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N-body simulations predict that cold dark matter (CDM) halo-assembly occurs in two phases: (i) a fast-accretion phase with a rapidly deepening potential well; and (ii) a slow-accretion phase character...
In order to explain the main characteristics of the observed population of extrasolar planets and the giant planets in the Solar System, we need to get a clear understanding of which are the initial c...
We develop a new method which measures the projected density distribution wp(rp)n of photometric galaxies surrounding a set of spectroscopically-identified galaxies, and simultaneously the projected c...
Flat central density profiles from scalar field dark matter halos
Two Scenarios for the Formation of Cuspy Density Profiles in Elliptical Galaxies
Density Profiles of Dark Halos from their Mass Accretion Histories
Simulated dark matter haloes are tted by self-similar, universal density pro les, where the scaled parameters depend only on a scaled (truncation) radius,  = R=r0, which, in turn, is supposed to b...
A NUMERICAL FIT OF ANALYTICAL TO SIMULATED DENSITY PROFILES IN DARK MATTER HALOES.

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