Binary black hole merger in galactic nuclei: post-Newtonian simulations
I Berentzen, M Preto, P Berczik, D Merritt… - The Astrophysical …, 2009 - iopscience.iop.org
I Berentzen, M Preto, P Berczik, D Merritt, R Spurzem
The Astrophysical Journal, 2009•iopscience.iop.orgThis paper studies the formation and evolution of binary supermassive black holes (SMBHs)
in rotating galactic nuclei, focusing on the role of stellar dynamics. We present the first N-
body simulations that follow the evolution of the SMBHs from kiloparsec separations all the
way to their final relativistic coalescence, and that can robustly be scaled to real galaxies.
The N-body code includes post-Newtonian $(\cal {P\! N\!}) $
in rotating galactic nuclei, focusing on the role of stellar dynamics. We present the first N-
body simulations that follow the evolution of the SMBHs from kiloparsec separations all the
way to their final relativistic coalescence, and that can robustly be scaled to real galaxies.
The N-body code includes post-Newtonian $(\cal {P\! N\!}) $
Abstract
This paper studies the formation and evolution of binary supermassive black holes (SMBHs) in rotating galactic nuclei, focusing on the role of stellar dynamics. We present the first N-body simulations that follow the evolution of the SMBHs from kiloparsec separations all the way to their final relativistic coalescence, and that can robustly be scaled to real galaxies. The N-body code includes post-Newtonian
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