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

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 …

The 1990 National Academy of Science final report of its review of the Inertial Confinement
Fusion Program recommended completion of a series of target physics objectives on the 10 …

This book concerns itself with the physics of systems having high-energydensity. By high-
energy-density systems, we refer to those having a pressure above one million …

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 …

An analytical model of the nonlinear bubble evolution of single-mode, classical Rayleigh-
Taylor instability at arbitrary Atwood numbers (AT) is presented. The model is based on an …

Reaching ignition in direct-drive (DD) inertial confinement fusion implosions requires
achieving central pressures in excess of 100 Gbar. The OMEGA laser system [TR Boehly et …

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 …

The late-time development of Richtmyer–Meshkov instability is studied in shock tube
experiments. This investigation makes use of the experimental apparatus and visualization …