J K wrote:
>> What else could one try, to get the wfc somehow converged?
Paolo Giannozzi wrote:
>hard to say (especially withouth the ouput). Are you sure that spin
>polarization
>is not a source of trouble close to the transition state?
I have not tried this up to now, because i would
On Mon, 13 Oct 2008, Leonardo Matheus wrote:
LM> Hello,
hello leonardo,
LM> I'm trying to calculate Hirshfeld charges as a postprocess. To do so,
LM> I need to obtain the atomic rho for each atom, in real space. I've
LM> seen that "atomic_rho.f90" calculates the total rho as a superposition
LM>
Hello,
I'm trying to calculate Hirshfeld charges as a postprocess. To do so,
I need to obtain the atomic rho for each atom, in real space. I've
seen that "atomic_rho.f90" calculates the total rho as a superposition
of the individual atomic ones, obtained from the pseudopotentials.
But I couldn't
On Mon, 13 Oct 2008, Nguyen Ngoc Ha wrote:
NNH> It's a reaction H2+H = H+H2, the reaction chosen to be test but please
note that phase_space = coarse-grained.
NNH> > Why are you fixing the middle atom? I believe in this
NNH> > example you don't
NNH> > need to fix any atom (I assume its a
On Mon, 2008-10-13 at 10:03 +0200, Marcello Rosini wrote:
> Hi everybody,
> I had a problem with xcrysden when reading the output of a pw 4.*
> relaxation. The problem is that in the output also the fixed flags of
> the atom coordinates are present, while it was not so in the previous
>
On Sun, 2008-10-12 at 16:56 -0700, Paul M. Grant wrote:
> How does one make an animated axsf file using XCrySDen directly? For
> example, suppose I want save in an axsf file the animation of an
> isosurface of charge density moving through a given unit cell.
The *.axsf file is meant for
On Mon, 13 Oct 2008, Paul M. Grant wrote:
PG> Thanks, again, Axel.
PG>
PG> You probably know ImageMagick can be incorporated into XCrySDen, along with
PG> the "animation tools" Whirlgif and mpeg_encode. However, the latter two
PG> will not be "raised" by XCrySDen unless the file type is axsf.
On Mon, 13 Oct 2008, Paul M. Grant wrote:
paul,
PG> To begin with, let me see if I understand some of the basics of the *.save
PG> folders:
PG> 1. pw.x with the scf option saves the scf charge density and spin data in
PG> two binaries named charge-density.dat and spin-polarization.dat (is there
On Mon, 13 Oct 2008, Janos Kiss wrote:
hi janos,
JK> I was also concerned about this aspect, but when i did a quick and
JK> rough test calculation, the wfc convergence was not particularly better,
and
JK> one SCF step took a lot longer time. Therefore, i just killed it
impatiently
JK> iirc.
On Mon, Oct 13, 2008 at 12:53 AM, Paul M. Grant wrote:
> Axel, thanks for getting back on this. Let me think about your suggestion
> and see what others have to comment as well.
>
> Reflecting on "animation" in general a little more, I wonder if there's a
> Linux screen capture tool available
Here is my input
calculation = 'smd' ,
restart_mode = 'from_scratch' ,
outdir = '/home/hthp/Desktop/TMP/' ,
pseudo_dir =
'/home/hthp/Desktop/QUANTUM/espresso-4.0.2/pseudo/' ,
prefix = 'H2+H' ,
/
On Oct 13, 2008, at 16:15 , Nguyen Ngoc Ha wrote:
> ATOMIC_POSITIONS angstrom
> first_image
> H -2.4165926530.00.01 0 0
> H 0.00.00.00 0 0
> H 0.8243343410.00.01 0 0
>
On Oct 10, 2008, at 19:15 , Janos Kiss wrote:
> Is this behavior completely normal in an NEB calculation with
> PWSCF, or this
> is an issue with my particular system/setup only?
the latter you say, and a bit of the former as well: your particular
system seems
to be a nasty one, and NEB
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On Oct 13, 2008, at 6:37 , Paul M. Grant wrote:
> [...] the method used to calculate the mesh used for the
> aluminum example of epsilon.x is unclear (at least to me).
which aluminum example of epsilon.x you are referring to?
Paolo
---
Paolo Giannozzi, Dept of Physics, University of Udine
via
Thanks, again, Axel.
You probably know ImageMagick can be incorporated into XCrySDen, along with
the "animation tools" Whirlgif and mpeg_encode. However, the latter two
will not be "raised" by XCrySDen unless the file type is axsf. You're
suggestion to use ImageMagick is a good one and I'll
Look in the PH directory and not PW or PP? How obvious! Should'a thought
about that myself (just kidding, ;-)!
I knew that e-p calculations produced a table of N(Ef) as a function of
broadening parameter, but figured that route was even more clumsy than the
ones I've been pursuing...and anyway,
Gladly,
this is my third attempt at posting this reply, I cannot paste the
.axsf file or attach it, because its too large. The message bounces
back to me with a "moderator approval pending" message. I think
approval is still pending, so I apologize for making you download the
file from a 3rd
On Sun, 12 Oct 2008, Paul M. Grant wrote:
paul,
PG> Axel, thanks for getting back on this. Let me think about your suggestion
PG> and see what others have to comment as well.
it is actually quite difficult to give a recommendation,
since everybody uses a different nomenclature when it comes
On Oct 13, 2008, at 1:47 , Paul M. Grant wrote:
> There must be an easier way to get the density-of-states at the
> Fermi level
>
I think that the simplest way is to use function dos_ef,
in PH/elphon.f90
P.
---
Paolo Giannozzi, Dept of Physics, University of Udine
via delle Scienze 208, 33100
Hi everybody,
I had a problem with xcrysden when reading the output of a pw 4.*
relaxation. The problem is that in the output also the fixed flags of
the atom coordinates are present, while it was not so in the previous
versions.
I modified few lines in the source code, in order to make
;*
> *>* Wang
> *>* **
> *>*
> *
>
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Dear PWscf users,
I like using SMD and Metadynamics to investigate free energy suface (That
implemented in PWscf code) but I see there are so few of examples for SMD.
For testing purpose only with phase_space = 'coarse-grained', I'm still failed.
Here is my input:
...
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