Dear Felix
If I am correct, PBE contains self-interaction error, that means it may give a
wrong number when you use it to calculate a single electron system such as
hydrogen. Mayben you could try B3LYP or HSE.
Best wishes
--
庞瑞(PANG Rui)
South University of Science and
00 10.0000
&PROJWFC
outdir='./'
degauss=0.01
DeltaE=0.001
lsym=.false.
/
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenzhen,Guangdong___
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understand the reason but I seldom
get convergence when using semi-core PPs in periodical cases with PWSCF.
Good luck
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenzhen,Guangdong
Dear Aditya
Just run projwfc.x on your wavefunction file of band structure, you can get the
AO components of every kpoints. See PP/example05.
Good luck
Pang Rui
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088
Dear Zhang
Maybe there is nothing wrong, you chose a MPI version, but your aministrator
may not allow you to directly run it in the front-end. Just try to submit a
parallel job and see if it end normally.
Sincerely
PangRui
--
庞瑞(PANG Rui)
South University of
interfaced with pw.x can do
this job such as CALYPSO. If the structure is not the major property you
concern, you can use a MD process and reduce the temperature step by step.
Good luck
PangRui
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of
Dear Nicola
Thanks very much for your valuable comment.
Sincerely
PangRui
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenzhen,Guangdong
-- Original
orbitals so that everyone use
wannier function? Or is there any misundertanding of me in using these
conception?
Welcome for any suggestion.
Sincerely
PangRui
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088
everyone use wannier function? Or is there any
misundertanding of me in using these conception?
Welcome for any suggestion.
Sincerely
PangRui
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenzhen
can see 16 kpoints with the
same weights, that means no symmetry is used. You may try it yourself to
confirm how to use nosym.
Sincerely
Pang Rui
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenz
Dear Tao
In my experience, setting nosym=.ture. is safer if you are interested in
magnetic issues, even in many case, as SOC and noncollinear included, the
symmetry of the system will be destroyed so that the code does not use symmetry
actually.
Sincerely
Pang Rui
.
Sincerely
Pang Rui
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenzhen,Guangdong
-- Original --
From: "Paolo Giannozzi";
Date: Sat, Aug 15, 201
Dear Mohsen
You can find it on
http://theossrv1.epfl.ch/Main/Pseudopotentials
Sincerely
PangRui
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenzhen,Guangdong
-- Original
Ah, it is intersting. I also got a similar problem but with PWCOND. And I found
the code stoped at a line of sum, quite unblievable. But my PW.X works well. I
think it is not a memory problem.
--
庞瑞(PANG Rui)
South University of Science and Technology of China
003F2241ED1D Unknown Unknown Unknown
pwcond.x 00497F29 Unknown Unknown Unknown"
So could anyone tell me how can I fix this error so that I can using more
cores to excute pwcond.x? I met this problem in both 5.1.2 and 5.2.
Thanks very much for a
more core electrons as
valence electrons, it may be important for heavier elements. More detail can be
found in the pseudopotential generating note released with QE.
Sincerely
Pang Rui
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of
Dear David
You set "starting_magnetization(3)=0.5", but you only have two elements.
Therefore , the starting_magnetization of Fe is actually zero.
Best wishes.
Pang Rui
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physic
Dear Elham
I think usually, for gaussian smearing, 0.2eV is enough for relaxation and
0.05-0.01 eV is good for DOS and magnetic properties. You can always get a good
results by setting enough narrow gaussian smearing.
Sincerely
--
庞瑞(PANG Rui)
South University of
Dear Yang
They can be found in
http://theossrv1.epfl.ch/Main/Pseudopotentials
Sincerely
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenzhen,Guangdong
-- Original
4908337 16.709063233460618
K_POINTS automatic
4 4 1 0 0 0
CELL_PARAMETERS angstrom
7.667936645865039 0.000 0.000
0.000 7.667936645865040 0.000
0.000 0.0
Dear siham
I think you can download from
http://theossrv1.epfl.ch/Main/Pseudopotentials
Best wishes
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenzhen,Guangdong
I just test, what one need is just adding an 's' after http,
https://www.mail-archive.com/pw_forum@pwscf.org/
is accessable at least for me
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenzhen
.
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenzhen,Guangdong
-- Original --
From: "Andrea Floris";
Date: Tue, Jun 9, 2015 06:36 AM
To:
0), wk = 0.0069444
k( 171) = ( 0.667 -0.833 0.000), wk = 0.0069444
k( 172) = ( -0.833 0.833 0.000), wk = 0.0138889
Thanks for your help.
Best wishes.
--
庞瑞(PANG Rui)
South University of Sci
.
Best wishes!
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenzhen,Guangdong___
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http://pwscf.org/mailman/listinfo/pw_forum
be used?
--
庞瑞(PANG Rui)
South University of Science and Technology of China/Department of Physics
No.1088,Xueyuan Road, Shenzhen,Guangdong___
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Pw_forum@pwscf.org
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atomic orbits which are
already eignvalues of angular operator? It seems impossible if they are defined
as (3.200) in the book of "Modern quantum chemistry".Is there any
misunderstanding of me?
--
庞瑞(PANG Rui)
South University of Science and Technolog
luck.
--
庞瑞(PANG Rui)
南方科技大学/物理系
深圳市南山区西丽学苑大道1088号
-- Original --
From: "Jun Yin";
Date: Thu, Jan 15, 2015 08:27 PM
To: "pw_forum";
Subject: [Pw_forum] Projected density of state onto isolated molecula
Dear all
I am trying a nscf calculation on a slab model. The scf converged well.
But when I switched to nscf calculation, c_bands convergence warning
appeared, and the calculation ended with an error like this
CG style diagonalization
c_bands: ** eigenvalues not converged
c_bands: **
In my experience, the London correction on DFT usually overestimates the
interaction so that lead to smaller distance. I suggest you use LDA or
functionals that include vdw corrections inside.
On Fri, 17 Oct 2014 18:56:05 +0800 (GMT+08:00), plgong
wrote:
> Dear pwscf user,
>Recently, I calcul
diamond. Maybe they
are not well convergened.
As you suggest, I will post further questions on Wannier list if I have.
Best wishes
Pang Rui
On Sun, 12 Oct 2014 21:54:11 +, Giovanni Pizzi
wrote:
> Dear Pang,
> just a comment on my previous message: I was thinking to the Hamiltonian
> i
integral, otherwise, according to Cauchy Inequality, the sum in larger
grids will always be smaller than the sum in smaller grids.
Sincerely
Pang Rui
On Sat, 11 Oct 2014 11:37:37 +0800 (GMT+08:00), 高淼
wrote:
> Dear all,I find in a spin polarized calculation, the quantity named
> "Magnetic
real numbers to parameter a TB model?
Best wishes!
Pang Rui
--
PostDoc
Department of Physics, South University of Science and Technology of China
Shenzhen, Guangdong, PRC, 518500
___
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You can modify the parameter.f90 in Modules and recompile then try again.
On Thu, 9 Oct 2014 17:59:43 +0800, "dingfu.shao"
wrote:
> Dear QE developer,
>
> I want to calculate the Fermi surface nesting function, which
> needs a Fermi surface calculation with a very dense grid of
>
they be constructed using the output of
projwfc.x? As far as I know, the imaginary part is missing for the
projection coefficient.
Best wishes.
Pang Rui
On Thu, 18 Sep 2014 12:14:52 +0200, Juanjo Mel?ndez
wrote:
> Dear Pang
>
> Have a look to these:
>
> Bernholc and Pantelide
SOC is part of relativistic effects, I think you can do the calculation
with QE.
On Mon, 22 Sep 2014 07:48:08 +0800, ??? wrote:
> Dear all,
> I want to calculate the electron-phonon coupling of the materials with
> spin-orbit coupling. Can QE
> ?calculate it? I saw the QE 5.0 can calculate the e
Dear Juan
I am quite interested in how you evaluate Green function by using a
projection calculation(no matter what kind of GF), is there any reference
related?
Best wishes
On Wed, 17 Sep 2014 21:19:23 +0200 (CEST), Juan Jose Melendez Martinez
wrote:
> Dear Tommaso
>
> I am not sure to u
Dear Tao:
I used to calculate FeTPP on Au with a single point calculation, and I met
converge problems,too. I am not sure if yours is the same as mine. I solved
it by increasing ECUT. The following is the input file. Hope it can be
useful for you.
&control
pseudo_dir = "~/pr/QE5/pseudo"
out
Dear all
I want use the KS orbitals expanded in AO basis to do something. In the
standard output of pwjwfc.x, there are several
psi = 0.186*[# 0]+.
But I found that the so called psi was in fact |psi|^2, because sum of the
coefficients is equal to |psi|^2. Thus the phase factor is missing.
you just se "Nia" or just invent a new name that suits you.
>
> kind regards
>
>
> On 08/03/2014 04:15 PM, Pang Rui wrote:
>> Hi,everyone.
>> In the Input describtion of PW, naming an atom as X_* is allowed.
>> However,
>> as I test, if X has
Hi,everyone.
In the Input describtion of PW, naming an atom as X_* is allowed. However,
as I test, if X has two letters, an error will occure as followed(take the
attachment as an example)
"Error in routine read_cards (1):
species Ni_a in ATOMIC_POSITIONS is nonexistent"
If I switch Ni to C, t
You just need to set ecutrho = 160. I can run your input with this
correction smoothly on my machine.
On Tue, 15 Jul 2014 11:00:39 +0530, siddheshwar chopra
wrote:
> Dear Dr. Giovanni Pizzi,
> I re ran the i/p file.. i corrected the ecutrho value. But unfortunately
> the same error persists. Pleas
bda prefactor). Does it work with
> a smaller constrained moment, say 2.5?
>
> GS
>
> On 07/04/2014 04:31 PM, Pang Rui wrote:
>> Dear Gabriele Sclauzero:
>> I covered the output, so I gave a new one with the same problems.The
>> input
>> file can be seen in
_PARAMETERS angstrom
8.00.0.
0.0 8.00.
0.0 0.0 8.0
On Fri, 4 Jul 2014 13:36:09 +0200, Gabriele Sclauzero
wrote:
> Dear Pang Rui,
>
> It's difficult to judge just from the input. Has the scf converged?
true
when they are used to generate trial wave functions. You can check this by
run the inputfile. If I have misunderstandings, Please tell me.
On Fri, 4 Jul 2014 15:44:21 +0400, Nguyen Chuong
wrote:
> Dear Pang Rui,
>
> starting_magnetization on atomic type i in a spin polarized cal
Dear Nguyen Chuong
It puzzled me for quite a long time. But I have checked the relation of
the output constraint energy and the output magnetic moment, and
experienced several calculations with QE5.0.2. It seemed that that when the
starting magnetizations are interpreted as the target values of
mag
Dear all
Could anyone gave me some suggestion to do the constraint magnetic moment
calculation?
I followed the constraint magnetic moment calculation of the following
handson with PWSCF.
http://www.vasp.at/vasp-workshop/slides/handsonIV.pdf
VASP uses the same method of PWSCF on constraint MM. Howev
Dear all
I want to calculate the magnetic coupling constants to get the Curie
temperature. So I tried to get some spin configuration. I start the
calculation as is showed in the end of this mail with lamda=2. The target
atom(Ni2) did not show the antiferromagnetic moment as I want but a 0.2
miuB
Maybe you can check if different starting magnetizations converge into
one.
On Tue, 17 Jun 2014 02:02:41 +, "Kurth, Michael R."
wrote:
> Dear Juanjo,
>
> Thank you for the advice. We did try a DFT+U calculation only on the
> neodymium atoms, but it was also with the default number of bands.
in these three magnetic moments? Which one
should be used?
Best wishes
Pang Rui
--
Department of Physics, South University of Science and Technology of China
Dear Pourya
You should use full relativistic pesudopotential(files with .rel) for Mo.
And I suggest you set a starting magnetization. In my experience the band
gap usually gets reduced when SOI added.
Best Wishes
Pang Rui
On Fri, 06 Jun 2014 20:17:55 +0900, pourya
wrote:
> Dear all
> H
Dear Filippo,
The GPU is NVIDIA Tesla C2050, I thinke the cluster is generally all
right. It belongs to a supercomputing center and I saw someone run GPU code
on it.
Regards Pangrui
On Thu, 22 May 2014 10:14:20 +0100, Filippo Spiga
wrote:
> Dear ??,
>
> I am aware about a problem in one of the ro
Dear Marcos
I have performed a 77-atom B3LYP calculation using VASP on 36 cores. It
crushed and showed segmentation fault. Then I tried on a machine with
larger memory, it worked, but spent 3 days finishing a loop, so I quit.
In my opinion, the hybrid function calculation is quite time consuming an
Dear all:
I want to calculate the magnetic coupling constant J so that I can get the
Cruie temperature. How can I achieve this by using QE?
In some of the articles, the exchange parameter J was calculated by the
energy difference of antiferromagnetism(AFM) state and ferromagnetism(FM)
state. Howev
Dear Tommaso:
I think maybe there are some misuderstanding. The following is what I do.
1:calculate a scf and save all the output(the key is the *.save folder in
fact)
2:Bulid several folders, for example, 10.
3:Copy the scf file into the 10 folders
4:Put the perturbative input files which have di
http://hjklol.mit.edu/content/calculating-hubbard-u
I have some problems to excute the fortran code in the material of
Mr.Cococcioni, and reading the code takes a lot of effort. Until now I do
not quite understand how he obtained a supercell result without calculating
the supercell.
The above tutor
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