A NUMERICAL TREATMENT OF ANISOTROPIC RADIATION FIELDS COUPLED WITH RELATIVISTIC RESISTIVE MAGNETOFLUIDS

We develop a numerical scheme for solving fully special relativistic, resistive radiation magnetohydrodynamics. Our code guarantees conservation of total mass, momentum, and energy. The radiation energy density and the radiation flux are consistently updated using the M-1 closure method, which can r...

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Veröffentlicht in:	The Astrophysical journal 2013-08, Vol.772 (2), p.1-16
Hauptverfasser:	Takahashi, Hiroyuki R, OHSUGA, KEN
Format:	Artikel
Sprache:	eng
Schlagworte:	ADVECTION ANISOTROPY Approximation APPROXIMATIONS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS Computational fluid dynamics DIFFUSION ENERGY DENSITY Energy dissipation ENERGY LOSSES Fluid flow MAGNETIC RECONNECTION MAGNETIC REYNOLDS NUMBER MAGNETOHYDRODYNAMICS Mathematical analysis Mathematical models MATRICES NUMERICAL ANALYSIS OHM LAW RADIANT HEAT TRANSFER RADIATION FLUX RELATIVISTIC RANGE SOURCE TERMS
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