The matrix elements and energies needed to calculate vibrational-rotational state resolved cross sections and rate coefficients for radiative association of H and H and for photodissociation of H_2^ are presented for applications to simulations of chemistry in the early universe and to stellar atmospheres.
The matrix elements and energies needed to calculate vibrational-rotational state resolved cross sections and rate coefficients for radiative association of H and H+ and for photodissociation of H_2^+ are presented for applications to simulations of chemistry in the early universe and to stellar atmospheres.
