Entanglement Entropy at Large Central Charge
Thomas Hartman
TL;DR
The paper demonstrates that in 2d CFTs with large central charge and a sparse light spectrum, the leading large-$c$ contribution to the Renyi entropies of N disjoint intervals is universal and governed solely by the Virasoro vacuum block. By formulating and solving a monodromy problem for semiclassical conformal blocks, it shows that entanglement entropies factorize into sums of single-interval entropies in the appropriate channels, with a phase structure mirroring holographic minimal-surface prescriptions. The results reproduce the Ryu–Takayanagi formula for holographic entanglement entropy and its generalization to multiple intervals, providing a microscopic CFT understanding via vacuum exchanges and Liouville theory connections. The approach extends to k-point blocks and N-interval configurations, establishing a deep link between 3d gravity, Liouville theory, and Virasoro symmetry in the semiclassical regime. It also discusses the limitations and potential extensions, including phase transitions and non-vacuum contributions beyond leading order.
Abstract
Two-dimensional conformal field theories with a large central charge and a small number of low-dimension operators are studied using the conformal block expansion. A universal formula is derived for the Renyi entropies of N disjoint intervals in the ground state, valid to all orders in a series expansion. This is possible because the full perturbative answer in this regime comes from the exchange of the stress tensor and other descendants of the vacuum state. Therefore, the Renyi entropy is related to the Virasoro vacuum block at large central charge. The entanglement entropy, computed from the Renyi entropy by an analytic continuation, decouples into a sum of single-interval entanglements. This field theory result agrees with the Ryu-Takayanagi formula for the holographic entanglement entropy of a 2d CFT, applied to any number of intervals, and thus can be interpreted as a microscopic calculation of the area of minimal surfaces in 3d gravity.
