论文标题
FRB排放机制与观测
FRB emission mechanisms vs. observations
论文作者
论文摘要
目前，广泛认为快速无线电爆发（FRB）是由磁铁中磁能释放驱动的相干发射的来源。但是，确切的排放机制尚不清楚。存在两个主要框架：磁层发射和外部相对论冲击的辐射。在这篇简短的评论中，我描述了两种方法的基础知识，并讨论了如何通过现代观察来探测它们。
Presently, it is broadly assumed that fast radio bursts (FRBs) are sources of coherent emission powered by the magnetic energy release in magnetars. However, the exact emission mechanism is not known, yet. Two main frameworks exist: magnetospheric emission and radiation from external relativistic shocks. In this brief review, I describe basics of both approaches and discuss how they are probed by modern observations.
