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 …

In order to accurately model implosion hydrodynamics in a radiation-hydrodynamics code, it
is essential to include accurate accounting for energy deposition physics. In inertial …

This paper investigates the influence of different broadband perturbations on the evolution of
a Richtmyer–Meshkov turbulent mixing layer initiated by a Mach 1.84 shock traversing a …

High-resolution large-eddy simulations of turbulent mixing at the inner surface of a dense
shell which undergoes forced compression by a spherically imploding shock wave are …

High-resolution three-dimensional implicit large eddy simulations of implosion in spherical
geometries are presented. The growth of perturbations is due to Rayleigh–Taylor (RT) and …

This paper considers a dense imploding spherical shell, where perturbations on the inner
surface grow due to hydrodynamic instabilities, geometric convergence and compression. A …

Compressible turbulent mixing evolving from Richtmyer-Meshkov and Rayleigh-Taylor
instabilities and Bell-Plesset effects has been investigated using high-resolution implicit …

In this paper, the Richtmyer–Meshkov instabilities in spherical and cylindrical converging
geometries with a Mach number of approximately 1.5 are investigated by using the high …

In this study, ensembles of experimental data are presented and utilized to compare and
validate two models used in the simulation of variable-density (Atwood= 0.22), compressible …