Universal constraints on energy flow and SYK thermalization

A bstract We study the dynamics of a quantum system in thermal equilibrium that is suddenly coupled to a bath at a different temperature, a situation inspired by a particular black hole evaporation protocol. We prove a universal positivity bound on the integrated rate of change of the system energy which holds perturbatively in the system-bath coupling. Applied to holographic systems, this bound implies a particular instance of the averaged null energy condition. We also study in detail the particular case of two coupled SYK models in the limit of many fermions using the Schwinger-Keldysh non-equilibrium formalism. We solve the resulting Kadanoff-Baym equations both numerically and analytically in various limits. In particular, by going to low temperature, this setup enables a detailed study of the evaporation of black holes in JT gravity.

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Publication Details

Journal
Journal of High Energy Physics
Published
2024-08-05
DOI
https://doi.org/10.1007/jhep08(2024)034
Citations
17
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
5.94
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article

Universal constraints on energy flow and SYK thermalization

Ahmed Almheiri, Alexey Milekhin, Brian Swingle
17 citations
Journal of High Energy Physics
Black Holes and Theoretical Physics
5.94
article

Universal constraints on energy flow and SYK thermalization

Ahmed Almheiri, Alexey Milekhin, Brian Swingle
article en
17 citations

Abstract

A bstract We study the dynamics of a quantum system in thermal equilibrium that is suddenly coupled to a bath at a different temperature, a situation inspired by a particular black hole evaporation protocol. We prove a universal positivity bound on the integrated rate of change of the system energy which holds perturbatively in the system-bath coupling. Applied to holographic systems, this bound implies a particular instance of the averaged null energy condition. We also study in detail the particular case of two coupled SYK models in the limit of many fermions using the Schwinger-Keldysh non-equilibrium formalism. We solve the resulting Kadanoff-Baym equations both numerically and analytically in various limits. In particular, by going to low temperature, this setup enables a detailed study of the evaporation of black holes in JT gravity.

Journal of High Energy PhysicsVol. 2024(8)
Princeton University (US), Institute for Advanced Study (US), Joint Center for Quantum Information and Computer Science (US), University of Maryland, College Park (US)
Affordable and clean energy
Openalex Percentile: Top 3%
Black Holes and Theoretical Physics
5.94
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Universal constraints on energy flow and SYK thermalization — Ahmed Almheiri, Alexey Milekhin, et al. · Journal of High Energy Physics (2024) | TGRS Research Map | TGRS