Manu: saving work
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@ -475,14 +475,14 @@ as follows:
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\eeq
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\eeq
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while the ensemble density matrix
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while the ensemble density matrix
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and the ensemble density read
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and the ensemble density read
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\beq
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\beq\label{eq:ens1RDM}
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\bGam{\bw}
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\bGam{\bw}
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= \sum_{K\geq 0} \ew{K} \bGam{(K)}
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= \sum_{K\geq 0} \ew{K} \bGam{(K)}
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\equiv \eGam{\mu\nu}{\bw}
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\equiv \eGam{\mu\nu}{\bw}
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= \sum_{K\geq 0} \ew{K} \eGam{\mu\nu}{(K)},
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= \sum_{K\geq 0} \ew{K} \eGam{\mu\nu}{(K)},
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\eeq
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\eeq
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and
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and
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\beq
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\beq\label{eq:ens_dens_from_ens_1RDM}
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\n{\bGam{\bw}}{}(\br{}) = \sum_{\mu\nu} \AO{\mu}(\br{}) \eGam{\mu\nu}{\bw} \AO{\nu}(\br{}),
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\n{\bGam{\bw}}{}(\br{}) = \sum_{\mu\nu} \AO{\mu}(\br{}) \eGam{\mu\nu}{\bw} \AO{\nu}(\br{}),
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\eeq
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\eeq
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respectively.
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respectively.
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@ -1055,15 +1055,20 @@ as $\ew{2}$ increases. The variations in the ensemble
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weights are essentially linear or quadratic.
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weights are essentially linear or quadratic.
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\manurev{This can be rationalized as follows. As readily seen from
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\manurev{This can be rationalized as follows. As readily seen from
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Eqs.~(\ref{eq:EI-eLDA}) and (\ref{eq:ind_HF-like_ener}), the individual
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Eqs.~(\ref{eq:EI-eLDA}) and (\ref{eq:ind_HF-like_ener}), the individual
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HF-like exchange does not depend explicitly on the weights, which means
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HF-like energies do not depend explicitly on the weights, which means
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that the above-mentioned variations originate from the eLDA correlation
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that the above-mentioned variations originate from the eLDA correlation
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functional [second and third terms on the right-hand side of
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functional [second and third terms on the right-hand side of
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Eq.~(\ref{eq:EI-eLDA})]. If, for analysis purposes, we consider the
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Eq.~(\ref{eq:EI-eLDA})]. If, for analysis purposes, we consider the
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Taylor expansions around the uniform density regime in Eqs.~(\ref{eq:Taylor_exp_ind_corr_ener_eLDA}) and (\ref{eq:Taylor_exp_DDisc_term})
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Taylor expansions around the uniform density regime in
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}They are induced by the
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Eqs.~(\ref{eq:Taylor_exp_ind_corr_ener_eLDA}) and
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eLDA correlation functional, as readily seen from
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(\ref{eq:Taylor_exp_DDisc_term}), contributions with an explicit weight
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Eqs.~\eqref{eq:Taylor_exp_ind_corr_ener_eLDA} and
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dependence still remain after summation. As both the ensemble density and
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\eqref{eq:Taylor_exp_DDisc_term}. In the biensemble, the weight dependence of the first
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the ensemble correlation energy per particle vary linearly with the
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weights $\bw$ [see Eqs.~(\ref{eq:ens1RDM}),
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(\ref{eq:ens_dens_from_ens_1RDM}), and
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(\ref{eq:decomp_ens_correner_per_part})], the latter contributions will contain both linear and quadratic terms in
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$\bw$, as readily seen from Eq.~(\ref{eq:Taylor_exp_DDisc_term}) [see the second term on the right-hand
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side].} In the biensemble, the weight dependence of the first
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excited-state energy is reduced as the correlation increases. On the other hand, switching from a bi- to a triensemble
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excited-state energy is reduced as the correlation increases. On the other hand, switching from a bi- to a triensemble
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systematically enhances the weight dependence, due to the lowering of the
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systematically enhances the weight dependence, due to the lowering of the
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ground-state energy, as $\ew{2}$ increases.
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ground-state energy, as $\ew{2}$ increases.
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