Self-Consistent Solution for an Axisymmetric Pulsar Model

Details Self-Consistent Solution for an Axisymmetric Pulsar Model Self-Consistent Solution for an Axisymmetric Pulsar Model

May 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974phrvl..32.1019k&link_type=abstract

Physical Review Letters, vol. 32, Issue 18, pp. 1019-1022

Physics

23

Scientific paper

A spinning neutron star surrounded by a magnetosphere is widely accepted as the basic pulsar model. We have obtained a self-consistent numerical solution for the case when the rotation and magnetic axes are aligned. The field lines close even beyond the light radius RL, and with Crab-pulsar parameters 5 × 1037 erg/sec are carried away by relativistic particles. An equatorial region of high-energy density is found near RL which could be the region of observed radio emission.

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