Turbulent mixing induced by hydrodynamic instabilities is found in many high-and low-
energy-density regimes, ranging from supernovae to inertial confinement fusion to scramjet …

Turbulent hydrodynamic mixing induced by the Rayleigh–Taylor (RT) and Richtmyer–
Meshkov (RM) instabilities occurs in settings as varied as exploding stars (supernovae) …

The theoretical, numerical, and experimental study of compressible, variable-density, and
incompressible turbulent mixing associated with Richtmyer–Meshkov (RM), Rayleigh–Taylor …

Abstract Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM) instabilities are well-known
pathways towards turbulent mixing layers, in many cases characterized by significant mass …

This Introduction summarizes and provides a perspective on the papers representing one of
the key themes of the 'Turbulent mixing and beyond'programme—the hydrodynamic …

Hydrodynamic instabilities such as Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM)
instabilities usually appear in conjunction with the Kelvin–Helmholtz (KH) instability and are …

In diverse areas of science and technology, including inertial confinement fusion (ICF),
astrophysics, geophysics, and engineering processes, turbulent mixing induced by …

Turbulent mixing, induced by Rayleigh–Taylor (RT), Richtmyer–Meshkov (RM), and Kelvin–
Helmholtz (KH) instabilities, broadly occurs in both natural phenomena, such as supernova …

High-speed flows are prone to hydrodynamic interfacial instabilities that evolve to
turbulence, thereby intensely mixing different fluids and dissipating energy. The lack of …

The purpose of this note is to summarize recent progress of the authors in understanding
turbulent mixing. We consider both Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM) …