Electron scattering from prebiotic ethylene glycol: An R-matrix study
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.
Authors
- Bobby Antony (ORCID: https://orcid.org/0000-0003-2073-9681)
- Irabati Chakraborty (ORCID: https://orcid.org/0000-0001-5667-1178)
Institutions
- Indian Institute of Technology Dhanbad (IN)
Publication Details
- Journal
- Journal of Applied Physics
- Published
- 2026-06-09
- DOI
- https://doi.org/10.1063/5.0334415
- Primary Topic
- Astrophysics and Star Formation Studies
- Type
- article
- Field-Weighted Citation Impact
- 0.00