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%% This BibTeX bibliography file was created using BibDesk.
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%% http://bibdesk.sourceforge.net/
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%% Created for Pierre-Francois Loos at 2020-04-08 14:13:22 +0200
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%% Created for Pierre-Francois Loos at 2020-04-09 10:05:15 +0200
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%% Saved with string encoding Unicode (UTF-8)
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@article{Woon_1994,
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Author = {Woon, D. and Dunning, T. H.},
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Date-Added = {2020-04-09 09:59:19 +0200},
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Date-Modified = {2020-04-09 10:00:56 +0200},
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Doi = {10.1063/1.466439},
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Journal = {J. Chem. Phys.},
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Pages = {2975--2988},
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Title = {Gaussian basis sets for use in correlated molecular calculations. IV. Calculation of static electrical response properties},
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Volume = {100},
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Year = {1994},
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Bdsk-Url-1 = {https://doi.org/10.1063/1.466439}}
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@article{Kendall_1992,
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Author = {Kendall, R. A. and Dunning, T. H. and Harisson, R. J.},
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Date-Added = {2020-04-09 09:58:17 +0200},
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Date-Modified = {2020-04-09 10:01:10 +0200},
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Doi = {10.1063/1.462569},
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Journal = {J. Chem. Phys.},
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Pages = {6796--6806},
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Title = {Electron affinities of the first-row atoms revisited. Systematic basis sets and wave functions},
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Volume = {96},
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Year = {1992},
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Bdsk-Url-1 = {https://doi.org/10.1063/1.462569}}
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@article{Dunning_1989,
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Author = {T. H. {Dunning, Jr.}},
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Date-Added = {2020-04-09 09:55:22 +0200},
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Date-Modified = {2020-04-09 09:55:22 +0200},
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Doi = {10.1063/1.456153},
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Journal = {J. Chem. Phys.},
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Pages = {1007},
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Title = {Gaussian basis sets for use in correlated molecular calculations. I. The atoms boron through neon and hydrogen},
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Volume = {90},
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Year = {1989},
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Bdsk-Url-1 = {https://doi.org/10.1063/1.456153}}
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@misc{numgrid,
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Author = {R. Bast},
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Date-Added = {2020-04-09 09:23:10 +0200},
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Date-Modified = {2020-04-09 09:23:10 +0200},
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Doi = {10.5281/zenodo.2659208},
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Month = {May},
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Note = {\url{https://github.com/dftlibs/numgrid}},
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Publisher = {Zenodo},
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Title = {numgrid: numerical integration grid for molecules},
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Url = {https://github.com/dftlibs/numgrid},
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Year = {2019},
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Bdsk-Url-1 = {https://github.com/LCPQ/quantum_package},
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Bdsk-Url-2 = {http://dx.doi.org/10.5281/zenodo.200970}}
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@misc{QuAcK,
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Author = {P. F. Loos},
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Date-Added = {2020-04-09 09:19:41 +0200},
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Date-Modified = {2020-04-09 09:33:32 +0200},
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Doi = {10.5281/zenodo.3745928},
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Note = {\url{https://github.com/pfloos/QuAcK}},
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Publisher = {Zenodo},
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Title = {{{QuAcK: a software for emerging quantum electronic structure methods}}},
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Url = {https://github.com/pfloos/QuAcK},
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Year = {2019},
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Bdsk-Url-1 = {https://github.com/LCPQ/quantum_package},
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Bdsk-Url-2 = {http://dx.doi.org/10.5281/zenodo.200970}}
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@article{Fromager_2020,
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Archiveprefix = {arXiv},
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Author = {Emmanuel Fromager},
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@ -27,7 +90,8 @@
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Pages = {L5},
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Title = {Autoionizing States of the Hydrogen Molecule.},
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Volume = {7},
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Year = {1974}}
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Year = {1974},
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Bdsk-Url-1 = {https://doi.org/10.1088/0022-3700/7/1/002}}
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@article{Mielke_2005,
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Author = {S. L. Mielke and D. W. Schwenke and K. A. Peterson},
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@ -91,13 +155,6 @@
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Pages = {arXiv:2003.05553},
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Title = {A weight-dependent local correlation density-functional approximation for ensembles},
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Year = {submitted}}
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@article{Fromager_2020,
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title={Individual correlations in ensemble density-functional theory: State-driven/density-driven decomposition without additional Kohn-Sham systems},
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author={Fromager, Emmanuel},
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journal={arXiv:2001.08605},
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year={submitted},
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url={https://arxiv.org/abs/2001.08605}}
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@article{Lindh_2001,
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Author = {R. Lindh and P.-A. Malmqvist and L. Gagliardi},
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@ -376,7 +433,8 @@
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@article{Perdew_1983,
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Author = {J. P. Perdew and M. Levy},
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Date-Added = {2019-09-05 12:04:19 +0200},
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Date-Modified = {2019-09-05 12:13:34 +0200},
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Date-Modified = {2020-04-09 10:05:15 +0200},
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Doi = {10.1103/PhysRevLett.51.1884},
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Journal = {Phys. Rev. Lett.},
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Pages = {1884},
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Title = {Physical Content of the Exact Kohn-Sham Orbital Energies: Band Gaps and Derivative Discontinuities},
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@ -183,12 +183,12 @@ However, Loos and Gill have recently shown that there exists other UEGs which co
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Electrons restricted to remain on the surface of a $\cD$-sphere (where $\cD$ is the dimensionality of the surface of the sphere) are an example of finite UEGs (FUEGs). \cite{Loos_2011b}
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In particular, we combine these FUEGs with the usual infinite UEG (IUEG) to construct a weigh-dependent LDA correlation functional for ensembles, which is specifically designed to compute double excitations within GOK-DFT, and automatically incorporates the infamous derivative discontinuity contribution to the excitation energies through its explicit ensemble weight dependence. \cite{Levy_1995, Perdew_1983}
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%The paper is organised as follows.
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%In Sec.~\ref{sec:theo}, the theory behind GOK-DFT is presented.
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%Section \ref{sec:func} provides details about the construction of the weight-dependent xc LDA functional.
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%The results of our calculations for the prototypical \ce{H2} molecule are reported and discussed in Sec.~\ref{sec:resdis}.
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%Finally, we draw our conclusions in Sec.~\ref{sec:ccl}.
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%Unless otherwise stated, atomic units are used throughout.
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The paper is organised as follows.
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In Sec.~\ref{sec:theo}, the theory behind GOK-DFT is presented.
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Section \ref{sec:compdet} provides the computational details.
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The results of our calculations for two-electron systems are reported and discussed in Secs.~\ref{sec:res_H2} and \ref{sec:res_He}.
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Finally, we draw our conclusions in Sec.~\ref{sec:ccl}.
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Unless otherwise stated, atomic units are used throughout.
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%%%%%%%%%%%%%%%%%%%%
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%%% THEORY %%%
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@ -248,7 +248,7 @@ is the density matrix operator, $\lbrace \Det{I}{\bw} \rbrace_{0 \le I \le \nEns
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\end{split}
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\end{equation}
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is the ensemble Hartree-exchange-correlation (Hxc) functional.
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Note that the weight-independent Hartree functional $\E{\Ha}{}[\n{}{}]$ causes the infamous ghost-interaction error (GIE) \cite{Gidopoulos_2002, Pastorczak_2014, Alam_2016, Alam_2017, Gould_2017} in eDFT, which is supposed to be cancelled by the weight-dependent xc functional $\E{\xc}{\bw}[\n{}{}]$.
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Note that the weight-independent Hartree functional $\E{\Ha}{}[\n{}{}]$ causes the infamous ghost-interaction error \cite{Gidopoulos_2002, Pastorczak_2014, Alam_2016, Alam_2017, Gould_2017} in eDFT, which is supposed to be cancelled by the weight-dependent xc functional $\E{\xc}{\bw}[\n{}{}]$.
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From the GOK-DFT ensemble energy expression in Eq.~\eqref{eq:Ew-GOK}, we obtain \cite{Gross_1988b,Deur_2019}
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\begin{equation}
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@ -312,15 +312,15 @@ where $\e{\ex}{\ew{}}(\n{}{})$ and $\e{\co}{\ew{}}(\n{}{})$ are the weight-depen
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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\section{Computational details}
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\label{sec:compdet}
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The self-consistent GOK-DFT calculations have been performed with the \texttt{QuAcK} software, freely available on \texttt{github}, where the present functional has been implemented.
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The self-consistent GOK-DFT calculations have been performed in a restricted formalism with the \texttt{QuAcK} software, \cite{QuAcK} which is freely available on \texttt{github}, and where the present weight-dependent functionals have been implemented.
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For more details about the self-consistent implementation of GOK-DFT, we refer the interested reader to Ref.~\onlinecite{Loos_2020} where additional technical details can be found.
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For all calculations, we use a restricted formalism and the aug-cc-pVXZ (X = D, T, and Q) Dunning's family of atomic basis sets.
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Numerical quadratures are performed with the \texttt{numgrid} library using 194 angular points (Lebedev grid) and a radial precision of $10^{-6}$. \cite{Becke_1988,Lindh_2001}
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For all calculations, we use the aug-cc-pVXZ (X = D, T, Q, and 5) Dunning family of atomic basis sets. \cite{Dunning_1989,Kendall_1992,Woon_1994}
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Numerical quadratures are performed with the \texttt{numgrid} library \cite{numgrid} using 194 angular points (Lebedev grid) and a radial precision of $10^{-6}$. \cite{Becke_1988,Lindh_2001}
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This study deals only with spin-unpolarised systems, \ie, $\n{\uparrow}{} = \n{\downarrow}{} = \n{}{}/2$ (where $\n{\uparrow}{}$ and $\n{\downarrow}{}$ are the spin-up and spin-down electron densities).
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Moreover, we restrict our study to the case of a two-state ensemble (\ie, $\nEns = 2$) where both the ground state ($I=0$ with weight $1 - \ew{}$) and the first doubly-excited state ($I=1$ with weight $\ew{}$) are considered.
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Although we should have $0 \le \ew{} \le 1/2$ to ensure the GOK variational principle, we will sometimes ``violate'' this variational constraint.
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Although one should have $0 \le \ew{} \le 1/2$ to ensure the GOK variational principle, we will sometimes ``violate'' this variational constraint.
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Indeed, the limit $\ew{} = 1$ is of particular interest as it corresponds to a genuine saddle point of the KS equations, and match perfectly the results obtained with the maximum overlap method (MOM) developed by Gilbert, Gill and coworkers. \cite{Gilbert_2008,Barca_2018a,Barca_2018b}
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Moreover, the limits $\ew{} = 0$ and $\ew{} = 1$ are the only two weights for which there is no ghost-interaction error.
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\titou{Moreover, the limits $\ew{} = 0$ and $\ew{} = 1$ are the only two weights for which there is no ghost-interaction error.}
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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\section{Hydrogen molecule}
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@ -340,9 +340,9 @@ First, we compute the ensemble energy of the \ce{H2} molecule (at equilibrium bo
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In the case of \ce{H2}, the ensemble is composed by the $1\sigma_g^2$ ground state and the lowest doubly-excited state of configuration $1\sigma_u^2$, which has an autoionising resonance nature. \cite{Bottcher_1974}
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The ensemble energy $\E{}{\ew{}}$ is depicted in Fig.~\ref{fig:Ew_H2} as a function of the weight $0 \le \ew{} \le 1$.
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Because this exchange functional does not depend on the ensemble weight, there is no contribution from the ensemble derivative term [last term in Eq.~\eqref{eq:dEdw}].
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As anticipated, $\E{}{\ew{}}$ is far from being linear, which means that the excitation energy obtained via the derivative of the local energy varies significantly with the weight of the double excitation (see Fig.~\ref{fig:Om_H2}).
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As anticipated, $\E{}{\ew{}}$ is far from being linear, which means that the excitation energy obtained via the derivative of the ensemble energy varies significantly with the weight of the double excitation (see Fig.~\ref{fig:Om_H2}).
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Taking as a reference the full configuration interaction (FCI) value of $28.75$ eV obtained with the aug-mcc-pV8Z basis set, \cite{Barca_2018a} one can see that the excitation energy varies by more than $8$ eV from $\ew{} = 0$ to $1/2$.
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Note that the exact xc correlation ensemble functional would yield a perfectly linear energy and, hence, the same value of the excitation energy independently of $\ew{}$.
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Note that the exact xc ensemble functional would yield a perfectly linear energy and, hence, the same value of the excitation energy independently of $\ew{}$.
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\begin{figure}
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\includegraphics[width=\linewidth]{Ew_H2}
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@ -365,8 +365,8 @@ Note that the exact xc correlation ensemble functional would yield a perfectly l
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\subsection{Weight-dependent exchange functional}
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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Second, in order to remove this spurious curvature of the ensemble energy (which is mostly due to the ghost-interaction error, but not only), one can easily reverse-engineer (for this particular system and basis set) a local exchange functional to make $\E{}{\ew{}}$ as linear as possible for $0 \le \ew{} \le 1$.
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Doing so, we have found that the present weight-dependent exchange functional (denoted as GIC-S in the following as its main purpose is to correct for the ghost-interaction error), represented in Fig.~\ref{fig:Cx_H2},
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Second, in order to remove this spurious curvature of the ensemble energy (which is mostly due to the ghost-interaction error, but not only), one can easily reverse-engineer (for this particular system, geometry, and basis set) a local exchange functional to make $\E{}{\ew{}}$ as linear as possible for $0 \le \ew{} \le 1$.
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Doing so, we have found that the present weight-dependent exchange functional (denoted as GIC-S in the following as its main purpose is to correct for the ghost-interaction error)
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\begin{equation}
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\e{\ex}{\ew{},\text{GIC-S}}(\n{}{}) = \Cx{\ew{}} \n{}{1/3},
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\end{equation}
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@ -379,22 +379,23 @@ and
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\begin{subequations}
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\begin{align}
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\alpha & = + 0.575\,178,
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\\
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&
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\beta & = - 0.021\,108,
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\\
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&
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\gamma & = - 0.367\,189,
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\end{align}
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\end{subequations}
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makes the ensemble almost perfectly linear (see Fig.~\ref{fig:Ew_H2}), and the excitation energy much more stable and closer to the FCI reference (see Fig.~\ref{fig:Om_H2}).
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As readily seen from Eq.~\eqref{eq:Cxw}, $\Cx{\ew{}}$ reduces to $\Cx{}$ for $\ew{} = 0$.
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Note that we are not only using data from $\ew{} = 0$ to $\ew{} = 1/2$, but we also consider ensemble energies for $1/2 < \ew{} \le 1$, which is strictly forbidden by the GOK variational principle. \cite{Gross_1988a}
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However, it is important to ensure that the weight-dependent functional does not affect the two ghost-interaction-free limits at $\ew{} = 0$ and $\ew{} = 1$.
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Therefore, by construction, the weight-dependent correction vanishes for these two limiting weight values (see Fig.~\ref{fig:Cx_H2}).
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As readily seen from Eq.~\eqref{eq:Cxw} and graphically illustrated in Fig.~\ref{fig:Cx_H2}, the weight-dependent correction does not affect the two ghost-interaction-free limits at $\ew{} = 0$ and $\ew{} = 1$, as $\Cx{\ew{}}$ reduces to $\Cx{}$ in these two limits.
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Note that we are not only using data from $0 \le \ew{} \le 1/2$, but we also consider ensemble energies for $1/2 < \ew{} \le 1$, which is strictly forbidden by the GOK variational principle. \cite{Gross_1988a}
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However, it is important to ensure that the weight-dependent functional does not alter the $\ew{} = 1$, which corresponds to a genuine saddle point of the KS equations, as mentioned above.
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Finally, let us mention that, around $\ew{} = 0$, the behaviour of Eq.~\eqref{eq:Cxw} is linear.
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\begin{figure}
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\includegraphics[width=0.8\linewidth]{Cx_H2}
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\caption{
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$\Cx{\ew{}}/\Cx{\ew{}=0}$ as a function of $\ew{}$ [see Eq.~\eqref{eq:Cxw}].
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$\Cx{\ew{}}/\Cx{\ew{}=0}$ as a function of $\ew{}$ [see Eq.~\eqref{eq:Cxw}] for the \ce{H2} molecule at equilibrium bond length and the aug-cc-pVTZ basis set.
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\titou{T2: Add the same curve for He and stretch H2.}
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\label{fig:Cx_H2}
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}
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\end{figure}
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@ -733,8 +734,6 @@ Excitation energies (in eV) associated with the lowest double excitation of \ce{
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HF & FCI & aug-cc-pV5Z & & & & 8.69 \\
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\end{tabular}
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\end{ruledtabular}
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\fnt[1]{Reference \onlinecite{Mielke_2005}.}
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\fnt[2]{Reference \onlinecite{Barca_2018a}.}
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\end{table*}
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%%% %%% %%% %%%
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