Neutrino Oscillations in the Dualized Standard Model

Details Neutrino Oscillations in the Dualized Standard Model Neutrino Oscillations in the Dualized Standard Model

1998-02-25

arxiv.org/abs/hep-ph/9802420v1

Phys.Rev.D58:053003,1998

Physics

High Energy Physics

High Energy Physics - Phenomenology

16 pages, Latex, 5 figures using eps

Scientific paper

10.1103/PhysRevD.58.053003

A method developed from the Dualized Standard Model for calculating the quark CKM matrix and masses is applied to the parallel problem in neutrino oscillations. Taking the parameters determined from quarks and the masses of two neutrinos: $m_3^2 \sim 10^{-2} - 10^{-3} eV^2$ suggested by atmospheric neutrino data, and $m_2^2 \sim 10^{-10} eV^2$ suggested by the long wave-length oscillation (LWO) solution of the solar neutrino problem, one obtains from a parameter-free calculation all the mixing angles in reasonable agreement with existing experiment. However, the scheme is found not to accommodate comfortably the mass values $m_2^2 \sim 10^{-5} eV^2$ suggested by the MSW solution for solar neutrinos.

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