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| Report/Contribution to a conference proceedings/Contribution to a book | PUBDB-2018-01742 |
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2018
Verlag Deutsches Elektronen-Synchrotron
Hamburg
ISBN: 978-3-945931-17-2
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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2017-02/kelley_katharine
Report No.: DESY-PROC-2017-02
Abstract: We investigate the use of next generation radio telescopes such as the Square Kilometre Array (SKA) to detect axion two-photon coupling in the astrophysical environment. The uncertainty surrounding astrophysical magnetic fields presents new challenges, but with a frequency range corresponding to axions of mass $1.7-57\mu$eV and a spectral profile with a number of distinguishing features, SKA-mid offers a tantalising opportunity to constrain axion dark matter properties. To determine the sensitivity of SKA-mid to an axion signal, we consider observations of the Galactic centre and interstellar medium, and find that this new telescope could allow us to probe axion couplings $\gtrsim10^{-16}$GeV$^{-1}$.
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Book/Proceedings/Report
13th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2017
13th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2017, ThessalonikiThessaloniki, Greece, 15 May 2017 - 19 May 2017
Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC (2018) [10.3204/DESY-PROC-2017-02]
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