journal article Open Access Dec 01, 2021

Symmetry Breaking in Dynamical Encounters in the Disks of Active Galactic Nuclei

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Abstract
Abstract
The disks of active galactic nuclei (AGNs) may be important sites of binary black hole (BBH) mergers. Here we show via numerical experiments with the high-accuracy, high-precision code SpaceHub that broken symmetry in dynamical encounters in AGN disks can lead to asymmetry between prograde and retrograde BBH mergers. The direction of the hardening asymmetry depends on the initial binary semimajor axis. Under the assumption that the spin of the BHs becomes aligned with the angular momentum of the disk on a short timescale compared with the encounter timescale, an asymmetric distribution of mass-weighted projected spin χ
eff is predicted in LIGO–Virgo detections of BBH mergers from AGN disks. In particular, this model predicts that positive χ
eff BBH mergers are most likely for encounters with massive tertiaries in migration traps at radial distances ≳500–600 gravitational radii.
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Citations
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References
Details
Published
Dec 01, 2021
Vol/Issue
923(2)
Pages
L23
License
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Funding
NSF Award: AST-200683
Simons Foundation Award: 533845
FONDECYT INICIACION Award: 11180005
Millenium Nucleus Award: NCN19-058
Cite This Article
Yi-Han Wang, Barry McKernan, Saavik Ford, et al. (2021). Symmetry Breaking in Dynamical Encounters in the Disks of Active Galactic Nuclei. The Astrophysical Journal Letters, 923(2), L23. https://doi.org/10.3847/2041-8213/ac400a