GRMHD_con2prim is a general-purpose framework that comes with various methods for the recovery of primitive variables from conservative variables in general-relativistic magnetohydrodynamics (GRMHD) with dynamical spacetimes. GRMHD_con2prim is available at the Zenodo repository with DOI 10.5281/zenodo.1213306. A separate updated development version is available at https://bitbucket.org/dsiegel/grmhd_con2prim. The associated detailed methods paper is: Siegel, D., Moesta, P., Desai, D., Wu, S. (2018), "Recovery schemes for primitive variables in general-relativistic magnetohydrodynamics", ApJS accepted, https://arxiv.org/abs/1712.07538. The DOI of the Zenodo repository (and the url of the development repository if appropriate) as well as ...
We present a new numerical code that solves the general relativistic magneto-hydrodynamical (GRMHD) ...
The accurate modelling of astrophysical scenarios involving compact objects and magnetic fields, suc...
We present a new numerical code, X-ECHO, for general relativistic magnetohydrodynamics (GR...
General relativistic magnetohydrodynamic (GRMHD) simulations represent a fundamental tool to probe v...
Conservative numerical schemes for general relativistic magnetohydrodynam-ics (GRMHD) require a meth...
Conservative numerical schemes for general relativistic magnetohydrodynamics (GRMHD) require a metho...
We present the new general-relativistic magnetohydrodynamics (GRMHD) capabilities of the Einstein To...
General relativistic magnetohydrodynamic (GRMHD) simulations represent a fundamental tool to probe v...
Recent developments in compact object astrophysics, especially the discovery of merging neutron star...
We present a new numerical code that solves the general relativistic magneto-hydrodynamical (GRMHD) ...
In the extreme violence of merger and mass accretion, compact objects like black holes and neutron s...
Recent developments in compact object astrophysics, especially the discovery of merging neutron star...
We have developed a new three-dimensional general relativistic magnetohydrodynamic (GRMHD) code by u...
We present a new numerical code that solves the general relativistic magneto-hydrodynamical (GRMHD) ...
The accurate modelling of astrophysical scenarios involving compact objects and magnetic fields, suc...
We present a new numerical code, X-ECHO, for general relativistic magnetohydrodynamics (GR...
General relativistic magnetohydrodynamic (GRMHD) simulations represent a fundamental tool to probe v...
Conservative numerical schemes for general relativistic magnetohydrodynam-ics (GRMHD) require a meth...
Conservative numerical schemes for general relativistic magnetohydrodynamics (GRMHD) require a metho...
We present the new general-relativistic magnetohydrodynamics (GRMHD) capabilities of the Einstein To...
General relativistic magnetohydrodynamic (GRMHD) simulations represent a fundamental tool to probe v...
Recent developments in compact object astrophysics, especially the discovery of merging neutron star...
We present a new numerical code that solves the general relativistic magneto-hydrodynamical (GRMHD) ...
In the extreme violence of merger and mass accretion, compact objects like black holes and neutron s...
Recent developments in compact object astrophysics, especially the discovery of merging neutron star...
We have developed a new three-dimensional general relativistic magnetohydrodynamic (GRMHD) code by u...
We present a new numerical code that solves the general relativistic magneto-hydrodynamical (GRMHD) ...
The accurate modelling of astrophysical scenarios involving compact objects and magnetic fields, suc...
We present a new numerical code, X-ECHO, for general relativistic magnetohydrodynamics (GR...