Evidence for Neutrino Mass: A Decade of Discovery

Details Evidence for Neutrino Mass: A Decade of Discovery Evidence for Neutrino Mass: A Decade of Discovery

2004-12-10

arxiv.org/abs/hep-ex/0412032v2

Physics

High Energy Physics

High Energy Physics - Experiment

Invited talk at SEESAW25: International Conference on the Seesaw Mechanism and Neutrino Mass, Paris, France, 10-11 June 2004

Scientific paper

Neutrino mass and mixing are amongst the major discoveries of recent years. From the observation of flavor change in solar and atmospheric neutrino experiments to the measurements of neutrino mixing with terrestrial neutrinos, recent experiments have provided consistent and compelling evidence for the mixing of massive neutrinos. The discoveries at Super-Kamiokande, SNO, and KamLAND have solved the long-standing solar neutrino problem and demand that we make the first significant revision of the Standard Model in decades. Searches for neutrinoless double-beta decay probe the particle nature of neutrinos and continue to place limits on the effective mass of the neutrino. Possible signs of neutrinoless double-beta decay will stimulate neutrino mass searches in the next decade and beyond. I review the recent discoveries in neutrino physics and the current evidence for massive neutrinos.

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