Topology change in canonical JT gravity resolves the firewall paradox by making the connected two-interior branch dominate after Page time, with gravitational constraints annihilating the firewall branch and identifying horizon vacuum and early radiation purity as the same Dirac observable.
Failure of the split property in gravity and the information paradox
3 Pith papers cite this work. Polarity classification is still indexing.
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Typical states in large-N holographic CFTs exhibit UV and IR length scales set by energy and charges, producing factorization that isolates black holes via a corona of saturated entanglement wedges and extends ETH to rotating ensembles.
When topology sums generate nontrivial baby-universe sectors, the holography of information refines to an alpha-sectorwise statement, making the absence of firewalls conditional on global sector data rather than local geometry alone.
citing papers explorer
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Smooth horizons from topology change in canonical quantum gravity
Topology change in canonical JT gravity resolves the firewall paradox by making the connected two-interior branch dominate after Page time, with gravitational constraints annihilating the firewall branch and identifying horizon vacuum and early radiation purity as the same Dirac observable.
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Entanglement inequalities, black holes and the architecture of typical states
Typical states in large-N holographic CFTs exhibit UV and IR length scales set by energy and charges, producing factorization that isolates black holes via a corona of saturated entanglement wedges and extends ETH to rotating ensembles.
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Topology sums, sectorwise holography, and horizon normalcy
When topology sums generate nontrivial baby-universe sectors, the holography of information refines to an alpha-sectorwise statement, making the absence of firewalls conditional on global sector data rather than local geometry alone.