Journal article
Intermediate-mass black holes' effects on compact object binaries
- Abstract:
- 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 ${M}_{\odot }$ each. Observations of binaries in the Galactic center may strongly constrain the population of IMBHs therein.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, 1.1MB, Terms of use)
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- Publisher copy:
- 10.3847/1538-4357/ab7921
Authors
- Publisher:
- IOP Publishing
- Journal:
- The Astrophysical Journal More from this journal
- Volume:
- 892
- Issue:
- 2
- Article number:
- 130
- Publication date:
- 2020-04-06
- Acceptance date:
- 2020-02-21
- DOI:
- EISSN:
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1538-4357
- ISSN:
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0004-637X
- Language:
-
English
- Keywords:
- Pubs id:
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1128023
- Local pid:
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pubs:1128023
- Deposit date:
-
2020-08-24
Terms of use
- Copyright holder:
- The American Astronomical Society.
- Copyright date:
- 2020
- Rights statement:
- ©2020. The American Astronomical Society.
- Notes:
- Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
- Licence:
- CC Attribution (CC BY)
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