new equations for excitation energies
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@ -2,7 +2,10 @@
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0.0457 0.0450 0.0435 0.0409 0.0362 0.0241 0.0033
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0.0861 0.0838 0.0793 0.0712 0.0571 0.0377 0.0196
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0.1044 0.1036 0.1022 0.0997 0.0953 0.0830 0.0540
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0.1447 0.1424 0.1380 0.1300 0.1162 0.0966 0.0703
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0.1447 0.1424 0.1380 0.1300 0.1162 0.0966 0.0703
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-0.1356 -0.1342 -0.1314 -0.1264 -0.1176 -0.1037 -0.0849
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-0.1356 -0.1342 -0.1314 -0.1263 -0.1174 -0.1031 -0.0834
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-0.1356 -0.1341 -0.1314 -0.1262 -0.1172 -0.1026 -0.0824
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0.0000 0.0000 0.0000 0.0000 0.0000 0.0000 0.0000
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0.0172 0.0163 0.0147 0.0117 0.0067 -0.0004 -0.0080
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0.0416 0.0402 0.0376 0.0329 0.0253 0.0140 0.0005
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@ -11,6 +14,9 @@
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0.1080 0.1056 0.1011 0.0925 0.0772 0.0538 0.0325
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0.0092 0.0081 0.0060 0.0022 -0.0035 -0.0081 -0.0047
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0.1010 0.0986 0.0943 0.0862 0.0719 0.0523 0.0373
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-0.1160 -0.1154 -0.1141 -0.1115 -0.1069 -0.0991 -0.0870
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-0.1160 -0.1154 -0.1140 -0.1115 -0.1069 -0.0991 -0.0872
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-0.1160 -0.1153 -0.1140 -0.1115 -0.1069 -0.0991 -0.0871
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-0.0196 -0.0188 -0.0174 -0.0148 -0.0106 -0.0044 0.0029
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-0.0024 -0.0025 -0.0027 -0.0032 -0.0040 -0.0050 -0.0056
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0.0220 0.0213 0.0201 0.0180 0.0146 0.0093 0.0027
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@ -622,7 +622,7 @@ Equation \eqref{eq:ec} is depicted in Fig.~\ref{fig:Ec} for each state alongside
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\caption{
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\label{tab:OptGap_2}
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Deviation from the FCI quantities (in hartree) of the individual energies, $\E{(I)}$, and the corresponding excitation energies, $\Ex{(I)}$, for the ground ($I=0$), singly-excited ($I=1$) and doubly-excited ($I=2$) states of 2-boxium (i.e.,~$\Nel = 2$ electrons in a box of length $L$).
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The values of the derivative discontinuity $\DD{c}{(I)}$ are also reported.
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The values of the ensemble correlation derivative $\DD{c}{(I)}$ are also reported.
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(DNC = KS calculation does not converge.)
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}
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\begin{ruledtabular}
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@ -685,7 +685,7 @@ Equation \eqref{eq:ec} is depicted in Fig.~\ref{fig:Ec} for each state alongside
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\caption{
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\label{tab:OptGap_3}
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Deviation from the FCI quantities (in hartree) of the individual energies, $\E{(I)}$, and the corresponding excitation energies, $\Ex{(I)}$, for the ground ($I=0$), singly-excited ($I=1$) and doubly-excited ($I=2$) states of 3-boxium (i.e.,~$\Nel = 3$ electrons in a box of length $L$).
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The values of the derivative discontinuity $\DD{c}{(I)}$ are also reported.
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The values of the ensemble correlation derivative $\DD{c}{(I)}$ are also reported.
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}
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\begin{ruledtabular}
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\begin{tabular}{lclddddddd}
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@ -748,7 +748,7 @@ Equation \eqref{eq:ec} is depicted in Fig.~\ref{fig:Ec} for each state alongside
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\caption{
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\label{tab:OptGap_4}
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Deviation from the FCI quantities (in hartree) of the individual energies, $\E{(I)}$, and the corresponding excitation energies, $\Ex{(I)}$, for the ground ($I=0$), singly-excited ($I=1$) and doubly-excited ($I=2$) states of 4-boxium (i.e.,~$\Nel = 4$ electrons in a box of length $L$).
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The values of the derivative discontinuity $\DD{c}{(I)}$ are also reported.
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The values of the ensemble correlation derivative $\DD{c}{(I)}$ are also reported.
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}
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\begin{ruledtabular}
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\begin{tabular}{lclddddddd}
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@ -810,7 +810,7 @@ Equation \eqref{eq:ec} is depicted in Fig.~\ref{fig:Ec} for each state alongside
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\caption{
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\label{tab:OptGap_5}
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Deviation from the FCI quantities (in hartree) of the individual energies, $\E{(I)}$, and the corresponding excitation energies, $\Ex{(I)}$, for the ground ($I=0$), singly-excited ($I=1$) and doubly-excited ($I=2$) states of 5-boxium (i.e.,~$\Nel = 5$ electrons in a box of length $L$).
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The values of the derivative discontinuity $\DD{c}{(I)}$ are also reported.
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The values of the ensemble correlation derivative $\DD{c}{(I)}$ are also reported.
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}
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\begin{ruledtabular}
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\begin{tabular}{lclddddddd}
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@ -872,7 +872,7 @@ Equation \eqref{eq:ec} is depicted in Fig.~\ref{fig:Ec} for each state alongside
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\caption{
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\label{tab:OptGap_6}
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Deviation from the FCI quantities (in hartree) of the individual energies, $\E{(I)}$, and the corresponding excitation energies, $\Ex{(I)}$, for the ground ($I=0$), singly-excited ($I=1$) and doubly-excited ($I=2$) states of 6-boxium (i.e.,~$\Nel = 6$ electrons in a box of length $L$).
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The values of the derivative discontinuity $\DD{c}{(I)}$ are also reported.
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The values of the ensemble correlation derivative $\DD{c}{(I)}$ are also reported.
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}
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\begin{ruledtabular}
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\begin{tabular}{lclddddddd}
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@ -935,7 +935,7 @@ Equation \eqref{eq:ec} is depicted in Fig.~\ref{fig:Ec} for each state alongside
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\caption{
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\label{tab:OptGap_7}
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Deviation from the FCI quantities (in hartree) of the individual energies, $\E{(I)}$, and the corresponding excitation energies, $\Ex{(I)}$, for the ground ($I=0$), singly-excited ($I=1$) and doubly-excited ($I=2$) states of 7-boxium (i.e.,~$\Nel = 7$ electrons in a box of length $L$).
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The values of the derivative discontinuity $\DD{c}{(I)}$ are also reported.
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The values of the ensemble correlation derivative $\DD{c}{(I)}$ are also reported.
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}
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\begin{ruledtabular}
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\begin{tabular}{lclddddddd}
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@ -71,7 +71,7 @@
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\newcommand{\opGam}[1]{\hat{\Gamma}^{#1}}
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\newcommand{\bh}{\boldsymbol{h}}
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\newcommand{\bF}[1]{\boldsymbol{F}^{#1}}
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\newcommand{\Ex}[1]{\Omega^{#1}}
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\newcommand{\Ex}[2]{\Omega_\text{#1}^{#2}}
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% elements
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@ -302,7 +302,7 @@ where the KS wavefunctions fulfill the ensemble density constraint
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\sum_{K\geq 0} \ew{K} \n{\Det{(K),\bw}[\n{}{}]}{}(\br{}) = \n{}{}(\br{}).
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\eeq
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The (approximate) description of the correlation part is discussed in
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Sec.~\ref{sec:eDFA}.\\
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Sec.~\ref{sec:eDFA}.
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In practice, the ensemble energy is not the most interesting quantity, and one is more concerned with excitation energies or individual energy levels (for geometry optimizations, for example).
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As pointed out recently in Ref.~\cite{Deur_2019}, the latter can be extracted
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@ -314,7 +314,7 @@ exactly from a single ensemble calculation as follows:
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where, according to the normalization condition of Eq.~(\ref{eq:weight_norm_cond}),
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\beq
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\pdv{\E{}{\bw}}{\ew{K}}= \E{}{(K)} -
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\E{}{(0)}\equiv\Ex{(K)}
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\E{}{(0)}\equiv\Ex{}{(K)}
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\eeq
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corresponds to the $K$th excitation energy.
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According to the {\it variational} ensemble energy expression of
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@ -825,7 +825,7 @@ as well as {\it curvature}~\cite{Alam_2016,Alam_2017}:
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The ensemble energy is of course expected to vary linearly with the ensemble
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weights [see Eq.~(\ref{eq:exact_GOK_ens_ener})].
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These errors are essentially removed when evaluating the individual energy
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levels on the basis of Eq.~\eqref{eq:exact_ind_ener_rdm}.\\
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levels on the basis of Eq.~\eqref{eq:exact_ind_ener_rdm}.
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Turning to the density-functional ensemble correlation energy, the
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following ensemble local density approximation (eLDA) will be employed:
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@ -835,8 +835,8 @@ following ensemble local density approximation (eLDA) will be employed:
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where the correlation energy per particle $\e{c}{\bw}(\n{}{})$ is \textit{weight dependent}.
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As shown in Sec.~\ref{sec:eDFA}, the latter can be constructed, for
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example, from a finite uniform electron gas model.
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\titou{Manu, I think we should clearly define here what the expression of the ensemble energy with and without GOC.
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What do you think?}
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%\titou{Manu, I think we should clearly define here what the expression of the ensemble energy with and without GOC.
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%What do you think?}
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Combining Eq.~\eqref{eq:exact_ind_ener_rdm} with Eq.~\eqref{eq:eLDA_corr_fun} leads to our final energy level expression within KS-eLDA:
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\beq\label{eq:EI-eLDA}
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@ -881,8 +881,36 @@ density-functional approximation that incorporates ensemble weight
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dependencies explicitly, thus allowing for the description of derivative
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discontinuities [see Eq.~\eqref{eq:excited_ener_level_gs_lim} and the
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comment that follows] {\it via} the last term on the right-hand side
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of Eq.~\eqref{eq:EI-eLDA}.\\
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of Eq.~\eqref{eq:EI-eLDA}.
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\titou{The GIC KS-eLDA ensemble energy is thus given by
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\beq\label{eq:Ew-eLDA}
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\E{GIC-eLDA}{\bw}=\sum_{I\geq0}\ew{I}\E{{eLDA}}{(I)},
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\eeq
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while the uncorrected KS-eLDA ensemble energy obtained via Eq.~\eqref{eq:min_with_HF_ener_fun} can be recast as
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\beq\label{eq:Ew-GIC-eLDA}
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\E{eLDA}{\bw}=\E{GIC-eLDA}{\bw}+\WHF[
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\bGam{\bw}]-\sum_{I\geq0}\ew{I}\WHF[ \bGam{(I)}].
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\eeq
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%Manu, would it be useful to add this equation and the corresponding text?
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%I think it is useful for the discussion later on when we talk about the different contributions to the excitation energies.
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%This shows clearly that there is a correction due to the correlation functional itself as well as a correction due to the ensemble correlation derivative
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The corresponding excitation energies are
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\beq\label{eq:Om-eLDA}
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\begin{split}
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\Ex{eLDA}{(I)}
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& =
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\Ex{HF}{(I)}
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\\
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& + \int \fdv{\E{c}{\bw}[\n{\bGam{\bw}}{}]}{\n{}{}(\br{})}
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\qty[ \n{\bGam{(I)}}{}(\br{}) - \n{\bGam{(0)}}{}(\br{}) ] d\br{}
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\\
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& + \int \n{\bGam{\bw}}{}(\br{})
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\left. \pdv{\e{c}{\bw}(\n{}{})}{\ew{I}} \right|_{\n{}{}=\n{\bGam{\bw}}{}(\br{})} d\br{},
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\end{split}
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\eeq
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with $\Ex{HF}{(I)} = \E{HF}{(I)} - \E{HF}{(0)}$, where the last term is the ensemble correlation derivative contribution to the excitation energy.
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}
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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\section{Density-functional approximations for ensembles}
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\label{sec:eDFA}
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@ -1116,15 +1144,7 @@ The deviation from linearity of the three-state ensemble energy $\E{}{(\ew{1},\e
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in Fig.~\ref{fig:EvsW} as a function of both $\ew{1}$ and $\ew{2}$ while
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fulfilling the restrictions on the ensemble weights to ensure the GOK
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variational principle [\ie, $0 \le \ew{2} \le 1/3$ and $\ew{2} \le \ew{1} \le (1-\ew{2})/2$].
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To illustrate the magnitude of the ghost interaction error (GIE), we report the KS-eLDA ensemble energy with and without ghost interaction correction (GIC) as explained above [see Eqs.~\eqref{eq:WHF} and \eqref{eq:EI-eLDA}].
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\titou{Manu will move this to the theory section later on
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\beq
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\E{GIC-eLDA}{\bw}=\sum_{I\geq0}\ew{I}\E{{eLDA}}{(I)},
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\eeq
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\beq
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\E{eLDA}{\bw}=\E{GIC-eLDA}{\bw}+\WHF[
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\bGam{\bw}]-\sum_{I\geq0}\ew{I}\WHF[ \bGam{(I)}]
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\eeq}
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To illustrate the magnitude of the ghost interaction error (GIE), we report the KS-eLDA ensemble energy with and without ghost interaction correction (GIC) as explained above \titou{[see Eqs.~\eqref{eq:Ew-GIC-eLDA} and \eqref{eq:Ew-eLDA}]}.
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As one can see in Fig.~\ref{fig:EvsW}, without GIC, the
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ensemble energy becomes less and less linear as $L$
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gets larger, while the GIC makes the ensemble energy almost
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@ -1150,7 +1170,7 @@ linear.
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It is important to note that, even though the GIC removes the explicit
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quadratic terms from the ensemble energy, a non-negligible curvature
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remains in the GIC-eLDA ensemble energy due to the optimization of the
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ensemble KS orbitals in the presence of GIE [see Eq.~\eqref{eq:min_with_HF_ener_fun}].
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ensemble KS orbitals in the presence of GIE \titou{[see Eqs.~\eqref{eq:min_with_HF_ener_fun} and \eqref{eq:Ew-eLDA}]}.
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%However, this orbital-driven error is small (in our case at
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%least) \trashEF{as the correlation part of the ensemble KS potential $\delta
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%\E{c}{\bw}[\n{}{}] /\delta \n{}{}(\br{})$ is relatively small compared
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@ -1187,7 +1207,7 @@ Interesting also to see that the reverse occurs in the tri-ensemble.}
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\includegraphics[width=\linewidth]{EvsL_5}
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\caption{
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\label{fig:EvsL}
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Excitation energies (multiplied by $L^2$) associated with the single excitation $\Ex{(1)}$ (bottom) and double excitation $\Ex{(2)}$ (top) of 5-boxium for various methods and box length $L$.
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Excitation energies (multiplied by $L^2$) associated with the single excitation $\Ex{}{(1)}$ (bottom) and double excitation $\Ex{}{(2)}$ (top) of 5-boxium for various methods and box length $L$.
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Graphs for additional values of $\nEl$ can be found as {\SI}.
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}
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\end{figure}
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@ -1200,11 +1220,12 @@ In other words, each excitation is dominated by a sole, well-defined reference S
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However, when the box gets larger (\ie, $L$ increases), there is a strong mixing between the different excitation degrees.
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In particular, the single and double excitations strongly mix, which makes their assignment as single or double excitations more discutable. \cite{Loos_2019}
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This can be clearly evidenced by the weights of the different configurations in the FCI wave function.
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% TITOU: shall we keep the paragraph below?
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Therefore, it is paramount to construct a two-weight correlation functional
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(\ie, a triensemble functional, as we have done here) which
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allows the mixing of singly- and doubly-excited configurations.
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Using a single-weight (\ie, a biensemble) functional where only the ground state and the lowest singly-excited states are taken into account, one would observe a neat deterioration of the excitation energies (as compared to FCI) when the box gets larger.
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\titou{Shall we add results for the biensemble to illustrate this?}
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\titou{Titou will add results for the biensemble to illustrate this.}
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%\manu{Well, neglecting the second excited state is not the same as
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%considering the $w_2=0$ limit. I thought you were referring to an
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%approximation where the triensemble calculation is performed with
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@ -1212,13 +1233,13 @@ Using a single-weight (\ie, a biensemble) functional where only the ground state
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%because, in this limit, you may still have a derivative discontinuity
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%correction. The latter is absent if you truly neglect the second excited
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%state in your ensemble functional. This should be clarified.}\\
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\manu{Are the results in the supp mat? We could just add "[not
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shown]" if not. This is fine as long as you checked that, indeed, the
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results deteriorate ;-)}
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\manu{Should we add that, in the bi-ensemble case, the ensemble
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correlation derivative $\partial \epsilon^\bw_{\rm c}(n)/\partial w_2$
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is neglected (if this is really what you mean (?)). I guess that this is the reason why
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the second excitation energy would not be well described (?)}
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%\manu{Are the results in the supp mat? We could just add "[not
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%shown]" if not. This is fine as long as you checked that, indeed, the
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%results deteriorate ;-)}
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%\manu{Should we add that, in the bi-ensemble case, the ensemble
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%correlation derivative $\partial \epsilon^\bw_{\rm c}(n)/\partial w_2$
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%is neglected (if this is really what you mean (?)). I guess that this is the reason why
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%the second excitation energy would not be well described (?)}
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As shown in Fig.~\ref{fig:EvsL}, all methods provide accurate estimates of the excitation energies in the weak correlation regime (\ie, small $L$).
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When the box gets larger, they start to deviate.
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@ -1286,7 +1307,7 @@ electrons.
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\includegraphics[width=\linewidth]{EvsL_5_HF}
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\caption{
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\label{fig:EvsLHF}
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Error with respect to FCI (in \%) associated with the single excitation $\Ex{(1)}$ (bottom) and double excitation $\Ex{(2)}$ (top) as a function of the box length $L$ for 5-boxium at the KS-eLDA (solid lines) and eHF (dashed lines) levels.
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Error with respect to FCI (in \%) associated with the single excitation $\Ex{}{(1)}$ (bottom) and double excitation $\Ex{}{(2)}$ (top) as a function of the box length $L$ for 5-boxium at the KS-eLDA (solid lines) and eHF (dashed lines) levels.
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Zero-weight (\ie, $\ew{1} = \ew{2} = 0$, red lines) and state-averaged (\ie, $\ew{1} = \ew{2} = 1/3$, blue lines) calculations are reported.
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}
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\end{figure}
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@ -1299,7 +1320,7 @@ To do so, we have reported in Fig.~\ref{fig:EvsLHF} the error percentage
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(with respect to FCI) on the excitation energies obtained at the KS-eLDA
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and HF\manu{-like} levels [see Eqs.~\eqref{eq:EI-eLDA} and
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\eqref{eq:ind_HF-like_ener}, respectively] as a function of the box
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length $L$ in the case of 5-boxium.\\
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length $L$ in the case of 5-boxium.
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\manu{Manu: there is something I do not understand. If you want to
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evaluate the importance of the ensemble correlation derivatives you
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should only remove the following contribution from the $K$th KS-eLDA
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21357
Notebooks/eDFT_FUEG.nb
21357
Notebooks/eDFT_FUEG.nb
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