Abstract
The most general, renormalizable Lagrangian that includes massive neutrinos contains "right-handed neutrino" Majorana masses of order M. While there are prejudices in favor of M Mweak, virtually nothing is known about the magnitude of M. I argue that the Liquid Scintillator Neutrino Detector (LSND) anomaly provides, currently, the only experimental hint: M∼1eV. If this is the case, the LSND mixing angles are functions of the active neutrino masses and mixing and, remarkably, adequate fits to all data can be naturally obtained. I also discuss consequences of this "eV-seesaw" for supernova neutrino oscillations, tritium beta-decay, neutrinoless double-beta-decay, and cosmology.
Original language | English (US) |
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Article number | 033005 |
Pages (from-to) | 1-5 |
Number of pages | 5 |
Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |
Volume | 72 |
Issue number | 3 |
DOIs | |
State | Published - Aug 1 2005 |
ASJC Scopus subject areas
- Nuclear and High Energy Physics
- Physics and Astronomy (miscellaneous)