http://arxiv.org/abs/1412.2606
The matrix elements and energies needed to calculate vibrational-rotational state resolved cross sections and rate coefficients for radiative association of H and p and for photodissociation of H${}_2^+$ are presented for applications to simulations of chemistry in the early Universe and to stellar atmospheres.
J. Babb
Tue, 9 Dec 14
21/64
Comments: 8 pages, 1 figure, ApJS accepted