Hi, Juliana,
you can find attached a slightly modified version of the program gnubands. It
generates two files, bands-up.dat and bands-down.dat.
Best regards,
Roberto
From: Juliana Morbec
To: siest...@listserv.uam..es
Sent: Sunday, January 25, 2009 2:13:09 A
an 16, 2009 at 10:27 PM, Roberto Veiga wrote:
Ok, so I have how to know if the reaction is endothermic or not just by
calculating the four isolated systems (the two reactants and the two products).
But in order to know if the reaction is spontaneous for T>0, I have to compute
also the chang
ess...
Roberto
From: N H
To: SIESTA-L@listserv.uam.es
Sent: Friday, January 16, 2009 10:11:41 PM
Subject: Re: [SIESTA-L] Hess's law
If you have correwctly calculated all intial and finals states the answer is
yes!
On Fri, Jan 16, 2009 at 10:02 PM, Rober
Hello,
if I have a substitution reaction as follows:
AB+CD-->AC+BD
and I calculate the four systems isolated with Siesta, can I calculate the
enthalpy of such a reaction as stated by the Hess's law? Or there is any
subtlety?
Thanks in advance,
Roberto
?
Thanks in advance,
Roberto Veiga
Oleksander,
I know. As I said, I am just trying to find out, maybe in a desperate way, how
to correctly calculate the solvation enthalpy of carbon in alpha-iron with
Siesta in order to be able to reproduce results in the literature, which have
been obtained with plane-waves. What I sent you was
stability of the
iron phases, TZ is enough. This base was used to check the convergence of the
total energy with the basis set.
-Original Message-
From: Siesta, Self-Consistent DFT LCAO program, http://www.uam.es/siesta on
behalf of Roberto Veiga
Sent: Wed 1/7/2009 21:10
To
What you are calculating here is the cohesive energy, calculated via lone
C atom which is completely different from it's energy in graphite.
Well, I am just trying to figure out what to do, maybe in wrong ways most of
time. Up to now, the best result I obtained for C interstitial in ir
That would be great, really. I did that in this way (for what I called DZP-DZP):
%block PAO.Basis
Fe 2
n=4 0 2 P 1
0.000 0.000
n=3 2 2 P 1
0.000 0.000
%endblock PAO.Basis
Then I varied EnergyShift and SplitNorm iteratively w
The polarization orbital (only one) is applied atop of other orbitals in
the basis, i.e. you cannot have P for both s and d. That's why DZP-DZP
sounds weird.
Hmmm... I did not know that. Thanks!
To be frank, I need to be less lazy and go deeper into the Siesta paper (it is
here
you
cannot reach a quantitative agreement at all, neither with experiments nor PW.
Of course, I know you cannot apply the correction only when it interests you...
Thanks,
Roberto Veiga
From: Oleksandr Voznyy <[EMAIL PROTECTED]>
To: SIESTA-L@listserv.uam.es
out how to apply the correction. If I replace E(Fe16) by E(Fe16+C_ghost)
and E(C) by E(C+Fe16_ghost), things become worst. Does anyone have any idea on
how apply a BSSE correction in this case?
Thanks in advance,
Roberto Veiga
do
On 04/11/2008, at 11:38, Roberto Veiga wrote:
Thank you, Eduardo. How do I obtain the total number of basis functions for a
condensed system? Should I take into account more than the atoms explicitly
defined in my input?
Roberto
From: Eduardo Anglada &
s
Sent: Tuesday, November 4, 2008 9:45:34 AM
Subject: Re: [SIESTA-L] Bulk cohesion energy
Hi,
At the beginning of each SIESTA run, during the generation
of the atomic orbitals, the number of basis functions for each
species is written.
Best
Eduardo
On 03/11/2008, at 21:05, Roberto Veiga wrote:
Where in the output can I find the number of basis functions?
Roberto
From: Oleksandr Voznyy <[EMAIL PROTECTED]>
To: SIESTA-L@listserv.uam.es
Sent: Monday, November 3, 2008 3:41:53 PM
Subject: Re: [SIESTA-L] Bulk cohesion energy
> I did like that:
> E=E(Fe-bulk
4.78
eV, and the experimental value is 4.28 eV. So I think that in this case the
BSSE correction is negligible.
Thanks,
Roberto Veiga
PhD student
INSA-Lyon
PS.: As a suggestion: it would be nice if some Siesta advanced users provide us
with some useful examples on how to calculate things like bi
Yes. But you have to do it with identical grid.
And also don't forget about basis set superposition error (BSSE) corrections,
i.e. your single atom should have the ghost atoms around it in the same
geometry as in your bulk (nearest neighbors would be enough).
Ok, but, see, the bcc Fe unit
Hi:
I would like to know how to calculate the bulk cohesion energy of a crystalline
solid (in my case, Fe) with Siesta. I guess it is the difference between the
total energies of the atom in the bulk and the isolated atom.
Thanks,
Roberto
Hello:
I would like to know how to generate a pseudopotential including some of the
core electrons in it, besides the usual valence ones. A simple sample input
would be nice.
Thanks in advance,
Roberto
I got a problem doing that... the formation of a vacancy is exothermic! If I do
the calculation in this way:
Ef=Et(64)-Et(63)-Et(64)/64
C'est bizarre!
Roberto Veiga
PhD student
INSA-Lyon
- Original Message
From: Pablo A. Denis <[EMAIL PROTECTED]>
To: SIESTA-L@listserv.
Ok, but allowing the system to relax with the ghost? I mean, would not the
ghost atom have any (artificial) affect to the final optimized geometry?
[]s,
Roberto Veiga
- Original Message
From: Oleksandr Voznyy <[EMAIL PROTECTED]>
To: SIESTA-L@listserv.uam.es
Sent: Wednesday, Au
bulk/64)/64...
Eformation = E(64)- E(63) - E(64)/64
if you need N2 you use N2 for example or NH3...
etc...
best regards,
pablo
- Original Message -----
From: Roberto Veiga
To: SIESTA-L@listserv.uam.es
Sent: Sunday, August 03, 2008 3:13 PM
Subject: Re
From: Roberto Veiga
To: SIESTA-L@listserv.uam.es
Sent: Friday, August 01, 2008 10:08 AM
Subject: [SIESTA-L] Vacancy formation energy
Hi, everybody:
I would like to calculate the formation energy for a single vacancy in
bcc-iron (64-atoms supercell). The more obvious way (at least it is
? Is it completely wrong?
Roberto Veiga
PhD student
INSA-Lyon
y with:
Diag.DivideAndConquer False
Regards
Eduardo
On 10/07/2008, at 13:24, Roberto Veiga wrote:
Sorry. I forgot to give a title to the message.
Roberto
- Forwarded Message
From: Roberto Veiga <[EMAIL PROTECTED]>
To: SIESTA-L@listserv.uam.es
Sent: Thursday, July 10, 2008 1:17:3
Dear Eduardo:
are those pseudopotentials for metals, without partial core correction,
suitable for, ahn, "useful" calculations?
[]s,
Roberto Veiga
PhD student
INSA-Lyon
- Original Message
From: Eduardo Anglada <[EMAIL PROTECTED]>
To: SIESTA-L@listserv.uam.es
Sent:
anymore. Besides, if you remove the
SuperCell block, it works like a charm.
A+,
Roberto
- Original Message
From: Alexandre Lebon <[EMAIL PROTECTED]>
To: "Siesta, Self-Consistent DFT LCAO program, [EMAIL PROTECTED]
http://www.uam.es/siesta"; <[EMAIL PROTECTED]>;
Sorry. I forgot to give a title to the message.
Roberto
- Forwarded Message
From: Roberto Veiga <[EMAIL PROTECTED]>
To: SIESTA-L@listserv.uam.es
Sent: Thursday, July 10, 2008 1:17:31 PM
Subject: [SIESTA-L]
Hello everybody:
I had the following problem when trying to perfor, a
works if the SuperCell block is not available. As one can see,
it is based on the input for Fe in Siesta examples directory.
Any idea?
[]s,
Roberto Veiga
PhD student
INSA-Lyon
Hello everyone:
does any of you have (and would like to share) optimized basis for bcc-Fe?
Regards,
Roberto
PhD student
INSA-Lyon
Yes, there is a post-processing tool for PDOS in the Util directory
(pdosxml, somehting like that). The only problem with it is... you
have to change the code and make it every time you want to plot
another orbital. That is boring, hehehe!
Regards,
Roberto
2007/10/16, Lindsay Shuller <[EMAIL PRO
Hi:
I'm gonna do some spin polarized calculations in which molecular
oxygen is adsorbed onto a surface. I'd like to know how to represent
triplet oxygen (as initial state) in the Siesta's input.
Regards,
Roberto
--
"If I have seen farther than others it is because of a myopia surgery."
Dear all:
can anyone suggest to me a simples input file for a graphene sheet?
Regards,
Roberto Veiga
Dear Navaratnarajah:
here you have capped (5,5) and (10,0) nanotubes. I hope it be useful for
you.
Regards,
Roberto
2006/7/13, navaratnarajah kuganathan <[EMAIL PROTECTED]>:
Dear Siesta users,
I am performing calcualtions on carbon nanotubes.Could you please suggest
any method for generatin
radially
deformed.
Regards,
Roberto Veiga
2006/6/26, Michael Shin <[EMAIL PROTECTED]>:
Thank you much *navaratnarajah kuganathan *
I solved that problem now, but I observed one thing that how can we find
the width of the Gaussian broadening for Nanotubes bcos wen I chnage
Gaussian broadening
Hi,
does anyone have a LDA pseudo for Fe?
[]s,
Roberto
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