中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Secular evolution of compact binaries revolving around a spinning massive black hole

文献类型:期刊论文

作者Fang, Y; Huang, QG
刊名PHYSICAL REVIEW D
出版日期2019
卷号99期号:10页码:103005
关键词GRAVITATIONAL-WAVES PERTURBATIONS MOTION MASSES
ISSN号2470-0010
DOI10.1103/PhysRevD.99.103005
英文摘要The leading order effect of the spin of a distant supermassive black hole on the orbit of a compact binary revolving around it appears at the 1.5 post Newtonian expansion through coupling with the inner and outer orbital angular momenta and makes an oscillating characteristic contribution to the secular evolution of the compact binary eccentricity over a long timescale compared to the Kozai-Lidov dynamics caused by a nonspinning supermassive black hole.
学科主题Astronomy & Astrophysics ; Physics
语种英语
源URL[http://ir.itp.ac.cn/handle/311006/23434]  
专题理论物理研究所_理论物理所1978-2010年知识产出
作者单位1.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
2.Univ Chinese Acad Sci, Sch Phys Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
3.Hunan Normal Univ, Synerget Innovat Ctr Quantum Effects & Applicat, 36 Lushan Lu, Changsha 410081, Hunan, Peoples R China
4.[Fang, Yun
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Fang, Y,Huang, QG. Secular evolution of compact binaries revolving around a spinning massive black hole[J]. PHYSICAL REVIEW D,2019,99(10):103005.
APA Fang, Y,&Huang, QG.(2019).Secular evolution of compact binaries revolving around a spinning massive black hole.PHYSICAL REVIEW D,99(10),103005.
MLA Fang, Y,et al."Secular evolution of compact binaries revolving around a spinning massive black hole".PHYSICAL REVIEW D 99.10(2019):103005.

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来源:理论物理研究所

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