Astrophysical Reaction Rates as a Challenge for Nuclear Reaction Theory
High Energy Astrophysical Phenomena
2015-05-19 v1 Solar and Stellar Astrophysics
Nuclear Experiment
Nuclear Theory
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.
Keywords
Cite
@article{arxiv.1005.4611,
title = {Astrophysical Reaction Rates as a Challenge for Nuclear Reaction Theory},
author = {T. Rauscher},
journal= {arXiv preprint arXiv:1005.4611},
year = {2015}
}
Comments
8 pages, 2 figures; invited talk at OMEG10, March 2010. To appear in the OMEG10 proceedings published by AIP