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In order to obtain periodic orbitals, starting from non periodic ones it is sufficient to replace the Cartesian coordinates
with a simple periodic function
that take into account the appropriate periodicity of the box. In this thesis we used:
 |
(4.3) |
and the new distance is defined as
 |
(4.4) |
In doing so, we have only to compute gradients and Laplacian with the chain rule:
where
This transformation has been applied to all orbitals appearing in the wave-function and also to the one-body term and the two-body Jastrow.
We remark here that also the normalization constant of a given orbital has to be changed in a periodic system. Namely its integral over the simulation cell has to be equal to one.
 |
(4.5) |
For instance a normal Gaussian in three-dimension:
 |
(4.6) |
becomes after the substitution 4.3:
![$\displaystyle \Phi'(r') = \left ( L e^{-\frac{k L^2}{\pi^2}} I_0 \left [ \frac{k L^2 }{\pi^2} \right ] \right )^{-3/2} e^{ -k r'^2}$](img414.png) |
(4.7) |
where
is the modified Bessel function of the first kind and
is the size of the simulation box and
is the periodic distance 4.4.
Next: The wave-function for high
Up: Periodic Wave-Function
Previous: Periodic Wave-Function
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Claudio Attaccalite
2005-11-07