Neutrino Oscillations Wikipedia, the Free Encyclopedia
Neutrino oscillations - Wikipedia, the free encyclopedia http://en.wikipedia.org/wiki/Neutrino_oscillations Neutrino oscillations From Wikipedia, the free encyclopedia Neutrino oscillations are a quantum mechanical phenomenon predicted by Bruno Pontecorvo whereby a neutrino created with a specific lepton flavor (electron, muon or tau) can later be measured to have a different flavor. The probability of measuring a particular flavor for a neutrino varies periodically as it propagates. Neutrino oscillation is of theoretical and experimental interest since observation of the phenomenon implies that the neutrino has a nonzero mass, which is not part of the original Standard Model of particle physics. A zero mass particle would have to travel at the speed of light. At the speed of light, time stands still so no change (and, therefore, no oscillation) is possible. Therefore if particles change, they must have mass. Contents 1 Observations 1.1 Solar neutrino oscillation 1.2 Atmospheric neutrino oscillation 1.3 Reactor neutrino oscillations 1.4 Beam neutrino oscillations 1.5 Decay oscillations GSI anomaly 2 Theory 2.1 Classical analogue of neutrino oscillation 2.2 Pontecorvo–Maki–Nakagawa–Sakata matrix 2.3 Propagation and interference 2.4 Two neutrino case 3 Theory, graphically 3.1 Two neutrino probabilities in vacuum 3.2 Three neutrino probabilities 4 Observed values of oscillation parameters 5 Origins of neutrino mass 5.1 Seesaw mechanism 5.2 Other sources 1 of 15 09.10.2010 г. 20:28 Neutrino oscillations - Wikipedia, the free encyclopedia http://en.wikipedia.org/wiki/Neutrino_oscillations 6 See also 7 Notes 8 References 9 External links Observations A great deal of evidence for neutrino oscillations has been collected from many sources, over a wide range of neutrino energies and with many different detector technologies.