  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.
