Chiral gravitational waves and primordial black holes in UV-protected Natural Inflation
Juan P. Beltr\'an Almeida, Nicol\'as Bernal, Dario Bettoni, Javier, Rubio

TL;DR
This paper proposes a UV-protected Natural Inflation model with Chern-Simons interactions that supports sub-Planckian inflation, generates primordial black holes as dark matter, and predicts observable chiral gravitational waves.
Contribution
It introduces a novel inflation scenario combining gravitational and quantum friction, enabling sub-Planckian potentials, primordial black hole dark matter, and detectable chiral gravitational waves.
Findings
Supports sub-Planckian inflation potentials
Predicts primordial black hole formation as dark matter
Forecasts observable chiral gravitational wave background
Abstract
We consider an UV-protected Natural Inflation scenario involving Chern-Simons-like interactions between the inflaton and some beyond the Standard Model gauge fields. The accelerated expansion of the Universe is supported by a combination of a gravitationally-enhanced friction sensitive to the scale of inflation and quantum friction effects associated with the explosive production of gauge fluctuations. The synergy of these two velocity-restraining mechanisms allows for: Natural Inflation potentials involving only sub-Planckian coupling constants, the generation of a dark matter component in the form of primordial black holes, and a potentially observable background of chiral gravitational waves at small scales.
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