Computer Science
Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.2500b&link_type=abstract
"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an
Computer Science
Scientific paper
We consider a stellar mass black hole orbiting a primary super-massive Kerr black hole while always staying inside the accretion disk of the primary. We show that due to the accretion of matter from the disk, which is not necessarily Keplerian, the specific energy and angular momentum of the companion is modified. This affects the orbital evolution of the companion which was already lossing angular momentum and energy due to gravity wave emission. With an illustrative example, we show that the presence of the disk could significantly change the infall time of the companion towards the central black hole and modify the characteristic 'chirp' signal of the binary.
Basu Prasad
Chakrabarti Sandip K.
Goswami Kushalendu
Mondal Soumen
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