Minimal decoherence from inflation
C.P. Burgess, R. Holman, Greg Kaplanek, Jerome Martin, Vincent Vennin

TL;DR
This paper calculates the minimal rate at which inflationary cosmological fluctuations decohere due to gravitational interactions, revealing that decoherence is efficient at high inflation scales and providing insights into quantum effects in the early universe.
Contribution
It introduces a controlled Open Effective Field Theory approach to compute inflationary decoherence, considering only self-interactions from General Relativity in single-clock models.
Findings
Decoherence is suppressed by slow-roll parameters and energy density.
Decoherence is enhanced by the volume within the Hubble scale.
At GUT-scale inflation, decoherence is nearly complete for most scales.
Abstract
We compute the rate with which super-Hubble cosmological fluctuations are decohered during inflation, by their gravitational interactions with unobserved shorter-wavelength scalar and tensor modes. We do so using Open Effective Field Theory methods, that remain under control at the late times of observational interest, contrary to perturbative calculations. Our result is minimal in the sense that it only incorporates the self-interactions predicted by General Relativity in single-clock models (additional interaction channels should only speed up decoherence). We find that decoherence is both suppressed by the first slow-roll parameter and by the energy density during inflation in Planckian units, but that it is enhanced by the volume comprised within the scale of interest, in Hubble units. This implies that, for the scales probed in the Cosmic Microwave Background, decoherence is…
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