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Astrophysical reaction rates as a challenge for nuclear reaction theory
Editor(s)
Tanihara, I and Shima, T and Ong, HJ and Tamii, A and Kishimoto, T and Toki, H and Kajino, T and Kubono, S
Book title (Conference Proceedings)
The 10th International Symposium on Origin of Matter and Evolution of Galaxies
Volume
1269
Place of Conference
10th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG10), Osaka, JAPAN, MAR 08-10, 2010
Publisher
AIP Press
Place of Publication
Woodbury, NY
Pages
S. 247-254
ISSN/ISBN
978-0-7354-0819-7
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.
