Probing keV mass QCD axions with the SACLA X-ray free electron laser
Charles Heaton, Jack W. D. Halliday, Taito Osaka, Ichiro Inoue, Sifei Zhang, Ahmed Alsulami, Joshua T. Y. Chu, Mila Fitzgerald, Takaki Hatsui, Motoaki Nakatsutsumi, Haruki Nishino, Atsushi O. Tokiyasu, Robert Bingham, Subir Sarkar, Gianluca Gregori

TL;DR
This paper reports an experimental search for QCD axions and axion-like particles using the SACLA X-ray free electron laser, significantly extending bounds on axion-photon coupling across a broad mass range, including the QCD axion region.
Contribution
It introduces a novel light-shining-through-wall experiment utilizing Laue crystals and the Bormann effect to probe axions from keV to tens of eV masses, improving existing bounds.
Findings
Extended bounds on axion-photon coupling by over an order of magnitude.
Achieved sensitivity reaching the QCD axion coupling prediction in the 3460-3480 eV mass range.
Provided the most stringent laboratory constraints for certain axion mass ranges.
Abstract
Axions are hypothetical particles, proposed to account for the invariance of CP symmetry in quantum chromodynamics. While axions and axion-like-particles are well-motivated by string theory and beyond-Standard-Model extensions, they have remained elusive to experimental searches even after significant effort over many decades. Building on a recent development using an X-ray free electron laser to search for cosmologically favoured axions of mass eV, we extend previous bounds on the ALP-photon coupling, , by over an order of magnitude. We exploit the Bormann effect of Laue crystals in a light-shining-through-wall experiment, with broad sensitivity to 22 eV. Moreover for (3460, 3480) eV our sensitivity reaches down to the QCD axion coupling prediction, providing the most stringent laboratory constraints in this mass range.
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Astrophysics and Cosmic Phenomena · Quantum Chromodynamics and Particle Interactions
