Abstract

We study 2-point and 3-point functions in CFT at finite temperature for large dimension operators using holography. The 2-point function leads to a universal formula for the holographic free energy in d dimensions in terms of the c-anomaly coefficient. By including α′ corrections to the black brane background, we reproduce the leading correction at strong coupling. In turn, 3-point functions have a very intricate structure, exhibiting a number of interesting properties. In simple cases, we find an analytic formula. When the dimensions satisfy ∆i = ∆j + ∆k, the thermal 3-point function satisfies a factorization property. We argue that in d > 2 factorization is a reflection of the semiclassical regime.

Highlights

  • This was studied in general in [1] for the case of the 2-point function, finding an elegant expansion in terms of Gegenbauer polynomials, whose coefficients incorporate both the OPE data as well as the non-zero vacuum expectation values in the thermal background

  • We study 2-point and 3-point functions in CFT at finite temperature for large dimension operators using holography

  • The 2-point function leads to a universal formula for the holographic free energy in d dimensions in terms of the c-anomaly coefficient

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Summary

Holographic 3-point functions: setting up the stage

We are interested on thermal correlation functions of scalar operators in holographic ddimensional CFT’s. We will mostly focus on the case where operators are inserted at the same spatial point, which, with no loss of generality can be taken to be 0, that is, we will consider xi = (ti, 0). The finite temperature state is dual to a black brane in AdSd+1. Each operator is dual to a fluctuating scalar field φi in the black brane in AdSd+1 with its mass related by the standard holographic formula to the dimension of the dual operator, d ∆= +. We shall consider operators of large scaling dimensions. For such operators, ∆ ≈ mR when mR 1. The bulk lagrangian is obtained by expanding the corresponding gravitational action in the fluctuations, where terms higher-than-quadratic in the fluctuations — suppressed by

N in terms of CFT variables
Thermal 2-point functions in d dimensions
Universal formula for the free energy
Thermal 3-point correlation functions with reflection symmetry
Factorization
Adding x dependence
Factorization property as a sign of a semiclassical limit
Discussion
Factorization property as a requirement for holography
Bootstrap conditions from factorization
A Details on the geodesic arcs
The saddle-point equations for xI and τI
B Conditions on OPE coefficients from factorization
Full Text
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