activity
20062026
most citedClumps and streams in the local dark matter distribution

882 citations · 5.5k across the 184 of their papers we have counts for

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7 papers · 1 filter

astro-ph2008★ 76 cited

The Graininess of Dark Matter Haloes

Marcel Zemp, Jürg Diemand, Michael Kuhlen +5

We use the recently completed one billion particle Via Lactea II LambdaCDM simulation to investigate local properties like density, mean velocity, velocity dispersion, anisotropy,…

astro-ph2008★ 389 cited

Quantifying the heart of darkness with GHALO - a multi-billion particle simulation of our galactic halo

Joachim Stadel, Doug Potter, Ben Moore +5

We perform a series of simulations of a Galactic mass dark matter halo at different resolutions, our largest uses over three billion particles and has a mass resolution of 1000 M_s…

astro-ph2008★ 882 cited

Clumps and streams in the local dark matter distribution

J. Diemand, M. Kuhlen, P. Madau +4

In cold dark matter cosmological models, structures form and grow by merging of smaller units. Numerical simulations have shown that such merging is incomplete; the inner cores of…

astro-ph2006★ 623 cited

Fundamental differences between SPH and grid methods

Oscar Agertz, Ben Moore, Joachim Stadel +17

We have carried out a hydrodynamical code comparison study of interacting multiphase fluids. The two commonly used techniques of grid and smoothed particle hydrodynamics (SPH) show…

astro-ph2006

Dark Satellites and Cosmic Reionization

Andrea V. Maccio', Ben Moore, Joachim Stadel +1

A possible explanation of the present discrepancy between the abundance of galactic subhaloes predicted by N-Body simulations with those observed in the Local Group is presented. W…

astro-ph2006★ 555 cited

Concentration, Spin and Shape of Dark Matter Haloes: Scatter and the Dependence on Mass and Environment

Andrea V. Maccio', Aaron A. Dutton, Frank C. van den Bosch +3

We use a series of cosmological N-body simulations for a flat LCDM cosmology to investigate the properties of dark matter haloes in the mass range 3.0e9-3.0e13 Msun. These properti…