Aims.We present a new numerical code, ECHO, based on a Eulerian conservative high-order scheme for time dependent three-dimensional general relativistic magnetohydrodynamics (GRMHD) and magnetodynamics (GRMD). ECHO is aimed at providing a shock-capturing conservative method able to work at an arbitrary level of formal accuracy (for smooth flows), where the other existing GRMHD and GRMD schemes yield an overall second order at most. Moreover, our goal is to present a general framework based on the 3+1 Eulerian formalism, allowing for different sets of equations and different algorithms and working in a generic space-time metric, so that ECHO may be easily coupled to any solver for Einstein's equations. Methods.Our finite-difference c...
We present a new numerical code that solves the general relativistic magneto-hydrodynamical (GRMHD) ...
Due to the prevalence of magnetic fields in astrophysical environments, magnetohydrodynamic (MHD) si...
Conservative numerical schemes for general relativistic magnetohydrodynam-ics (GRMHD) require a meth...
Aims.We present a new numerical code, ECHO, based on a Eulerian conservative high-order scheme for t...
The main features of a novel numerical code for astrophysical fluids and magneto-fluids named ECHO (...
We present a new numerical code, X-ECHO, for general relativistic magnetohydrodynamics (GR...
ABSTRACT We describe a conservative, shock-capturing scheme for evolving the equations of general re...
We have developed a new three-dimensional general relativistic magnetohydrodynamic (GRMHD) code, RAI...
The accurate modelling of astrophysical scenarios involving compact objects and magnetic fields, suc...
The accurate modelling of astrophysical scenarios involving compact objects and magnetic fields, suc...
We present the new general-relativistic magnetohydrodynamics (GRMHD) capabilities of the Einstein To...
We present a new numerical code that solves the general relativistic magneto-hydrodynamical (GRMHD) ...
A new code and methodology are introduced for solving the fully general relativistic magnetohydrodyn...
Multidimensional shock-capturing numerical schemes for special relativistic hydrodynamics (RHD) are ...
A third order shock-capturing numerical scheme for three-dimensional special relativistic magnetohy...
We present a new numerical code that solves the general relativistic magneto-hydrodynamical (GRMHD) ...
Due to the prevalence of magnetic fields in astrophysical environments, magnetohydrodynamic (MHD) si...
Conservative numerical schemes for general relativistic magnetohydrodynam-ics (GRMHD) require a meth...
Aims.We present a new numerical code, ECHO, based on a Eulerian conservative high-order scheme for t...
The main features of a novel numerical code for astrophysical fluids and magneto-fluids named ECHO (...
We present a new numerical code, X-ECHO, for general relativistic magnetohydrodynamics (GR...
ABSTRACT We describe a conservative, shock-capturing scheme for evolving the equations of general re...
We have developed a new three-dimensional general relativistic magnetohydrodynamic (GRMHD) code, RAI...
The accurate modelling of astrophysical scenarios involving compact objects and magnetic fields, suc...
The accurate modelling of astrophysical scenarios involving compact objects and magnetic fields, suc...
We present the new general-relativistic magnetohydrodynamics (GRMHD) capabilities of the Einstein To...
We present a new numerical code that solves the general relativistic magneto-hydrodynamical (GRMHD) ...
A new code and methodology are introduced for solving the fully general relativistic magnetohydrodyn...
Multidimensional shock-capturing numerical schemes for special relativistic hydrodynamics (RHD) are ...
A third order shock-capturing numerical scheme for three-dimensional special relativistic magnetohy...
We present a new numerical code that solves the general relativistic magneto-hydrodynamical (GRMHD) ...
Due to the prevalence of magnetic fields in astrophysical environments, magnetohydrodynamic (MHD) si...
Conservative numerical schemes for general relativistic magnetohydrodynam-ics (GRMHD) require a meth...