Semiclassical OPE coefficients from 3D gravity
Chi-Ming Chang, Ying-Hsuan Lin
TL;DR
This work derives a universal semiclassical formula for OPE coefficients in 2D CFTs with a weak light spectrum by equating the crossing equation to the fusion transformation of the vacuum Virasoro block and evaluating the semiclassical fusion kernel. The authors express the universal OPE coefficients as the semiclassical limit of the fusion kernel, and they corroborate this with a gravity calculation: the regularized Einstein-Hilbert action for a geometry with three conical defects, analytically continued, reproduces the same universal result after Liouville normalization. A key insight is that when deficit angles violate the triangle inequality, the bulk geometry develops a horizon-like structure, hinting at a deeper link between universality in CFT data and bulk causal structure. The study thus unifies a conformal bootstrap derivation with a holographic bulk computation, using Liouville theory and 3D gravity to illuminate the interplay between crossing symmetry, OPE data, and gravitational saddles. Potential extensions include higher-dimension operators, BTZ regimes, and more intricate bulk topologies such as multi-boundary wormholes.
Abstract
We present a closed form expression for the semiclassical OPE coefficients that are universal for all 2D CFTs with a "weak" light spectrum, by taking the semiclassical limit of the fusion kernel. We match this with a properly regularized and normalized bulk action evaluated on a geometry with three conical defects, analytically continued in the deficit angles beyond the range for which a metric with positive signature exists. The analytically continued geometry has a codimension-one coordinate singularity surrounding the heaviest conical defect. This singularity becomes a horizon after Wick rotating to Lorentzian signature, suggesting a connection between universality and the existence of a horizon.
