A semiclassical ramp in SYK and in gravity

TL;DR

This paper proposes a semiclassical explanation for the ramp behavior in the spectral form factor of SYK models and black holes, linking nonperturbative saddle points to late-time correlations in finite entropy systems.

Contribution

It introduces a novel semiclassical saddle point approach to explain the ramp in SYK and black hole models, connecting collective field theory with black hole geometry.

Findings

Identifies a two-replica saddle point with zero action in SYK.

Links black hole solutions to a periodically identified two-sided black hole.

Provides a candidate explanation for late-time spectral correlations.

Abstract

In finite entropy systems, real-time partition functions do not decay to zero at late time. Instead, assuming random matrix universality, suitable averages exhibit a growing "ramp" and "plateau" structure. Deriving this non-decaying behavior in a large $N$ collective field description is a challenge related to one version of the black hole information problem. We describe a candidate semiclassical explanation of the ramp for the SYK model and for black holes. In SYK, this is a two-replica nonperturbative saddle point for the large $N$ collective fields, with zero action and a compact zero mode that leads to a linearly growing ramp. In the black hole context, the solution is a two-sided black hole that is periodically identified under a Killing time translation. We discuss but do not resolve some puzzles that arise.