Seesaw Neutrino Mass Ratios with Radiative Corrections

Details Seesaw Neutrino Mass Ratios with Radiative Corrections Seesaw Neutrino Mass Ratios with Radiative Corrections

1992-06-26

arxiv.org/abs/hep-ph/9206256v1

Phys.Lett. B309 (1993) 91-94

Physics

High Energy Physics

High Energy Physics - Phenomenology

8 pp., plain tex, with jnl macros incl, FERMILAB-PUB-92/149-T

Scientific paper

10.1016/0370-2693(93)91509-L

In the canonical up-quark seesaw, the ratios of light neutrino masses are more easily predicted than the masses themselves. Under explicitly enumerated neccesary but minimal assumptions, these ratios are obtained, including radiative corrections. The predictions remain uncertain only by the top quark mass and triviality mass limit, and the power law of the seesaw. The tau neutrino is specially affected by the non-linear effect of the heavy top quark mass. The derived ratios have application to solar, atmospheric, and cosmological neutrinos and laboratory neutrino oscillation searches. The seesaw with charged lepton masses instead is briefly considered. Submitted to Phys Lett B.

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