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

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 C_{2}∝∫∫dxdv〈f^{2}〉-a quantity that here plays the role of (negative) entropy of the distribution function. We find that C_{2} 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 C_{2} 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 C_{2} 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 C_{2} is to both high k and high s simultaneously. Integrating over velocity (spatial) wave numbers, the k-space (s-space) flux of C_{2} 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.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1103/physreve.109.065210

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Oxford college:
St John's College
Role:
Author
ORCID:
0000-0003-2105-1475
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Oxford college:
Balliol College
Role:
Author
ORCID:
0000-0002-0206-7271
More by this author
Role:
Author
ORCID:
0000-0002-3415-2067
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Oxford college:
Merton College
Role:
Author
ORCID:
0000-0003-4421-1128
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Oxford college:
University College
Role:
Author
ORCID:
0000-0002-0177-1689


More from this funder
Funder identifier:
https://ror.org/01bj3aw27
Grant:
DEFG0293ER54197


Publisher:
American Physical Society
Journal:
Physical Review E More from this journal
Volume:
109
Issue:
6
Article number:
65210
Place of publication:
United States
Publication date:
2024-06-14
Acceptance date:
2024-02-02
DOI:
EISSN:
2470-0053
ISSN:
2470-0045
Pmid:
39021007


Language:
English
Keywords:
Pubs id:
2009327
Local pid:
pubs:2009327
Source identifiers:
W4399669952
Deposit date:
2025-04-19
ARK identifier:

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