Fast radio bursts

被引：87
作者：
Katz, J. I. [1 ,2 ]
机构：
[1] Washington Univ, Dept Phys, St Louis, MO 63130 USA
[2] Washington Univ, McDonnell Ctr Space Sci, St Louis, MO 63130 USA
来源：
PROGRESS IN PARTICLE AND NUCLEAR PHYSICS | 2018年 / 103卷
关键词：
Fast radio bursts; Astronomical transients; Coherent emission; MAGNETIZED NEUTRON-STARS; GAMMA-RAY BURSTS; GIANT PULSES; HOST GALAXY; FRB; 121102; EMISSION; MODEL; PULSARS; ENVIRONMENT; MECHANISM;
D O I：
10.1016/j.ppnp.2018.07.001
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
More than a decade after their discovery, astronomical Fast Radio Bursts remain enigmatic. They are known to occur at "cosmological" distances, implying large energy and radiated power, extraordinarily high brightness temperature and coherent emission. Yet their source objects, the means by which energy is released and their radiation processes remain unknown. This review is organized around these unanswered questions. (C) 2018 Elsevier B.V. All rights reserved.
引用
收藏
页码：1 / 18
页数：18
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