Polynomial models for the (2,2) post-merger waveform amplitudes of eccentric non-spinning binary black holes are constructed from numerical-relativity data as functions of symmetric mass ratio and two merger-time dynamical parameters.
Perturbations of the Vaidya metric in the frequency domain: Quasinormal modes and tidal response
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Generic Vaidya spacetimes with linear time-dependent mass, charge or rotation admit unique homothetic Killing vectors, allowing conformal mapping to stationary metrics and thermodynamic analysis of homothetic Killing horizons.
Renormalized dynamical tidal response functions for non-rotating black holes in GR carry inevitable ambiguities from renormalization scheme and flow initial condition, yielding scheme-dependent dynamical tidal Love numbers after MST-worldline EFT matching.
citing papers explorer
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Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms
Polynomial models for the (2,2) post-merger waveform amplitudes of eccentric non-spinning binary black holes are constructed from numerical-relativity data as functions of symmetric mass ratio and two merger-time dynamical parameters.
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Homothetic Killing horizons in generic Vaidya spacetimes
Generic Vaidya spacetimes with linear time-dependent mass, charge or rotation admit unique homothetic Killing vectors, allowing conformal mapping to stationary metrics and thermodynamic analysis of homothetic Killing horizons.
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Dynamical Tidal Response of Non-rotating Black Holes: Connecting the MST Formalism and Worldline EFT
Renormalized dynamical tidal response functions for non-rotating black holes in GR carry inevitable ambiguities from renormalization scheme and flow initial condition, yielding scheme-dependent dynamical tidal Love numbers after MST-worldline EFT matching.