Author:
Hashemi S. Rasoul,Barinovs Girts,Nyman Gunnar
Abstract
The degradation of indene is investigated using molecular dynamics (MD) with the ReaxFF force field and RRKM theory. Microcanonical rate constants are obtained over a broad energy range (8–25 eV). There is agreement between the results of the molecular dynamics and RRKM calculations at the lower energies, while the molecular dynamics rate constants are larger at the higher energies. At the lower energies there is also agreement with values obtained by using expressions for photodegradation of polyaromatic hydrocarbons from the literature. Values from those expressions however increase even faster with energy than our molecular dynamics rate constants do. At the same time those values are lower than an experimental result at 6.4 eV. This suggests that astrochemical models employing those values may result in unreliable polycyclic aromatic hydrocarbons abundances.
Subject
Astronomy and Astrophysics
Reference36 articles.
1. Photodestruction of pahs in the interstellar medium. ii. influence of the states of ionization and hydrogenation;Allain;Astronomy Astrophysics
2. Photodestruction of pahs in the interstellar medium. i. photodissociation rates for the loss of an acetylenic group;Allain;Astronomy Astrophysics
3. Discovery of the pure polycyclic aromatic hydrocarbon indene (c-c9h8) with gotham observations of tmc-1;Burkhardt;Astrophysical J. Lett.,2021
4. Discovery of c5h+ and detection of c3h+ in tmc-1 with the quijote line survey;Cernicharo;Astronomy Astrophysics