Adaptive Mesh Refinement and Relativistic MHD
arXiv:gr-qc/0702035 · doi:10.1142/9789812834300_0200
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.
3 Pages, Proceedings of the Marcel Grossmann Meeting XI