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PARTICLE ACCELERATION IN THE “UNFAVORABLE” ZONE OF A PULSAR |
| CHEN Lufan;LIANG Shaorong |
| Department of Physics, Beijing Normal University, Beijing |
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| Cite this article: |
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CHEN Lufan, LIANG Shaorong 1986 Chin. Phys. Lett. 3 137-140 |
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Abstract Many electromagnetic phenomena on the surface of a pulsar can be explained successfully by the Arons-Scharlemann model. Yet several related phenomena have not been accounted for. In this study we provide solutions for several hitherto unsolved problems in this model, such as the mechanism for the return currents, the relationships between modes of changing and nulling of pulsars and the source for the observed cosmic ray positrons with energies greater than IGeV. In addition, we propose an explanation for the distribution of pulsar periods.
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Published: 01 March 1986
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