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We extend the Ori-Thorne-Kesden procedure to consistently describe the non-quasi-circular transition around the ISCO from inspiral to plunge into a black hole of arbitrary spin, including near-extremal.
1901
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1901
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A. Ori and K. S. Thorne, “The Transition from inspiral to plunge for a compact body in a circular equatorial orbit around a massive, spinning black hole,” Phys. Rev
2000
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A. Buonanno and T. Damour, “Transition from inspiral to plunge in binary black hole coalescences,” Phys. Rev
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G. Compère and A. Druart, “Near-horizon Geodesics of High Spin Black Holes,” 2001.03478
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K. Glampedakis and D. Kennefick, “Zoom and whirl: Eccentric equatorial orbits around spinning black holes and their evolution under gravitational radiation reaction,” Phys. Rev
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S. A. Hughes and R. D. Blandford, “Black hole mass and spin coevolution by mergers,” Astrophys. J
2003
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M. C. Miller, “Probing general relativity with mergers of supermassive and intermediate-mass black holes,” Astrophys. J
2004
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A. Pound, E. Poisson, and B. G. Nickel, “Limitations of the adiabatic approximation to the gravitational self-force,” Phys. Rev
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2011
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2013
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2014
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A. Buonanno, Y. Chen, and T. Damour, “Transition from inspiral to plunge in precessing binaries of spinning black holes,” Phys. Rev
2006
Cited alongside, same era.
P. Amaro-Seoane, J. R. Gair, M. Freitag, M. Coleman Miller, I. Mandel, C. J. Cutler, and S. Babak, “Astrophysics, detection and science applications of intermediate- and extreme mass-ratio inspirals,” Class. Quant. Grav
2007
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2007
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2008
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2008
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M. Kesden, “Can binary mergers produce maximally spinning black holes?,” Phys. Rev
2008
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2009
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2014
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2014
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S. Hadar, A. P. Porfyriadis, and A. Strominger, “Fast plunges into Kerr black holes,” JHEP
2015
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2015
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S. E. Gralla, S. A. Hughes, and N. Warburton, “Inspiral into Gargantua,” Class. Quant. Grav
2016
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2017
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G. Compère, “The Kerr/CFT correspondence and its extensions,” Living Rev. Rel
2017
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2018
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