Inflection point inflation and dark energy in supergravity
arXiv:1503.05643 · doi:10.1103/PhysRevD.91.123502
Abstract
We consider an inflection point inflationary model in supergravity with a single chiral superfield and show that the predicted values of the scalar spectral index and tensor-to-scalar ratio are consistent with the Planck 2015 results. In this model supersymmetry is strongly broken after inflation, which results in a non-SUSY de-Sitter vacuum responsible for the recent accelerated expansion of the Universe.
accepted for publication in Phys. Rev. D
References in corpus (10)
- Gauge invariant MSSM inflaton
- New models of chaotic inflation in supergravity
- General inflaton potentials in supergravity
- Inflaton Decay through Supergravity Effects
- Analytic Classes of Metastable de Sitter Vacua
- Inflation in Supergravity with a Single Chiral Superfield
- Attraction towards an inflection point inflation
- Generic Scalar Potentials for Inflation in Supergravity with a Single Chiral Superfield
- Inflation and Dark Energy with a Single Superfield
- Bound on largest from sub-Planckian excursions of inflaton