Dark matter, density perturbations, and structure formation

被引:0
|
作者
A. Del Popolo
机构
[1] Boğçi University,Physics Department
[2] Università Statale di Bergamo,Dipartimento di Matematica
[3] Istanbul Technical University,Ayazaga Campus, Faculty of Science and Letters
来源
Astronomy Reports | 2007年 / 51卷
关键词
95.30.Sf; 95.35.+d; 98.70.Vc; 98.80.Bp; 98.80.Jk;
D O I
暂无
中图分类号
学科分类号
摘要
This paper provides a review of the types of dark matter that are thought to be fundamental components of the Universe, and their role in the origin and evolution of structures, together with some new original results concerning improvements to the spherical collapse model. In particular, we show how the spherical collapse model is modified when dynamical friction and tidal torques are taken into account.
引用
收藏
页码:169 / 196
页数:27
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