1. Resolved fine and hyperfine state-to-state rate coefficients for the rotational transitions of C3N induced by collision with He
- Author
-
Miguel Lara-Moreno, Thierry Stoecklin, Philippe Halvick, Institut des Sciences Moléculaires (ISM), and Université Montesquieu - Bordeaux 4-Université Sciences et Technologies - Bordeaux 1-École Nationale Supérieure de Chimie et de Physique de Bordeaux (ENSCPB)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Physics ,Scattering ,chemistry.chemical_element ,Astronomy and Astrophysics ,State (functional analysis) ,Collision ,01 natural sciences ,[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry ,chemistry ,Space and Planetary Science ,0103 physical sciences ,Potential energy surface ,[CHIM]Chemical Sciences ,Limit (mathematics) ,Atomic physics ,010306 general physics ,010303 astronomy & astrophysics ,Hyperfine structure ,Excitation ,Helium - Abstract
The fine and hyperfine resolved state-to-state rate coefficients for the rotational (de)excitation of C3N by collision with helium are computed. To this aim a 2D potential energy surface is calculated for this system. The recoupling method is used to obtain the fine and hyperfine structure resolved rate coefficients from spin-free close-coupling calculations. These results are compared with those given by the infinite-order sudden approximation and the M-randomizing limit. General propensity rules for the transitions are also found and analysed.
- Published
- 2021
- Full Text
- View/download PDF