clean up results
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@ -120,7 +120,7 @@
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\newcommand{\bruno}[1]{\textcolor{blue}{Bruno: #1}}
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\begin{document}
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\title{Weight dependence of local exchange-correlation functionals: double excitations in two-electron systems}
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\title{Weight Dependence of Local Exchange-Correlation Functionals: Double Excitations in Two-Electron Systems}
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\author{Clotilde \surname{Marut}}
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\affiliation{\LCPQ}
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@ -695,11 +695,11 @@ To investigate the weight dependence of the xc functional in the strong correlat
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For this particular geometry, the doubly-excited state becomes the lowest excited state.
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We then follow the same protocol as in Sec.~\ref{sec:H2}, and considering again the aug-cc-pVTZ basis set, we design a GIC-S functional for this system at $\RHH = 3.7$ bohr.
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It yields $\alpha = +0.019\,226$, $\beta = -0.017\,996$, and $\gamma = -0.022\,945$ [see Eq.~\eqref{eq:Cxw}].
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The weight-dependence of $\Cx{\ew{}}$ is illustrated in Fig.~\ref{fig:Cxw} (green curve).
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The weight dependence of $\Cx{\ew{}}$ is illustrated in Fig.~\ref{fig:Cxw} (green curve).
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One clearly sees that the correction brought by GIC-S is much more gentle than at $\RHH = 1.4$ bohr, which means that the ensemble energy obtained with the LDA exchange functional is much more linear at $\RHH = 3.7$ bohr.
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In other words, the ghost-interaction ``hole'' depicted in Fig.~\ref{fig:Cxw} is thus much more shallow at stretched geometry.
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Table \ref{tab:BigTab_H2st} reports, for the aug-cc-pVTZ basis set (which delivers converged results with respect to the size of the basis set), the same set of calculations as in Table \ref{tab:BigTab_H2}.
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As a reference value, we have computed a FCI/aug-cc-pV5Z excitation energy of $8.69$ eV, which compares well with previous studies. \cite{Senjean_2015}
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Table \ref{tab:BigTab_H2st} reports, for the aug-cc-pVTZ basis set (which delivers basis set converged results), the same set of calculations as in Table \ref{tab:BigTab_H2}.
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As a reference value, we computed a FCI/aug-cc-pV5Z excitation energy of $8.69$ eV, which compares well with previous studies. \cite{Senjean_2015}
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For $\RHH = 3.7$ bohr, it is much harder to get an accurate estimate of the excitation energy, the best match being reached with HF exchange.
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The GIC-S functional coupled or not with a correlation functional yield extremely stable excitation energies as a function of the weight, with only a few tenths of eV difference between the zero- and equi-weights limits.
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Nonetheless, the excitation energy is still off by 3 eV.
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@ -709,7 +709,7 @@ The fact that HF exchange yields better excitation energy hints at the effect of
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%%% TABLE I %%%
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\begin{table}
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\caption{
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Excitation energies (in eV) associated with the lowest double excitation of \ce{H2} with $\RHH = 3.7$ bohr obtained with the aug-cc-pVTZ basis set for various methods and combinations of xc functionals.
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Excitation energies (in eV) associated with the lowest double excitation of \ce{H2} at $\RHH = 3.7$ bohr obtained with the aug-cc-pVTZ basis set for various methods and combinations of xc functionals.
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\label{tab:BigTab_H2st}
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}
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\begin{ruledtabular}
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@ -739,6 +739,7 @@ Excitation energies (in eV) associated with the lowest double excitation of \ce{
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\end{table}
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%%% %%% %%% %%%
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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\subsection{Helium atom}
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\label{sec:He}
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@ -748,14 +749,16 @@ As a final example, we consider the \ce{He} atom which can be seen as the limiti
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In \ce{He}, the lowest doubly-excited state is an auto-ionising resonance state, extremely high in energy and lies in the continuum. \cite{Madden_1963}
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In Ref.~\onlinecite{Burges_1995}, highly-accurate calculations estimate an excitation energy of $2.126$ hartree.
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Nonetheless, it can be nicely described with a Gaussian basis set containing enough diffuse functions.
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This is why we have considered for this particular example the d-aug-cc-pVQZ basis set which contains two sets of diffuse functions.
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Consequently, we considered for this particular example the d-aug-cc-pVQZ basis set which contains two sets of diffuse functions.
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The excitation energies associated with this double excitation computed with various methods and combinations of xc functionals are gathered in Table \ref{tab:BigTab_He}.
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The parameters of the GIC-S weight-dependent exchange functional are $\alpha = +1.912\,574$, $\beta = +2.715\,267$, and $\gamma = +2.163\,422$ [see Eq.~\eqref{eq:Cxw}], the curvature of the ensemble energy being more pronounced in \ce{He} than in \ce{H2} (see the blue curve in Fig.~\ref{fig:Cxw}).
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The parameters of the GIC-S weight-dependent exchange functional (computed with the smaller aug-cc-pVTZ basis) are $\alpha = +1.912\,574$, $\beta = +2.715\,267$, and $\gamma = +2.163\,422$ [see Eq.~\eqref{eq:Cxw}], the curvature of the ensemble energy being more pronounced in \ce{He} than in \ce{H2} (blue curve in Fig.~\ref{fig:Cxw}).
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In other words, the ghost-interaction hole is deeper.
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The results reported in Table \ref{tab:BigTab_He} evidence this strong weight dependence of the excitation energies for HF or LDA exchange.
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The GIC-S exchange functional attenuates significantly this dependence, and when coupled with the eVWN5 weight-dependent correlation functional, the GIC-SeVWN5 excitation energy for $\ew{} = 0$ is only $8$ millihartree off the reference value.
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The GIC-S exchange functional attenuates significantly this dependence, and when coupled with the eVWN5 weight-dependent correlation functional, the GIC-SeVWN5 excitation energy for $\ew{} = 0$ is only $8$ millihartree (or $0.22$ eV) off the reference value.
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As in the case of \ce{H2}, the excitation energies obtained at zero-weight are more accurate than at equi-weight.
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As a final comment, let us stress that the present protocole does not rely on high-level calculations as the sole requirement for constructing the GIC-S functional is the linearity of the ensemble energy.
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As a final comment, let us stress that the present protocol does not rely on high-level calculations as the sole requirement for constructing the GIC-S functional is the linearity of the ensemble energy with respect to the weight of the double excitation.
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%%% TABLE I %%%
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@ -790,13 +793,47 @@ Excitation energies (in hartree) associated with the lowest double excitation of
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\fnt[1]{Explicitly-correlated calculations from Ref.~\onlinecite{Burges_1995}.}
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\end{table}
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%%% TABLE I %%%
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%\begin{table}
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%\caption{
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%Excitation energies (in eV) associated with the lowest double excitation of \ce{HNO} obtained with the aug-cc-pVDZ basis set for various methods and combinations of xc functionals.
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%\label{tab:BigTab_H2st}
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%}
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%\begin{ruledtabular}
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%\begin{tabular}{llcccc}
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% \mc{2}{c}{xc functional} & \mc{2}{c}{GOK} \\
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% \cline{1-2} \cline{3-4}
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% \tabc{x} & \tabc{c} & $\ew{} = 0$ & $\ew{} = 1/2$ & LIM & MOM \\
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% \hline
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% HF & & & & & \\
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% HF & VWN5 & & & & \\
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% S & & 1.72 & 4.00 & 2.86 & 3.99 \\
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% S & VWN5 & & & & \\
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% GIC-S & & 3.99 & 3.99 & 3.99 & 3.99 \\
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% GIC-S & VWN5 & 4.05 & 4.03 & 4.04 & 4.03 \\
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% \hline
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% S & PW92 & & & & 4.00\fnm[1] \\
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% PBE & PBE & & & & 4.13\fnm[1] \\
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% SCAN & SCAN & & & & 4.24\fnm[1] \\
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% B97M-V & B97M-V & & & & 4.33\fnm[1] \\
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% PBE0 & PBE0 & & & & 4.24\fnm[1] \\
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% \hline
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% \mc{5}{l}{Theoretical best estimate\fnm[2]} & 4.32 \\
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%\end{tabular}
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%\end{ruledtabular}
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%\fnt[1]{Square gradient minimization (SGM) approach from Ref.~\onlinecite{Hait_2020} obtained with the aug-cc-pVTZ basis set. SGM is theoretically equivalent to MOM.}
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%\fnt[2]{Theoretical best estimate from Ref.~\onlinecite{Loos_2019} obtained at the (extrapolated) FCI/aug-cc-pVQZ level.}
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%\end{table}
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%%% %%% %%% %%%
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%%%%%%%%%%%%%%%%%%
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%%% CONCLUSION %%%
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%%%%%%%%%%%%%%%%%%
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\section{Conclusion}
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\label{sec:ccl}
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In the light of the results obtained in this study on double excitations computed within the GOK-DFT framework, we believe that the development of more universal weight-dependent exchange and correlation functionals has a bright future, and we hope to be able to report on this in the near future.
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In the light of the results obtained in this study on double excitations computed within the GOK-DFT framework, we believe that the development of more universal weight-dependent exchange and correlation functionals has a bright future, and we hope to be able to report further on this in the near future.
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%%%%%%%%%%%%%%%%%%%%%%%%
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%%% ACKNOWLEDGEMENTS %%%
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