Probing for the Roots of the Standard Model

preprint1995arXivOpen access

Abstract

The differences between the N=0N=0 and N=1N=1 standard models are emphasized in formulating their short distance extension. We sketch methods to reproduce many of the small numbers in the model in terms of scale ratios, applying see-saw like ideas to the breaking of chiral symmetries. We sketch how the N=1N=1 standard model, outfitted with an extra family Abelian symmetry to reproduce the mass hierarchies, naturally fits superstring models, by making use of generic non-renormalizable operators.

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