Resistive General Relativistic MHD Simulations of Jet Formation around Kerr Black Hole

Details Resistive General Relativistic MHD Simulations of Jet Formation around Kerr Black Hole Resistive General Relativistic MHD Simulations of Jet Formation around Kerr Black Hole

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1585k&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Physics

Scientific paper

Recent general relativistic magnetohydrodynamic (GRMHD) simulations of jet formation show inevitable formation of anti-parallel magnetic field in black hole magnetospheres. In such situation, magnetic reconnections should take place and influence the jet acceleration drastically. However, all of present GRMHD simulations assumed electric resistivity to be zero, where the magnetic reconnection is forbidden. To investigate the magnetic reconnection near the black hole, we develop the numerical method of the resistive GRMHD.

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