The physics of fast radio bursts

被引：127

作者：

Xiao, Di ^{[1
,2
]}

Wang, FaYin ^{[1
,2
]}

Dai, ZiGao ^{[1
,2
]}

机构：

[1] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China

[2] Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210023, Peoples R China

来源：

SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY | 2021年 / 64卷 / 04期

基金：

中国国家自然科学基金;

关键词：

fast radio burst; neutron star; cosmology; COHERENT CURVATURE RADIATION; SYNCHROTRON MASER EMISSION; EINSTEINS EQUIVALENCE PRINCIPLE; MAGNETOSONIC SHOCK-WAVES; COMPACT DARK-MATTER; EVENT RATE COUNTS; GAMMA-RAY BURSTS; FRB; 121102; DISPERSION MEASURES; FLARING MAGNETAR;

D O I：

10.1007/s11433-020-1661-7

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

In 2007, a very bright radio pulse was identified in the archival data of the Parkes Telescope in Australia, marking the beginning of a new research branch in astrophysics. In 2013, this kind of millisecond bursts with extremely high brightness temperature takes a unified name, fast radio burst (FRB). Over the first few years, FRBs seemed very mysterious because the sample of known events was limited. With the improvement of instruments over the last five years, hundreds of new FRBs have been discovered. The field is now undergoing a revolution and understanding of FRB has rapidly increased as new observational data increasingly accumulate. In this review, we will summarize the basic physics of FRBs and discuss the current research progress in this area. We have tried to cover a wide range of FRB topics, including the observational property, propagation effect, population study, radiation mechanism, source model, and application in cosmology. A framework based on the latest observational facts is now under construction. In the near future, this exciting field is expected to make significant breakthroughs.

引用

页数：32

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