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The ROHF approach is of course only approximately valid for studies of the core-hole states as they are not the lowest states of a given symmetry. However, the great energy gap and the sharp distinction in electron density distribution between the core- and the lower-lying valence-excited states prevent the self-consistent field (SCF) procedure from a variational collapse.
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0006761854
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with contributions from R. D. Amos, R. J. Buenker, M. Dupuis et al. The package is derived from the original GAMESS code due to M. Dupuis, D. Spangler, and J. Wendoloski, Program No. QG01 (GAMESS)
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Program written by M. F. Guest, J. H. van Lenthe, J. Kendrick et al., with contributions from R. D. Amos, R. J. Buenker, M. Dupuis et al. The package is derived from the original GAMESS code due to M. Dupuis, D. Spangler, and J. Wendoloski, NRCC Software Catalog, Vol. 1, Program No. QG01 (GAMESS), 1980.
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The coupled perturbed Hartree-Fock (CPHF) equations required for Hessian evaluation could not been solved at the located stationary point, probably due to the increased inherent instability of the ROHF orbitals describing core-hole Rydberg state. Although we failed to compute vibrational frequencies which could prove directly that the true minimum was found, no other stationary point could be obtained even when less-symmetric guesses were used in the geometry optimization procedure.
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24
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0002192627
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