A natural solution to the μ-problem in dynamical supergravity model
Tomohiro Matsuda
Abstract
The Higgs mixing term coefficient μ is calculated in the supersymmetric theory which possesses a non-anomalous U(1)R symmetry in the limit of global supersymmetry. In this model, supersymmetry is assumed to be broken by gaugino condensation in the hidden sector when the supergravity effects are turned on. The soft breaking terms in the visible sector and the μ term of order the weak scale are produced in a simple manner.
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