The cosmic microwave background radiation

被引：52

作者：

Gawiser, E

Silk, J

机构：

[1] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[2] Univ Oxford, Dept Phys Astrophys, Oxford OX1 3NP, England

[3] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

[4] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

[5] Univ Calif Berkeley, Ctr Particle Astrophys, Berkeley, CA 94720 USA

来源：

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2000年 / 333卷 / 1-6期

关键词：

cosmology; cosmic microwave background;

D O I：

10.1016/S0370-1573(00)00025-9

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We summarize the theoretical and observational status of the study of the Cosmic Microwave Background radiation. Its thermodynamic spectrum is a robust prediction of the Hot Big Bang cosmology and has been confirmed observationally. There are now 75 observations of Cosmic Microwave Background anisotropy, which we present in a table with references. We discuss the theoretical origins of these anisotropies and explain the standard jargon associated with their observation. (C) 2000 Elsevier Science B.V. All rights reserved.

引用

页码：245 / 267

页数：23

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