More pi, please : what drives the formation of unsaturated molecules in the interstellar medium?

We present a computational investigation into the fragmentation pathways of ethanolamine (C2H7NO, EtA), propanol (C3H8O, PrO), butanenitrile (C4H7N, BuN), and glycolamide (C2H5NO2, GlA)—saturated organic molecules detected in the interstellar medium (ISM), particularly in the molecular cloud complex...

Full description

Autores:
Londoño Restrepo, Jhoan Alejandro
Tipo de recurso:
Trabajo de grado de pregrado
Fecha de publicación:
2025
Institución:
Universidad de Antioquia
Repositorio:
Repositorio UdeA
Idioma:
eng
OAI Identifier:
oai:bibliotecadigital.udea.edu.co:10495/45831
Acceso en línea:
https://hdl.handle.net/10495/45831
Palabra clave:
Cosmoquímica
Cosmochemistry
Moléculas interestelares
Interstellar molecules
Nubes moleculares
Molecular clouds
Compuestos orgánicos - Espectros
Organic compounds - Spectra
Dinámica molecular
Molecular dynamics
Química computacional
Computational chemistry
Reacciones de fragmentación
Fragmentation reactions
Rayos cósmicos
Cosmic rays
Radiación ultravioleta
Ultraviolet radiation
Evolución molecular
Molecular evolution
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http://id.loc.gov/authorities/subjects/sh85067528
http://id.loc.gov/authorities/subjects/sh88006798
http://id.loc.gov/authorities/subjects/sh2010104549
http://id.loc.gov/authorities/subjects/sh85086583
http://id.loc.gov/authorities/subjects/sh2020006312
http://id.loc.gov/authorities/subjects/sh92002824
http://id.loc.gov/authorities/subjects/sh85033155
http://id.loc.gov/authorities/subjects/sh85139506
http://id.loc.gov/authorities/subjects/sh85022912
Rights
openAccess
License
http://creativecommons.org/licenses/by-nc-sa/4.0/
Description
Summary:We present a computational investigation into the fragmentation pathways of ethanolamine (C2H7NO, EtA), propanol (C3H8O, PrO), butanenitrile (C4H7N, BuN), and glycolamide (C2H5NO2, GlA)—saturated organic molecules detected in the interstellar medium (ISM), particularly in the molecular cloud complex Sagittarius B2 (Sgr B2) and its molecular cloud G+0.693–0.027. Using electron-impact ionization data and Born–Oppenheimer molecular dynamics simulations, we investigate how cosmic rays, cosmic-ray-induced UV fields, and shock-induced heating can induce the fragmentation of these molecules, resulting in the formation of unsaturated species with extended pi-bond networks. Despite the attenuation of external UV radiation in G+0.693–0.027, these energetic processes are capable of driving partial transformations of saturated into unsaturated molecules, supporting the coexistence of species like EtA and GlA alongside unsaturated nitriles such as cyanoacetylene (HC3N), cyanopropyne (CH3C3N), and cyanoallene (CH2CCHCN). Our findings underscore the significance of high-energy mechanisms in enhancing chemical complexity within molecular clouds and offer insights into the pathways that govern the evolution of organic molecules in the ISM.