Mechanism of Atomic Hydrogen Addition Reactions on np-ASW
Jiao He, Shahnewaj M. Emtiaz, Gianfranco Vidali

TL;DR
This study investigates hydrogen addition reactions on interstellar dust grain analogs, finding temperature-independent reaction rates that suggest Eley-Rideal or hot-atom mechanisms dominate over traditional models.
Contribution
The paper provides experimental evidence that challenges existing models by demonstrating temperature independence, highlighting the importance of Eley-Rideal and hot-atom mechanisms in hydrogen reactions.
Findings
Reaction rate is temperature independent from 10 K to 50 K.
Langmuir-Hinshelwood mechanism does not explain observed rates.
Eley-Rideal and hot-atom mechanisms are likely dominant.
Abstract
Hydrogen, being the most abundant element, is the driver of many if not most reactions occurring on interstellar dust grains. In hydrogen atom addition reactions, the rate is usually determined by the surface kinetics of the hydrogen atom instead of the other reaction partner. Three mechanisms exist to explain hydrogen addition reactions on surfaces: Langmuir-Hinshelwood, Eley-Rideal, and hot-atom. In gas-grain models, which mechanism is assumed greatly affects the simulation results. In this work, we quantify the temperature dependence of the rates of atomic hydrogen addition reactions by studying the reaction of H+OO+OH on the surface of a film of non-porous amorphous solid water (np-ASW) in the temperature range from 10 K to 50 K. The reaction rate is found to be temperature independent. This disagrees with the results of simulations with a network of rate…
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