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.
& White, S.D.M., 2001, New Astronomy 6, 79
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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.