In Quest of the Missing C 2 H 6 O 2 Isomers in the Interstellar Medium: A Theoretical Search

Ethylene glycol (C H O ), the only diol detected in the interstellar medium (ISM), is a key component in the synthesis of prebiotic sugars. Its structural isomer, methoxymethanol, has also been found in the ISM. Our results show that neither ethylene glycol (ethane-1,2-diol) nor methoxymethanol is t...

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Veröffentlicht in:The journal of physical chemistry. A, Molecules, spectroscopy, kinetics, environment, & general theory Molecules, spectroscopy, kinetics, environment, & general theory, 2024-08, Vol.128 (32), p.6757-6762
Hauptverfasser: Noriega, Lisset, Gonzalez-Ortiz, Luis Armando, Ortíz-Chi, Filiberto, Ramírez, Sandra I, Merino, Gabriel
Format: Artikel
Sprache:eng
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Zusammenfassung:Ethylene glycol (C H O ), the only diol detected in the interstellar medium (ISM), is a key component in the synthesis of prebiotic sugars. Its structural isomer, methoxymethanol, has also been found in the ISM. Our results show that neither ethylene glycol (ethane-1,2-diol) nor methoxymethanol is the most stable isomer. Using high-level computational methods, we identified five isomers: two diols, one hydroxy ether, and two peroxides. The geminal diol 1,1-ethanediol (ethane-1,1-diol) is the most stable isomer, although it has not been detected in the ISM, whereas the two peroxides are less stable than the geminal diol by 60 kcal/mol. This study also provides the rotational constants and dipole moment for each conformer of every C H O isomer.
ISSN:1089-5639
1520-5215
DOI:10.1021/acs.jpca.4c04102