Modifs toto
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@ -1151,3 +1151,17 @@
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note = {}
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}
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@article{Nightingale_2001,
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author = {Nightingale, M. P. and Melik-Alaverdian, Vilen},
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title = {{Optimization of Ground- and Excited-State Wave Functions and van der Waals
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Clusters}},
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journal = {Phys. Rev. Lett.},
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volume = {87},
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number = {4},
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pages = {043401},
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year = {2001},
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month = {Jul},
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issn = {1079-7114},
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publisher = {American Physical Society},
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doi = {10.1103/PhysRevLett.87.043401}
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}
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@ -13,6 +13,8 @@
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]{hyperref}
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\urlstyle{same}
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\DeclareMathOperator*{\argmin}{arg\,min}
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\newcommand{\ie}{\textit{i.e.}}
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\newcommand{\eg}{\textit{e.g.}}
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\newcommand{\alert}[1]{\textcolor{red}{#1}}
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@ -36,6 +38,8 @@
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\newcommand{\EPT}{E_{\text{PT2}}}
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\newcommand{\EDMC}{E_{\text{FN-DMC}}}
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\newcommand{\Ndet}{N_{\text{det}}}
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\newcommand{\Nelec}{N_{\text{elec}}}
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\newcommand{\Nat}{N_{\text{atoms}}}
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\newcommand{\hartree}{$E_h$}
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\newcommand{\LCT}{Laboratoire de Chimie Th\'eorique (UMR 7616), Sorbonne Universit\'e, CNRS, Paris, France}
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@ -156,13 +160,13 @@ Another approach consists in considering the FN-DMC method as a
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\emph{post-FCI method}. The trial wave function is obtained by
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approaching the FCI with a selected configuration interaction (SCI)
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method such as CIPSI for instance.\cite{Giner_2013,Giner_2015,Caffarel_2016_2}
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\titou{When the basis set is increased, the trial wave function gets closer
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to the exact wave function, so the nodal surface can be systematically
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improved.\cite{Caffarel_2016} WRONG}
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This technique has the advantage \manu{of using the} FCI nodes in a given basis
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set \manu{, which is perfectly well defined and therefore makes the calculations} reproducible in a
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\toto{When the basis set is enlarged, the trial wave function gets closer to
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the exact wave function, so we expect the nodal surface to be
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improved.\cite{Caffarel_2016} }
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This technique has the advantage of using the FCI nodes in a given basis
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set, which is perfectly well defined and therefore makes the calculations reproducible in a
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black-box way without needing any expertise in QMC.
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\manu{Nevertheless,} this technique cannot be applied to large systems because of the
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Nevertheless, this technique cannot be applied to large systems because of the
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exponential scaling of the size of the trial wave function.
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Extrapolation techniques have been used to estimate the FN-DMC energies
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obtained with FCI wave functions,\cite{Scemama_2018} and other authors
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@ -225,8 +229,8 @@ of the wave functions is required.
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\subsection{CIPSI}
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%====================
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Beyond the single-determinant representation, the best
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multi-determinant wave function one can obtain \manu{in a given basis set} is the FCI.
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FCI is \manu{the ultimate goal of} \emph{post-Hartree-Fock} methods, and there exists several systematic
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multi-determinant wave function one can obtain in a given basis set is the FCI.
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FCI is the ultimate goal of \emph{post-Hartree-Fock} methods, and there exists several systematic
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improvements between the Hartree-Fock and FCI wave functions:
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increasing the maximum degree of excitation of CI methods (CISD, CISDT,
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CISDTQ, \emph{etc}), or increasing the complete active space
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@ -263,7 +267,7 @@ accuracy so all the CIPSI selections were made such that $\abs{\EPT} <
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\label{sec:rsdft}
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%=================================
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\manu{The range-separated DFT (RS-DFT)} was introduced in the seminal work of Savin,\cite{Sav-INC-96a,Toulouse_2004}
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The range-separated DFT (RS-DFT) was introduced in the seminal work of Savin,\cite{Sav-INC-96a,Toulouse_2004}
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where the Coulomb operator entering the electron-electron repulsion is split into two pieces:
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\begin{equation}
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\frac{1}{r}
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@ -279,7 +283,7 @@ where
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are the singular short-range (sr) part and the non-singular long-range (lr) part, respectively, $\mu$ is the range-separation parameter which controls how rapidly the short-range part decays, $\erf(x)$ is the error function, and $\erfc(x) = 1 - \erf(x)$ is its complementary version.
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The main idea behind RS-DFT is to treat the short-range part of the
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interaction \manu{using a density functional}, and the long-range part within a WFT method like FCI in the present case.
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interaction using a density functional, and the long-range part within a WFT method like FCI in the present case.
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The parameter $\mu$ controls the range of the separation, and allows
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to go continuously from the KS Hamiltonian ($\mu=0$) to
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the FCI Hamiltonian ($\mu = \infty$).
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@ -296,8 +300,8 @@ $\mathcal{F}^{\text{lr},\mu}$ is a long-range universal density
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functional and $\bar{E}_{\text{Hxc}}^{\text{sr,}\mu}$ is the
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complementary short-range Hartree-exchange-correlation (Hxc) density
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functional. \cite{Savin_1996,Toulouse_2004}
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\manu{The exact ground state energy can be therefore obtained as a minimization
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over a multi-determinant wave function as follows}:
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The exact ground state energy can therefore be obtained as a minimization
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over a multi-determinant wave function as follows:
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\begin{equation}
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\label{min_rsdft} E_0= \min_{\Psi} \qty{
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\mel{\Psi}{\hat{T}+\hat{W}_\text{{ee}}^{\text{lr},\mu}+\hat{V}_{\text{ne}}}{\Psi}
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@ -331,14 +335,12 @@ energy is obtained as
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E_0= \mel{\Psi^{\mu}}{\hat{T}+\hat{W}_\text{{ee}}^{\text{lr},\mu}+\hat{V}_{\text{ne}}}{\Psi^{\mu}}+\bar{E}^{\text{sr},\mu}_{\text{Hxc}}[n_{\Psi^\mu}].
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\end{equation}
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Note that, for $\mu=0$, \titou{the long-range interaction vanishes}, \ie,
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$w_{\text{ee}}^{\text{lr},\mu=0}(r) = 0$, and thus
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RS-DFT reduces to standard KS-DFT and $\Psi^\mu$
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is the KS determinant. For $\mu = \infty$, the long-range
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Note that for $\mu=0$ the long-range interaction vanishes, \ie,
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$w_{\text{ee}}^{\text{lr},\mu=0}(r) = 0$, and thus RS-DFT reduces to standard
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KS-DFT and $\Psi^\mu$ is the KS determinant. For $\mu = \infty$, the long-range
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interaction becomes the standard Coulomb interaction, \ie,
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$w_{\text{ee}}^{\text{lr},\mu\to\infty}(r) = r^{-1}$, and
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thus RS-DFT reduces to standard WFT and $\Psi^\mu$ is
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the FCI wave function.
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$w_{\text{ee}}^{\text{lr},\mu\to\infty}(r) = r^{-1}$, and thus RS-DFT reduces
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to standard WFT and $\Psi^\mu$ is the FCI wave function.
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%%% FIG 1 %%%
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\begin{figure*}
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@ -422,10 +424,9 @@ the pseudopotential is localized. Hence, in the DLA the fixed-node
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energy is independent of the Jastrow factor, as in all-electron
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calculations. Simple Jastrow factors were used to reduce the
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fluctuations of the local energy.
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The FN-DMC simulations are performed with the stochastic reconfiguration
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algorithm developed by Assaraf \textit{et al.}, \cite{Assaraf_2000}
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with a time step of $5 \times 10^{-4}$ a.u.
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\titou{All-electron move DMC?}
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The FN-DMC simulations are performed with all-electron moves using the
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stochastic reconfiguration algorithm developed by Assaraf \textit{et al.},
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\cite{Assaraf_2000} with a time step of $5 \times 10^{-4}$ a.u.
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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\section{Influence of the range-separation parameter on the fixed-node error}
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@ -434,8 +435,7 @@ with a time step of $5 \times 10^{-4}$ a.u.
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%%% TABLE I %%%
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\begin{table}
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\caption{Fixed-node energy $\EDMC$ (in \hartree{}) and number of determinants $\Ndet$ in \ce{H2O} for various trial wave functions $\Psi^{\mu}$.
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\titou{srPBE?}.}
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\caption{Fixed-node energy $\EDMC$ (in \hartree{}) and number of determinants $\Ndet$ in \ce{H2O} for various trial wave functions $\Psi^{\mu}$ obtained with the sr-PBE density functional.}
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\label{tab:h2o-dmc}
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\centering
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\begin{ruledtabular}
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@ -476,10 +476,11 @@ The first question we would like to address is the quality of the
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nodes of the wave function $\Psi^{\mu}$ obtained with an intermediate
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range separation parameter (\ie, $0 < \mu < +\infty$).
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For this purpose, we consider a weakly correlated molecular system, namely the water
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molecule \titou{near its equilibrium geometry.} \cite{Caffarel_2016}
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molecule near its equilibrium geometry. \cite{Caffarel_2016}
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We then generate trial wave functions $\Psi^\mu$ for multiple values of
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$\mu$, and compute the associated fixed-node energy keeping all the
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parameters having an impact on the nodal surface fixed \manu{such as CI coefficients and molecular orbitals}.
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$\mu$, and compute the associated fixed-node energy keeping fixed all the
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parameters such as the CI coefficients and molecular orbitals impacting the
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nodal surface.
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%======================================================
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\subsection{Fixed-node energy of $\Psi^\mu$}
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@ -501,19 +502,20 @@ and then the FN-DMC error raises until it reaches the $\mu=\infty$ limit (\ie, t
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For instance, with respect to the FN-DMC/VDZ-BFD energy at $\mu=\infty$,
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one can obtain a lowering of the FN-DMC energy of $2.6 \pm 0.7$~m\hartree{}
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with an optimal value of $\mu=1.75$~bohr$^{-1}$.
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\manu{This lowering in FN-DMC energy is to be compared with the $3.2 \pm 0.7$~m\hartree{} of gain in FN-DMC energy between the KS wave function ($\mu=0$) and the FCI wave function ($\mu=\infty$)}.
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When the basis set is increased, the gain in FN-DMC energy with
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respect to the FCI trial wave function is reduced, and the optimal
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value of $\mu$ is slightly shifted towards large $\mu$.
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This lowering in FN-DMC energy is to be compared with the $3.2 \pm
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0.7$~m\hartree{} gain in FN-DMC energy between the KS wave function ($\mu=0$)
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and the FCI wave function ($\mu=\infty$). When the basis set is increased, the
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gain in FN-DMC energy with respect to the FCI trial wave function is reduced,
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and the optimal value of $\mu$ is slightly shifted towards large $\mu$.
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Last but not least, the nodes of the wave functions $\Psi^\mu$ obtained with the srLDA
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exchange-correlation functional give very similar FN-DMC energies with respect
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to those obtained with the srPBE functional, even if the
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RS-DFT energies obtained with these two functionals differ by several
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tens of m\hartree{}.
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\manu{An other important aspect here regards the compactness of the trial wave functions $\Psi^\mu$:}
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\titou{at $\mu=1.75$~bohr$^{-1}$, $\Psi^{\mu}$ has \textit{only} $54\,540$ determinants at the srPBE/VDZ-BFD level, while the FCI wave function contains $200\,521$ determinants (see Table \ref{tab:h2o-dmc}). Even at the srPBE/VTZ-BFD level, we observe a reduction by a factor two in the number of determinants between the optimal $\mu$ value and $\mu = \infty$.
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The take-home message of this numerical study is that RS-DFT trial wave functions can yield a lower fixed-node energy with more compact multideterminant expansion as compared to FCI.}
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An other important aspect here regards the compactness of the trial wave functions $\Psi^\mu$:
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at $\mu=1.75$~bohr$^{-1}$, $\Psi^{\mu}$ has \textit{only} $54\,540$ determinants at the srPBE/VDZ-BFD level, while the FCI wave function contains $200\,521$ determinants (see Table \ref{tab:h2o-dmc}). Even at the srPBE/VTZ-BFD level, we observe a reduction by a factor two in the number of determinants between the optimal $\mu$ value and $\mu = \infty$.
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The take-home message of this numerical study is that RS-DFT trial wave functions can yield a lower fixed-node energy with more compact multideterminant expansion as compared to FCI.
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%======================================================
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\subsection{Link between RS-DFT and Jastrow factors }
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@ -521,11 +523,12 @@ The take-home message of this numerical study is that RS-DFT trial wave function
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%======================================================
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The data presented in Sec.~\ref{sec:fndmc_mu} evidence that, in a finite basis, RS-DFT can provide
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trial wave functions with better nodes than FCI wave function.
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Such behaviour can be directty compared to the common practice of
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Such behaviour can be directly compared to the common practice of
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re-optimizing the multideterminant part of a trial wave function $\Psi$ (the so-called Slater part) in the presence of the exponentiated Jastrow factor $e^J$. \cite{Umrigar_2005,Scemama_2006c,Umrigar_2007,Toulouse_2007,Toulouse_2008}
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Hence, in the present paragraph, we would like to elaborate further on the link between RS-DFT
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and wave function optimization in the presence of a Jastrow factor.
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\titou{T2: maybe we should mention that we only reoptimize the CI coefficients as it is of common practice to re-optimize more than this.}
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\toto{For simplicity in the comparison, the molecular orbitals and the Jastrow
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factor are kept fixed: only the CI coefficients are modified.}
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Let us assume a fixed Jastrow factor $J(\br_1, \ldots , \br_N)$,
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and a corresponding Slater-Jastrow wave function $\Phi = e^J \Psi$,
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@ -533,18 +536,19 @@ where $\Psi = \sum_I c_I D_I$ is a general linear combination of Slater determin
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The only remaining variational parameters in $\Phi$ are therefore the Slater part $\Psi$.
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Let us call $\Psi^J$ the linear combination of Slater determinant minimizing the variational energy
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\begin{equation}
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\Psi^J = \text{argmin}_{\Psi}\frac{ \mel{ \Psi }{ e^{J} H e^{J} }{ \Psi } }{\mel{ \Psi }{ e^{2J} }{ \Psi } }.
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\Psi^J = \argmin_{\Psi}\frac{ \mel{ \Psi }{ e^{J} \hat{H} e^{J} }{ \Psi } }{\mel{ \Psi }{ e^{2J} }{ \Psi } }.
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\end{equation}
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Such a wave function $\Psi^J$ satisfies the generalized hermitian eigenvalue equation
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Such a wave function $\Psi^J$ satisfies the generalized Hermitian eigenvalue equation
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\begin{equation}
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e^{J} H e^{J} \Psi^J = E e^{2J} \Psi^J,
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e^{J} \hat{H} \qty( e^{J} \Psi^J ) = E e^{2J} \Psi^J,
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\label{eq:ci-j}
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\end{equation}
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but also the non-hermitian transcorrelated eigenvalue problem \cite{many_things}
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but also the non-Hermitian \manu{transcorrelated eigenvalue problem \cite{many_things} MANU:CITATIONS}
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\begin{equation}
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\label{eq:transcor}
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e^{-J} H e^{J} \Psi^J = E \Psi^J,
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e^{-J} \hat{H} \qty( e^{J} \Psi^J) = E \Psi^J,
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\end{equation}
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which is much easier to handle despite its non-hermicity.
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which is much easier to handle despite its non-Hermiticity.
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Of course, the FN-DMC energy of $\Phi$ depends therefore only on the nodes of $\Psi^J$.
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In a finite basis set and with a quite accurate Jastrow factor, it is known that the nodes
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of $\Psi^J$ may be better than that of the FCI wave function, and therefore, we would like to compare $\Psi^J$ and $\Psi^\mu$.
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@ -555,8 +559,27 @@ function out of a large CIPSI calculation. Within this set of determinants,
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we solve the self-consistent equations of RS-DFT [see Eq.~\eqref{rs-dft-eigen-equation}]
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with different values of $\mu$. This gives the CI expansions $\Psi^\mu$.
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Then, within the same set of determinants we optimize the CI coefficients in the presence of
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a simple one- and two-body Jastrow factor. This gives the CI expansion $\Psi^J$.
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Then, we can easily compare $\Psi^\mu$ and $\Psi^J$ as they are developed
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a simple one- and two-body Jastrow factor \toto{$e^J$ of the form $\exp(J_{eN} + J_{ee})$ with
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\begin{eqnarray}
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J_\text{eN} & = & - \sum_{A=1}^{\Nat} \sum_{i=1}^{\Nelec} \left( \frac{\alpha_A\, r_{iA}}{1 + \alpha_A\, r_{iA}} \right)^2
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\label{eq:jast-eN} \\
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J_\text{ee} & = & \sum_{i=1}^{\Nelec} \sum_{j=1}^{i-1} \frac{a\, r_{ij}}{1 + b\, r_{ij}}. \label{eq:jast-ee}
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\end{eqnarray}
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$J_\text{eN}$ contains the electron-nucleus terms with a single parameter
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$\alpha_A$ per atom, and $J_\text{ee}$ contains the electron-electron terms
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where the indices $i$ and $j$ loop over all electrons. The parameters $a=1/2$
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and $b=0.89$ were fixed, and the parameters $\gamma_O=1.15$ and $\gamma_H=0.35$
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were obtained by energy minimization with a single determinant.
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The optimal CI expansion $\Psi^J$ is obtained by sampling the matrix elements
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of the Hamiltonian ($\mathbf{H}$) and the overlap ($\mathbf{S}$), in the
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basis of Jastrow-correlated determinants $e^J D_i$:
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\begin{eqnarray}
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H_{ij} & = & \left \langle \frac{e^J D_i}{\Psi^J}\, \frac{\hat{H}\, (e^J D_j)}{\Psi^J} \right \rangle \\
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S_{ij} & = & \left \langle \frac{e^J D_i}{\Psi^J}\, \frac{e^J D_j}{\Psi^J} \right \rangle
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\end{eqnarray}
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and solving Eq.~\eqref{eq:ci-j}.\cite{Nightingale_2001}}
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We can easily compare $\Psi^\mu$ and $\Psi^J$ as they are developed
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on the same Slater determinant basis.
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In Fig.~\ref{fig:overlap}, we plot the overlaps
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$\braket*{\Psi^J}{\Psi^\mu}$ obtained for water,
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@ -771,10 +794,7 @@ Another source of size-consistency error in QMC calculations originates
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from the Jastrow factor. Usually, the Jastrow factor contains
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one-electron, two-electron and one-nucleus-two-electron terms.
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The problematic part is the two-electron term, whose simplest form can
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be expressed as
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\begin{equation}
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J_\text{ee} = \sum_{i<j} \frac{a\, r_{ij}}{1 + b\, r_{ij}}.
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\end{equation}
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be expressed as in Eq.\eqref{eq:jast-ee}.
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The parameter
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$a$ is determined by cusp conditions, and $b$ is obtained by energy
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or variance minimization.\cite{Coldwell_1977,Umrigar_2005}
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