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@ -583,7 +583,7 @@ For a fixed value of the energy cutoff $\Lambda$, if $\abs*{\Delta_{pr}^{\nu}} \
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%%% FIG 2 %%%
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\begin{figure*}
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\includegraphics[width=0.8\linewidth]{fig2.pdf}
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\includegraphics[width=0.8\linewidth]{fig2}
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\caption{
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Functional form of the qs$GW$ self-energy (left) for $\eta = 1$ and the SRG-qs$GW$ self-energy (right) for $s = 1/(2\eta^2) = 1/2$.}
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\label{fig:plot}
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@ -671,7 +671,7 @@ The numerical data associated with this study are reported in the {\SupInf}.
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%%% FIG 3 %%%
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\begin{figure}
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\includegraphics[width=\linewidth]{fig3.pdf}
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\includegraphics[width=\linewidth]{fig3}
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\caption{
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Error [with respect to $\Delta$CCSD(T)] in the principal IP of water in the aug-cc-pVTZ basis set as a function of the flow parameter $s$ for SRG-qs$GW$.
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The HF and qs$GW$ values are reported as dashed lines.
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@ -681,7 +681,7 @@ The numerical data associated with this study are reported in the {\SupInf}.
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%%% FIG 4 %%%
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\begin{figure*}
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\includegraphics[width=\linewidth]{fig4.pdf}
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\includegraphics[width=\linewidth]{fig4}
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\caption{
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Error [with respect to $\Delta$CCSD(T)] in the principal IP of \ce{Li2}, \ce{LiH} and \ce{BeO} in the aug-cc-pVTZ basis set as a function of the flow parameter $s$ for the SRG-qs$GW$ method.
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The HF and qs$GW$ values are reported as dashed lines.
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@ -759,7 +759,7 @@ The SRG-qs$GW$ EA (absolute) error is monotonically decreasing from the HF value
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%%% FIG 5 %%%
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\begin{figure*}
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\includegraphics[width=\linewidth]{fig5.pdf}
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\includegraphics[width=\linewidth]{fig5}
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\caption{
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Histogram of the errors [with respect to $\Delta$CCSD(T)] for the principal IP of the $GW$50 test set calculated using HF, $G_0W_0$@HF, qs$GW$, and SRG-qs$GW$.
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All calculations are performed with the aug-cc-pVTZ basis.
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@ -775,14 +775,15 @@ However, there are still outliers with large errors.
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Self-consistency can mitigate the error of the outliers as the MAE at the qs$GW$ level is now \SI{0.57}{\eV} and the standard deviation of the error (SDE) is decreased from \SI{0.31}{\eV} for $G_0W_0$ to \SI{0.18}{\eV}.
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In addition, the MSE and MAE (\SI{0.23}{\eV} and \SI{0.25}{\eV}, respectively) are also slightly improved with respect to $G_0W_0$@HF.
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Now turning to the new method of this manuscript, \ie the SRG-qs$GW$ alternative self-consistent scheme.
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Let us now turn to the new method of this manuscript, the SRG-qs$GW$ self-consistent scheme.
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Table \ref{tab:tab1} shows the SRG-qs$GW$ values for $s=\num{e3}$.
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The statistical descriptors corresponding to this alternative static self-energy are all improved with respect to qs$GW$.
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In particular, the MSE and MAE are decreased by \SI{0.06}{\eV}
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In particular, the MSE and MAE are decreased by \SI{0.06}{\eV}.
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Of course, these are slight improvements but this is done with no additional computational cost and can be easily implemented by changing the form of the static approximation.
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The evolution of the statistical descriptors with respect to the various methods considered in Table \ref{tab:tab1} is graphically illustrated by Fig.~\ref{fig:fig4}.
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The decrease of the MSE and SDE correspond to a shift of the maximum toward zero and a shrink of the distribution width, respectively.
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The decrease of the MSE and SDE correspond to a shift of the maximum of the distribution toward zero and a contraction of the distribution width, respectively.
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%%% TABLE I %%%
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\begin{table*}
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\caption{Principal IP and EA (in eV) of the $GW$50 test set calculated using $\Delta$CCSD(T) (reference), HF, $G_0W_0$@HF, qs$GW$, and SRG-qs$GW$.
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The statistical descriptors associated with the errors with respect to the reference values are also reported.
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@ -858,15 +859,15 @@ The decrease of the MSE and SDE correspond to a shift of the maximum toward zero
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%%% FIG 6 %%%
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\begin{figure}
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\centering
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\includegraphics[width=\linewidth]{fig6.pdf}
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\includegraphics[width=\linewidth]{fig6}
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\caption{
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SRG-qs$GW$ and qs$GW$ MAEs for the principal IPs of the $GW$50 test set. The bottom and top axes are equivalent and related by $s=1/(2\eta^2)$. A different marker has been used for qs$GW$ at $\eta=0.05$ because the MAE includes only 48 molecules.
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\label{fig:fig6}}
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\end{figure}
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%%% %%% %%% %%%
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In addition to this improvement of accuracy, the SRG-qs$GW$ scheme has been found to be much easier to converge than its qs$GW$ counterpart.
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Indeed, up to $s=\num{e3}$ SRG-qs$GW$ self-consistency can be attained without any problems for the 50 compounds.
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In addition to this improvement in accuracy, the SRG-qs$GW$ scheme has been found to be much easier to converge than its qs$GW$ counterpart.
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Indeed, up to $s=\num{e3}$ SRG-qs$GW$, it is straightforward to reach self-consistency for the 50 compounds.
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For $s=\num{5e3}$, convergence could not be attained for 11 molecules out of 50.
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This means that some intruder states were included in the static correction for this value of $s$.
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However, this is not a problem as the MAE of the test set is already well converged at $s=\num{e3}$.
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@ -875,19 +876,19 @@ The convergence plateau of the MAE is reached around $s=50$ while the convergenc
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Therefore, for future studies using the SRG-qs$GW$ method, a default value of the flow parameter equal to $\num{5e2}$ or $\num{e3}$ is recommended.
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On the other hand, the qs$GW$ convergence behavior is more erratic.
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At $\eta=\num{e-2}$ ($s=\num{5e3}$), convergence could not be achieved for 13 molecules while 2 molecules were already problematic at $\eta=\num{5e-2}$ ($s=200$).
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But these convergence problems are much more dramatic than for SRG-qs$GW$ because the MAE definitely do not reach a convergence plateau before these problem arise (see the orange curve in Fig.~\ref{fig:fig6}).
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For example, out of the 37 molecules that could be converged for $\eta=\num{e-2}$ the variation of the IP with respect to $\eta=\num{5e-2}$ can go up to \SI{0.1}{\eV}.
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At $\eta=\num{e-2}$ ($s=\num{5e3}$), convergence could not be reached for 13 molecules while 2 systems were already problematic at $\eta=\num{5e-2}$ ($s=200$).
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These convergence problems are much more dramatic than for SRG-qs$GW$ because the MAE has not reached a convergence plateau before these problems arise (see the orange curve in Fig.~\ref{fig:fig6}).
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For example, out of the 37 molecules that could be converged for $\eta=\num{e-2}$, the variation of the IP with respect to $\eta=\num{5e-2}$ can go up to \SI{0.1}{\eV}.
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This difference of behavior is due to the energy (in)dependence of the regularizers.
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This difference in behavior is due to the energy (in)dependence of the regularizers.
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Indeed, the SRG regularizer first includes the terms that are important for the energy and finally adds the intruder states.
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On the other hand, the imaginary shift regularizer acts equivalently on intruder states and terms that contribute to the energy.
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%%% FIG 7 %%%
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\begin{figure*}
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\includegraphics[width=\linewidth]{fig7.pdf}
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\includegraphics[width=\linewidth]{fig7}
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\caption{
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Histogram of the errors [with respect to $\Delta$CCSD(T)] for the principal EA of the $GW$50 test set calculated using HF, $G_0W_0$@HF, qs$GW$ and SRG-qs$GW$.
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Histogram of the errors [with respect to $\Delta$CCSD(T)] for the principal EA of the $GW$50 test set calculated using HF, $G_0W_0$@HF, qs$GW$, and SRG-qs$GW$.
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All calculations are performed with the aug-cc-pVTZ basis.
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\label{fig:fig7}}
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\end{figure*}
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@ -895,9 +896,9 @@ On the other hand, the imaginary shift regularizer acts equivalently on intruder
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Finally, we compare the performance of HF, $G_0W_0$@HF, qs$GW$ and SRG-qs$GW$ again but for the principal EA energies.
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The raw results are given in Table \ref{tab:tab1} while the corresponding histograms of the error distribution are plotted in Fig.~\ref{fig:fig7}.
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The HF EAs are underestimated in average with a MAE of \SI{0.31}{\eV} and some large outliers, for \SI{-2.03}{\eV} for \ce{F2} and \SI{1.04}{\eV} for \ce{CH2O} for example.
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The HF EAs are, on average, underestimated with a MAE of \SI{0.31}{\eV} and some clear outliers, for \SI{-2.03}{\eV} for \ce{F2} and \SI{1.04}{\eV} for \ce{CH2O} for example.
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$G_0W_0$@HF mitigates the average error (MAE equal to \SI{0.16}{\eV}) but the minimum and maximum error values are not yet satisfactory.
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The performance of the two qs$GW$ schemes are quite similar for EA, \ie a MAE of \SI{\sim 0.1}{\electronvolt}.
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The performance of the two qs$GW$ schemes are quite similar for EA, \ie a MAE of \SI{\sim 0.1}{\eV}.
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The two partially self-consistent methods reduce as well the minimum value but interestingly, the three flavors of many-body perturbation theory considered here can not decrease the maximum error with respect to their HF starting point.
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Note that a positive EA means that the anion state is bound and therefore the methods considered here are well-suited to describe these EAs.
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