Particle acceleration at pulsar magnetic poles

Details Particle acceleration at pulsar magnetic poles Particle acceleration at pulsar magnetic poles

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975mnras.171..619h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 171, June 1975, p. 619-635.

Other

21

Electric Fields, Neutron Stars, Particle Acceleration, Pulsars, Stellar Magnetic Fields, Astronomical Models, Current Density, High Energy Electrons, Stellar Rotation, Stellar Winds

Scientific paper

Attempts have been made to explain the pulsar phenomenon in terms of a model in which electrons and ions are accelerated by large electric fields near the magnetic poles of rotating neutron stars. The following considerations indicate that these mechanisms are not possible in the axisymmetric situations for which they were invoked, and are unlikely to exist in other situations.

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