4.7 Article

Pairwise velocities of dark matter haloes: a test for the Λ cold dark matter model using the bullet cluster

期刊

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

  1. Nevada NASA
  2. NASA [NNX10AJ82H, NNX08AE57A]
  3. NSF [AST-0807491]
  4. UNLV
  5. Texas Advanced Computing Center (TACC)
  6. National Institute for Computational Sciences (NICS)
  7. Direct For Mathematical & Physical Scien
  8. Division Of Astronomical Sciences [0807491] Funding Source: National Science Foundation
  9. NASA [102264, NNX10AJ82H, 130122, NNX08AE57A] Funding Source: Federal RePORTER

向作者/读者索取更多资源

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.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.7
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据