Cosmic microwave background observations and cosmology

被引：0

作者：

De Bernardis, P ^{[1
]}

Masi, S ^{[1
]}

机构：

[1] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy

来源：

NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-BASIC TOPICS IN PHYSICS | 2003年 / 118卷 / 10-12期

关键词：

D O I：

10.1393/ncb/i2004-10048-3

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Observations of the Cosmic Microwave Background (CMB) play a pivotal role in the development of modern cosmology. Most of the predictions of the Hot Big Bang model are now experimentally confirmed, and the parameters of the model have recently been constrained to good accuracy. The so-called "Concordance cosmology", derived from observations of the CMB spectrum and anisotropy, from measurements of the large-scale distribution of galaxies, of the expansion of the Universe and of the abundance of light elements, requires significant contributions from dark matter (Omegam similar to 0.3) and dark energy (Omega(Lambda) similar to 0.65). Also, an initial inflation phase is required for the model to be self consistent. Here we focus on CMB anisotropy and CMB polarization observations and on their role in constraining the model.

引用

页码：1071 / 1081

页数：11

共 56 条

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