# Probing Cosmic Axions through Resonant Emission and Absorption in Atomic Systems with Superradiance

## TL;DR

This paper proposes a novel atomic physics method using superradiance to detect cosmic axions, potentially covering significant parameter space of QCD axion models, though background noise remains a challenge.

## Contribution

It introduces a new resonant emission and absorption technique in atomic systems with superradiance for axion detection, expanding experimental approaches in dark matter research.

## Key findings

- Most of the QCD axion parameter space can be probed with this method.
- Parahydrogen molecules and ytterbium atoms are promising candidates for experiments.
- Background noise is a major challenge needing future solutions.

## Abstract

The $\mu$eV-mass axion is one of the most promising candidates for cold dark matter, and remains to be a well-motivated solution to the CP problem of Quantum Chromodynamics (QCD) via the Peccei-Quinn mechanism. In this paper, we propose a novel method to detect the dark-matter axions in our galaxy via the resonant emission $|{\rm e}\rangle \to |{\rm g}\rangle + \gamma + \gamma^{\prime}_{} + a$ (or absorption $a + |{\rm e}\rangle \to |{\rm g}\rangle + \gamma + \gamma^{\prime}_{}$) in an atomic system with superradiance, where $|{\rm e}\rangle$ and $|{\rm g}\rangle$ stand for the excited and ground energy levels of atoms, respectively. A similar process via $|{\rm e}\rangle \to |{\rm g}\rangle + \gamma + a$ (or $a + |{\rm e}\rangle \to |{\rm g}\rangle + \gamma$) is also put forward to probe the axion-electron coupling. For the nominal experimental setup assuming a background-free environment, most of the parameter space for typical QCD axion models can be covered with parahydrogen molecules or ytterbium atoms. However, the background in a realistic experimental setup remains to be a major issue that needs to be solved in future studies. Searching for better atomic or molecular candidates may be required for a bigger signal-to-noise ratio.