Radiative association of C(3P) and H+: triplet states
Abstract
The radiative association of C(3P) and H+ is investigated by calculating cross-sections for photon emission into bound ro-vibrational states of CH+ from the vibrational continua of initial triplet d 3Π or b 3Σ- states. Potential energy curves and transition dipole moments are calculated using multireference configuration interaction (MRCI) methods with AV6Z basis sets. The cross-sections are evaluated using quantum-mechanical methods and rate coefficients are calculated. The rate coefficients are about 100 times larger than those for radiative association of C+(2Po) and H from the A 1Π state. We also confirm that the formation of CH+ by radiative association of C+(2Po) and H via the triplet c 3Σ+ state is a minor process.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- June 2017
- DOI:
- 10.1093/mnras/stx630
- arXiv:
- arXiv:1702.07777
- Bibcode:
- 2017MNRAS.468.2052B
- Keywords:
-
- astrochemistry;
- molecular data;
- molecular processes;
- scattering;
- ISM: molecules;
- galaxies: ISM;
- Physics - Atomic Physics;
- Astrophysics - Astrophysics of Galaxies;
- Physics - Chemical Physics
- E-Print:
- Accepted for publication in MNRAS. 7 pages, 7 figures