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