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Neutralino Dark Matter in MSSM Models with Non-Universal Higgs Masses

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3462670· OSTI ID:21410187
 [1]
  1. Theory Group and Texas Cosmology Center, University of Texas at Austin, TX 78712 (United States)
We consider the Minimal Supersymmetric Standard Model (MSSM) with varying amounts of non-universality in the soft supersymmetry-breaking contributions to the Higgs scalar masses. In addition to the constrained MSSM (CMSSM) in which these are universal with the soft supersymmetry-breaking contributions to the squark and slepton masses at the input GUT scale, we consider scenarios in which both the Higgs masses are non-universal by the same amount (NUHM1), and scenarios in which they are independently non-universal (NUHM2). As the lightest neutralino is a dark matter candidate, we demand that the relic density of neutralinos not be in conflict with measurements by WMAP and others, and examine the viable regions of parameter space. Prospects for direct detection of neutralino dark matter via elastic scattering in these scenarios are discussed.
OSTI ID:
21410187
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1241; ISSN APCPCS; ISSN 0094-243X
Country of Publication:
United States
Language:
English

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