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

With the advent of high-energy-density (HED) experimental facilities, such as high-energy
lasers and fast Z-pinch, pulsed-power facilities, millimeter-scale quantities of matter can be …

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 …

This review is concerned with the results of studies into the behavior of substances at
ultimately high pressures and temperatures obtainable by way of kinetic or electromagnetic …

We report a scrupulous analysis of data in supernova experiments that are conducted at
high power laser facilities in order to study core-collapse supernova SN1987A. Parameters …

We present the first results from high-energy-density laboratory astrophysics experiments
that explore the interaction of supersonic jets/outflows with an ambient medium. Our …

Past decades significantly advanced our understanding of Rayleigh–Taylor (RT) mixing. We
briefly review recent theoretical results and numerical modelling approaches and compare …

We describe a platform developed on the LULI2000 laser facility to investigate the evolution
of Rayleigh-Taylor instability (RTI) in scaled conditions relevant to young supernova …

Rayleigh–Taylor instability (RTI) occurs whenever fluids of different densities are
accelerated against the density gradient, as is the case for the target ablator in ICF …

Experiments have identified the Rayleigh–Taylor (RT) instability as one of the greatest
obstacles to achieving inertial confinement fusion. Consequently, mitigation strategies to …