Synchronizing the Consistency Relation

TL;DR

This paper investigates the consistency relations of the N-point function of density contrast in synchronous gauge during matter and radiation eras, clarifying the role of initial conditions and dynamical effects in the squeezed limit.

Contribution

It derives a simple, time-independent consistency relation in synchronous gauge and clarifies how initial and dynamical effects combine to satisfy this relation in the squeezed limit.

Findings

Single, time-independent consistency relation in synchronous gauge.

Compatibility between squeezed-limit relations and second-order perturbation theory.

Importance of averaging over oscillations for local observables during radiation era.

Abstract

We study the $N$-point function of the density contrast to quadratic order in the squeezed limit during the matter-dominated (MD) and radiation-dominated (RD) eras in synchronous gauge. Since synchronous gauge follows the free-fall frame of observers, the equivalence principle dictates that in the gradient approximation for the long-wavelength mode there is only a single, manifestly time-independent consistency relation for the $N$-point function. This simple form is dictated by the initial mapping between synchronous and local coordinates, unlike Newtonian gauge and its correspondingly separate dilation and Newtonian consistency relations. Dynamical effects only appear at quadratic order in the squeezed limit and are again characterized by a change in the local background, also known as the separate universe approach. We show that for the 3-point function the compatibility between these squeezed-limit relations and second-order perturbation theory requires both the initial and dynamical contributions to match, as they do in single-field inflation. This clarifies the role of evolution or late-time projection effects in establishing the consistency relation for observable bispectra, which is especially important for radiation acoustic oscillations and for establishing consistency below the matter-radiation equality scale in the MD era. Defining an appropriate angle and time average of these oscillations is also important for making separate universe predictions of spatially varying local observables during the RD era, which can be useful for a wider range of cosmological predictions beyond $N$-point functions.