The Open Effective Field Theory of Inflation
Santiago Agui Salcedo, Thomas Colas, Enrico Pajer

TL;DR
This paper develops an open effective field theory framework for inflation, incorporating dissipative and non-unitary effects, to better understand primordial perturbations and their observable signatures.
Contribution
It introduces a Schwinger-Keldysh path integral approach for an open EFT of inflation, including environment interactions and derivative expansion predictions.
Findings
Predicted an enhanced bispectrum near folded configurations.
Derived power spectrum and bispectrum depend on finite effective couplings.
Matched the open EFT to explicit inflationary models.
Abstract
In our quest to understand the generation of cosmological perturbations, we face two serious obstacles: we do not have direct information about the environment experienced by primordial perturbations during inflation, and our observables are practically limited to correlators of massless fields, heavier fields and derivatives decaying exponentially in the number of e-foldings. The flexible and general framework of open systems has been developed precisely to face similar challenges. Building on previous work, we develop a Schwinger-Keldysh path integral description for an open effective field theory of inflation, describing the possibly dissipative and non-unitary evolution of the Goldstone boson of time translations interacting with an unspecified environment, under the key assumption of locality in space and time. Working in the decoupling limit, we study the linear and interacting…
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Taxonomy
TopicsEconomic Theory and Policy · Economic theories and models
