Generalized thermodynamics and Fokker-Planck equations. Applications to stellar dynamics, two-dimensional turbulence and Jupiter's great red spot
Pierre-Henri Chavanis

TL;DR
This paper introduces a new class of generalized Fokker-Planck equations that conserve key physical quantities and maximize a generalized entropy, with applications spanning astrophysics, fluid dynamics, and biological systems, offering a systematic framework for modeling complex relaxation processes.
Contribution
The paper develops a novel relaxation equation based on generalized thermodynamics, unifying various entropy forms, and applies it to diverse physical systems including stellar and vortex dynamics.
Findings
New relaxation equation depends on a key skewness parameter.
Standard parametrizations are special cases at infinite temperature.
The approach links vortices, stars, and bacteria through entropy classification.
Abstract
We introduce a new set of generalized Fokker-Planck equations that conserve energy and mass and increase a generalized entropy until a maximum entropy state is reached. The concept of generalized entropies is rigorously justified for continuous Hamiltonian systems undergoing violent relaxation. Tsallis entropies are just a special case of this generalized thermodynamics. Application of these results to stellar dynamics, vortex dynamics and Jupiter's great red spot are proposed. Our prime result is a novel relaxation equation that should offer an easily implementable parametrization of geophysical turbulence. This relaxation equation depends on a single key parameter related to the skewness of the fine-grained vorticity distribution. Usual parametrizations (including a single turbulent viscosity) correspond to the infinite temperature limit of our model. They forget a fundamental…
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