Astrophysical Reaction Rates as a Challenge for Nuclear Reaction Theory

Rauscher, T. (2010) Astrophysical Reaction Rates as a Challenge for Nuclear Reaction Theory. In: 10th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG10), 2010-03-08 - 2010-03-10.
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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.
Item Type Conference or Workshop Item (Other)
Keywords compound reactions, stellar enhancement factor, reaction rates, hauser-feshbach model, nucleosynthesis, neutron-capture, cross-section, direct reactions
Date Deposited 15 May 2025 16:32
Last Modified 11 Oct 2026 23:01

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