http://arxiv.org/abs/2304.00072
For a quasi-molecular mechanism of cosmological recombination, a scheme of calculation based on a rigorous quantum-mechanical approach is elaborated. The probability of free-bound radiative transition into an excited state of a quasi-molecule temporarily formed by a colliding electron and two nearest neighboring protons is derived in a closed algebraic form.
T. Kereselidze, I. Noselidze and Z. Machavariani
Tue, 4 Apr 23
90/111
Comments: 10 pages, 2 figures