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Gauss-Hermit Integration

The matrix element of the non-local pseudopotential

$\displaystyle V^{\rm nl}({\bf G},{\bf G^\prime})$ $\displaystyle =$ $\displaystyle \sum_{L} {1 \over \Omega} \int d{\bf r}
e^{-i {\bf G} \cdot {\bf r}} \Delta V^{L}({\bf r}) e^{i {\bf G^\prime} \cdot {\bf r}}$ (178)
  $\displaystyle =$ $\displaystyle \sum_{L} \int_0^{\infty} dr \langle {\bf G} \mid Y_{\rm L} \rangl...
...elta V^{L}(r)
\langle Y_{\rm L} \mid {\bf G^\prime} \rangle_{\omega} \enspace ,$ (179)

where $ \langle \cdot \mid \cdot \rangle_{\omega} $ stands for an integration over the unit sphere. These integrals still depend on $ r$ . The integration over the radial coordinate is replaced by a numerical approximation

$\displaystyle \int_0^{\infty} r^2 f(r) dr \approx \sum_i w_i f(r_i) \enspace .$ (180)

The integration weights $ w_i$ and integration points $ r_i$ are calculated using the Gauss-Hermit scheme. The non-local pseudopotential is in this approximation
$\displaystyle V^{\rm nl}({\bf G},{\bf G^\prime})$ $\displaystyle =$ $\displaystyle \sum_{L} {1 \over \Omega} \sum_i w_i \Delta V^{L}(r_i)
\langle {\...
...gle_{\omega}^{r_i}
\langle Y_{\rm L} \mid {\bf G^\prime} \rangle_{\omega}^{r_i}$ (181)
  $\displaystyle =$ $\displaystyle \sum_{L} {1 \over \Omega} \sum_i w_i \Delta V^{L}(r_i) P_i^{L\star}({\bf G}) P_i^{L}({\bf G^\prime}) \enspace ,$ (182)

where the definition for the projectors $ P$

$\displaystyle P_i^{L}({\bf G}) = \langle Y_{\rm L} \mid {\bf G} \rangle_{\omega}^{r_i}$ (183)

has been introduced. The number of projectors per atom is the number of integration points (5 - 20 for low to high accuracy) multiplied by the number of angular momenta. For the case of s and p non-local components and 15 integration points this accounts to 60 projectors per atom.

The integration of the projectors can be done analytically

$\displaystyle P_i^{L}({\bf G})$ $\displaystyle =$ $\displaystyle \int_{\omega} Y_L^\star(\omega) e^{i G r_i} d\omega$ (184)
  $\displaystyle =$ $\displaystyle \int_{\omega} Y_L^\star(\omega) 4 \pi \sum_{l=0}^{\infty} i^l j_l(G r_i) \sum_{m\prime=-l}^l
Y_{lm\prime}^\star(\omega) Y_{lm\prime}(\bf G) d\omega$ (185)
  $\displaystyle =$ $\displaystyle 4 \pi i^l j_l(G r_i) Y_L (\hat G) \enspace ,$ (186)

where the expansion of a plane wave in spherical harmonics has been used. $ j_l$ are the spherical Bessel functions and $ \hat G$ the angular components of the Fourier vector $ {\bf G}$ .


next up previous contents index
Next: Kleinman-Bylander Scheme Up: Pseudopotentials in the Plane Previous: Pseudopotentials in the Plane   Contents   Index
Costas Bekas 2008-09-04