Dante's Inferno
Marcus Berg, Enrico Pajer, Stefan Sjors
TL;DR
The paper tackles the UV sensitivity of high-scale inflation by proposing Dante's Inferno, a two-field inflation model with two axions whose fundamental field ranges remain sub-Planckian. By adiabatically eliminating the heavy direction, the model yields an effective quadratic potential for φ_eff with a suppressed mass m_eff, reproducing chaotic-inflation-like predictions while easing the η-problem. It embeds this construction in Type IIB string theory as a two-axion generalization of axion monodromy, using ED1 instantons and NS5-brane monodromy to generate the necessary cosine and monodromy terms, with a hierarchical decay-constant ratio f_r/f_θ controlling backreaction. The results show that large tensor modes can be achieved within a controlled UV-complete framework, expanding the viable parameter space for stringy inflation and illustrating how multi-field monodromy can reconcile high-scale inflation with subplanckian microphysics.
Abstract
We present a simple two-field model of inflation and show how to embed it in string theory as a straightforward generalization of axion monodromy models. Phenomenologically, the predictions are equivalent to those of chaotic inflation, and in particular include observably large tensor modes. The whole high-scale large-field inflationary dynamics takes place within a region of field space that is parametrically subplanckian in diameter, hence improving our ability to control quantum corrections and achieve slow-roll inflation.
