Expressions for a K-adiabatic master equation for a bimolecular recombination rate constant krec are derived for a bimolecular reaction forming a complex with a single well or complexes with multiple well, where K is the component of the total angular momentum along the axis of least moment of inertia of the recombination product. The K-active master equation is also considered. The exact analytic solutions, i.e., the K-adiabatic and K-active steady-state population distribution function of reactive complexes, g(EJK) and g(EJ), respectively, are derived for the K-adiabatic and K-active master equation cases using properties of inhomogeneous integral equations (Fredholm type). The solutions accommodate arbitrary intermolecular energy transfer models, e.g., the single exponential, double exponential, Gaussian, step-ladder, and near-singularity models. At the high pressure limit, the krec for both the K-adiabatic and K-active master equations reduce, respectively, to the K-adiabatic and K-active bimolecular Rice–Ramsperger–Kassel–Marcus theory (high pressure limit expressions). Ozone and its formation from O + O2 are known to exhibit an adiabatic K. The ratio of the K-adiabatic to the K-active recombination rate constants for ozone formation at the high pressure limit is calculated to be ∼0.9 at 300 K. Results on the temperature and pressure dependence of the recombination rate constants and populations of O3 will be presented elsewhere.
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28 March 2016
Research Article|
March 29 2016
Bimolecular recombination reactions: K-adiabatic and K-active forms of the bimolecular master equations and analytic solutions
Nima Ghaderi
Nima Ghaderi
Noyes Laboratory of Chemical Physics,
California Institute of Technology
, 1200 E. California Blvd., Pasadena, California 91125, USA
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J. Chem. Phys. 144, 124114 (2016)
Article history
Received:
October 13 2015
Accepted:
March 03 2016
Citation
Nima Ghaderi; Bimolecular recombination reactions: K-adiabatic and K-active forms of the bimolecular master equations and analytic solutions. J. Chem. Phys. 28 March 2016; 144 (12): 124114. https://doi.org/10.1063/1.4944082
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