Low-temperature chemistry between water and hydroxyl radicals: H/D isotopic effects
arXiv:1511.02010 · doi:10.1093/mnras/stv2305
Abstract
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.
Accepted for publication in MNRAS
References in corpus (12)
- Interstellar water chemistry: from laboratory to observations
- Simulation of the Formation and Morphology of Ice Mantles on Interstellar Grains
- Laboratory evidence for efficient water formation in interstellar ices
- Photodesorption of water ice: a molecular dynamics study
- Formation of hydrogen peroxide and water from the reaction of cold hydrogen atoms with solid oxygen at 10K
- Multilayer formation and evaporation of deuterated ices in prestellar and protostellar cores
- Water Formation through a Quantum Tunneling Surface Reaction, OH + H2, at 10 K
- CO2 formation in quiescent clouds; an experimental study of the CO + OH pathway
- Modeling Heat Dissipation at the Nanoscale: An Embedding Approach for Chemical Reaction Dynamics on Metal Surfaces
- Interstellar Simulations Using A Unified Microscopic-Macroscopic Monte Carlo Model with a full Gas-Grain Network including Bulk Diffusion in Ice Mantles
- On the relevance of the H2 + O reaction pathway for the surface formation of interstellar water - A combined experimental and modeling study
- Thermal H/D exchange in polar ice - deuteron scrambling in space
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