Relaxation in self-gravitating systems

The long time-scale 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 meanfield 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 time-scales. 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. The stochastic gravitational fluctuations acting on the particles can generically be described by a correlated noise. Using this approach, we derive a diffusion equation for the actions in the test particle limit. We review how in the appropriate limits, this diffusion equation is equivalent to the inhomogeneous Balescu-Lenard and Landau equations. This approach reconciles the various resonant diffusion processes associated with long-term orbital distortions. Finally, by investigating the example of the Hamiltonian Mean-Field Model, we illustrate how the present method generically allows for alternative calculations of the long-term diffusion coefficients in inhomogeneous systems. © 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.