Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2005-11-09
Phys.Lett. B634 (2006) 520-525
Physics
High Energy Physics
High Energy Physics - Phenomenology
12 pages, model claified, references added and corrected
Scientific paper
10.1016/j.physletb.2006.02.022
We propose a scenario that the mass splitting between the first generation of the heavy Majorana neutrino and the other two generations of degenerate heavy neutrinos in the seesaw framework is responsible for the deviation of the solar mixing angle from the maximal mixing, while keeping the maximal mixing between the tau and muon neutrinos as it is. On top of the scenario, we show that the tiny breaking of the degeneracy of the two heavy Majorana neutrinos leads to the non-zero small mixing angle $U_{e3}$ in the PMNS matrix and the little deviation of the atmospheric neutrino mixing angle from the maximal mixing.
Kang Sin Kyu
Kim Chang Sub
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