Superstatistical entropy deformations regularize the Schwarzschild black hole interior singularity into a finite core, reproducing some loop quantum gravity features without polymer discretization.
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Constraints on deviations from Kerr black hole metrics are derived from binary black hole inspiral waveforms modeled with effective one-body methods and analyzed via the parameterized post-Einsteinian framework.
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Entropy-Deformed Hamiltonian Dynamics of Schwarzschild Black Holes: A Superstatistical Approach
Superstatistical entropy deformations regularize the Schwarzschild black hole interior singularity into a finite core, reproducing some loop quantum gravity features without polymer discretization.
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Testing black hole metrics with binary black hole inspirals
Constraints on deviations from Kerr black hole metrics are derived from binary black hole inspiral waveforms modeled with effective one-body methods and analyzed via the parameterized post-Einsteinian framework.