Asymmetric Dark Matter
arXiv:1308.4513 · doi:10.1063/1.4883455
Abstract
We review the theoretical framework underlying models of asymmetric dark matter, describe astrophysical constraints which arise from observations of neutron stars, and discuss the prospects for detecting asymmetric dark matter.
8 pages, 1 figure, LaTeX. Submitted to the proceedings of PPC 2013. v2 and v3: typos fixed and references corrected
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Cited by in corpus (6)
- Bounds on self-interacting fermion dark matter from observations of old neutron stars
- Dark matter relic density in Gauss-Bonnet braneworld cosmology
- Asymmetric dark matter in braneworld cosmology
- Dark matter relic density in scalar-tensor gravity revisited
- Stellar convective cores as dark matter probes
- Dark matter imprint on B neutrino spectrum