Perturbative Kähler Moduli Inflation

In this work, we present two classes of inflationary models in the framework of type IIB string theory. The inflatons correspond to blow-up Kähler modulus arising from compactifying type IIB string theory on a Calabi-Yau. Using perturbative corrections, we first highlight a procedure for stabilising more than one Kähler modulus. For the case of two Kähler moduli, we explicitly construct two classes of inflationary potentials within the Kähler cone which satisfy both EFT and cosmological constraints. The first class of models, arising from moduli redefinition of the blow-up mode, garners a potential of the form [Formula: see text] align with CMB data with scalar-to-tensor ratio [Formula: see text]. The second class of models, which have been recently proposed as loop blow-up inflation, have a form [Formula: see text], also agrees with CMB data with scalar-to tensor-ratio [Formula: see text]. Our work differs from the original loop blow-up inflation in terms of stabilization mechanism and subsequently the scalar-to tensor ratio.

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Publication Details

Journal
International Journal of Modern Physics D
Published
2026-10-30
DOI
https://doi.org/10.1142/s0218271826500719
Primary Topic
Cosmology and Gravitation Theories
Type
article
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article

Perturbative Kähler Moduli Inflation

Mishaal Hai, Md Shaikot Jahan Shuvo, Ahmed Rakin Kamal, Noshin Ferdous Shamma
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International Journal of Modern Physics D
Cosmology and Gravitation Theories
article

Perturbative Kähler Moduli Inflation

Mishaal Hai, Md Shaikot Jahan Shuvo, Ahmed Rakin Kamal, Noshin Ferdous Shamma
article en

Abstract

In this work, we present two classes of inflationary models in the framework of type IIB string theory. The inflatons correspond to blow-up Kähler modulus arising from compactifying type IIB string theory on a Calabi-Yau. Using perturbative corrections, we first highlight a procedure for stabilising more than one Kähler modulus. For the case of two Kähler moduli, we explicitly construct two classes of inflationary potentials within the Kähler cone which satisfy both EFT and cosmological constraints. The first class of models, arising from moduli redefinition of the blow-up mode, garners a potential of the form [Formula: see text] align with CMB data with scalar-to-tensor ratio [Formula: see text]. The second class of models, which have been recently proposed as loop blow-up inflation, have a form [Formula: see text], also agrees with CMB data with scalar-to tensor-ratio [Formula: see text]. Our work differs from the original loop blow-up inflation in terms of stabilization mechanism and subsequently the scalar-to tensor ratio.

International Journal of Modern Physics D
Openalex Percentile: Top 98%
Cosmology and Gravitation Theories
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Perturbative Kähler Moduli Inflation — Mishaal Hai, Md Shaikot Jahan Shuvo, et al. · International Journal of Modern Physics D (2026) | TGRS Research Map | TGRS