Collisionless relaxation of a Lynden-Bell plasma

  • R. J. Ewart
  • , A. Brown
  • , T. Adkins
  • , A. A. Schekochihin

Research output: Contribution to journalArticlepeer-review

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.

Original languageEnglish (US)
Article number925880501
JournalJournal of Plasma Physics
Volume88
Issue number5
DOIs
StatePublished - Oct 16 2022
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Condensed Matter Physics

Keywords

  • astrophysical plasmas
  • plasma dynamics
  • plasma nonlinear phenomena

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