Properties of Mg26 and Si26 in the sd shell model and the determination of the Al25(p,γ)Si26 reaction rate

Details Properties of Mg26 and Si26 in the sd shell model and the determination of the Al25(p,γ)Si26 reaction rate Properties of Mg26 and Si26 in the sd shell model and the determination of the Al25(p,γ)Si26 reaction rate

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011phrvc..83f5803r&link_type=abstract

Physical Review C, vol. 83, Issue 6, id. 065803

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5

Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Coulomb Energies, Shell Model, Radiative Capture

Scientific paper

We present theoretical results for the Al25(p,γ)Si26 resonance-capture rate. The isobaric mass multiplet equation is used to determine the energies and Jπ values of states in Si26 based upon those observed in Mg26 and Al26 together with sd shell calculations for the c coefficients. Three Hamiltonians for the sd shell, USD, USDA and USDB, are used to estimate the theoretical uncertainties in the γ-decay and proton-decay widths that go into the resonance-capture rate.

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