The conceptually simplest scenario for dark matter (DM) is that it is a stable thermal relic from standard Big Bang cosmology, in many SUSY models the lightest neutralino. The relic density determination selects special regions in SUSY model parameter space with concomitant implications for collider physics, dark matter searches and low energy measurements. By studying various one‐parameter extensions of the much‐studied mSUGRA model (where we relax the untested universality assumptions) constructed to be in accord with the measured relic density, we show that these implications are in general model‐dependent, so that LHC and DM measurements will provide clues to how sparticles acquire their masses. We point out some relatively robust implications for LHC and DM searches and conclude with an outlook for the future.
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10 February 2010
SUSY09: 7th International Conference on Supersymmetry and the Unification of Fundamental Interactions
5–10 June 2008
Boston (Massachusetts)
Research Article|
February 10 2010
Supersymmetry, Dark Matter and the LHC
Xerxes Tata
Xerxes Tata
Department of Physics and Astronomy, University of Hawaii, Honolulu, HI 96825 and Physics Department, University of Wisconsin, Madison, WI 53705
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Xerxes Tata
Department of Physics and Astronomy, University of Hawaii, Honolulu, HI 96825 and Physics Department, University of Wisconsin, Madison, WI 53705
AIP Conf. Proc. 1200, 145–154 (2010)
Citation
Xerxes Tata; Supersymmetry, Dark Matter and the LHC. AIP Conf. Proc. 10 February 2010; 1200 (1): 145–154. https://doi.org/10.1063/1.3327553
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