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Branches of {sup 33}S(p,{gamma}){sup 34}Cl at oxygen-neon nova temperatures

Journal Article · · Physical Review. C, Nuclear Physics
; ; ; ; ;  [1];  [2]
  1. Department of Physics, University of Washington, Seattle, Washington 98195-1560 (United States)
  2. Physik Department E12, Technische Universitaet Muenchen, D-85748 Garching (Germany)
Recent simulations of classical novae on oxygen-neon white-dwarf stars indicate that the isotopic ratio {sup 32}S/{sup 33}S has the potential to be a remarkable indicator of presolar grains of nova origin. The {sup 33}S(p,{gamma}){sup 34}Cl reaction influences this ratio directly by destroying {sup 33}S in novae. Additionally, {beta}-delayed {gamma} rays from the metastable state of {sup 34}Cl (t{sub 1/2}=32 min) have been suggested to be potential nova observables. We have measured the branches for known {sup 33}S(p,{gamma}){sup 34}Cl resonances that are activated at temperatures relevant to oxygen-neon novae. We provide the first reliable uncertainties on these branches and the first upper limits for several previously unmeasured branches.
OSTI ID:
21499645
Journal Information:
Physical Review. C, Nuclear Physics, Journal Name: Physical Review. C, Nuclear Physics Journal Issue: 4 Vol. 83; ISSN 0556-2813; ISSN PRVCAN
Country of Publication:
United States
Language:
English