Keywords
ab initio
calculation
astrochemistry
benzene excimer
cosmic photochemistry
interstellar medium
polycyclic aromatic hydrocarbons
Abstract
The reactive phenyl radical, electronically excited benzene monomer and dimer, their radical cations and low-atomic neutral hydrocarbons may be born in situ via the photodissociation/photoionization of a gaseous benzene monomer/dimer photo-desorbed from cosmic ice as well as via the subsequent dissociative recombination of the arisen benzene cations. The above-mentioned species can be the sources for the assembly into large polycyclic aromatic hydrocarbons, which can occur at very low temperatures and pressures in the interstellar medium.
Funders
Russian Science Foundation
23-13-00207
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