English

Radiative association of C(${}^3P$) and H${}^+$: Triplet states

Atomic Physics 2017-05-04 v2 Astrophysics of Galaxies Chemical Physics

Abstract

The radiative association of C(3P{}^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 d3Π\,{}^3\Pi or b3Σ\,{}^3\Sigma^- states. Potential energy curves and transition dipole moments are calculated using multi-reference 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){}^+({}^2{P^o}) and H from the A1Π\,{}^1\Pi state. We also confirm that the formation of CH+{}^+ by radiative association of C+(2Po){}^+({}^2{P^o}) and H via the triplet c3Σ+\,{}^3\Sigma^+ state is a minor process.

Keywords

Cite

@article{arxiv.1702.07777,
  title  = {Radiative association of C(${}^3P$) and H${}^+$: Triplet states},
  author = {James F. Babb and Brendan M. McLaughlin},
  journal= {arXiv preprint arXiv:1702.07777},
  year   = {2017}
}

Comments

Accepted for publication in MNRAS. 7 pages, 7 figures