Phenomenology of neutrino oscillations

Phenomenology of Neutrino Oscillations

We review the status of several phenomenological topics of current interest in neutrino oscillations: (i) Solar neutrino oscillations after the first Sudbury Neutrino Observatory measurements, including both model-independent and model-dependent results; (ii) Dominant νμ → ντ oscillations of atmospheric and K2K neutrinos, and possible subdominant oscillations induced by either extra states or e...

Phenomenology of Neutrino Oscillations at a Neutrino Factory

There have been several experiments 1,2,3,4,5,6,7,8,9,10,11 which suggest neutrino oscillations. It has been known in the two flavor framework that the solar neutrino deficit can be explained by neutrino oscillation with the set of parameters (∆m⊙, sin 2 2θ⊙) ≃ (O(10−5eV),O(10−2)) (small angle MSW solution), (O(10−5eV),O(1)) (large angle MSW solution), or (O(10−10eV),O(1)) (vacuum oscillation s...

Solar Neutrino Oscillation Phenomenology

Abstract. This article summarises the status of the solar neutrino oscillation phenomenology at the end of 2002 in the light of the SNO and KamLAND results. We first present the allowed areas obtained from global solar analysis and demonstrate the preference of the solar data towards the Large-Mixing-Angle (LMA) MSW solution. A clear confirmation in favor of the LMA solution comes from the KamL...

Neutrino Oscillation Phenomenology ∗ †

Phenomenology of Absolute Neutrino Masses

Solar, atmospheric and long-baseline neutrino oscillation experiments obtained convincing evidence that neutrinos are massive and mixed particles. Since on one hand solar and KamLAND experiments and on the other hand atmospheric and K2K experiments are sensitive to oscillations generated by different orders of magnitude of differences of squared neutrino masses, at least two independent ∆m SUN ...