Skewed exponential pairwise velocities from gaussian initial

Conditions Roman Juszkiewicz, Karl B. Fisher, Istvan Szapudi

Research output: Contribution to journalArticle

27 Citations (Scopus)

Abstract

Using an Eulerian perturbative calculation, we show that the distribution of relative pairwise velocities .that arises from the gravitational instability of Gaussian density fluctuations has asymmetric (skewed) exponential tails. The negative skewness is induced by the negative mean streaming velocity of pairs (the infall prevails over expansion), while the exponential tails arise because the relative pairwise velocity is a number-weighted, not a volume-weighted, statistic. The derived probability distribution is compared with N-body simulations and is shown to provide a reasonable fit.

Original languageEnglish
Pages (from-to)L1-L4
JournalAstrophysical Journal
Volume504
Issue number1 PART II
Publication statusPublished - Jan 1 1998

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Keywords

  • Galaxies: Interactions
  • Large-scale structure of universe

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Juszkiewicz, C. R., Fisher, K. B., & Szapudi, I. (1998). Skewed exponential pairwise velocities from gaussian initial. Astrophysical Journal, 504(1 PART II), L1-L4.