2013/07/02 by Mathew McCaskey, McCaskey, Mathew, Gabe Shaughnessy +1
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Atmospheric Ozone and Climate #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Experiment (hep-ex) #High Energy Physics - Phenomenology (hep-ph) #hep-ex #hep-ph
paper · pdf · doi:10.48550/arxiv.1307.0851
3 pages, 1 figure, Snowmass whitepaper submission
arxiv created 2013/07/02 · openalex publication_date 2013/07/02 · arxiv updated 2013/07/04 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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.