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

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

This book is on inertial confinement fusion, an alternative way to produce electrical power
from hydrogen fuel by using powerful lasers or particle beams. It involves the compression of …

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 …

The turbulent Rayleigh–Taylor instability is investigated over a comprehensive range of fluid
density ratio (R) 1.3⩽ R⩽ 50 [0.15⩽ A=(R− 1)/(R+ 1)⩽ 0.96] and different acceleration …

Basic fluid equations are the main ingredient in the development of theories of Rayleigh–
Taylor buoyancy-induced instability. Turbulence arises in the late stage of the instability …

The late-time nonlinear evolution of the three-dimensional (3D) Rayleigh–Taylor (RT) and
Richtmyer–Meshkov (RM) instabilities for random initial perturbations is investigated. Using …

This paper describes an experimental investigation of mixing due to Rayleigh–Taylor
instability between two miscible fluids. Attention is focused on the gravitationally driven …

ABSTRACT A pulsar wind nebula (PWN) inside a supernova remnant provides a unique
insight into the properties of the central neutron star, the relativistic wind powered by its loss …

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 …