Radiative stability of neutrino-mass textures

Abstract

Neutrino-mass textures proposed at high-scales are known to be unstable against radiative corrections especially for nearly degenerate eigen values. Within the renormalization group constraints we find a mechanism in a class of gauge theories which guarantees reproduction of any high-scale texture at low energies with radiative stability. We also show how the mechanism explains solar and atmospheric neutrino anomalies through the bimaximal texture at high scale.

4 pages REVTEX, 1 Postscript fig

References in corpus (1)

• Neutrino Mass Operator Renormalization Revisited

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