ELECTRONIC STRUCTURE OF SIO-SPECTROSCOPY AND PHOTODISSOCIATION
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Abstract
The SiO molecule has been observed in circumstellar envelopes and in several sources, in particular in star-forming regions but not in cold clouds. Very recent studies suggest that the formation of this species must certainly be linked to high temperatures. This molecule has been localised in regions where the ultraviolet photons are abundant and it is necessary to know the photo dissociation cross sections and reaction rates. We report have {ab-initio} calculations of the energies of the first singles excited states lying between the electronic ground state and the first dissociation asymptote. The atomic orbital basis act comprised 129 contracted functions including f functions on the two atoms. First, we have calculated the MCSCF (Mult configurational self consistent field) potential energy functions along the stretching coordinate (coov) for the single valence states
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Author Institution: DAMAp ET URAB12 du CNRS, Observ atoire de Paris-Meudon