Constraints on Energy Independent Solutions of the Solar Neutrino Problem

Details Constraints on Energy Independent Solutions of the Solar Neutrino Problem Constraints on Energy Independent Solutions of the Solar Neutrino Problem

1996-12-04

arxiv.org/abs/hep-ph/9612243v1

Phys.Lett. B395 (1997) 69-75

Physics

High Energy Physics

High Energy Physics - Phenomenology

16 pages, no figures, REVTEX

Scientific paper

10.1016/S0370-2693(97)00017-8

We analyze the latest published solar neutrino data assuming an arbitrary neutrino oscillation/conversion mechanism suppresses the electron neutrino flux from the Sun independent of energy. For oscillations/transitions into active (sterile) neutrinos such mechanisms are ruled out at 99.96 (99.9997) % C.L. assuming the standard solar model by Bahcall and Pinnsoneault '95 correctly predicts all solar neutrino fluxes within their estimated uncertainties. Even if one allows for $^8{\rm B}$ and $^7{\rm Be}$ solar neutrino fluxes that are vastly different from the ones in contemporary standard solar models these mechanisms are strongly disfavored by the data.

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