The electronic quenching of NO(A
2Σ+) with molecular partners occurs through
complex non-adiabatic
dynamics that occurs on multiple coupled potential energy surfaces.
Moreover, the propensity for NO(A
2Σ+) electronic quenching depends heavily on the strength and
nature of the intermolecular interactions between NO(A
2Σ+) and the molecular partner. In this
paper, we explore the electronic quenching mechanisms of three systems:
NO(A
2Σ+) + CH4, NO(A
2Σ+) + CH3OH, and NO(A
2Σ+) + CO2. Using EOM-EA-CCSD calculations, we rationalize
the very low electronic quenching cross-section of NO(A
2Σ+) + CH4 as well as the
outcomes observed in previous NO + CH4 photodissociation
studies. Our analysis of NO(A
2Σ+) + CH3OH suggests that it will undergo facile
electronic quenching mediated by reducing the intermolecular distance
and significantly stretching the O–H bond of CH3OH. For NO(A
2Σ+) + CO2, intermolecular attractions lead to a series of low-energy
ON–OCO conformations in which the CO2 is significantly
bent. For both the NO(A
2Σ+) + CH3OH and NO(A
2Σ+) + CO2 systems, we see evidence of the harpoon
mechanism and low-energy conical intersections between NO(A
2Σ+) + M and NO(X
2Π) + M. Overall, this work provides the first detailed
theoretical study on the NO(A
2Σ+) + M potential energy surface of each of these systems and
will inform future velocity map imaging experiments.