[HTML][HTML] Grid-based methods in relativistic hydrodynamics and magnetohydrodynamics
JM Martí, E Müller - Living reviews in computational astrophysics, 2015 - Springer
An overview of grid-based numerical methods used in relativistic hydrodynamics (RHD) and
magnetohydrodynamics (RMHD) is presented. Special emphasis is put on a comprehensive …
magnetohydrodynamics (RMHD) is presented. Special emphasis is put on a comprehensive …
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 …
calculations are described. It is intended primarily for applications in astrophysical fluid …
PLUTO: a numerical code for computational astrophysics
A Mignone, G Bodo, S Massaglia… - The Astrophysical …, 2007 - iopscience.iop.org
We present a new numerical code, PLUTO, for the solution of hypersonic flows in 1, 2, and 3
spatial dimensions and different systems of coordinates. The code provides a multiphysics …
spatial dimensions and different systems of coordinates. The code provides a multiphysics …
The PLUTO code for adaptive mesh computations in astrophysical fluid dynamics
A Mignone, C Zanni, P Tzeferacos… - The Astrophysical …, 2011 - iopscience.iop.org
We present a description of the adaptive mesh refinement (AMR) implementation of the
PLUTO code for solving the equations of classical and special relativistic …
PLUTO code for solving the equations of classical and special relativistic …
Higher-order accurate space-time schemes for computational astrophysics—Part I: finite volume methods
DS Balsara - Living reviews in computational astrophysics, 2017 - Springer
As computational astrophysics comes under pressure to become a precision science, there
is an increasing need to move to high accuracy schemes for computational astrophysics …
is an increasing need to move to high accuracy schemes for computational astrophysics …
A new efficient formulation of the HLLEM Riemann solver for general conservative and non-conservative hyperbolic systems
M Dumbser, DS Balsara - Journal of Computational Physics, 2016 - Elsevier
In this paper a new, simple and universal formulation of the HLLEM Riemann solver (RS) is
proposed that works for general conservative and non-conservative systems of hyperbolic …
proposed that works for general conservative and non-conservative systems of hyperbolic …
Parallel, grid-adaptive approaches for relativistic hydro and magnetohydrodynamics
Relativistic hydro and magnetohydrodynamics provide continuum fluid descriptions for gas
and plasma dynamics throughout the visible universe. We present an overview of state-of …
and plasma dynamics throughout the visible universe. We present an overview of state-of …
ECHO: a Eulerian conservative high-order scheme for general relativistic magnetohydrodynamics and magnetodynamics
L Del Zanna, O Zanotti, N Bucciantini… - Astronomy & …, 2007 - aanda.org
Aims. We present a new numerical code, ECHO, based on a Eulerian conservative high-
order scheme for time dependent three-dimensional general relativistic …
order scheme for time dependent three-dimensional general relativistic …
Magnetorotational core collapse of possible GRB progenitors–I. Explosion mechanisms
M Obergaulinger, MÁ Aloy - Monthly Notices of the Royal …, 2020 - academic.oup.com
We investigate the explosion of stars with zero-age main-sequence masses between 20 and
35 M⊙ and varying degrees of rotation and magnetic fields including ones commonly …
35 M⊙ and varying degrees of rotation and magnetic fields including ones commonly …
GRHydro: a new open-source general-relativistic magnetohydrodynamics code for the Einstein toolkit
We present the new general-relativistic magnetohydrodynamics (GRMHD) capabilities of the
Einstein toolkit, an open-source community-driven numerical relativity and computational …
Einstein toolkit, an open-source community-driven numerical relativity and computational …