Post-Newtonian Dynamics in Dense Star Clusters: Highly Eccentric, Highly Spinning, and Repeated Binary Black Hole Mergers

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	Post-Newtonian Dynamics in Dense Star Clusters: Highly Eccentric, Highly Spinning, and Repeated Binary Black Hole Mergers
	Rodriguez, Carl L.; Amaro-Seoane, Pau; Chatterjee, Sourav; Rasio, Frederic A.
	2018
Source Publication	PHYSICAL REVIEW LETTERS
Volume	120 Issue:15
Document Type	期刊论文
Identifier	http://ir.amss.ac.cn/handle/2S8OKBNM/33805
Collection	中国科学院数学与系统科学研究院
Recommended Citation GB/T 7714	Rodriguez, Carl L.,Amaro-Seoane, Pau,Chatterjee, Sourav,et al. Post-Newtonian Dynamics in Dense Star Clusters: Highly Eccentric, Highly Spinning, and Repeated Binary Black Hole Mergers[J]. PHYSICAL REVIEW LETTERS,2018,120(15).
APA	Rodriguez, Carl L.,Amaro-Seoane, Pau,Chatterjee, Sourav,&Rasio, Frederic A..(2018).Post-Newtonian Dynamics in Dense Star Clusters: Highly Eccentric, Highly Spinning, and Repeated Binary Black Hole Mergers.PHYSICAL REVIEW LETTERS,120(15).
MLA	Rodriguez, Carl L.,et al."Post-Newtonian Dynamics in Dense Star Clusters: Highly Eccentric, Highly Spinning, and Repeated Binary Black Hole Mergers".PHYSICAL REVIEW LETTERS 120.15(2018).

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