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Tidal heating in a binary black hole system is driven by the absorption of energy and angular momentum by the black hole's horizon.
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J. B. Hartle, Tidal Friction in Slowly Rotating Black Holes, Phys. Rev. D8
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E. E. Flanagan and S. A. Hughes, Measuring gravitational waves from binary black hole coalescences: 2. The Waves’ information and its extraction, with and without templates, Phys. Rev. D57
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I. Bena and D. R. Mayerson, Black Holes Lessons from Multipole Ratios, JHEP 03
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L. Barack, Gravitational self force in extreme mass-ratio inspirals, Class. Quant. Grav. 26
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S. A. Hughes, Evolution of circular, nonequatorial orbits of Kerr black holes due to gravitational wave emission. II. Inspiral trajectories and gravitational wave forms, Phys. Rev. D64
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2021
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2022
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2022
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K. G. Arun et al. (LISA), New horizons for fundamental physics with LISA, Living Rev. Rel. 25
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S. Datta, Probing horizon scale quantum effects with Love, Class. Quant. Grav. 39
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S. Datta, Horizon fluxes of binary black holes in eccentric orbits, (2023), arXiv:2305.03771 [gr-qc]
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