A LARGE-SCALE STRUCTURE MODEL FOR GRAVITATIONAL LENSING

被引:0
|
作者
BARTELMANN, M
SCHNEIDER, P
机构
关键词
COSMOLOGY; GRAVITATIONAL LENSING;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A large-scale structure formation model is presented which seems appropriate for some of the purposes of gravitational lensing. It is based on the adhesion approximation, which allows for a fast implementation of the time transfer of initial density perturbations. We apply a simple, but analytically tractable galaxy formation scheme to the model which is shown to yield the correct two-point correlation properties and the observed distance scale between galaxy clusters. Some of the lensing properties of the simulated matter distribution are investigated, and the impact of galaxy-galaxy correlations on lensing is studied using nearest-neighbor distance distributions. The results are obtained for both the HDM and CDM cosmogonies.
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页码:413 / 422
页数:10
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