Abstract

We study the OPE coefficients cΔ, J for heavy-light scalar four-point functions, which can be obtained holographically from the two-point function of a light scalar of some non-integer conformal dimension ΔL in an AdS black hole. We verify that the OPE coefficient cd,0 = 0 for pure gravity black holes, consistent with the tracelessness of the holographic energy-momentum tensor. We then study the OPE coefficients from black holes involving matter fields. We first consider general charged AdS black holes and we give some explicit low-lying examples of the OPE coefficients. We also obtain the recursion formula for the lowest-twist OPE coefficients with at most two current operators. For integer ΔL, although the OPE coefficients are not fully determined, we set up a framework to read off the coefficients γΔ,J of the log(z overline{z} ) terms that are associated with the anomalous dimensions of the exchange operators and obtain a general formula for γΔ,J. We then consider charged AdS black holes in gauged supergravity STU models in D = 5 and D = 7, and their higher-dimensional generalizations. The scalar fields in the STU models are conformally massless, dual to light operators with ΔL = d − 2. We derive the linear perturbation of such a scalar in the STU charged AdS black holes and obtain the explicit OPE coefficient cd−2,0. Finally, we analyse the asymptotic properties of scalar hairy AdS black holes and show how cd,0 can be nonzero with exchanging scalar operators in these backgrounds.

Highlights

  • The AdS/CFT correspondence establishes an insightful routine to investigate a strongly coupled conformal field theory (CFT) by using appropriate weakly coupled gravity in antide Sitter (AdS) spacetime and vice versa [1]

  • We study the OPE coefficients c∆,J for heavy-light scalar four-point functions, which can be obtained holographically from the two-point function of a light scalar of some non-integer conformal dimension ∆L in an AdS black hole

  • We studied the holographic OPE coefficients for heavy-light scalar four-point functions in the heavy limit where the heavy scalars approximately create a black hole background OH |0 |BH

Read more

Summary

Introduction

The AdS/CFT correspondence establishes an insightful routine to investigate a strongly coupled conformal field theory (CFT) by using appropriate weakly coupled gravity in antide Sitter (AdS) spacetime and vice versa [1]. This implies in particular that the OPE coefficient cd,0 must vanish when the CFT does not have an additional scalar operator of conformal dimension d It was verified [24] that c4,0 = 0 from pure gravity black holes. We verify the consistency that the OPE coefficient cd,0 associated with the trace of stress tensor does vanish for general d This fact motivates us to consider black holes with matters such that more primary operators can engage in, for instance, contributing to cd,0 = 0. In appendix B, the linearized equation for scalars in the variables considered in this paper is presented

OPE coefficients from holography
Four-point functions and conformal blocks
Lowest-twist OPE from pure gravities
The construction and explicit examples
Lowest-twist analysis
Recursion relation for general n
Anomalous conformal dimensions
An explicit demonstration
An alternative derivation
Gauged supergravity examples
Supergravity inspired models
AdS scalar hairy black holes and their asymptotic structures
Conclusions
A Conformal blocks
B Scalar equation
Full Text
Published version (Free)

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