Affiliation:
1. Department of Physics, University of Cyprus, P.O. Box 20537, 1678 Nicosia, Cyprus
Abstract
We review the realization of Starobinsky-type inflation within induced-gravity supersymmetric (SUSY) and non-SUSY models. In both cases, inflation is in agreement with the current data and can be attained for sub-Planckian values of the inflation. The corresponding effective theories retain perturbative unitarity up to the Planck scale and the inflation mass is predicted to be 3·1013 GeV. The supergravity embedding of these models is achieved by employing two gauge singlet chiral superfields, a superpotential that is uniquely determined by a continuous R and a discrete Zn symmetry and several (semi)logarithmic Kähler potentials that respect these symmetries. Checking various functional forms for the noninflation accompanying field in the Kähler potentials, we identify four cases which stabilize it without invoking higher order terms.
Subject
Nuclear and High Energy Physics
Cited by
19 articles.
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1. Fermion mass, axion dark matter, and leptogenesis in SO(10) GUT;Physical Review D;2024-03-07
2. Formulating E- & T-Model Inflation in Supergravity;Journal of Physics: Conference Series;2022-11-01
3. An alternative framework for E-model inflation in supergravity;The European Physical Journal C;2022-05
4. Supersymmetric ν-inflaton Dark Matter;Journal of Cosmology and Astroparticle Physics;2021-04-01
5. Non-oscillatory no-scale inflation;Journal of Cosmology and Astroparticle Physics;2021-03-01