An exceptionally light axion: Strong CP and Dark Matter

TL;DR

This paper proposes a new extremely light axion model based on a $Z_ N$ symmetry, which can solve the strong CP problem and account for dark matter, with distinctive phenomenology and enhanced experimental prospects.

Contribution

It introduces a novel $Z_ N$ symmetry framework that produces an ultra-light axion, including the first fuzzy dark matter QCD axion, and explores its unique misalignment mechanisms and experimental implications.

Findings

A new ultra-light axion model consistent with dark matter

Enhanced axion interactions improve detection prospects

Potential for discovery in upcoming ALP experiments

Abstract

We explore whether the axion which solves the strong CP problem can naturally be much lighter than the canonical QCD axion. The $Z_\mathcal{N}$ symmetry proposed by Hook, with $\mathcal{N}$ mirror and degenerate worlds coexisting in Nature and linked by the axion field, is considered and the associated phenomenology is studied in detail. On a second step, we show that dark matter can be accounted for by this extremely light axion. This includes the first proposal of a "fuzzy dark matter" QCD axion. A novel misalignment mechanism occurs -- trapped misalignment -- due to the peculiar temperature dependence of the $Z_\mathcal{N}$ axion potential, which in some cases can also dynamically source the recently proposed kinetic misalignment mechanism. The resulting universal enhancement of all axion interactions relative to those of the canonical QCD axion has a strong impact on the prospects of ALP experiments such as ALPS II, IAXO and many others. For instance, even Phase I of Casper Electric could discover this axion.