A Langevin model with Holtsmark noise predicts that a 6x10^9 solar-mass black hole in an M87-like galaxy wanders about 6 parsecs from the galactic center over 10 Gyr due to stellar encounters.
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Brownian motion of supermassive black holes in galaxy cores
A Langevin model with Holtsmark noise predicts that a 6x10^9 solar-mass black hole in an M87-like galaxy wanders about 6 parsecs from the galactic center over 10 Gyr due to stellar encounters.