Fitting string inflation to real cosmological data: the Fibre Inflation case. (arXiv:2004.01210v3 [astro-ph.CO] UPDATED)
<a href="http://arxiv.org/find/astro-ph/1/au:+Cicoli_M/0/1/0/all/0/1">Michele Cicoli</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Valentino_E/0/1/0/all/0/1">Eleonora Di Valentino</a>
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.
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.
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