Manu: saving work

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Emmanuel Fromager 2020-02-11 10:11:16 +01:00
parent 1184d379c3
commit 3bf0fca3ad

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@ -333,14 +333,26 @@ _{n=n_{\opGamma{\bw}}}.
\eeq
For implementation purposes, we will use in the rest of this work
(one-electron reduced) density matrices rather than Slater determinants
as basic variables. If we denote ${\bmg}^{(K)}$
(one-electron reduced) density matrices
as basic variables, rather than Slater determinants. If we expand the
(spin-) orbitals [from which the latter are constructed] in an atomic
orbital (AO) basis,
\beq
\Gamma_{\mu\nu}^{(K)}=\sum_{p\in (K)}c_{\mu p}c_{\nu p}
\varphi_p({\bfx})=\sum_{\mu}c_{{\mu p}}\AO{\mu}(\bfx),
\eeq
then the density matrix elements obtained from the
determinant $\Phi^{(K)}$ can be expressed as follows in the AO basis:
\beq
\Gamma_{\mu\nu}^{(K)}=\sum_{p\in (K)}c_{\mu p}c_{\nu p},
\eeq
where the summation runs over the spin-orbitals that are occupied in
$\Phi^{(K)}$.
$\Phi^{(K)}$. We can then construct the ensemble density matrix
\beq
{\bmg}^{{\bw}}=\sum_{K\geq 0}w_K{\bmg}^{(K)}
\eeq
and compute the ensemble density as follows:
$n^{\bw}({\br})=$
can be determined.
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%\subsection{Hybrid GOK-DFT}
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