Gravitational waves from plunges into Gargantua
We analytically compute time domain gravitational waveforms produced in the final stages of extreme mass ratio inspirals of non-spinning compact objects into supermassive nearly extremal Kerr black holes. Conformal symmetry relates all corotating equatorial orbits in the geodesic approximation to ci...
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Published in | Classical and quantum gravity Vol. 35; no. 10; pp. 104002 - 104066 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
IOP Publishing
24.05.2018
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Subjects | |
Online Access | Get full text |
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