Abstract
The analysis of the energies and times of arrival of neutrino events in the Kamioka and Irvine-Michigan-Brookhaven detectors yields two mass groupings at 22 eV and the other at 4 eV, if all neutrinos were released rapidly at the supernova. A preliminary assignment of flavors to the neutrinos producing these events is attempted; this is beset with problems unless there is mixing and are emitted more copiously than e. Large statistical and systematic uncertainties necessitate caution in assessing this interpretation.
| Original language | English |
|---|---|
| Pages (from-to) | 1685-1687 |
| Number of pages | 3 |
| Journal | Physical Review D |
| Volume | 37 |
| Issue number | 6 |
| DOIs | |
| State | Published - 1988 |
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