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CH<sub>2</sub>OO Criegee intermediate UV absorption cross-sections and kinetics of CH<sub>2</sub>OO + CH<sub>2</sub>OO and CH<sub>2</sub>OO + I as a function of pressure

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53

References

2020

Year

Abstract

The UV absorption cross-sections of the Criegee intermediate CH<sub>2</sub>OO, and kinetics of the CH<sub>2</sub>OO self-reaction and the reaction of CH<sub>2</sub>OO with I are reported as a function of pressure at 298 K. Measurements were made using pulsed laser flash photolysis of CH<sub>2</sub>I<sub>2</sub>/O<sub>2</sub>/N<sub>2</sub> gas mixtures coupled with time-resolved broadband UV absorption spectroscopy at pressures between 6 and 300 Torr. Results give a peak absorption cross-section of (1.37 ± 0.29) × 10<sup>-17</sup> cm<sup>2</sup> at ∼340 nm and a rate coefficient for the CH<sub>2</sub>OO self-reaction of (8.0 ± 1.1) × 10<sup>-11</sup> cm<sup>3</sup> s<sup>-1</sup>, with no significant pressure dependence of the absorption cross-sections or the self-reaction kinetics over the range investigated. The rate coefficient for the reaction between CH<sub>2</sub>OO and I demonstrates pressure dependence over the range investigated, with a Lindemann fit giving k<sub>0</sub> = (4.4 ± 1.0) × 10<sup>-29</sup> cm<sup>6</sup> s<sup>-1</sup> and k<sub>∞</sub> = (6.7 ± 0.6) × 10<sup>-11</sup> cm<sup>3</sup> s<sup>-1</sup>. The origins of IO in the system have been investigated, the implications of which are discussed.

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