Dear Asa
You have to explicitly say all atoms. The polarization is per-atom,
and not per-species.
regards
Lucas
On Tue, Apr 7, 2009 at 09:36, asa aravindh mails2...@gmail.com wrote:
Dear Ricardo..
Thanks for your reply.. actually what I meant is ,, if all atoms are
polarised..
is it enough
I meant GDIS... which supports (among others) SIESTA (and GULP) input files...
On Fri, Apr 3, 2009 at 22:40, Lucas Fernandez Seivane
queve...@gmail.com wrote:
try GULP
On Fri, Apr 3, 2009 at 20:41, Ary Junior aryjun...@gmail.com wrote:
Hi all, is there any graphical user interface
try GULP
On Fri, Apr 3, 2009 at 20:41, Ary Junior aryjun...@gmail.com wrote:
Hi all, is there any graphical user interface for maintain siesta input
files?
Thanks very much!!!
Hi Sarah
in the block you put the energy gap you want to plot. Therefore, you
should run siesta twice and in two separate directories,
one in a energy range that just contais the HOMO and another one for the LUMO
If they are at HOMO: -3.29089 and LUMO: -3.17099
%block LocalDensityOfStates
that for finding the HOMO and
LUMO we should look at the EIG file. Is it the only way to do so?
On Sun, Feb 22, 2009 at 7:40 PM, Lucas Fernandez Seivane
queve...@gmail.com wrote:
Hi Sarah
in the block you put the energy gap you want to plot. Therefore, you
should run siesta twice and in two
Dear Lamjed
I succesfully built siesta in solaris 10 using sun compilers, you can
get them at http://developers.sun.com/sunstudio/downloads/index.jsp.
Regards
On Fri, Feb 20, 2009 at 1:22 PM, Lamjed debbichi
lamjed.debbi...@ipcms.u-strasbg.fr wrote:
Dear siesta users
i would like to install
Dear All
Look at the input. Your system is too small to see any benefit from
parallelizing over orbitals (default behaviour):
initatomlists: Number of atoms, orbitals, and projectors: 64 256 576
* Maximum dynamic memory allocated =16 MB (this is per node, so
probably 8*16=128 MB or
Dear Swaroop
Please look for an .XV file (or maybe a .STRUCT one) to see if the cell
sizes you are writing are there (.XV is in Bohr!)
all the best
lucas
On Fri, 23 May 2008, M.Sairam Swaroop wrote:
Dear Eduardo
After you mentioned i noticed tha the mesh does not change ... i have
Hi to all
What about setting a reasonabla LatticeConstant??? look in out.fdf for
LatticeConstant and copy the variable... in case there is no one just set
it to something like 8 A, should be enough (but I may be wrong)
Regards
On Fri, 18 Aug 2006, Weili Wang wrote:
Thanks, Dear Rurali,
Dear Nichols
Set
DM.MixSCF1 T
Otherwise, no mixing is performed upon restarting so dDmax grows a lot!!
See the manual:
'DM.MixSCF1
(logical): Logical variable to indicate whether mixing is done in the
first SCF cycle or not. Usually, mixing should not be done in the first
cycle, to
Dear Weili
This problem is not SIESTA related but compiler related. I assume you are
compiling siesta with intel fortran compiler. This symbol is part of the
libraries of the compiler. Does 'ldd siesta' give any warning? Is the
variable LD_LIBRARY_PATH defined? If you do 'echo
Hi to all
Take a look at the atom makefile, and change f77 to an appropiate fortran
90 compiler (like the one you are currently using to compile siesta)
Best wishes
Lucas
On Tue, 27 Jun 2006, Chin-Cheng Su wrote:
Hi all,
In siesta's sub-folder /Pseudo/atom, I got the error message when
Hi
The energy in Siesta is not variational with the mesh. It is absolutely
convergent, though (the oscilations in energy decrease with the increasing
of the mesh). Take a look at http://arxiv.org/abs/cond-mat/0406424 (Figure
1) for an example with iron
Best regards
On Tue, 27 Jun 2006,
What about writing some shell script such as
cat in.fdf | siesta output.o
and run it with mpirun?
best wishes
Lucas
P.S.: By the way, it usually is a fault of mpirun and not of the code in
question (in this case SIESTA).
On Thu, 8 Jun 2006, Jose Luis Rodriguez-Lopez wrote:
Dear siesta
Dear Rob
Does the file mpi_siesta.mod actually exist in the Src folder? in case it
does not, enter in the Src/MPI folder and type make. Does it give any
output? Type make pi3 and try to run the program. Does it run?
In case the modules cannot be built, what's the output of ifort -V? mine
Are you using a block like this?
BandLinesScale pi/a
%block BandLines # These are comments
1 0.000 0.000 0.000 \Gamma # Begin at Gamma
50 2.000 0.000 0.000 X # 25 points from Gamma to X
20 2.000 1.000 0.000 W # 10 points from X to W
30 1.000 1.000
In fact, the simulation runs but gives warnings. So if you are asking if
SIESTA would run, it will, but the ressults probably would not be very
good.
Best Wishes
# Ph.D. Student Lucas Fernández Seivane Tlf:
I think the bigger the pulay means a bigger 'average of SCF steps' is
taken into account, so the convergence should be quicker... but your
mileage may vary...
Best Wishes
# Ph.D. Student Lucas Fernández Seivane
What about doing a wrapper in bash? something like
#!/bin/bash
cd /home/quevedin/Si-nuevos/lattice/so/5.445
. /etc/profile
echo Running siesta
cat Si.fdf | ./siesta
Best Wishes
Lucas Fernández Seivane
Universidad de Oviedo
Oviedo, Asturias, SPAIN
SIESTA always uses periodic boundary conditions. There is a default box size,
I think it's cubic and its default side must be specified in the manual. You
had better specify it explicitly, in whatever shape and size you feel is
appropriate.
No, if you just put the position of the atoms in
Hi alex, I give you a brief report:
# Au 0 6 1 01.
#(species label, l, n, z, is_polarized, popul)
I think these are self-explanatory.
Radius Value of the radial part
0. 1.01031937732
0.620708387692E-02 1.01031715705
Have you tried with relativistic pseudos (puttig pbr instead of pbs)? You
may also find some improvement.
Best wishes
# Ph.D. Student Lucas Fernández Seivane Tlf: (+34) 985 102946 #
# Departamento de Fisica,
Hi Aleksey
The output files ORB.something are the radial part of the orbitals (I
think you have to multiply them by r**l).
Best wishes
# Ph.D. Student Lucas Fernández Seivane Tlf: (+34) 985 102946 #
#
I personally use
FFLAGS= -w -mp -tpp7 -xW -O3 -static
but your mileage may vary, specially with the -x thing
Foi um prazer
# Ph.D. Student Lucas Fernández Seivane Tlf: (+34) 985 102946 #
# Departamento de Fisica,
Hi to all the community
In the siesta.F file, when calculating the number of supercells the code
is like this: (lines 689-701)
C Find required supercell
do i = 1,3
mscell(1:3,i) = 0.0_dp
if (gamma) then
nsc(i) = 1
mscell(i,i) = 1
else
Hi to all
It is completely posible, in fact the Oviedo group uses it a lot on a 12
PCs cluster (Pentium 4, ethernet100). As
a lot of people has noted here, you have to take care to compile all the
libraries properly (BLAS, LAPACK, SCALAPACK).
As other people has previously told, if you really
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