LORBIT: Difference between revisions
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</math> | </math> | ||
In case of non-collinear calculations ({{TAGBL|LNONCOLLINEAR}}=.TRUE.) the lines after "total charge" correspond to the diagonal average of the density tensor | In case of non-collinear calculations ({{TAGBL|LNONCOLLINEAR}}=.TRUE.) the lines after "total charge" correspond to the diagonal average | ||
<math> \frac{\rho_{\alpha l}^{\uparrow\uparrow} - \rho_{\alpha l}^{\downarrow \downarrow}}{2} </math> | |||
of the density tensor | |||
<math> | <math> | ||
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of the spinor <math>|\Psi_{n{\bf k}}\rangle=\left(\begin{matrix}\chi_{n{\bf k}}^\uparrow \\\chi_{n{\bf k}}^\downarrow \end{matrix}\right)</math> | of the spinor <math>|\Psi_{n{\bf k}}\rangle=\left(\begin{matrix}\chi_{n{\bf k}}^\uparrow \\\chi_{n{\bf k}}^\downarrow \end{matrix}\right)</math> | ||
Similarly, the lines after "magnetization (x)" correspond to the partial magnetization density projected onto the x direction and two additional entries "magnetization (y)", "magnetization (z)" are written for the y and z direction and are calculated from the three Pauli matrices | |||
<math> | |||
\sigma^x = \left(\begin{matrix} | |||
0 & 1 \\ | |||
1 & 0 \\ | |||
\end{matrix}\right), \quad | |||
\sigma^y = \left(\begin{matrix} | |||
0 & -i \\ | |||
i & 0 \\ | |||
\end{matrix}\right), \quad | |||
\sigma^z = \left(\begin{matrix} | |||
1 & 0 \\ | |||
0 & -1 \\ | |||
\end{matrix}\right) | |||
</math> | |||
via | |||
<math> | |||
m_{\alpha l}^j = \frac{1}{2}\sum_{\mu,\nu=1}^2 \sigma^j_{\mu \nu} \rho_{\alpha l}^{\mu \nu}. | |||
</math> | |||
== Related Tags and Sections == | == Related Tags and Sections == |
Revision as of 17:01, 8 January 2019
LORBIT = 0 | 1 | 2 | 5 | 10 | 11 | 12
Default: LORBIT = None
Description: LORBIT, together with an appropriate RWIGS, determines whether the PROCAR or PROOUT files are written.
LORBIT RWIGS tag files written 0 required DOSCAR and PROCAR 1 required DOSCAR and lm-decomposed PROCAR 2 required DOSCAR and lm-decomposed PROCAR + phase factors 5 required DOSCAR and PROOUT 10 ignored DOSCAR and PROCAR 11 ignored DOSCAR and lm-decomposed PROCAR 12 ignored DOSCAR and lm-decomposed PROCAR + phase factors
Remark:
For LORBIT = 11 and ISYM = 2 the partial charge densities are not correctly symmetrized and can result in different charges for symmetrically equivalent partial charge densities. This issue if fixed as of version >=6. For older versions of vasp a two-step procedure is recommended:
- 1. Self-consistent calculation with symmetry switched on (ISYM=2)
- 2. Recalculation of the partial charge density with symmetry switched off (ISYM=0)
To avoid unnecessary large WAVECAR files it recommended to set LWAVE=.FALSE. in step 2
If LORBIT is set the partial charge densities can be found in the OUTCAR
total charge # of ion s p d tot ------------------------------------------ 1 1.514 0.000 0.000 1.514 2 0.123 0.345 0.000 0.468
Here the first column corresponds to the ion index , the s, p, d,... columns correspond to the partial charges for defined as
The are obtained from the projection of the (occupied) wavefunctions onto spherical harmonics that are non zero within spheres of a radius RWIGS centered at ion and the last column is the sum .
Note that depending on the system an "f" column can be found as well.
In case of collinear calculations (ISPIN=2) the magnetization densities are written to the OUTCAR
magnetization (x) # of ion s p d tot ------------------------------------------ 1 0.000 0.000 0.000 0.000 2 0.000 0.245 0.000 0.245
Here the magnetization density (projection axis is the z-axis) is calculated from the difference in the up and down spin channel
In case of non-collinear calculations (LNONCOLLINEAR=.TRUE.) the lines after "total charge" correspond to the diagonal average of the density tensor
which is determined from the projected components
of the spinor
Similarly, the lines after "magnetization (x)" correspond to the partial magnetization density projected onto the x direction and two additional entries "magnetization (y)", "magnetization (z)" are written for the y and z direction and are calculated from the three Pauli matrices
via