Symmetrizations of RMHD equations and stability of relativistic current–vortex sheets
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We consider the equations of relativistic magnetohydrodynamics (RMHD) in the case of special relativity. Starting by computations in the fluid's rest frame and then applying Lorentz transformations, we derive a covariant symmetric formulation of RMHD in terms of the primitive (physical) variables. This symmetric system is important for the study of various initial boundary value problems. We also find a so-called secondary symmetrization whose direct consequence is the extension of the sufficient stability condition obtained earlier for non-relativistic planar current–vortex sheets to the relativistic case. As in non-relativistic settings, this implies the local-in-time existence of corresponding smooth nonplanar current–vortex sheets.
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FREISTÜHLER, Heinrich, Yuri TRAKHININ, 2013. Symmetrizations of RMHD equations and stability of relativistic current–vortex sheets. In: Classical and Quantum Gravity. 2013, 30(8), 085012. ISSN 0264-9381. eISSN 1361-6382. Available under: doi: 10.1088/0264-9381/30/8/085012BibTex
@article{Freistuhler2013Symme-26466, year={2013}, doi={10.1088/0264-9381/30/8/085012}, title={Symmetrizations of RMHD equations and stability of relativistic current–vortex sheets}, number={8}, volume={30}, issn={0264-9381}, journal={Classical and Quantum Gravity}, author={Freistühler, Heinrich and Trakhinin, Yuri}, note={Article Number: 085012} }
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