Dark Matter Abundance and Electroweak Baryogenesis in the CMSSM

Details Dark Matter Abundance and Electroweak Baryogenesis in the CMSSM Dark Matter Abundance and Electroweak Baryogenesis in the CMSSM

1999-07-15

arxiv.org/abs/hep-ph/9907365v1

Phys.Lett. B463 (1999) 214-224

Physics

High Energy Physics

High Energy Physics - Phenomenology

14 pages in LaTeX, including 7 encapsulated postscript figures

Scientific paper

10.1016/S0370-2693(99)00975-2

The Minimal Supersymmetric Standard Model has a candidate dark matter particle in its spectrum and may be able to generate the baryon asymmetry of the Universe (BAU) at the electroweak phase transition. In the Constrained MSSM, we find the area of parameter space which is allowed by accelerator and precision tests, which produces a relic dark matter abundance in the observationally favored window 0.1

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