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.

arXiv comment8 pages, 1 figure, ApJS accepted

References in corpus (3)

• 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
• Theoretical study of the line profiles of the hydrogen perturbed by collisions with protons

Cited by in corpus (5)

• Photodissociation and photoionisation of atoms and molecules of astrophysical interest
• A sample of 1959 massive galaxy clusters at high redshifts
• Role of the H${}_2^{+}$ channel in the primordial star formation under strong radiation field and the critical intensity for the supermassive star formation
• Modelling the cosmological Lyman-Werner background radiation field in the Early Universe
• Semiclassical Treatment of High-Lying Electronic States of H${}_2^{+}$