New- vs. chaotic- inflations

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Published 23 February 2016 © 2016 IOP Publishing Ltd and Sissa Medialab srl
, , Citation Gabriela Barenboim and Wan-Il Park JCAP02(2016)061 DOI 10.1088/1475-7516/2016/02/061

1475-7516/2016/02/061

Abstract

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 Script O(10−4–10−3).

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10.1088/1475-7516/2016/02/061