Chemistry on rotating grain surfaces: ro-thermal hopping and segregation of molecules in ice mantles
Thiem Hoang

TL;DR
This paper investigates how suprathermal rotation of interstellar grains, driven by radiative torques, enhances molecular mobility and segregation in icy grain mantles, impacting astrochemical processes.
Contribution
It introduces the concept of ro-thermal hopping, showing how grain spin enhances molecule mobility and segregation beyond thermal effects in space environments.
Findings
Centrifugal force from grain rotation increases radical mobility.
Ro-thermal hopping depends on radiation energy density and gas density.
Grain rotation enables segregation at lower temperatures than previously observed.
Abstract
Grain surfaces play a central role in the formation and desorption of molecules in space. To form molecules on a grain surface, adsorbed species trapped in binding sites must be mobile and migrate to adjacent sites. Thermal hopping is a popular mechanism for the migration of adsorbed species when the grain surface is warmed up by stellar radiation. However, previous studies disregarded the fact that grains can be spun-up to suprathermal rotation by radiative torques (RATs) during grain heating process. To achieve an accurate model of surface astrochemistry, in this paper, we study the effect of grain suprathermal rotation by RATs on thermal hopping of adsorbed species on icy grain mantles. We find that centrifugal force due to grain suprathermal rotation can increase the mobility of radicals on/in the ice mantle compared to the prediction by thermal hopping, and we term this mechanism…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Advanced Chemical Physics Studies · nanoparticles nucleation surface interactions
