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Published October 12, 2023 | Published
Journal Article Open

A-Band Absorption Spectrum of the ClSO Radical: Electronic Structure of the Sulfinyl Group

Abstract

Sulfur oxide species (RSO) play a critical role in many fields, ranging from biology to atmospheric chemistry. Chlorine-containing sulfur oxides may play a key role in sulfate aerosol formation in Venus' cloud layer by catalyzing the oxidation of SO to SO₂ via sulfinyl radicals (RSO). We present results from the gas-phase UV–vis transient absorption spectroscopy study of the simplest sulfinyl radical, ClSO, generated from the pulsed-laser photolysis of thionyl chloride at 248 nm (at 40 Torr of N₂ and 292 K). A weak absorption spectrum from 350 to 480 nm with a peak at 385 nm was observed, with partially resolved vibronic bands (spacing = 226 cm⁻¹), and a peak cross section σ(385 nm) = (7.6 ± 1.9) × 10⁻²⁰ cm². From ab initio calculations at the EOMEE-CCSD/ano-pVQZ level, we assigned this band to 1²A′ ← X²A″ and 2²A′ ← X²A″ transitions. The spectrum was modeled as a sum of a bound-to-free transition to the 1²A′ state and a bound-to-bound transition to the 2²A′ state with similar oscillator strengths; the prediction agreed well with the observed spectrum. We attributed the vibronic structure to a progression in the bending vibration of the 2²A′ state. Further calculations at the XDW-CASPT2 level predicted a conical intersection between the excited 1²A′ and 2²A′ potential energy surfaces near the Franck–Condon region. The geometry of the minimum-energy conical intersection was similar to that of the ground-state geometry. The lack of structure at shorter wavelengths could be evidence of a short excited-state lifetime arising from strong vibronic coupling. From simplified molecular orbital analysis, we attributed the ClSO spectrum to transitions involving the out-of-plane π/π* orbitals along the S–O bond and the in-plane orbital possessing a σ/σ* character along the S–Cl bond. We hypothesize that these orbitals are common to other sulfinyl radicals, RSO, which would share a combination of a strong and a weak transition in the UV (near 300 nm) and visible (400–600 nm) regions.

Copyright and License

© 2023 The Authors. Published by American Chemical Society. This publication is licensed under CC-BY 4.0.

 

Acknowledgement

The experimental research herein was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration (NASA). Financial support was provided by the NASA Solar System Working Program, Grant 80NM0018F0612, and partial fellowship support for W.C. from the J. Yang and Family Foundation.

Contributions

The manuscript was written through contributions of all authors. W.C. performed the experiments and calculations. G.H.J. performed additional calculations. All authors have given approval to the final version of the manuscript.

Conflict of Interest

The authors declare no competing financial interest.

Additional Information

Published as part of The Journal of Physical Chemistry virtual special issue "Marsha I. Lester Festschrift".

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Additional details

Created:
October 17, 2023
Modified:
October 17, 2023