Phase-space entropy cascade and irreversibility of stochastic heating in nearly collisionless plasma turbulence

Author:

Nastac Michael L.123ORCID,Ewart Robert J.14ORCID,Sengupta Wrick56ORCID,Schekochihin Alexander A.17ORCID,Barnes Michael18ORCID,Dorland William D.133ORCID

Affiliation:

1. University of Oxford

2. St. John's College

3. University of Maryland

4. Balliol College

5. Princeton University

6. Princeton Plasma Physics Laboratory

7. Merton College

8. University College

Abstract

We consider a nearly collisionless plasma consisting of a species of “test particles” in one spatial and one velocity dimension, stirred by an externally imposed stochastic electric field—a kinetic analog of the Kraichnan model of passive advection. The mean effect on the particle distribution function is turbulent diffusion in velocity space—known as stochastic heating. Accompanying this heating is the generation of fine-scale structure in the distribution function, which we characterize with the collisionless (Casimir) invariant C2dxdvf2—a quantity that here plays the role of (negative) entropy of the distribution function. We find that C2 is transferred from large scales to small scales in both position and velocity space via a phase-space cascade enabled by both particle streaming and nonlinear interactions between particles and the stochastic electric field. We compute the steady-state fluxes and spectrum of C2 in Fourier space, with k and s denoting spatial and velocity wave numbers, respectively. In our model, the nonlinearity in the evolution equation for the spectrum turns into a fractional Laplacian operator in k space, leading to anomalous diffusion. Whereas even the linear phase mixing alone would lead to a constant flux of C2 to high s (towards the collisional dissipation range) at every k, the nonlinearity accelerates this cascade by intertwining velocity and position space so that the flux of C2 is to both high k and high s simultaneously. Integrating over velocity (spatial) wave numbers, the k-space (s-space) flux of C2 is constant down to a dissipation length (velocity) scale that tends to zero as the collision frequency does, even though the rate of collisional dissipation remains finite. The resulting spectrum in the inertial range is a self-similar function in the (k,s) plane, with power-law asymptotics at large k and s. Our model is fully analytically solvable, but the asymptotic scalings of the spectrum can also be found via a simple phenomenological theory whose key assumption is that the cascade is governed by a “critical balance” in phase space between the linear and nonlinear timescales. We argue that stochastic heating is made irreversible by this entropy cascade and that, while collisional dissipation accessed via phase mixing occurs only at small spatial scales rather than at every scale as it would in a linear system, the cascade makes phase mixing even more effective overall in the nonlinear regime than in the linear one. Published by the American Physical Society 2024

Funder

Engineering and Physical Sciences Research Council

Simons Foundation

Science and Technology Facilities Council

U.S. Department of Energy

Publisher

American Physical Society (APS)

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