Scale interactions and anisotropy in Rayleigh-Taylor turbulence
Dongxiao Zhao, Riccardo Betti, Hussein Aluie

TL;DR
This paper investigates energy transfer mechanisms in Rayleigh-Taylor turbulence, revealing differences between 2D and 3D flows, and clarifying the roles of baropycnal and deformation work in energy cascades.
Contribution
It introduces a coarse-graining method to analyze scale interactions in RT turbulence without Fourier transforms, highlighting distinct energy transfer processes in 2D and 3D.
Findings
In 3D, kinetic energy cascades to smaller scales via deformation work.
In 2D, energy re-channels to larger scales, enhancing mixing layer growth.
Large-scale flow isotropization occurs in 2D due to upscale energy transfer.
Abstract
We study energy scale-transfer in Rayleigh-Taylor (RT) flows by coarse-graining in physical space without Fourier transforms, allowing scale analysis along vertical direction. Two processes are responsible for kinetic energy flux across scales: baropycnal work , due to large-scale pressure gradients acting on small-scales of density and velocity, and deformation work , due to multi-scale velocity. Our coarse-graining analysis shows how these fluxes exhibit self-similar evolution that is quadratic-in-time, similar to RT mixing layer. We find that is a conduit for potential energy, transferring energy non-locally from the largest scales to smaller scales in the inertial range where takes over. In 3D, continues a persistent cascade to smaller scales, whereas in 2D re-channels the energy back to larger scales despite the lack of vorticity…
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Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Particle Dynamics in Fluid Flows · Computational Fluid Dynamics and Aerodynamics
