Geant4-IcyMoons: Simulating Electron Interaction Physics in Irradiated Astrophysical Ices
Gideon Yoffe, Jacques Pienaar, Ioanna Kyriakou, Dimitris Emfietzoglou, S\'ebastien Incerti, Hoang Tran, Yohai Kaspi

TL;DR
This paper introduces Geant4-IcyMoons, a Monte Carlo simulation tool for modeling electron interactions with water ice in astrophysical environments, applied to Europa's surface to understand radiation effects.
Contribution
It presents the first transport-ready Monte Carlo simulation of electron irradiation in water ice, enabling detailed study of radiation effects on icy surfaces.
Findings
Electron energy deposition varies between Europa's hemispheres due to different electron energies.
Low-energy electrons deposit energy in the upper 0.1 cm of ice on the trailing hemisphere.
Higher-energy electrons penetrate tens of centimeters on the leading hemisphere.
Abstract
Energetic particles continuously process water ice across astrophysical and planetary environments, from interstellar clouds and comets to icy planetary surfaces. Interpreting the resulting observables requires a physically grounded description of the underlying interactions, both to identify radiation-driven signatures and to distinguish them from superimposed chemical, thermal, and microphysical effects. We present Geant4-IcyMoons, an extension of Geant4-DNA developed for irradiated water ice and, ultimately, for materials embedded within it. In this study, we model the elastic and inelastic interactions of electrons with amorphous and hexagonal ice. For the first time, this enables a transport-ready Monte Carlo simulation of electron irradiation in water ice, linking incident-particle environments to the evolution of icy surfaces. We apply this framework to Jupiter's moon Europa as a…
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