Modelling of stellar convection
F Kupka, HJ Muthsam - Living Reviews in Computational Astrophysics, 2017 - Springer
The review considers the modelling process for stellar convection rather than specific
astrophysical results. For achieving reasonable depth and length we deal with …
astrophysical results. For achieving reasonable depth and length we deal with …
MPI-AMRVAC 3.0: Updates to an open-source simulation framework
Context. Computational astrophysics nowadays routinely combines grid-adaptive
capabilities with modern shock-capturing, high resolution spatio-temporal integration …
capabilities with modern shock-capturing, high resolution spatio-temporal integration …
[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 …
Gamma-ray burst afterglows in the multimessenger era: numerical models and closure relations
G Ryan, H Van Eerten, L Piro… - The Astrophysical Journal, 2020 - iopscience.iop.org
Gamma-ray bursts (GRBs) associated with gravitational wave events are, and will likely
continue to be, viewed at a larger inclination than GRBs without gravitational wave …
continue to be, viewed at a larger inclination than GRBs without gravitational wave …
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 …
Driving outflows with relativistic jets and the dependence of active galactic nucleus feedback efficiency on interstellar medium inhomogeneity
AY Wagner, GV Bicknell… - The Astrophysical …, 2012 - iopscience.iop.org
We examine the detailed physics of the feedback mechanism by relativistic active galactic
nucleus (AGN) jets interacting with a two-phase fractal interstellar medium (ISM) in the kpc …
nucleus (AGN) jets interacting with a two-phase fractal interstellar medium (ISM) in the kpc …
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 …
Relativistic jet feedback in evolving galaxies
AY Wagner, GV Bicknell - The Astrophysical Journal, 2011 - iopscience.iop.org
Over cosmic time, galaxies grow through the hierarchical merging of smaller galaxies.
However, the bright region of the galaxy luminosity function is incompatible with the simplest …
However, the bright region of the galaxy luminosity function is incompatible with the simplest …