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• W3048333850 abstract "Axions may be produced in abundance inside stellar cores and then convert into observable X-rays in the Galactic magnetic fields. We focus on the Quintuplet and Westerlund 1 super star clusters, which host large numbers of hot, young stars including Wolf-Rayet stars; these stars produce axions efficiently through the axion-photon coupling. We use Galactic magnetic field models to calculate the expected X-ray flux locally from axions emitted from these clusters. We then combine the axion model predictions with archival Nuclear Spectroscopic Telescope Array (NuSTAR) data from 10 - 80 keV to search for evidence of axions. We find no significant evidence for axions and constrain the axion-photon coupling $g_{agammagamma} lesssim 3.6 times 10^{-12}$ GeV$^{-1}$ for masses $m_a lesssim 5 times 10^{-11}$ eV at 95% confidence." @default.
• W3048333850 created "2020-08-13" @default.
• W3048333850 creator A5007873152 @default.
• W3048333850 creator A5021962612 @default.
• W3048333850 creator A5048786530 @default.
• W3048333850 date "2020-12-22" @default.
• W3048333850 modified "2023-10-17" @default.
• W3048333850 title "X-Ray Searches for Axions from Super Star Clusters" @default.
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• W3048333850 doi "https://doi.org/10.1103/physrevlett.125.261102" @default.
• W3048333850 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/33449711" @default.
• W3048333850 hasPublicationYear "2020" @default.
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