PaperPanorama

arXiv:1512.05657·v3·High Energy Physics — Phenomenology

Starobinsky-Type Inflation With Products of Kaehler Manifolds

C. Pallis🇨🇾 · N. Toumbas🇨🇾

PDFarXivINSPIREDOI

Abstract

We present a novel realization of Starobinsky-type inflation within Supergravity using two chiral superfields. The proposed superpotential is inspired by induced-gravity models. The Kaehler potential contains two logarithmic terms, one for the inflaton T and one for the matter-like field S, parameterizing the SU(1,1)/U(1)x SU(2)/U(1) Kaehler manifold. The two factors have constant curvatures -m/n and 2/n2, where n, m are the exponents of T in the superpotential and Kaehler potential respectively, and 0<n2<=6. The inflationary observables depend on the ratio 2n/m only. Essentially they coincide with the observables of the original Starobinsky model. Moreover, the inflaton mass is predicted to be 3x10^13 GeV.

Comments: Final version with some typos corrected

Citation historyopen in Citation History ↗