Water formation at low temperatures by surface O2 hydrogenation I: characterization of ice penetration
S. Ioppolo, H. M. Cuppen, C. Romanzin, E. F. van Dishoeck, H., Linnartz

TL;DR
This study investigates how the structure of O2 ice influences water formation at low temperatures through hydrogenation, revealing complex reaction mechanisms and the need to consider additional surface reactions.
Contribution
It provides detailed experimental insights into H-atom penetration and reaction mechanisms in O2 ice, highlighting the incomplete nature of existing hydrogenation schemes.
Findings
H-atom penetration depends on ice temperature, thickness, and structure.
Reaction and diffusion compete, affecting water and hydrogen peroxide formation.
Ozone formation indicates additional reaction pathways beyond O2 hydrogenation.
Abstract
Water is the main component of interstellar ice mantles, is abundant in the solar system and is a crucial ingredient for life. The formation of this molecule in the interstellar medium cannot be explained by gas-phase chemistry only and its surface hydrogenation formation routes at low temperatures (O, O2, O3 channels) are still unclear and most likely incomplete. In a previous paper we discussed an unexpected zeroth-order H2O production behavior in O2 ice hydrogenation experiments compared to the first-order H2CO and CH3OH production behavior found in former studies on hydrogenation of CO ice. In this paper we experimentally investigate in detail how the structure of O2 ice leads to this rare behavior in reaction order and production yield. In our experiments H atoms are added to a thick O2 ice under fully controlled conditions, while the changes are followed by means of reflection…
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