On the reconstruction of Lifshitz spacetimes
Simon A. Gentle, Cynthia Keeler
TL;DR
The paper investigates reconstructing Lifshitz spacetimes from boundary data using three holographic diagnostics: differential entropy (hole-ography), causal wedges, and entanglement wedges. The Lifshitz background introduces two key complications relative to AdS: (i) light rays with transverse momentum fail to reach the boundary, and (ii) the Lifshitz boundary is degenerate, complicating entanglement-based reconstructions; using the Lifshitz metric $ds^2 = L^2\left(-\frac{dt^2}{u^{2z}} + \frac{dx^2}{u^2} + \frac{du^2}{u^2}\right)$ with $z\ge1$, the authors examine how each reconstruction program fares. They find that (i) differential entropy can reconstruct only a subset of time-varying bulk curves, with certain curves non-reconstructible due to turning light rays; (ii) the causal wedge degenerates when the radial cut-off is removed, making a nondegenerate wedge dependent on a cut-off; and (iii) the entanglement wedge in Lifshitz generally does not close with extremal surfaces alone and requires including boundary-emitted light-sheets, signaling a departure from the AdS/HRT paradigm. These results indicate that naive RT/HRT prescriptions must be revised for Lifshitz holography and motivate exploring non-relativistic boundary structures (e.g., Newton–Cartan frameworks) or alternative bulk reconstruction schemes.
Abstract
We consider the reconstruction of a Lifshitz spacetime from three perspectives: differential entropy (or "hole-ography"), causal wedges and entanglement wedges. We find that not all time-varying bulk curves in vacuum Lifshitz can be reconstructed via the differential entropy approach, adding a caveat to the general analysis of \cite{Headrick:2014eia}. We show that the causal wedge for Lifshitz spacetimes degenerates, while the entanglement wedge requires the additional consideration of a set of boundary-emanating light-sheets. The need to include bulk surfaces with no clear field theory interpretation in the differential entropy construction and the change in the entanglement wedge formation both serve as warnings against a naive application of holographic entanglement entropy proposals in Lifshitz spacetimes.
