Maximal mixing neutrino models

Details Maximal mixing neutrino models Maximal mixing neutrino models

1998-04-17

arxiv.org/abs/hep-ph/9804310v1

J.Phys.G24:1249-1260,1998

Physics

High Energy Physics

High Energy Physics - Phenomenology

23 pages, no figures, ReVTeX. Original version written in March 1997; revised and updated in March 1998. To appear in J Phys G

Scientific paper

10.1088/0954-3899/24/7/007

We account for the solar and atmospheric neutrino problems by introducing maximal mixing between conventional and sterile neutrino partners. We achieve this by invoking a seesaw-like mechanism which not only provides us with maximally mixed neutrino/sterile-neutrino mass eigenstates but also accounts for the relative suppression of the neutrino masses compared to the charged fermion masses. In obtaining such an extended seesaw mechanism we are required to introduce a new U(1) global symmetry together with an extended Higgs sector.

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