Reconciling axion quality with post-inflation cosmology
Luca Di Luzio, Samuele Di Valeriano, Marco Nardecchia, Enrico Nardi
Abstract
We address the axion quality/cosmology tension that often plagues QCD axion models in post-inflationary Peccei-Quinn (PQ) breaking scenarios. In the proposed framework, the PQ symmetry emerges accidentally from an SU(N)L× SU(N)R gauge symmetry spontaneously broken to SU(N)L+R, and its quality is protected because PQ breaking first appears at operator dimension N. Moreover, the construction avoids the domain-wall problem, ensures that no stable fractionally charged relic survives SU (N)L+R confinement, and remains free of Landau poles below the scale of PQ-breaking operators. The exotic quarks required to generate the PQ anomaly hadronize into unstable mesons and cosmologically stable neutral baryons. However, plausible arguments indicating a strong suppression of baryon formation in SU(N) gauge theories at large N, suggest that their contribution to the dark matter energy density remains subdominant. Combining cosmological constraints with PQ quality and perturbativity requirements yields a viable parameter space in which the axion makes up most of the dark matter and its mass remains predictable.
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