Cores in dwarf galaxies from dark matter with a Yukawa potential.

Phys Rev Lett

Institute for Theory & Computation, Harvard University, 60 Garden Street, Cambridge, Massachusetts 02138, USA.

Published: April 2011

We show that cold dark matter particles interacting through a Yukawa potential could naturally explain the recently observed cores in dwarf galaxies without affecting the dynamics of objects with a much larger velocity dispersion, such as clusters of galaxies. The velocity dependence of the associated cross section as well as the possible exothermic nature of the interaction alleviates earlier concerns about strongly interacting dark matter. Dark matter evaporation in low-mass objects might explain the observed deficit of satellite galaxies in the Milky Way halo and have important implications for the first galaxies and reionization.

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http://dx.doi.org/10.1103/PhysRevLett.106.171302DOI Listing

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