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

When discussing research in physics and in science more generally, it is common to ascribe
equal importance to the three components of the scientific trinity: theoretical, experimental …

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

▪ Abstract The ability of turbulent flows to effectively mix entrained fluids to a molecular scale
is a vital part of the dynamics of such flows, with wide-ranging consequences in nature and …

The turbulent Rayleigh–Taylor instability is investigated in the limit of strong mode-coupling
using a variety of high-resolution, multimode, three dimensional numerical simulations NS …

A large-eddy simulation technique is described for computing Rayleigh–Taylor instability.
The method is based on high-wavenumber-preserving subgrid-scale models, combined with …

Star formation is a complex multi-scale phenomenon that is of significant importance for
astrophysics in general. Stars and star formation are key pillars in observational astronomy …

This paper investigates the influence of different three-dimensional multi-mode initial
conditions on the rate of growth of a mixing layer initiated via a Richtmyer–Meshkov …

Turbulent Richtmyer–Meshkov instability (RMI) is investigated through a series of high
resolution three-dimensional simulations of two initial conditions with eight independent …

The self-similar evolution to turbulence of a multi-mode Rayleigh–Taylor mix at small density
differences (slope, similar to other canonical turbulent flows. A scaling argument is …