Near-BPS AdS4 Kerr-Newman black holes are described by an SU(1,1|1) super-Schwarzian theory, yielding a predicted mass gap of order N^{-3/2} and a continuous spectrum above it in ABJM.
Teitelboim,Gravitation and Hamiltonian Structure in Two Space-Time Dimensions, Phys
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The spectrum of near-BPS Kerr-Newman black holes and the ABJM mass gap
Near-BPS AdS4 Kerr-Newman black holes are described by an SU(1,1|1) super-Schwarzian theory, yielding a predicted mass gap of order N^{-3/2} and a continuous spectrum above it in ABJM.