A no-scale inflationary model to fit them all

John Ellis, Marcos A.G. García, Dimitri V. Nanopoulos, Keith A. Olive

Research output: Contribution to journalArticlepeer-review

54 Citations (Scopus)
148 Downloads (Pure)

Abstract

The magnitude of B-mode polarization in the cosmic microwave background as measured by BICEP2 favours models of chaotic inflation with a quadratic m2 phgr2/2 potential, whereas data from the Planck satellite favour a small value of the tensor-to-scalar perturbation ratio r that is highly consistent with the Starobinsky R +R2 model. Reality may lie somewhere between these two scenarios. In this paper we propose a minimal two-field no-scale supergravity model that interpolates between quadratic and Starobinsky-like inflation as limiting cases, while retaining the successful prediction ns sime 0.96.
Original languageEnglish
Article number044
Number of pages22
JournalJournal Of Cosmology And Astroparticle Physics
Volume2014
Issue number08
Early online date19 Aug 2014
DOIs
Publication statusPublished - 19 Aug 2014

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