Lower Bounds on U_{e3}
arXiv:1010.1206 · doi:10.1103/PhysRevD.83.033002
Abstract
We give minimal values for the smallest lepton mixing parameter U_{e3}, applying 2-loop renormalization group equations in an effective theory approach. This is relevant in scenarios that predict an inverted neutrino mass spectrum with the smallest mass and U_{e3} being zero at tree level, a situation known to be preserved at 1-loop order. At 2-loop, U_{e3} is generated at a level of 10^{-12}-10^{-14}. Such small values are of interest in supernova physics. Corresponding limits for the normal mass ordering are several orders of magnitude larger. Our results show that U_{e3} can in general expected be to be non-zero.
5 pages, 2 figures. Matches published version
References in corpus (9)
- Double Beta Decay, Majorana Neutrinos, and Neutrino Mass
- Neutrino Mass Hierarchy and Stepwise Spectral Swapping of Supernova Neutrino Flavors
- Neutrino physics from precision cosmology
- Model Predictions for Neutrino Oscillation Parameters
- Scaling in the Neutrino Mass Matrix
- The smallest neutrino mass
- The discrete flavor symmetry D5
- Inverted Mass Hierarchy from Scaling in the Neutrino Mass Matrix: Low and High Energy Phenomenology
- Flavor Neutrino Masses giving sinθ_{13}=0