Evolution of the Pulsar Magnetosphere

Details Evolution of the Pulsar Magnetosphere Evolution of the Pulsar Magnetosphere

Jan 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973natur.241..184e&link_type=abstract

Nature, Volume 241, Issue 5386, pp. 184-185 (1973).

Computer Science

5

Scientific paper

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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