The distribution of counts in cells in the non-linear regime

被引:0
作者
Sheth, RK
机构
关键词
galaxies; clusters; general; evolution; formation; cosmology; theory; dark matter;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Press-Schechter approach is used to provide an approximate description of the counts in cells distribution in the non-linear regime. Simple, illustrative models for the spatial distribution and internal structure of Press-Schechter clumps are assumed. Then, these distributions of non-linear Press-Schechter clumps are smoothed with a large-scale filter. The resulting evolved, smoothed distributions of counts in (large) cells are compared with the predictions of linear and quasi-linear theory. The agreement between these Press-Schechter models and the quasi-linear analyses increases as the initial power on large scales decreases. These simple models are also used to compute estimates of the skewness in the highly non-linear regime. The non-linear, Press-Schechter values of the skewness and higher order moments are scale-dependent, and are in good agreement with the values measured, in the non-linear regime, in N-body simulations. For initial power spectra of current interest, the quasi-linear value of the skewness is always within a factor of two or three of the non-linear values in these models.
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页码:1124 / 1132
页数:9
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