Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
10724094 | Physics Letters B | 2010 | 4 Pages |
Abstract
Among neutrino mixings, the reactor mixing angle, θ13, is observed to be almost vanishing and is consistent with θ13=0. We discuss how the condition of θ13=0 constrains models of neutrino mixings and show that, for flavor neutrino masses given by Mij(i,j=e,μ,Ï), two conditions of MeÏ=âe2iγtanθ23Meμ and MÏÏ=e4iγMμμ+e2iγ(2/tan2θ23)MÎ¼Ï lead to θ13=0, where θ23 is the atmospheric neutrino mixing angle and γ is its associated phase. The rephasing invariance can select two phases provided by α=arg(Meμ) and β=arg(MeÏ), giving γ=(βâα)/2.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Keisuke Yuda, Masaki Yasuè,