Cosmological quantum entanglement
Eduardo Martin-Martinez, Nicolas C. Menicucci

TL;DR
This paper reviews how quantum entanglement arises in cosmological settings, especially in expanding universes, and discusses its implications for cosmic structure formation, potential observational signatures, and laboratory analogues.
Contribution
It synthesizes recent theoretical and experimental research on cosmological quantum entanglement, highlighting new insights into its role in universe expansion and structure formation.
Findings
Entanglement is produced by spacetime expansion in quantum fields.
Entanglement signatures can distinguish curvature effects from thermal heating.
Quantum fluctuations and entanglement influence the formation of cosmic structures.
Abstract
We review recent literature on the connection between quantum entanglement and cosmology, with an emphasis on the context of expanding universes. We discuss recent theoretical results reporting on the production of entanglement in quantum fields due to the expansion of the underlying spacetime. We explore how these results are affected by the statistics of the field (bosonic or fermionic), the type of expansion (de Sitter or asymptotically stationary), and the coupling to spacetime curvature (conformal or minimal). We then consider the extraction of entanglement from a quantum field by coupling to local detectors and how this procedure can be used to distinguish curvature from heating by their entanglement signature. We review the role played by quantum fluctuations in the early universe in nucleating the formation of galaxies and other cosmic structures through their conversion into…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
