Manu: saving work in the discussion
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@ -1273,8 +1273,13 @@ drastically.
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%drives the all thing.\\}
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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 ghost-interaction error {[see Eqs.~\eqref{eq:min_with_HF_ener_fun} and \eqref{eq:Ew-eLDA}]}.
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remains in the GIC-eLDA ensemble energy. \manu{This might be due to
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\textit{(i)} the correlation eLDA
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functional, which induces linear or quadratic weight dependencies of the individual
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energies [see Eqs.~\eqref{eq:Taylor_exp_ind_corr_ener_eLDA} and
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\eqref{eq:Taylor_exp_DDisc_term}], and \textit{(ii)} the optimization of the
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ensemble KS orbitals in the presence of ghost-interaction errors {[see
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Eqs.~\eqref{eq:min_with_HF_ener_fun} and \eqref{eq:WHF}]}}.
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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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