CRPA of SrVO3
The following tutorial describes how to perform CRPA calculations, which is available as of VASP 6.
Task
Calculation of the Coulomb matrix elements in the constrained Random Phase Approximation (CRPA) of SrVO3 between the Vanadium t2g states.
Performing a CRPA calculation with VASP is a 3-step procedure: a DFT groundstate calculation, a calculation to obtain a number of virtual orbitals, and the actual CRPA calculation itself.
N.B.: This example involves quite a number of individual calculations. The easiest way to run this example is to execute:
./doall.sh
In any case, one can consider the doall.sh script to be an overview of the steps described below.
DFT groundstate calculation
The first step is a conventional DFT (in this case PBE) groundstate calculation.
- INCAR (see INCAR.DFT)
SYSTEM = SrVO3 # system name NBANDS = 36 # small number of bands ISMEAR = 0 # Gaussian smearing EDIFF = 1E-8 # high precision for groundstate calculation KPAR = 2 # parallelization of k-points in two groups
Copy the aforementioned file to INCAR:
cp INCAR.DFT INCAR
The POSCAR file describes the structure of the system:
SrVO3 3.84652 #cubic fit for 6x6x6 k-points +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
This file remains unchanged in the following.
The KPOINTS file describes how the first Brillouin zone is sampled. In the first step we use a uniform k-point sampling:
Automatically generated mesh 0 Gamma 4 4 4 0 0 0
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.
Run VASP. If all went well, one should obtain a WAVECAR file containing the PBE wavefunction.
Obtain DFT virtual orbitals and long-wave limit
Use following INCAR file to increase the number of virtual states and to determine the long-wave limit of the polarizability (stored in WAVEDER):
- INCAR (see INCAR.PBE)
SYSTEM = SrVO3 # system name ISMEAR = 0 # Gaussian smearing KPAR = 2 # parallelization of k-points in two groups ALGO = Exact # exact diagonalization NELM = 1 # one electronic step suffices, since WAVECAR from previous step is present NBANDS = 96 # need for a lot of bands in GW LOPTICS = .TRUE. # we need d phi/ d k for GW calculations for long-wave limit
Restart VASP. At this stage it is a good idea to make a safety copy of the WAVECAR and WAVEDER files since we will repeatedly need them in the calculations that follow:
cp WAVECAR WAVECAR.PBE cp WAVEDER WAVEDER.PBE
CRPA Calculation
Calculate the CRPA interaction parameters for the t2g states by using the PBE wavefunction as input
cp WAVECAR.PBE WAVECAR cp WAVEDER.PBE WAVEDER
And use following input file as
- INCAR (see INCAR.CRPA) and run vasp
SYSTEM = SrVO3 # system name ISMEAR = 0 # Gaussian smearing NCSHMEM = 1 # switch off shared memory for chi ALGO = CRPA # Switch on CRPA NBANDS = 96 # CRPA needs many empty states PRECFOCK = Fast # fast mode for FFTs NTARGET_STATES = 1 2 3 # exclude wannier states 1 - 3 in screening LWRITE_WANPROJ = .TRUE. # write wannier projection file
| Warning: As of version 6.2.0 run this tutorial successfully by adding following lines to INCAR. For older version copy wannier90.win.CRPA to wannier90.win and omit these lines in INCAR. |
NUM_WANN = 3 WANNIER90_WIN = " num_bands= 96 # because bands 21, 22, 23 do not cross with other bands # one can exclude all other bands in wannierization like so # and omit the definition of an energy window like so exclude_bands = 1-20, 24-96
begin projections V:dxy;dxz;dyz end projections "
The CRPA interaction values for can be found in the OUTCAR:
spin components: 1 1, frequency: 0.0000 0.0000
screened Coulomb repulsion U_iijj between MLWFs:
1 2 3
1 3.3746 2.3385 2.3385
2 2.3385 3.3746 2.3385
3 2.3385 2.3385 3.3746
screened Coulomb repulsion U_ijji between MLWFs:
1 2 3
1 3.3746 0.4429 0.4429
2 0.4429 3.3746 0.4429
3 0.4429 0.4429 3.3746
screened Coulomb repulsion U_ijij between MLWFs:
1 2 3
1 3.3746 0.4429 0.4429
2 0.4429 3.3746 0.4429
3 0.4429 0.4429 3.3746
averaged interaction parameter
screened Hubbard U = 3.3746 -0.0000
screened Hubbard u = 2.3385 0.0000
screened Hubbard J = 0.4429 -0.0000
- N.B.: The frequency point can be set by OMEGAMAX in the INCAR. For instance to evaluate the CRPA interaction matrix at eV, add
OMEGAMAX = 10
to the INCAR and restart VASP. In contrast, adding following two lines to the INCAR
OMEGAMAX = 10 NOMEGAR = 0
tells VASP to calculate the interaction on the imaginary frequency axis at . This can be used to evaluate at a specific Matsubara frequency point.
In addition, the bare Coulomb interaction matrix is calculated for a high VCUTOFF and low energy cutoff ENCUTGW and written in that order to the OUTCAR file. Look for the lines similar to:
spin components: 1 1
bare Coulomb repulsion V_iijj between MLWFs:
1 2 3
1 16.3485 15.0984 15.0984
2 15.0984 16.3485 15.0984
3 15.0984 15.0984 16.3485
bare Coulomb repulsion V_ijji between MLWFs:
1 2 3
1 16.3485 0.5351 0.5351
2 0.5351 16.3485 0.5351
3 0.5351 0.5351 16.3485
bare Coulomb repulsion V_ijij between MLWFs:
1 2 3
1 16.3485 0.5351 0.5351
2 0.5351 16.3485 0.5351
3 0.5351 0.5351 16.3485
averaged bare interaction
bare Hubbard U = 16.3485 -0.0000
bare Hubbard u = 15.0984 -0.0000
bare Hubbard J = 0.5351 0.0000
CRPA calculation with spacetime Algorithm
Note that the same frequency grid is used as for ALGO=RPA (RPA correlation energy calculation) and can not be changed directly. To calculate the CRPA interaction for a set of automatically chosen imaginary frequency points use once again the PBE wavefunction as input
cp WAVECAR.PBE WAVECAR cp WAVEDER.PBE WAVEDER
Currently, this step requires the WANPROJ file from previous step, no wannier90.win file is necessary. You can also, delete WANPROJ and define a wannier projection as in the previous step in the INCAR.
Select the space-time CRPA algorithm with following file:
- INCAR (see INCAR.CRPAR)
SYSTEM = SrVO3 # system name ISMEAR = 0 # Gaussian smearing NCSHMEM = 1 # switch off shared memory for chi ALGO = CRPAR # Switch on CRPA on imaginary axis NBANDS = 96 # CRPA needs many empty states PRECFOCK = Fast # fast mode for FFTs NTARGET_STATES = 1 2 3 # exclude wannier states 1 - 3 in screening NCRPA_BANDS = 21 22 23 # remove bands 21-23 in screening, currently required for space-time algo NOMEGA = 12 # use 12 imaginary frequency points NTAUPAR = 4 # distribute 12 time points into 4 groups
Run VASP and make a copy of the output file
cp OUTCAR OUTCAR.CRPAR
After a successful run, the interaction values are written to the OUTCAR file. Here is the result for the first frequency point:
spin components: 1 1, frequency: 0.0000 0.2248
screened Coulomb repulsion U_iijj between MLWFs:
1 2 3
1 3.3798 2.3436 2.3436
2 2.3436 3.3798 2.3436
3 2.3436 2.3436 3.3798
screened Coulomb repulsion U_ijji between MLWFs:
1 2 3
1 3.3798 0.4433 0.4433
2 0.4433 3.3798 0.4433
3 0.4433 0.4433 3.3798
screened Coulomb repulsion U_ijij between MLWFs:
1 2 3
1 3.3798 0.4433 0.4433
2 0.4433 3.3798 0.4433
3 0.4433 0.4433 3.3798
averaged interaction parameter
screened Hubbard U = 3.3798 -0.0000
screened Hubbard u = 2.3436 0.0000
screened Hubbard J = 0.4433 -0.0000
- N.B.: The number of frequency points should be large enough to guarantee for an accurate Fourier transformation of the CRPA polarizability matrix from the imaginary time to imaginary frequency domain. See ACFDT/RPA calculations for more information.
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