Low-frequency scattering calculations show scalar probes through the MMP wormhole are mostly reflected or trapped at early times with late leakage to half the black-hole cross-section, while charged massless fermions transmit with unit probability via a Callan-Rubakov-like channel.
Bilotta, A Traversable Wormhole from the Kerr Black Hole, arXiv e-prints 10.48550/arXiv.2304.07356 (2023), arXiv:2304.07356 [hep-th]
3 Pith papers cite this work. Polarity classification is still indexing.
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Fermionic double-trace deformation modifies the two-point function in Kerr/CFT to supply negative energy that opens a traversable wormhole, with traversability peaking at early times and increasing with near-extremal rotation.
Double trace deformations create traversable wormholes in AdS5 black branes via gravitational shear and sound channel perturbations that violate ANEC in the hydrodynamic limit.
citing papers explorer
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How traversable is a traversable wormhole?
Low-frequency scattering calculations show scalar probes through the MMP wormhole are mostly reflected or trapped at early times with late leakage to half the black-hole cross-section, while charged massless fermions transmit with unit probability via a Callan-Rubakov-like channel.
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Kerr/CFT Traversable Wormhole with Fermionic Double-Trace Deformation
Fermionic double-trace deformation modifies the two-point function in Kerr/CFT to supply negative energy that opens a traversable wormhole, with traversability peaking at early times and increasing with near-extremal rotation.
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Traversable wormhole with double trace deformations via gravitational shear and sound channels
Double trace deformations create traversable wormholes in AdS5 black branes via gravitational shear and sound channel perturbations that violate ANEC in the hydrodynamic limit.