Superstatistical entropy deformations regularize the Schwarzschild black hole interior singularity into a finite core, reproducing some loop quantum gravity features without polymer discretization.
T 2Gγ 1− α± Gγ2 r C3 C1 !# .(44) The remaining phase-space variables are then given by b(T) =−γtan
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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.