About which files do you have to worry:
INCAR POSCAR POTCAR KPOINTSBefore using one of the supplied PAW potentials intensively, it is not only necessary to test the potential for various bulk phases, but the potential also needs to reproduce the eigenvalues and the total energy of the free atom for which it was created. If the energy cutoff and the cell size are sufficiently large, the agreement between the atomic reference calculation (EATOM in the POTCAR file) and a calculation using VASP is usually better than 1 meV (although errors can be 10 meV for some transition metals). In most cases, calculations for a spherical atom are relatively fast and unproblematic. For the calculation the
Monkhorst Pack 0 Monkhorst Pack 1 1 1 0 0 0
A simple cubic cell is usually recommended; the size of the cell depends on the element in question. Some values for reliable results are compiled in Tab. 4. These cells are also large enough to perform calculations on dimers, explained in the next section. The POSCAR file is similar to:
atom
1
10.00000 .00000 .00000
.00000 10.00000 .00000
.00000 .00000 10.00000
1
cart
0 0 0
The INCAR file can be very simple
SYSTEM = Pd: atom ENCUT = 200.00 eV # energy cut-off for the calculation PREC = Normal # Normal precision LREAL = .FALSE ! real space projection .FALSE. or Auto ISMEAR = 0; SIGMA=0.1 use smearing methodThe only difference to the bulk calculation is that Gaussian smearing should be used. Mind: Extract the correct value for the energy. For atoms and molecules, the value
In some rare cases, the real LDA/GGA groundstate might differ
from the configuration for which the potential was
generated (most transition metals, see Sec. 10), since
the occupancies have been set manually during the pseudopotential generation.
For Pd, for instance, a
configuration was
chosen to be the reference configuration, which is not the
LDA/GGA groundstate of the atom. In this case, it is necessary
to set the occupancies in VASP manually in order to obtain the same
energy as the one found in the POTCAR file.
This can be done including the following lines in the
INCAR file:
LDIAG = .FALSE. ! keep ordering of eigenstates fixed ISMEAR = -2 ! keep occupancies fixed FERWE = 5*0.9 0.5 ! set the occupancies manually(5*0.9 is interpreted as 0.9 0.9 0.9 0.9 0.9). To determine the an initial WAVECAR file, it might be necessary to perform initial calculations using ICHARG=12 (i.e. fixed atomic charge density) and to continue with the setting above. After a successful atomic calculation compare the differences between the eigenvalues with those obtained by the pseudopotential generation program. The total energy written by VASP should be essentially zero (since the atomic reference energy EATOM is subtracted).
Another illustrative example: If the energy of an atom with a particular configuration needs to be calculated, i.e. spin polarized Fe with a valence configuration of 3d6.2 4s1.8, the calculation has to be done in two step. First a non selfconsistent calculation with the following INCAR must be performed:
ISPIN = 2 ICHARG = 12 MAGMOM = 4 ! magnetization in Fe is 4This first step is required to determine a set of orbitals. From the OUTCAR file the level ordering can be determined:
k-point 1 : 0.0000 0.0000 0.0000
band No. band energies
1 -5.0963
2 -5.0963
3 -5.0954
4 -5.0954
5 -5.0954
6 -4.6929
7 -0.7528
8 -0.7528
Spin component 2
k-point 1 : 0.0000 0.0000 0.0000
band No. band energies
1 -3.6296
2 -2.2968
3 -2.2968
4 -2.2889
5 -2.2889
6 -2.2889
7 -0.1247
8 -0.1247
In the spin up component, the
ISTART = 1 ! read in the WAVECAR file
ISPIN = 2
MAGMOM = 4
AMIX = 0.2 ; BMIX = 0.0001 ! recommended mixing for magnetic systems
LDIAG = .FALSE. ! keep ordering of eigenstates fixed
! (Loewdin subspace rotation)
ISMEAR = -2 ! keep occupancies fixed
FERWE = 5*1 1*1 3*0 ! d5 s1, 3 other orbitals zero occ.
FERDO = 0.8 5*0.24 3*0 ! s0.8 d1.2 other orbitals zero occ.
The determination of the spin-polarized broken symmetry
groundstate of atoms is discussed in the next section 9.5.