Random Tensor Networks with Non-trivial Links

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Random tensor networks are a powerful toy model for understanding the entanglement structure of holographic quantum gravity. However, unlike holographic quantum gravity, their entanglement spectra are flat. It has therefore been argued that a better model consists of random tensor networks with link states that are not maximally entangled, i.e., have non-trivial spectra. In this work, we initiate a systematic study of the entanglement properties of these networks. We employ tools from free probability, random matrix theory, and one-shot quantum information theory to study random tensor networks with bounded and unbounded variation in link spectra, and in cases where a subsystem has one or multiple minimal cuts. If the link states have bounded spectral variation, the limiting entanglement spectrum of a subsystem with two minimal cuts can be expressed as a free product of the entanglement spectra of each cut, along with a Marchenko–Pastur distribution. For a class of states with unbounded spectral variation, analogous to semiclassical states in quantum gravity, we relate the limiting entanglement spectrum of a subsystem with two minimal cuts to the distribution of the minimal entanglement across the two cuts. In doing so, we draw connections to previous work on split transfer protocols, entanglement negativity in random tensor networks, and Euclidean path integrals in quantum gravity.

OriginalsprogEngelsk
TidsskriftAnnales Henri Poincare
Antal sider106
ISSN1424-0637
DOI
StatusE-pub ahead of print - 2024

Bibliografisk note

Funding Information:
NC is supported in part by the Department of Energy via the GeoFlow consortium (QuantISED Award DE-SC0019380). CL acknowledges support from the projects ESQuisses (ANR-20-CE47-0014-01), STARS (ANR-20-CE40-0008), Qtraj (ANR-20-CE40-0024-01), and Random Tensors (ANR-11-LABX-0040) of the French National Research Agency (ANR). GP is supported by the UC Berkeley Physics Department, the Simons Foundation through the “It from Qubit” program, the Department of Energy via the GeoFlow consortium (QuantISED Award DE-SC0019380), and AFOSR award FA9550-22-1-0098. He also acknowledges support from an IBM Einstein Fellowship at the Institute for Advanced Study. MW acknowledges support by the NWO through Grant OCENW.KLEIN.267, by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy - EXC 2092 CASA - 390781972, by the BMBF through project Quantum Methods and Benchmarks for Resource Allocation (QuBRA), and by European Research Council (ERC), funded by the European Union. Views and opinions expressed are, however, those of the authors only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them.

Publisher Copyright:
© 2023, The Author(s).

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