English

Universal non-thermal power-law distribution functions from the self-consistent evolution of collisionless electrostatic plasmas

Solar and Stellar Astrophysics 2024-11-13 v2 Astrophysics of Galaxies High Energy Astrophysical Phenomena Statistical Mechanics Plasma Physics Space Physics

Abstract

Distribution functions of collisionless systems are known to show non-thermal power law tails. Interestingly, collisionless plasmas in various physical scenarios, (e.g., the ion population of the solar wind) feature a v5v^{-5} tail in the velocity (vv) distribution, whose origin has been a long-standing mystery. We show this power law tail to be a natural outcome of the self-consistent collisionless relaxation of driven electrostatic plasmas. We perform a quasilinear analysis of the perturbed Vlasov-Poisson equations to show that the coarse-grained mean distribution function (DF), f0f_0, follows a quasilinear diffusion equation with a diffusion coefficient D(v)D(v) that depends on vv through the plasma dielectric constant. If the plasma is isotropically forced on scales much larger than the Debye length with a white noise-like electric field, then D(v)v4D(v)\sim v^4 for σ<v<ωP/k\sigma<v<\omega_{\mathrm{P}}/k, with σ\sigma the thermal velocity, ωP\omega_{\mathrm{P}} the plasma frequency and kk the maximum wavenumber of the perturbation; the corresponding f0f_0, in the quasi-steady state, develops a v(d+2)v^{-\left(d+2\right)} tail in dd dimensions (v5v^{-5} tail in 3D), while the energy (EE) distribution develops an E2E^{-2} tail irrespective of the dimensionality of space. Any redness of the noise only alters the scaling in the high vv end. Non-resonant particles moving slower than the phase-velocity of the plasma waves (ωP/k\omega_{\mathrm{P}}/k) experience a Debye-screened electric field, and significantly less (power law suppressed) acceleration than the near-resonant particles. Thus, a Maxwellian DF develops a power law tail. The Maxwellian core (v<σv<\sigma) eventually also heats up, but over a much longer timescale than that over which the tail forms. We definitively show that self-consistency (ignored in test-particle treatments) is crucial for the development of the universal v5v^{-5} tail.

Keywords

Cite

@article{arxiv.2408.07127,
  title  = {Universal non-thermal power-law distribution functions from the self-consistent evolution of collisionless electrostatic plasmas},
  author = {Uddipan Banik and Amitava Bhattacharjee and Wrick Sengupta},
  journal= {arXiv preprint arXiv:2408.07127},
  year   = {2024}
}

Comments

Accepted for publication in ApJ; 13 pages, 7 figures