Theoretical Implications of the Combined Solar Neutrino Observations

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dc.creatorBludman, S. A.
dc.creatorHata, N.
dc.creatorKennedy, D. C.
dc.creatorLangacker, P. G.
dc.date1992-12-08
dc.date1992-12-10
dc.date.accessioned2026-07-07T13:02:37Z
dc.date.available2026-07-07T13:02:37Z
dc.descriptionConstraints 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.
dc.description(2 pages), UPR-531-T, Latex, 4 figures upon request. Revised version replacing hep-ph/9212241 which was missing macro esprc2.tex
dc.identifierhttps://arxiv.org/abs/hep-ph/9212241
dc.identifierhttp://arxiv.org/abs/hep-ph/9212241
dc.identifierNucl.Phys.Proc.Suppl.31:156,1993
dc.identifierdoi:10.1016/0920-5632(93)90128-S
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/226506
dc.subjectHigh Energy Physics - Phenomenology
dc.titleTheoretical Implications of the Combined Solar Neutrino Observations
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