English

Velocity Differences as a Probe of Non--Gaussian Density Fields

Astrophysics 2009-10-22 v1

Abstract

We examine the multi--point velocity field for non--Gaussian models as a probe of non--Gaussian behavior. The two--point velocity correlation is not a useful indicator of a non--Gaussian density field, since it depends only on the power spectrum, even for non--Gaussian models. However, we show that the distribution of velocity differences \bfv1\bfv2\bfv_1 - \bfv_2, where \bfv1\bfv_1 and \bfv2\bfv_2 are measured at the points \bfr1\bfr_1 and \bfr2\bfr_2, respectively, is a good probe of non--Gaussian behavior, in that p(\bfv1\bfv2)p(\bfv_1 - \bfv_2) tends to be non--Gaussian whenever the density field is non--Gaussian. As an example, we examine the behavior of p(\bfv1\bfv2)p(\bfv_1 - \bfv_2) for non--Gaussian seed models, in which the density field is the convolution of a distribution of points with a set of density profiles. We apply these results to the global texture model.

Cite

@article{arxiv.astro-ph/9405011,
  title  = {Velocity Differences as a Probe of Non--Gaussian Density Fields},
  author = {Paolo Catelan and Robert J. Scherrer},
  journal= {arXiv preprint arXiv:astro-ph/9405011},
  year   = {2009}
}

Comments

18 pages, LATEX style, SISSA-37-94-A, OSU-TA-4-94

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