Methane formation in cold regions from carbon atoms and molecular hydrogen
Thanja Lamberts, Gleb Fedoseev, Marc van Hemert, Danna Qasim, Ko-Ju, Chuang, Julia C. Santos, and Harold Linnartz

TL;DR
This study investigates the role of molecular hydrogen in methane formation on icy grains in cold regions, revealing new reaction pathways and mechanisms that could influence astrochemical models.
Contribution
It demonstrates that molecular hydrogen can participate in methane synthesis on icy surfaces, introducing previously unconsidered reaction pathways and tunneling mechanisms.
Findings
Methane can form via reactions involving H$_2$ on icy surfaces.
Reactions like CH + H$_2$ are barrierless and significant.
Molecular hydrogen plays a more important role in methane formation than previously thought.
Abstract
Methane is typically thought to be formed in the solid state on the surface of cold interstellar icy grain mantles via the successive atomic hydrogenation of a carbon atom. In the current work we investigate the potential role of molecular hydrogen in the CH reaction network. We make use of an ultra-high vacuum cryogenic setup combining an atomic carbon atom beam and both atomic and/or molecular beams of hydrogen and deuterium on a HO ice. These experiments lead to the formation of methane isotopologues detected in situ through reflection absorption infrared spectroscopy. Most notably, CH is formed in an experiment combining C atoms with H on amorphous solid water, albeit slower than in experiments with H atoms present. Furthermore, CHD is detected in an experiment of C atoms with H and D on HO ice. CD, however, is only formed when D atoms are…
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