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Neutrino Mixing

2003/10/20 by Carlo Giunti, Giunti, Carlo, Marco Laveder +1
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #High Energy Physics - Experiment (hep-ex) #High Energy Physics - Phenomenology (hep-ph) #Nuclear Experiment (nucl-ex) #astro-ph #hep-ex #hep-ph #nucl-ex

paper · pdf · doi:10.48550/arxiv.hep-ph/0310238

54 pages; final version published in 'Developments in Quantum Physics - 2004', edited by F. Columbus and V. Krasnoholovets, Nova Science Publishers, Inc

arxiv created 2004/10/01 · arxiv updated 2009/12/01

Abstract

In this review we present the main features of the current status of neutrino physics. After a review of the theory of neutrino mixing and oscillations, we discuss the current status of solar and atmospheric neutrino oscillation experiments. We show that the current data can be nicely accommodated in the framework of three-neutrino mixing. We discuss also the problem of the determination of the absolute neutrino mass scale through Tritium beta-decay experiments and astrophysical observations, and the exploration of the Majorana nature of massive neutrinos through neutrinoless double-beta decay experiments. Finally, future prospects are briefly discussed.

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