Simulations of gas-free disc galaxy mergers find primary SMBH mass grows 52-64 times initial seed while secondary grows 6-33 times, mostly from bulge and halo particles, sometimes ejecting the secondary SMBH.
and Wadsley, J., 2009 ApJ, 696, L89
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N-Body Simulations of Gas-free Disc Galaxies with SMBH Seed in Binary Systems
Simulations of gas-free disc galaxy mergers find primary SMBH mass grows 52-64 times initial seed while secondary grows 6-33 times, mostly from bulge and halo particles, sometimes ejecting the secondary SMBH.