期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 419, 期 4, 页码 3560-3570出版社
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2011.20000.x
关键词
galaxies: clusters: general; galaxies: evolution; galaxies: formation; cosmology: theory; dark matter
资金
- Nevada NASA
- NASA [NNX10AJ82H, NNX08AE57A]
- NSF [AST-0807491]
- UNLV
- Texas Advanced Computing Center (TACC)
- National Institute for Computational Sciences (NICS)
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [0807491] Funding Source: National Science Foundation
- NASA [102264, NNX10AJ82H, 130122, NNX08AE57A] Funding Source: Federal RePORTER
The existence of a bullet cluster (such as 1E 0657-56) poses a challenge to the concordance ? cold dark matter (?CDM) model. Here we investigate the velocity distribution of dark matter (DM) halo pairs in large N-body simulations with differing box sizes (250 h-1 Mpc Gpc) and resolutions. We examine various basic statistics such as the halo masses, pairwise halo velocities (v12), collisional angles and pair separation distances. We then compare our results to the initial conditions required to reproduce the observational properties of 1E 0657-56 in non-cosmological hydrodynamical simulations.
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