VELOCITY DIFFERENCES AS A PROBE OF NON-GAUSSIAN DENSITY FIELDS

Citation
P. Catelan et Rj. Scherrer, VELOCITY DIFFERENCES AS A PROBE OF NON-GAUSSIAN DENSITY FIELDS, The Astrophysical journal, 445(1), 1995, pp. 1-6
Citations number
44
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
0004637X
Volume
445
Issue
1
Year of publication
1995
Part
1
Pages
1 - 6
Database
ISI
SICI code
0004-637X(1995)445:1<1:VDAAPO>2.0.ZU;2-1
Abstract
We examine the multipoint linear velocity field for non-Gaussian model s as a probe of non-Gaussian behavior. The two-point velocity correlat ion is not a useful indicator of a non-Gaussian density field, since i t depends only on the power spectrum, even for non-Gaussian models. Ho wever, we show that the distribution of velocity differences v(1) - v( 2), where v(1) and v(2) are measured at the points r(1) and r(2), resp ectively, is a good probe of non-Gaussian behavior, in that p(v(1) - v (2)) tends to be non-Gaussian when the density field is non-Gaussian. As an example, we examine the behavior of p(v(1) - v(2)) for non-Gauss ian seed models, in which the density field is the convolution of a di stribution of points with a set of density profiles. We apply these re sults to the global texture model.