Cosmic Purity Lost: Perturbative and Resummed Late-Time Inflationary Decoherence

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Hauptverfasser: Burgess, C. P., Colas, Thomas, Holman, R., Kaplanek, Greg, Vennin, Vincent
Format: Preprint
Veröffentlicht: 2024
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author Burgess, C. P.
Colas, Thomas
Holman, R.
Kaplanek, Greg
Vennin, Vincent
author_facet Burgess, C. P.
Colas, Thomas
Holman, R.
Kaplanek, Greg
Vennin, Vincent
contents We compute the rate with which unobserved fields decohere other fields to which they couple, both in flat space and in de Sitter space, for spectator scalar fields prepared in their standard adiabatic vacuum. The process is very efficient in de Sitter space once the modes in question pass outside the Hubble scale, displaying the tell-tale phenomenon of secular growth that indicates the breakdown of perturbative methods on a time scale parameterically long compared with the Hubble time. We show how to match the perturbative evolution valid at early times onto a late-time Lindblad evolution whose domain of validity extends to much later times, thereby allowing a reliable resummation of the perturbative result beyond the perturbative regime. Super-Hubble modes turn out to be dominantly decohered by unobserved modes that are themselves also super-Hubble. Although our calculation is done for spectator fields, if applied to curvature perturbations during inflation our observations here could close a potential loophole in recent calculations of the late-time purity of the observable primordial fluctuations.
format Preprint
id arxiv_https___arxiv_org_abs_2403_12240
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Cosmic Purity Lost: Perturbative and Resummed Late-Time Inflationary Decoherence
Burgess, C. P.
Colas, Thomas
Holman, R.
Kaplanek, Greg
Vennin, Vincent
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Phenomenology
High Energy Physics - Theory
We compute the rate with which unobserved fields decohere other fields to which they couple, both in flat space and in de Sitter space, for spectator scalar fields prepared in their standard adiabatic vacuum. The process is very efficient in de Sitter space once the modes in question pass outside the Hubble scale, displaying the tell-tale phenomenon of secular growth that indicates the breakdown of perturbative methods on a time scale parameterically long compared with the Hubble time. We show how to match the perturbative evolution valid at early times onto a late-time Lindblad evolution whose domain of validity extends to much later times, thereby allowing a reliable resummation of the perturbative result beyond the perturbative regime. Super-Hubble modes turn out to be dominantly decohered by unobserved modes that are themselves also super-Hubble. Although our calculation is done for spectator fields, if applied to curvature perturbations during inflation our observations here could close a potential loophole in recent calculations of the late-time purity of the observable primordial fluctuations.
title Cosmic Purity Lost: Perturbative and Resummed Late-Time Inflationary Decoherence
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Phenomenology
High Energy Physics - Theory
url https://arxiv.org/abs/2403.12240