I don't know Bandup, but if it is well structured it should be quite easy
to adapt it to the new format of data files.
Otherwise, you may try "unfold" by Pietro Bonfà:
https://bitbucket.org/bonfus/unfold-x/src/master/
Paolo
On Thu, Oct 8, 2020 at 4:15 AM William Hewett <
Hi users,
The gather_grid function is a 1D array with dimensions nr1x * nr2x * nr3x.
Does it follow the convention written in the developer's manual -- written
as a 3D array with dimensions nr1x, nr2x, nr3x, is the innermost loop x,
then y, and the outermost loop z?
Best regards,
Andrew
Dear Dr. Giannozzi,
For QE input to be portable, not only wfcdir but also max_seconds
should be read from environment variables. Time limit differs with
batch queues.
Best regards,
---Sender---
Takahiro Chiba
Undergraduate at Hokkaido University
takahiro_ch...@eis.hokudai.ac.jp
-
Hi QE Users,
I'm wanting to unfold a band structure calculation on a supercell, I've
tried Bandup (https://github.com/band-unfolding/bandup) however it seems
the current version of Bandup is not compatible with versions of QE post
6.3. My calculation requires QE 6.6.
Does anyone know if it is
l is used in pslibrary to distinguish the PP with larger core radii.
It means lower accuracy.
Andrea
On Wed, 2020-10-07 at 13:45 +, 박민규 wrote:
> Dear all,
>
> I have a small question.
>
> For example Ga in PSlibrary table, there are two pseudopotentials
> that share almost identical
Dear Mr. Marchand, Dr. Giannozzi, and all QE users,
No "pwscf.wfcN" was found in "wfcdir" because he did calculation='scf'
and disk_io='low', I suspect. When I do "relax" calculation with
disk_io='low' option, QE 6.5 with intel MPI 18 on CentOS 6 does write
"pwscf.wfcN" in "wfcdir", where N is
Dear all,
I have a small question.
For example Ga in PSlibrary table, there are two pseudopotentials that share
almost identical name:
Ga.rel-pbe-dn-kjpaw_psl.1.0.0.UPF
Ga.rel-pbe-dnl-kjpaw_psl.1.0.0.UPF
I understand the meaning of “d" and “n” based on the explanation of QE website.
I think wfcdir is still used when wavefunctions are saved to disk during
the scf calculation (option disk_io='high', that shouldn't be normally
used) but not for writing the final data.
Is there a good reason to use wfcdir? My opinion is that it should be
deleted, together with outdir and
If your cluster has a disk per node with a local (i.e., directly accessible
by the node but not visible from other nodes) you may try to write data to
that disk. It's a pain in the *** and may require some tweaking, but it
might work. You need to ensure that the directories are there (they are
Hello Thomas,
1/2
They haven't specified any parameters to my knowledge that would lead to such a
large error. There may be slight difference in the thresholds of energetic
convergence, but they should yield errors on a much smaller scale.
2/2
RE: box sizes - We did briefly fall foul of
Dear Lorenzo and Michel,
thank you for your reply. Yes, unfortunately I am using a small cluster
and, for memory issues, I cannot use the SSD-based local scratch. Thus I
am forced to use a
non-parallel NFS. From your answers, I understand that, given
the situation, the huge difference between
Dear Gabriel,
1/2, are your sims. reproducing *all* of the ref. params? (eg. are
cell parameters the same?)
any missing params. would contribute by adding an *unknown*
magnitude of error...
2/2, my guess would be that your evaluation of dE_a is wrong due to
*different cell sizes*
Dear Users,
Problem:
I am performing calculations with the optB88-vdW functional to obtain
adsorption energies of small aromatic molecules on metallic surface facets
(Pt(111) and phenol for the cases discussed here). Unfortunately, the
adsorption energies obtained from these calculations are
Dear Prof. Pietro and users,
Yes, you have correctly pointed out and I have understood now. I want to
check the variation with higher kmesh (8,9,10) and have found that the
program is killed for 8*8*8 kmesh itself. The required static and dynamical
RAM are 8.59 and 13.64 GB respectively (as
Thank you Matteo and Lorenzo!
h_psi.f90 looks promising, and I will take a look at pw2wannier.f90 for
seeing how to apply H to an orbital.
Do you or others have any pointers on the inner product, either in
reciprocal space or real space?
___
Quantum
You can find an example of how H|psi> is done (and the subroutines you
have to call before to be sure that everything is in place) in
PP/src/pw2wannier90.f90
I would recommend you compute just to begin with, and
verify that it is \epsilon_i \delta_ij
On 07/10/2020 09:15, Matteo Cococcioni
Dear Andrew,
I would first compute | \psi'_l > = U_lm | \psi_m> using some linear
algebra routine (as done in the code in many places by summing over plane
waves), then compute
H |\psi'_l > (e.g., using h_psi.f90), finally the product with < \psi'_n |.
HTH
Matteo
Il giorno mer 7 ott 2020 alle
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