Abstract

In the first part of the paper, we discuss different versions of the AdS/CFT dictionary out of equilibrium. We show that the Skenderis - van Rees prescription and the "extrapolate" dictionary are equivalent at the level of "in-in" two point functions of free scalar fields in arbitrary asymptotically AdS spacetimes. In the second part of the paper, we calculate two point correlation functions in dynamical spacetimes using the "extrapolate" dictionary. These calculations are performed for conformally coupled scalar fields in examples of spacetimes undergoing gravitational collapse, the AdS$_2$-Vaidya spacetime and the AdS$_3$-Vaidya spacetime, which allow us to address the problem of thermalization following a quench in the boundary field theory. The computation of the correlators is formulated as an initial value problem in the bulk spacetime. Finally, we compare our results for AdS$_3$-Vaidya to results in the previous literature obtained using the geodesic approximation and we find qualitative agreement.

Highlights

  • The AdS/CFT duality relates the dynamics of strongly coupled non-equilibirium quantum field theory to semiclassical gravitational dynamics [1, 2]

  • We show that the Skenderis-van Rees prescription and the “extrapolate” dictionary are equivalent at the level of “in-in” two point functions of free scalar fields in arbitrary asymptotically AdS spacetimes

  • In the second part of the paper, we calculate two point correlation functions in dynamical spacetimes using the “extrapolate” dictionary. These calculations are performed for conformally coupled scalar fields in examples of spacetimes undergoing gravitational collapse, the AdS2-Vaidya spacetime and the AdS3-Vaidya spacetime, which allow us to address the problem of thermalization following a quench in the boundary field theory

Read more

Summary

Introduction

The AdS/CFT duality relates the dynamics of strongly coupled non-equilibirium quantum field theory to semiclassical gravitational dynamics [1, 2]. In the first part of this paper, we will show that the “extrapolate” dictionary, when generalized to real time (in an obvious way), is equivalent to the SvR dictionary, for “in-in” two point correlators of a free scalar field in an arbitrary asymptotically AdS spacetime. We will demonstrate this by directly constructing a solution to the SvR equations of motion in the glued spacetime and show that this solution is related to a boundary limit of the bulk to bulk two point function.

On the holographic dictionary out of equilibrium
Two point functions as initial value problems
Equivalence of two out of equilibrium dictionaries
Proof of equivalence of the two dictionaries
Two point functions in AdS2-Vaidya
AdS2-Vaidya spacetime The AdS2 metric is given by ds2
Calculation of correlation functions
AdS3-Vaidya spacetime
Correlation functions in AdS3 and BTZ backgrounds
Calculation of the AdS3-Vaidya correlator
Thermalization of the Feynman correlator
Why does the Feynman correlator thermalize?
Comparison with geodesic approximation
Conclusions
A Identities between two point functions
B Initial state path integrals
C Calculational details on the AdS3-Vaidya correlator
Step 1
Step 2: evolve the Feynman propagator to the BTZ side
D Estimating the numerical error
E Summary of geodesic approximation results

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.