IBER 2023

MICROSOLVATION OF α-PINENE OXIDE AS OBSERVED BY BROADBAND ROTATIONAL SPECTROSCOPY

6 Sept 2023, 18:35

1h

Department of Physics, University of Coimbra

Poster Communication Poster Session

Speakers

C. CABEZAS (Instituto de Física Fundamental, CSIC, C/ Serrano 121, 28006 Madrid, Spain) E.M. NEEMAN (Univ. Lille, UMR 8523 - PhLAM - Physique des Lasers Atomes et Molecules, F-59000 Lille, France) I. Peña (Departamento de Química Física y Química Inorgánica, Facultad de Ciencias-Instituto CINQUIMA, Universidad de Valladolid, Paseo de Belén 7, 47011 Valladolid, Spain) J. R MORAN (Departamento de Química Física y Química Inorgánica, Facultad de Ciencias-Instituto CINQUIMA, Universidad de Valladolid, Paseo de Belén 7, 47011 Valladolid, Spain) N. OSSEIRAN (Univ. Lille, UMR 8523 - PhLAM - Physique des Lasers Atomes et Molecules, F-59000 Lille, France) S. COLLIGNON (Univ. Lille, UMR 8523 - PhLAM - Physique des Lasers Atomes et Molecules, F-59000 Lille, France) T.R. HUET (Univ. Lille, UMR 8523 - PhLAM - Physique des Lasers Atomes et Molecules, F-59000 Lille, France) W. Li (Departamento de Química Física y Química Inorgánica, Facultad de Ciencias-Instituto CINQUIMA, Universidad de Valladolid, Paseo de Belén 7, 47011 Valladolid, Spain)

Description

α-pinene is the most abundant monoterpene in the atmosphere and its oxidation yields to several oxygenated species that play a major role in the formation of secondary organic aerosols. α-pinene oxide (C${}_{10}$H${}_{16}$O) is generated from the reaction of ozone with α-pinene and has been shown to contribute to the formation of organosulfates under atmospheric conditions. Thus, understanding its interactions with atmospheric molecules is crucial to explain the first steps of molecular aggregation in the aerosol formation. Here, we present the investigation of the hydrates of α-pinene oxide, C${}_{10}$H${}_{16}$O· · ·(H${}_2$O)${}_n$ (n=1,2), using two different chirped-pulse Fourier transform microwave spectrometers operating in the 2-18 GHz frequency range,${}^{1,2}$ supported by quantum chemical calculations. The hydrates consist of water chains anchored to the oxygen atom of α-pinene oxide by a primary O−H· · ·O hydrogen bond and further stabilized by secondary C−H· · ·O interactions. The structures of these hydrates have been further confirmed by the analysis of the rotational spectra of their ${}^{18}$O water isotopologues and compared with those of related
species.

References
${}^1$ doi:10.1063/5.0147909, E. M. Neeman, N. Osseiran, T. R. Huet, The gas-phase structure determination of α-pinene oxide: An endo-cyclic epoxide of atmospheric interest, J. Chem. Phys. 158, 154304 (2023).
${}^2$ doi:10.1016/j.saa.2021.120846, C. Cabezas, M. Juanes, R. T. Saragi, A. Lesarri, I. Peña, Water binding to the atmospheric oxidation product methyl vinyl ketone, Spectrochim. Acta A Mol. Biomol. Spectrosc. 270, 120846 (2022).

Presentation materials

COIMBRA.pdf