@Article{Gariazzo_etal2017,
author="Gariazzo, S.
and Mena, O.
and Miralles, V.
and Ramirez, H.
and Boubekeur, L.",
title="Running of featureful primordial power spectra",
journal="Physical Review D",
year="2017",
publisher="Amer Physical Soc",
volume="95",
number="12",
pages="123534--7pp",
abstract="Current measurements of the temperature and polarization anisotropy power spectra of the cosmic microwave background (CMB) seem to indicate that the naive expectation for the slow-roll hierarchy within the most simple inflationary paradigm may not be respected in nature. We show that a primordial power spectrum with localized features could in principle give rise to the observed slow-roll anarchy when fitted to a featureless power spectrum. From a model comparison perspective, and assuming that nature has chosen a featureless primordial power spectrum, we find that, while with mock Planck data there is only weak evidence against a model with localized features, upcoming CMB missions may provide compelling evidence against such a nonstandard primordial power spectrum. This evidence could be reinforced if a featureless primordial power spectrum is independently confirmed from bispectrum and/or galaxy clustering measurements.",
optnote="WOS:000404475200004",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=3186), last updated on Thu, 13 Jul 2017 15:02:16 +0000",
issn="2470-0010",
doi="10.1103/PhysRevD.95.123534",
opturl="http://arxiv.org/abs/1701.08977",
opturl="https://doi.org/10.1103/PhysRevD.95.123534",
archivePrefix="arXiv",
eprint="1701.08977",
language="English"
}