Berry phases, wormholes and factorization in AdS/CFT
Souvik Banerjee, Moritz Dorband, Johanna Erdmenger, René Meyer, Anna-Lena Weigel
TL;DR
Addressing the factorization puzzle in AdS/CFT, the paper shows that wormholes are encoded as Berry phases in 2D holographic CFTs. It develops a tripartite classification of Berry phases—Virasoro, gauge, and modular—each linked to a different bulk diffeomorphism and wormhole geometry. The Virasoro sector is realized as holonomies of coadjoint orbits; gauge Berry phases arise from asymptotic symmetries with a boundary time shift; modular Berry phases for subregions connect to the Crofton form on kinematic space and exhibit entanglement-entropy transitions in thermal states. Together these results illuminate how bulk non-factorization manifests as boundary geometric phases and suggest connections to subregion complexity.
Abstract
For two-dimensional holographic CFTs, we demonstrate the role of Berry phases for relating the non-factorization of the Hilbert space to the presence of wormholes. The wormholes are characterized by a non-exact symplectic form that gives rise to the Berry phase. For wormholes connecting two spacelike regions in gravitational spacetimes, we find that the non-exactness is linked to a variable appearing in the phase space of the boundary CFT. This variable corresponds to a loop integral in the bulk. Through this loop integral, non-factorization becomes apparent in the dual entangled CFTs. Furthermore, we classify Berry phases in holographic CFTs based on the type of dual bulk diffeomorphism involved. We distinguish between Virasoro, gauge and modular Berry phases, each corresponding to a spacetime wormhole geometry in the bulk. Using kinematic space, we extend a relation between the modular Hamiltonian and the Berry curvature to the finite temperature case. We find that the Berry curvature, given by the Crofton form, characterizes the topological transition of the entanglement entropy in presence of a black hole.
