Sensitivity of inflationary predictions to pre-inflationary phases
Sina Bahrami, Eanna E. Flanagan

TL;DR
This paper investigates how pre-inflationary radiation-dominated phases influence inflationary predictions, finding minor deviations in the power spectrum that are unlikely to be observed with current CMB data.
Contribution
It introduces a model with a radiation-dominated pre-inflationary era and derives a natural initial state, analyzing its impact on inflationary predictions.
Findings
Deviations from standard power spectrum are predicted at large scales.
Deviations are too small for near-future CMB detection.
A natural initial state for perturbations is identified.
Abstract
How sensitive are the predictions of inflation to pre-inflationary conditions when the number of efolds of inflation is not too large? In an attempt to address this question, we consider a simple model where the inflationary era is preceded by an era dominated by a radiation fluid, which is coupled to the inflaton only gravitationally and which extends back to the Planck era. We show that there is a natural generalized Bunch-Davies vacuum state for perturbations to the coupled inflaton-gravity-fluid system at early times. With this choice of initial state the model predicts interesting deviations from the standard power spectrum of single field slow-roll inflation at large scales. However, the deviations are too small to be observable in near future CMB observations.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
