Neutrino Physics aPaul Langacker1, bJens Erler2, and bEduardo Peinado3 aDepartment of Physics, University of Pennsylvania, Philadelphia, PA 19104, USA bInstituto de F´ısica, Universidad Nacional Aut´onoma de M´exico, 01000 M´exico D.F., M´exico Abstract The theoretical and experimental bases of neutrino mass and mixing are reviewed. A brief chronological evolution of the weak interactions, the electroweak Standard Model, and neutrinos is presented. Dirac and Majorana mass terms are explained as well as models such as the seesaw mechanism. Schemes for two, three and four neutrino mixings are presented. 11th Mexican School of Particles and Fields arXiv:hep-ph/0506257v1 24 Jun 2005 August 2004 1E-mail:
[email protected] 2E-mail: erler@fisica.unam.mx 3E-mail: epeinado@nirvana.fisica.uson.mx Contents 1 The Fermi Theory 1 2 Intermediate Vector Bosons (IVB) and SU(2)W × U(1)Y 3 3 Aspects of the SU(2)W × U(1)Y Theory 4 3.1 TheWeakChargedCurrent .......................... 7 3.2 TheWeakNeutralCurrent. 8 4 Neutrino Preliminaries 9 4.1 WeylSpinors .................................. 10 4.2 ActiveandSterileNeutrinos . ... 10 5 Neutrino Mass Models 11 5.1 FermionMasses................................. 11 5.2 DiracMass ................................... 11 5.3 MajoranaMass ................................. 12 5.4 Mixedmodels .................................. 13 5.5 SpecialCases .................................. 14 5.6 ExtensiontoThreeFamilies . .. 15 5.7 ModelsofNeutrinoMass. .. .. .. 17 6 Laboratory and Astrophysical Constraints on Neutrino Counting and Mass 18 6.1 LaboratoryLimits ............................... 18 6.2 CosmologicalConstraints. ... 19 6.3 NeutrinoOscillations . .. 20 7 Atmospheric Neutrinos 21 8 Solar Neutrinos 22 9 Neutrino Oscillation Patterns 25 9.1 ThreeNeutrinoPatterns . 25 9.2 FourNeutrinoPatterns. 26 10 Conclusions 27 i 1 The Fermi Theory The history of the weak interactions dates back to the discovery of radioactivity by Bec- querel in 1896 [1].