Scalar Dark Matter From Theory Space

Details Scalar Dark Matter From Theory Space Scalar Dark Matter From Theory Space

2003-06-18

arxiv.org/abs/hep-ph/0306161v2

Phys.Rev. D69 (2004) 065022

Physics

High Energy Physics

High Energy Physics - Phenomenology

18 pages, 2 figures, version to appear in PRD

Scientific paper

10.1103/PhysRevD.69.065022

The scalar dark matter candidate in a prototypical theory space little Higgs model is investigated. We review all details of the model pertinent to dark matter. We perform a thermal relic density calculation including couplings to the gauge and Higgs sectors of the model. We find two regions of parameter space that give acceptable dark matter abundances. The first region has a dark matter candidate with a mass of order 100 GeV, the second region has a heavy candidate with a mass greater than about 500 GeV$. The dark matter candidate in either region is an admixture of an SU(2) triplet and an SU(2) singlet, thereby constituting a WIMP (weakly interacting massive particle).

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