# Window for preferred axion models

**Authors:** Luca Di Luzio, Federico Mescia, Enrico Nardi

arXiv: 1705.05370 · 2017-10-11

## TL;DR

This paper defines precise phenomenological criteria for the axion window, focusing on hadronic axion models, to better constrain the axion-photon coupling and identify realistic models within this parameter space.

## Contribution

It introduces a systematic classification of hadronic axion models based on phenomenological constraints and explores bounds on axion-photon coupling across different scenarios.

## Key findings

- Identified upper and lower bounds on axion-photon coupling as a function of axion mass.
- Showed that pre-inflationary scenarios restrict axion-photon coupling to within 20% of the hadronic window.
- Demonstrated that realistic DFSZ models are encompassed within the hadronic axion window.

## Abstract

We discuss phenomenological criteria for defining "axion windows", namely regions in the parameter space of the axion-photon coupling where realistic models live. Currently, the boundaries of this region depend on somewhat arbitrary criteria, and it would be highly desirable to specify them in terms of precise phenomenological requirements. We first focus on hadronic axion models within post-inflationary scenarios, in which the initial abundance of the new vectorlike quarks $Q$ is thermal. We classify their representations $R_Q$ by requiring that $i)$ the $Q$ are sufficiently short lived to avoid issues with long-lived strongly interacting relics, $ii)$ the theory remains weakly coupled up to the Planck scale. The more general case of multiple $R_Q$ is also studied, and the absolute upper and lower bounds on the axion-photon coupling as a function of the axion mass is identified. Pre-inflationary scenarios in which the axion decay constant remains bounded as $f_a\leq 5\cdot 10^{11}\,$GeV allow for axion-photon couplings only about 20% larger. Realistic Dine-Fischler-Srednicki-Zhitnitsky type of axion models also remain encompassed within the hadronic axion window. Some mechanisms that can allow to enhance the axion-photon coupling to values sizeably above the preferred window are discussed.

## Full text

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## Figures

3 figures with captions in the complete paper: https://tomesphere.com/paper/1705.05370/full.md

## References

102 references — full list in the complete paper: https://tomesphere.com/paper/1705.05370/full.md

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Source: https://tomesphere.com/paper/1705.05370