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De Sitter Space, Double-Scaled SYK, and the Separation of Scales in the Semiclassical Limit (2209.09999v1)

Published 20 Sep 2022 in hep-th and gr-qc

Abstract: In the semiclassical limit of de Sitter gravity a separation of scales takes place that divides the theory into a "cosmic" sector and a "microscopic" sector. A similar separation takes place in the double-scaled limit of SYK theory. We examine the scaling behaviors that accompany these limits and find parallels that support the previously conjectured duality between Jackiw-Teitelboim gravity (with positive cosmological constant), and double-scaled SYK. This paper is a companion to "dS JT Gravity and Double-Scaled SYK" by Adel Rahman, to appear simultaneously with this paper.

Citations (48)

Summary

  • The paper demonstrates a duality between semiclassical de Sitter gravity and double-scaled SYK, showing an infinite separation of cosmic and microscopic scales.
  • It utilizes a double-scaled SYK perturbative expansion akin to large N Yang-Mills techniques, drawing parallels with string theory in AdS/CFT contexts.
  • The study introduces 'tomperature' and emergent string scales to regulate infrared divergences and elucidate fast scrambling dynamics in quantum gravity.

Overview of "De Sitter Space, Double-Scaled SYK, and the Separation of Scales in the Semiclassical Limit"

This paper, authored by Leonard Susskind, explores the connections between de Sitter (dS) gravity in the semiclassical limit and the Sachdev-Ye-Kitaev (SYK) model, particularly in a double-scaled scenario. The paper focuses on the hypothesized duality between Jackiw-Teitelboim (JT) gravity and double-scaled SYK models, aiming to understand the separation of scales in these theories.

Key Concepts and Findings

  • Separation of Scales in de Sitter Space:

The work explores the semiclassical limit (SCL) of de Sitter space, characterized by infinite entropy and diverging horizon area. It emphasizes the division into cosmic and microscopic sectors, where micro scales remain insensitive to the cosmic scale, exemplified by a flat-space limit for local phenomena. On the other hand, phenomena sensitive to the cosmic scale are distinct and decoupled from microscopic details, leading to an infinite separation of scales in the limit.

  • Double-Scaled SYK Theory:

The paper explores the double-scaled SYK model, where the number of degrees of freedom, NN, approaches infinity, and the parameter qq, related to the interaction locality, scales appropriately. The SYK model's perturbative expansion in this limit is connected to large NN Yang-Mills theories, highlighting parallels in non-perturbative and 1/N expansion methods, shedding light on similarities with string theories in AdS/CFT contexts.

  • Emergent Dynamics and String Scale:

An emergent string scale is discussed in the context of SYK dynamics, appearing non-perturbatively through the solution of Schwinger-Dyson equations, regulating infrared divergences. The dynamical scale serves as a pivotal element in understanding the holographic framework of de Sitter dualities.

  • Tomperature and Cosmic Scale:

The concept of 'tomperature' is introduced as a measure of cosmic energy fluctuations, tying it to the Gibbons-Hawking temperature, thus bridging SYK parameters and cosmic gravity scales.

  • Scrambling and Correlation Functions:

Scrambling processes in these models reveal fast and hyperfast behaviors depending on the time units adopted, elucidating the dual nature of time evolution in cosmic and string scales. The SYK model's fermionic degrees of freedom display confinement near the horizon, suggesting mechanisms that mirror cosmic phenomena and provide insights into field propagation in holographic settings.

Implications and Speculations

This exploration of dualities between double-scaled SYK models and JT dS gravity contributes to understanding holographic principles beyond traditional AdS/CFT paradigms. The separation of scales and the interplay between cosmic, string, and microscopic phenomena carry implications for quantum gravity, entropy, and information scrambling, potentially offering paths toward resolving or further exploring key theoretical puzzles in cosmological and holographic theories.

Looking ahead, this paper poses challenges and opportunities in reconciling observational cosmic phenomena with theoretical models, inviting future research on the intricate relationships between micro and cosmic scales in diverse gravitational contexts. The parallels drawn to string theories also suggest directions for investigating non-locality and holographic duality with implications for both theoretical and observational physics.

Concluding, this work reinforces the significance of carefully decoupling and examining different scales in quantum gravity, highlighting the intricate web of connections that may one day converge in a unified holographic framework for understanding the universe.

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