Imprint of the black hole interior on thermal four-point correlators
Joydeep Chakravarty
TL;DR
The paper develops a boundary-based protocol to image the black hole interior by mapping high-frequency boundary correlators to local flat-space amplitudes near an interior bulk point. Central to the approach is a boundary integral transform that analytic-continues exterior operators into interior left-moving modes, yielding a factorization of the thermal four-point function into flat-space scattering data with an overall $\mathcal{O}(e^{-\beta\omega/2})$ suppression. The construction hinges on directed wavepackets smeared on boundary hyperboloids and a WKB/geodesic-based dictionary linking boundary operators to interior bulk oscillators, enabling a 3→1 or 2→2 interior amplitude description on an in-in contour. The work also analyzes boundary hyperboloids, AdS-Rindler geometry, and Planar BTZ examples to illustrate how interior physics can be diagnosed from boundary data, with implications for bulk locality, holographic cameras, and the flat-space limit in finite-temperature holography. Overall, the framework offers a concrete, though intricate, route to probe interior bulk dynamics via thermal correlators and two-sided boundary constructions, while noting limitations near the singularity and the need for further generalization to dynamical collapse and more general wormhole geometries.
Abstract
We consider correlators smeared against directed wavepackets over a thermal state dual to a single-sided planar AdS black hole. In the large frequency limit, our measurement is simplified using a bulk WKB description. We propose a dictionary that maps the action of smeared boundary operators to flat-space oscillators near an interior bulk point on the thermal state, by analytically continuing late-time operators from the right to the left boundary via an integral transform. Using the dictionary the smeared correlator factorizes to a flat-space like scattering amplitude about the interior event. Our transformed correlators describe local physics in the two-sided black hole interior, while incurring a suppression of $\mathcal{O}(e^{-βω/ 2})$. These measurements necessitate a non-trivial time ordering of operators living on boundary hyperboloids which are causally connected to the past light cone of the bulk point, as well as on a corresponding future branch.
