Option of three pseudo--Dirac neutrinos
Wojciech Krolikowski

TL;DR
This paper explores a pseudo-Dirac neutrino model as an alternative to the see-saw mechanism, explaining neutrino oscillation phenomena and suggesting a specific neutrino mass matrix structure.
Contribution
It introduces a novel pseudo-Dirac neutrino framework with a specific mass matrix form, providing a consistent explanation for various neutrino oscillation observations.
Findings
Neutrino oscillations explain solar and atmospheric neutrino deficits.
The model accommodates LSND results with adjustable parameters.
Atmospheric neutrinos mainly oscillate into tau neutrinos.
Abstract
As an alternative for popular see-saw mechanism, the option of three pseudo% -Dirac neutrinos is discussed, where for their Majorana and Dirac masses. The actual neutrino mass matrix is assumed in the form of tensor product M^{(\nu)} \otimes {(\{array} {cc} \lambda^{(L)} & 1 1 & \lambda^{(R)} \{array})}, where is a neutrino family mass matrix () and with , and being taken as universal for three neutrino families. It is shown that three neutrino effects (deficits of solar 's and atmospheric 's as well as the possible LSND excess of 's in accelerator beam) can be nicely described by the corresponding neutrino oscillations, though the LSND effect may, alternatively, be eliminated (by a…
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Taxonomy
TopicsNeutrino Physics Research · Astrophysics and Cosmic Phenomena · Particle accelerators and beam dynamics
