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- W2015512074 abstract "We derive a model that describes the dynamics of a Brownian particle, such as a massive black hole, in a stellar system dominated by gravitational forces, and examine whether it achieves a state of equipartition of kinetic energy with the stars. This problem has been considered before only for stellar systems with an isothermal Maxwellian distribution of velocities; here we study other examples and confirm our calculations with N-body simulations. We show that in certain cases the black hole's steady state kinetic energy can be very far from equipartition." @default.
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- W2015512074 date "2002-03-07" @default.
- W2015512074 modified "2023-10-17" @default.
- W2015512074 title "Brownian Motion in Gravitationally Interacting Systems" @default.
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- W2015512074 doi "https://doi.org/10.1103/physrevlett.88.121103" @default.
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