Exploring ALPs beyond the canonical

TL;DR

This paper explores non-standard kinetic terms for axion-like particles, revealing expanded parameter spaces for dark matter and providing updated cosmological constraints, including isocurvature fluctuation limits.

Contribution

It introduces models with singular kinetic terms for ALPs, extending the viable parameter space beyond the canonical pseudo-Nambu-Goldstone boson framework.

Findings

Increased parameter space for ALPs as dark matter candidates.

Derived a general formula for isocurvature fluctuations in anharmonic potentials.

Updated QCD axion dark matter constraints using recent data.

Abstract

Axion-like particles (ALPs) are interesting dark matter candidates both from the theoretical as well as from the experimental perspective. Usually they are motivated as pseudo-Nambu-Goldstone bosons. In this case one of their most important features is that their coupling to other particles is suppressed by a large scale, the vacuum expectation value of the field breaking the symmetry that gives rise to them. This naturally endows them with very weak interactions but also restricts the maximal field value and therefore the regions where sufficient dark matter is produced. In this paper we investigate deviations from this simplest setup, where the potential and interactions are as expected for a pseudo-Nambu-Goldstone boson, but the kinetic term has singularities. This leads to a significantly increased area in parameter space where such particles can be dark matter and can be probed by current and near future experiments. We discuss cosmological limits and in the course of this give a simple derivation of a formula for isocurvature fluctuations in models with general anharmonic potentials. As an application of this formula we give an update of the isocurvature constraints for QCD axion dark matter models, using the most recent results for the QCD topological susceptibility and the newest Planck data.