On the exclusion of an astrophysical solution to the solar neutrino problem.

Details On the exclusion of an astrophysical solution to the solar neutrino problem. On the exclusion of an astrophysical solution to the solar neutrino problem.

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993eaas.book.....b&link_type=abstract

On the exclusion of an astrophysical solution to the solar neutrino problem., by Berezinsky, V.. Bonn Univ. (Germany), Dec 1993

Astronomy and Astrophysics

Astrophysics

Scientific paper

The exclusion of astrophysical solution of the solar neutrino problem is reviewed and analysed. The crucial element of the analysis is the ratio of data of the Homestake to the Kamiokande experiments. An astrophysical solution is shown to be excluded unless the ν37Cl-cross-section is considerably underestimated or unless there are large systematic errors in the Homestake or Kamiokande experiments. New astrophysical phenomena, not included in the Standard Solar Model (SSM) and uncertainties in the nuclear rates in the core of the Sun cannot explain the observed data of the Homestake and Kamiokande detectors simultaneously. This implies neutrino oscillations as the solution to the solar neutrino problem and thus as the first evidence for a phenomenon beyond the Standard Model.

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