MG14 - Talk detail

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Abstract

Fast radio bursts (FRBs) are newly discovered radio transient sources. Their high dispersion measures indicate they may be extragalactic. But due to the lack of observational data in other wavelengths, their progenitors still remain unclear. Here we suggest the collisions between neutron stars and asteroids/comets as a promising mechanism for FRBs. During the impact process, a hot plasma fireball will form after the material of the small body penetrates into the neutron star surface. The ionized matter inside the fireball will then expand along the magnetic field lines. Coherent radiation from the thin shell at the top of the fireball will account for the observed FRBs. Our scenario can reasonably explain the main features of FRBs, such as their durations, luminosities, and the event rate. We argue that for a single neutron star, FRBs are not likely to happen repeatedly in a forseeable time span since such impacts are of low probability. We predict that faint remnant X-ray emissions should be associated with FRBs, which may be detected by future rapid follow-up observations of FRBs.

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