Understanding the kinetics of the HCN system is critical
to several
disciplines in science and engineering, including interstellar chemistry,
atmospheric reentry, and combustion, to name a few. This paper constructs
a rovibrational state-specific kinetic mechanism for the HCN system,
leveraging electronic structure calculations, classical scattering
dynamics, and state-to-state kinetics. To this aim, three accurate
potential energy surfaces (PESs), 1
A′, 3
A′, and 3
A″, are constructed using multireference configuration interaction
(MRCI) calculations for a comprehensive arrangement of the nuclei.
Quasi-classical scattering calculations provide elementary reaction
rate constants resulting from the interaction between the CN, CH,
and NH molecules with H, N, and C atoms, respectively. The rovibrational
collisional model developed comprises 50 million bound–bound
and free-bound collisional processes. This model is used to study
the dynamics of energy transfer and dissociation in an isochoric and
isothermal chemical reactor via the solution of the
master equation for a wide temperature range from 1000 to 10,000 K.
This study unravels the dynamics of dissociation of the molecules
in the HCN system, which the PESs primarily control via the formation of short-lived intermediates that shortcut the dissociation
pathway. The exchange processes in CH and NH enhance the dissociation
by over 80%. The importance of exchange processes is also highlighted
in comparing the quasi-steady state and thermal dissociation rates
with state-of-the-art rate models and experimental fits.