Numerical simulation of turbulent fluid dynamics needs to either parametrize turbulence—
which introduces large uncertainties—or explicitly resolve the smallest scales—which is …

The newly updated GIZMO and Simba based simulation, Simba-C, with its new stellar
feedback, chemical enrichment, and recalibrated AGN feedback, allows for a detailed study …

Supernovae (SNe) explosions are thought to be an important source of dust in galaxies. At
the same time strong shocks from SNe are known as an efficient mechanism of dust …

Coagulation in the dense interstellar medium (ISM) is an important process that determines
the size of the largest grains. We use submillimetre galaxies (SMGs) as laboratories of grain …

We study the linear growth and non-linear saturation of the 'acoustic Resonant Drag
Instability'(RDI) when the dust grains, which drive the instability, have a wide, continuous …

The radiative properties of interstellar dust are affected not only by the grain size distribution
but also by the grain porosity. We develop a model for the evolution of size-dependent grain …

The decrease rate of dust mass due to strong shock waves (vs≥ 150 km s− 1) from
supernovae (SNe) estimated for the Milky Way interstellar medium significantly exceeds the …

Particle transports in carriers with even-odd alternating dispersions (introduced in Part I) are
investigated. For the third-order dispersion as in Korteweg-de-Vries (KdV), such alternating …

Variations in the grain size distribution are to be expected in the interstellar medium (ISM)
owing to grain growth and destruction. In this work, we present a dust collision model to be …

The newly updated\texttt {GIZMO} and\texttt {Simba} based simulation,\texttt {Simba-C}, with
its new stellar feedback, chemical enrichment, and recalibrated AGN feedback, allows for a …