@Article{Barenboim+Park2016,
author="Barenboim, G.
and Park, W. I.",
title="New- vs. chaotic- inflations",
journal="Journal of Cosmology and Astroparticle Physics",
year="2016",
publisher="Iop Publishing Ltd",
volume="02",
number="2",
pages="061--20pp",
optkeywords="inflation; physics of the early universe; cosmology of theories beyond the SM",
abstract="We show that {\textquoteleft}{\textquoteleft}spiralized{\textquoteright}{\textquoteright} 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 O(10(-4)-10(-3)).",
optnote="WOS:000372467600062",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=2589), last updated on Fri, 15 Apr 2016 12:55:44 +0000",
issn="1475-7516",
doi="10.1088/1475-7516/2016/02/061",
opturl="https://arxiv.org/abs/1504.02080",
opturl="https://doi.org/10.1088/1475-7516/2016/02/061",
language="English"
}