A sudden small change in the second derivative of the inflaton potentialcan result in a universal local feature in the spectrum of primordialperturbations generated during inflation. The exact solution describingthis feature \\cite{minu} is characterized by a step in the spectral indexmodulated by characteristic oscillations and results in a large running of thespectral index localized over a few e-folds of scale. In this paper weconfront this step-like feature with the 5 year WMAP results and demonstratethat it provides a better fit to this data than a featureless initial spectrum.If such a feature exists at all, then it should lie at sufficiently large scalesk0 ≲ 0.003 Mpc−1 corresponding to l ≲ 40. The signof the effect is shown to correspond to the negative running of nslocalized near this scale. This feature could arise as a result of a`mini-waterfall'-type fast second order phase transitionexperienced by an auxiliary heavy field during inflation, in a modelsimilar to hybrid inflation (though for a different choice of parameters).If this is the case, then theauxiliary field should be positively coupled to the inflaton.
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