Fast radio bursts from axion stars moving through pulsar magnetospheres

被引:49
|
作者
Buckley, James H. [1 ,2 ]
Dev, P. S. Bhupal [1 ,2 ]
Ferrer, Francesc [1 ,2 ]
Huang, Fa Peng [1 ,2 ]
机构
[1] Washington Univ, Dept Phys, St Louis, MO 63130 USA
[2] Washington Univ, McDonnell Ctr Space Sci, St Louis, MO 63130 USA
关键词
INVARIANCE; SEARCH; PHOTON; LIGHT;
D O I
10.1103/PhysRevD.103.043015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 similar to 10(-13) M-circle dot composed of similar to 10 mu eV axions can account for most of the mysterious fast radio bursts.
引用
收藏
页数:6
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