2004
DOI: 10.1016/j.physletb.2004.08.070
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Neutralino relic density in a supersymmetric U(1) model

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Cited by 41 publications
(13 citation statements)
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“…Inclusion of the kinetic mixing in the Stueckelberg extension enhances significantly the parameter space where new physics can exist consistent with the stringent LEP, Tevatron, and WMAP constraints. This parameter space includes the possibility of a narrow Z 0 resonance very distinct from the Z 0 of the conventional models [23][24][25].…”
Section: Introductionmentioning
confidence: 99%
“…Inclusion of the kinetic mixing in the Stueckelberg extension enhances significantly the parameter space where new physics can exist consistent with the stringent LEP, Tevatron, and WMAP constraints. This parameter space includes the possibility of a narrow Z 0 resonance very distinct from the Z 0 of the conventional models [23][24][25].…”
Section: Introductionmentioning
confidence: 99%
“…In the nMSSM (also in the S-model in the decoupling limit), because of the small χ 0 1 mass, the Z pole is the dominant channel [11,14]. To obtain an acceptable relic density with only the Z pole annihilation contribution, the lower M χ 0 1 bound is M χ 0 1 ∼ > 30 GeV which is allowed for only small tan β , while the solution for a 2.4σ deviation from the SM of (g − 2) µ favors large tan β , which allows only small M χ 0 1 .…”
Section: Discussionmentioning
confidence: 99%
“…It is then possible to satisfy the relic density constraints consistent with WMAP data [41,46]. For other possible candidates arising from U (1) extensions see [47,48].…”
Section: Milli Weak Dark Mattermentioning
confidence: 97%