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

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 $|\mathrm{e}⟩\to |\mathrm{g}⟩+\gamma +{\gamma }_{}^{\prime }+a$ (or absorption $a+|\mathrm{e}⟩\to |\mathrm{g}⟩+\gamma +{\gamma }_{}^{\prime }$) in an atomic system with superradiance, where $|\mathrm{e}⟩$ and $|\mathrm{g}⟩$ stand for the excited and ground energy levels of atoms, respectively. A similar process via $|\mathrm{e}⟩\to |\mathrm{g}⟩+\gamma +a$ (or $a+|\mathrm{e}⟩\to |\mathrm{g}⟩+\gamma$) 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.

Comments: 8 pages, 4 figures, published in PRD