Abstract
The mechanisms and kinetics of the formation of two-ring polycyclic aromatic hydrocarbons via the recombination of benzyl (C7H7) and propargyl (C3H3) radicals under the circumstellar envelopes’ conditions of carbon-rich stars of the asymptotic giant branch, as well as their combustion, were refined on the basis of high-level quantum chemistry methods and the advanced transition state theory. Based on the constructed diagrams of potential energy surfaces and the calculated temperature- and pressure-dependence rate constants of the processes, the reaction pathways and their relative contributions to the composition of the final products are revealed. It is shown that under the conditions of the circumstellar envelopes of the asymptotic giant branch stars, stabilization of the initial complexes C10H10, in contrast to the combustion flame, does not occur, which contributes to an increase in the yield of two-cyclic reaction products.
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Funding
The reported study was funded by RFBR according to the research project no. 20-33-90137 in Samara University, and also was funded by Ministry of Science and Higher Education of the Russian Federation (agreement no. 075-15-2021-597) at the Samara Branch of P.N. Lebedev Physical Institute of the Russian Academy of Sciences.
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Krasnoukhov, V.S., Pivovarov, P.S., Zagidullin, M.V. et al. Formation of Two-ring Polycyclic Aromatic Hydrocarbons via the Recombination of Benzyl and Propargyl Radicals under the Circumstellar Envelopes Conditions of Asymptotic Giant Branch Stars. Astron. Rep. 66, 811–826 (2022). https://doi.org/10.1134/S1063772922090074
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DOI: https://doi.org/10.1134/S1063772922090074