New- vs. chaotic-inflations
Cosmology and Nongalactic Astrophysics
2016-03-16 v4 High Energy Physics - Phenomenology
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 .
Cite
@article{arxiv.1504.02080,
title = {New- vs. chaotic-inflations},
author = {Gabriela Barenboim and Wan-Il Park},
journal= {arXiv preprint arXiv:1504.02080},
year = {2016}
}
Comments
17 pages, 1 figure, 2 tables: the published version