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Simulated dark matter profiles are often modelled as a ‘NFW’ density profile rather than a single power law. Recently, attention has turned to the rather rigorous power-law behaviour exhibited by the ‘pseudo phase-space density’ of the dark matter halo, which is defined dimensionally in terms of the local density and velocity dispersion of the dark matter particles. The non-power-law behaviour ...
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ژورنال
عنوان ژورنال: Nature Physics
سال: 2008
ISSN: 1745-2473,1745-2481
DOI: 10.1038/nphys946