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Title: Excited potential energy surfaces of CH[sub 3]SH from the [ital ab] [ital initio] effective valence shell Hamiltonian method

Journal Article · · Journal of Chemical Physics; (United States)
DOI:https://doi.org/10.1063/1.467406· OSTI ID:7141601
; ;  [1];  [2]
  1. The James Franck Institute and the Department of Chemistry, The University of Chicago, Chicago, Illinois 60637 (United States)
  2. Cray Research, Inc., Egan, Minnesota 55123 (United States)

The ground and first and second [sup 1][ital A][double prime] potential surfaces of methyl mercaptan (CH[sub 3]SH) are calculated as a function of the C--S and S--H bond coordinates using the [ital ab] [ital initio] effective valence shell Hamiltonian ([ital H][sup [nu]]) method. The computations for this highly nontrivial system provide the first serious tests for choosing restricted valence spaces and for computing global potential energy surfaces with the [ital H][sup [nu]] methods. The quasidegeneracy constraints on the [ital H][sup [nu]] method suggest choosing a valence space which consists of the two (3[ital a][double prime] and 10[ital a][prime]) highest energy occupied orbitals in the ground state and the three lowest [ital a][prime] unoccupied orbitals. The global potential surfaces are computed with a modest basis, but larger basis set computations at selected geometries test convergence for vertical excitation energies, ionization potentials, and C--S and S--H bond energies. The calculations are compared to both experiment and other calculations for this system. The computations assist in the interpretation of CH[sub 3]SH photodissociation dynamics observed by Butler and co-workers.

DOE Contract Number:
FG02-92ER14305
OSTI ID:
7141601
Journal Information:
Journal of Chemical Physics; (United States), Vol. 101:6; ISSN 0021-9606
Country of Publication:
United States
Language:
English