Manu: started polishing the theory section

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Emmanuel Fromager 2020-02-04 15:00:50 +01:00
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@ -98,6 +98,7 @@
\newcommand{\bfx}{\bf{x}} \newcommand{\bfx}{\bf{x}}
\newcommand{\bfr}{\bf{r}} \newcommand{\bfr}{\bf{r}}
\DeclareMathOperator*{\argmin}{arg\,min} \DeclareMathOperator*{\argmin}{arg\,min}
\newcommand{\blue}[1]{{\textcolor{blue}{#1}}}
%%%% %%%%
\begin{document} \begin{document}
@ -169,33 +170,9 @@ Atomic units are used throughout.
\label{sec:eDFT} \label{sec:eDFT}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection{Kohn--Sham formulation of GOK-DFT} \subsection{GOK-DFT}
Let us start from the analog for ensembles of Levy's universal
functional,
\beq\label{eq:ens_LL_func}
F^{\bw}[n]&=&
\underset{\hat{\gamma}^{{\bw}}\rightarrow n}{\rm min}\left\{{\rm
Tr}\left[\hat{\gamma}^{{\bw}}\left(\hat{T}+\hat{W}_{\rm
ee}\right)\right]\right\}
\eeq
where ${\rm
Tr}$ denotes the trace. The minimization over trial ensemble density matrix operators
$\hat{\gamma}^{{\bw}}=\sum_{K\geq0}w_K\vert\Psi^{(K)}\rangle\langle\Psi^{(K)}\vert$
is performed under the following density constraint:
\beq
{\rm
Tr}\left[\hat{\gamma}^{{\bw}}\hat{n}(\br)\right]=\sum_{K\geq0}w_Kn_{\Psi^{(K)}}(\br)=n(\br),
\eeq
where $\hat{n}(\br)$ is the density operator, $n_{\Psi}$ denotes the
density of wavefunction $\Psi$, and
$\bw\equiv\left(w^{(1)},w^{(2)},\ldots\right)$ is the collection of
(decreasing) ensemble weights assigned to the excited states. Note that
$w_0=1-\sum_{K>0}w_K\geq 0$.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection{Hybrid GOK-DFT} \subsection{Hybrid GOK-DFT}
\label{sec:geKS}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
Since Hartree and exchange energy contributions cannot be separated in Since Hartree and exchange energy contributions cannot be separated in
the one-dimensional case, we introduce in the following an alternative the one-dimensional case, we introduce in the following an alternative
@ -268,28 +245,8 @@ determinants $\Phi^{(K)}$. Note that the density matrices
${\bmg}^{(K)}={\bmg}^{\Phi^{(K)}}$ are idempotent and diagonal in the ${\bmg}^{(K)}={\bmg}^{\Phi^{(K)}}$ are idempotent and diagonal in the
same spin-orbital basis). On the other hand, the ensemble same spin-orbital basis). On the other hand, the ensemble
density matrix ${\bmg}^{{\bw}}=\sum_{K\geq 0}w_K{\bmg}^{(K)}$, which is a convex combination of the ${\bmg}^{(K)}$ density matrix ${\bmg}^{{\bw}}=\sum_{K\geq 0}w_K{\bmg}^{(K)}$, which is a convex combination of the ${\bmg}^{(K)}$
matrices, is {\it not} idempotent, unless ${\bw}=0$. Indeed, matrices, is {\it not} idempotent, unless ${\bw}=0$.
\beq Using an ensemble is, in this context,
\left[{\bmg}^{{\bw}}\right]^2&=&\sum_{K,L\geq
0}w_Kw_L{\bmg}^{(K)}{\bmg}^{(L)}
\nonumber\\
&=&\sum_{K\geq
0}\left(w_K\right)^2{\bmg}^{(K)}+\sum_{K\neq L\geq
0}w_Kw_L{\bmg}^{(K)}{\bmg}^{(L)}
\nonumber\\
&=&
{\bmg}^{{\bw}}+\sum_{K,L\geq
0}w_K\left(w_L-\delta_{KL}\right){\bmg}^{(K)}{\bmg}^{(L)}
\nonumber\\
&=&{\bmg}^{{\bw}}+w_0{\bmg}^{(0)}\times\sum_{K>0}w_K\left(2{\bmg}^{(K)}-1\right)
\nonumber\\
&&+\sum_{K, L >0
}w_K\left(w_L-\delta_{KL}\right){\bmg}^{(K)}{\bmg}^{(L)}
\nonumber\\
&\neq&{\bmg}^{{\bw}}
.
\eeq
This is of course expected since using an ensemble is, in this context,
analogous to assigning analogous to assigning
fractional occupation numbers (which are determined from the ensemble fractional occupation numbers (which are determined from the ensemble
weights) to the KS orbitals.\\ weights) to the KS orbitals.\\
@ -532,6 +489,120 @@ Hxc}(n)}{\partial w_K}\right|_{n=n_{\bmg^{\bw}}(\br)}.
\eeq \eeq
} }
\subsection{Approximations}
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 described at the local density level of approximation.
At this
level of approximation, the two correlation functionals $\overline{E}^{{\bw}}_{\rm
c}[n]$ and ${E}^{{\bw}}_{\rm
c}[n]$ are actually identical and can be expressed as
\beq\label{eq:eLDA_corr_fun}
{E}^{{\bw}}_{\rm
c}[n]=\int d\br\;n(\br)\epsilon_{c}^{\bw}(n(\br)).
\eeq
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,
\beq
{\bmg}^{\bw}\approx\argmin_{{\bm\gamma}^{\bw}}
\Big\{
{\rm
Tr}\left[{\bm \gamma}^{{\bw}}{\bm h}\right]+W_{\rm
HF}\left[{\bm\gamma}^{\bw}\right]
+
{E}^{{\bw}}_{\rm
c}\left[n_{\bm\gamma^{\bw}}\right]
%+E^{{\bw}}_{\rm c}\left[n_{\hat{\Gamma}^{{\bw}}}\right]
\Big\},
\nonumber\\
\eeq
and
\beq
E^{(I)}&&\approx{\rm
Tr}\left[{\bmg}^{(I)}{\bm h}\right]
+\frac{1}{2} \Tr(\bmg^{(I)} \, \bG \,
\bmg^{(I)})
\nonumber\\
&&+{E}^{{\bw}}_{\rm
c}\left[n_{\bmg^{\bw}}\right]
+\int d\br\,\dfrac{\delta {E}^{{\bw}}_{\rm
c}\left[n_{\bmg^{\bw}}\right]}{\delta
n({\br})}\left(n_{\bmg^{(I)}}(\br)-n_{\bmg^{\bw}}(\br)\right)
\nonumber\\
&&+\sum_{K>0}\left(\delta_{IK}-w_K\right)\left. \dfrac{\partial {E}^{{\bw}}_{\rm
c}\left[n\right]}{\partial w_K}\right|_{n=n_{\bmg^{\bw}}}
,
\eeq
thus leading to the final implementable expression [see Eq.~(\ref{eq:eLDA_corr_fun})]
\beq
E^{(I)}&&\approx{\rm
Tr}\left[{\bmg}^{(I)}{\bm h}\right]
+\frac{1}{2} \Tr(\bmg^{(I)} \, \bG \,
\bmg^{(I)})
\nonumber\\
&&+\int d\br\,
{\epsilon}^{{\bw}}_{\rm
c}(n_{\bmg^{\bw}}(\br))\,n_{\bmg^{(I)}}(\br)
\nonumber\\
&&
+\int d\br\,\left.\dfrac{\partial {\epsilon}^{{\bw}}_{\rm
c}(n)}{\partial n}\right|_{n=n_{\bmg^{\bw}}(\br)}n_{\bmg^{\bw}}(\br)\left(n_{\bmg^{(I)}}(\br)-n_{\bmg^{\bw}}(\br)\right)
\nonumber\\
&&
+\int d\br\,\sum_{K>0}\left(\delta_{IK}-w_K\right)n_{\bmg^{\bw}}(\br)\left.
\dfrac{\partial {\epsilon}^{{\bw}}_{\rm
c}(n)}{\partial w_K}\right|_{n=n_{\bmg^{\bw}}(\br)}.
\eeq
\blue{$================================$}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\section{Theory (old)}
\label{sec:eDFT_old}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection{Kohn--Sham formulation of GOK-DFT}
Let us start from the analog for ensembles of Levy's universal
functional,
\beq\label{eq:ens_LL_func}
F^{\bw}[n]&=&
\underset{\hat{\gamma}^{{\bw}}\rightarrow n}{\rm min}\left\{{\rm
Tr}\left[\hat{\gamma}^{{\bw}}\left(\hat{T}+\hat{W}_{\rm
ee}\right)\right]\right\}
\eeq
where ${\rm
Tr}$ denotes the trace. The minimization over trial ensemble density matrix operators
$\hat{\gamma}^{{\bw}}=\sum_{K\geq0}w_K\vert\Psi^{(K)}\rangle\langle\Psi^{(K)}\vert$
is performed under the following density constraint:
\beq
{\rm
Tr}\left[\hat{\gamma}^{{\bw}}\hat{n}(\br)\right]=\sum_{K\geq0}w_Kn_{\Psi^{(K)}}(\br)=n(\br),
\eeq
where $\hat{n}(\br)$ is the density operator, $n_{\Psi}$ denotes the
density of wavefunction $\Psi$, and
$\bw\equiv\left(w^{(1)},w^{(2)},\ldots\right)$ is the collection of
(decreasing) ensemble weights assigned to the excited states. Note that
$w_0=1-\sum_{K>0}w_K\geq 0$.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection{Hybrid GOK-DFT}
\label{sec:geKS}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection{Exact ensemble exchange in hybrid GOK-DFT} \subsection{Exact ensemble exchange in hybrid GOK-DFT}
@ -635,82 +706,6 @@ Tr}\left[{\bm F}^{(L)}\frac{\partial \bmg^{(L)}}{\partial w_K}\right]
correlation LDA and ghost interaction correction correlation LDA and ghost interaction correction
} }
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 described at the local density level of approximation.
At this
level of approximation, the two correlation functionals $\overline{E}^{{\bw}}_{\rm
c}[n]$ and ${E}^{{\bw}}_{\rm
c}[n]$ are actually identical and can be expressed as
\beq\label{eq:eLDA_corr_fun}
{E}^{{\bw}}_{\rm
c}[n]=\int d\br\;n(\br)\epsilon_{c}^{\bw}(n(\br)).
\eeq
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,
\beq
{\bmg}^{\bw}\approx\argmin_{{\bm\gamma}^{\bw}}
\Big\{
{\rm
Tr}\left[{\bm \gamma}^{{\bw}}{\bm h}\right]+W_{\rm
HF}\left[{\bm\gamma}^{\bw}\right]
+
{E}^{{\bw}}_{\rm
c}\left[n_{\bm\gamma^{\bw}}\right]
%+E^{{\bw}}_{\rm c}\left[n_{\hat{\Gamma}^{{\bw}}}\right]
\Big\},
\nonumber\\
\eeq
and
\beq
E^{(I)}&&\approx{\rm
Tr}\left[{\bmg}^{(I)}{\bm h}\right]
+\frac{1}{2} \Tr(\bmg^{(I)} \, \bG \,
\bmg^{(I)})
\nonumber\\
&&+{E}^{{\bw}}_{\rm
c}\left[n_{\bmg^{\bw}}\right]
+\int d\br\,\dfrac{\delta {E}^{{\bw}}_{\rm
c}\left[n_{\bmg^{\bw}}\right]}{\delta
n({\br})}\left(n_{\bmg^{(I)}}(\br)-n_{\bmg^{\bw}}(\br)\right)
\nonumber\\
&&+\sum_{K>0}\left(\delta_{IK}-w_K\right)\left. \dfrac{\partial {E}^{{\bw}}_{\rm
c}\left[n\right]}{\partial w_K}\right|_{n=n_{\bmg^{\bw}}}
,
\eeq
thus leading to the final implementable expression [see Eq.~(\ref{eq:eLDA_corr_fun})]
\beq
E^{(I)}&&\approx{\rm
Tr}\left[{\bmg}^{(I)}{\bm h}\right]
+\frac{1}{2} \Tr(\bmg^{(I)} \, \bG \,
\bmg^{(I)})
\nonumber\\
&&+\int d\br\,
{\epsilon}^{{\bw}}_{\rm
c}(n_{\bmg^{\bw}}(\br))\,n_{\bmg^{(I)}}(\br)
\nonumber\\
&&
+\int d\br\,\left.\dfrac{\partial {\epsilon}^{{\bw}}_{\rm
c}(n)}{\partial n}\right|_{n=n_{\bmg^{\bw}}(\br)}n_{\bmg^{\bw}}(\br)\left(n_{\bmg^{(I)}}(\br)-n_{\bmg^{\bw}}(\br)\right)
\nonumber\\
&&
+\int d\br\,\sum_{K>0}\left(\delta_{IK}-w_K\right)n_{\bmg^{\bw}}(\br)\left.
\dfrac{\partial {\epsilon}^{{\bw}}_{\rm
c}(n)}{\partial w_K}\right|_{n=n_{\bmg^{\bw}}(\br)}.
\eeq
\alert{Secs. \ref{sec:KS-eDFT}-\ref{sec:E_I} should maybe be moved to an appendix or merged \alert{Secs. \ref{sec:KS-eDFT}-\ref{sec:E_I} should maybe be moved to an appendix or merged
with the theory section (?)} with the theory section (?)}
@ -1062,6 +1057,34 @@ E.~F.~thanks the \textit{Agence Nationale de la Recherche} (MCFUNEX project, Gra
\end{acknowledgements} \end{acknowledgements}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%% REMOVED FROM THE MAIN TEXT by Manu %%%%%%%%%%%%
\iffalse%%%%
Indeed,
\beq
\left[{\bmg}^{{\bw}}\right]^2&=&\sum_{K,L\geq
0}w_Kw_L{\bmg}^{(K)}{\bmg}^{(L)}
\nonumber\\
&=&\sum_{K\geq
0}\left(w_K\right)^2{\bmg}^{(K)}+\sum_{K\neq L\geq
0}w_Kw_L{\bmg}^{(K)}{\bmg}^{(L)}
\nonumber\\
&=&
{\bmg}^{{\bw}}+\sum_{K,L\geq
0}w_K\left(w_L-\delta_{KL}\right){\bmg}^{(K)}{\bmg}^{(L)}
\nonumber\\
&=&{\bmg}^{{\bw}}+w_0{\bmg}^{(0)}\times\sum_{K>0}w_K\left(2{\bmg}^{(K)}-1\right)
\nonumber\\
&&+\sum_{K, L >0
}w_K\left(w_L-\delta_{KL}\right){\bmg}^{(K)}{\bmg}^{(L)}
\nonumber\\
&\neq&{\bmg}^{{\bw}}
.
\eeq
%%%% End -- REMOVED FROM THE MAIN TEXT by Manu %%%%%%%%%%%%
\fi%%%
\bibliography{eDFT} \bibliography{eDFT}
\end{document} \end{document}