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Kinetic theory of stellar systems, two-dimensional vortices and HMF model

机译:恒星系统的动力学理论,二维涡旋和HMF模型

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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.
机译:我们讨论了恒星系统的动力学理论,二维涡旋和哈密顿平均场模型,并强调了它们的类比和差异。我们描述了整个系统的演化,并讨论了由统计力学预测的朝玻尔兹曼分布弛豫的时间尺度。我们还考虑了“测试”粒子在“场”粒子池中的弛豫,并借助Fokker-Planck方程进行分析,该方程涉及由摩擦或漂移抵消的扩散项。

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