Probing the neutrino mass matrix in next generation neutrino oscillation experiments

Abstract

We review the current status of the neutrino mass and mixing parameters needed to reconstruct the neutrino mass matrix. A comparative study of the precision in the measurement of oscillation parameters expected from the next generation solar, atmospheric, reactor and accelerator based experiments is presented. We discuss the potential of $0\nu \beta \beta$ experiments in determining the neutrino mass hierarchy and the importance of a better ${\theta }_{12}$ measurement for it.

Prepared for 5th International Conference on Non-accelerator New Physics (NANP 05), Dubna, Russia, 20-25 Jun 2005

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• Turbulent Supernova Shock Waves and the Sterile Neutrino Signature in Megaton Water Detectors
• Low and High Energy Phenomenology of Quark-Lepton Complementarity Scenarios
• Probing neutrino oscillations from supernovae shock waves via the IceCube detector
• Optimizing the greenfield Beta-beam
• Unraveling neutrino parameters with a magical beta-beam experiment at INO
• Confusing Sterile Neutrinos with Deviation from Tribimaximal Mixing at Neutrino Telescopes
• On Probing theta_{23} in Neutrino Telescopes
• Large and Almost Maximal Neutrino Mixing within the Type II See-Saw Mechanism
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• Solar Model Parameters and Direct Measurements of Solar Neutrino Fluxes
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• Magic Baseline Beta Beam
• The effect of primordial fluctuations on neutrino oscillations
• Getting Information on |U_{e3}|^2 from Neutrino-less Double Beta Decay