Theoretical Implications of the Combined Solar Neutrino Observations

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

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High Energy Physics - Phenomenology

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http://salesiana.dossiersoluciones.com/handle/123456789/226506

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/hep-ph/9212241
 http://arxiv.org/abs/hep-ph/9212241
 Nucl.Phys.Proc.Suppl.31:156,1993
 doi:10.1016/0920-5632(93)90128-S

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arXiv