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- W3100886913 abstract "It was recently found that the soft X-ray excess in the center of the Coma cluster can be fitted by conversion of axion-like-particles (ALPs) of a cosmic axion background (CAB) to photons. We extend this analysis to the outskirts of Coma, including regions up to 5 Mpc from the center of the cluster. We extract the excess soft X-ray flux from ROSAT All-Sky Survey data and compare it to the expected flux from ALP to photon conversion of a CAB. The soft X-ray excess both in the center and the outskirts of Coma can be simultaneously fitted by ALP to photon conversion of a CAB. Given the uncertainties of the cluster magnetic field in the outskirts we constrain the parameter space of the CAB. In particular, an upper limit on the CAB mean energy and a range of allowed ALP-photon couplings are derived." @default.
- W3100886913 created "2020-11-23" @default.
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- W3100886913 date "2015-01-08" @default.
- W3100886913 modified "2023-09-24" @default.
- W3100886913 title "ALP conversion and the soft X-ray excess in the outskirts of the Coma cluster" @default.
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- W3100886913 doi "https://doi.org/10.1088/1475-7516/2015/01/011" @default.
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