Abstract
In this talk we present our results on the seasonal variation of the solar neutrino flux in the context of the MSW solutions to the solar neutrino problem due to the non-zero latitude at the Super-Kamiokande site. We calculate this seasonal dependence and compare it with the expectations in the no-oscillation case as well as just-so scenario, in the light of the latest Super-Kamiokande 708-day data. The seasonal dependence can be sizeable in the large mixing angle MSW solution and would be correlated with the day-night effect.
| Original language | English |
|---|---|
| Pages (from-to) | 89-94 |
| Number of pages | 6 |
| Journal | Nuclear Physics B - Proceedings Supplements |
| Volume | 81 |
| Issue number | 1-3 |
| DOIs | |
| State | Published - Feb 2000 |
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