Abstract

The rate constant for OH−(H2O)2+CH3I reaction was determined by selected ion flow tube (SIFT) experiments for temperatures in the range of 298–398K. It is found to be an order of magnitude smaller than the collision capture rate constant, a result substantially different than found previously for the OH−+CH3I and OH−(H2O)+CH3I reactions. The rate constants for these reactions are only ∼25% and ∼two times smaller, respectively, than their collision capture rate constants. Only two product ions are observed experimentally, i.e. I− and I−(H2O), and their respective percentage yields are 90:10 and 83:17 at 298 and 348K. The kinetics for the OH−(H2O)2+CH3I reaction were also studied by direct dynamics simulations using the DFT/B97-1/ECP/d electronic structure theory, the same theory used in previous direct dynamics simulations of the OH−+CH3I and OH−(H2O)+CH3I reactions. Simulations for OH−(H2O)2+CH3I at 387K give respective percentage yields of 91:9 for I− and I−(H2O), in good agreement with the experimental results. For both the experiments and simulations, the microsolvated ion I−(H2O)2 is not formed and the formation of I− dominates I−(H2O). For the OH−+CH3I and OH−(H2O)+CH3I reactions the experimental and direct dynamics simulation rate constants agree. However, this is not the case for OH−(H2O)2+CH3I, for which the simulation rate constant is 8–9 times larger than the experimental value. Comparisons of the experimental, simulation, and collision capture rate constants for the OH−(H2O)2+CH3I reaction indicate the height of the submerged SN2 barrier for the reaction is an important feature of its potential energy surface. The actual barrier is expected to be higher than the value given by the DFT/B97-1 calculations. In future work it will be important to perform higher level electronic structure calculations and establish an accurate value for this barrier. Preliminary calculations reported here indicate the barrier height is sensitive to the electronic structure method.

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