Abstract
The dynamics of the three-body recombination of the Cs+ and Br− ions with the formation of products with the lowest internal energy in the presence of the neutral atoms R = Hg, Xe, and Kr as third bodies is studied. The efficiency of the process is characterized by the effectivity function, which represents the dependence of the internal energy of the nascent molecule on the ion encounter energy and the third body energy. The Hg and Xe atoms are demonstrated to exhibit similar efficiencies in stabilizing the CsBr molecules, significantly superior to that of the Kr atom. The effectivity of each third body as an acceptor of excess energy of the molecules formed in recombination is determined by the structure of the potential energy surface of the individual R-Cs+-Br− system, the masses of the third bodies, and the dynamics of three-body collisions leading to recombination.
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