Multireference configuration interaction study of the predissociation of C via its state
arXiv:2206.03540 · doi:10.1063/5.0097451
Abstract
Photodissociation is one of the main destruction pathways for dicarbon (C) in astronomical environments such as diffuse interstellar clouds, yet the accuracy of modern astrochemical models is limited by a lack of accurate photodissociation cross sections in the vacuum ultraviolet range. C features a strong predissociative electronic transition near 130 nm originally measured in 1969; however, no experimental studies of this transition have been carried out since, and theoretical studies of the state are limited. In this work, potential energy curves of excited electronic states of C are calculated with the aim of describing the predissociative nature of the state and providing new ab initio photodissociation cross sections for astrochemical applications. Accurate electronic calculations of 56 singlet, triplet, and quintet states are carried out at the DW-SA-CASSCF/MRCI+Q level of theory with a CAS(8,12) active space and the aug-cc-pV5Z basis set augmented with additional diffuse functions. Photodissociation cross sections arising from the vibronic ground state to the state are calculated by a coupled-channel model. The total integrated cross section through the and bands is 1.19810cmcm, giving rise to a photodissociation rate of 5.0210 s under the standard interstellar radiation field, much larger than the rate in the Leiden photodissociation database. In addition, we report a new state that should be detectable via a strong band around 116 nm.
33 pages, 13 figures; Accepted by The Journal of Chemical Physics
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