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@ -404,7 +404,7 @@ Taking the static limit, \ie, $W(\omega=0)$, for the screened Coulomb potential,
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\begin{pmatrix}
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\begin{pmatrix}
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R & C
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R & C
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\\
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\\
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-C^* & R^{*}
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-C^* & -R^{*}
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\end{pmatrix}
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\end{pmatrix}
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\begin{pmatrix}
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\begin{pmatrix}
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X^m
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X^m
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@ -427,7 +427,7 @@ with electron-hole ($eh$) eigenstates written as
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\end{equation}
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\end{equation}
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where $m$ indexes the electronic excitations.
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where $m$ indexes the electronic excitations.
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The $\lbrace \phi_{i/a} \rbrace$ are, in the case of $G_0W_0$ and ev$GW$, the input (KS) eigenstates used to build the $GW$ self-energy.
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The $\lbrace \phi_{i/a} \rbrace$ are, in the case of $G_0W_0$ and ev$GW$, the input (KS) eigenstates used to build the $GW$ self-energy.
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The resonant and anti-resonant parts of the BSE Hamiltonian read
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The resonant and coupling parts of the BSE Hamiltonian read
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\begin{gather}
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\begin{gather}
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R_{ai,bj} = \qty( \varepsilon_a^{\GW} - \varepsilon_i^{\GW} ) \delta_{ij} \delta_{ab} + \kappa (ia|jb) - W_{ij,ab},
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R_{ai,bj} = \qty( \varepsilon_a^{\GW} - \varepsilon_i^{\GW} ) \delta_{ij} \delta_{ab} + \kappa (ia|jb) - W_{ij,ab},
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\\
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\\
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@ -446,7 +446,7 @@ $(ia|jb)$ bare Coulomb term defined as
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\phi_i(\br) \phi_a(\br) v(\br-\br')
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\phi_i(\br) \phi_a(\br) v(\br-\br')
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\phi_j(\br') \phi_b(\br'),
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\phi_j(\br') \phi_b(\br'),
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\end{equation}
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\end{equation}
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Neglecting the anti-resonant term $C$ in Eq.~\eqref{eq:BSE-eigen}, which is usually much smaller than its resonant counterpart $R$, leads to the well-known Tamm-Dancoff approximation.
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Neglecting the coupling term $C$ between the resonant term $R$ and anti-resonant term $-R^*$ in Eq.~\eqref{eq:BSE-eigen}, leads to the well-known Tamm-Dancoff approximation.
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As compared to TD-DFT,
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As compared to TD-DFT,
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\begin{itemize}
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\begin{itemize}
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\item the $GW$ quasiparticle energies $\lbrace \varepsilon_{i/a}^{\GW} \rbrace$ replace the KS eigenvalues
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\item the $GW$ quasiparticle energies $\lbrace \varepsilon_{i/a}^{\GW} \rbrace$ replace the KS eigenvalues
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