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