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Fitting string inflation to real cosmological data: the Fibre Inflation case
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In this paper we show how the string landscape can be constrained using observational data. We illustrate this idea by focusing on Fibre Inflation which is a promising class of string inflationary models in type IIB flux compactifications. We determine the values of the microscopic flux-dependent parameters which yield the best fit to the most recent cosmological datasets.
Forward citations
Cited by 4 Pith papers
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