Cosmic Microwave Background cosmology - New economy model universe

被引：0

作者：

Smoot, GF ^{[1
]}

机构：

[1] Univ Calif Berkeley, LBNL, Berkeley, CA 94720 USA

来源：

PARTICLE PHYSICS AND COSMOLOGY: THE INTERFACE | 2005年 / 188卷

关键词：

CMB; cosmology; Sachs-Wolf plateau; acoustic peaks; damping tail; polarisation; foregrounds;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review the CMB spectrum and the upper limits on the effects which would distort the Planck black-body distribution, such as Compton scattering, reionisation, plasma effects. The experimental analysis of the angular anisotropies is discussed, as well as the physics pertinent to the different angular momentum regions. The connection between cosmology and the observed inhomogeneities and the determination of the cosmological parameters are summarised, as well as the underlying assumptions. The physical origin of the polarisation of the CMB is explained, and the first experimental results are recalled.

引用

页码：279 / 310

页数：32

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