push for Enzo

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Pierre-Francois Loos 2022-04-25 14:10:41 +02:00
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\maketitle
%%%%%%%%%%%%%%%%%%%%%%%%
\section{Energy differences}
%%%%%%%%%%%%%%%%%%%%%%%%
\subsection{$\eta$ shift}
\begin{figure}
\includegraphics[width=0.33\linewidth]{eta_0_1}
\includegraphics[width=0.33\linewidth]{eta_1}
\includegraphics[width=0.33\linewidth]{eta_10}
\caption{Difference between non-regularized and regularized quasiparticle energies $\eps{p}{\GW}-\reps{p}{\GW}$ computed with $\eta = 0.1$ (left), $\eta = 1$ (center), and $\eta = 10$ (right) as functions of the internuclear distance $\RHH$ (in \si{\angstrom}) of \ce{H2} at the {\GOWO}@HF/6-31G level. }
\end{figure}
\begin{figure}
\includegraphics[width=0.6\linewidth]{eta_0_1}
\caption{Difference between non-regularized and regularized quasiparticle energies $\eps{p}{\GW}-\reps{p}{\GW}$ computed with $\eta = 0.1$ as functions of the internuclear distance $\RHH$ (in \si{\angstrom}) of \ce{H2} at the {\GOWO}@HF/6-31G level. }
\includegraphics[width=0.33\linewidth]{kappa_0_1}
\includegraphics[width=0.33\linewidth]{kappa_1}
\includegraphics[width=0.33\linewidth]{kappa_10}
\caption{Difference between non-regularized and regularized quasiparticle energies $\eps{p}{\GW}-\reps{p}{\GW}$ computed with computed with $\kappa = 0.1$ (left), $\kappa = 1$ (center), and $\kappa = 10$ (right) as functions of the internuclear distance $\RHH$ (in \si{\angstrom}) of \ce{H2} at the {\GOWO}@HF/6-31G level. }
\end{figure}
\begin{figure}
\includegraphics[width=0.6\linewidth]{eta_1}
\caption{Difference between non-regularized and regularized quasiparticle energies $\eps{p}{\GW}-\reps{p}{\GW}$ computed with $\eta = 1$ as functions of the internuclear distance $\RHH$ (in \si{\angstrom}) of \ce{H2} at the {\GOWO}@HF/6-31G level. }
\includegraphics[width=0.45\linewidth]{f2_eta_1}
\hspace{0.05\textwidth}
% \includegraphics[width=0.45\linewidth]{f2_eta_1}
\caption{Ground-state potential energy surface of \ce{F2} around its equilibrium geometry obtained at various levels of theory with the cc-pVDZ basis set for $\eta = 1$.}
\end{figure}
\begin{figure}
\includegraphics[width=0.6\linewidth]{eta_10}
\caption{Difference between non-regularized and regularized quasiparticle energies $\eps{p}{\GW}-\reps{p}{\GW}$ computed with $\eta = 10$ as functions of the internuclear distance $\RHH$ (in \si{\angstrom}) of \ce{H2} at the {\GOWO}@HF/6-31G level. }
\includegraphics[width=0.45\linewidth]{f2_kappa_1}
\hspace{0.05\textwidth}
\includegraphics[width=0.45\linewidth]{f2_kappa_10}
\caption{Ground-state potential energy surface of \ce{F2} around its equilibrium geometry obtained at various levels of theory with the cc-pVDZ basis set for $\kappa = 1$ (left) and $\kappa = 10$ (right).
For $\kappa = 10$, the black and gray curves are superposed.}
\end{figure}
\subsection{$\kappa$ shift}
\begin{figure}
\includegraphics[width=0.6\linewidth]{kappa_0_1}
\caption{Difference between non-regularized and regularized quasiparticle energies $\eps{p}{\GW}-\reps{p}{\GW}$ computed with $\kappa = 0.1$ as functions of the internuclear distance $\RHH$ (in \si{\angstrom}) of \ce{H2} at the {\GOWO}@HF/6-31G level. }
\end{figure}
\begin{figure}
\includegraphics[width=0.6\linewidth]{kappa_10}
\caption{Difference between non-regularized and regularized quasiparticle energies $\eps{p}{\GW}-\reps{p}{\GW}$ computed with $\kappa = 10$ as functions of the internuclear distance $\RHH$ (in \si{\angstrom}) of \ce{H2} at the {\GOWO}@HF/6-31G level. }
\end{figure}
%%%%%%%%%%%%%%%%%%%%%%%%
\section{\ce{F2} ground state}
%%%%%%%%%%%%%%%%%%%%%%%%
\begin{figure}
\includegraphics[width=0.6\linewidth]{f2_eta_1}
\caption{Ground-state potential energy surface of \ce{F2} around its equilibrium geometry obtained at various levels of theory with the cc-pVDZ basis set.}
\end{figure}
\begin{figure}
\includegraphics[width=0.6\linewidth]{f2_kappa_1}
\caption{Ground-state potential energy surface of \ce{F2} around its equilibrium geometry obtained at various levels of theory with the cc-pVDZ basis set.}
\end{figure}
\begin{figure}
\includegraphics[width=0.6\linewidth]{f2_kappa_10}
\caption{Ground-state potential energy surface of \ce{F2} around its equilibrium geometry obtained at various levels of theory with the cc-pVDZ basis set.}
\end{figure}
%%%%%%%%%%%%%%%%%%%%%%%%
\bibliography{ufGW}

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@ -373,7 +373,7 @@ Therefore, one can conclude that this downfall of $GW$ is a key signature of str
\includegraphics[width=\linewidth]{fig4}
\caption{
\label{fig:H2reg}
Difference between regularized and non-regularized quasiparticle energies $\reps{p}{\GW} - \eps{p}{\GW}$ computed with $\eta = 1$ as functions of the internuclear distance $\RHH$ (in \si{\angstrom}) of \ce{H2} at the {\GOWO}@HF/6-31G level.
Difference between regularized and non-regularized quasiparticle energies $\reps{p}{\GW} - \eps{p}{\GW}$ computed with $\alert{\kappa} = 1$ as functions of the internuclear distance $\RHH$ (in \si{\angstrom}) of \ce{H2} at the {\GOWO}@HF/6-31G level.
}
\end{figure}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
@ -430,7 +430,7 @@ Our investigations have shown that the following energy-dependent regularizer
f_\kappa(\Delta) = \frac{1-e^{-2\Delta^2/\kappa^2}}{\Delta}
\end{equation}
derived from the (second-order) perturbative analysis of the similarity renormalization group (SRG) equations \cite{Wegner_1994,Glazek_1994,White_2002} by Evangelista \cite{Evangelista_2014} is particularly convenient and effective for our purposes.
Increasing $\kappa$ gradually integrates out states with denominators $\Delta$ larger than $\kappa$ while the states with $\Delta \ll \kappa$ are not decoupled from the reference space, hence avoiding intruder state problems. \cite{Li_2019a}
Increasing $\alert{\kappa}$ gradually integrates out states with denominators $\Delta$ larger than $\alert{\kappa}$ while the states with $\Delta \ll \alert{\kappa}$ are not decoupled from the reference space, hence avoiding intruder state problems. \cite{Li_2019a}
Figure \ref{fig:H2reg_zoom} compares the non-regularized and regularized quasiparticle energies in the two regions of interest for various $\eta$ values.