Statistical Properties and Cosmological Applications of Fast Radio Bursts

被引:4
作者
Wu, Qin [1 ]
Wang, Fa-Yin [1 ,2 ]
机构
[1] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Peoples R China
[2] Nanjing Univ, Key Lab Modern Astron & Astrophys, Nanjing 210093, Peoples R China
基金
中国国家自然科学基金;
关键词
MAGNETOSPHERIC CURVATURE RADIATION; COSMIC REIONIZATION HISTORY; SELF-ORGANIZED CRITICALITY; INVERSE COMPTON-SCATTERING; WAITING TIME STATISTICS; FRB; 121102; INTERGALACTIC MEDIUM; RAY-BURST; MISSING BARYONS; MAGNETIC-FIELD;
D O I
10.1088/0256-307X/41/11/119801
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Fast radio burst (FRB) is a type of extragalactic radio signal characterized by millisecond duration, extremely high brightness temperature, and large dispersion measure. It remains a mystery in the universe. Advancements in instrumentation have led to the discovery of 816 FRB sources and 7622 bursts from 67 repeating FRBs (https://blinkverse.alkaidos.cn/). This field is undergoing rapid development, rapidly advancing our understanding of the physics of FRBs as new observational data accumulates. The accumulation of data has also promoted exploration of our universe. In this review, we summarize the statistical analysis and cosmological applications using large samples of FRBs, including the energy functions, the waiting time distributions of repeating FRBs, probe of missing baryons and circumgalactic medium in the universe, measurements of cosmological parameters, exploration of the epoch of re-ionization history, and research of the gravitational lensing of FRBs.
引用
收藏
页数:20
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