The 14N(7Be,8B)13C reaction and the 7Be(p,γ)8B S factor

Details The 14N(7Be,8B)13C reaction and the 7Be(p,γ)8B S factor The 14N(7Be,8B)13C reaction and the 7Be(p,γ)8B S factor

Nov 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999phrvc..60e5803a&link_type=abstract

Physical Review C (Nuclear Physics), Volume 60, Issue 5, November 1999, id. 055803

Physics

Nuclear Physics

34

Transfer Reactions, Solar Neutrinos, Hydrostatic Stellar Nucleosynthesis, Elastic Scattering

Scientific paper

The 14N(7Be,8B)13C reaction was studied using an 85 MeV 7Be radioactive beam. The asymptotic normalization coefficients for the virtual transitions 7Be+p<-->8B were determined from the measured cross section. These coefficients specify the amplitude of the tail of the 8B overlap function in the 7Be+p channel, and were used to calculate the astrophysical S factor for the direct capture reaction 7Be(p,γ)8B at solar energies S17(0). We find that S17(0)=16.6+/-1.9 eV b.

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