Reanalysis of Rate Data for the Reaction CH<sub>3</sub> + CH<sub>3</sub> → C<sub>2</sub>H<sub>6</sub> Using Revised
Cross Sections and a Linearized Second-Order Master Equation
posted on 2015-07-16, 00:00authored byM. A. Blitz, N. J.
B. Green, R. J. Shannon, M. J. Pilling, P. W. Seakins, C. M. Western, S. H. Robertson
Rate
coefficients for the CH<sub>3</sub> + CH<sub>3</sub> reaction,
over the temperature range 300–900 K, have been corrected for
errors in the absorption coefficients used in the original publication
(Slagle et al., J. Phys. Chem. 1988, 92, 2455−2462). These corrections necessitated the development
of a detailed model of the B̃<sup>2</sup>A<sub>1</sub>′
(3s)–X̃<sup>2</sup>A<sub>2</sub>″ transition in
CH<sub>3</sub> and its validation against both low temperature and
high temperature experimental absorption cross sections. A master
equation (ME) model was developed, using a local linearization of
the second-order decay, which allows the use of standard matrix diagonalization
methods for the determination of the rate coefficients for CH<sub>3</sub> + CH<sub>3</sub>. The ME model utilized inverse Laplace transformation
to link the microcanonical rate constants for dissociation of C<sub>2</sub>H<sub>6</sub> to the limiting high pressure rate coefficient
for association, <i>k</i><sub>∞</sub>(<i>T</i>); it was used to fit the experimental rate coefficients using the
Levenberg–Marquardt algorithm to minimize χ<sup>2</sup> calculated from the differences between experimental and calculated
rate coefficients. Parameters for both <i>k</i><sub>∞</sub>(<i>T</i>) and for energy transfer ⟨Δ<i>E</i>⟩<sub>down</sub>(<i>T</i>) were varied
and optimized in the fitting procedure. A wide range of experimental
data were fitted, covering the temperature range 300–2000 K.
A high pressure limit of <i>k</i><sub>∞</sub>(<i>T</i>) = 5.76 × 10<sup>–11</sup>(<i>T</i>/298 K)<sup>−0.34</sup> cm<sup>3</sup> molecule<sup>–1</sup> s<sup>–1</sup> was obtained, which agrees well with the best
available theoretical expression.