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) |
|---|---|
| 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