[QE-users] NEB calculation
mehrdad zamzamian
mehrdad.zamzamian at gmail.com
Tue Sep 17 12:46:40 CEST 2019
yes, i do i did scf calculation. i obtained the relaxation position of the
atoms in 2 conditions (first case before migration and the last case after
the vacancy reached to its position). i also obtained the formation energy
of the vacancy.
Best regards
S.M.Zamzamian
e-mail: mehrdad.zamzamian at gmail.com
Iran, Tehran
Sharif University of Technology
On Tue, Sep 17, 2019 at 3:04 PM Nicola Marzari <nicola.marzari at epfl.ch>
wrote:
>
>
> Try first to do a scf calculation of a vacancy. Are you able to do that?
> A relaxation? A vacancy formation energy?
>
> nicola
>
>
>
>
> On 17/09/2019 09:12, mehrdad zamzamian wrote:
> > Hi all dear QE users
> > I want to calculate the vacancy migration in alpha-Fe. I defined 2by2by2
> > supercell and used NEB but i could not achieve any convergence or a
> > proper result. searching in archives did not help. at the end of this
> > message is my input and a part of the output. I tested various changes
> > like k-point, ds, num_of_images, PP ... but nothing happened. my first
> > image gave the result of ~300eV!!!! then i gave some error (although the
> > calculation was being run) the second image was ~180 then the third
> > image i gave ~300. i also saw the atoms in xcrysden, they collapsed
> > during the calculation!!!Is there any idea about this problem? i
> appreciate.
> > ------------------------------------------------------
> > BEGIN
> > BEGIN_PATH_INPUT
> > &PATH
> > restart_mode = 'from_scratch'
> > string_method = 'neb',
> > nstep_path = 50,
> > ds = 1.D0,
> > opt_scheme = "broyden",
> > num_of_images = 12,
> > CI_scheme = "no-CI",
> > path_thr = 0.1,
> > /
> > END_PATH_INPUT
> > BEGIN_ENGINE_INPUT
> > &CONTROL
> > prefix = ""
> > pseudo_dir = "",
> > /
> > &SYSTEM
> > a = 5.69623e+00
> > degauss = 1.00000e-02
> > ecutrho = 2.25000e+02
> > ecutwfc = 2.50000e+01
> > ibrav = 1
> > nat = 15
> > nspin = 2
> > ntyp = 1
> > occupations = "smearing"
> > smearing = "gaussian"
> > starting_magnetization(1) = 2.00000e-01
> > /
> > &ELECTRONS
> > mixing_beta = 0.01
> > conv_thr = 1.0d-8
> > electron_maxstep=200
> > /
> > &IONS
> > /
> > ATOMIC_SPECIES
> > Fe 55.84500 Fe.pbe-nd-rrkjus.UPF
> > BEGIN_POSITIONS
> > FIRST_IMAGE
> > ATOMIC_POSITIONS (angstrom)
> > Fe 0.000000 0.000000 0.000000
> > Fe 1.424058 1.424058 1.424058
> > Fe 0.000000 0.000000 2.848116
> > Fe 1.424058 1.424058 4.272174
> > Fe 0.000000 2.848116 0.000000
> > Fe 1.424058 4.272174 1.424058
> > Fe 0.000000 2.848116 2.848116
> > Fe 1.424058 4.272174 4.272174
> > Fe 2.848116 0.000000 0.000000
> > Fe 4.272174 1.424058 1.424058
> > Fe 2.848116 0.000000 2.848116
> > Fe 4.272174 1.424058 4.272174
> > Fe 2.848116 2.848116 0.000000
> > Fe 4.272174 4.272174 1.424058
> > Fe 2.848116 2.848116 2.848116
> > LAST_IMAGE
> > ATOMIC_POSITIONS (angstrom)
> > Fe 0.000000 0.000000 0.000000
> > Fe 1.424058 1.424058 1.424058
> > Fe 0.000000 0.000000 2.848116
> > Fe 1.424058 1.424058 4.272174
> > Fe 0.000000 2.848116 0.000000
> > Fe 1.424058 4.272174 1.424058
> > Fe 0.000000 2.848116 2.848116
> > Fe 1.424058 4.272174 4.272174
> > Fe 2.848116 0.000000 0.000000
> > Fe 4.272174 1.424058 1.424058
> > Fe 2.848116 0.000000 2.848116
> > Fe 4.272174 1.424058 4.272174
> > Fe 2.848116 2.848116 0.000000
> > Fe 4.272174 4.272174 1.424058
> > Fe 4.272174 4.272174 4.272174
> > END_POSITIONS
> > K_POINTS (automatic)
> > 5 5 5 0 0 0
> > END_ENGINE_INPUT
> > END
> > ---------------------------------------
> > Best regards
> > S.M.Zamzamian
> > e-mail: mehrdad.zamzamian at gmail.com <mailto:mehrdad.zamzamian at gmail.com>
> > Iran, Tehran
> > Sharif University of Technology
> >
> > _______________________________________________
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> >
>
>
> --
> ----------------------------------------------------------------------
> Prof Nicola Marzari, Chair of Theory and Simulation of Materials, EPFL
> Director, National Centre for Competence in Research NCCR MARVEL, EPFL
> http://theossrv1.epfl.ch/Main/Contact http://nccr-marvel.ch/en/project
>
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