Theoretical implications of the combined solar neutrino observations
| Autor: | Dallas C. Kennedy, Sidney A. Bludman, Paul Langacker, Naoya Hata |
|---|---|
| Rok vydání: | 1993 |
| Předmět: |
Physics
Nuclear and High Energy Physics Particle physics Solar neutrino SAGE High Energy Physics::Phenomenology FOS: Physical sciences Core temperature Atomic and Molecular Physics and Optics High Energy Physics - Phenomenology High Energy Physics - Phenomenology (hep-ph) Physics::Space Physics Astrophysics::Solar and Stellar Astrophysics High Energy Physics::Experiment Astrophysics::Earth and Planetary Astrophysics GALLEX |
| Zdroj: | Nuclear Physics B - Proceedings Supplements. 31:156-160 |
| ISSN: | 0920-5632 |
| DOI: | 10.1016/0920-5632(93)90128-s |
| Popis: | 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. Comment: (2 pages), UPR-531-T, Latex, 4 figures upon request. Revised version replacing hep-ph/9212241 which was missing macro esprc2.tex |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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