Geometric surprises in the Python's lunch conjecture
Abstract
A bulge surface, on a time reflection-symmetric Cauchy slice of a holographic spacetime, is a non-minimal extremal surface that occurs between two locally minimal surfaces homologous to a given boundary region. According to the python's lunch conjecture of Brown et al., the bulge's area controls the complexity of bulk reconstruction, in the sense of the amount of post-selection that needs to be overcome for the reconstruction of the entanglement wedge beyond the outermost extremal surface. We study the geometry of bulges in a variety of classical spacetimes, and discover a number of surprising features that distinguish them from more familiar extremal surfaces such as Ryu-Takayanagi surfaces: they spontaneously break spatial isometries, both continuous and discrete; they are sensitive to the choice of boundary infrared regulator; they can self-intersect; and they probe entanglement shadows, orbifold singularities, and compact spaces such as the sphere in AdSₚ × 𝑆^𝑞. These features imply, according to the python's lunch conjecture, novel qualitative differences between complexity and entanglement in the holographic context. We also find, surprisingly, that extended black brane interiors have a non-extensive complexity; similarly, for multi-boundary wormhole states, the complexity pleateaus after a certain number of boundaries have been included.
Copyright and License
© G. Arora et al. This work is licensed under the Creative Commons Attribution 4.0 International License. Published by the SciPost Foundation.
Acknowledgement
We thank Chris Akers, Raphael Bousso, Åsmund Folkestad, Brianna Grado-White, Guglielmo Grimaldi, Veronika Hubeny, Dominik Neuenfeld, Geoff Penington, Mukund Rangamani, Arvin Shahbazi-Moghaddam, and especially Netta Engelhardt and Brian Swingle for useful conversations.
Funding
We are grateful to the long term workshop YITP-T-23-01 held at YITP, Kyoto University, as well as to the Simons Foundation, the Institute for Advanced Study, and the Centro de Ciencias de Benasque Pedro Pascual, where part of this work was completed. This work was supported in part by the Department of Energy through awards DE-SC0009986 and QuantISED DE-SC0020360, and partly by the Simons Foundation through the It from Qubit Simons Collaboration.
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SciPostPhys_16_6_152.pdf
Additional details
Funding
- Kyoto University
- YITP-T-23-01
- Simons Foundation
- Institute for Advanced Study
- United States Department of Energy
- DE-SC0009986
- United States Department of Energy
- DE-SC0020360