arXiv · 1108.1816
Null infinity waveforms from extreme-mass-ratio inspirals in Kerr spacetime
Abstract
We describe the hyperboloidal compactification for Teukolsky equations in Kerr spacetime. We include null infinity on the numerical grid by attaching a hyperboloidal layer to a compact domain surrounding the rotating black hole and the orbit of an inspiralling point particle. This technique allows us to study, for the first time, gravitational waveforms from large- and extreme-mass-ratio inspirals in Kerr spacetime extracted at null infinity. Tests and comparisons of our results with previous calculations establish the accuracy and efficiency of the hyperboloidal layer method.
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Anıl Zenginoğlu, Gaurav Khanna. 2011-12-12. Null infinity waveforms from extreme-mass-ratio inspirals in Kerr spacetime. https://doi.org/10.1103/physrevx.1.021017
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