Inverting the ground state of interstellar CH

Astronomy and Astrophysics – Astronomy

Scientific paper

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Ground State, Hydrocarbons, Interstellar Chemistry, Molecular Excitation, Angular Momentum, Cloud Physics, Microwave Emission, Molecular Spectra, Radio Sources (Astronomy)

Scientific paper

Gwinn and Townes (1968) have conjectured a collision mechanism whereby a certain half of a Lambda-doublet will be more strongly excited during rotational excitation of an open-shell diatomic molecule from the ground state. This paper assumes that the Gwinn-Townes conjecture is valid. Certain matrix elements of the scalar product between the angular momentum of a molecule's end-over-end rotation and its electrons' orbital angular momentum perpendicular to their plane of motion are calculated, and the preferred states corresponding to a specific spatial orientation of the molecule's cloud of valence electrons are identified. The results are used to derive the level populations of CH in model-cloud calculations and to investigate systematically the regions of physical parameters which yield the observed inversion of the ground state of CH. Effects of near-IR and UV pumps in the case of CH are briefly considered along with line-overlap effects.

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