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The best inflationary models after Planck

Martin J.
•
Ringeval C.
•
Trotta R.
•
Vennin V.
2014
  • journal article

Periodico
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Abstract
We compute the Bayesian evidence and complexity of 193 slow-roll single-field models of inflation using the Planck 2013 Cosmic Microwave Background data, with the aim of establishing which models are favoured from a Bayesian perspective. Our calculations employ a new numerical pipeline interfacing an inflationary effective likelihood with the slow-roll library ASPIC and the nested sampling algorithm MultiNest. The models considered represent a complete and systematic scan of the entire landscape of inflationary scenarios proposed so far. Our analysis singles out the most probable models (from an Occam's razor point of view) that are compatible with Planck data, while ruling out with very strong evidence 34% of the models considered. We identify 26% of the models that are favoured by the Bayesian evidence, corresponding to 15 different potential shapes. If the Bayesian complexity is included in the analysis, only 9% of the models are preferred, corresponding to only 9 different potential shapes. These shapes are all of the plateau type. © 2014 IOP Publishing Ltd and Sissa Medialab srl.
DOI
10.1088/1475-7516/2014/03/039
WOS
WOS:000333667900039
Archivio
http://hdl.handle.net/20.500.11767/116905
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-84897557944
Diritti
closed access
Soggetti
  • CMBR experiments

  • cosmological paramete...

  • ination

  • physics of the early ...

  • Settore FIS/05 - Astr...

Scopus© citazioni
166
Data di acquisizione
Jun 7, 2022
Vedi dettagli
Web of Science© citazioni
186
Data di acquisizione
Mar 25, 2024
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