ar X iv : 0 80 4 . 13 11 v 4 [ nu cl - t h ] 7 N ov 2 00 8 Neutrino masses from the “ Darmstadt oscillations ”

ar X iv : 0 80 4 . 13 11 v 3 [ nu cl - t h ] 6 N ov 2 00 8 Neutrino masses from the “ Darmstadt oscillations ”

Atominstitut der Österreichischen Universitäten, Technische Universität Wien, Wiedner Hauptstraße 8-10, A-1040 Wien, Österreich, Stefan Meyer Institut für subatomare Physik, Österreichische Akademie der Wissenschaften, Boltzmanngasse 3, A-1090, Wien, Österreich, c Petersburg Nuclear Physics Institute, 188300 Gatchina, Orlova roscha 1, Russian Federation, Excellence Cluster Universe Technische U...

ar X iv : 0 80 4 . 13 11 v 5 [ nu cl - t h ] 2 6 M ar 2 00 9 Neutrino masses from the GSI anomaly

Atominstitut der Österreichischen Universitäten, Technische Universität Wien, Wiedner Hauptstraße 8-10, A-1040 Wien, Österreich, Stefan Meyer Institut für subatomare Physik, Österreichische Akademie der Wissenschaften, Boltzmanngasse 3, A-1090, Wien, Österreich, c Petersburg Nuclear Physics Institute, 188300 Gatchina, Orlova roscha 1, Russian Federation, Excellence Cluster Universe Technische U...

ar X iv : h ep - p h / 00 11 11 7 v 1 8 N ov 2 00 0 1 ( Mis ) Understanding the Atmospheric Neutrino Anomaly

ar X iv : h ep - p h / 02 11 13 8 v 1 1 1 N ov 2 00 2 1 Neutrino Oscillations , SUSY See - Saw Mechanism and Charged Lepton

Neutrino oscillations give clear evidence for non-vanishing neutrino masses and lepton-flavor violation (LFV) in the neutrino sector. This provides strong motivation to search for signals of LFV also in the charged lepton sector, and to probe the SUSY seesaw mechanism. We compare the sensitivity of rare radiative decays on the right-handed Majorana mass scale MR with the reach in slepton-pair p...

ar X iv : h ep - p h / 02 11 13 4 v 1 1 0 N ov 2 00 2 Neutrino Mass , Mixing , and Flavor Change ∗

The theoretical basics of neutrino mass and mixing are reviewed. Dirac and Majorana masses are explained, and added together to produce the see-saw picture of the lightness of neutrinos. This picture predicts that neutrinos are Majorana particles. The character, and an apparent paradox, of Majorana neutrinos are examined. The physics of neutrino flavor change (oscillation), in vacuo and in matt...