Abstract
The basic properties of relativistic magnetohydrodynamics, as a hyperbolic system of quasi-linear conservation laws, are discussed. These are then used to develop a multidimensional Godunov-type numerical scheme that enforces the magnetic flux conservation. This scheme is based on linear Riemann solvers and has second-order accuracy in smooth regions. The results of thorough test calculations demonstrate that the scheme is robust and can cope with truly ultrarelativistic problems.
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Komissarov, S. S. (1999). A Godunov-type scheme for relativistic magnetohydrodynamics. Monthly Notices of the Royal Astronomical Society, 303(2), 343–366. https://doi.org/10.1046/j.1365-8711.1999.02244.x
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