Assisted inspirals of stellar mass black holes embedded in AGN discs: Solving the 'final au problem'

Nicholas C. Stone*, Brian D. Metzger, Zoltán Haiman

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

323 Scopus citations

Abstract

We explore the evolution of stellar mass black hole binaries (BHBs) which are formed in the self-gravitating discs of active galactic nuclei (AGN). Hardening due to three-body scattering and gaseous drag are effective mechanisms that reduce the semimajor axis of a BHB to radii where gravitational waves take over, on time-scales shorter than the typical lifetime of the AGN disc. Taking observationally motivated assumptions for the rate of star formation in AGN discs, we find a rate of disc-induced BHB mergers (R ~ 3 yr-1 Gpc-3, but with large uncertainties) that is comparable with existing estimates of the field rate of BHB mergers, and the approximate BHB merger rate implied by the recent Advanced LIGO detection of GW150914. BHBs formed thorough this channel will frequently be associated with luminous AGN, which are relatively rare within the sky error regions of future gravitationalwave detector arrays. This channel could also possess a (potentially transient) electromagnetic counterpart due to super-Eddington accretion on to the stellar mass black hole following the merger.

Original languageAmerican English
Pages (from-to)946-954
Number of pages9
JournalMonthly Notices of the Royal Astronomical Society
Volume464
Issue number1
DOIs
StatePublished - 1 Jan 2017
Externally publishedYes

Bibliographical note

Publisher Copyright:
© 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.

Keywords

  • Galaxies: nuclei
  • Gravitational waves
  • Quasars: general
  • Quasars: supermassive black holes

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