English

Starobinsky Inflation with T-Model Kaehler Geometries

High Energy Physics - Phenomenology 2025-03-07 v2 Cosmology and Nongalactic Astrophysics High Energy Physics - Theory

Abstract

We present novel implementations of Starobisky-like inflation within Supergravity adopting Kaehler potentials for the inflaton which parameterize hyperbolic geometries known from the T-model inflation. The associated superpotentials are consistent with an R and a global or gauge U(1)_X symmetries. The inflaton is represented by a gauge-singlet or non-singlet superfield and is accompanied by a gauge-singlet superfield successfully stabilized thanks to its compact contribution into the total Kaehler potential. Keeping the Kaehler manifold intact, a conveniently violated shift symmetry is introduced which allows for a slight variation of the predictions of Starobinsky inflation: The (scalar) spectral index exhibits an upper bound which lies close to its central observational value whereas the constant scalar curvature of the inflaton-sector Kaehler manifold increases with the tensor-to-scalar ratio.

Keywords

Cite

@article{arxiv.2502.00636,
  title  = {Starobinsky Inflation with T-Model Kaehler Geometries},
  author = {C. Pallis},
  journal= {arXiv preprint arXiv:2502.00636},
  year   = {2025}
}
R2 v1 2026-06-28T21:29:17.772Z