Equilibrium and nonequilibrium properties of Euler turbulence
Mahendra K. Verma, Soumyadeep Chatterjee

TL;DR
This paper investigates the equilibrium and nonequilibrium behaviors of 2D and 3D Euler turbulence through simulations, confirming theoretical predictions and revealing persistent order in certain conditions.
Contribution
It provides direct simulation-based verification of equilibrium turbulence theory and explores the nonequilibrium evolution of 2D Euler turbulence with ordered initial conditions.
Findings
Equilibrium spectra match Maxwell-Boltzmann distribution
2D Euler turbulence remains out of equilibrium with ordered initial conditions
Hydrodynamic entropy decreases over time in 2D turbulence
Abstract
In this article, we report the equilibrium and nonequilibrium features of two-dimensional (2D) and three-dimensional (3D) Euler turbulence. To obtain a full range of equilibrium spectra, we perform pseudo-spectral simulations of Euler turbulence using -correlated velocity field as an initial condition. These simulations provide zero energy flux and Maxwell-Boltzmann distribution for the velocity field, thus providing direct verification of the absolute equilibrium theory of turbulence. However, for ordered initial condition, 2D Euler turbulence remains out of equilibrium, with flow getting more ordered with time. We show that the hydrodynamic entropy of 2D Euler turbulence decreases with time, even though the system is isolated.
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Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Solar and Space Plasma Dynamics · Navier-Stokes equation solutions
