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Stress tensor correlators in three-dimensional gravity

Arjun Bagchi, Daniel Grumiller, Wout Merbis

TL;DR

This work tests flat space holography in three dimensions by computing arbitrary connected boundary stress-tensor correlators holographically in 3D Einstein gravity and matching them to 2D Galilean conformal field theory (GCFT$_2$) Ward identities. It develops and utilizes recursion relations derived from Ward identities, both in AdS$_3$/CFT$_2$ via the Chern–Simons formulation and in flat space, to determine all $n$-point correlators, obtaining explicit 2-, 3-, 4-, and 5-point results. The central charges are found to satisfy $c_L=0$ and $c_M=12k=3/G_N$, and the flat space results agree with GCFT predictions, confirming the consistency of flat space holography in 3D. The methodology provides a framework to extend these checks to other 3D gravity theories and holographic setups.

Abstract

We calculate holographically arbitrary n-point correlators of the boundary stress tensor in three-dimensional Einstein gravity with negative or vanishing cosmological constant. We provide explicit expressions up to 5-point (connected) correlators and show consistency with the Galilean conformal field theory Ward identities and recursion relations of correlators, which we derive. This provides a novel check of flat space holography in three dimensions.

Stress tensor correlators in three-dimensional gravity

TL;DR

This work tests flat space holography in three dimensions by computing arbitrary connected boundary stress-tensor correlators holographically in 3D Einstein gravity and matching them to 2D Galilean conformal field theory (GCFT) Ward identities. It develops and utilizes recursion relations derived from Ward identities, both in AdS/CFT via the Chern–Simons formulation and in flat space, to determine all -point correlators, obtaining explicit 2-, 3-, 4-, and 5-point results. The central charges are found to satisfy and , and the flat space results agree with GCFT predictions, confirming the consistency of flat space holography in 3D. The methodology provides a framework to extend these checks to other 3D gravity theories and holographic setups.

Abstract

We calculate holographically arbitrary n-point correlators of the boundary stress tensor in three-dimensional Einstein gravity with negative or vanishing cosmological constant. We provide explicit expressions up to 5-point (connected) correlators and show consistency with the Galilean conformal field theory Ward identities and recursion relations of correlators, which we derive. This provides a novel check of flat space holography in three dimensions.

Paper Structure

This paper contains 7 sections, 30 equations.