Binary neutron star mergers: a review of Einstein's richest laboratory
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 …
Numerical hydrodynamics and magnetohydrodynamics in general relativity
JA Font - Living Reviews in Relativity, 2008 - Springer
This article presents a comprehensive overview of numerical hydrodynamics and magneto-
hydrodynamics (MHD) in general relativity. Some significant additions have been …
hydrodynamics (MHD) in general relativity. Some significant additions have been …
[BOOK][B] Riemann solvers and numerical methods for fluid dynamics: a practical introduction
EF Toro - 2013 - books.google.com
In 1917, the British scientist LF Richardson made the first reported attempt to predict the
weather by solving partial differential equations numerically, by hand! It is generally …
weather by solving partial differential equations numerically, by hand! It is generally …
HARM: a numerical scheme for general relativistic magnetohydrodynamics
We describe a conservative, shock-capturing scheme for evolving the equations of general
relativistic magnetohydrodynamics. The fluxes are calculated using the Harten, Lax, & van …
relativistic magnetohydrodynamics. The fluxes are calculated using the Harten, Lax, & van …
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 …
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 …
Dust formation and survival in supernova ejecta
The presence of dust at high redshift requires efficient condensation of grains in supernova
(SN) ejecta, in accordance with current theoretical models. Yet observations of the few well …
(SN) ejecta, in accordance with current theoretical models. Yet observations of the few well …
Magnetic acceleration of relativistic active galactic nucleus jets
We present numerical simulations of axisymmetric, magnetically driven relativistic jets. Our
special-relativistic, ideal-magnetohydrodynamics numerical scheme is specifically designed …
special-relativistic, ideal-magnetohydrodynamics numerical scheme is specifically designed …
A new efficient formulation of the HLLEM Riemann solver for general conservative and non-conservative hyperbolic systems
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 …