Simulating the Dynamics of Binary Black Holes in Nuclear Gaseous Discs

Details Simulating the Dynamics of Binary Black Holes in Nuclear Gaseous Discs Simulating the Dynamics of Binary Black Holes in Nuclear Gaseous Discs

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..58d&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 58-58"

Physics

Scientific paper

Massive black hole binaries may form in galaxy collisions. The main focus of our study is their pairing inside a gaseous circum-nuclear disc. We study the black holes dynamics and accretion history from few hundred parsecs down to sub-parsec separations. This may allow address issues concerning fueling, mass growth and nuclear activity during the latest phases of the merger until their coalescence. The comprehension of these physical processes is essential to asses their detectability by the LISA experiment, and their electro-magnetic identification.

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