Abstract
We discuss the kinetic theories of stellar systems, two-dimensional vortices and Hamiltonian mean field model, stressing their analogies and differences. We describe the evolution of the system as a whole and discuss the timescale of relaxation towards the Boltzmann distribution predicted by statistical mechanics. We also consider the relaxation of a “test” particle in a bath of “field” particles and analyze it with the aid of a Fokker–Planck equation involving a term of diffusion counterbalanced by a friction or a drift.
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Chavanis, PH. Kinetic theory of stellar systems, two-dimensional vortices and HMF model. Theor. Comput. Fluid Dyn. 24, 217–239 (2010). https://doi.org/10.1007/s00162-009-0129-2
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DOI: https://doi.org/10.1007/s00162-009-0129-2