The periodic origin of fast radio bursts

Abstract

Fast radio bursts (FRBs) are pulsed radio signals with a duration of milliseconds and a large dispersion measure (DM). Recent observations indicate that FRB 180916 and FRB 121102 show periodic activities. Some theoretical models have been proposed to explain periodic FRBs, and here we test these using corresponding X-ray and $\gamma$-ray observations. We find that the orbital periodic model, the free precession model, the radiation-driven precession model, the fall-back disk precession model where eccentricity is due to the internal magnetic field, and the rotation periodic model are not consistent with observations. The geodetic precession model is the most likely periodic model for FRB 180916. We also propose methods to test the periodic models with yet-to-be-obtained observational data in the future.

arXiv comment8 pages, 6 figures, typos corrected, published in A&A, https://doi.org/10.1051/0004-6361/202142321

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• Rotation Measure Variations and Reversals of Repeating Fast Radio Bursts in Massive Binary Systems
• High frequency study of FRB 20180916B using the 100-m Effelsberg radio telescope
• Memory in the Burst Occurrence of Repeating FRBs
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• Neutron star phase transition as the origin for the fast radio bursts and soft gamma-ray repeaters of SGR J1935+2154
• A comprehensive search for Long and Short Periodic Features from an Extremely Active Cycle of FRB 20240114A
• Periodic Activities of Fast Radio Burst Repeaters from Precessing Magnetars with Evolving Obliquity
• Symmetry Breaking in Repeating Fast Radio Bursts
• AT2020hur: A Possible Optical Counterpart of FRB 180916B