Paper
19 November 2015 Highly excited vibrational states of 18O3 as a test of the ozone potential energy surface
Evgeniya Starikova, Alain Barbe, Marie-Renée De Backer, Didier Mondelain, Samir Kassi, Alain Campargue, Vladimir G. Tyuterev
Author Affiliations +
Proceedings Volume 9680, 21st International Symposium Atmospheric and Ocean Optics: Atmospheric Physics; 96800L (2015) https://doi.org/10.1117/12.2205973
Event: XXI International Symposium Atmospheric and Ocean Optics. Atmospheric Physics, 2015, Tomsk, Russian Federation
Abstract
This work is a part of our systematic investigation of the very weak absorption spectra of 16O3 and 18O3 by high sensitivity Cavity Ring Down Spectroscopy between 5850 and 7920 cm-1. In total, 29 vibrational bands of 16O3 and 24 bands of 18O3 have been assigned in this range. Here we present the recent results of analyses of highly excited states of 18O3 ozone, located near the dissociation energy (D0~8560 cm-1). The comparison of the vibrational band centers obtained from the analysis with the predictions based on the potential energy surface (PES) suggests that the hypothesis of the “reef structure” at the ozone transition state towards the dissociation is not confirmed by spectroscopic observations. In this work, we focus on the comparison between theoretical and experimental values of the 18O3 vibrational levels near the dissociation limit.
© (2015) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Evgeniya Starikova, Alain Barbe, Marie-Renée De Backer, Didier Mondelain, Samir Kassi, Alain Campargue, and Vladimir G. Tyuterev "Highly excited vibrational states of 18O3 as a test of the ozone potential energy surface", Proc. SPIE 9680, 21st International Symposium Atmospheric and Ocean Optics: Atmospheric Physics, 96800L (19 November 2015); https://doi.org/10.1117/12.2205973
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KEYWORDS
Ozone

Spectroscopy

Photoemission spectroscopy

Absorption

Atmospheric optics

Molecules

Chemistry

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