Generalized thermodynamics and Fokker-Planck equations: Applications to stellar dynamics and two-dimensional turbulence

Pierre-Henri Chavanis
Phys. Rev. E 68, 036108 – Published 12 September 2003
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Abstract

We introduce a class of generalized Fokker-Planck equations that conserve energy and mass and increase a generalized entropy functional until a maximum entropy state is reached. Nonlinear Fokker-Planck equations associated with Tsallis entropies are a special case of these equations. Applications of these results to stellar dynamics and vortex dynamics are proposed. Our prime result is a relaxation equation that should offer an easily implementable parametrization of two-dimensional turbulence. Usual parametrizations (including a single turbulent viscosity) correspond to the infinite temperature limit of our model. They forget a fundamental systematic drift that acts against diffusion as in Brownian theory. Our generalized Fokker-Planck equations can have applications in other fields of physics such as chemotaxis for bacterial populations. We propose the idea of a classification of generalized entropies in “classes of equivalence” and provide an aesthetic connection between topics (vortices, stars, bacteria,) which were previously disconnected.

  • Received 12 November 2002

DOI:https://doi.org/10.1103/PhysRevE.68.036108

©2003 American Physical Society

Authors & Affiliations

Pierre-Henri Chavanis*

  • Laboratoire de Physique Théorique, Université Paul Sabatier, 118 route de Narbonne, 31062 Toulouse Cedex 4, France

  • *Email address: chavanis@irsamc.ups-tlse.fr

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Vol. 68, Iss. 3 — September 2003

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