Simple Model for (3+2) Neutrino Oscillations
arXiv:hep-ph/0312285 · doi:10.1016/j.physletb.2004.03.086
Abstract
We formulate a set of naturalness criteria for sterile neutrinos (ν') to be light, needed for reconciling the LSND neutrino anomaly with the other neutrino data. A light sterile neutrino becomes as natural as the light active neutrinos if it carries quantum numbers of a chiral gauge symmetry broken at the TeV scale. The simplest such theory is shown to be an SU(2) gauge theory with the ν' transforming as a spin 3/2 multiplet. We develop this model and show that it leads naturally to the phenomenologically viable (3+2) neutrino oscillation scheme. We also present next-to-minimal models for light sterile neutrinos based on a chiral U(1) gauge symmetry.
12 pages in LaTeX, typos corrected, reference added
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- Naturally light right-handed neutrinos in a 3-3-1 Model
- Anomaly-Free Sets of Fermions
- General solution to the U(1) anomaly equations
- Exotic Charges, Multicomponent Dark Matter and Light Sterile Neutrinos
- MiniBooNE Results and Neutrino Schemes with 2 sterile Neutrinos: Possible Mass Orderings and Observables related to Neutrino Masses
- Constraining Mass Spectra with Sterile Neutrinos from Neutrinoless Double Beta Decay, Tritium Beta Decay and Cosmology
- Chiral Gauge Models for Light Sterile Neutrinos
- Sterile Neutrinos and Global Symmetries
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- Influence of a keV sterile neutrino on neutrino-less double beta decay -- how things changed in the recent years
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- Avoiding BBN Constraints on Mirror Models for Sterile Neutrinos
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- model with symmetry for activesterile neutrino mixing
- Active-sterile neutrino mixing in the absence of bare active neutrino mass
- Multichannel oscillations and relations between LSND, KARMEN and MiniBooNE, with and without CP violation
- Simple Theory of Chiral Fermion Dark Matter
- Anomaly-free chiral and its scotogenic implication
- Measuring the mass of a sterile neutrino with a very short baseline reactor experiment
- Neutrino Self-Interactions
- Chiral dark matter and radiative neutrino masses from gauged U(1) symmetry
- TeV-scale gravity in Horava-Witten theory on a compact complex hyperbolic threefold
- Local demands on sterile neutrinos
- Neutrino oscillations, and the origin of pulsar velocities and dark matter