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We investigate the parameter space of a specific class of model within thedeflected mirage mediation (DMM) scenario. We look at neutralino properties andcompute the thermal relic density as well as interaction rates with xenondirect detection experiments. We find that there are portions of the parameterspace which are in line with the current WMAP constraints. Further we find thatnone of the investigated parameter space is in conflict with current boundsfrom the Xenon10 experiment and that future large-scale liquid xenonexperiments will probe a large portion of the model space.

Dark matter signals in deflected mirage mediation