Abstract
Neutrino oscillations as solutions of the solar neutrino problems and the atmospheric neutrino deficits may restrict neutrino mass squared differences and mixing angles in the three-neutrino mixing scheme. Currently we have several solutions depending on the interpretation of the solar neutrino problem. Combining the neutrino oscillation solutions and a mass matrix ansatz, we investigate the neutrino mass bounds and find a possible leptonic (Formula presented)-violating rephasing-invariant quantity (Formula presented) for the large mixing angle MSW and just-so vacuum oscillation solutions, and (Formula presented) for the small mixing angle MSW solution.
| Original language | English |
|---|---|
| Pages (from-to) | 7 |
| Number of pages | 1 |
| Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |
| Volume | 62 |
| Issue number | 7 |
| DOIs | |
| State | Published - 2000 |
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