A Decade and a Half of Fast Radio Burst Observations

被引:26
|
作者
Caleb, Manisha [1 ]
Keane, Evan [2 ]
机构
[1] Univ Manchester, Dept Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England
[2] Natl Univ Ireland Galway, Ctr Astron, Univ Rd, Galway H91 TK33, Ireland
基金
欧洲研究理事会;
关键词
radio astronomy; fast radio burst; transient radio sources; EVENT RATE COUNTS; GAMMA-RAY BURST; FRB; 121102; MULTIFREQUENCY OBSERVATIONS; MULTIPLE-SCATTERING; DISPERSION MEASURE; HOST GALAXY; EMISSION; UNIVERSE; REDSHIFT;
D O I
10.3390/universe7110453
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Fast radio bursts (FRBs) have a story which has been told and retold many times over the past few years as they have sparked excitement and controversy since their pioneering discovery in 2007. The FRB class encompasses a number of microsecond- to millisecond-duration pulses occurring at Galactic to cosmological distances with energies spanning about 8 orders of magnitude. While most FRBs have been observed as singular events, a small fraction of them have been observed to repeat over various timescales leading to an apparent dichotomy in the population. & SIM;50 unique progenitor theories have been proposed, but no consensus has emerged for their origin(s). However, with the discovery of an FRB-like pulse from the Galactic magnetar SGR J1935+2154, magnetar engine models are the current leading theory. Overall, FRB pulses exhibit unique characteristics allowing us to probe line-of-sight magnetic field strengths, inhomogeneities in the intergalactic/interstellar media, and plasma turbulence through an assortment of extragalactic and cosmological propagation effects. Consequently, they are formidable tools to study the Universe. This review follows the progress of the field between 2007 and 2020 and presents the science highlights of the radio observations.
引用
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页数:34
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