Dear Eduardo Anglada,
Last month I have posted asimilar question
about Qtot in some spin polarized GGA calculations. in my case Qup = 126.5 and
Qdown = 126.5. The correct values shold be 127 and 126. I did not have
incomplete scf convergence or an excesive el
Dear Ren,
it is not possible to obtain a good interlayer
interaction with PBE. Check the literature and you will find that more many
VDW interactions is repulsive. LDA may give some acceptable results but just
by a fortuitous error cancelation.
All the DFT methos fails whe
Dear Siesta user,
I have recently installed Ubuntu 7.1 on a
core 2 duo machine. I would like to know if somebody has installed siesta on
it? I have been able to install ifort and mkl but when I try to compile the
atom program or siesta the congifure.log tells me
hi roberto,
I think that you may replace Et(1) by E(64)/64. perhaps the
other users can correct me, if I am making a mistake...
best regards,
pablo
- Original Message -
From: Roberto Veiga
To: SIESTA-L@listserv.uam.es
Sent: Friday, A
calculate the formation energy of a single vacancy in a 64-atoms bcc lattice?
[]s,
Roberto
- Original Message
From: Pablo A. Denis <[EMAIL PROTECTED]>
To: SIESTA-L@listserv.uam.es
Sent: Monday, September 1, 2008 10:39:54 AM
Subject: Re: [SIESTA-L] Vacancy formation energy
I think that there is another issue that may be more important. the orbital
confining cut-off. Are you using the default PAO.EnergyShift = 0.02 Ry? The
default values is way too large...
The results can change a lot if you use larger values. In you case I would
try with 0.01 Ry and 0.001 Ry. The
Hi Stephan,
I do not think that this is a ''great'' difference, but
maybe you can try with a smaller PAO.EnergyShift, 0.001 Ry...
best regards,
pablo
- Original Message -
From: Stefan Leiding
To: SIESTA-L@listserv.uam.es
Sent: Monday
Hi Yusia,
my experience with siesta is small so maybe I am wrong, but
for the Energyshift it is better to have a smaller value so the cut-off radius
of the orbitals is longer and thus, the basis set is more extended. Also, a
smaller PAO.EnergyShift reduces the BSSE very much.
Dear Siesta users,
I have a problem on how it is defined the
chemical potential of nitrogen if I use NH3. It is correct to estimate it in
this way:
Energy(NH3) = u(N) + 3u(H)
-Energy(NH3) is the total energy of NH3
-u(H) is the chemcial potential of H, for whi
Thank you very much for your answers Ian and Andrei.
The smearing (5K) improved the situation. The spin up is 123.7 and the spin
down 123.3, but there is 0.3 spin in the wrong place. The energy is nearly
the same, only 0.0005 eV lower, thus at least in energetic terms i do not
expect this to b
supported by SIESTA and try
them !!!
Best wishes,
Imad
"Pablo A. Denis" <[EMAIL PROTECTED]> a écrit :
Dear Oleksandr,
Thank you very much for your answer. I have been playing a little with the
basis sets. The problem was basis set. BSSE optimization i
Dear Oleksandr,
Thank you very much for your answer. I have been playing a little with the
basis sets. The problem was basis set. BSSE optimization is important, but
only for the default DZP. The interaction energies without BSSE are
atractive by 10-18 kcal/mol, very huge as usual for siesta.
Dear Oleksandr,
Thanks for your answer. I did CG relaxation, in
the mail I only included a part of the .fdf, maybe I was doing a mistake
when estimating the BSSE correction.
It is true LDA should give the atracction. Indeed, when I optimize including
BSSE I obtain
Dear siesta users,
i am performing some tests in pi stacked complexes, small systems like the
benzene dimer. The problem that I am facing is that when I use LDA/DZP
methodology I find that the interaction between the perfect sandwich benzene
dimer (BBS) (two benzenes in perfect alingment) is r
Dear Siesta users,
We are having some problems with the band
structure. The face this problem when we have metallic systems which have for
example 2 bands which crosses the fermi level ( a (n,n) SWCNT for example).
When we use gnubands to plot get the bands.dat, th
Dear Andrei Postnikov,
thank you very much for your
answer (one more time!).
what I mean when I said that that the results did not change, was that we
used a denser k-mesh along gamma to X (600 points) and it was still very
difficult to decide how the
ed, Apr 15, 2009 at 12:41 PM, Pablo A. Denis wrote:
Dear Andrei Postnikov,
thank you very much for your answer
(one more time!).
what I mean when I said that that the results did not change, was that we
used a denser k-mesh along gamma to X (600 points) and it was still very
difficult to decide how
Hi walter,
Siesta "eats" a lot of RAM, so the next time that you buy
computers buy as much RAM as you can (at least more than 2gb per core).
Your can reduce the amount of memory required using the options:
DirectPhi .true.
and
SaveMemory .true.
You save some memory at th
hi reza,
please post your .fdf so we can check it...
best regards,
pablo
- Original Message -
From: Reza Kalantari
To: SIESTA-L@listserv.uam.es
Sent: Sunday, May 31, 2009 4:53 PM
Subject: [SIESTA-L] Molecules Interaction suaitable bas
Dear Zhiyong,
you can try to reduce the broadening to 0.005, 0.120 is
(maybe) to high, and increase the number of points to 2000, but it may not
help. Also, sometimes a shift of the kpoints can help (not always).
I have the same problem very frequently, the DOS is not
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