Collisionless relaxation of a Lynden-Bell plasma
Abstract
Plasmas whose Coulomb-collision rates are very small may relax on shorter timescales to non-Maxwellian quasi-equilibria, which, nevertheless, have a universal form, with dependence on initial conditions retained only via an infinite set of Casimir invariants enforcing phase-volume conservation. These are distributions derived by Lynden-Bell (Mon. Not. R. Astron. Soc., vol. 136, 1967, p. 101) via a statistical-mechanical entropy-maximisation procedure, assuming perfect mixing of phase-space elements. To show that these equilibria are reached dynamically, one must derive an effective `collisionless collision integral' for which they are fixed points - unique and inevitable provided the integral has an appropriate H-theorem. We describe how such collision integrals are derived and what assumptions are required for them to have a closed form, how to prove the H-theorems for them, and why, for a system carrying sufficiently large electric-fluctuation energy, collisionless relaxation should be fast. It is suggested that collisionless dynamics may favour maximising entropy locally in phase space before converging to global maximum-entropy states. Relaxation due to interspecies interaction is examined, leading, inter alia, to spontaneous transient generation of electron currents. The formalism also allows efficient recovery of `true' collision integrals for both classical and quantum plasmas.
- Publication:
-
Journal of Plasma Physics
- Pub Date:
- October 2022
- DOI:
- 10.1017/S0022377822000782
- arXiv:
- arXiv:2201.03376
- Bibcode:
- 2022JPlPh..88e9201E
- Keywords:
-
- astrophysical plasmas;
- plasma dynamics;
- plasma nonlinear phenomena;
- Physics - Plasma Physics;
- Astrophysics - High Energy Astrophysical Phenomena;
- Astrophysics - Solar and Stellar Astrophysics;
- Condensed Matter - Statistical Mechanics;
- Nonlinear Sciences - Chaotic Dynamics
- E-Print:
- 46 pages, 4 figures, submitted to JPP