Fluid phonons and inflaton quanta at the protoinflationary transition

TL;DR

This paper investigates how quantum and thermal fluctuations in an irrotational fluid influence the transition from a decelerated protoinflationary phase to an accelerated inflationary epoch, highlighting the effects of transition sharpness and fluid-inflaton interactions.

Contribution

It provides a detailed analysis of fluid and inflaton fluctuations during the protoinflationary transition, emphasizing the role of transition dynamics and pump field properties in shaping curvature perturbations.

Findings

Sharp transitions suppress inhomogeneities

Delayed transitions enhance curvature perturbations

Transition dynamics depend on pump field monotonicity

Abstract

Quantum and thermal fluctuations of an irrotational fluid are studied across the transition regime connecting a protoinflationary phase of decelerated expansion to an accelerated epoch driven by a single inflaton field. The protoinflationary inhomogeneities are suppressed when the transition to the slow roll phase occurs sharply over space-like hypersurfaces of constant energy density. If the transition is delayed, the interaction of the quasi-normal modes related, asymptotically, to fluid phonons and inflaton quanta leads to an enhancement of curvature perturbations. It is shown that the dynamics of the fluctuations across the protoinflationary boundaries is determined by the monotonicity properties of the pump fields controlling the energy transfer between the background geometry and the quasi-normal modes of the fluctuations. After corroborating the analytical arguments with explicit numerical examples, general lessons are drawn on the classification of the protoinflationary transition.