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...

Full description

Saved in:
Bibliographic Details
Main Authors: Bansal, Sukṛti (Author) , Brunelli, Luca (Author) , Cicoli, Michele (Author) , Hebecker, Arthur (Author) , Küspert, Ruben (Author)
Format: Article (Journal)
Language:English
Published: July 31, 2024
In: Journal of high energy physics
Year: 2024, Issue: 7, Pages: 1-40
ISSN:1029-8479
DOI:10.1007/JHEP07(2024)289
Online Access:Verlag, kostenfrei, Volltext: https://doi.org/10.1007/JHEP07(2024)289
Get full text
Author Notes:Sukṛti Bansal, Luca Brunelli, Michele Cicoli, Arthur Hebecker and Ruben Kuespert
Description
Summary: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.
Item Description:Gesehen am 14.07.2025
Physical Description:Online Resource
ISSN:1029-8479
DOI:10.1007/JHEP07(2024)289