How Well Do We (and Will We) Know Solar Neutrino Fluxes and Oscillation Parameters?

Details How Well Do We (and Will We) Know Solar Neutrino Fluxes and Oscillation Parameters? How Well Do We (and Will We) Know Solar Neutrino Fluxes and Oscillation Parameters?

1995-12-20

arxiv.org/abs/hep-ph/9512378v1

Phys.Rev.D53:4211-4225,1996

Physics

High Energy Physics

High Energy Physics - Phenomenology

37 pages, uuencoded Z-compressed postscript file (with figures); Submitted to Physical Review D

Scientific paper

10.1103/PhysRevD.53.4211

Assuming neutrino oscillations occur, the pp electron neutrino flux is uncertain by at least a factor of two, the ${\rm ^8B}$ flux by a factor of five, and the ${\rm ^7Be}$ flux by a factor of forty-five. Calculations of the expected results of future solar neutrino experiments (SuperKamiokande, SNO, BOREXINO, ICARUS, HELLAZ, and HERON) are used to illustrate the extent to which these experiments will restrict the range of the allowed neutrino mixing parameters. We present an improved formulation of the ``luminosity constraint'' and show that at 95\% confidence limit this constraint establishes the best available limits on the rate of creation of pp neutrinos in the solar interior and provides the best upper limit to the ${\rm ^7Be}$ neutrino flux.

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