EMRIs resonantly drive zero-damped modes of near-extremal Kerr black holes, with the pole recovered from real-frequency orbital data via complex-response tomography.
Celestial mechanics in Kerr space- time
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The work establishes conservation of several quantities in Kerr black hole scattering and presents evidence that a spinning probe satisfies asymptotic integrability to quartic spin order at all post-Minkowskian orders.
Tidal force calculations in Kerr spacetime show survival of plunge along polar axis is possible for supermassive rotating black holes but not stellar-mass ones.
citing papers explorer
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Long-Lived Ringing of Near-Extremal Kerr Black Holes Resonantly Driven by Extreme-Mass-Ratio Inspirals
EMRIs resonantly drive zero-damped modes of near-extremal Kerr black holes, with the pole recovered from real-frequency orbital data via complex-response tomography.
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Unexpected Symmetries of Kerr Black Hole Scattering
The work establishes conservation of several quantities in Kerr black hole scattering and presents evidence that a spinning probe satisfies asymptotic integrability to quartic spin order at all post-Minkowskian orders.
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A Plunge into the Chasm: Surviving Tidal Effects in Kerr Spacetime
Tidal force calculations in Kerr spacetime show survival of plunge along polar axis is possible for supermassive rotating black holes but not stellar-mass ones.