General Relativistic Simulation of Magnetohydrodynamic Energy Extraction of a Rotating Black Hole

Details General Relativistic Simulation of Magnetohydrodynamic Energy Extraction of a Rotating Black Hole General Relativistic Simulation of Magnetohydrodynamic Energy Extraction of a Rotating Black Hole

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..289..319k&link_type=abstract

The Proceedings of the IAU 8th Asian-Pacific Regional Meeting, Volume I, held 2-5 July 2002 at National Center of Sciences, Hito

Astronomy and Astrophysics

Astrophysics

Scientific paper

We have developed the numerical method for general relativistic magnetohydrodynamic simulations in Kerr space-time. The method is applied to the basic astrophysical problem of the Kerr black hole activity in a large-scale strong magnetic field. The numerical result shows that the magnetic field extracts the rotational energy of the black hole with negative energy-at-infinity.

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