Evaluation of the degradation cross-cection as stopping power dependence for pure and mixture molecular samples at cryogenic temperatures

  • A. L.F. de Barros
  • , C. Mejia
  • , D. V. Doreste
  • , A. Domaracka
  • , P. Boduch
  • , H. Rothard
  • , E. F. da Silveira

Research output: Contribution to journalArticlepeer-review

Abstract

Ices in interstellar and planetary environments are constantly altered by cosmic radiation. Using FTIR spectroscopy, we analyse radiation-induced changes in ices containing H2O, CO, CO2, and CH3OH, molecules abundant in the Solar System and interstellar medium. Molecular degradation is quantified by apparent cross-sections that scale with the electronic stopping power (Se). Literature data reveal a power-law dependence, σd ∝ Sen, influenced by thickness, sputtering yield, and radiochemical effects. This empirical relationship serves as a benchmark for assessing molecular stability and the interplay between sputtering and radiolysis, improving models of chemical evolution in astrophysical ices.

Keywords

  • Astrochemistry
  • Circumstellar clouds
  • Methods: Laboratory ion irradiation
  • Molecules

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