3-D GRMHD and GRPIC Simulations of Disk-Jet Coupling and Emission

Details 3-D GRMHD and GRPIC Simulations of Disk-Jet Coupling and Emission 3-D GRMHD and GRPIC Simulations of Disk-Jet Coupling and Emission

2006-12-12

arxiv.org/abs/astro-ph/0612328v1

Astronomy and Astrophysics

Astrophysics

3 pages, 1 figure, Proceedings of the Eleventh Marcel Grossmann Meeting on General Relativity, edited by H. Kleinert, R.T. Jan

Scientific paper

We investigate jet formation in black-hole systems using 3-D General Relativistic Particle-In-Cell (GRPIC) and 3-D GRMHD simulations. GRPIC simulations, which allow charge separations in a collisionless plasma, do not need to invoke the frozen condition as in GRMHD simulations. 3-D GRPIC simulations show that jets are launched from Kerr black holes as in 3-D GRMHD simulations, but jet formation in the two cases may not be identical. Comparative study of black hole systems with GRPIC and GRMHD simulations with the inclusion of radiate transfer will further clarify the mechanisms that drive the evolution of disk-jet systems.

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