{ "id": "2110.15887", "version": "v1", "published": "2021-10-29T16:24:18.000Z", "updated": "2021-10-29T16:24:18.000Z", "title": "Carbon Atom Reactivity with Amorphous Solid Water: H$_2$O Catalyzed Formation of H$_2$CO", "authors": [ "Germán Molpeceres", "Johannes Kästner", "Gleb Fedoseev", "Danna Qasim", "Richard Schömig", "Harold Linnartz", "Thanja Lamberts" ], "comment": "Accepted for publication in JPCL", "doi": "10.1021/acs.jpclett.1c02760", "categories": [ "astro-ph.GA" ], "abstract": "We report new computational and experimental evidence of an efficient and astrochemically relevant formation route to formaldehyde (H$_2$CO). This simplest carbonylic compound is central to the formation of complex organics in cold interstellar clouds, and is generally regarded to be formed by the hydrogenation of solid-state carbon monoxide. We demonstrate H$_2$CO formation via the reaction of carbon atoms with amorphous solid water. Crucial to our proposed mechanism is a concerted proton transfer catalyzed by the water hydrogen bonding network. Consequently, the reactions $^3$C + H$_2$O -> $^3$HCOH and $^1$HCOH -> $^1$H$_2$CO can take place with low or without barriers, contrary to the high-barrier traditional internal hydrogen migration. These low barriers or absence thereof explain the very small kinetic isotope effect in our experiments when comparing the formation of H$_2$CO to D$_2$CO. Our results reconcile the disagreement found in the literature on the reaction route: C + H$_2$O -> H$_2$CO.", "revisions": [ { "version": "v1", "updated": "2021-10-29T16:24:18.000Z" } ], "analyses": { "keywords": [ "amorphous solid water", "carbon atom reactivity", "catalyzed formation", "high-barrier traditional internal hydrogen migration", "small kinetic isotope effect" ], "tags": [ "journal article" ], "publication": { "publisher": "ACS" }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }