The astrophysical S-factor for the ^7Be(p,γ)^8B reaction, and implications for neutrino physics

Details The astrophysical S-factor for the ^7Be(p,γ)^8B reaction, and implications for neutrino physics The astrophysical S-factor for the ^7Be(p,γ)^8B reaction, and implications for neutrino physics

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..nws.h1001s&link_type=abstract

American Physical Society, Fourth Annual Meeting of the Northwest Section, abstract #H1.001

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Until recently, the S-factor S_17(0) for the ^7Be(p,γ)^8B reaction contributed the largest single uncertainty to solar model calculations of the neutrino flux from decay of ^8B in the Sun. A new experiment(A.R. Junghans et al., Phys. Rev. Lett. 88), 041101-1 (2002), and to be published, together with other recent experiments, is leading to a much-improved determination of S_17(0). The importance of this result for neutrino physics will be discussed.

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