Violation of the zeroth law of turbulence in space plasmas

TL;DR

This paper demonstrates that in strongly magnetized space plasma turbulence, the zeroth law of turbulence is violated due to a barrier at ion scales, leading to energy accumulation and spectral features matching observations.

Contribution

It reveals the violation of the zeroth law in space plasmas and introduces a barrier mechanism at ion scales caused by turbulence imbalance, supported by simulations and theoretical analysis.

Findings

Energy builds up at large scales in imbalanced turbulence.

Spectral features match in situ observations of space plasmas.

Barrier at ion scales influences plasma heating and spectral breaks.

Abstract

The zeroth law of turbulence states that, for fixed energy input into large-scale motions, the statistical steady state of a turbulent system is independent of microphysical dissipation properties. The behavior, which is fundamental to nearly all fluid-like systems from industrial processes to galaxies, occurs because nonlinear processes generate smaller and smaller scales in the flow, until the dissipation -- no matter how small -- can thermalize the energy input. Using direct numerical simulations and theoretical arguments, we show that in strongly magnetized plasma turbulence such as that recently observed by the Parker Solar Probe (PSP) spacecraft, the zeroth law is routinely violated. Namely, when such turbulence is "imbalanced" -- when the large-scale energy input is dominated by Alfv\'en waves propagating in one direction (the most common situation in space plasmas) -- nonlinear conservation laws imply the existence of a "barrier" at scales near the ion gyroradius. This causes energy to build up over time at large scales. The resulting magnetic-energy spectra bear a strong similarity to those observed in situ, exhibiting a sharp, steep kinetic transition range above and around the ion-Larmor scale, with flattening at yet smaller scales, thus resolving the decade-long puzzle of the position and variability of ion-kinetic spectral breaks in plasma turbulence. The "barrier" effect also suggests that how a plasma is forced at large scales (the imbalance) may have a crucial influence on thermodynamic properties such as the ion-to-electron heating ratio.