Solar neutrinos from the decay of B8

John N. Bahcall and Barry R. Holstein
Phys. Rev. C 33, 2121 – Published 1 June 1986
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Abstract

The spectrum of neutrinos produced by the beta decay of B8 in the sun is computed including forbidden corrections to the weak interactions. The total cross section for absorption by Cl37 of B8 neutrinos is (1.06±0.1)×1042 cm2. The uncertainty is determined by calculating the cross section using different measured spectra for the alpha particles that result from the decay of B8 to Be8 and by varying the transition matrix elements consistent with the branching ratios measured using delayed protons emitted in the beta decay of Ca37.

  • Received 27 January 1986

DOI:https://doi.org/10.1103/PhysRevC.33.2121

©1986 American Physical Society

Authors & Affiliations

John N. Bahcall

  • Institute for Advanced Study, Princeton, New Jersey 08540

Barry R. Holstein

  • Princeton University, Princeton, New Jersey 08540

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Issue

Vol. 33, Iss. 6 — June 1986

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