Manu: sving work in II Cwq

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Emmanuel Fromager 2020-02-25 12:42:14 +01:00
parent d150248c25
commit 42c7682b09

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@ -200,7 +200,7 @@ Atomic units are used throughout.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
The GOK ensemble energy~\cite{Gross_1988a,Oliveira_1988,Gross_1988b} is defined as
\beq
\beq\label{eq:exact_GOK_ens_ener}
\E{}{\bw}=\sum_{K \geq 0} \ew{K} \E{}{(K)},
\eeq
where the $K$th energy level $\E{}{(K)}$ [$K=0$ refers to the ground state] is the eigenvalue of the electronic Hamiltonian $\hH = \hh + \hWee$, where
@ -576,28 +576,35 @@ w}_K
\subsection{Approximations}\label{subsec:approx}
%%%%%%%%%%%%%%%
As Hartree and exchange energies cannot be separated in the one-dimensional systems considered in the rest of this work, we will substitute the Hartree--Fock (HF) density-matrix-functional interaction energy,
In the following, GOK-DFT will be applied
to one-dimension
spin-polarized systems where
Hartree and exchange energies cannot be separated.
For that reason, we will substitute the Hartree--Fock (HF) density-matrix-functional interaction energy,
\beq\label{eq:eHF-dens_mat_func}
\WHF[\bGam{}] = \frac{1}{2} \Tr[\bGam{} \bG \bGam{}],
\eeq
for the Hx density-functional energy in the variational energy
expression of Eq.~\eqref{eq:var_ener_gokdft}:
\beq
expression of Eq.~\eqref{eq:var_ener_gokdft}, thus leading to the
following approximation:
\beq\label{eq:min_with_HF_ener_fun}
\bGam{\bw}
\approx \argmin_{\bgam{\bw}}
\rightarrow \argmin_{\bgam{\bw}}
\qty{
\Tr[\bgam{\bw} \bh ] + \WHF[ \bgam{\bw}] + \E{c}{\bw}[\n{\bgam{\bw}}{}]
}.
\eeq
\titou{Manu, I don't really understand the $\approx$ sign in the previous equation}
The minimizing ensemble density matrix fulfills the following
stationarity condition
The minimizing ensemble density matrix in Eq.~(\ref{eq:min_with_HF_ener_fun}) fulfills the following
stationarity condition:
\beq\label{eq:commut_F_AO}
\bF{\bw} \bGam{\bw} \bS = \bS \bGam{\bw} \bF{\bw},
\eeq
where $\bS \equiv \eS{\mu\nu} = \braket*{\AO{\mu}}{\AO{\nu}}$ is the metric and the ensemble Fock-like matrix reads
where $\bS \equiv \eS{\mu\nu} = \braket*{\AO{\mu}}{\AO{\nu}}$ is the
overlap matrix and the ensemble Fock-like matrix reads
\beq
\bF{\bw} \equiv \eF{\mu\nu}{\bw} = \eh{\mu\nu}{\bw} + \sum_{\la\si} \eG{\mu\nu\la\si} \eGam{\la\si}{\bw}
\bF{\bw} \equiv \eF{\mu\nu}{\bw} = \eh{\mu\nu}{\bw} +
\sum_{\la\si} \eG{\mu\nu\la\si} \eGam{\la\si}{\bw},
\eeq
with
\beq
@ -726,9 +733,15 @@ and
\fi%%%%%%%%%%%
%%%%% end Manu
%%%%%%%%%%%%%%%%%%%%
Note that this approximation, where the ensemble density matrix is optimized from a non-local exchange potential [rather than a local one, as expected from Eq.~\eqref{eq:var_ener_gokdft}] is applicable to real (three-dimensional) systems.
As readily seen from Eq.~\eqref{eq:eHF-dens_mat_func}, \textit{ghost interactions}~\cite{Gidopoulos_2002, Pastorczak_2014, Alam_2016, Alam_2017, Gould_2017}
and curvature~\cite{} will be introduced in the Hx energy:
Note that, within the approximation of Eq.~(\ref{eq:min_with_HF_ener_fun}), the ensemble density matrix is
optimized with a non-local exchange potential rather than a
density-functional local one, as expected from
Eq.~\eqref{eq:var_ener_gokdft}. This procedure is actually general, \ie,
applicable to not-necessarily spin polarized and real (higher-dimension) systems.
As readily seen from Eq.~\eqref{eq:eHF-dens_mat_func}, inserting the
ensemble density matrix into the HF interaction energy functional
introduces unphysical \textit{ghost interaction} errors~\cite{Gidopoulos_2002, Pastorczak_2014, Alam_2016, Alam_2017, Gould_2017}
as well as {\it curvature}~\cite{Alam_2016,Alam_2017}:
\beq\label{eq:WHF}
\begin{split}
\WHF[\bGam{\bw}]
@ -737,14 +750,19 @@ and curvature~\cite{} will be introduced in the Hx energy:
& + \sum_{L>K\geq 0} \ew{K} \ew{L}\Tr[\bGam{(K)} \bG \bGam{(L)}].
\end{split}
\eeq
These errors will be removed when computing individual energies according to Eq.~\eqref{eq:exact_ind_ener_rdm}.
The ensemble energy is of course expected to vary linearly with the ensemble
weights [see Eq.~(\ref{eq:exact_GOK_ens_ener})].
These errors are essentially removed when evaluating the individual energy
levels on the basis of Eq.~\eqref{eq:exact_ind_ener_rdm}.\\
Turning to the density-functional ensemble correlation energy, the following eLDA functional will be employed:
Turning to the density-functional ensemble correlation energy, the
following ensemble local density approximation (eLDA) will be employed:
\beq\label{eq:eLDA_corr_fun}
\E{c}{\bw}[\n{}{}] = \int \n{}{}(\br{}) \e{c}{\bw}(\n{}{}(\br{})) d\br{},
\E{c}{\bw}[\n{}{}]\approx \int \n{}{}(\br{}) \e{c}{\bw}(\n{}{}(\br{})) d\br{},
\eeq
where the correlation energy per particle is \textit{weight dependent}.
Its construction from a finite uniform electron gas model is discussed in detail in Sec.~\ref{sec:eDFA}.
where the correlation energy per particle $\e{c}{\bw}(\n{}{})$ is \textit{weight dependent}.
As shown in Sec.~\ref{sec:eDFA}, the latter can be constructed, for
example, from a finite uniform electron gas model.
\titou{Manu, I think we should clearly define here what the expression of the ensemble energy with and without GOC.
What do you think?}
@ -752,8 +770,10 @@ Combining Eq.~\eqref{eq:exact_ind_ener_rdm} with Eq.~\eqref{eq:eLDA_corr_fun} le
\beq\label{eq:EI-eLDA}
\begin{split}
\E{\titou{eLDA}}{(I)}
& \titou{\approx} \Tr[\bGam{(I)} \bh] + \frac{1}{2} \Tr[\bGam{(I)} \bG \bGam{(I)}]
& =
\E{HF}{(I)}
\\
%\Tr[\bGam{(I)} \bh] + \frac{1}{2} \Tr[\bGam{(I)} \bG \bGam{(I)}]
& + \int \e{c}{\bw}(\n{\bGam{\bw}}{}(\br{})) \n{\bGam{(I)}}{}(\br{}) d\br{}
\\
&
@ -765,7 +785,17 @@ Combining Eq.~\eqref{eq:exact_ind_ener_rdm} with Eq.~\eqref{eq:eLDA_corr_fun} le
\end{split}
\eeq
\titou{T2: I think we should specify what those terms are physically... Maybe earlier in the manuscript?}
where
\beq
\E{HF}{(I)}=\Tr[\bGam{(I)} \bh] + \frac{1}{2} \Tr[\bGam{(I)} \bG \bGam{(I)}]
\eeq
is the analog for ground {\it and} excited states of the HF energy.
Let us stress that, to the best of our knowledge, eLDA is the first
density-functional approximation that incorporates weight
dependencies explicitly, thus allowing for the description of derivative
discontinuities [see Eq.~\eqref{eq:excited_ener_level_gs_lim} and the
comment that follows] {\it via} the last term on the right-hand side
of Eq.~\eqref{eq:EI-eLDA}.\\
\titou{In order to test the influence of the derivative discontinuity on the excitation energies, it is useful to perform ensemble HF (labeled as eHF) calculations in which the correlation effects are removed.
In this case, the individual energies are simply defined as
\beq\label{eq:EI-eHF}