Supersonic jets, particularly shock-containing jets, often exhibit high-intensity, discrete-
frequency acoustic tones. These tones are the signature of an aeroacoustic resonance loop …

We present the first 4π–three-dimensional (3D) simulation of the last minutes of oxygen shell
burning in an 18 M⊙ supernova progenitor up to the onset of core collapse. A moving inner …

The interaction between isotropic turbulence and a normal shock wave is investigated
through a series of direct numerical simulations at different Reynolds numbers and mean …

A theoretical framework to study linear and nonlinear Richtmyer–Meshkov instability (RMI) is
presented. This instability typically develops when an incident shock crosses a corrugated …

Fallback in core-collapse supernova explosions is potentially of significant importance for
the birth spins of neutron stars and black holes. It has recently been pointed out that the …

Shock–turbulence interactions are investigated using well-resolved direct numerical
simulations (DNS) and analysis at a range of Reynolds, mean and turbulent Mach numbers …

High-speed turbulent flows with shock waves are characterized by high localized surface
heat transfer rates. Computational predictions are often inaccurate due to the limitations in …

The structure of a shock wave interacting with isotropic turbulence is investigated. General
principles of similarity scaling show that consistency with known physical limiting behavior …

In this work, we use numerical simulation and linear inviscid theory to study the
thermodynamic field generated by the interaction of a shock wave with homogeneous …

The interaction between a weakly turbulent free stream and a hypersonic shock wave is
investigated theoretically by using linear interaction analysis (LIA). The formulation is …