Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1998-07-08
Phys.Rev.D59:017304,1999
Physics
High Energy Physics
High Energy Physics - Phenomenology
11 pages, LaTex file, 2 figures included using epsfig, some mistakes corrected, references added, numerical results unchanged
Scientific paper
10.1103/PhysRevD.59.017304
We consider the case that the solar neutrino deficit is due to the vacuum oscillation. The lepton mass matrices with nearly bi-maximal mixings are needed in order to explain both solar and atmospheric neutrino deficit. A texture with the symmetry of flavour democracy or $S_3$ has been investigated by taking account of the symmetry breaking terms of the charged lepton mass matrix. It is found that predicted mixings can be considerably changed from the neutrino mixings $\sin^2 2\th_\odot\simeq 1$ and $\sin^2 2\th_{\rm atm}\simeq 8/9$ at the symmetric limit. The correlation between $|U_{e3}|$ and $|U_{e1}U_{e2}^*|$ is also presented. The test of the model is discussed by focusing on the three flavor analyses in the solar neutrinos, atmospheric neutrinos and long baseline experiments.
No associations
LandOfFree
Vacuum Neutrino Oscillations of Solar Neutrinos and Lepton Mass Matrices does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Vacuum Neutrino Oscillations of Solar Neutrinos and Lepton Mass Matrices, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Vacuum Neutrino Oscillations of Solar Neutrinos and Lepton Mass Matrices will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-607406