Collisional Studies of Neutral Species at Very Low Temperature

In traditional collisional studies, the large number of thermally populated states and the nature of the molecular interaction cause much of the complexity. Thus, it is expected that the very large reduction in the number of thermally populated states at low temperature will make the relation between observables and the fundamental interactions significantly more direct.

A substantial body of experimental pressure broadening data has now been obtained by use of the collisional cooling technique ( 386, 411, 413, 418, 419, 420, 423, 441, 442, 449, 456) for CO, H2S, HDO, CH3F, and NO in collision with He and H2. For a few of these intermolecular potentials obtained either by ab initio techniques or from the analyses of the spectra of weakly bound complexes are available and theoretical methods (e.g. MOLSCAT) make possible a direct comparison between experiment and theory.

Due to the fundamental role played by CO - He in quantum chemistry as well as astrophysics, this system has been the subject of extensive study (Green and Thaddeus) (Green and Palma) (Cohen et al.) (Korona, et al.). The figure shows a comparision between experimental results and MOLSCAT calculations based on an early ab initio intermolecular potential (IMP) due to Thomas, Kraemer, and Dierksen (Dierksen, Kraemer, and Thomas) and a more recent IMP derived from the spectrum of the CO - He complex (Chuaqui, Le Roy, and McKellar).
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