Post-merger signals from asymmetric black hole binaries develop extra time-frequency peaks for strong aligned spin and a broken sky symmetry for mild precessing spin, consistent with the horizon-geometry correlation idea.
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Time-frequency structure in the post-merger binary black hole gravitational wave signal
Post-merger signals from asymmetric black hole binaries develop extra time-frequency peaks for strong aligned spin and a broken sky symmetry for mild precessing spin, consistent with the horizon-geometry correlation idea.