Kinetic theory quantitatively matches ensemble-averaged N-body simulations of a cold galactic disc, with strong collective effects, softening bias, and large realization-to-realization scatter near instability.
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On the long-term evolution of razor-thin galactic discs: Balescu-Lenard prediction and perspectives
Kinetic theory quantitatively matches ensemble-averaged N-body simulations of a cold galactic disc, with strong collective effects, softening bias, and large realization-to-realization scatter near instability.