English

Generating Entangled Inflationary Quantum States

High Energy Physics - Theory 2019-02-05 v1 Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology

Abstract

Entangled inflationary quantum states offer an interesting alternative to the standard Bunch-Davies vacuum. While they can be viewed from the point of view of a theory of effective initial states, it has been unclear exactly how such states might be generated. Using a model involving two scalar fields Φ,Σ\Phi,\Sigma we show that if {\em both} fields have non-zero time dependent expectation values ϕ,σ\phi,\sigma respectively, and if the interaction potential V(Φ,Σ)V(\Phi,\Sigma) when evaluated at these expectation values has ϕσV(ϕ,σ)0\partial_{\phi}\partial_{\sigma}V(\phi, \sigma)\neq 0, this can serve as a source term for the entanglement kernel describing the state within the Gaussian approximation around the expectation values. We also show how cubic interactions between the metric perturbation ζ\zeta and a scalar Σ\Sigma can be used to generate a source term for entanglement.

Keywords

Cite

@article{arxiv.1902.00521,
  title  = {Generating Entangled Inflationary Quantum States},
  author = {R. Holman and Benoit J. Richard},
  journal= {arXiv preprint arXiv:1902.00521},
  year   = {2019}
}

Comments

13 pages

R2 v1 2026-06-23T07:29:48.012Z