“…Similar conclusions have been reached for the behavior of EEs at the surface of ice: while relaxation into a bulk solvated state is likely to be the ultimate fate of EEs initially attached to the ice surface, the kinetics of bulk solvation, at least below 150 K, is believed to be very slow (>1 ms) [3,13]. Based on the long lifetime of excess electrons at ice surfaces, it has been hypothesized that, in ice stratospheric clouds, excess electrons produced by cosmic rays, may catalyze some of the chemical reactions that lead to the formation of the radical halogen species responsible for the decomposition of ozone [2,3]. The relevance of this process to the depletion of the antarctic ozone is still under dispute [14 -16]; but its broader impact onto the rich electron-driven chemistry of condensed halogenated compounds is discussed, e.g., in [17].…”