18F(α,p)21Ne Reaction: Neutron Source For r-Process In Supernovae

Details 18F(α,p)21Ne Reaction: Neutron Source For r-Process In Supernovae 18F(α,p)21Ne Reaction: Neutron Source For r-Process In Supernovae

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..819..581l&link_type=abstract

CAPTURE GAMMA-RAY SPECTROSCOPY AND RELATED TOPICS: 12th International Symposium. AIP Conference Proceedings, Volume 819, pp. 58

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2

3H-, 3He-, And 4He-Induced Reactions, 6<=A<=19, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments

Scientific paper

The reaction rate of 18F(α,p)21Ne has been studied using the inverse reaction 21Ne(p,α)18F. This has been measured by the activation method in the energy range of the relevant Gamow window. Experimental results will be discussed and compared with the results of Hauser-Feshbach calculations and previous measurements.

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