Inflationary Particle Production and the Swampland

TL;DR

This paper examines how an infinite tower of states, motivated by string theory and the Swampland Distance Conjecture, affects inflationary observables, finding that their impact is generally suppressed in weakly coupled regimes, preserving standard inflation predictions.

Contribution

It provides a detailed analysis of particle production effects during inflation from a string-inspired tower of states and shows their negligible impact on inflationary observables in weak coupling regimes.

Findings

Tower-induced corrections are suppressed by (H/Λ_sp)^{2+p}

Inflationary phenomenology remains consistent with observations

Explicit analysis across various inflationary potentials

Abstract

We investigate the impact of particle production during inflation in scenarios where an infinite tower of states features a mass scale that decreases exponentially along the inflationary trajectory. Such couplings naturally arise in string effective field theories and are in fact motivated by the Swampland Distance Conjecture (SDC). We show that the corrections to inflationary observables sourced by the tower scale as $(H/\Lambda_{\text{sp}})^{2+p}$, with $H$ being the Hubble scale, $\Lambda_{\text{sp}}$ being the species scale, that is the quantum gravity cut-off, and $p\geq 1$ characterizes the density of states in the tower. As a result, in gravitationally weakly coupled cosmological effective theories, the tower-induced contributions are suppressed relative to the standard single-field predictions, leaving the inflationary phenomenology essentially unchanged. We demonstrate this explicitly across a set of well-motivated inflationary potentials, and we compare the resulting predictions with the most recent observational constraints, including those from the Atacama Cosmology Telescope.