$\lambda\phi^4$ as an Effective Theory in de Sitter
Sebastian Cespedes, Zhehan Qin, Dong-Gang Wang

TL;DR
This paper analyzes effective field theories for scalar fields in de Sitter space, revealing how the cutoff scale influences unitarity, state evolution, and the sign of the quartic coupling, with implications for cosmological models.
Contribution
It provides a complete analytic matching of $bbb4$ theories with UV models, highlighting non-unitary effects and the behavior of the quartic coupling as the cutoff varies.
Findings
Unitary description when cutoff is above horizon scale
Emergence of mixed states and diffusive effects below horizon scale
Loop-level matching shows quartic coupling becomes negative as cutoff decreases
Abstract
Effective field theories (EFTs) provide a powerful framework to parametrise unknown aspects of possible ultraviolet (UV) physics. For scalar fields in de Sitter space, however, new emergent phenomena can arise when the cut-off scale of the theory lies below the horizon scale , as seen in the stochastic formalism of inflation. In this work, we study EFTs that, at leading order, reproduce the standard quartic theory in de Sitter, but with a variable cut-off identified with the mass of an integrated-out hidden sector. We perform the complete analytic computation for the tree- and loop-level matching between the effective theory and two possible UV realisations. We find that when the cut-off is much larger than the horizon, the theory admits a unitary description, up to exponentially suppressed corrections. In contrast, when the cut-off is lowered below , the system…
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