On the interior geometry of a typical black hole microstate
Jan de Boer, Rik van Breukelen, Sagar F. Lokhande, Kyriakos Papadodimas, Erik Verlinde
TL;DR
The paper extends the Gao–Jafferis–Wall traversability framework to one-sided black holes dual to typical CFT states by employing state-dependent mirror operators and a double-trace perturbation. It shows that negative-energy shocks produced by V = O(0) tetilde{O}(0) can reveal behind-horizon physics via a CFT correlator, linking horizon smoothness to canonical-vs-typical state correlators at scrambling time. A central conjecture equates the one-sided and two-sided correlators in the large-N limit for low-frequency modes, supported by ETH-based arguments and SYK numerics, and it is extended to a Hayden–Preskill–like information-recovery protocol using mirror operators. Together, these results provide a concrete CFT realization of interior access for typical microstates and emphasize the role of state-dependent observables in black hole information transfer.
Abstract
We argue that the region behind the horizon of a one-sided black hole can be probed by an analogue of the double-trace deformation protocol of Gao-Jafferis-Wall. This is achieved via a deformation of the CFT Hamiltonian by a term of the form ${\cal O} \widetilde{\cal O}$, where $\widetilde{\cal O}$ denote the state-dependent "mirror operators". We argue that this deformation creates negative energy shockwaves in the bulk, which allow particles inside the horizon to escape and to get directly detected in the CFT. This provides evidence for the smoothness of the horizon of black holes dual to typical states. We argue that the mirror operators allow us to perform an analogue of the Hayden-Preskill decoding protocol. Our claims rely on a technical conjecture about the chaotic behavior of out-of-time-order correlators on typical pure states at scrambling time.
