Abstract

We consider the $AdS_{3}/CFT_{2}$ duality between certain coset WZW theories at large central charge and Vasiliev 3D higher spin gravity with a single complex field. On the gravity side, we discuss a higher spin black hole solution with chemical potential coupled to the spin-4 charge. We compute the perturbative expansion of the higher spin charges and of the partition function at high order in the chemical potential. The result is obtained with its exact dependence on the parameter $\lambda$ characterising the symmetry algebra $\mbox{hs}[\lambda]$. The cases of $\lambda=0,1$ are successfully compared with a CFT calculation. The special point $\lambda=\infty$, the Bergshoeff-Blencowe-Stelle limit, is also solved in terms of the exact generating function for the partition function. The thermodynamics of both the spin-4 and the usual spin-3 black holes is studied in order to discuss the $\lambda$ dependence of the BTZ critical temperature $T_{\rm BTZ}(\lambda)$. In the spin-3 case, it is shown that $T_{\rm BTZ}(\lambda)$ converges for large $\lambda$ to the critical point of the $\lambda=\infty$ known partition function previously found by the authors. In the spin-4 black hole, the picture is qualitatively similar and $T_{\rm BTZ}(\infty)$ is accurately determined by various numerical methods.

Highlights

  • Gravity theories with interacting higher spin gauge fields plays an important role in the study of AdS/CFT correspondence [1, 2]

  • We discuss a higher spin black hole solution with chemical potential coupled to the spin-4 charge

  • The O(α8) expansion of the partition function in powers of the spin-3 charge chemical potential α [7] has been confirmed by the computations in [10,11,12] at generic values of the parameter λ

Read more

Summary

Introduction

Gravity theories with interacting higher spin gauge fields plays an important role in the study of AdS/CFT correspondence [1, 2]. The physical meaning of the constants μs is that of chemical potentials acting as sources for the higher spin charges appearing in a+ (the subleading terms will be discussed later) This interpretation can be supported by a more constructive approach where one shows that, for non constant charges Ws = Ws(z, z) and μs = μs(z, z), the bulk equations of motion reduce to the Ward identities of the asymptotic chiral algebra in presence of deformations associated with the higher spin fields [6]. The standard way to fix the charges as functions of the chemical potentials is to impose smoothness of the horizon in the form of the following (infinite) set of equations [6, 9] These holonomy conditions must be consistent with thermodynamics. They will fix the structure of the various terms in the connection including the subleading terms

The spin-3 black hole
The spin-4 black hole
Perturbative expansion
The spin-3 case
The spin-4 case
Scalar propagator in the spin-4 background
Large λ resummation
Conclusions
J6 charge
J8 charge
J10 charge
J16 charge
E The Bulirsch-Stoer extrapolation algorithm
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