Formation of Supermassive Black Hole Seeds

被引：120

作者：

Latif, Muhammad A. ^{[1
,2
]}

Ferrara, Andrea ^{[3
]}

机构：

[1] Univ Paris 06, Sorbonne Univ, Inst Astrophys Paris, 98 Bis Bd Arago, F-75014 Paris, France

[2] CNRS, UMR 7095, 98 Bis Bd Arago, F-75014 Paris, France

[3] Scuola Normale Super Pisa, Piazza Cavalieri 7, I-56126 Pisa, Italy

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | 2016年 / 33卷

基金：

美国国家科学基金会;

关键词：

(galaxies:) quasars: supermassive black holes; cosmology: theory; galaxies: high-redshift; INITIAL MASS FUNCTION; HIGH-REDSHIFT FORMATION; DIGITAL SKY SURVEY; PRIMORDIAL STAR-FORMATION; ATOMIC COOLING HALOES; POPULATION-III STARS; YOUNG OPEN CLUSTERS; DARK-MATTER HALOES; TO; QUASARS; DIRECT COLLAPSE;

D O I：

10.1017/pasa.2016.41

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The detection of quasars at z > 6 unveils the presence of supermassive black holes of a few billion solar masses. The rapid formation process of these extreme objects remains a fascinating and open issue. Such discovery implies that seed black holes must have formed early on, and grown via either rapid accretion or BH/galaxy mergers. In this theoretical review, we discuss in detail various BH seed formation mechanisms and the physical processes at play during their assembly. We discuss the three most popular BH formation scenarios, involving the (i) core-collapse of massive stars, (ii) dynamical evolution of dense nuclear star clusters, (iii) collapse of a protogalactic metal free gas cloud. This article aims at giving a broad introduction and an overview of the most advanced research in the field.

引用

页数：16

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