de Ciencia de Materials de Barcelona - C
fixes.
We would be grateful for any bug reports. Please follow the guidelines in the
Docs/REPORTING_BUGS file.
Regards,
Alberto
Dr. Alberto Garcia -- Email: alber...@icmab.es
Institut de Ciencia de Materials de Barcelona - CSIC
Campus de la UAB, E-08193 Bellaterra, SPAIN
Tel: +34-93
Hi Bing,
This is a cosmetic bug that only affects the creation of the optional XML file.
The psf file would still be correct.
The bug has been fixed in siesta-3.1-pl18, available on the Siesta website.
Alberto
On Oct 12, 2012, at 4:01 AM, Huang Bing wrote:
> Hi, siesta users
>
>
Hi, Brad,
Please try the updated version (siesta-3.1-pl11) from the Siesta website.
Best regards,
Alberto
On Sat, Oct 6, 2012 at 6:32 AM, Brad Wells wrote:
> Hi Siesta Users,
>
> I am interested in using the new Hirshfeld code for calculating partial
> charges, as th
Dear Siesta users,
A new development snapshot (siesta-trunk-408.tgz) is available for download by
eligible users at the Siesta website.
This snapshot contains the latest bugfixes, and is a step closer to a
beta-relase that will include the new functionality we have been
working on since the 3.0
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