Astrophysical Reaction Rates as a Challenge for Nuclear Reaction Theory
The relevant energy ranges for stellar nuclear reactions are introduced. Low-energy compound and direct reactions are discussed. Stellar modifications of the cross sections are presented. Implications for experiments are outlined.
Published in10th Int Symposium on Origin of Matter and Evolution of Galaxies
RelationsSchool of Physics, Astronomy and Mathematics
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Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn Skakun, Ye; Rauscher, T. (EDP Sciences, 2008)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 ...
Skakun, Ye; Rauscher, T. (American Institute of Physics, 2010)Astrophysical S-factors of (p,n) reactions on (99)Ru, (100)Ru, (101)Ru, and (102)Ru were derived from the sum of experimental isomeric and ground states cross sections measured in the incident proton energy range of 5-9 ...
Tables of nuclear cross sections and reaction rates : An addendum to the paper "Astrophysical reaction rates from statistical model calculations" Rauscher, T.; Thielemann, Friedrich-Karl (2001-09)In a previous publication (ATOMIC DATA AND NUCLEAR DATA TABLES 75, 1 (2000)), we gave seven-parameter analytical fits to theoretical reaction rates derived from nuclear cross sections calculated in the statistical model ...