Nuclear energy levels of ^31S and astrophysical implications

Details Nuclear energy levels of ^31S and astrophysical implications Nuclear energy levels of ^31S and astrophysical implications

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aps..dnp.jd005w&link_type=abstract

American Physical Society, 2007 Annual Meeting of the Division of Nuclear Physics, October 10-13,2007, abstract #JD.005

Physics

Nuclear Physics

Scientific paper

Nucleosynthesis in the mass range from silicon to calcium in oxygen-neon novae is heavily influenced by the unmeasured strength of the ^30P(p,γ)^31S reaction. We have studied the ^31P(^3He,t)^31S and ^31P(^3He,t)^31S^*(p)^30P reactions to measure resonance energies and proton branching ratios in the ^30 P + p system. Our results will be presented in the contexts of novae, x-ray bursts and oxygen burning in massive stars. A direct measurement of resonance strengths in the ^30P(p,γ)^ 31S reaction is planned for the future.

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