Modern astrophysical simulations aim to accurately model an ever-growing array of physical
processes, including the interaction of fluids with magnetic fields, under increasingly …

Hydrodynamical numerical methods that converge with high-order hold particular promise
for astrophysical studies, as they can in principle reach prescribed accuracy goals with …

We investigate the numerical performance of a Discontinuous Galerkin (DG) hydrodynamics
implementation when applied to the problem of driven, isothermal supersonic turbulence …

We present a new numerical scheme which combines the spectral difference (SD) method
up to arbitrary high order with a-posteriori limiting using the classical MUSCL-Hancock …

Stellar convection poses two main gargantuan challenges for astrophysical fluid solvers: low-
Mach number flows and minuscule perturbations over steeply stratified hydrostatic …

We study in this paper three variants of the high-order Discontinuous Galerkin (DG) method
with Runge-Kutta (RK) time integration for the induction equation, analysing their ability to …

Owing to increases in computing power, high-order Eulerian schemes will likely become
instrumental in simulations of turbulence and magnetic field amplification in astrophysical …

El presente trabajo muestra la implementación de distintos métodos numéricos para la
descripción computacional de la dinámica de fluidos en entornos astrofísicos. Dichas …

Throughout the universe a primary way of transferring large scale kinetic energy down to
viscous scales where it can heat gas, mix chemical elemental abundances, regulate star …