Atomic oxygen in its first excited singlet state, O(D), is an important species in the photochemistry of several planetary atmospheres and has been predicted to be a potentially important reactive species on interstellar ices. Here, we report the results of a kinetic study of the reactions of O(D) with methanol, CHOH, and acetonitrile, CHCN, over the 50-296 K temperature range. A continuous supersonic flow reactor is used to attain these low temperatures coupled with pulsed laser photolysis and pulsed laser-induced fluorescence to generate and monitor O(D) atoms, respectively. Secondary experiments examining the atomic hydrogen product channels of these reactions are also performed, through laser-induced fluorescence measurements of H(S) atom formation. On the kinetic side, the rate constants for these reactions are seen to be large (>2 × 10 cm s) and consistent with barrierless reactions, although they display contrasting dependences as a function of temperature. On the product formation side, both reactions are seen to yield non-negligible quantities of atomic hydrogen. For the O(D) + CHOH reaction, the derived yields are in good agreement with the conclusions of previous experimental and theoretical works. For the O(D) + CHCN reaction, whose H-atom formation channels had not previously been investigated, electronic structure calculations of several new product formation channels are performed to explain the observed H-atom yields. These calculations demonstrate the barrierless and exothermic nature of the relevant exit channels, confirming that atomic hydrogen is also an important product of the O(D) + CHCN reaction.

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http://dx.doi.org/10.1021/acs.jpca.2c01946DOI Listing

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