Theoretical Implications of the Combined Solar Neutrino Observations

Details Theoretical Implications of the Combined Solar Neutrino Observations Theoretical Implications of the Combined Solar Neutrino Observations

1992-12-08

arxiv.org/abs/hep-ph/9212241v2

Nucl.Phys.Proc.Suppl.31:156,1993

Physics

High Energy Physics

High Energy Physics - Phenomenology

(2 pages), UPR-531-T, Latex, 4 figures upon request. Revised version replacing hep-ph/9212241 which was missing macro esprc2.t

Scientific paper

10.1016/0920-5632(93)90128-S

Constraints on the core temperature of the Sun and on neutrino-oscillation parameters are obtained by comparing the combined Homestake, Kamiokande, SAGE and GALLEX solar neutrino data with Standard Solar Models (SSM) and with non-standard solar models parameterized by a phenomenological central temperature ($T_c$). If the Sun is 2\% cooler or 3\% warmer than predicted by SSMs, the MSW parameters we determine are consistent with different grand unified theories.

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