What do we learn from the CMB observations?

被引：8

作者：

Rubakov, V. A. ^{[1
]}

Vlasov, A. D. ^{[2
]}

机构：

[1] Russian Acad Sci, Inst Nucl Res, Moscow, Russia

[2] Inst Theoret & Expt Phys, Moscow 117259, Russia

来源：

PHYSICS OF ATOMIC NUCLEI | 2012年 / 75卷 / 09期

关键词：

Dark Matter; Atomic Nucleus; Gravitational Wave; Angular Spectrum; Scalar Perturbation;

D O I：

10.1134/S1063778812090116

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

We give an account, at nonexpert and quantitative level, of physics behind the CMB temperature anisotropy and polarization and their peculiar features. We discuss, in particular, how cosmological parameters are determined from the CMB measurements and their combinations with other observations. We emphasize that CMB is the major source of information on the primordial density perturbations and, possibly, gravitational waves, and discuss the implication for our understanding of the extremely early Universe.

引用

页码：1123 / 1141

页数：19

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