The physical mechanisms of fast radio bursts

被引：247
作者：
Zhang, Bing [1 ]
机构：
[1] Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA
来源：
NATURE | 2020年 / 587卷 / 7832期
关键词：
SYNCHROTRON MASER EMISSION; FRB; MODEL; PULSES; NONDETECTION; PULSARS; LIMITS;
D O I：
10.1038/s41586-020-2828-1
中图分类号：
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号：
07 ; 0710 ; 09 ;
摘要：
The mechanisms and origins of fast radio bursts are reviewed in connection with data and insights from the neighbouring fields of gamma-ray bursts and radio pulsars. 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.
引用
收藏
页码：45 / 53
页数：9
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