Astrophysical Reaction Rates as a Challenge for Nuclear Reaction Theory
arXiv:1005.4611 · doi:10.1063/1.3485143
Abstract
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.
8 pages, 2 figures; invited talk at OMEG10, March 2010. To appear in the OMEG10 proceedings published by AIP