Abstract
Differential cross sections and excitation functions for the reaction 63Cu(α, p) 66Zn have been measured over the energy range E α = 6–10 MeV. Results of statistical model calculations are compared to the excitation functions for individual proton groups and are found to give good representations to within about a factor of two. The data and the calculated cross sections are used to determine the thermonuclear reaction rates for temperatures of astrophysical interest.
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