%0 Journal Article
%T New- vs. chaotic- inflations
%A Barenboim, G.
%A Park, W. I.
%J Journal of Cosmology and Astroparticle Physics
%D 2016
%V 02
%N 2
%I Iop Publishing Ltd
%@ 1475-7516
%G English
%F Barenboim+Park2016
%O WOS:000372467600062
%O exported from refbase (https://references.ific.uv.es/refbase/show.php?record=2589), last updated on Fri, 15 Apr 2016 12:55:44 +0000
%X 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 O(10(-4)-10(-3)).
%K inflation
%K physics of the early universe
%K cosmology of theories beyond the SM
%R 10.1088/1475-7516/2016/02/061
%U https://arxiv.org/abs/1504.02080
%U https://doi.org/10.1088/1475-7516/2016/02/061
%P 061-20pp