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 (Tc). If the Sun is 2% cooler of 3% warmer than predicted by SSMs, the MSW parameters we determine are consistent with different grand unified theories.
Original language | English (US) |
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Pages (from-to) | 156-160 |
Number of pages | 5 |
Journal | Nuclear Physics B (Proceedings Supplements) |
Volume | 31 |
Issue number | C |
DOIs | |
State | Published - Apr 1993 |
All Science Journal Classification (ASJC) codes
- Atomic and Molecular Physics, and Optics
- Nuclear and High Energy Physics