Squeezed vacua and primordial features in effective theories of inflation at N2LO
Eugenio Bianchi, Mauricio Gamonal

TL;DR
This paper derives a detailed theoretical expression for phase features in the primordial power spectrum during inflation, incorporating effects beyond leading order in effective theories, with implications for interpreting cosmological data.
Contribution
It provides a closed-form, next-to-next-leading order (N2LO) expression for the phase in primordial features within effective inflationary theories, connecting it to observable parameters like the scalar tilt.
Findings
Derived a closed-form expression for the phase _k in inflationary models.
Connected the phase _k to the scalar tilt n_s in the Starobinsky model.
Predicted a negative shift and running frequency in primordial features.
Abstract
A finite duration of cosmic inflation can result in features in the primordial power spectrum that carry information about a quantum gravity phase before inflation. While the almost scale-invariant power spectrum for the quasi-Bunch-Davies vacuum is fully determined by the inflationary background dynamics, the Bogoliubov coefficients and for the squeezed vacuum depend on new physics beyond inflation and have been used to produce phenomenological templates for the features. The phase vanishes in de Sitter space and therefore is often neglected, but it results in non-trivial effects in quasi-de Sitter inflationary geometries. Here we consider a large class of effective theories of inflation and provide…
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Solar and Space Plasma Dynamics
