Thermalization of mutual and tripartite information in strongly coupled two dimensional conformal field theories
V. Balasubramanian, A. Bernamonti, N. Copland, B. Craps, F. Galli
TL;DR
The paper investigates how mutual and tripartite information thermalize in strongly coupled two-dimensional conformal field theories using holography. Energy injection is modeled by a Vaidya-AdS3 background, and entanglement entropies are computed from geodesic lengths to obtain I(A,B) and I3(A,B,C) for various interval configurations. Mutual information generically rises from the vacuum value to a peak before decaying to the thermal value, with the peak timing depending on interval sizes and separations; a simple causality-based picture explains much of this behavior. Tripartite information remains nonzero and time-dependent during the process and is typically non-positive, contrasting with some quenched, large-time results in the literature and underscoring the importance of initial long-range correlations in dynamical holographic setups.
Abstract
The mutual and tripartite information between pairs and triples of disjoint regions in a quantum field theory are sensitive probes of the spread of correlations in an equilibrating system. We compute these quantities in strongly coupled two-dimensional conformal field theories with a gravity dual following the homogenous deposition of energy. The injected energy is modeled in anti-de Sitter space as an infalling shell, and the information shared by disjoint intervals is computed in terms of geodesic lengths in this background. For given widths and separation of the intervals, the mutual information typically starts at its vacuum value, then increases in time to reach a maximum, and then declines to the value at thermal equilibrium. A simple causality argument qualitatively explains this behavior. The tripartite information is generically non-zero and time-dependent throughout the process. This contrasts with (but does not contradict) the time-independent tripartite information one finds after a two-dimensional quantum quench in the limit of large time and distance scales compared to the initial inverse mass gap.
