Theory of Neutrino Masses and Mixings

Abstract

Neutrino physics is going through a revolutionary progress. In this talk I review what we have learned and why neutrino mass is so important. Neutrino masses and mixings are already shedding new insight into the origin of flavor. Given the evidences for neutrino mass, leptogenesis is gaining momentum as the origin of cosmic baryon asymmetry. Best of all, we will learn a lot more in the coming years.

Talk at Lepton Photon 2001. 18 pages, LaTeX2e, uses ws-p10x7.cls

References in corpus (7)

• Leptogenesis from $\tilde{N}$-dominated early universe
• Global Analysis of Solar Neutrino Oscillations Including SNO CC Measurement
• Model-dependent and independent implications of the first Sudbury Neutrino Observatory results
• Interpreting the LSND anomaly: sterile neutrinos or CPT-violation or...?
• Global analysis of Solar neutrino oscillation evidence including SNO and implications for Borexino
• Erratum for "Supersymmetric Electroweak Baryogenesis"
• E1 Working Group Summary: Neutrino Factories and Muon Colliders

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• Solar models and solar neutrino oscillations
• Massive Neutrinos and (Heterotic) String Theory
• Life, the universe, and everything - 42 fundamental questions
• Neutrino Physics
• Numerical consistency check between two approaches to radiative corrections for neutrino masses and mixings
• Discriminating neutrino mass models using Type II seesaw formula