Bombardment of CO ice by cosmic rays: I. Experimental insights into the microphysics of molecule destruction and sputtering

TL;DR

This study experimentally investigates how cosmic ray ions cause molecule destruction and sputtering in CO ice, revealing that electronic excitations are more influential than previously thought and that stopping power alone does not fully explain these processes.

Contribution

The paper provides new experimental insights into the microscopic mechanisms of radiolysis and sputtering in astrophysical ices, highlighting the role of electronic excitations and the limitations of stopping power as a sole predictor.

Findings

Electronic excitations are a more efficient channel for radiolysis and sputtering.

Stopping power does not solely control molecule destruction and sputtering.

Charge state and CO$^+$ production rate have negligible effects.

Abstract

We present a dedicated experimental study of microscopic mechanisms controlling radiolysis and sputtering of astrophysical ices due to their bombardment by cosmic ray ions. Such ions are slowed down due to inelastic collisions with bound electrons, resulting in ionization and excitation of ice molecules. In experiments on CO ice irradiation, we show that the relative contribution of these two mechanisms of energy loss to molecule destruction and sputtering can be probed by selecting ion energies near the peak of the electronic stopping power. We have observed a significant asymmetry, both in the destruction cross section and the sputtering yield, for pairs of ion energies corresponding to same values of the stopping power on either side of the peak. This implies that the stopping power does not solely control these processes, as usually assumed in the literature. Our results suggest that electronic excitations represent a significantly more efficient channel for radiolysis and, possibly, also for sputtering of CO ice. We also show that the charge state of incident ions as well as the rate for CO$^+$ production in the ice have negligible effect on these processes.