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We analytically compute the observational appearance of an isotropically emitting point source on a circular, equatorial orbit near the horizon of a rapidly spinning black hole.
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1972
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C. T. Cunningham and J. M. Bardeen, “The Optical Appearance of a Star Orbiting an Extreme Kerr Black Hole,” ApJ 173
1972
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Gordon and Breach, New York, NY, 1973
J. M. Bardeen, “Timelike and null geodesics in the Kerr metric,” in Black Holes (Les Astres Occlus) · 1973
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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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J. Bardeen and G. T. Horowitz, “Extreme Kerr throat geometry: A vacuum analog of AdS_2 x S2̂,” Phys. Rev. D 60
1999
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N. Andersson and K. Glampedakis, “Superradiance Resonance Cavity Outside Rapidly Rotating Black Holes,” Physical Review Letters
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K. Glampedakis and N. Andersson, “Late-time dynamics of rapidly rotating black holes,” Phys. Rev. D 64
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S. E. Vázquez and E. P. Esteban, “Strong-field gravitational lensing by a Kerr black hole,” Nuovo Cimento B Serie
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A. E. Broderick and A. Loeb, “Imaging optically-thin hotspots near the black hole horizon of Sgr A* at radio and near-infrared wavelengths,” MNRAS 367
2006
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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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2012
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R. Narayan and J. E. McClintock, “Observational Evidence for Black Holes,” ArXiv e-prints
2013
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2016
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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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