Merger Rate Distribution of Primordial Black Hole Binaries

doi:10.3847/1538-4357/aad6e2

ITP OpenIR > SCI期刊论文

	Chen, ZC ; Huang, QG
	Merger Rate Distribution of Primordial Black Hole Binaries
Source Publication	ASTROPHYSICAL JOURNAL
Language	英语
Keyword	MASS
Abstract	Up to now several gravitational-wave events from the coalescences of black hole binaries have been reported by LIGO/VIRGO, and imply that black holes should have an extended mass function. We work out the merger rate distribution of primordial black hole (PBH) binaries with a general mass function by taking into account the torques by all PBHs and linear density perturbations. In the future, many more coalescences of black hole binaries are expected to be detected, and the one-dimensional and two-dimensional merger rate distributions will be crucial for reconstructing the mass function of PBHs.
	2018
ISSN	0004-637X
Volume	864 Issue:1 Pages:61
Subject Area	Astronomy & Astrophysics
MOST Discipline Catalogue	Astronomy & Astrophysics
DOI	10.3847/1538-4357/aad6e2
Indexed By	SCIE
Citation statistics	Cited Times:32[WOS] [WOS Record] [Related Records in WOS]
Document Type	期刊论文
Identifier	http://ir.itp.ac.cn/handle/311006/22828
Collection	SCI期刊论文计算平台成果
Affiliation	1.[Chen, Zu-Cheng 2.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China 3.Univ Chinese Acad Sci, Sch Phys Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China 4.Yangzhou Univ, Coll Phys Sci & Technol, Ctr Gravitat & Cosmol, Yangzhou 225009, Jiangsu, Peoples R China 5.Hunan Normal Univ, Synerget Innovat Ctr Quantum Effects & Applicat, Changsha 410081, Hunan, Peoples R China
Recommended Citation GB/T 7714	Chen, ZC,Huang, QG. Merger Rate Distribution of Primordial Black Hole Binaries[J]. ASTROPHYSICAL JOURNAL,2018,864(1):61.
APA	Chen, ZC,&Huang, QG.(2018).Merger Rate Distribution of Primordial Black Hole Binaries.ASTROPHYSICAL JOURNAL,864(1),61.
MLA	Chen, ZC,et al."Merger Rate Distribution of Primordial Black Hole Binaries".ASTROPHYSICAL JOURNAL 864.1(2018):61.

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