Abstract

Planar black holes in AdS have long-lived quasinormal modes which capture the physics of charge and momentum diffusion in the dual field theory. How should we characterize the effective dynamics of a probe system coupled to the conserved currents of the dual field theory? Specifically, how would such a probe record the long-lived memory of the black hole and its Hawking fluctuations? We address this question by exhibiting a universal gauge invariant framework which captures the physics of stochastic diffusion in holography: a designer scalar with a gravitational coupling governed by a single parameter, the Markovianity index. We argue that the physics of gauge and gravitational perturbations of a planar Schwarzschild-AdS black hole can be efficiently captured by such designer scalars. We demonstrate that this framework allows one to decouple, at the quadratic order, the long-lived quasinormal and Hawking modes from the short-lived ones. It furthermore provides a template for analyzing fluctuating open quantum field theories with memory. In particular, we use this set-up to analyze the diffusive Hawking photons and gravitons about a planar Schwarzschild-AdS black hole and derive the quadratic effective action that governs fluctuating hydrodynamics of the dual CFT. Along the way we also derive results relevant for probes of hyperscaling violating backgrounds at finite temperature.

Highlights

  • Black holes when disturbed settle down after classically ringing in quasinormal modes [1, 2]

  • How should we characterize the effective dynamics of a probe system coupled to the conserved currents of the dual field theory? how would such a probe record the long-lived memory of the black hole and its Hawking fluctuations? We address this question by exhibiting a universal gauge invariant framework which captures the physics of stochastic diffusion in holography: a designer scalar with a gravitational coupling governed by a single parameter, the Markovianity index

  • We argue that the physics of gauge and gravitational perturbations of a planar Schwarzschild-anti-de Sitter (AdS) black hole can be efficiently captured by such designer scalars

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Summary

Introduction: remembrance of a black hole’s past

Black holes when disturbed settle down after classically ringing in quasinormal modes [1, 2]. The quasinormal modes signify dissipation into a medium and the Hawking modes correspond to the attendant quantum statistical fluctuations. Quasinormal modes of AdS black holes correspond to thermalization rates of the dual field theory [4]. Massless spin-1 and spin-2 fields in planar AdS black holes have long-lived quasinormal modes with dispersions that are characteristic of hydrodynamic fluctuations [5,6,7]. Correspond to the charge and momentum diffusion, and (attenuated) sound waves in the dual field theory plasma One can trace their origins to the underlying gauge invariance of massless spin-1 and spin-2 fields manifested as global conservation laws for charge currents and energy-momentum tensor. Our goal in this work is to provide a unified treatment of the diffusive modes of AdS black holes and obtain an effective action governing their dynamics

Open quantum systems with memory
Synopsis of salient results
Outline of the paper
Review of the grSK geometry
Designing gravitational probes with memory
Designer scalar and gauge probes
Origins of the designer fields
Markovianity and lack thereof: memories lost and regained
Analytic versus monodromy modes and their interpretation
The well of memory: hydrodynamic moduli space
Analytic continuation into the hydrodynamic moduli space
Observables on hydrodynamic moduli space
Time-reversal invariant scalar system 1
Explicit parameterization of ingoing Green’s function
Counterterms and boundary correlators
Time reversal invariant scalar system 2: non-Markovian dynamics
Parameterization of the ingoing solution
The non-Markovian inverse Green’s function and dispersion relations
Two observations about non-Markovian scalars
Counterterms and boundary correlators: non-Markovian scalar
Solution and on-shell action on grSK geometry
Markovian probes
Non-Markovian probes
The Gaussian Wilsonian influence functional
Time-reversal invariant gauge system
Decomposition of gauge field modes
The non-Markovian charge diffusion scalar
Maxwell action and Wilsonian influence phase
Gravitational perturbations
10 Discussion
Full Text
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