Gravitational waves from binary black holes as probes of the structure formation history

被引：5
|
作者：
Nakama, Tomohiro [1 ]
机构：
[1] Hong Kong Univ Sci & Technol, Jockey Club Inst Adv Study, Hong Kong, Peoples R China
来源：
PHYSICS OF THE DARK UNIVERSE | 2020年 / 28卷
关键词：
COSMIC STAR-FORMATION; DARK-MATTER; ENRICHMENT; GALAXIES;
D O I：
10.1016/j.dark.2020.100476
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Gravitational-wave detectors on earth have detected gravitational waves from merging compact objects in the local Universe. In future we will detect gravitational waves from higher-redshift sources, which trace the high-redshift structure formation history. That is, by observing high-redshift gravitational-wave events we will be able to probe structure formation history. This will provide additional insight into the early Universe when primordial fluctuations are generated and also into the nature of dark matter. (C) 2020 Elsevier B.V. All rights reserved.
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页数：4
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