Electroweak baryogenesis and dark matter in a minimal extension of the MSSM

A. Menon, D. E. Morrissey, and C. E. M. Wagner
Phys. Rev. D 70, 035005 – Published 19 August 2004
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Abstract

We examine the possibility of electroweak baryogenesis and dark matter in the nMSSM, a minimal extension of the MSSM with a singlet field. This extension avoids the usual domain wall problem of the NMSSM, and also appears as the low energy theory in models of dynamical electroweak symmetry breaking with a so-called fat-Higgs boson. We demonstrate that a strong, first order electroweak phase transition, necessary for electroweak baryogenesis, may arise in regions of parameter space where the lightest neutralino provides an acceptable dark matter candidate. We investigate the parameter space in which these two properties are fulfilled and discuss the resulting phenomenology. In particular, we show that there are always two light CP-even and one light CP-odd Higgs bosons with masses smaller than about 250 GeV. Moreover, in order to obtain a realistic relic density, the lightest neutralino mass tends to be smaller than MZ/2, in which case the lightest Higgs boson decays predominantly into neutralinos.

  • Received 7 May 2004

DOI:https://doi.org/10.1103/PhysRevD.70.035005

©2004 American Physical Society

Authors & Affiliations

A. Menon, D. E. Morrissey, and C. E. M. Wagner

  • HEP Division, Argonne National Laboratory, 9700 Cass Ave., Argonne, Illinois 60439, USA
  • Enrico Fermi Institute, Univ. of Chicago, 5640 S. Ellis Ave., Chicago, Illinois 60637, USA

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Issue

Vol. 70, Iss. 3 — 1 August 2004

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