351. Energetics of the protonation of CO: Implications for the observation of HOC+ in dense interstellar clouds
- Author
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David A. Dixon, Andrew Komornicki, and Wolfgang P. Kraemer
- Subjects
Proton ,Electronic correlation ,Chemistry ,Interstellar cloud ,Ab initio ,General Physics and Astronomy ,Zero-point energy ,Protonation ,Molecular orbital theory ,Physical and Theoretical Chemistry ,Atomic physics ,Affinities ,Molecular physics - Abstract
A number of molecular species on the H3CO(+) energy hypersurface is examined. Ab initio molecular orbital theory is used to determine the structures and relative energetics of the two isomers of HCO(+) and HOC(+) together with the affinity of CO for protonation at either end. The proton affinities of H2 and H2CO are also examined. The calculations are performed using large basis sets and include the effects of electron correlation. The calculated vibrational frequencies are used to correct for zero point energy differences. The results show that the proton affinities of H2 and CO to form HOC(+) are within 1 kcal of each other. The calculations demonstrate that there is no thermodynamic driving force to form HOC(+) in collisions of H3(+) with CO, and that the formation of HCO(+) in such collisions is very exoergic. A plausible mechanism is suggested to explain the differences observed between the laboratory and the interstellar medium.
- Published
- 1984
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