Binary neutron star mergers: a review of Einstein's richest laboratory
L Baiotti, L Rezzolla - Reports on Progress in Physics, 2017 - iopscience.iop.org
In a single process, the merger of binary neutron star systems combines extreme gravity, the
copious emission of gravitational waves, complex microphysics and electromagnetic …
copious emission of gravitational waves, complex microphysics and electromagnetic …
Neutron star merger remnants
S Bernuzzi - General Relativity and Gravitation, 2020 - Springer
Binary neutron star mergers observations are a unique way to constrain fundamental
physics and astrophysics at the extreme. The interpretation of gravitational-wave events and …
physics and astrophysics at the extreme. The interpretation of gravitational-wave events and …
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 …
Enzo: An adaptive mesh refinement code for astrophysics
This paper describes the open-source code Enzo, which uses block-structured adaptive
mesh refinement to provide high spatial and temporal resolution for modeling astrophysical …
mesh refinement to provide high spatial and temporal resolution for modeling astrophysical …
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 …
Hyperbolic divergence cleaning for the MHD equations
In simulations of magnetohydrodynamic (MHD) processes the violation of the divergence
constraint causes severe stability problems. In this paper we develop and test a new …
constraint causes severe stability problems. In this paper we develop and test a new …
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 …
algorithms can be combined with shock-capturing Godunov type base schemes. They fall …
Simulations of stellar convection with CO5BOLD
B Freytag, M Steffen, HG Ludwig… - Journal of …, 2012 - Elsevier
High-resolution images of the solar surface show a granulation pattern of hot rising and
cooler downward-sinking material–the top of the deep-reaching solar convection zone …
cooler downward-sinking material–the top of the deep-reaching solar convection zone …
A unified framework for the construction of one-step finite volume and discontinuous Galerkin schemes on unstructured meshes
In this article, a conservative least-squares polynomial reconstruction operator is applied to
the discontinuous Galerkin method. In a first instance, piecewise polynomials of degree N …
the discontinuous Galerkin method. In a first instance, piecewise polynomials of degree N …
Athena: a new code for astrophysical MHD
JM Stone, TA Gardiner, P Teuben… - The Astrophysical …, 2008 - iopscience.iop.org
A new code for astrophysical magnetohydrodynamics (MHD) is described. The code has
been designed to be easily extensible for use with static and adaptive mesh refinement. It …
been designed to be easily extensible for use with static and adaptive mesh refinement. It …