GUT Model Predictions for Neutrino Oscillation Parameters Compatible with the Large Mixing Angle Solar Solution
arXiv:hep-ph/0108070 · doi:10.1103/PhysRevD.65.073004
Abstract
Within the framework of an SO(10) GUT model that can accommodate both the atmospheric and the LMA solar neutrino mixing solutions, we present explicit predictions for the neutrino oscillation parameters \sin^2 2θ_{13}, \sin^2 2θ_{12}, \sin^2 2θ_{23}, and Δm^2_{21}. Precise measurements of \sin^2 2θ_{12} and Δm^2_{21} by KamLAND can be used to precisely determine the GUT model parameters. We find that the model can then be tested at Neutrino Superbeams and Neutrino Factories with precision neutrino oscillation measurements of \sin^2 2θ_{23}, \sin^2 2θ_{13}, and the leptonic CP phase δ_{CP}.
22 pages, 7 figures, title changed, CP phase results and figures corrected and Majorana phase predictions included, along with expanded explanation of the applied phase transformations
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- An SO(10) GUT Model With Lopsided Mass Matrix and Neutrino Mixing Angle theta_13
- Lepton Flavor Violation in the SUSY-GUT Models with Lopsided Mass Matrix
- Leptogenesis in Realistic SO(10) Models
- Neutrino Mass Models
- Lifting a Realistic SO(10) Grand Unified Model to Five Dimensions
- Resource Letter: The Standard Model and Beyond
- The Origin of Mass
- GUT Implications from Neutrino Mass