English

A Natural Solution to the MU Problem

High Energy Physics - Phenomenology 2008-11-26 v1

Abstract

We propose a simple mechanism for solving the μ\mu 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 H1H2H_1H_2 is an allowed operator by all the symmetries of the theory, it is natural to promote the usual renormalizable superpotential WoW_o to Wo+λWoH1H2W_o+\lambda W_o H_1H_2, yielding an effective μ\mu parameter whose size is directly related to the gravitino mass once supersymmetry is broken (this result is maintained if H1H2H_1H_2 couples with different strengths to the various terms present in WoW_o). On the other hand, the μ\mu term must be absent from WoW_o, otherwise the natural scale for μ\mu would be MPM_P. 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)SU(2)\times 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\mu problem can be gracefully implemented.

Keywords

Cite

@article{arxiv.hep-ph/9302227,
  title  = {A Natural Solution to the MU Problem},
  author = {J. A. Casas and C. Munoz},
  journal= {arXiv preprint arXiv:hep-ph/9302227},
  year   = {2008}
}

Comments

11 pages, CERN-TH.6764/92