Results 111 to 120 of about 145,656 (172)
Horizontal symmetry: masses and mixing angles of quarks and leptons of different generations; neutrino mass and neutrino oscillation [PDF]
Z.G. Berezhiani, Dzh L. Chkareuli
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NEUTRINO OSCILLATION AND STELLAR COLLAPSE [PDF]
A. Pérez-Canyellas, J. Bernabéu
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Neutrino Oscillations, Masses and Mixing [PDF]
The original B. Pontecorvo idea of neutrino oscillations is discussed. Neutrino mixing and basics of neutrino oscillations in vacuum and in matter are considered. Recent evidences in favour of neutrino oscillations, obtained in Super-Kamiokande, SNO, KamLAND and other neutrino experiments are discussed.
arxiv
Different Schemes of Neutrino Oscillations in MÖssbauer Neutrino Experiment [PDF]
We comment on the paper "On application of the time-energy uncertainty relation to M\"ossbauer neutrino experiments" (see arXiv: 0803.1424) in which our paper "Time-energy uncertainty relations for neutrino oscillation and M\"ossbauer neutrino experiment" (see arXiv: 0803.0527) has been criticized.
arxiv
Experimental constraints on the neutrino oscillations and a simple model of three-flavor mixing [PDF]
Piotr A. Ra̧czka+2 more
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Long-wavelength oscillations and the new gallium solar neutrino signals [PDF]
V. Barger+2 more
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Solar neutrino data, solar model uncertainties and neutrino oscillations [PDF]
Lawrence M. Krauss+2 more
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Kinetic Equation with Neutrino Oscillations in the Early Universe [PDF]
H. Granek, Bruce H. J. McKellar
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PHENOMENOLOGY OF NEUTRINO OSCILLATIONS AT A NEUTRINO FACTORY [PDF]
It is shown in the three flavor framework that neutrino factories enable us to measure some of the oscillation parameters, such as the sign of $ m_{32}^2$, $ _{13}$, $ $. Some efforts are made to determine the parameters (the muon energy and the neutrino path length) of a neutrino factory to optimize the signals.
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Remark on neutrino oscillations
AbstractThe oscillations of ultra-relativistic neutrinos are realized by the propagation of assumed zero-mass on-shell neutrinos with the speed of light in vacuum combined with the phase modulation by the small mass term $$\exp [-i(m^{2}_{\nu _{k}}/2|\vec {p}|)\tau ]$$ exp
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