3-D General Relativistic MHD Simulations of Generating Jets
K. -I. Nishikawa, S. Koide, K. Shibata, T. Kudoh, H. Sol
Abstract
We have performed a first fully 3-D GRMHD simulation with Schwarzschild black hole with a free falling corona. The initial simulation results show that a jet is created as in previous axisymmetric simulations. However, the time to generate the jet is longer than in the 2-D simulations. We expect that due to the additional azimuthal dimension the dynamics of jet formation can be modified.
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