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Universal role of curvature in vacuum entanglement

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arxiv 2311.15019 v2 pith:IUYE55WC submitted 2023-11-25 gr-qc hep-thquant-ph

classification gr-qchep-thquant-ph
keywords curvatureentanglementspacetimearbitraryboldsymbolcurvedexplorefeatures
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abstract

We highlight some universal features concerning the role of spacetime curvature in the entanglement induced between quantum probes coupled to a quantum field in a suitable vacuum state. The probes are initially causally disconnected and non-entangled. We explore the parameter space $\{{\omega}, d_0, \boldsymbol{v}_0\}$ spanned by the energy gap $\omega$ of the detectors, and the initial values of separation distance $d_0$ and relative velocity $\boldsymbol{v}_0$, both covariantly defined in arbitrary curved spacetime. We also obtain numerical results in de Sitter spacetimes and use these to explore strong curvature regime, while also corroborating our perturbative results in arbitrary curved spacetime. Our analysis shows that curvature can induce entanglement features in certain regions of the above parameter space, in a manner which facilitates using entanglement as a probe of spacetime curvature.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Can spacetime fluctuations generate entanglement between co-moving accelerated detectors?

    gr-qc 2025-04 conditional novelty 6.0 of 10

    Two uniformly accelerated Unruh-DeWitt detectors in nested Rindler frames harvest shift-independent entanglement from the Rindler vacuum whenever their trajectories are separated by any nonzero amount.

  2. Toward the Observation of Entangled Pairs in BEC analogue Expanding Universes

    gr-qc 2024-11 conditional novelty 6.0 of 10

    Repeated expansion-contraction cycles in a BEC analogue universe should make phonon-pair entanglement detectable at about 2 sigma now and above 3.3 sigma with modest upgrades.

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