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      Next-to-Minimal Supersymmetric Standard Model with the Gauge Mediation of Supersymmetry Breaking

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          Abstract

          We study the Next-to-Minimal Supersymmetric Standard Model (NMSSM) as the simplest candidate solution to the μ-problem in the context of the gauge mediation of supersymmetry breaking (GMSB). We first review various proposals to solve the μ-problem in models with the GMSB. We find none of them entirely satisfactory and point out that many of the scenarios still lack quantitative studies, and motivate the NMSSM as the simplest possible solution. We then study the situation in the Minimal Supersymmetric Standard Model (MSSM) with the GMSB and find that an order 10% cancellation is necessary between the μ-parameter and the soft SUSY-breaking parameters to correctly reproduce MZ. Unfortunately, the NMSSM does not to give a phenomenologically viable solution to the μ-problem. We present quantitative arguments which apply both for the low-energy and high-energy GMSB and prove that the NMSSM does not work for either case. Possible modifications to the NMSSM are then discussed. The NMSSM with additional vector-like quarks works phenomenologically, but requires an order a few percent cancellation among parameters. We point out that this cancellation has the same origin as the cancellation required in the MSSM.

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          A Model of Direct Gauge Mediation

          We present a simple model of gauge mediation (GM) which does not have a messenger sector or gauge singlet fields. The standard model gauge groups couple directly to the sector which breaks supersymmetry dynamically. This is the first phenomenologically viable example of this type in the literature. Despite the direct coupling, the model can preserve perturbative gauge unification. This is achieved by the inverted hierarchy mechanism which generates a large scalar expectation value compared to the size of supersymmetry breaking. There is no dangerous negative contribution to the squark, slepton masses due to two-loop renormalization group equation. The potentially non-universal supergravity contribution to the scalar masses can be suppressed enough to maintain the virtue of the gauge mediation. The model is completely chiral, and one does not need to forbid mass terms for the messenger fields by hand. Beyond the simplicity of the model, it possesses cosmologically desirable features compared to the original models of GM: an improved gravitino and string moduli cosmology. The Polonyi problem is back unlike in the original GM models, but is still much less serious than in hidden sector models.
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            Journal
            07 November 1997
            1997-12-11
            Article
            10.1103/PhysRevD.57.5676
            hep-ph/9711264
            4d181206-33e5-4fc0-99c7-0010518e466f
            History
            Custom metadata
            UCB-PTH-97/46,LBNL-41028
            Phys.Rev.D57:5676-5696,1998
            36 pages, LaTeX, epsf.sty, 5 figures, references added, comments on some other papers based on our misundestanding corrected, none of our results changed
            hep-ph

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