The NMSSM at the Cosmic Frontier for Snowmass 2013

Understand

We examine the NMSSM at the cosmic frontier in the post Higgs discovery world.

• For DM relic abundance consistent with measurement, we find the neutralino can either be singlino or bino dominated.
• Wino and higgsino DM generally yield a lower abundance, but offer opportunities of detection at IceCube.
• For both cases, future SI direct detection experiments cover a majority of the model, including nearly all of the bino and higgsino scenarios.