Resurrecting quadratic inflation in no-scale supergravity in light of BICEP2

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

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The magnitude of primordial tensor perturbations reported by the BICEP2 experiment is consistent with simple models of chaotic inflation driven by a single scalar field with a power-law potential ∝ φn : n ≳ 2, in contrast to the WMAP and Planck results, which favored models resembling the Starobinsky R+R2 model if running of the scalar spectral index could be neglected. While models of inflation with a quadratic potential may be constructed in simple N = 1 supergravity, these constructions are more challenging in no-scale supergravity. We discuss here how quadratic inflation can be accommodated within supergravity, focusing primarily on the no-scale case. We also argue that the quadratic inflaton may be identified with the supersymmetric partner of a singlet (right-handed) neutrino, whose subsequent decay could have generated the baryon asymmetry via leptogenesis.

Original languageEnglish (US)
Article number037
JournalJournal of Cosmology and Astroparticle Physics
Issue number5
StatePublished - May 2014


  • gravitational waves and CMBR polarization
  • ination
  • supersymmetry and cosmology


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