VELOCITY DIFFERENCES AS A PROBE OF NON-GAUSSIAN DENSITY FIELDS

被引:10
|
作者
CATELAN, P
SCHERRER, RJ
机构
[1] SISSA,SCH ADV INT STUDIES,I-34014 TRIESTE,ITALY
[2] OHIO STATE UNIV,DEPT PHYS,COLUMBUS,OH 43210
来源
ASTROPHYSICAL JOURNAL | 1995年 / 445卷 / 01期
关键词
COSMOLOGY; THEORY; GALAXIES; CLUSTERS; GENERAL; GALAXIES DISTANCES AND REDSHIFTS; LARGE-SCALE STRUCTURE OF UNIVERSE;
D O I
10.1086/175666
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We examine the multipoint linear 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 v(1) - v(2), where v(1) and v(2) are measured at the points r(1) and r(2), respectively, 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-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.
引用
收藏
页码:1 / 6
页数:6
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