Just enough inflation: power spectrum modifications at large scales

Abstract

We show that models of `just enough' inflation, where the slow-roll evolution lasted only $50-60$ e-foldings, feature modifications of the CMB power spectrum at large angular scales. We perform a systematic and model-independent analysis of any possible non-slow-roll background evolution prior to the final stage of slow-roll inflation. We find a high degree of universality since most common backgrounds like fast-roll evolution, matter or radiation-dominance give rise to a power loss at large angular scales and a peak together with an oscillatory behaviour at scales around the value of the Hubble parameter at the beginning of slow-roll inflation. Depending on the value of the equation of state parameter, different pre-inflationary epochs lead instead to an enhancement of power at low-$\ell$, and so seem disfavoured by recent observational hints for a lack of CMB power at $\ell \lesssim 40$. We also comment on the importance of initial conditions and the possibility to have multiple pre-inflationary stages.

31 pages, 13 figures

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• Power Spectrum of Inflationary Attractors
• Corrections to $n_s$ and $n_t$ from high scale physics
• Large Scale Suppression of Scalar Power on a Spatial Condensation
• Signatures of the Very Early Universe: Inflation, Spatial Curvature and Large Scale Anomalies