Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
9861595 | Physics Letters B | 2005 | 9 Pages |
Abstract
It is found that the atmospheric neutrino mixing angle of θatm is determined to be tanθatm=Im(B)/Im(C) for B=Mνeνμ and C=MνeνÏ, where Mij is the ij element of Mνâ Mν with Mν as a complex symmetric neutrino mass matrix in the (νe, νμ, νÏ)-basis. Another mixing angle, θ13, defined as Ue3=sinθ13eâiδ is subject to the condition: tan2θ13â|sinθatmB+cosθatmC| and the CP-violating Dirac phase of δ is identical to the phase of sinθatmB*+cosθatmC*. The smallest value of |sinθ13| is achieved at tanθatm=âRe(C)/Re(B) that yields the maximal CP-violation and that implies C=âκB* for the maximal atmospheric neutrino mixing of tanθatm=κ=±1. The generic smallness of |sinθ13| can be ascribed to the tiny violation of the electron number conservation.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Ichiro Aizawa, Masaki Yasuè,