Influence of surface and bulk water ice on the reactivity of a water-forming reaction
Thanja Lamberts, Johannes K\"astner

TL;DR
This study investigates how surface and bulk water ice influence the rate of a key water-forming reaction on interstellar grains, using advanced modeling to account for quantum tunneling effects at very low temperatures.
Contribution
It introduces a multiscale modeling approach combining DFT and force fields to evaluate reaction rates on icy surfaces, revealing the impact of hydrogen bonding and ice structure on reactivity.
Findings
Binding energies vary with hydrogen bonding environment.
Highly amorphous ice can block reaction pathways.
Reaction rate constants can be up to two orders of magnitude higher than the lower limit.
Abstract
On the surface of icy dust grains in the dense regions of the interstellar medium a rich chemistry can take place. Due to the low temperature, reactions that proceed via a barrier can only take place through tunneling. The reaction H + HO HO + OH is such a case with a gas-phase barrier of 26.5 kJ/mol. Still the reaction is known to be involved in water formation on interstellar grains. Here, we investigate the influence of a water ice surface and of bulk ice on the reaction rate constant. Rate constants are calculated using instanton theory down to 74 K. The ice is taken into account via multiscale modeling, describing the reactants and the direct surrounding at the quantum mechanical level with density functional theory (DFT), while the rest of the ice is modeled on the molecular mechanical level with a force field. We find that HO binding…
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