Black Hole Dynamics and Gravitational Radiation in Galactic Nuclei

Details Black Hole Dynamics and Gravitational Radiation in Galactic Nuclei Black Hole Dynamics and Gravitational Radiation in Galactic Nuclei

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21114005l&link_type=abstract

American Astronomical Society, AAS Meeting #211, #140.05; Bulletin of the American Astronomical Society, Vol. 39, p.989

Astronomy and Astrophysics

Astronomy

Scientific paper

Galactic nuclei are promising hosts of gravitational radiation sources such as extreme mass ratio inspirals (EMRIs), which are a primary target of the future space-based detector LISA. The tidal separation of stellar mass black hole binaries could produce unique EMRI signatures, providing valuable insight into the innermost regions of galaxies. We will present results of simulations of binaries near the galactic center, with a focus on tidal separations and induced mergers of the binary members. This work is supported by NASA GSRP.

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