A Natural Solution to the MU Problem
J. A. Casas, C. Munoz
Abstract
We propose a simple mechanism for solving the μ problem in the context of minimal low--energy supergravity models. This is based on the appearance of non--renormalizable couplings in the superpotential. In particular, if H1H2 is an allowed operator by all the symmetries of the theory, it is natural to promote the usual renormalizable superpotential Wo to Wo+λWo H1H2, yielding an effective μ parameter whose size is directly related to the gravitino mass once supersymmetry is broken (this result is maintained if H1H2 couples with different strengths to the various terms present in Wo). On the other hand, the μ term must be absent from Wo, otherwise the natural scale for μ would be MP. Remarkably enough, this is entirely justified in the supergravity theories coming from superstrings, where mass terms for light fields are forbidden in the superpotential. We also analyse the SU(2)× U(1) breaking, finding that it takes place satisfactorily. Finally, we give a realistic example in which supersymmetry is broken by gaugino condensation, where the mechanism proposed for solving the μ problem can be gracefully implemented.
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