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We consider a rapidly spinning black hole surrounded by an equatorial, geometrically thin, slowly accreting disk that is stationary and axisymmetric.
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C. T. Cunningham and J. M. Bardeen, “The Optical Appearance of a Star Orbiting an Extreme Kerr Black Hole,” ApJ 183
1973
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2008
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2009
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M. Guica, T. Hartman, W. Song, and A. Strominger, “The Kerr/CFT correspondence,” Phys. Rev. D 80
2009
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2010
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2016
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G. Compère and R. Oliveri, “Near-horizon extreme Kerr magnetospheres,” Phys. Rev. D 93
2016
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S. E. Gralla, A. Lupsasca, and A. Strominger, “Near-horizon Kerr magnetosphere,” Phys. Rev. D 93
2016
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2016
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2012
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2012
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2013
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2014
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2014
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2014
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2014
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2015
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2016
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A. C. Fabian, “The innermost extremes of black hole accretion,” Astron. Nachr
2016
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2017
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2017
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2017
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2017
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2017
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2017
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2017
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S. E. Gralla and P. Zimmerman, “Critical Exponents of Extremal Kerr Perturbations,” ArXiv e-prints
2017
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2017
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