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

  • Ana Lucia Ferreira de Barros (First Author)
  • , Christian Fernando Mejía Guamán
  • , Davi V. Doreste
  • , Alicja Domaracka
  • , Philippe Boduch
  • , Hermann Rothard
  • , Enio Frota da Silveira (Last Author)
  • Centro Federal de Educação Tecnológica Celso Suckow da Fonseca
  • Boulevard Henri Becquerel
  • Pontifícia Universidade Católica do Rio de Janeiro

Research output: Contribution to journal › Article › peer-review

1 Scopus citations

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.

Original languageEnglish
Article number165926
Pages (from-to)1-16
Number of pages16
JournalNuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms
Volume570
Early online date10 Nov 2025
DOIs
StatePublished - Jan 2026

Keywords

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

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