Fluid phonons and inflaton quanta at the protoinflationary transition

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.

30 pages, 3 figures

References in corpus (5)

• Non-gaussianities and the Stimulated creation of quanta in the inflationary universe
• Enhanced polarization of CMB from thermal gravitational waves
• Hanbury Brown-Twiss interferometry and second-order correlations of inflaton quanta
• Cosmological status of Lagrangian theory of density perturbations
• Gradient expansion, curvature perturbations and magnetized plasmas

Cited by in corpus (5)

• No-hair conjectures, primordial shear and protoinflationary initial conditions
• Fluid phonons, protoinflationary dynamics and large-scale gravitational fluctuations
• The symmetries of inflationary magnetogenesis and the plasma initial conditions
• Violation of consistency relations and the protoinflationary transition
• Has inflation really solved the problems of flatness and absence of relics?