Speaker
Christopher Redino
(S)
Description
The motivations and prospects for detecting separately identifiable dark matter candidates in a SUSY framework at the LHC are discussed. The majority of SUSY parameter space does not predict neutralinos that match the observed dark matter relic abundance, but a second candidate can easily be introduced. This parameter space is interesting because it contains models with a low amount of electroweak fine tuning.
Author
Christopher Redino
(S)
