Water binding to the atmospheric oxidation product methyl vinyl ketone.


Journal

Spectrochimica acta. Part A, Molecular and biomolecular spectroscopy
ISSN: 1873-3557
Titre abrégé: Spectrochim Acta A Mol Biomol Spectrosc
Pays: England
ID NLM: 9602533

Informations de publication

Date de publication:
05 Apr 2022
Historique:
received: 20 10 2021
accepted: 29 12 2021
pubmed: 17 1 2022
medline: 9 2 2022
entrez: 16 1 2022
Statut: ppublish

Résumé

Methyl vinyl ketone is one of the major oxidation products of isoprene, and therefore, an important precursor of secondary organic aerosol. Understanding its interactions with water is relevant to gain insight into aerosol formation and improve the predictive power of atmospheric chemistry models. The molecular complex formed between methyl vinyl ketone and water has been generated in a supersonic jet and characterized using high-resolution microwave spectroscopy in combination with quantum chemistry calculations. In this study, we show that methyl vinyl ketone interacts with water forming four 1:1 isomers connected by O - H···O and C - H···O hydrogen bond interactions. Water has been found to preferentially bind to the antiperiplanar conformation of methyl vinyl ketone. Evidence of a large amplitude motion arising from the methyl internal rotation has been found in the rotational spectra of the dimer. The threefold methyl internal rotation barrier heights have been further determined and discussed for all the species.

Identifiants

pubmed: 35033807
pii: S1386-1425(21)01423-2
doi: 10.1016/j.saa.2021.120846
pii:
doi:

Substances chimiques

Butanones 0
Water 059QF0KO0R
3-buten-2-one AR7642I1MP

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

120846

Informations de copyright

Copyright © 2022 The Authors. Published by Elsevier B.V. All rights reserved.

Déclaration de conflit d'intérêts

Declaration of Competing Interest The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.

Auteurs

Carlos Cabezas (C)

Instituto de Física Fundamental (IFF-CSIC), Group of Molecular Astrophysics, C/ Serrano 121, Madrid 28006, Spain. Electronic address: carlos.cabezas@csic.es.

Marcos Juanes (M)

Departamento de Química Física y Química Inorgánica, Facultad de Ciencias, Universidad de Valladolid, Paseo de Belén 7, Valladolid 47011, Spain.

Rizalina T Saragi (RT)

Departamento de Química Física y Química Inorgánica, Facultad de Ciencias, Universidad de Valladolid, Paseo de Belén 7, Valladolid 47011, Spain.

Alberto Lesarri (A)

Departamento de Química Física y Química Inorgánica, Facultad de Ciencias-I.U. CINQUIMA, Universidad de Valladolid, Paseo de Belén 7, Valladolid 47011, Spain.

Isabel Peña (I)

Departamento de Química Física y Química Inorgánica, Facultad de Ciencias, Universidad de Valladolid, Paseo de Belén 7, Valladolid 47011, Spain. Electronic address: ipencal@qf.uva.es.

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Classifications MeSH