On the Asymptotic Nature of Cosmological Effective Theories
Carlos Duaso Pueyo, Harry Goodhew, Ciaran McCulloch, Enrico Pajer

TL;DR
This paper reveals that cosmological effective field theories are inherently asymptotic due to factorial growth of operator contributions in expanding spacetimes, affecting their convergence and predictive power.
Contribution
It demonstrates the asymptotic nature of cosmological EFTs and introduces resummation methods to extract meaningful predictions, contrasting with flat spacetime EFT behavior.
Findings
Operator contributions grow factorially with dimension in expanding backgrounds.
EFT predictions can be recovered through resummation techniques.
In the infinite sound speed limit, EFT reproduces full theory results.
Abstract
Much of our intuition about Effective Field Theories (EFTs) stems from their formulation in flat spacetime, yet EFTs have become indispensable tools in cosmology, where time-dependent backgrounds are the norm. In this work, we demonstrate that in spacetimes undergoing significant expansion-such as accelerated FLRW and de Sitter backgrounds-the contributions of operators with mass dimension to physical observables grow factorially with at fixed couplings. This behavior stands in stark contrast to static flat spacetime. As a result, the cosmological EFT expansion is generally asymptotic rather than convergent, even at tree level. To illustrate this phenomenon, we analyze simple toy models involving a massless or conformally coupled scalar field interacting with a heavy scalar with zero or infinite sound speed. We demonstrate that meaningful EFT predictions can still be…
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