Constraints on axion-like particles from non-observation of spectral modulations for X-ray point sources

Abstract

We extend previous searches for X-ray spectral modulations induced by ALP-photon conversion to a variety of new sources, all consisting of quasars or AGNs located in or behind galaxy clusters. We consider a total of seven new sources, with data drawn from the Chandra archive. In all cases the spectrum is well fit by an absorbed power-law with no evidence for spectral modulations, allowing constraints to be placed on the ALP-photon coupling parameter ga(γ)(γ). Two sources are particularly good: the Seyfert galaxy 2E3140 in A1795 and the AGN NGC3862 within the cluster A1367, leading to 95% bounds for light ALPs (ma lesssim 10(−)(12) eV) of ga(γ)(γ) lesssim 1.5 × 10(−)(12) GeV(−)(1) and ga(γ)(γ) lesssim 2.4 × 10(−)(12) GeV(−)(1) respectively.