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. 2022 Jul;607(7918):256-259.
doi: 10.1038/s41586-022-04841-8. Epub 2022 Jul 13.

Sub-second periodicity in a fast radio burst

CHIME/FRB CollaborationBridget C Andersen  1   2 Kevin Bandura  3   4 Mohit Bhardwaj  1   2 P J Boyle  1   2 Charanjot Brar  1   2 Daniela Breitman  5   6   7 Tomas Cassanelli  6   7 Shami Chatterjee  8 Pragya Chawla  1   2 Jean-François Cliche  1   2 Davor Cubranic  9 Alice P Curtin  1   2 Meiling Deng  10   11 Matt Dobbs  1   2 Fengqiu Adam Dong  9 Emmanuel Fonseca  1   2 B M Gaensler  6   7 Utkarsh Giri  10   12 Deborah C Good  9 Alex S Hill  11   13 Alexander Josephy  1   2 J F Kaczmarek  11 Zarif Kader  1   2 Joseph Kania  4   14 Victoria M Kaspi  1   2 Calvin Leung  15   16 D Z Li  17 Hsiu-Hsien Lin  18   19 Kiyoshi W Masui  15   16 Ryan Mckinven  6   7 Juan Mena-Parra  15 Marcus Merryfield  1   2 B W Meyers  9 D Michilli  20   21   22   23 Arun Naidu  1   2 Laura Newburgh  24 C Ng  6 Anna Ordog  11   13 Chitrang Patel  1   6 Aaron B Pearlman  1   2 Ue-Li Pen  6   10   18   19   25 Emily Petroff  1   2   26 Ziggy Pleunis  1   2   6 Masoud Rafiei-Ravandi  10   12 Mubdi Rahman  27 Scott Ransom  28 Andre Renard  6 Pranav Sanghavi  3   4 Paul Scholz  6 J Richard Shaw  9 Kaitlyn Shin  15   16 Seth R Siegel  1   2 Saurabh Singh  1   2 Kendrick Smith  10 Ingrid Stairs  9 Chia Min Tan  1   2 Shriharsh P Tendulkar  29   30 Keith Vanderlinde  6   7 D V Wiebe  9 Dallas Wulf  1   2 Andrew Zwaniga  1   2
Affiliations

Sub-second periodicity in a fast radio burst

CHIME/FRB Collaboration et al. Nature. 2022 Jul.

Abstract

Fast radio bursts (FRBs) are millisecond-duration flashes of radio waves that are visible at distances of billions of light years1. The nature of their progenitors and their emission mechanism remain open astrophysical questions2. Here we report the detection of the multicomponent FRB 20191221A and the identification of a periodic separation of 216.8(1) ms between its components, with a significance of 6.5σ. The long (roughly 3 s) duration and nine or more components forming the pulse profile make this source an outlier in the FRB population. Such short periodicity provides strong evidence for a neutron-star origin of the event. Moreover, our detection favours emission arising from the neutron-star magnetosphere3,4, as opposed to emission regions located further away from the star, as predicted by some models5.

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