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Title: Internal state distributions of CO from HNCO photodissociation

Journal Article · · J. Chem. Phys.; (United States)
DOI:https://doi.org/10.1063/1.453215· OSTI ID:6365896

The internal state distributions of CO produced by photodissociation of HNCO at 1930 (230.1 nm) and at 10 200 cm/sup -1/ (193.3 nm) in excess of the dissociation energy are determined from multiphoton ionization spectra of the CO fragment measured under collision-free conditions. The rotational state distribution of the CO produced at the lower photolysis energy is characterized by a temperature of (491 +- 23) K. The rotational state distribution of CO produced by photodissociation at the higher photon energy in not well characterized by a temperature. This latter distribution has maximum population near J = 37, extends beyond J = 65, and accounts for --20% of the available energy in excess of that necessary to rupture the HN--CO bond. An impulsive dissociation model assuming that dissociation occurs from an excited HNCO complex containing a nonlinear N--C--O configuration accounts for the average CO rotational excitation while phase-space theory does not agree with the observed distributions. Fitting a semiclassical model to the data using a logically constructed potential energy surface and a ground-state-dependent function provides a useful parametrization for the impulsive dissociation. Although not absolute, this analysis suggests that the dissociation occurs directly on a repulsive excited state potential energy surface.

Research Organization:
Combustion Research Facility, Sandia National Laboratories, Livermore, California 94550
OSTI ID:
6365896
Journal Information:
J. Chem. Phys.; (United States), Vol. 87:3
Country of Publication:
United States
Language:
English