New- vs. chaotic-inflations
classification
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hep-ph
keywords
modelschaotic-inflationchaotic-inflationscontrastdirectexperimentallyidentifiedmathcal
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We show that "spiralized" models of new-inflation can be experimentally identified mostly by their positive spectral running in direct contrast with most chaotic-inflation models which have negative runnings typically in the range of $\mathcal{O}(10^{-4}-10^{-3})$.
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