Geometric Phases Characterise Operator Algebras and Missing Information
Souvik Banerjee, Moritz Dorband, Johanna Erdmenger, Anna-Lena Weigel
TL;DR
The paper builds a concrete link between geometric (Berry) phases and the algebraic structure of von Neumann algebras, showing that a vanishing geometric phase enables a well-defined trace while nonzero phases signal missing information across observer patches. Starting from simple bipartite spin systems and using the Sz SZK (entanglement-orbit) construction, it ties the phase to entanglement properties and entanglement temperature, then generalises to infinite-spin systems where the phase controls the existence of traces and the algebra type (II vs III). In holographic AdS/CFT, time-translation phases reveal a common centre in the left-right algebras of an eternal black hole and encode how 1/N corrections move the system from type III to type II, enabling a trace in the latter. The work further interprets geometric phases as indicators of missing information for local observers, both with and without entanglement, and discusses multiple Berry-phase variants (Virasoro, gauge, modular) in wormhole spacetimes, culminating in prospects for Hawking-Page transitions and symmetry-resolved entanglement geometry.
Abstract
We show how geometric phases may be used to fully describe quantum systems, with or without gravity, by providing knowledge about the geometry and topology of its Hilbert space. We find a direct relation between geometric phases and von Neumann algebras. In particular, we show that a vanishing geometric phase implies the existence of a well-defined trace functional on the algebra. We discuss how this is realised within the AdS/CFT correspondence for the eternal black hole. On the other hand, a non-vanishing geometric phase indicates missing information for a local observer, associated to reference frames covering only parts of the quantum system considered. We illustrate this with several examples, ranging from a single spin in a magnetic field to Virasoro Berry phases and the geometric phase associated to the eternal black hole in AdS spacetime. For the latter, a non-vanishing geometric phase is tied to the presence of a centre in the associated von Neumann algebra.
