Proposed importance of HOCO chemistry: Inefficient formation of CO from CO and OH reactions on ice dust
arXiv:2410.01373 · doi:10.3847/1538-4357/ad8235
Abstract
With the advent of JWST ice observations, dedicated studies on the formation reactions of detected molecules are becoming increasingly important. One of the most interesting molecules in interstellar ice is CO. Despite its simplicity, the main formation reaction considered, CO + OH -> CO + H through the energetic HOCO* intermediate on ice dust, is subject to uncertainty because it directly competes with the stabilization of HOCO as a final product which is formed through energy dissipation of HOCO* to the water ice. When energy dissipation to the surface is effective during reaction, HOCO can be a dominant product. In this study, we experimentally demonstrate that the major product of the reaction is indeed not CO, but rather the highly reactive radical HOCO. The HOCO radical can later evolve into CO through H-abstraction reactions, but these reactions compete with addition reactions, leading to the formation of carboxylic acids (R-COOH). Our results highlight the importance of HOCO chemistry and encourage further exploration of the chemistry of this radical.
Accepted in ApJ; 23 pages, 9 figures
References in corpus (12)
- Formation of complex organic molecules in hot molecular cores through nondiffusive grain-surface and ice-mantle chemistry
- Formation of Complex Organic Molecules in Cold Interstellar Environments through non-diffusive grain-surface and ice-mantle chemistry
- CO2 formation in quiescent clouds; an experimental study of the CO + OH pathway
- Discovery of the elusive carbonic acid (HOCOOH) in space
- Where does the energy go during the interstellar NH formation on water ice? A computational study
- Surface Diffusion of Carbon Atoms as a Driver of Interstellar Organic Chemistry
- Behavior of Hydroxyl Radicals on Water Ice at Low Temperatures
- Reaction dynamics on amorphous solid water surfaces using interatomic machine learned potentials. Microscopic energy partition revealed from the P + H -> PH reaction
- Cracking the Puzzle of CO2 Formation on Interstellar Ices. Quantum Chemical and Kinetic Study of the CO + OH -> CO2 + H Reaction
- Direct Determination of the Activation Energy for Diffusion of OH Radicals on Water Ice
- The formation of CO through consumption of gas-phase CO on vacuum-UV irradiated water ice
- Determination of the branching ratio of CHOH + OH reaction on water ice surface at 10 K
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