Solar neutrino observations with the Homestake 37Cl detector

Details Solar neutrino observations with the Homestake 37Cl detector Solar neutrino observations with the Homestake 37Cl detector

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..243.1122l&link_type=abstract

Intersections between particle and nuclear physics. AIP Conference Proceedings, Volume 243, pp. 1122-1133 (1992).

Physics

Nuclear Physics

10

Lepton-Induced Reactions, 20<=A<=38

Scientific paper

The continuous twenty year record of these measurements of the solar neutrino flux with the Homestake chlorine detector, indicates that the average solar neutrino flux is 2.2+/-0.3 SNU and that this νe flux appears to vary with the 11 year solar activity cycle. Higher νe fluxes are observed during solar quiet periods and lower νe fluxes during solar active periods. When the Homestake data is combined with the Kamiokande results, the region of overlap between the two experiments is for an observed to predicted 8B neutrino flux ratio of about 0.4 and very little low energy neutrino flux. If the Kamiokande results are corrected for MSW effects, neutral current scatterings by non-electron neutrinos, then both the 8B and the 7Be fluxes are about 1/3 of the Standard Solar Model predictions.

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