{ "id": "1807.09281", "version": "v1", "published": "2018-07-24T18:00:09.000Z", "updated": "2018-07-24T18:00:09.000Z", "title": "Intermediate-Mass Ratio Inspirals in Galactic Nuclei", "authors": [ "Giacomo Fragione", "Nathan Leigh" ], "comment": "8 pages, 5 figures, 1 Table", "categories": [ "astro-ph.GA", "astro-ph.HE" ], "abstract": "In this paper, we study the secular dynamical evolution of binaries composed of intermediate-mass and stellar-mass black holes (IMBHs and SBHs, respectively) in orbit about a central super-massive black hole (SMBH) in galactic nuclei. Such BH triplets could form via the inspiral of globular clusters toward galactic nuclei due to dynamical friction, or even major/minor galaxy mergers. We perform, for reasonable initial conditions that we justify, sophisticated $N$-body simulations that include both regularization and Post-Newtonian corrections. We find that mass segregation combined with Kozai-Lidov oscillations induced by the primary SMBH can effectively merge IMBH-SBH binaries on time-scales much shorter than gravitational wave emission alone. Moreover, the rate of such extreme mass ratio inspirals could be high ($\\sim 1\\ \\mathrm{Gpc}^{-3}\\ \\mathrm{yr}^{-1}$) in the local Universe, but these are expected to be associated with recent GC infall or major/minor mergers, making the observational signatures of such events (e.g., tidal debris) good diagnostics for searching for SMBH-IMBH-SBH mergers. A small fraction could also be associated with tidal disruption events by the IMBH-SBH during inspiral.", "revisions": [ { "version": "v1", "updated": "2018-07-24T18:00:09.000Z" } ], "analyses": { "keywords": [ "galactic nuclei", "intermediate-mass ratio inspirals", "extreme mass ratio inspirals", "central super-massive black hole", "tidal disruption events" ], "note": { "typesetting": "TeX", "pages": 8, "language": "en", "license": "arXiv", "status": "editable" } } }