Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn

Skakun, Ye and Rauscher, T. (2008) Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn. In: Int Conf on Nuclear Data for Science and Technology :. EDP Sciences, FRA, pp. 1325-1327. ISBN 978-2-7598-0091-9
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Astrophysical S-factors and reaction rates were derived from available cross sections of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn isotopes at incident proton energies up to 9 MeV. The statistical theory predictions of the observable quantities are similar to 2 times smaller at near threshold energies and have better agreement at higher energies.


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