Regular black holes in quasi-topological gravity lack null thin shells in standard distributional theory, invalidating the usual mass inflation derivation and leaving inner horizon stability unresolved.
Colombeau, Multiplication of Distributions: A Tool in Mathematics, Numerical Engineering and Theoretical Physics, Lecture Notes in Mathematics1532, 1 (1992)
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On mass inflation and thin shells in quasi-topological gravity
Regular black holes in quasi-topological gravity lack null thin shells in standard distributional theory, invalidating the usual mass inflation derivation and leaving inner horizon stability unresolved.