Early galaxy formation and its large-scale effects

被引：330
作者：
Dayal, Pratika [1 ]
Ferrara, Andrea [2 ]
机构：
[1] Univ Groningen, Kapteyn Astron Inst, Landleven 12, NL-9717 AD Groningen, Netherlands
[2] Scuola Normale Super Pisa, Piazza Cavalieri 7, I-56126 Pisa, Italy
来源：
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2018年 / 780卷
基金：
欧盟地平线“2020”;
关键词：
High-Redshift; Intergalactic medium; Galaxy formation; First stars; Reionization; Cosmology theory; LY-ALPHA-EMITTERS; COLD DARK-MATTER; LYMAN-BREAK GALAXIES; STAR-FORMING GALAXIES; HIGH-REDSHIFT GALAXIES; ULTRAVIOLET LUMINOSITY DENSITY; HUBBLE-SPACE-TELESCOPE; POPULATION-III STARS; 1ST BILLION YEARS; ULTRA-DEEP FIELD;
D O I：
10.1016/j.physrep.2018.10.002
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
Galaxy formation is at the heart of our understanding of cosmic evolution. Although there is a consensus that galaxies emerged from the expanding matter background by gravitational instability of primordial fluctuations, a number of additional physical processes must be understood and implemented in theoretical models before these can be reliably used to interpret observations. In parallel, the astonishing recent progresses made in detecting galaxies that formed only a few hundreds of million years after the Big Bang is pushing the quest for more sophisticated and detailed studies of early structures. In this review, we combine the information gleaned from different theoretical models/studies to build a coherent picture of the Universe in its early stages which includes the physics of galaxy formation along with the impact that early structures had on large-scale processes as cosmic reionization and metal enrichment of the intergalactic medium. (C) 2018 Elsevier B.V. All rights reserved.
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页码：1 / 64
页数：64
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