Phys. Rev. C 60, 055803 (1999) [5 pages]The 14N(7Be,8B)13C reaction and the 7Be(p,γ)8B S factorReceived 20 July 1999; published 8 October 1999 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. © 1999 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevC.60.055803
DOI:
10.1103/PhysRevC.60.055803
PACS:
25.60.Je, 26.65.+t, 26.20.+f, 25.60.Bx
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