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Astrophysical Haloscopes · Around

2017

Astrophysical Haloscopes

Sigl, Guenter

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We compute the fluxes of radio photons from conversion of axion-like particle dark matter in cosmic magnetic fields.

We find that for axion-like particle masses around $10^{-6}\,$eV and effective coupling constants to photons $g_{a\gamma}\gtrsim10^{-13}\,{\rm GeV}^{-1}$ strongly magnetized nearby stellar winds may give detectable line-like radio photon signals, although predicted fluxes are highly uncertain due to the poorly known structure of the magnetic fields.
Nevertheless, it may be worth while to conduct a dedicated search in the direction of such sources.
When combined with a possible future laboratory detection of axion-like dark matter such observations may in turn provide information on the small scale magnetic field structure in such objects.

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