$ΔN$ Formalism and Conserved Currents in Cosmology

Abstract

The $ΔN$ formalism, based on the counting of the number of e-folds during inflation in different local patches of the Universe, has been introduced several years ago as a simple and physically intuitive approach to calculate (non-linear) curvature perturbations from inflation on large sales, without resorting to the full machinery of (higher-order) perturbation theory. Later on, it was claimed the equivalence with the results found by introducing a conserved fully non-linear current $ζ_μ$, thereby allowing to directly connect perturbations during inflation to late-Universe observables. We discus some issues arising from the choice of the initial hyper-surface in the $ΔN$ formalism. By using a novel exact expression for $ζ_μ$, valid for any barotropic fluid, we find that it is not in general related to the standard uniform density curvature perturbation $ζ$; such a result conflicts with the claimed equivalence with $ΔN$ formalism. Moreover, a similar analysis is done for the proposed non-perturbative generalization ${\cal R}_μ$ of the comoving curvature perturbation ${\cal R}$.