Toward Unraveling Cyanopolyyne Surface Chemistry: A Preview on Isolated Systems From HC3N to Ethyl Cyanide and Propylamine
Cyanopolyynes, a family of nitrogen containing carbon chains, are common in the interstellar medium and possibly form the backbone of species relevant to prebiotic chemistry.
Following their gas phase formation, they are expected to freeze out on ice grains in cold interstellar regions. In this work we present the hydrogenation reaction network of isolated HC3N, the smallest cyanopolyyne, that consists over-a-barrier radical-neutral reactions and barrierless radical-radical reactions.
We employ density functional theory, coupled cluster and multiconfigurational methods to obtain activation and reaction energies for the hydrogenation network of HC3N. This work explores the reaction network of the isolated molecule and constitutes a preview on the reactions occurring on the ice grain surface.
We find that the reactions where the hydrogen atom adds to the carbon chain at carbon atom opposite of the cyano-group give the lowest and most narrow barriers. Subsequent hydrogenation leads to the astrochemically relevant vinyl cyanide and ethyl cyanide. Alternatively, the cyano-group can hydrogenate via radical-radical reactions, leading to the fully saturated propylamine. These results can be extrapolated to give insight into the general reactivity of carbon chains on interstellar ices.
Marten T. Raaphorst, Joan Enrique-Romero, Thanja Lamberts
Comments: In press in ACS Earth and Space Chemistry, accepted 5 May 2025
Subjects: Astrophysics of Galaxies (astro-ph.GA)
Cite as: arXiv:2505.19908 [astro-ph.GA](or arXiv:2505.19908v1 [astro-ph.GA] for this version)
https://doi.org/10.48550/arXiv.2505.19908
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Related DOI:
https://doi.org/10.1021/acsearthspacechem.5c00021
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Submission history
From: Marten Raaphorst
[v1] Mon, 26 May 2025 12:38:27 UTC (248 KB)
https://arxiv.org/abs/2505.19908
Astrobiology, Astrochemistry,
