Constraining self-interacting dark matter with the Milky Way’s dwarf spheroidals

@article{Zavala2013ConstrainingSD,
  title={Constraining self-interacting dark matter with the Milky Way’s dwarf spheroidals},
  author={Jes{\'u}s Zavala and Mark Vogelsberger and UW MatthewG.Walker and Pi and HarvardCfA},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2013},
  volume={431}
}
Self-Interacting Dark Matter is an attractive alternative to the Cold Dark Matter paradigm only if it is able to substantially reduce the central densities of dwarf-size haloes while keeping the densities and shapes of cluster-size haloes within current constraints. Given the seemingly stringent nature of the latter, it was thought for nearly a decade that Self-Interacting Dark Matter would be viable only if the cross section for self-scattering was strongly velocitydependent. However, it has… Expand

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