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S17(0) determined from the Coulomb breakup of 83 MeV /nucleon 8B
Authors:Davids B  Anthony D W  Aumann T  Austin S M  Baumann T  Bazin D  Clement R R  Davids C N  Esbensen H  Lofy P A  Nakamura T  Sherrill B M  Yurkon J
Affiliation:National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, MI 48824, USA. davids@kvi.nl
Abstract:A kinematically complete measurement was made of the Coulomb dissociation of 8B nuclei on a Pb target at 83 MeV/nucleon. The cross section was measured at low relative energies in order to infer the astrophysical S factor for the 7Be(p,gamma)8B reaction. A first-order perturbation theory analysis including E1, E2, and M1 transitions was employed to extract the E1 strength relevant to neutrino-producing reactions in the solar interior. By fitting the measured cross section from E(rel) = 130 to 400 keV, we find S17(0) = 17.8(+1.4)(-1.2) eV b.
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