CAFE: A New Relativistic MHD Code
arXiv:1408.5846 · doi:10.1088/0067-0049/218/2/24
Abstract
We introduce CAFE, a new independent code designed to solve the equations of Relativistic ideal Magnetohydrodynamics (RMHD) in 3D. We present the standard tests for a RMHD code and for the Relativistic Hydrodynamics (RHD) regime since we have not reported them before. The tests include the 1D Riemann problems related to blast waves, head-on collision of streams and states with transverse velocities, with and without magnetic field, which is aligned or transverse, constant or discontinuous across the initial discontinuity. Among the 2D and 3D tests, without magnetic field we include the 2D Riemann problem, a one dimensional shock tube along a diagonal, the high speed Emery wind tunnel, the Kelvin-Helmholtz instability, a set of jets and a 3D spherical blast wave, whereas in the presence of a magnetic field we show the magnetic rotor, the cylindrical explosion, a case of Kelvin-Helmholtz instability and a 3D magnetic field advection loop. The code uses High Resolution Shock Capturing methods and we present the error analysis for a combination that uses the HLLE flux formula combined with linear, PPM and fifth order WENO reconstructors. We use the flux-CT and the divergence cleaning methods to control the divergence free magnetic field constraint.
30 pages, 110 png figures, 4 tables. Accepted for publication in the Astrophysical Journal Supplement. More numerical details, tests and additional references
References in corpus (8)
- Three-Dimensional General Relativistic Radiation Magnetohydrodynamical Simulation of Super-Eddington Accretion, using a new code HARMRAD with M1 Closure
- ECHO: an Eulerian Conservative High Order scheme for general relativistic magnetohydrodynamics and magnetodynamics
- THC: a new high-order finite-difference high-resolution shock-capturing code for special-relativistic hydrodynamics
- WhiskyMHD: a new numerical code for general relativistic magnetohydrodynamics
- High-Order Fully General-Relativistic Hydrodynamics: new Approaches and Tests
- An HLLC Solver for Relativistic Flows -- II. Magnetohydrodynamics
- Relativistic Hydrodynamic Flows Using Spatial and Temporal Adaptive Structured Mesh Refinement
- Local Kelvin-Helmholtz instability and synchrotron modulation in Pulsar Wind Nebulae
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