Black Holes and Random Matrices
Jordan S. Cotler, Guy Gur-Ari, Masanori Hanada, Joseph Polchinski,, Phil Saad, Stephen H. Shenker, Douglas Stanford, Alexandre Streicher, and, Masaki Tezuka

TL;DR
This paper explores how the late-time horizon fluctuations of large AdS black holes exhibit quantum chaotic behavior described by random matrix theory, using the SYK model as a key example.
Contribution
It demonstrates that black hole horizon fluctuations follow random matrix dynamics at late times and provides estimates for the crossover time from early to late time behavior.
Findings
Random matrix behavior observed at late times in SYK model
Exact early time behavior determined in a double scaling limit
Provisional estimates for crossover times in large AdS black holes
Abstract
We argue that the late time behavior of horizon fluctuations in large anti-de Sitter (AdS) black holes is governed by the random matrix dynamics characteristic of quantum chaotic systems. Our main tool is the Sachdev-Ye-Kitaev (SYK) model, which we use as a simple model of a black hole. We use an analytically continued partition function as well as correlation functions as diagnostics. Using numerical techniques we establish random matrix behavior at late times. We determine the early time behavior exactly in a double scaling limit, giving us a plausible estimate for the crossover time to random matrix behavior. We use these ideas to formulate a conjecture about general large AdS black holes, like those dual to 4D super-Yang-Mills theory, giving a provisional estimate of the crossover time. We make some preliminary comments about challenges to understanding the late…
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