Relaxation in self-gravitating systems
Jean-Baptiste Fouvry, Ben Bar-Or

TL;DR
This paper develops a new formalism to describe the long-term stochastic evolution of particles in self-gravitating systems, linking mean field dynamics with resonant two-body encounters through a Gaussian noise approach.
Contribution
It introduces the $ ext{eta}$-formalism, deriving a diffusion equation for actions that unifies existing kinetic equations and enables new calculations of diffusion coefficients.
Findings
The $ ext{eta}$-formalism models gravitational fluctuations as Gaussian noise.
The diffusion equation is shown to be equivalent to Balescu-Lenard and Landau equations.
Application to the Hamiltonian Mean Field Model demonstrates the method's effectiveness.
Abstract
The long timescale evolution of a self-gravitating system is generically driven by two-body encounters. In many cases, the motion of the particles is primarily governed by the mean field potential. When this potential is integrable, particles move on nearly fixed orbits, which can be described in terms of angle-action variables. The mean field potential drives fast orbital motions (angles) whose associated orbits (actions) are adiabatically conserved on short dynamical timescales. The long-term stochastic evolution of the actions is driven by the potential fluctuations around the mean field and in particular by "resonant two-body encounters", for which the angular frequencies of two particles are in resonance. We show that the stochastic gravitational fluctuations acting on the particles can generically be described by a correlated Gaussian noise. Using this approach, the so-called…
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