作者: Sarantos Marinakis , Indigo Lily Dean , Jacek Kłos , François Lique
DOI: 10.1039/C5CP03696H
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摘要: We present a new set of potential energy surfaces (PESs) for the CH(X2Π)–He van der Waals system. Ab initio calculations CH–He PES were carried out using open-shell single- and double-excitation coupled cluster approach with non-iterative perturbational treatment triple excitations [RCCSD(T)]. The augmented correlation-consistent polarized valence quadruple-zeta (aug-cc-pVQZ) basis was employed by mid-bond functions. Integral cross sections rotational excitation in collisions calculated compared available experimental results. newly constructed reproduces results CH(X2Π, v = 0)–He better than any previously PES. Differential (DCS) are presented first time this system discussed within context rainbows. Finally, our work provides rate thermal coefficients that crucially needed astrochemical modelling future anticipated experiments collisions.