Invisible Axions and Large-Radius Compactifications
Keith R. Dienes, Emilian Dudas, and Tony Gherghetta

TL;DR
This paper explores how placing the QCD axion in large extra dimensions leads to novel effects such as adjustable mass, rapid oscillations causing decoherence, and implications for cosmological energy dissipation, offering new paths to axion invisibility.
Contribution
It introduces the concept of bulk axions in large extra dimensions, revealing effects like mass independence, axion oscillations, and accelerated energy dissipation, which are novel compared to traditional four-dimensional models.
Findings
Axion mass can be independent of Peccei-Quinn scale.
Laboratory axion oscillations cause rapid decoherence.
Kaluza-Klein modes can accelerate cosmological energy dissipation.
Abstract
We study some of the novel effects that arise when the QCD axion is placed in the ``bulk'' of large extra spacetime dimensions. First, we find that the mass of the axion can become independent of the energy scale associated with the breaking of the Peccei-Quinn symmetry. This implies that the mass of the axion can be adjusted independently of its couplings to ordinary matter, thereby providing a new method of rendering the axion invisible. Second, we discuss the new phenomenon of laboratory axion oscillations (analogous to neutrino oscillations), and show that these oscillations cause laboratory axions to ``decohere'' extremely rapidly as a result of Kaluza-Klein mixing. This decoherence may also be a contributing factor to axion invisibility. Third, we discuss the role of Kaluza-Klein axions in axion-mediated processes and decays, and propose several experimental tests of the…
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