Dark Matter Relic Density and Supersymmetry at the LHC

Details Dark Matter Relic Density and Supersymmetry at the LHC Dark Matter Relic Density and Supersymmetry at the LHC

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aps..tsf.b3004a&link_type=abstract

American Physical Society, 2007 Joint Fall Meeting of the Texas Sections of the APS and AAPT; Zone 13 of SPS, October 18-20, 200

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The theory of Supersymmetry (SUSY) could provide a fundamental link between early Big Bang cosmology and particle physics by providing a possible explanation to the origin and abundances of the Dark Matter. WMAP measurements, in addition to other experimental results, help constrain the SUSY parameter space to a region known as the co-annihilation region where the stau and the neutralino (LSP) are nearly the same mass (mass difference ˜ 5-15GeV). We present one approach to extracting information about the Dark Matter candidate at the LHC in addition to the different parameters of the minimal Supergravity (mSUGRA) model of SUSY.

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