Superhorizon entanglement entropy from particle decay in inflation
Louis Lello, Daniel Boyanovsky, Richard Holman

TL;DR
This paper studies how particle decay during inflation leads to superhorizon entanglement entropy, revealing quantum correlations across the horizon and their growth with volume, with potential implications for cosmological observations.
Contribution
It extends a unitary quantum field theoretical method to analyze superhorizon entanglement entropy from particle decay in inflationary cosmology, including infrared effects and generalizations to wave packets.
Findings
Entanglement between superhorizon and subhorizon fluctuations due to particle decay.
Entanglement entropy grows with physical volume as more modes cross the horizon.
Decay processes may influence non-Gaussianity and CMB anomalies.
Abstract
In inflationary cosmology all particle states decay as a consequence of the lack of kinematic thresholds. The decay of an initial single particle state yields an \emph{entangled quantum state of the product particles}. We generalize and extend a manifestly unitary field theoretical method to obtain the time evolution of the quantum state. We consider the decay of a light scalar field with mass with a cubic coupling in de Sitter space-time. Radiative corrections feature an infrared enhancement manifest as poles in and we obtain the quantum state in an expansion in . To leading order in the pure state density matrix describing the decay of a particle with sub-horizon wavevector is dominated by the emission of superhorizon quanta, describing \emph{entanglement between superhorizon and subhorizon fluctuations and correlations across the horizon}.…
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