Journal
ASTROPHYSICAL JOURNAL
Volume 634, Issue 2, Pages 921-927Publisher
IOP PUBLISHING LTD
DOI: 10.1086/497108
Keywords
accretion, accretion disks; black hole physics; galaxies : active; galaxies : nuclei; gravitational waves
Categories
Ask authors/readers for more resources
Angular momentum loss to circumbinary gas provides a possible mechanism for overcoming the last parsec'' problem and allowing the most massive black hole binaries formed from galactic mergers to coalesce. Here we show that if gas disks also catalyze the merger of the somewhat lower mass binaries detectable with the Laser Interferometer Space Antenna (LISA), then there may be a purely gravitational wave signature of the role of gas in the form of a small but finite eccentricity just prior to merger. Numerical simulations suggest that eccentricity, excited by the interaction between the binary and surrounding gas disk, is only partially damped during the final phase of gravitational radiation-driven inspiral. We estimate a typical eccentricity at 1 week prior to coalescence of e approximate to 0.01. Higher terminal eccentricities, which can approach e 0: 1, are possible if the binary has an extreme mass ratio. The detection of even a small eccentricity prior to merger by LISA provides a possible discriminant between gas-driven inspirals and those effected by stellar processes.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available