标题： 快速射电暴是由中子星产生的吗？ 显示英文标题

标题： Are Fast Radio Bursts Made By Neutron Stars?

摘要： 流行的重复快速射电暴（或许所有快速射电暴）模型涉及中子星，因为它们具有高旋转或磁静能量密度。这些模型有两种形式：类似于旋转无线电暂现源的巨大但罕见的脉冲，以及类似于软伽马重复源的爆发。这里我汇集了最近得到加强的针对这些模型的证据，包括银河系微FRB的缺失，并将FRB 180916.J0158+65的16天周期性归因于由大质量黑洞吸积盘产生的喷流的进动。 显示英文摘要

摘要： Popular models of repeating Fast Radio Bursts (and perhaps of all Fast Radio Bursts) involve neutron stars because of their high rotational or magnetostatic energy densities. These models take one of two forms: giant but rare pulsar-like pulses like those of Rotating RAdio Transients and outbursts like those of Soft Gamma Repeaters. Here I collate the evidence, recently strengthened, against these models, including the absence of Galactic micro-FRB, and attribute the 16 day periodicity of FRB 180916.J0158+65 to the precession of a jet produced by a massive black hole's accretion disc.