ar X iv : h ep - p h / 06 10 06 4 v 2 5 O ct 2 00 6 Neutrino oscillations : theory and phenomenology 1

ar X iv : h ep - p h / 06 10 06 4 v 1 5 O ct 2 00 6 Neutrino oscillations : theory and phenomenology 1

Abstract. A brief overview of selected topics in the theory and phenomenology of neutrino oscillations is given. These include: oscillations in vacuum and in matter; phenomenology of 3-flavour neutrino oscillations and effective 2-flavour approximations; CP and T violation in neutrino oscillations in vacuum and in matter; matter effects on νμ ↔ ντ oscillations; parametric resonance in neutrino ...

ar X iv : h ep - p h / 06 05 22 8 v 1 2 2 M ay 2 00 6 FLAVOR NEUTRINO OSCILLATIONS AND TIME - ENERGY UNCERTAINTY RELATION 1

We consider neutrino oscillations as non stationary phenomenon based on Schrodinger evolution equation and mixed states of neutrinos with definite flavors. We show that time-energy uncertainty relation plays a crucial role in neutrino oscillations. We compare neutrino oscillations with B 0 d ⇆ ¯ B 0 d oscillations.

ar X iv : h ep - p h / 01 06 32 4 v 3 1 5 O ct 2 00 1 Anderson Theorem for Color Superconductor

Ginzburg-Landau functional is derived for a system possessing both chiral and diquark condensates. Anderson theorem for such a system is formulated and proved.

ar X iv : h ep - p h / 06 03 05 3 v 2 3 O ct 2 00 6 OUTP - 06 06 P Triviality and the ( Supersymmetric ) See - Saw

For the D = 5 Majorana neutrino mass operator to have a see-saw ultraviolet completion that is viable up to the Planck scale, the see-saw scale is bounded above due to triviality limits on the see-saw couplings. For supersymmetric see-saw models, with realistic neutrino mass textures, we compare constraints on the see-saw scale from triviality bounds, with those arising from experimental limits...

ar X iv : h ep - p h / 06 05 10 7 v 2 24 O ct 2 00 6 Monopole confinement by flux tube