# Revealing nonperturbative effects in the SYK model

**Authors:** Irina Aref'eva, Mikhail Khramtsov, Igor Volovich

arXiv: 1905.04203 · 2020-01-08

## TL;DR

This paper investigates the complex phase structure of coupled SYK chains with nonlocal interactions, revealing nonperturbative effects and saddle points that influence large N dynamics, with comparisons to local interaction models.

## Contribution

It introduces a novel analysis of nonperturbative saddle points in coupled SYK models with nonlocal interactions, highlighting their role in large N physics and phase structure.

## Key findings

- Multiple phases identified in nonlocal SYK models.
- Non-zero replica-nondiagonal correlators in saddle points.
- Differences in phase structure between local and nonlocal interactions.

## Abstract

We study the large $N$ saddle points of two SYK chains coupled by an interaction that is nonlocal in Euclidean time. We start from analytic treatment of the free case with $q=2$ and perform the numerical study of the interacting case $q=4$. We show that in both cases there is a nontrivial phase structure with infinite number of phases. Every phase correspond to a saddle point in the non-interacting two-replica SYK. The nontrivial saddle points have non-zero value of the replica-nondiagonal correlator in the sense of quasi-averaging, when the coupling between replicas is turned off. Thus, the nonlocal interaction between replicas provides a protocol for turning the nonperturbatively subleading effects in SYK into non-equilibrium configurations which dominate at large $N$. For comparison we also study two SYK chains with local interaction for $q=2$ and $q=4$. We show that the $q=2$ model also has a similar phase structure, whereas in the $q=4$ model, dual to the traversable wormhole, the phase structure is different.

## Full text

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## Figures

28 figures with captions in the complete paper: https://tomesphere.com/paper/1905.04203/full.md

## References

41 references — full list in the complete paper: https://tomesphere.com/paper/1905.04203/full.md

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Source: https://tomesphere.com/paper/1905.04203