Intermediate-mass Black Holes' Effects on Compact Object Binaries

被引:12
作者
Deme, Barnabas [1 ]
Meiron, Yohai [1 ,2 ]
Kocsis, Bence [1 ]
机构
[1] Eotvos Lorand Univ, Inst Phys, Pazmany Ps 1-A, H-1117 Budapest, Hungary
[2] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada
基金
美国国家科学基金会; 加拿大自然科学与工程研究理事会; 欧洲研究理事会;
关键词
Galactic center; Intermediate-mass black holes; NEUTRON-STAR MERGERS; GALACTIC-CENTER; ALGORITHMIC REGULARIZATION; HYPERVELOCITY STARS; STELLAR CLUSTERS; SECULAR DYNAMICS; AGN DISCS; ORBITS; SEGREGATION; ENCOUNTERS;
D O I
10.3847/1538-4357/ab7921
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Although their existence is not yet confirmed observationally, intermediate-mass black holes (IMBHs) may play a key role in the dynamics of galactic nuclei. In this paper, we neglect the effect of the nuclear star cluster itself and investigate only how a small reservoir of IMBHs influences the secular dynamics of stellar-mass black hole binaries, using N-body simulations. We show that our simplifications are valid and that the IMBHs significantly enhance binary evaporation by pushing the binaries into the Hill-unstable region of parameter space, where they are separated by the supermassive black hole's tidal field. For binaries in the S-cluster region of the Milky Way, IMBHs drive the binaries to merge in up to 1%-6% of cases, assuming five IMBHs within 5 pc of mass 104 M. each. Observations of binaries in the Galactic center may strongly constrain the population of IMBHs therein.
引用
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页数:10
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