The Mean Pairwise Peculiar Velocity in Cosmological [ITAL]N[/ITAL]-Body Simulations: Time Variation, Scale Dependence, and the Stable Condition

Author:

Fukushige Toshiyuki,Suto Yasushi

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 8 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Pairwise velocities of dark matter haloes: a test for the Λ cold dark matter model using the bullet cluster;Monthly Notices of the Royal Astronomical Society;2011-11-21

2. Energy ranking preservation in an N-body cosmological simulation;Monthly Notices of the Royal Astronomical Society;2006-07-21

3. PPPM and TreePM Methods on GRAPE Systems for CosmologicalN-Body Simulations;Publications of the Astronomical Society of Japan;2005-12-25

4. Mass-Loss Timescale of Star Clusters in an External Tidal Field. I. Clusters on Circular Orbits;Publications of the Astronomical Society of Japan;2005-02-25

5. Stable clustering, the halo model and non-linear cosmological power spectra;Monthly Notices of the Royal Astronomical Society;2003-06-01

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