Reaction rate for 31S(p,γ)32Cl and its influence on the SiP cycle in hot stellar hydrogen burning

Details Reaction rate for 31S(p,γ)32Cl and its influence on the SiP cycle in hot stellar hydrogen burning Reaction rate for 31S(p,γ)32Cl and its influence on the SiP cycle in hot stellar hydrogen burning

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvc..50.1185v&link_type=abstract

Physical Review C (Nuclear Physics), Volume 50, Issue 2, August 1994, pp.1185-1193

Physics

Nuclear Physics

12

Charge-Exchange Reactions, Radiative Capture, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, 20<=A<=38

Scientific paper

The excitation energies of the proton unbound states in 32Cl have been measured in the 32S(3He,t)32Cl charge exchange reaction with high accuracy. The partial widths of the unbound levels have been calculated to derive the resonance strengths of these states in the 31S(p,γ)32Cl reaction channel. The reaction rate for the 31S(p,γ)32Cl reaction has been calculated and is compared with previous estimates. The role of this reaction for the closure of the SiP cycle is discussed in terms of the temperature and density conditions in hot stellar hydrogen burning.

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