saving work 1st part of Xav part
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BSEdyn.tex
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BSEdyn.tex
@ -273,9 +273,9 @@ Unless otherwise stated, atomic units are used.
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\label{sec:theory}
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%%%%%%%%%%%%%%%%%%%%%%%%
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In this Section, following Strinati's seminal work, \cite{Strinati_1988} we first derive in some details the theoretical foundations leading to the dynamical Bethe-Salpeter equation.
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We present, in a second step, the perturbative implementation of the dynamical correction as compared to the standard static approximation. \cite{Rohlfing_2000,Ma_2009a,Ma_2009b,Baumeier_2012b}
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More details about this derivation are provided as {\SI}.
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In this Section, following Strinati's seminal work, \cite{Strinati_1988} we first derive in some details the theoretical foundations leading to the dynamical BSE.
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Additional details about this derivation are provided as {\SI}.
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We present, in a second step, the perturbative implementation of the dynamical correction as compared to the standard static approximation.
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%================================
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\subsection{General dynamical BSE theory}
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@ -286,15 +286,36 @@ The two-particle correlation function $L(1,2; 1',2')$ --- a central quantity in
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iL(1,2; 1',2') = \pdv{G(1,1')}{U(2',2)}
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\end{equation}
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where, \eg, $1 \equiv (\bx_1 t_1)$ is a space-spin plus time composite variable.
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The relation between $G$ and the charge density $\rho(1) = -i G(1,1^+)$ provides a direct connection with the density-density susceptibility $\chi(1,2) = L(1,2;1^+,2^+)$ at the core of TD-DFT.
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(The notation $1^+$ means that the time $t_1$ is taken at $t_1^{+} = t_1 + 0^+$ where $0^+$ is a small positive infinitesimal.)
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The two-body correlation function $L$ satisfies the self-consistent Bethe-Salpeter equation \cite{Strinati_1988}
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The relation between $G$ and the one-body charge density $\rho(1) = -i G(1,1^+)$ provides a direct connection with the density-density susceptibility $\chi(1,2) = L(1,2;1^+,2^+)$ at the core of TD-DFT.
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(The notation $1^+$ means that the time $t_1$ is taken at $t_1^{+} = t_1 + 0^+$, where $0^+$ is a small positive infinitesimal.)
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The two-body correlation function $L$ satisfies the self-consistent BSE \cite{Strinati_1988}
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\begin{multline} \label{eq:BSE}
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L(1,2; 1',2') = L_0(1,2;1',2')
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\\
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+ \int d3456 \, L_0(1,4;1',3) \Xi(3,5;4,6) L(6,2;5,2'),
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\end{multline}
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where
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\begin{subequations}
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\begin{align}
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\label{eq:L0}
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iL_0(1, 4; 1', 3) & = G(1, 3)G(4, 1'),
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\\
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\label{eq:L}
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iL(1,2; 1',2') & = - G_2(1,2;1',2') + G(1,1') G(2,2'),
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\end{align}
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\end{subequations}
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can be expressed as a function of the one- and two-body Green's functions
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\begin{subequations}
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\begin{align}
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\label{eq:G1}
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G(1,1') & = - i \mel{N}{T \hpsi(1) \hpsi^{\dagger}(1')}{N},
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\\
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\label{eq:G2}
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G_2(1,2;1',2') & = - \mel{N}{T \hpsi(1) \hpsi(2) \hpsi^{\dagger}(2') \hpsi^{\dagger}(1')}{N},
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\end{align}
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\end{subequations}
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and
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\begin{equation}
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\Xi(3,5;4,6) = i \fdv{[v_\text{H}(3) \delta(3,4) + \Sigma_\text{xc}(3,4)]}{G(6,5)}
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\end{equation}
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@ -303,20 +324,9 @@ is the BSE kernel that takes into account the self-consistent variation of the H
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v_\text{H}(1) = - i \int d2 \, v(1,2) G(2,2^+),
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\end{equation}
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[where $\delta$ is Dirac's delta function and $v$ is the bare Coulomb operator] and the exchange-correlation self-energy $ \Sigma_\text{xc}$ with respect to the variation of $G$.
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$L$ and $L_0$ can be expressed as a function of the one- and two-body ($G_2$) Green's functions as follows:
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\begin{gather}
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\label{eq:L0}
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iL_0(1, 4; 1', 3) = G(1, 3)G(4, 1'),
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\\
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\label{eq:L}
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iL(1,2; 1',2') = - G_2(1,2;1',2') + G(1,1') G(2,2'),
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\\
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\label{eq:G2}
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i^2 G_2(1,2;1',2') = \mel{N}{T \hpsi(1) \hpsi(2) \hpsi^{\dagger}(2') \hpsi^{\dagger}(1')}{N},
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\end{gather}
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where the field operators $\Hat{\psi}(\bx t)$ and $\Hat{\psi}^{\dagger}(\bx't')$ remove and add an electron (respectively) to the $N$-electron ground state $\ket{N}$ in space-spin-time positions ($\bx t$) and ($\bx't'$), while $T$ is the time-ordering operator.
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In Eqs.~\eqref{eq:G1} and \eqref{eq:G2}, the field operators $\Hat{\psi}(\bx t)$ and $\Hat{\psi}^{\dagger}(\bx't')$ remove and add an electron (respectively) to the $N$-electron ground state $\ket{N}$ in space-spin-time positions ($\bx t$) and ($\bx't'$), while $T$ is the time-ordering operator.
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The resolution of the dynamical BSE equation \cite{Strinati_1988} starts with the expansion of $G_2$ and $L$ over the complete orthonormalized set of $N$-electron excited states $\ket{N,s}$ (with $\ket{N,0} \equiv \ket{N}$).
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The resolution of the dynamical BSE equation \cite{Strinati_1988} starts with the expansion of $L_0$ and $L$ [see Eqs.~\eqref{eq:L0} and \eqref{eq:L}] over the complete orthonormalized set of $N$-electron excited states $\ket{N,s}$ (with $\ket{N,0} \equiv \ket{N}$).
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In the optical limit of instantaneous electron-hole creation and destruction, imposing $t_{2'} = t_2^+$ and $t_{1'} = t_1^+$, one gets
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\begin{equation}
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\begin{split}
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