Evolution of the Pulsar Magnetosphere

  title={Evolution of the Pulsar Magnetosphere},
  author={V. G. Endean},
BEFORE the discovery of pulsars, Hoyle, Narlikar and Wheeler1 reasoned that the magnetic neutron star would have a very tenuous atmosphere. In 1969, Goldreich and Julian2 reached a different conclusion. They argued that the electromagnetic forces near the surface of a rotating magnetic neutron star are so large by comparison with the gravitational forces that charged particles must be pulled out of the star at a sufficient rate for a dense magnetosphere to be generated. 
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