Abstract
We study the radio signals generated when an axion star enters the magnetosphere of a neutron star. As the axion star moves through the resonant region where the plasma-induced photon mass becomes equal to the axion mass, the axions can efficiently convert into photons, giving rise to an intense, transient radio signal. We show that a dense axion star with a mass ∼10-13 M composed of ∼10 μeV axions can account for most of the mysterious fast radio bursts.
Original language | English |
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Article number | 043015 |
Journal | Physical Review D |
Volume | 103 |
Issue number | 4 |
DOIs | |
State | Published - Feb 24 2021 |