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.
Gravitationally Collapsing Dust in $(2+1)$ Dimensions
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abstract
We investigate the circumstances under which gravitationally collapsing dust can form a black hole in three-dimensional spacetime.
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hep-th 1years
2025 1verdicts
UNVERDICTED 1representative citing papers
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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.