Tidal heating imprints from black hole horizons can be captured by two effective parameters and modeled through merger, offering a future test to distinguish black holes from exotic horizonless objects.
in The Physics of Accretion onto Black Holes (eds Falanga, M
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Characterizing the Properties and Constitution of Compact Objects in Gravitational-Wave Binaries
Tidal heating imprints from black hole horizons can be captured by two effective parameters and modeled through merger, offering a future test to distinguish black holes from exotic horizonless objects.