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General relativistic plasmas around rotating black holes

Published online by Cambridge University Press:  24 February 2011

Shinji Koide
Shinji Koide*
Affiliation:
Faculty of Science, Kumamoto University, 2-39-1 Kurokami, Kumamoto, 860-8555, Japan email: koidesin@sci.kumamoto-u.ac.jp
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Abstract

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We show one of possible directions of general relativistic MHD (GRMHD) calculations of astrophysical relativistic jet formation. This was motivated by observations of radio knot ejections associated with high energy flares of an AGN in M87 and micro-quasars. We introduce a modified version of a solar flare model for the phenomenon. In the model, we have to consider a process beyond the ideal GRMHD. Especially, we focus on the special features of general relativistic plasmas around rotating black holes.

Keywords

black hole physicsgravitationMHDrelativityplasmas

Information

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S275: Jets at all Scales , September 2010 , pp. 32 - 40
Copyright
Copyright © International Astronomical Union 2011

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