OK up to Sec IIIc
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@ -299,7 +299,7 @@ unless otherwise stated, atomic units will be used throughout.
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\label{fig:FCI}}
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\end{figure*}
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To illustrate the concepts discussed throughout this article, we consider the symmetric Hubbard dimer at half filling, \ie\ with two opposite-spin fermions.
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To illustrate the concepts discussed throughout this article, we consider the symmetric Hubbard dimer at half filling, \ie, with two opposite-spin fermions.
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Analytically solvable models are essential in theoretical chemistry and physics as their mathematical simplicity compared to realistic systems (e.g., atoms and molecules) allows new concepts and methods to be
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easily tested while retaining the key physical phenomena.
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@ -730,7 +730,7 @@ unrestricted reference orbitals.
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Although practically convenient for electronic structure calculations, the MP partitioning is not
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the only possibility and alternative partitionings have been considered including:
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i) the Epstein-Nesbet (EN) partitioning which consists in taking the diagonal elements of $\hH$ as the zeroth-order Hamiltonian. \cite{Nesbet_1955,Epstein_1926}
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i) the Epstein-Nesbet (EN) partitioning which consists in taking the diagonal elements of $\hH$ as the zeroth-order Hamiltonian, \cite{Nesbet_1955,Epstein_1926}
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ii) the weak correlation partitioning in which the one-electron part is consider as the unperturbed Hamiltonian $\hH^{(0)}$ and the two-electron part is the perturbation operator $\hV$, and
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iii) the strong coupling partitioning where the two operators are inverted compared to the weak correlation partitioning. \cite{Seidl_2018}
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While an in-depth comparison of these different approaches can offer insight into
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@ -770,7 +770,7 @@ The divergence of RMP expansions for stretched bonds can be easily understood fr
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Firstly, the exact wave function becomes increasingly multi-configurational as the bond is stretched, and the
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RHF wave function no longer provides a qualitatively correct reference for the perturbation expansion.
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Secondly, the energy gap between the bonding and antibonding orbitals associated with the stretch becomes
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increasingly small at larger bond lengths, leading to a divergence, for example, in the second-order MP correction \eqref{eq:EMP2}.
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increasingly small at larger bond lengths, leading to a divergence, for example, in the \trash{second-order MP} \titou{MP2} correction \eqref{eq:EMP2}.
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In contrast, the origin of slow UMP convergence is less obvious as the reference UHF energy remains
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qualitatively correct at large bond lengths and the orbital degeneracy is avoided.
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Furthermore, this slow convergence can also be observed in molecules with a UHF ground state at the equilibrium
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