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The feasible photoinduced growth of polycyclic aromatic hydrocarbons from cosmic benzene ice

Vera Andreevna Terashkevich 1
Vera Andreevna Terashkevich
Elena Alexandrovna Pazyuk 1
Elena Alexandrovna Pazyuk
Andrey Vladislavovich Stolyarov 1
Andrey Vladislavovich Stolyarov
Published 2025-03-31
CommunicationVolume 35, Issue 3, 324-326
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Terashkevich V. A., Pazyuk E. A., Stolyarov A. V. The feasible photoinduced growth of polycyclic aromatic hydrocarbons from cosmic benzene ice // Mendeleev Communications. 2025. Vol. 35. No. 3. pp. 324-326.
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Terashkevich V. A., Pazyuk E. A., Stolyarov A. V. The feasible photoinduced growth of polycyclic aromatic hydrocarbons from cosmic benzene ice // Mendeleev Communications. 2025. Vol. 35. No. 3. pp. 324-326.
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TY - JOUR
DO - 10.71267/mencom.7639
UR - https://mendcomm.colab.ws/publications/10.71267/mencom.7639
TI - The feasible photoinduced growth of polycyclic aromatic hydrocarbons from cosmic benzene ice
T2 - Mendeleev Communications
AU - Terashkevich, Vera Andreevna
AU - Pazyuk, Elena Alexandrovna
AU - Stolyarov, Andrey Vladislavovich
PY - 2025
DA - 2025/03/31
PB - Mendeleev Communications
SP - 324-326
IS - 3
VL - 35
ER -
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@article{2025_Terashkevich,
author = {Vera Andreevna Terashkevich and Elena Alexandrovna Pazyuk and Andrey Vladislavovich Stolyarov},
title = {The feasible photoinduced growth of polycyclic aromatic hydrocarbons from cosmic benzene ice},
journal = {Mendeleev Communications},
year = {2025},
volume = {35},
publisher = {Mendeleev Communications},
month = {Mar},
url = {https://mendcomm.colab.ws/publications/10.71267/mencom.7639},
number = {3},
pages = {324--326},
doi = {10.71267/mencom.7639}
}
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Terashkevich, Vera Andreevna, et al. “The feasible photoinduced growth of polycyclic aromatic hydrocarbons from cosmic benzene ice.” Mendeleev Communications, vol. 35, no. 3, Mar. 2025, pp. 324-326. https://mendcomm.colab.ws/publications/10.71267/mencom.7639.

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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