Squeezed vacua and primordial features in effective theories of inflation at N2LO
A finite duration of cosmic inflation can result in features $mathcal{P}_{mathcal{R}}(k)=|alpha_k-beta_k,mathrm{e}^{mathrm{i}delta_k}|^2 mathcal{P}_{mathcal{R}}^{(0)}(k)$ in the primordial power spectrum that carry information about a quantum gravity phase before inflation. While the almost-scale-invariant power spectrum $mathcal{P}_{mathcal{R}}^{(0)}$ for the quasi-Bunch-Davies vacuum is fully determined by the inflationary background dynamics, the Bogoliubov coefficients $alpha_k$ and $beta_k$ for the squeezed vacuum depend on new physics beyond inflation and have been used to produce phenomenological templates for the features. In this paper, we consider a large class of effective theories of inflation and compute the relative phase $delta_k$. While this phase vanishes in de Sitter space, here we show that it is fully determined by the inflationary background dynamics and we compute it up to the next-to-next-leading order (N2LO) in a Hubble-flow expansion. In particular, for the Starobinsky model of inflation we find that this relative phase can be expressed in terms of the scalar tilt $n_mathrm{s}$ as $delta_k=frac{pi}{2}(n_mathrm{s}-1)-frac{pi}{4}(n_mathrm{s}-1)^2,ln(k/k_*)$. The relative phase results in a negative shift and a running frequency that have been considered in the most studied phenomenological templates for primordial features, thus providing precise theoretical predictions for upcoming cosmological observations.