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The physical mechanisms of fast radio bursts

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  • Bing Zhang

    (University of Nevada, Las Vegas)

Abstract

Fast radio bursts are mysterious millisecond-duration transients prevalent in the radio sky. Rapid accumulation of data in recent years has facilitated an understanding of the underlying physical mechanisms of these events. Knowledge gained from the neighbouring fields of gamma-ray bursts and radio pulsars has also offered insights. Here I review developments in this fast-moving field. Two generic categories of radiation model invoking either magnetospheres of compact objects (neutron stars or black holes) or relativistic shocks launched from such objects have been much debated. The recent detection of a Galactic fast radio burst in association with a soft gamma-ray repeater suggests that magnetar engines can produce at least some, and probably all, fast radio bursts. Other engines that could produce fast radio bursts are not required, but are also not impossible.

Suggested Citation

  • Bing Zhang, 2020. "The physical mechanisms of fast radio bursts," Nature, Nature, vol. 587(7832), pages 45-53, November.
    • Handle: RePEc:nat:nature:v:587:y:2020:i:7832:d:10.1038_s41586-020-2828-1
    DOI: 10.1038/s41586-020-2828-1
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    Cited by:

    1. Xinyu Ma & Zhaoyu Cai & Chijie Zhuang & Xiangdong Liu & Zhecheng Zhang & Kewei Liu & Bo Cao & Jinliang He & Changxi Yang & Chengying Bao & Rong Zeng, 2024. "Integrated microcavity electric field sensors using Pound-Drever-Hall detection," Nature Communications, Nature, vol. 15(1), pages 1-8, December.
    2. F. Y. Wang & G. Q. Zhang & Z. G. Dai & K. S. Cheng, 2022. "Repeating fast radio burst 20201124A originates from a magnetar/Be star binary," Nature Communications, Nature, vol. 13(1), pages 1-9, December.

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