Loop blow-up inflation

We present a new model of string inflation driven by a blow-up Kähler modulus of type IIb compactifications with a potential generated by string loops. Slow-roll is naturally realized thanks to the fact that the blow-up mode is a leading-order flat direction lifted by string loops which are unavoid...

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Hauptverfasser: Bansal, Sukṛti (Verfasst von) , Brunelli, Luca (Verfasst von) , Cicoli, Michele (Verfasst von) , Hebecker, Arthur (Verfasst von) , Küspert, Ruben (Verfasst von)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: July 31, 2024
In: Journal of high energy physics
Year: 2024, Heft: 7, Pages: 1-40
ISSN:1029-8479
DOI:10.1007/JHEP07(2024)289
Online-Zugang:Verlag, kostenfrei, Volltext: https://doi.org/10.1007/JHEP07(2024)289
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Verfasserangaben:Sukṛti Bansal, Luca Brunelli, Michele Cicoli, Arthur Hebecker and Ruben Kuespert
Beschreibung
Zusammenfassung:We present a new model of string inflation driven by a blow-up Kähler modulus of type IIb compactifications with a potential generated by string loops. Slow-roll is naturally realized thanks to the fact that the blow-up mode is a leading-order flat direction lifted by string loops which are unavoidable and generate a plateau at large field values. We check that throughout the whole inflationary dynamics the effective field theory is under control. We perform a phenomenological analysis determining the exact number of efoldings by studying the post-inflationary evolution. We determine the values of the microscopic parameters which lead to agreement with CMB data, together with the prediction of a tensor-to-scalar ratio of order r ∼ 10−5.
Beschreibung:Gesehen am 14.07.2025
Beschreibung:Online Resource
ISSN:1029-8479
DOI:10.1007/JHEP07(2024)289