Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1996-11-19
Mod.Phys.Lett. A12 (1997) 1175-1184
Physics
High Energy Physics
High Energy Physics - Phenomenology
9 pages, RevTex, no figures
Scientific paper
10.1142/S0217732397001205
Assuming three light neutrinos are Majorana particles, we propose mass matrix ansatz for the charged leptons and Majorana neutrinos with family symmetry $S_{3} $ broken into $S_{1}$ and $S_{2}$, respectively. Each matrix has three parameters, which are fixed by measured charged lepton masses, differences of squared neutrino masses relevant to the solar and the atmospheric neutrino puzzles, and the masses of three light Majorana neutrinos as a candidate for hot dark matter with $\sum |m_{\nu}| \sim 6 eV$. The resulting neutrino mixing is compatible with the data for the current upper limit, $ < m_{\nu_e} >_{th} < 0.8 eV$, of neutrino-less double beta decay experiments, and the current data for various types of neutrino oscillation experiments. One solution of our model predicts that $\nu_{\mu} \rightarrow \nu_{\tau}$ oscillation probability is about $< 0.008$ with $\Delta m^{2} \sim 10^{-2} eV^2$, which may not be accessible at CHORUS and other ongoing experiments.
Kang Kyungsik
Kang Sin Kyu
Kim Jihn E.
Ko Pyungwon
No associations
LandOfFree
Almost maximally broken permutation symmetry for neutrino mass matrix 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 Almost maximally broken permutation symmetry for neutrino mass matrix, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Almost maximally broken permutation symmetry for neutrino mass matrix will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-310417