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 …

Spontaneous mixing of fluids at unstably stratified interfaces occurs in a wide variety of
atmospheric, oceanic, geophysical and astrophysical flows. The Rayleigh–Taylor instability …

A turbulence model is developed to described the self-similar growth of the Rayleigh-Taylor
(RT) and Richtmyer-Meshkov (RM) instabilities. The model describes the dominant eddies in …

Simultaneous advances in numerical methods and computing, theoretical techniques, and
experimental diagnostics have all led independently to better understanding of Rayleigh …

The self-similar nonlinear evolution of the multimode ablative Rayleigh-Taylor instability
(ARTI) is studied numerically in both two and three dimensions. It is shown that the nonlinear …

This study proposes a three-dimensional non-orthogonal multiple-relaxation-time (NMRT)
phase-field multiphase lattice Boltzmann (PFLB) model within a recently established unified …

The self-similar nonlinear evolution of the multimode ablative Rayleigh–Taylor instability
(RTI) and the ablation-generated vorticity effect are studied for a range of initial conditions …

A new hohlraum geometry or “Frustraum” is proposed that may enable 2–3× higher capsule
absorbed x-ray energy than for nominally sized capsules in standard cylinders. The …