|  Re: Spin-orbit interaction and electron structure in NCDFT ( No.1 ) | 
|  Date: 2018/01/07 07:48 Name: Daniil
 
Hi,
 Any information or advices about this case?
 
 Best regards,
 Daniil
 | 
|  Re: Spin-orbit interaction and electron structure in NCDFT ( No.2 ) | 
|  Date: 2018/01/08 13:36 Name: Chi-Cheng Lee  <cclee.physics@gmail.com>
 
Hi Daniil,
 From a user's point of view, I guess the default energy cutoff is too small to give a noticeable
 distorted charge density from the cubic one. The charge density could also not converge very well.
 This might not be due to the difference between openmx and turbomole.
 Could you try to add the following parameter?
 
 scf.energycutoff 200
 
 and also try to change 200 to 300, 400, or 500 to see if there is any difference in the spin density?
 For me, I would also add
 
 Atoms.UnitVectors.Unit Ang
 <Atoms.UnitVectors
 10 0 0
 0 10 0
 0 0 10
 Atoms.UnitVectors>
 
 to specify the unit cell size and I will also set k point to 1 1 1, such as
 
 scf.Kgrid 1 1 1
 
 to save time.
 
 Cheers,
 Chi-Cheng
 
 
 | 
|  Re: Spin-orbit interaction and electron structure in NCDFT ( No.3 ) | 
|  Date: 2018/01/08 14:43 Name: T. Ozaki
 
Hi, 
 I checked "nb.out" and "nb.sden.cube" stored in "openmx-so", and found that
 the charge distribution deviates from the cubic one. It can be seen that the Mulliken
 populations violate the cubic symmetry. In addition to this, if you carefully look at
 isosurface of the cube file, the distribution looks like tetragonal rather than cubic,
 while "nb.sden.cube" stored in "openmx-noso" remains cubic.
 Also, please be careful that there is freedom in the distribution due to degeneracy
 of the spin-orbit states, which may cause the difference between OpenMX and TURBOMOLE.
 
 Regards,
 
 TO
 | 
|  Re: Spin-orbit interaction and electron structure in NCDFT ( No.4 ) | 
|  Date: 2018/01/16 04:52 Name: Daniil
 
Thank you for answers.
 I tried to increase scf.energycutoff, but with only small, if any, effect. Yes, under close study cube files are slightly distorted from cubic symmetry, but much less than in turbomole case.
 
 As for LJ-distribution:
 Correct me, if I am wrong, but in first order, SO interaction is proportional to l*s, so that degeneracy between j=l±s states should disappear.
 Thus, electrons must redistribute, which can be seen in case of Turbomole calculations: initial non-so distribution is 1.6:2.4 = 4:6, where 4 and 6 are total numbers of j=1.5 and j=2.5 states for D-shell, while under SO interaction j=1.5 states become lower by energy and their total occupation increases to 1.74.
 
 Best regards,
 Daniil
 | 
|  Re: Spin-orbit interaction and electron structure in NCDFT ( No.5 ) | 
|  Date: 2018/03/05 23:48 Name: Daniil
 
Hi,
 Can you please comment on LJ-distribution? The D1/3-D3/2 degeneracy should vanish with SO enabled.
 
 Best regards,
 Daniil
 | 
|  Re: Spin-orbit interaction and electron structure in NCDFT ( No.6 ) | 
|  Date: 2018/03/23 00:44 Name: T. Ozaki
 
Hi, 
 In OpenMX the population of each state is determined by the Fermi-Dirac function, which is not a proper treatment
 for an isolate system like atom especially with a high temperature.
 With the spin-orbit coupling I found that the populations vary depending on the electronic temperature as follows:
 
 At 10 K
 spin up spin down
 d3z^2-r^2 0 0.370180785 0.001097401
 dx^2-y^2 0 0.826992544 0.000216028
 dxy 0 0.802166556 0.000220739
 dxz 0 0.999197203 0.000354755
 dyz 0 0.999197364 0.000354753
 sum over m 3.997734451 0.002243677
 
 At 300 K
 
 d3z^2-r^2 0 0.822098488 0.000719802
 dx^2-y^2 0 0.789486124 0.000154999
 dxy 0 0.769269179 0.000157835
 dxz 0 0.808441550 0.000555007
 dyz 0 0.808446917 0.000555006
 sum over m 3.997742258 0.002142649
 
 This would be responsible for the problem.
 
 Regards,
 
 TO
 | 
|  Re: Spin-orbit interaction and electron structure in NCDFT ( No.7 ) | 
|  Date: 2018/03/24 07:15 Name: Daniil
 
Thanks for your explanation.
 I tried to perform low-temperature calculations, but scf seems to be very unstable with 10K. How did you achieve convergence? I tried to increase scf.Mixing.History and scf.Mixing.StartPulay, but with no effect.
 
 And are there any other drawbacks to using low temperature, except for scf instability?
 
 Best regards,
 Daniil
 | 
|  Re: Spin-orbit interaction and electron structure in NCDFT ( No.8 ) | 
|  Date: 2018/03/24 09:09 Name: T. Ozaki
 
Hi, 
 The following is a set of parameters I used:
 
 
 scf.XcType GGA-PBE # LDA|LSDA
 scf.SpinOrbit.Coupling on
 scf.SpinPolarization NC # On|Off
 scf.maxIter 300 # default=40
 scf.ElectronicTemperature 10.0 # default=300 (K)
 scf.energycutoff 1000.0 # default=150 (Ry)
 scf.EigenvalueSolver Cluster # Recursion|Cluster|Band
 scf.Kgrid 1 1 1 # means 4x4x4
 scf.Mixing.Type rmm-diish # Simple|Rmm-Diis|Gr-Pulay|Kerker|Rmm-Diisk
 scf.Init.Mixing.Weight 0.01 # default=0.30
 scf.Min.Mixing.Weight 0.001 # default=0.001
 scf.Max.Mixing.Weight 0.200 # default=0.40
 scf.Mixing.History 20 # default=5
 scf.Mixing.StartPulay 15 # default=6
 scf.criterion 1.0e-8 # default=1.0e-6 (Hartree)
 
 
 Regards,
 
 TO
 | 
|  Re: Spin-orbit interaction and electron structure in NCDFT ( No.9 ) | 
|  Date: 2018/03/24 21:30 Name: Daniil
 
Thanks! With your parameters, calculation did converge, with occupations similar to yours:d3z^2-r^2 0 0.365803842 0.001118400 0.366922242 0.364685441 0.0004 -37.0934
 dx^2-y^2 0 0.829987864 0.000217503 0.830205368 0.829770361 0.0004 -35.8720
 dxy 0 0.803548928 0.000222626 0.803771554 0.803326302 0.0004 -35.8685
 dxz 0 0.999177628 0.000357497 0.999535125 0.998820132 0.0005 -34.0179
 dyz 0 0.999177633 0.000357496 0.999535129 0.998820136 0.0005 -37.1983
 sum over m 3.997695895 0.002273522 3.999969417 3.995422373
 But, unfortunately, it still yielded 1.6/2.4 ratio for d-electrons.
 
 Best regards,
 Daniil
 | 
|  Re: Spin-orbit interaction and electron structure in NCDFT ( No.10 ) | 
|  Date: 2018/04/19 04:02 Name: Daniil
 
Hi,
 Is it possible to perform 0K calculations in OpenMX? I tried to increase scf parameters, but convergence was not achieved yet. So, does it make sense to continue, or there are some fundamental restrictions in scf algorithms?
 
 Best regards,
 Daniil
 |