State resolved data for radiative association of H and p and for photodissociation of H${}_2^{+}$

Abstract

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.

8 pages, 1 figure, ApJS accepted

References in corpus (2)

• Vibrational level population of H${}_2$ and H${}_2^{+}$ in the early Universe
• Cosmological production of H_2 before the formation of the first galaxies

Cited by in corpus (1)

• Modelling the cosmological Lyman-Werner background radiation field in the Early Universe