Diffusion Monte Carlo Calculations of Minimum Energy Paths for the Isotopic Variants of the CH3+ + H2 ← CH5+ ←→ CH3+ + H2 Reaction

Astronomy and Astrophysics – Astrophysics

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Protonated methane is of interest to astrochemists due to its presumed importance as a reaction intermediate in the reaction involving CH3+ + HD within the interstellar medium. However, within the interstellar medium there is a nonstatistical H/D isotopic abundance observed for the isotopologues of CH3+. Kinetic studies performed by Gerlich and co-workers determined that the reactions CH3-nDn+ + HD → CH4-nDn+1+ → CH2-nDn+1+ + H_2 have identical net rate constants regardless of the value of n.
We have calculated zero-point corrected energies and wave functions of the CH3+ + H2 system and its deuterated analogs as functions of the center of mass separation between CH3+ and H2, R. We can divide these simulations into distinct ranges of R; long-range interactions, complexation, and intermediate distances. Analysis of the wave functions associated with these three ranges of R allows us to study how zero-point energy influences the approach geometries that are sampled during low-energy collisions.
O. Asvany, S. Schlemmer, D. Gerlich, Astrophys. J. 617, 685 (2004).
C. E. Hinkle, A. B. McCoy, J. Phys. Chem. Lett. 1, 562 (2010).

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