Non-Unitary Neutrino Propagation From Neutrino Decay
arXiv:1407.6631 · doi:10.1016/j.physletb.2015.01.002
Abstract
Neutrino propagation in space-time is not constrained to be unitary if very light states - lighter than the active neutrinos - exist into which neutrinos may decay. If this is the case, neutrino flavor-change is governed by a handful of extra mixing and "oscillation" parameters, including new sources of CP-invariance violation. We compute the transition probabilities in the two- and three-flavor scenarios and discuss the different phenomenological consequences of the new physics. These are qualitatively different from other sources of unitarity violation discussed in the literature.
8 pages, no figures
References in corpus (5)
- Unitarity of the Leptonic Mixing Matrix
- Status of Oscillation plus Decay of Atmospheric and Long-Baseline Neutrinos
- Neutrino Decays over Cosmological Distances and the Implications for Neutrino Telescopes
- Neutrino flux ratios at neutrino telescopes: The role of uncertainties of neutrino mixing parameters and applications to neutrino decay
- Cosmological neutrino mass detection: The best probe of neutrino lifetime
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- Analytic treatment of 3-flavor neutrino oscillation and decay in matter
- Neutrino non-radiative decay and the diffuse supernova neutrino background
- Effects of the Violation of the Equivalence Principle at DUNE
- violation due to a Majorana phase in two flavor neutrino oscillations with decays
- Majorana CP-violating phases and NSI effects in Neutrino Decay
- Majorana CP Violation Insights from Decaying Neutrinos