Starobinsky Inflation with T-Model Kähler Geometries

We present novel implementations of Starobisky-like inflation within supergravity adopting Kähler potentials for the inflaton which parameterizes hyperbolic geometries known from 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 Kähler potential. Keeping the Kähler manifold intact, a conveniently violated shift symmetry is introduced which allows for slight variation in 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 Kähler manifold increases with the tensor-to-scalar ratio.

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Publication Details

Journal
Universe
Published
2025-02-21
DOI
https://doi.org/10.3390/universe11030075
Citations
2
Primary Topic
Geometry and complex manifolds
Type
article
Field-Weighted Citation Impact
8.18
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article

Starobinsky Inflation with T-Model Kähler Geometries

C. Pallis
2 citations
Universe
Geometry and complex manifolds
8.18
article

Starobinsky Inflation with T-Model Kähler Geometries

C. Pallis
article en
2 citations

Abstract

We present novel implementations of Starobisky-like inflation within supergravity adopting Kähler potentials for the inflaton which parameterizes hyperbolic geometries known from 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 Kähler potential. Keeping the Kähler manifold intact, a conveniently violated shift symmetry is introduced which allows for slight variation in 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 Kähler manifold increases with the tensor-to-scalar ratio.

UniverseVol. 11(3)
Aristotle University of Thessaloniki (GR)
Openalex Percentile: Top 4%
Geometry and complex manifolds
8.18
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