Answers are grounded in this paper and cite their sources.
R-Matrix study examines electron scattering effects on ethylene glycol, aiding astrochemical interpretation.
Ethylene glycol is a prebiotically relevant complex organic molecule detected in interstellar and cometary environments, yet quantitative low-energy electron–ethylene glycol scattering data remain limited for astrochemical modeling. This work presents an R-matrix study of low-energy electron collisions with ethylene glycol over a 0–12 eV energy range, using static exchange (SE), static exchange plus polarization (SEP), and configuration interaction (CI) models with 6-311G* and cc-pVTZ basis sets. We compute elastic, excitation, and differential cross-sections within a close-coupling framework. The dataset offers benchmark inputs for astrochemical models, supporting interpretation of ethylene glycol abundances in space and refining constraints on electron-induced prebiotic pathways.
No takes yet. Share an insight, caveat, or question.
Chakraborty et al. (2026) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: