The Solar Neutrino Problem

1981 ◽  
pp. 399-406
Author(s):  
Ian W. Roxburgh
Keyword(s):  
Solar Neutrino ◽  
Solar Neutrino Problem

NEUTRINO OSCILLATION AND LEPTON MASS MATRIX

1994 ◽  
Vol 09 (01) ◽  
pp. 41-50 ◽  
Author(s):  
KEN-ITI MATUMOTO ◽  
DAIJIRO SUEMATSU
Keyword(s):  
Solar Neutrino ◽  
Phase Structure ◽  
Quark Mass ◽  
Mass Matrix ◽  
Lepton Sector ◽  
Solar Neutrino Problem ◽  
Quark Sector ◽  
Mass Matrices ◽  
Suppression Mechanism ◽  
The Right

We apply the empirical quark mass matrices to the lepton sector and study the solar neutrino problem and the atmospheric vμ deficit problem simultaneously. We show that their consistent explanation is possible on the basis of these matrices. The lepton sector mass matrices need the phase structure which is different from the ones of the quark sector. However, even if the phase structure of the mass matrices is identical in both sectors, an interesting suppression mechanism of sin 2 2θ12 which is related to the solar neutrino problem can be induced from the right-handed neutrino Majorana mass matrix. We discuss such a possibility through the concrete examples.

Topological geometrodynamics and the solar neutrino problem

1992 ◽  
Vol 31 (2) ◽  
pp. 245-267
Author(s):  
Matti Pitk�nen ◽  
Petri M�h�nen
Keyword(s):  
Solar Neutrino ◽  
Solar Neutrino Problem

The solar-neutrino problem

1991 ◽  
Vol 104 (10) ◽  
pp. 1577-1579
Author(s):  
V. de Sabbata ◽  
C. Sivaram
Keyword(s):  
Solar Neutrino ◽  
Solar Neutrino Problem

From CKM Matrix to MNS Matrix: A Model Based on SUSY SO(10) × U(2)F Symmetry

2001 ◽  
Vol 16 (supp01c) ◽  
pp. 893-895
Author(s):  
Mu-Chun Chen ◽  
K. T. Mahanthappa
Keyword(s):  
Solar Neutrino ◽  
Realistic Model ◽  
Flavor Symmetry ◽  
Solar Neutrino Problem ◽  
Ckm Matrix ◽  
Mixing Angles ◽  
Model Based

We construct a realistic model based on SUSY SO(10) with U(2) flavor symmetry. A set of symmetric mass textures give rise to very good predictions; 15 masses and 6 mixing angles are predicted by 11 parameters. Both the vacuum oscillation and LOW solutions are favored for the solar neutrino problem.

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