Global Embedding of Fibre Inflation Models
Michele Cicoli, Francesco Muia, Pramod Shukla
TL;DR
This paper advances string cosmology by constructing the first explicit globally consistent Type IIB Calabi–Yau orientifold embeddings of fibre inflation within LVS framework, using CYs with $h^{1,1}=3$ that are K3 (or $\mathbb{T}^4$) fibred over $\mathbb{P}^1$ and include a shrinkable rigid divisor. It performs a Kreuzer–Skarke scan to identify 45 suitable weak Swiss-cheese geometries, then builds globally consistent orientifold and D3/D7-brane setups, computing string-loop and higher-derivative ($F^4$) corrections to realize the fibre inflation potential and study their impact on inflaton dynamics. The explicit global model analysis shows that the flat fibre direction can be lifted to yield a controlled plateau, enabling inflation with predictions such as $r$ around $0.006$–$0.01$ and $n_s$ in the Planck-preferred range, while also validating moduli stabilisation and EFT consistency. A key limitation is that $h^{1,1}=3$ cannot accommodate a chiral visible sector, motivating future work on $h^{1,1}=4$ Calabi–Yau manifolds to incorporate visible-sector chirality and a concrete dS uplifting mechanism.
Abstract
We present concrete embeddings of fibre inflation models in globally consistent type IIB Calabi-Yau orientifolds with closed string moduli stabilisation. After performing a systematic search through the existing list of toric Calabi-Yau manifolds, we find several examples that reproduce the minimal setup to embed fibre inflation models. This involves Calabi-Yau manifolds with $h^{1,1}= 3$ which are K3 fibrations over a $\mathbb{P}^1$ base with an additional shrinkable rigid divisor. We then provide different consistent choices of the underlying brane set-up which generate a non-perturbative superpotential suitable for moduli stabilisation and string loop corrections with the correct form to drive inflation. For each Calabi-Yau orientifold setting, we also compute the effect of higher derivative contributions and study their influence on the inflationary dynamics.
