3-D General Relativistic MHD Simulations of Generating Jets

Details 3-D General Relativistic MHD Simulations of Generating Jets 3-D General Relativistic MHD Simulations of Generating Jets

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...19913204n&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #132.04; Bulletin of the American Astronomical Society, Vol. 33, p.1498

Astronomy and Astrophysics

Astronomy

Scientific paper

We have investigated the dynamics of an accretion disk around Schwarzschild black holes initially threaded by a uniform poloidal magnetic field in a non-rotating corona (either in a steady-state infalling state) around a non-rotating black hole using a 3-D GRMHD with the ``axisymmetry'' along the z-direction. Magnetic field is tightly twisted by the rotation of the disk, and plasmas in the shocked region of the disk are accelerated by J x B force to form bipolar relativistic jets. In order to investigate variabilities of generated relativistic jets and magnetic field structure inside jets, we have performed calculations using the 3-D GRMHD code with a full 3-dimensional system without the axisymmetry. We have investigated how the third dimension affects the global disk dynamics and jet generation. We will perform simulations with various incoming flows from an accompanying star.

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