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arxiv: astro-ph/9909317 · v3 · submitted 1999-09-17 · 🌌 astro-ph · nucl-ex· nucl-th

A Measurement of the Coulomb Dissociation of 8B at 254 MeV/nucleon and the 8B Solar Neutrino Flux

classification 🌌 astro-ph nucl-exnucl-th
keywords nucleoncoulombdissociationfactoradoptedagreesastrophysicalcoulomb-dissociation
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We have measured the Coulomb dissociation of 8B into 7Be and proton at 254 MeV/nucleon using a large-acceptance focusing spectrometer. The astrophysical S17 factor for the 7Be(p,gamma)8B reaction at E{c.m.} = 0.25-2.78 MeV is deduced yielding S17(0)=20.6 \pm 1.2 (exp.) \pm 1.0 (theo.) eV-b. This result agrees with the presently adopted zero-energy S17 factor obtained in direct-reaction measurements and with the results of other Coulomb-dissociation studies performed at 46.5 and 51.2 MeV/nucleon.

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