Late Time Correlation Functions, Baby Universes, and ETH in JT Gravity
Phil Saad

TL;DR
This paper demonstrates that correlation functions in JT gravity exhibit behavior consistent with an ensemble of Hamiltonians obeying ETH, with topology change via baby universes explaining non-decaying features.
Contribution
It provides a detailed bulk gravitational explanation for ETH and random matrix statistics in black hole microstates through baby universe topology changes.
Findings
Correlation functions show ramp and plateau behavior.
Baby universes induce topology change explaining non-decay.
Agreement with ensemble average predictions in JT gravity.
Abstract
Quantum black holes are described by a large number of macroscopically indistinguishable microstates. Correlation functions of fields outside the horizon at long time separation probe this indistinguishability. The simplest of these, the thermal two-point function, oscillates erratically around a nonperturbatively small average "ramp" and "plateau" after an initial period of decay; these non-decaying averaged features are signatures of the discreteness of the black hole spectrum. For a theory described by an ensemble of Hamiltonians, the two-point function follows this averaged behavior. In this paper we study certain correlation functions in Jackiw-Teitelboim (JT) gravity and find precise agreement with the behavior expected for a theory described by an ensemble of Hamiltonians with random matrix statistics -- the eigenstates obey the Eigenstate Thermalization Hypothesis (ETH) and the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
