TY  - JOUR
AU  - Escudero, M.
AU  - Ramirez, H.
AU  - Boubekeur, L.
AU  - Giusarma, E.
AU  - Mena, O.
PY  - 2016
DA  - 2016//
TI  - The present and future of the most favoured inflationary models after Planck 2015
T2  - J. Cosmol. Astropart. Phys.
JO  - Journal of Cosmology and Astroparticle Physics
SP  - 020
EP  - 21pp
VL  - 02
IS  - 2
PB  - Iop Publishing Ltd
KW  - inflation
KW  - cosmological parameters from CMBR
KW  - CMBR experiments
AB  - The value of the tensor-to-scalar ratio r in the region allowed by the latest Planck 2015 measurements can be associated to a large variety of inflationary models. We discuss here the potential of future Cosmic Microwave Background cosmological observations in disentangling among the possible theoretical scenarios allowed by our analyses of current Planck temperature and polarization data. Rather than focusing only on r, we focus as well on the running of the primordial power spectrum, alpha(s) and the running thereof, beta(s). If future cosmological measurements, as those from the COrE mission, confirm the current best-fit value for beta(s) greater than or similar to 10(-2) as the preferred one, it will be possible to rule-out the most favoured inflationary models.
SN  - 1475-7516
UR  - https://arxiv.org/abs/1509.05419
UR  - https://doi.org/10.1088/1475-7516/2016/02/020
DO  - 10.1088/1475-7516/2016/02/020
LA  - English
N1  - WOS:000372467600021
ID  - Escudero_etal2016
ER  -