Manu: fixing my corrections
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@ -121,9 +121,7 @@
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\begin{document}
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\title{Weight-dependent local density-functional \manu{approximation to
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ensemble correlation energies}}
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%\title{Weight-dependent local density-functional approximations for ensembles}
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\title{A weight-dependent local correlation density-functional approximation for ensembles}
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\author{Pierre-Fran\c{c}ois Loos}
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\email{loos@irsamc.ups-tlse.fr}
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@ -1272,16 +1270,16 @@ drastically.
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%when looking at your curves, this assumption cannot be made when the
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%correlation is strong. It is not clear to me which integral ($W_{01}?$)
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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 \manu{Hx} terms from the ensemble energy, a non-negligible curvature
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remains in the GIC-eLDA ensemble energy \manu{when the electron
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correlation is strong}. \manu{This is due to
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It is important to note that, even though the GIC removes the explicitly
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quadratic Hx terms from the ensemble energy, a non-negligible curvature
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remains in the GIC-eLDA ensemble energy when the electron
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correlation is strong. This is due to
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\textit{(i)} the correlation eLDA
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functional, which contributes linearly (or even quadratically) to 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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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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