In the beginning: the first sources of light and the reionization of the universe

被引:866
作者
Barkana, R
Loeb, A
机构
[1] Inst Adv Study, Princeton, NJ 08540 USA
[2] Harvard Univ, Dept Astron, Cambridge, MA 02138 USA
来源
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2001年 / 349卷 / 02期
关键词
D O I
10.1016/s0370-1573(01)00019-9
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The formation of the first stars and quasars marks the transformation of the universe from its smooth initial state to its clumpy current state. In popular cosmological models, the first sources of light began to form at a redshift z=30 and reionized most of the hydrogen in the universe by z=7. Current observations are at the threshold of probing the hydrogen reionization epoch. The study of high-redshift sources is likely to attract major attention in observational and theoretical cosmology over the next decade. (C) 2001 Elsevier Science B.V. All rights reserved.
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收藏
页码:126 / 238
页数:113
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