http://arxiv.org/abs/1511.02010
Sets of systematic laboratory experiments are presented — combining Ultra High Vacuum cryogenic and plasma-line deposition techniques — that allow us to compare H/D isotopic effects in the reaction of H2O (D2O) ice with the hydroxyl radical OD (OH). The latter is known to play a key role as intermediate species in the solid-state formation of water on icy grains in space. The main finding of our work is that the reaction H2O + OD –> OH + HDO occurs and that this may affect the HDO/H2O abundances in space. The opposite reaction D2O + OH –> OD + HDO is much less effective, and also given the lower D2O abundances in space not expected to be of astronomical relevance. The experimental results are extended to the other four possible reactions between hydroxyl and water isotopes and are subsequently used as input for Kinetic Monte Carlo simulations. This way we interpret our findings in an astronomical context, qualitatively testing the influence of the reaction rates.
T. Lamberts, G. Fedoseev, F. Puletti, et. al.
Mon, 9 Nov 15
5/55
Comments: Accepted for publication in MNRAS