3-D GRMHD Simulations of Generating Jets

Details 3-D GRMHD Simulations of Generating Jets 3-D GRMHD Simulations of Generating Jets

2002-08-05

arxiv.org/abs/astro-ph/0208092v1

Astronomy and Astrophysics

Astrophysics

4 pages, 1 fig (color), Proc. 4th Microquasar Workshop, 2002; Proceedings of the 4th Microquasar Workshop, 2002, eds. Duroucho

Scientific paper

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 the previous simulations using the axisymmetric geometry with the mirror symmetry at the equator. However, the time to generate the jet is longer than in the 2-D axisymmetric simulations. We expect that due to the additional freedom in the azimuthal dimension without axisymmetry with respect to the z axis and reflection symmetry with respect to the equatorial plane, the dynamics of jet formation can be modified. Further simulations are required for the study of instabilities along the azimuthal direction such as accretion-eject instability

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