The Secular Dressed Diffusion Equation

The secular dressed diffusion equation describes the long-term evolution of collisionless systems of particles with long-range interactions, such as self-gravitating systems submitted to a weak external stochastic perturbation. We successively consider nonrotating spatially homogeneous systems, rota...

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Main Author: Pierre-Henri Chavanis
Format: Article
Language:English
Published: MDPI AG 2023-01-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/9/2/68
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author Pierre-Henri Chavanis
author_facet Pierre-Henri Chavanis
author_sort Pierre-Henri Chavanis
collection DOAJ
description The secular dressed diffusion equation describes the long-term evolution of collisionless systems of particles with long-range interactions, such as self-gravitating systems submitted to a weak external stochastic perturbation. We successively consider nonrotating spatially homogeneous systems, rotating spatially homogeneous systems, and spatially inhomogeneous systems. We contrast the secular dressed diffusion equation applying to collisionless systems perturbed by an externally imposed stochastic field from the Lenard–Balescu equation applying to isolated systems evolving because of discreteness effects (“collisions”). We discuss the connection between these two equations when the external noise is produced by a random distribution of field particles.
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spelling doaj.art-71c990856b344a0eae6fcadf64caaa972023-11-16T23:40:29ZengMDPI AGUniverse2218-19972023-01-01926810.3390/universe9020068The Secular Dressed Diffusion EquationPierre-Henri Chavanis0Laboratoire de Physique Théorique, Université de Toulouse, CNRS, UPS, 31062 Toulouse, FranceThe secular dressed diffusion equation describes the long-term evolution of collisionless systems of particles with long-range interactions, such as self-gravitating systems submitted to a weak external stochastic perturbation. We successively consider nonrotating spatially homogeneous systems, rotating spatially homogeneous systems, and spatially inhomogeneous systems. We contrast the secular dressed diffusion equation applying to collisionless systems perturbed by an externally imposed stochastic field from the Lenard–Balescu equation applying to isolated systems evolving because of discreteness effects (“collisions”). We discuss the connection between these two equations when the external noise is produced by a random distribution of field particles.https://www.mdpi.com/2218-1997/9/2/68self-gravitating systemskinetic theoryFokker–Planck equationangle-action variablescollective effects
spellingShingle Pierre-Henri Chavanis
The Secular Dressed Diffusion Equation
Universe
self-gravitating systems
kinetic theory
Fokker–Planck equation
angle-action variables
collective effects
title The Secular Dressed Diffusion Equation
title_full The Secular Dressed Diffusion Equation
title_fullStr The Secular Dressed Diffusion Equation
title_full_unstemmed The Secular Dressed Diffusion Equation
title_short The Secular Dressed Diffusion Equation
title_sort secular dressed diffusion equation
topic self-gravitating systems
kinetic theory
Fokker–Planck equation
angle-action variables
collective effects
url https://www.mdpi.com/2218-1997/9/2/68
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