Formation of the large-scale structure of the Universe

被引：9
|
作者：
Lukash, V. N. [1 ]
Mikheeva, E. V. [1 ]
Malinovsky, A. M. [1 ]
机构：
[1] Russian Acad Sci, PN Lebedev Phys Inst, Ctr Astro Space, Moscow 117997, Russia
来源：
PHYSICS-USPEKHI | 2011年 / 54卷 / 10期
关键词：
MASS FUNCTION; GALAXIES; MODEL; FLUCTUATIONS; EVOLUTION; CLUSTERS; VELOCITY; BIAS;
D O I：
10.3367/UFNe.0181.201110a.1017
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
In this review, the formation, evolution, and decay of the large-scale structure of the Universe is discussed in the context of observational data, numerical simulations, and the Cosmological Standard Model (CSM). Problems concerning measuring and interpreting cosmological parameters, determining the composition of matter, and normalizing density perturbation spectra are especially highlighted.
引用
收藏
页码：983 / 1005
页数：23
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