arXiv · 1407.1048
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.
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Michele Cicoli, Sean Downes, Bhaskar Dutta, Francisco G. Pedro, Alexander Westphal. 2014-07-03. Just enough inflation: power spectrum modifications at large scales. https://doi.org/10.1088/1475-7516%2F2014%2F12%2F030
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