Opening up a window on the postinflationary QCD axion

Abstract

The QCD axion cosmology depends crucially on whether the QCD axion is present during inflation or not. We point out that contrary to the standard criterion, the Peccei-Quinn (PQ) symmetry could remain unbroken during inflation, even when the axion decay constant, $f_a$, is (much) above the inflationary Hubble scale, $H_I$. This is achieved through the heavy-lifting of the PQ scalar field due to its leading non-renormalizable interaction with the inflaton, encoded in a high-dimensional operator which respects the approximate shift symmetry of the inflaton. The mechanism opens up a new window for the post-inflationary QCD axion and significantly enlarges the parameter space, in which the QCD axion dark matter with $f_a>H_I$ could be compatible with high-scale inflation and free from constraints on axion isocurvature perturbations. There also exist non-derivative couplings, which still keep the inflaton shift symmetry breaking under control, to achieve the heavy-lifting of the PQ field during inflation. Additionally, by introducing an early matter domination era, more parameter space of high $f_a$ could yield the observed DM abundance.

v1: 9 pages, 1 figure; v2: PRL version, 10 pages, 1 figure, references added, discussions expanded, main conclusions unchanged

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Cited by in corpus (6)

• The Interplay between the Dark Matter Axion and Primordial Black Holes
• Diraxiogenesis
• The Quality/Cosmology Tension for a Post-Inflation QCD Axion
• New mechanism for primordial black hole formation from the QCD axion
• Revisiting Isocurvature Bounds on the Minimal QCD Axion
• Minimal solution to the axion isocurvature problem from a nonminimal coupling