Binary Dynamics in Galactic Nuclei

Details Binary Dynamics in Galactic Nuclei Binary Dynamics in Galactic Nuclei

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...207.0605l&link_type=abstract

American Astronomical Society Meeting 207, #06.05; Bulletin of the American Astronomical Society, Vol. 37, p.1159

Astronomy and Astrophysics

Astronomy

Scientific paper

Extreme mass ratio inspirals, in which a stellar-mass compact object spirals into a supermassive black hole, can be produced by tidal separation of compact object binaries as well as the more commonly considered two-body capture by gravitational wave emission. Tidal separation will produce events with near-zero eccentricity in the observation band of the Laser Interferometer Space Antenna. Detailed analysis of the dynamics of compact-object binaries near the galactic center is a key step in understanding these zero-eccentricity events. We will present the results of N-body simulations, which aim to determine the survival rates and properties of compact-object binaries in the central few parsecs of galactic nuclei.

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