Proof of the zeroth law of turbulence in one-dimensional compressible magnetohydrodynamics and shock heating

The zeroth law is one of the oldest conjectures in turbulence that is still unproven. Here, we consider weak solutions of one-dimensional compressible magnetohydrodynamics and demonstrate that the lack of smoothness of the fields introduces a dissipative term, named inertial dissipation, into the expression of energy conservation that is neither viscous nor resistive in nature. We propose exact solutions assuming that the kinematic viscosity and the magnetic diffusivity are equal, and we demonstrate that the associated inertial dissipation is positive and equal on average to the mean viscous dissipation rate in the limit of small viscosity, proving the conjecture of the zeroth law of turbulence and the existence of an anomalous dissipation. As an illustration, we evaluate the shock heating produced by discontinuities detected by Voyager in the solar wind around 5 AU. We deduce a heating rate of similar to 10(-1)8 Jm(-3) s(-1), which is significantly higher than the value obtained from the turbulent fluctuations. This suggests that collisionless shocks can be a dominant source of heating in the outer solar wind.

Automated summary

This study examines weak solutions of one-dimensional compressible magnetohydrodynamics, demonstrating that lack of smoothness in fields introduces inertial dissipation named inertial dissipation and proposing exact solutions assuming equal kinematic viscosity and magnetic diffusivity. In the limit of small viscosity, inertial dissipation is shown to be positive and equal on average to mean viscous dissipation rate, validating the conjecture of the zeroth law of turbulence and the presence of anomalous dissipation. The findings suggest collisionless shocks could be a primary source of heating in the outer solar wind, with a heating rate significantly higher than that obtained from turbulent fluctuations.