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@ -507,6 +507,17 @@ $4.$ & $0 .3189$ & $0 .8867$ & $0 .3328$ & $0 .2172$ & $0 .9453$ & $0 \
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\end{figure}
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\end{figure}
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%%% %%% %%%
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%%% %%% %%%
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%%% FIG 3 %%%
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\begin{figure}
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\includegraphics[width=0.5\linewidth]{H2_BSE_RHF}
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\caption{
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Excitation energies with respect to the $\text{X}\,{}^1 \Sigma_g^+$ ground state of the $\text{B}\,{}^1\Sigma_u^+$ (red), $\text{E}\,{}^1\Sigma_g^+$ (black), and $\text{F}\,{}^1\Sigma_g^+$ (blue) states of \ce{H2} obtained with the cc-pVQZ basis at the (SF-)BSE level of theory.
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The reference EOM-CCSD excitation energies are represented as solid lines, while the results obtained with and without spin-flip are represented as dashed and dotted lines, respectively.
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In this case, the spin-conserved calculations have been performed with a restricted reference while the spin-flip calculations have been performed with an unrestricted reference.
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\label{fig:H2_RHF}}
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\end{figure}
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%%% %%% %%%
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%%%%%%%%%%%%%%%%%%%%%%%%
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%%%%%%%%%%%%%%%%%%%%%%%%
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\bibliography{sfBSE}
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\bibliography{sfBSE}
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%%%%%%%%%%%%%%%%%%%%%%%%
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%%%%%%%%%%%%%%%%%%%%%%%%
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@ -890,7 +890,7 @@ A similar graph comparing (SF-)dBSE and EOM-CCSD excitation energies can be foun
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This unfortunate feature is due to the appearance of the symmetry-broken UHF solution and the lack of self-consistent in {\GOWO}.
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This unfortunate feature is due to the appearance of the symmetry-broken UHF solution and the lack of self-consistent in {\GOWO}.
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Indeed, $R = 1.2~\AA$ corresponds to the location of the well-known Coulson-Fischer point. \cite{Coulson_1949}
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Indeed, $R = 1.2~\AA$ corresponds to the location of the well-known Coulson-Fischer point. \cite{Coulson_1949}
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Note that, as mentioned earlier, all the calculations are performed with a UHF reference even the ones based on a closed-shell singlet reference.
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Note that, as mentioned earlier, all the calculations are performed with a UHF reference even the ones based on a closed-shell singlet reference.
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If one relies solely on the restricted HF solution, this kink disappears and one obtains smooth potential energy curves.}
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If one relies solely on the restricted HF solution, this kink disappears and one obtains smooth potential energy curves (see {\SI}).}
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The right side of Fig.~\ref{fig:H2} shows the amount of spin contamination as a function of the bond length for SF-CIS (top), SF-TD-BH\&HLYP (center), and SF-BSE (bottom).
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The right side of Fig.~\ref{fig:H2} shows the amount of spin contamination as a function of the bond length for SF-CIS (top), SF-TD-BH\&HLYP (center), and SF-BSE (bottom).
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Overall, one can see that $\expval{\hS^2}$ behaves similarly for SF-CIS and SF-BSE with a small spin contamination of the $\text{B}\,{}^1\Sigma_u^+$ at short bond length. In contrast, the $\text{B}$ state is much more spin contaminated at the SF-TD-BH\&HLYP level.
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Overall, one can see that $\expval{\hS^2}$ behaves similarly for SF-CIS and SF-BSE with a small spin contamination of the $\text{B}\,{}^1\Sigma_u^+$ at short bond length. In contrast, the $\text{B}$ state is much more spin contaminated at the SF-TD-BH\&HLYP level.
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@ -66,7 +66,8 @@ I recommend this manuscript for publication after the minor points addressed:}
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\alert{The kink in the SF-BSE@$G_0W_0$ and SF-dBSE/$G_0W_0$ curves for \ce{H2} are due to the appearance of the symmetry-broken UHF solution.
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\alert{The kink in the SF-BSE@$G_0W_0$ and SF-dBSE/$G_0W_0$ curves for \ce{H2} are due to the appearance of the symmetry-broken UHF solution.
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Indeed, $R = 1.2~\AA$ corresponds to the location of the well-known Coulson-Fischer point.
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Indeed, $R = 1.2~\AA$ corresponds to the location of the well-known Coulson-Fischer point.
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Note that, as mentioned in our manuscript, all the calculations are performed with a UHF reference (even the ones based on a closed-shell singlet reference).
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Note that, as mentioned in our manuscript, all the calculations are performed with a UHF reference (even the ones based on a closed-shell singlet reference).
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Of course, if one relies solely on the RHF solution, this kink disappears (see figure below). it would be, nonetheless, inconsistent with the rest of the paper.
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Of course, if one relies solely on the RHF solution, this kink disappears as illustrated by the figure below which has been also included in the Supporting Information.
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However, it would be inconsistent with the rest of the paper.
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The appearance of this kink is now discussed in the revised version of the manuscript.
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The appearance of this kink is now discussed in the revised version of the manuscript.
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At the ev$GW$ level, this kink would certainly still exist as one does not self-consistently optimised the orbitals in this case.
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At the ev$GW$ level, this kink would certainly still exist as one does not self-consistently optimised the orbitals in this case.
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However, it would likely disappear at the qs$GW$ level but it remains to be confirmed (work is currently being done in this direction).
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However, it would likely disappear at the qs$GW$ level but it remains to be confirmed (work is currently being done in this direction).
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