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The CMSSM parameter space at large tanβ
Authors:John Ellis  Toby Falk  Gerardo Ganis  Keith A Olive and Mark Srednicki
Institution:

a TH Division, CERN, Geneva, Switzerland

b Theoretical Physics Institute, School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA

c INFN, Università di Roma II ‘Tor Vergata’, Rome, Italy

d Department of Physics, University of California, Santa Barbara, CA 93106, USA

Abstract:We extend previous combinations of LEP and cosmological relic density constraints on the parameter space of the constrained MSSM, with universal input supersymmetry-breaking parameters, to large tanβ. We take account of the possibility that the lightest Higgs boson might weigh about 115 GeV, but also retain the possibility that it might be heavier. We include the most recent implementation of the bsγ constraint at large tanβ. We refine previous relic density calculations at large tanβ by combining a careful treatment of the direct-channel Higgs poles in annihilation of pairs of neutralinos χ with a complete treatment of χ–Image coannihilation, and discuss carefully uncertainties associated with the mass of the b quark. We find that coannihilation and pole annihilations allow the CMSSM to yield an acceptable relic density at large tanβ, but it is consistent with all the constraints only if mχ>140 (180) GeV for μ>0 (μ<0) for our default choices Image  GeV, mt=175 GeV, and A0=0.
Keywords:
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