Manu: started polishing the theory. Saving work.

This commit is contained in:
Emmanuel Fromager 2019-10-11 12:43:35 +02:00
parent 89038f94fb
commit 34607cf900

View File

@ -381,9 +381,7 @@ Hxc}\left[n_{\bmg^{\bw}}\right]
\Big\} \Big\}
, ,
\eeq \eeq
where $n_{\bmg^{\bw}}$ where $n_{\bmg^{\bw}}$ is the density obtained from the density matrix
\manu{I am in favor of using $n_{{\bmg}^{{\bw}}}$ rather than $n_{\bmg^{\bw}}$,
for clarity} is the density obtained from the density matrix
${\bmg}^{\bw}$ and ${\bm h}={\bm t}+{\bm v}_{\rm ext}$ is the total one-electron ${\bmg}^{\bw}$ and ${\bm h}={\bm t}+{\bm v}_{\rm ext}$ is the total one-electron
Hamiltonian matrix representation. When the minimum is reached, the Hamiltonian matrix representation. When the minimum is reached, the
ensemble energy and its derivatives can be used to extract individual ensemble energy and its derivatives can be used to extract individual
@ -607,7 +605,7 @@ Tr}\left[{\bm F}^{(L)}\frac{\partial \bmg^{(L)}}{\partial w_K}\right].
According to Eqs.~(\ref{eq:indiv_ener_from_ens}), According to Eqs.~(\ref{eq:indiv_ener_from_ens}),
(\ref{eq:exact_Eens_EEXX}), and (\ref{eq:XE_EEXX}), (\ref{eq:exact_Eens_EEXX}), and (\ref{eq:XE_EEXX}),
\beq \beq\label{eq:exact_ind_ener_OEP-like}
E^{(I)}&&={\rm E^{(I)}&&={\rm
Tr}\left[{\bmg}^{(I)}{\bm h}\right] Tr}\left[{\bmg}^{(I)}{\bm h}\right]
+\frac{1}{2} \Tr(\bmg^{(I)} \, \bG \, +\frac{1}{2} \Tr(\bmg^{(I)} \, \bG \,
@ -628,7 +626,28 @@ Tr}\left[{\bm F}^{(L)}\frac{\partial \bmg^{(L)}}{\partial w_K}\right]
. .
\eeq \eeq
\subsection{Two-step ghost-interaction-corrected calculation}
In order to compute (approximate) energy levels within generalized
GOK-DFT we use a two-step procedure. The first step consists in
optimizing variationally the ensemble density matrix according to
Eq.~(\ref{eq:var_princ_Gamma_ens}) with an approximate Hxc ensemble
functional where (i) the ghost-interaction correction functional $\overline{E}^{{\bw}}_{\rm
Hx}[n]$ in
Eq.~(\ref{eq:exact_GIC}) is
neglected, for simplicity, and (ii) the weight-dependent correlation
energy is descrive at the local density level of approximation. More
details about the construction of such a functional will be given in the
following. In order to remove ghost interactions from the variational energy
expression used in the first step, we then employ the (in-principle-exact)
expression in Eq.~(\ref{eq:exact_ind_ener_OEP-like}). In this second
step, the response of the individual density matrices to weight
variations (last term on the right-hand side of
Eq.~(\ref{eq:exact_ind_ener_OEP-like})) is neglected. The complete GIC
procedure can be summarized as follows,
\alert{Secs. \ref{sec:KS-eDFT}-\ref{sec:E_I} should maybe be moved to an appendix or merged
with the theory section (?)}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection{KS-eDFT for excited states} \subsection{KS-eDFT for excited states}
\label{sec:KS-eDFT} \label{sec:KS-eDFT}
@ -719,7 +738,6 @@ The (state-independent) Levy-Zahariev shift and the so-called derivative discont
\end{align} \end{align}
Because the Levy-Zahariev shift is state independent, it does not contribute to excitation energies [see Eq.~\eqref{eq:Ex}]. Because the Levy-Zahariev shift is state independent, it does not contribute to excitation energies [see Eq.~\eqref{eq:Ex}].
The only remaining piece of information to define at this stage is the weight-dependent Hartree-exchange-correlation functional $\be{Hxc}{\bw}(\n{}{})$. The only remaining piece of information to define at this stage is the weight-dependent Hartree-exchange-correlation functional $\be{Hxc}{\bw}(\n{}{})$.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\section{Density-functional approximations for ensembles} \section{Density-functional approximations for ensembles}
\label{sec:eDFA} \label{sec:eDFA}