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20032008
most citedThe survival and disruption of CDM micro-haloes: implications for direct and indirect detection experiments

117 citations · 424 across the 7 of their papers we have counts for

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9 papers · 1 filter

astro-ph200869 cited

Fossil remnants of reionization in the halo of the Milky Way

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

Our recently completed one billion particle Via Lactea II simulation of a Milky Way-sized dark matter halo resolves over 50,000 gravitationally bound clumps orbiting today within t…

astro-ph200876 cited

Formation and accretion history of terrestrial planets from runaway growth through to late time: implications for orbital eccentricity

Ryuji Morishima, Max W. Schmidt, Joachim Stadel +1

Remnant planetesimals might have played an important role in reducing the orbital eccentricities of the terrestrial planets after their formation via giant impacts. However, the po…

astro-ph200873 cited

Discreteness Effects in Lambda Cold Dark Matter Simulations: A Wavelet-Statistical View

Alessandro B. Romeo, Oscar Agertz, Ben Moore +1

The effects of particle discreteness in N-body simulations of Lambda Cold Dark Matter (LambdaCDM) are still an intensively debated issue. In this paper we explore such effects, tak…

astro-ph200788 cited

The formation of ultra-compact dwarf galaxies and nucleated dwarf galaxies

Tobias Goerdt, Ben Moore, Stelios Kazantzidis +3

Ultra compact dwarf galaxies (UCDs) have similar properties as massive globular clusters or the nuclei of nucleated galaxies. Recent observations suggesting a high dark matter cont…

astro-ph2007191 cited

The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures

Victor P. Debattista, Ben Moore, Thomas Quinn +5

Cold dark matter cosmogony predicts triaxial dark matter halos, whereas observations find quite round halos. This is most likely due to the condensation of baryons leading to round…

astro-ph2007128 cited

The Cosmic Code Comparison Project

Katrin Heitmann, Zarija Lukic, Patricia Fasel +11

Current and upcoming cosmological observations allow us to probe structures on smaller and smaller scales, entering highly nonlinear regimes. In order to obtain theoretical predict…