Multi-wavelength and Multi-messenger Counterparts of Fast Radio Bursts

Abstract

Fast radio bursts are brief, highly dispersed bursts detected in the radio band, originating from cosmological distances. The only such event detected in the Milky Way galaxy, FRB 20200428DD, was associated with an X-ray burst emitted by a magnetar named SGR J1935+2154, revealing the first case of a multi-wavelength counterpart of an FRB. Counterparts in other wavelengths accompanying or following FRBs, as well as the bright emission associated with the progenitor of the FRB engine, have been proposed in various FRB models, but no robust detection has been made so far. In general, FRBs as we know them are not favorite multi-messenger emitters. Nonetheless, possible neutrino and gravitational wave emission signals associated with FRBs or FRB-like events have been discussed in the literature. Here I review these suggested multi-wavelength and multi-messenger counterparts of FRBs or FRB-like events and the observational progress in searching for these signals. The topics include multi-wavelength (X-rays, $\gamma$-rays, optical) emission and neutrino emission from FRBs within the framework of the magnetar source models and possible FRB-like events associated with gravitational waves.

Invited review published in Annual Review of Nuclear and Particle Science, the author's version

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Cited by in corpus (4)

• A Practical Framework for Estimating the Repetition Likelihood of Fast Radio Bursts from Spectral Morphology
• Fast Radio Bursts from non-resonant Alfvén waves and synchrotron maser emission in the magnetar wind
• Evidence of the association of repeating fast-radio-burst sources with fast-spinning super-twisted magnetars
• Unveiling the spectral morphological division of fast radio bursts with CHIME/FRB Catalog 2