Nonlocal Entanglement and Directional Correlations of Primordial
  Perturbations on the Inflationary Horizon
  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 $\Delta_S^2\approx H t_P$, the product of inflationary
expansion rate $H$ with Planck time $t_P$, 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. New statistical estimators are developed to study unique
signatures in CMB anisotropy and large scale galaxy surveys.
