Structure of 22Mg and its implications for explosive nucleosynthesis

Details Structure of 22Mg and its implications for explosive nucleosynthesis Structure of 22Mg and its implications for explosive nucleosynthesis

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phrvc..63f5807c&link_type=abstract

Physical Review C, vol. 63, Issue 6, id. 065807

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Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Other Resonances, Transfer Reactions, 20<=A<=38

Scientific paper

The locations of 18Ne+α resonances have been measured as excited states in 22Mg using the 12C(16O,6He)22Mg reaction. Eighteen new levels were discovered in the range 0<=Ec.m.<=3 MeV above the 18Ne+α threshold. The 18Ne(α,p)21Na reaction rate in the temperature range 0.2<=T<=1.0 GK has been calculated using the results from the present measurements, and the implications for nuclear burning in explosive stellar scenarios are discussed. This study also yielded energy-level information on low-lying 21Na + p resonances of importance to the 21Na(p,γ)22Mg reaction, one of the key links in the NeNa cycles in novae.

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