Both multiphase gas and magnetic fields are ubiquitous in astrophysics. However, the
influence of magnetic fields on mixing of the different phases is still largely unexplored. In …

Modelling the turbulent diffusion of thermal energy, momentum, and metals is required in all
galaxy evolution simulations due to the ubiquity of turbulence in galactic environments. The …

Turbulence in protoplanetary disks induces collisions between dust grains, and thus
facilitates grain growth. We investigate the two fundamental assumptions about the …

While magnetized turbulence is ubiquitous in many astrophysical and terrestrial systems,
our understanding of even the simplest physical description of this phenomena, ideal …

We revisit the problem of how energy transfer through the turbulent cascade operates in
compressible hydrodynamic turbulence. In general, there is no conservative compressible …

Turbulence simulations play a key role in advancing the general understanding of the
physical properties of turbulence and in interpreting astrophysical observations of turbulent …

Magnetized turbulence is ubiquitous in many astrophysical and terrestrial plasmas but no
universal theory exists. Even the detailed energy dynamics in magnetohydrodynamic (MHD) …

We present a generic mechanism for the thermal damping of compressive waves in the
interstellar medium (ISM), occurring due to radiative cooling. We solve for the dispersion …

Magnetohydrodynamic (MHD) turbulence affects both terrestrial and astrophysical plasmas.
The properties of magnetized turbulence must be better understood to more accurately …

Many terrestrial and astrophysical plasmas encompass very large dynamical ranges in
space and time, which are not accessible by direct numerical simulations. Thus, idealized …