modifs
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@ -249,7 +249,7 @@ which was first introduced by Faleev and co-workers \cite{Faleev_2004,vanSchilfg
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The corresponding matrix elements are
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\begin{equation}
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\label{eq:sym_qsGW}
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\Sigma_{pq}^{\titou{\text{qs}}}(\eta) = \frac{1}{2} \sum_{r\nu} \qty( \frac{\Delta_{pr\nu}}{\Delta_{pr\nu}^2 + \titou{\eta^2}} +\frac{\Delta_{qr\nu}}{\Delta_{qr\nu}^2 + \titou{\eta^2}} ) W_ {p,r\nu} \titou{W_{q,r\nu}}.
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\Sigma_{pq}^{\text{qs}}(\eta) = \frac{1}{2} \sum_{r\nu} \qty( \frac{\Delta_{pr\nu}}{\Delta_{pr\nu}^2 + \titou{\eta^2}} +\frac{\Delta_{qr\nu}}{\Delta_{qr\nu}^2 + \titou{\eta^2}} ) W_ {p,r\nu} W_{q,r\nu}.
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\end{equation}
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with $\Delta_{pr\nu} = \epsilon_p - \epsilon_r - \sgn(\epsilon_r-\epsilon_F)\Omega_\nu$ (where $\epsilon_F$ is the energy of the Fermi level).
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One of the main results of the present manuscript is the derivation, from first principles, of an alternative static Hermitian form for the $GW$ self-energy.
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@ -265,6 +265,7 @@ One can deal with them by introducing \textit{ad hoc} regularizers.
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Several other regularizers are possible \cite{Stuck_2013,Rostam_2017,Lee_2018a,Evangelista_2014b,Shee_2021} and in particular, it was shown in Ref.~\onlinecite{Monino_2022} that a regularizer inspired by the SRG had some advantages over the imaginary shift.
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Nonetheless, it would be more rigorous, and more instructive, to obtain this regularizer from first principles by applying the SRG formalism to many-body perturbation theory.
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This is the central aim of the present work.
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\PFL{SRG is energy-dependent.}
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%%%%%%%%%%%%%%%%%%%%%%
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\section{The similarity renormalization group}
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@ -332,30 +333,29 @@ Then, as performed in Sec.~\ref{sec:srggw}, one can collect order by order the t
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By applying the SRG to $GW$, our aim is to gradually remove the coupling between the quasiparticle and the satellites resulting in a renormalized quasiparticle equation.
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However, to do so, one must identify the coupling terms in Eq.~\eqref{eq:quasipart_eq}, which is not straightforward.
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A way around this problem is to transform Eq.~\eqref{eq:quasipart_eq} to its upfolded version which elegantly highlights the coupling terms in the process.
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The upfolded $GW$ quasiparticle equation is \cite{Bintrim_2021,Tolle_2022}
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A way around this problem is to transform Eq.~\eqref{eq:quasipart_eq} to its upfolded version which elegantly highlights the coupling terms: \cite{Bintrim_2021,Tolle_2022}
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\begin{equation}
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\label{eq:GWlin}
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\begin{pmatrix}
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\bF & \bW^{\text{2h1p}} & \bW^{\text{2p1h}} \\
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(\bW^{\text{2h1p}})^\dag & \bC^{\text{2h1p}} & \bO \\
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(\bW^{\text{2p1h}})^\dag & \bO & \bC^{\text{2p1h}} \\
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\end{pmatrix}
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\begin{pmatrix}
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\bZ^{\text{1h/1p}} \\
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\bZ^{\text{2h1p}} \\
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\bZ^{\text{2p1h}} \\
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\end{pmatrix}
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=
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\begin{pmatrix}
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\bZ^{\text{1h/1p}} \\
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\bZ^{\text{2h1p}} \\
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\bZ^{\text{2p1h}} \\
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\end{pmatrix}
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\boldsymbol{\epsilon},
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\end{pmatrix},
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% \begin{pmatrix}
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% \bZ^{\text{1h/1p}} \\
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% \bZ^{\text{2h1p}} \\
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% \bZ^{\text{2p1h}} \\
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% \end{pmatrix}
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% =
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% \begin{pmatrix}
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% \bZ^{\text{1h/1p}} \\
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% \bZ^{\text{2h1p}} \\
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% \bZ^{\text{2p1h}} \\
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% \end{pmatrix}
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% \boldsymbol{\epsilon},
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\end{equation}
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where $\boldsymbol{\epsilon}$ is a diagonal matrix collecting the quasiparticle and satellite energies, the 2h1p and 2p1h matrix elements are
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%where $\boldsymbol{\epsilon}$ is a diagonal matrix collecting the quasiparticle and satellite energies,
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where the 2h1p and 2p1h matrix elements are
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\begin{subequations}
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\begin{align}
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C^\text{2h1p}_{i\nu,j\mu} & = \left(\epsilon_i - \Omega_\nu\right)\delta_{ij}\delta_{\nu\mu},
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@ -380,7 +380,7 @@ The usual $GW$ non-linear equation can be obtained by applying L\"owdin partitio
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\end{equation}
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which can be further developed to recover exactly Eq.~\eqref{eq:GW_selfenergy}.
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Equations \eqref{eq:GWlin} and \eqref{eq:quasipart_eq} \titou{yield exactly the same energies} but one is linear and the other is not.
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Equations \eqref{eq:GWlin} and \eqref{eq:quasipart_eq} yield exactly the quasiparticle and satellite energies but one is linear and the other is not.
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The price to pay for this linearity is that the size of the matrix in the former is $\order{K^3}$ while it is only $\order{K}$ in the latter.
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We refer to Ref.~\onlinecite{Bintrim_2021} for a detailed discussion of the up/downfolding processes of the $GW$ equations (see also Refs.~\onlinecite{Tolle_2022,Scott_2023}).
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@ -524,7 +524,7 @@ which can be solved by simple integration along with the initial condition $\bF^
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At $s=0$, the second-order correction vanishes while, for $s\to\infty$, it tends towards the following static limit
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\begin{equation}
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\label{eq:static_F2}
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F_{pq}^{(2)}(\infty) = \sum_{r\nu} \frac{\Delta_{pr\nu}+ \Delta_{qr\nu}}{\Delta_{pr\nu}^2 + \Delta_{qr\nu}^2} W_{p,r\nu} \titou{W_{q,r\nu}}.
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F_{pq}^{(2)}(\infty) = \sum_{r\nu} \frac{\Delta_{pr\nu}+ \Delta_{qr\nu}}{\Delta_{pr\nu}^2 + \Delta_{qr\nu}^2} W_{p,r\nu} W_{q,r\nu}.
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\end{equation}
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Note that, in the limit $s\to\infty$, the dynamic part of the self-energy [see Eq.~\eqref{eq:srg_sigma}] tends to zero.
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\titou{Therefore, the SRG flow continuously transforms the dynamic part $\widetilde{\bSig}(\omega; s)$ into a static correction $\widetilde{\bF}(s)$.}
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@ -607,7 +607,7 @@ Then the accuracy of the IP yielded by the traditional and SRG schemes will be s
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%%% %%% %%% %%%
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This section starts by considering a prototypical molecular system, \ie the water molecule, in the aug-cc-pVTZ cartesian basis set.
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Figure~\ref{fig:fig1} shows the error of various methods for the principal IP with respect to (w.r.t.) the CCSD(T) reference value.
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Figure~\ref{fig:fig1} shows the error of various methods for the principal IP with respect to the CCSD(T) reference value.
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The HF IP (dashed black line) is overestimated, this is a consequence of the missing correlation, a result which is now well understood. \cite{Lewis_2019} \ANT{I should maybe search for another ref as well.}
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\PFL{Check Szabo\&Ostlund, section on Koopman's theorem.}
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The usual qs$GW$ scheme (dashed blue line) brings a quantitative improvement as the IP is now within \SI{0.3}{\electronvolt} of the reference.
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