Abstract
Flavor changing (FC) neutrino-matter interactions can account for the zenith-angle-dependent deficit of atmospheric neutrinos observed in the SuperKamiokande experiment, without directly invoking either neutrino mass or mixing. We find that FC νπ-matter interactions provide a good fit to the observed zenith angle distributions, comparable in quality to the neutrino oscillation hypothesis. The required FC interactions arise naturally in many attractive extensions of the standard model.
| Original language | English |
|---|---|
| Pages (from-to) | 3202-3205 |
| Number of pages | 4 |
| Journal | Physical Review Letters |
| Volume | 82 |
| Issue number | 16 |
| DOIs | |
| State | Published - 1999 |
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