Evolution of Dark Matter Halo Density Profiles and Substructure from $\Lambda$CDM Simulations

Abstract
We use , although a weakly shallower subhalo profile is favored by the data. We discuss the implications that our results have on gravitational lensing studies of halo structure.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

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