Physics
Scientific paper
Feb 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994sci...263..785s&link_type=abstract
Science, Volume 263, Issue 5148, pp. 785-787
Physics
95
Scientific paper
Knowledge of the abundance of H_3^+ is needed in interstellar and planetary atmospheric chemistry. An important destruction mechanism of H_3^+ is low-energy electron impact followed by dissociation, but estimates of the reaction rate span several orders of magnitude. As an attempt to resolve this uncertainty, the cross section for dissociative recombination of vibrationally cold H_3^+ has been measured with an ion storage ring down to collision energies below 1 millielectron volt. A rate coefficient of 1.15 x 10-7 cubic centimeters per second at 300 kelvin was deduced. The cross section scaled with collision energy according to E-1.15, giving the rate a temperature dependence of T-0.65.
Brostrom Lars
Danared Håkan
Datz Sheldon
Filevich A.
Källberg Anders
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