Relaxation to universal non-Maxwellian equilibria in a collisionless plasma

Generic equilibria are derived for turbulent relaxing plasmas via an entropy-maximization procedure that accounts for the short-time conservation of certain collisionless invariants. The conservation of these collisionless invariants endows the system with a partial "memory" of its prior conditions but is imperfect on long time scales due to the development of a turbulent cascade to small scales, which breaks the precise conservation of phase volume, making this memory imprecise. The equilibria are still determined by the short-time collisionless invariants, but the invariants themselves are driven to a universal form by the nature of the turbulence. This is numerically confirmed for the case of beam instabilities in one-dimensional electrostatic plasmas, where sufficiently strong turbulence appears to cause the distribution function of particle energies to develop a universal power-law tail, with exponent -2.

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Publication Details

Journal
Proceedings of the National Academy of Sciences
Published
2025-04-22
DOI
https://doi.org/10.1073/pnas.2417813122
Citations
6
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
6.93

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article

Relaxation to universal non-Maxwellian equilibria in a collisionless plasma

Pablo J. Bilbao, A. A. Schekochihin, Thales Silva, Luís O. Silva et al.
6 citations
Proceedings of the National Academy of Sciences
Solar and Space Plasma Dynamics
6.93
article

Relaxation to universal non-Maxwellian equilibria in a collisionless plasma

Pablo J. Bilbao, A. A. Schekochihin, Thales Silva, Luís O. Silva, Robert J. Ewart, Michael L. Nastac
article en
6 citations

Abstract

Generic equilibria are derived for turbulent relaxing plasmas via an entropy-maximization procedure that accounts for the short-time conservation of certain collisionless invariants. The conservation of these collisionless invariants endows the system with a partial "memory" of its prior conditions but is imperfect on long time scales due to the development of a turbulent cascade to small scales, which breaks the precise conservation of phase volume, making this memory imprecise. The equilibria are still determined by the short-time collisionless invariants, but the invariants themselves are driven to a universal form by the nature of the turbulence. This is numerically confirmed for the case of beam instabilities in one-dimensional electrostatic plasmas, where sufficiently strong turbulence appears to cause the distribution function of particle energies to develop a universal power-law tail, with exponent -2.

Proceedings of the National Academy of SciencesVol. 122(17)
University of Lisbon (PT), Kingston College (GB), University of Oxford (GB), Plasma (Russia) (RU), St. John's School (US), Instituto Superior Técnico (PT)
Engineering and Physical Sciences Research Council, Science and Technology Facilities Council
Life in Land
Openalex Percentile: Top 3%
Solar and Space Plasma Dynamics
6.93
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