Proton-decaying states in Mg22 and the nucleosynthesis of Na22 in novae
PHYSICAL REVIEW C(2003)
Abstract
Populating states in Mg-22 via the (p,t) reaction in inverse kinematics with a 55-MeV /nucleon Mg-24 beam, we have measured the proton-decay branching ratios of the levels at 5.96 MeV and 6.05 MeV and obtained an experimental upper limit on the branching ratio of the 5.71-MeV state. On the basis of the present and previous measurements, we assign spins and parities to the 5.96-MeV and 6.05-MeV states. We combine our branching ratios with independent measurements of the lifetimes of these states or their Ne-22 analogs to compute the resonance strengths and thereby the astrophysical rate of the Na-21(p,gamma)Mg-22 reaction. We perform hydrodynamic calculations of nova outbursts with this new rate and analyze its impact on Na-22 yields.
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Key words
Astrophysical Reaction Rates
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