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arXiv · 2403.13581

A novel PBH production mechanism from non-Abelian gauge fields during inflation

Ema Dimastrogiovanni·Matteo Fasiello·Alexandros Papageorgiou
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Abstract

We consider the case of axion-like particles (ALPs) during inflation. When coupled to a non-Abelian gauge sector via a Chern-Simons term, ALPs support an intriguing, testable, phenomenology with very distinctive features including chiral primordial gravitational waves. For sufficiently small values of the gauge vev and coupling, scalar perturbations in the gauge sector exhibit a known instability. We harness the power of such instability for primordial black hole (PBH) generation. In the case of an axion-inflaton, one is dynamically driven into a strong-backreaction regime that crosses the instability band thereby sourcing a peaked scalar spectrum leading to PBH production and the related scalar-induced gravitational waves. Remarkably, this dynamics is largely insensitive to the initial conditions and the shape of the potential, highlighting the universal nature of the sourcing mechanism. In the case of spectator ALPs one can identify the parameter space that sets off the strong backreaction regime and the ensuing features. We show that spectator ALP models may also access the scalar instability region without triggering strong backreaction.

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Ema Dimastrogiovanni, Matteo Fasiello, Alexandros Papageorgiou. 2024-03-20. A novel PBH production mechanism from non-Abelian gauge fields during inflation. https://arxiv.org/abs/2403.13581

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