Nonlocal entanglement and directional correlations of primordial perturbations on the inflationary horizon

Hogan, Craig

doi:10.1103/PhysRevD.99.063531

Title: Nonlocal entanglement and directional correlations of primordial perturbations on the inflationary horizon

Journal Article · Mon Mar 25 00:00:00 EDT 2019 · Physical Review D

DOI:https://doi.org/10.1103/PhysRevD.99.063531· OSTI ID:1484457

Hogan, Craig ^[1]

Univ. of Chicago, Chicago, IL (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

Models are developed to estimate properties of relic cosmic perturbations with “spooky” nonlocal correlations on the inflationary horizon, analogous to those previously posited for information on black hole event horizons. Scalar curvature perturbations are estimated to emerge with a dimensionless power spectral density Δ²_S ≈ Ht_P, the product of inflationary expansion rate H with Planck time tP, larger than standard inflaton fluctuations. Current measurements of the spectrum are used to derive constraints on parameters of the effective potential in a slow-roll background. It is shown that spooky nonlocality can create statistically homogeneous and isotropic primordial curvature perturbations that are initially directionally antisymmetric. In conclusion, new statistical estimators are developed to study unique signatures in cosmic microwave background anisotropy and large-scale galaxy surveys.

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Research Organization:: Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: AC02-07CH11359

OSTI ID:: 1484457

Alternate ID(s):: OSTI ID: 1546198

Report Number(s):: arXiv:1811.03283; FERMILAB-PUB-18-178-A; PRVDAQ; 1702652

Journal Information:: Physical Review D, Vol. 99, Issue 6; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 10 works

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