Particle physics model of curvaton inflation in a stable universe

Zoltán Péli, István Nándori, Zoltán Trócsányi

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We investigate a particle physics model for cosmic inflation based on the following assumptions: (i) there are at least two complex scalar fields; (ii) the scalar potential is bounded from below and remains perturbative up to the Planck scale; (iii) we assume slow-roll inflation with maximally correlated adiabatic and entropy fluctuations 50-60 e-folds before the end of inflation. The energy scale of the inflation is set automatically by the model. Assuming also at least one massive right-handed neutrino, we explore the allowed parameter space of the scalar potential as a function of the Yukawa coupling of this neutrino.

Original languageEnglish
Article number063533
JournalPhysical Review D
Issue number6
Publication statusPublished - Mar 15 2020


ASJC Scopus subject areas

  • Physics and Astronomy (miscellaneous)

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