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- W2015661663 abstract "We study the wide latitude available in choosing the reference space and the zeroth order Hamiltonian H0 for complete reference space multireference perturbation theory. This effective Hamiltonian Heff method employs a general one-body form of H0 which is varied by using different molecular orbitals and orbital energies. An energy gap is imposed between the zeroth order reference and secondary space states by forcing the valence orbitals to be degenerate. The forced valence orbital degeneracy removes the occurrence of detrimentally small perturbation energy denominators. Extensive computations are provided for the nitrogen molecule, where calculated ground state spectroscopic constants are compared with full configuration interaction computations and calculated vertical excitation energies are compared with multireference coupled cluster computations. It is demonstrated that the forced reference space degeneracy can lead to certain perturbation denominators becoming too small for practical convergence. This characteristic is illustrated by a simple two-orbital model which stresses the need for important zeroth order excitation energies (equivalent to the factors appearing in the perturbation energy denominators) to exceed those in an Epstein–Nesbet perturbation partitioning. This simple model illustrates the general behavior found in all the more extensive Heff computations. In many cases where zeroth order excitation energies are too small for satisfactory third order results, improvements are obtained by using an H0 which redefines the orbital energies in order to increase problematic zeroth order excitation energies. The necessary orbital energy shifts are identified by examining the first order wave functions from larger reference spaces and the zeroth order energies. Frequently, fractional occupancy Fock-type operators are employed to provide the requisite orbital energy shifts. Some of the reference spaces investigated deviate extremely from quasidegeneracy and, thus, appear to be beyond the range of applicability of the forced degeneracy Heff method. Novel techniques are employed for properly treating some of these cases, including the use of orbitals which optimize the quasidegeneracy of the reference space and minimize energy denominator problems. By considering reference spaces of varying sizes, we describe the tradeoff between employing large reference spaces, which provide excellent first order descriptions, and the difficulties imposed by the fact that larger reference spaces severely violate the quasidegeneracy constraints of the Heff method. The same tradeoff exists when the optimal first order CASSCF orbitals are compared with orbitals generated by a VN−1 potential. The VN−1 potential orbitals, which produce relatively quasidegenerate reference spaces, are equivalent to the sequential SCF orbitals used in previous Heff computations, but are more simply obtained by a unitary transformation. The forced degenerate valence orbital energy εv̄ is computed from an averaging scheme for the valence orbital energies. The ground state N2 computations contrast two averaging schemes—populational and democratic. Democratic averaging weighs all valence orbitals equally, while populational averaging weighs valence orbitals in proportion to their ground state populations. Populational averaging is determined to be useful only in situations where core–core and core–valence correlation are unimportant. A Fock-type operator used by Roos and co-workers is employed to uniquely define CASSCF orbitals within their invariant subspaces. This operator is found to be more compatible with populational than democratic averaging, especially when the reference space contains high lying orbitals." @default.
- W2015661663 created "2016-06-24" @default.
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- W2015661663 date "1995-01-15" @default.
- W2015661663 modified "2023-09-23" @default.
- W2015661663 title "Application of complete space multireference many-body perturbation theory to N2: Dependence on reference space and <i>H</i>0" @default.
- W2015661663 cites W1562867712 @default.
- W2015661663 cites W1948575633 @default.
- W2015661663 cites W1966420236 @default.
- W2015661663 cites W1966865869 @default.
- W2015661663 cites W1968053160 @default.
- W2015661663 cites W1968623807 @default.
- W2015661663 cites W1971275758 @default.
- W2015661663 cites W1977216274 @default.
- W2015661663 cites W1977783398 @default.
- W2015661663 cites W1981025138 @default.
- W2015661663 cites W1981790977 @default.
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- W2015661663 cites W1987904096 @default.
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- W2015661663 cites W1995729567 @default.
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- W2015661663 cites W1996745384 @default.
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- W2015661663 cites W2012778107 @default.
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- W2015661663 cites W2018632465 @default.
- W2015661663 cites W2030708072 @default.
- W2015661663 cites W2033450749 @default.
- W2015661663 cites W2033618515 @default.
- W2015661663 cites W2045207371 @default.
- W2015661663 cites W2046157418 @default.
- W2015661663 cites W2046343871 @default.
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- W2015661663 cites W2063860218 @default.
- W2015661663 cites W2067710218 @default.
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- W2015661663 cites W2068855384 @default.
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- W2015661663 doi "https://doi.org/10.1063/1.468919" @default.
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