Monotonicity preserving weighted essentially non-oscillatory schemes with increasingly high order of accuracy

DS Balsara, CW Shu - Journal of Computational Physics, 2000 - Elsevier
In this paper we design a class of numerical schemes that are higher-order extensions of the
weighted essentially non-oscillatory (WENO) schemes of G.-S. Jiang and C.-W. Shu (1996) …

Simulations of cosmic ray propagation

M Hanasz, AW Strong, P Girichidis - Living Reviews in Computational …, 2021 - Springer
We review numerical methods for simulations of cosmic ray (CR) propagation on galactic
and larger scales. We present the development of algorithms designed for …

Partially ionized plasmas in astrophysics

JL Ballester, I Alexeev, M Collados, T Downes… - Space Science …, 2018 - Springer
Partially ionized plasmas are found across the Universe in many different astrophysical
environments. They constitute an essential ingredient of the solar atmosphere, molecular …

Smoothed particle hydrodynamics and magnetohydrodynamics

DJ Price - Journal of Computational Physics, 2012 - Elsevier
This paper presents an overview and introduction to smoothed particle hydrodynamics and
magnetohydrodynamics in theory and in practice. Firstly, we give a basic grounding in the …

The∇· B= 0 constraint in shock-capturing magnetohydrodynamics codes

G Tóth - Journal of Computational Physics, 2000 - Elsevier
Seven schemes to maintain the∇· B= 0 constraint numerically are compared. All these
algorithms can be combined with shock-capturing Godunov type base schemes. They fall …

Splitting methods

RI McLachlan, GRW Quispel - Acta Numerica, 2002 - cambridge.org
I thought that instead of the great number of precepts of which logic is composed, I would
have enough with the four following ones, provided that I made a firm and unalterable …

HARM: a numerical scheme for general relativistic magnetohydrodynamics

CF Gammie, JC McKinney, G Tóth - The Astrophysical Journal, 2003 - iopscience.iop.org
We describe a conservative, shock-capturing scheme for evolving the equations of general
relativistic magnetohydrodynamics. The fluxes are calculated using the Harten, Lax, & van …

The Athena++ adaptive mesh refinement framework: design and magnetohydrodynamic solvers

JM Stone, K Tomida, CJ White… - The Astrophysical …, 2020 - iopscience.iop.org
The design and implementation of a new framework for adaptive mesh refinement
calculations are described. It is intended primarily for applications in astrophysical fluid …

A staggered mesh algorithm using high order Godunov fluxes to ensure solenoidal magnetic fields in magnetohydrodynamic simulations

DS Balsara, DS Spicer - Journal of Computational Physics, 1999 - Elsevier
The equations of magnetohydrodynamics (MHD) have been formulated as a hyperbolic
system of conservation laws. In that form it becomes possible to use higher order Godunov …

A multi-state HLL approximate Riemann solver for ideal magnetohydrodynamics

T Miyoshi, K Kusano - Journal of Computational Physics, 2005 - Elsevier
A new multi-state Harten–Lax–van Leer (HLL) approximate Riemann solver for the ideal
magnetohydrodynamic (MHD) equations is developed based on the assumption that the …