Post-Newtonian dynamics in dense star clusters: Binary black holes in the LISA band

doi:10.1103/PhysRevD.99.063003

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	Post-Newtonian dynamics in dense star clusters: Binary black holes in the LISA band
	Kremer, Kyle 1,2; Rodriguez, Carl L.3; Amaro-Seoane, Pau 4,5,6,7; Breivik, Katelyn 8; Chatterjee, Sourav 2,9; Katz, Michael L.1,2; Larson, Shane L.1,2; Rasio, Frederic A.1,2; Samsing, Johan 10; Ye, Claire S.1,2; Zevin, Michael 1,2
	2019-03-06
发表期刊	PHYSICAL REVIEW D
ISSN	2470-0010
卷号	99 期号:6 页码:12
摘要	The dynamical processing of black holes in the dense cores of globular clusters (GCs) makes them efficient factories for producing binary black holes (BBHs). Here we explore the population of BBHs that form dynamically in GCs and may be observable at mHz frequencies or higher with the future space-based gravitational-wave observatory LISA. We use our Monte Carlo stellar dynamics code, which includes gravitational radiation reaction effects for all BH encounters. By creating a representative local universe of GCs, we show that up to dozens of these systems may be resolvable by LISA. Approximately one-third of these binaries will have measurable eccentricities (e > 10(-3)) in the LISA band, and a small number (less than or similar to 5) may evolve from the LISA band to the LIGO band during the LISA mission.
DOI	10.1103/PhysRevD.99.063003
语种	英语
资助项目	National Aeronautics and Space Administration (NASA) ATP Grant[NNX14AP92G] ; National Science Foundation (NSF)[AST-1716762] ; NSF Graduate Research Fellowship Program[DGE-1324585] ; Ramon y Cajal Programme of the Ministry of Economy, Industry and Competitiveness of Spain ; COST Action GWverse[CA16104] ; National Key R&D Program of China[2016YFA0400702] ; NSF of China[11721303] ; NSF[DGE-0948017] ; CIERA ; NASA through Chandra Grant by the Chandra X-ray Observatory Center[TM5-16004X/NAS8-03060] ; Hubble Space Telescope Archival Research (from the Space Telescope Science Institute[HST-AR-14555.001-A] ; Research in Astronomy, Incorporated, under NASA[NAS5-26555] ; NASA[NAS8-03060]
WOS研究方向	Astronomy & Astrophysics ; Physics
WOS类目	Astronomy & Astrophysics ; Physics, Particles & Fields
WOS记录号	WOS:000460660000001
出版者	AMER PHYSICAL SOC
引用统计
文献类型	期刊论文
条目标识符	http://ir.amss.ac.cn/handle/2S8OKBNM/34125
专题	中国科学院数学与系统科学研究院
通讯作者	Kremer, Kyle
作者单位	1.Northwestern Univ, Dept Phys & Astron, Evanston, IL 60202 USA 2.CIERA, Evanston, IL 60202 USA 3.MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA 4.CSIC, ICE, Inst Space Sci, Carrer Can Magrans S-N, Barcelona 08193, Spain 5.IEEC, Campus UAB,Carrer Can Magrans S-N, Barcelona 08193, Spain 6.Chinese Acad Sci, Acad Math & Syst Sci, Inst Appl Math, Beijing 100190, Peoples R China 7.Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 8.Univ Toronto, Canadian Inst Theoret Astrophys, 60 St George St, Toronto, ON M5S 3H8, Canada 9.Tata Inst Fundamental Res, Homi Bhabha Rd, Mumbai 400005, Maharashtra, India 10.Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
推荐引用方式 GB/T 7714	Kremer, Kyle,Rodriguez, Carl L.,Amaro-Seoane, Pau,et al. Post-Newtonian dynamics in dense star clusters: Binary black holes in the LISA band[J]. PHYSICAL REVIEW D,2019,99(6):12.
APA	Kremer, Kyle.,Rodriguez, Carl L..,Amaro-Seoane, Pau.,Breivik, Katelyn.,Chatterjee, Sourav.,...&Zevin, Michael.(2019).Post-Newtonian dynamics in dense star clusters: Binary black holes in the LISA band.PHYSICAL REVIEW D,99(6),12.
MLA	Kremer, Kyle,et al."Post-Newtonian dynamics in dense star clusters: Binary black holes in the LISA band".PHYSICAL REVIEW D 99.6(2019):12.