Fast Radio Bursts: Collisions between Neutron Stars and Asteroids/Comets

TL;DR

This paper proposes that collisions between neutron stars and small celestial bodies like asteroids or comets could generate fast radio bursts (FRBs), explaining their main observed features and predicting faint X-ray emissions.

Contribution

It introduces a novel collision-based model for FRBs, linking impact events to observed radio bursts and associated faint X-ray signals.

Findings

The model explains FRB durations, luminosities, and event rates.

FRBs are unlikely to repeat from a single neutron star due to low impact probability.

Faint X-ray emissions are predicted to accompany FRBs but are difficult to detect.

Abstract

Fast radio bursts (FRBs) are newly discovered radio transient sources. Their high dispersion measures indicate an extragalactic origin. 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, but it may be too faint to be detected by detectors at work.