{ "id": "1102.4855", "version": "v1", "published": "2011-02-23T21:07:00.000Z", "updated": "2011-02-23T21:07:00.000Z", "title": "Fast coalescence of massive black hole binaries from mergers of galactic nuclei: implications for low-frequency gravitational-wave astrophysics", "authors": [ "Miguel Preto", "Ingo Berentzen", "Peter Berczik", "Rainer Spurzem" ], "comment": "6 pages, 4 figures, 1 table. Submitted to ApJL", "categories": [ "astro-ph.GA", "gr-qc" ], "abstract": "We investigate a purely stellar dynamical solution to the Final Parsec Problem. Galactic nuclei resulting from major mergers are not spherical, but show some degree of triaxiality. With $N$-body simulations, we show that massive black hole binaries (MBHB) hosted by them will continuously interact with stars on centrophilic orbits and will thus inspiral---in much less than a Hubble time---down to separations at which gravitational wave (GW) emission is strong enough to drive them to coalescence. Such coalescences will be important sources of GWs for future space-borne detectors such as the {\\it Laser Interferometer Space Antenna} (LISA). Based on our results, we expect that LISA will see between $\\sim 10$ to $\\sim {\\rm few} \\times 10^2$ such events every year, depending on the particular MBH seed model as obtained in recent studies of merger trees of galaxy and MBH co-evolution. Orbital eccentricities in the LISA band will be clearly distinguishable from zero with $e \\gtrsim 0.001-0.01$.", "revisions": [ { "version": "v1", "updated": "2011-02-23T21:07:00.000Z" } ], "analyses": { "keywords": [ "massive black hole binaries", "low-frequency gravitational-wave astrophysics", "galactic nuclei", "fast coalescence", "implications" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/2041-8205/732/2/L26", "journal": "The Astrophysical Journal", "year": 2011, "month": "May", "volume": 732, "number": 2 }, "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable", "inspire": 890687, "adsabs": "2011ApJ...732L..26P" } } }