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We argue that the event horizon of a binary black hole merger, in the extreme-mass-ratio limit where one of the black holes is much smaller than the other, can be described in an exact analytic way.
K. Schwarzschild, “On the gravitational field of a mass point according to Einstein’s theory,” Sitzungsber. Preuss. Akad. Wiss. Berlin (Math. Phys.) (1916) S 189 [physics/9905030]
1916
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S. A. Caveny and R. A. Matzner, “Adaptive event horizon tracking and critical phenomena in binary black hole coalescence,” Phys. Rev. D 68
2003
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2008
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2009
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2011
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2011
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R. Emparan and M. Martínez, in preparation
Cited in the paper.
R. Emparan and M. Martínez, “Black String Flow,” JHEP 1309
2013
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M. Sun and Y. C. Huang, “Kerr Black string flow,” Nucl. Phys. B 897
2015
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2016
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