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A Flat Space Analogue for the Quantum Origin of Structure

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arxiv 2203.10042 v1 pith:YSIJ5V7B submitted 2022-03-18 hep-th astro-ph.COhep-phquant-ph

A Flat Space Analogue for the Quantum Origin of Structure

classification hep-th astro-ph.COhep-phquant-ph
keywords correlatorsdetectorsin-inquantumstructurecosmologicalenergyentanglement
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The analytic structure of non-Gaussian correlators in inflationary cosmologies has recently been proposed as a test of the quantum origin of structure in the universe. To further understand this proposal, we explore the analogous equal-time in-in correlators in flat space and show they exhibit the same features as their cosmological counterparts. The quantum vacuum is uniquely identified by in-in correlators with a total energy pole and no additional poles at physical momenta. We tie this behavior directly to the S-matrix and show that poles at physical momenta always arise from scattering of particles present in the initial state. We relate these flat-space in-in correlators to the probability amplitude for exciting multiple Unruh-de Witt detectors. Localizing the detectors in spacetime, through the uncertainty principle, provides the energy and momentum needed to excite the vacuum and explains the connection to cosmological particle production. In addition, the entanglement of these detectors provides a probe of the entangled state of the underlying field and connects the properties of the correlators to the range of entanglement of the detectors.

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Cited by 1 Pith paper

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  1. When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity

    gr-qc 2026-01 conditional novelty 6.0

    In ultra-slow-roll inflation, the Wigner function of the inflationary Goldstone field becomes negative and its negativity grows with the scale factor squared, so the perturbations do not automatically become classical.