The Structure of cold dark matter halos

@article{Navarro1996TheSO,
  title={The Structure of cold dark matter halos},
  author={Julio F. Navarro and Carlos S. Frenk and Simon D. M. White},
  journal={The Astrophysical Journal},
  year={1996},
  volume={462},
  pages={563-575}
}
High resolution N-body simulations show that the density profiles of dark matter halos formed in the standard CDM cosmogony can be fit accurately by scaling a simple “universal” profile. Regardless of their mass, halos are nearly isothermal over a large range in radius, but significantly shallower than r -2 near the center and steeper than r -2 in the outer regions. The characteristic overdensity of a halo correlates strongly with halo mass in a manner consistent with the mass dependence of the… 
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TLDR
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