Explaining Nonlinearities in Black Hole Ringdowns from Symmetries
arXiv:2301.09345 · doi:10.1103/PhysRevD.108.L021501
Abstract
It has been recently pointed out that nonlinear effects are necessary to model the ringdown stage of the gravitational waveform produced by the merger of two black holes giving rise to a remnant Kerr black hole. We show that this nonlinear behaviour is explained, both on the qualitative and quantitative level, by near-horizon symmetries of the Kerr black hole within the Kerr/CFT correspondence.
arXiv comment5 pages
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- Spin dependence of black hole ringdown nonlinearities
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- Nonlinear ringdown at the black hole horizon
- Non-linear Black Hole Ringdowns: an Analytical Approach
- Nonlinear quasinormal mode detectability with next-generation gravitational wave detectors
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- Landscape of stellar-mass black-hole spectroscopy with third-generation gravitational-wave detectors
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- Black-hole spectroscopy: quasinormal modes, ringdown stability and the pseudospectrum
- Quadratic Mode Couplings in Rotating Black Holes and Their Detectability
- Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors