A Dynamical Model to Track the SMBBH's Path Towards Coalescence

Details A Dynamical Model to Track the SMBBH's Path Towards Coalescence A Dynamical Model to Track the SMBBH's Path Towards Coalescence

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21944202m&link_type=abstract

American Astronomical Society, AAS Meeting #219, #442.02

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Scientific paper

We follow the evolution of supermasive binary black holes (SMBBH) in the last stages of their evolution, a few pc. We have used a semianalytical model that includes a BHs binary system with triple disks, the mass added to the circumbinary disk due to cosmic accretion and the corresponding exchange of angular momentum
between accretion, mass transfer and orbital motion. While the circumbinary
disk removes angular momentum, the cosmological mass transfer adds some
fraction of its angular momentum to the orbital angular momentum of the SMBBH.

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