The reaction branching 31P(p, γ)/31P(p, α) in the RP-process

Details The reaction branching 31P(p, γ)/31P(p, α) in the RP-process The reaction branching 31P(p, γ)/31P(p, α) in the RP-process

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991nupha.533..153i&link_type=abstract

Nuclear Physics A, Volume 533, Issue 1, p. 153-169.

Physics

Nuclear Physics

11

Nuclear Reactions

Scientific paper

The reactions 31P(p, γ)32S and 31P(p, α)28Si have been studied in the energy range 280-620 keV to investigate the influence of low-energy resonances on the stellar reaction rates. Several new resonances have been observed and the resonance strengths for both reaction channels have been determined. The reaction rates have been calculated from the present results and are compared with the results of Hauser-Feshbach calculations.

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