Review of Experimental Data on Alpha-Induced Reactions on Some Nuclei (Mg-24, Si-28, S-32, Ar-36, Ca-40) in Terms of Astrophysical Applications

Details Review of Experimental Data on Alpha-Induced Reactions on Some Nuclei (Mg-24, Si-28, S-32, Ar-36, Ca-40) in Terms of Astrophysical Applications Review of Experimental Data on Alpha-Induced Reactions on Some Nuclei (Mg-24, Si-28, S-32, Ar-36, Ca-40) in Terms of Astrophysical Applications

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..769.1386d&link_type=abstract

INTERNATIONAL CONFERENCE ON NUCLEAR DATA FOR SCIENCE AND TECHNOLOGY. AIP Conference Proceedings, Volume 769, pp. 1386-1389 (200

Physics

Nuclear Physics

1

3H-, 3He-, And 4He-Induced Reactions, 20<=A<=38, 39<=A<=58, Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments

Scientific paper

The present report gives a detailed analysis of experimental works and a review of alpha-induced reaction cross-section data of five alpha-alpha nuclei, Mg-24, Si-28, S-32, Ar-36 and Ca-40, for incident alpha energy up to 20 MeV. Alpha-induced reactions play an important role in the helium burning stage of stars, novae, and supernovae. These reactions are basic to the CNO and Al-Mg cycles, and also to the production of neutrons producing S and R processes occurring in stars. Thus, the availability of cross-section data for these reactions is a prime need for the study of nuclear interactions taking place in stars.
These data have been compiled as part of an international collaboration, funded in part by the Civilian Research & Development Foundation, and are available in the EXFOR databases.

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