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arXiv · gr-qc/0702035

Adaptive Mesh Refinement and Relativistic MHD

David Neilsen·Eric W. Hirschmann·Matthew Anderson·Steven L. Liebling
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Abstract

We solve the general relativistic magnetohydrodynamics equations using distributed parallel adaptive mesh refinement. We discuss strong scaling tests of the code, and present evolutions of Michel accretion and a TOV star.

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David Neilsen, Eric W. Hirschmann, Matthew Anderson, Steven L. Liebling. 2007-02-06. Adaptive Mesh Refinement and Relativistic MHD. https://doi.org/10.1142/9789812834300_0200

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