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New- vs. chaotic- inflations

  • University of Valencia

Research output: Contribution to journalReview articlepeer-review

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 (10-4-10-3).

Original languageEnglish
Article number061
JournalJournal of Cosmology and Astroparticle Physics
Volume2016
Issue number2
DOIs
StatePublished - 2016.02.23

Keywords

  • cosmology of theories beyond the SM
  • inflation
  • physics of the early universe

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