NEUTRINO MASSES AND NEUTRINO OSCILLATIONS

2009 ◽  
Author(s):  
H. Fritzsch ◽  
Vladimir Lebedev ◽  
Mikhail Feigel’man

1990 ◽  
Vol 121 ◽  
pp. 213-230
Author(s):  
Haim Harari

AbstractWe discuss bounds on neutrino masses using an analysis based on direct measurements, cosmological bounds, oscillation experiments, the solar neutrino puzzle and theoretical considerations on neutrino decays. We present four possible solutions for the mass range of the three neutrino flavors. We outline experiments which can distinguish among these solutions and discuss their implications for the cosmological dark matter problem.


2007 ◽  
Vol 653 (2-4) ◽  
pp. 267-277 ◽  
Author(s):  
V. Barger ◽  
D. Marfatia ◽  
K. Whisnant

Author(s):  
Shun Zhou

Abstract Three-flavor neutrino oscillations in matter can be described by three effective neutrino masses mi (for i = 1, 2, 3) and the effective mixing matrix Vαi (for α = e, µ, τ and i = 1, 2, 3). When the matter parameter a ≡ 2√2GFNeE is taken as an independent variable, a complete set of first-order ordinary differential equations for m2 i and |Vαi|2have been derived in the previous works. In the present paper, we point out that such a system of differential equations possesses both the continuous symmetries characterized by one-parameter Lie groups and the discrete symmetry associated with the permutations of three neutrino mass eigenstates. The implications of these symmetries for solving the differential equations and looking for differential invariants are discussed.


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