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 …

Inertial confinement fusion (ICF) has existed as a field of study since the 1970s, but the field
was born out of the Cold War. In the decades since the 1960s, pioneering research …

In diverse areas of science and technology, including inertial confinement fusion (ICF),
astrophysics, geophysics, and engineering processes, turbulent mixing induced by …

Star formation is such a complex process that accurate numerical tools are needed to
quantitatively examine the mass distribution and accretion of fragments in collapsing …

Massive stars produce so much light that the radiation pressure they exert on the gas and
dust around them is stronger than their gravitational attraction, a condition that has long …

This paper describes the design and implementation of our new multigroup,
multidimensional radiation hydrodynamics code F ornax and provides a suite of code tests …

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

We perform numerical simulations of a disc–planet system using various grid-based and
smoothed particle hydrodynamics (SPH) codes. The tests are run for a simple setup where …

We present a new code, CASTRO, that solves the multicomponent compressible
hydrodynamic equations for astrophysical flows including self-gravity, nuclear reactions, and …