Bandstructure of SrVO3 in GW: Difference between revisions

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=== Bandstructure using WANNIER90 ===
=== Bandstructure using WANNIER90 ===
Again, add the following line to your {{FILE|INCAR}} to have VASP call [http://www.wannier.org WANNIER90]:
<pre>
LWANNIER90_RUN = .TRUE.
</pre>
and use the following [http://www.wannier.org WANNIER90] input:


*wannier.win.gw
*wannier.win.gw
Line 175: Line 181:
end projections
end projections
</pre>
</pre>
Copy the above to {{FILE|wannier90.win}}:
cp wannier90.win.dft wannier90.win
and redo the GW calculation.


== Download ==
== Download ==

Revision as of 14:21, 12 September 2012

Description: the GW bandstructure of SrVO3 using VASP and WANNIER90.


Performing a GW calculation with VASP is a 3-step procedure: a DFT groundstate calculation, a calculation to obtain a number of virtual orbitals, and the actual GW calculation itself. In this example we will also see how the results of the GW calculation may be postprocessed with WANNIER90 to obtain the dispersion of the bands along the usual high symmetry directions in reciprocal space.

The DFT groundstate calculation

Everthing starts with a conventional DFT (in this LDA) groundstate calculation:

  • INCAR.DFT
System  = SrVO3

ISMEAR = -5
EMIN = -20 ; EMAX = 20 ; NEDOS = 1000  # usefull energy range for density of states

EDIFF = 1E-8                           # high precision for groundstate calculation

KPAR = 3

Copy the aforementioned file to INCAR:

cp INCAR.DFT INCAR
  • KPOINTS
Automatically generated mesh
       0
Gamma
 4 4 4

Mind: this is definitely not dense enough for a high-quality description of SrVO3, but in the interest of speed we will live with it.

  • POSCAR
SrVO3
3.77706  #taken from 9x9x9 with sigma=0.2 ismear=2
 +1.0000000000  +0.0000000000  +0.0000000000 
 +0.0000000000  +1.0000000000  +0.0000000000 
 +0.0000000000  +0.0000000000  +1.0000000000 
Sr V O
 1 1 3
Direct
 +0.0000000000  +0.0000000000  +0.0000000000 
 +0.5000000000  +0.5000000000  +0.5000000000 
 +0.5000000000  +0.5000000000  +0.0000000000 
 +0.5000000000  +0.0000000000  +0.5000000000 
 +0.0000000000  +0.5000000000  +0.5000000000

Analysis of the DOS

Add the following line to your INCAR file:

LORBIT = 11

Bandstructure using WANNIER90

Add the following line to your INCAR to have VASP call WANNIER90:

LWANNIER90_RUN = .TRUE.

WANNIER90 takes its input from the file wannier90.win. To construct Wannier functions for the Vanadium t2g manifold in SrVO3, and plot the dispersion of the associated bands along R-G-X-M, one may use the following settings:

  • wannier90.win.dft
bands_plot = true

begin kpoint_path
R  0.50000000  0.50000000  0.50000000  G  0.00000000  0.00000000  0.00000000
G  0.00000000  0.00000000  0.00000000  X  0.50000000  0.00000000  0.00000000
X  0.50000000  0.00000000  0.00000000  M  0.50000000  0.50000000  0.00000000
M  0.50000000  0.50000000  0.00000000  G  0.00000000  0.00000000  0.00000000
end kpoint_path

num_wann =    3

num_bands=    3

exclude_bands : 1-20, 24-36

begin projections
V:dxy;dxz;dyz
end projections

Copy the above to wannier90.win:

cp wannier90.win.dft wannier90.win

and restart VASP.

The Vanadium t2g band dispersion thus obtained, may conveniently be visualized with gnuplot:

gnuplot -persist plotme.dft

Obtain DFT virtual orbitals

  • INCAR.DFT.all
System  = SrVO3

ISMEAR = -5
EMIN = -20 ; EMAX = 20 ; NEDOS = 1000  # usefull energy range for density of states

ALGO = Exact  ; NELM = 1               # exact diagonalization one step suffices
EDIFF = 1E-8                           # high precision for groundstate calculation
NBANDS = 96                            # need for a lot of bands in GW
LOPTICS = .TRUE.                       # we need d phi/ d k  for GW calculations

KPAR = 3

Copy the aforementioned file to INCAR:

cp INCAR.DFT.all INCAR

and restart VASP.

The GW calculation

  • INCAR.GW0
System  = SrVO3

ISMEAR = -5
EMIN = -20 ; EMAX = 20 ; NEDOS = 1000  # usefull energy range for density of states

NBANDS = 96                            # need for a lot of bands in GW

ALGO = GW0                             # 
NELM = 1                               # one step so this is really G0W0
PRECFOCK = Fast                        # select fast mode for FFT's 
ENCUTGW = 100                          # energy cutoff for response function
NOMEGA = 200                           # metal, we need a lot of frequency points
MAXMEM = 2500                          # memory per core
NKRED = 2                              # sample down the GW to a coarse 2x2x2 grid

KPAR = 3

Copy the aforementioned file to INCAR:

cp INCAR.GW0 INCAR

Analysis of the DOS

Bandstructure using WANNIER90

Again, add the following line to your INCAR to have VASP call WANNIER90:

LWANNIER90_RUN = .TRUE.

and use the following WANNIER90 input:

  • wannier.win.gw
bands_plot = true

begin kpoint_path
R  0.50000000  0.50000000  0.50000000  G  0.00000000  0.00000000  0.00000000
G  0.00000000  0.00000000  0.00000000  X  0.50000000  0.00000000  0.00000000
X  0.50000000  0.00000000  0.00000000  M  0.50000000  0.50000000  0.00000000
M  0.50000000  0.50000000  0.00000000  G  0.00000000  0.00000000  0.00000000
end kpoint_path

num_wann =    3

num_bands=    3

exclude_bands : 1-20, 24-96

begin projections
V:dxy;dxz;dyz
end projections

Copy the above to wannier90.win:

cp wannier90.win.dft wannier90.win

and redo the GW calculation.

Download


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