Theoretical Implications of the Combined Solar Neutrino Observations

Preprint

9 December 1992

preprint
Published by arXiv in arXiv

Abstract

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.

Keywords

OBSERVATIONS CONSTRAINTS
THEORETICAL IMPLICATIONS
STANDARD SOLAR MODELS
NEUTRINO OBSERVATIONS
COMBINED SOLAR
SOLAR NEUTRINO
COOLER
SSMS

All Related Versions

Version 1, 1992-12-09, ArXiv
Version 2, 1992-12-10, ArXiv
Published version: Nuclear Physics B - Proceedings Supplements, 31, 156.

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