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Radiative Origin of the Fermion Mass Hierarchy: A Realistic and Predictive Approach

Zurab Berezhiani, Riccardo Rattazzi

hep-pharXiv:hep-ph/9210252

Abstract

The up-down splitting within quark families increases with the family number: mu ~ md, mc > ms, mt >> mb. We show an approach that realizes this feature of the spectrum in a natural way. We suggest that the mass hierarchy is first generated by radiative effects in a sector of heavy isosinglet fermions, and then projected to the ordinary light fermions by means of a seesaw mixing. The hierarchy appears then inverted in the light fermion sector. We present a simple left-right symmetric gauge model in which the P- and CP-parities and an isotopical &#34;up-down&#34; symmetry are softly (or spontaneously) broken in the Higgs potential. Experimentally consistent predictions are obtained. The Cabibbo angle is automatically in the needed range: ThetaC ~ 0.2. The top quark is naturally heavy, but not too heavy: mt < 150 GeV.

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