On the electrodynamics of counter stream in pulsar’s inner annular cap region |
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Authors: | K.J. Lee G.J. Qiao H.G. Wang R.X. Xu |
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Affiliation: | 1. Astronomy Department, School of Physics, Peking University, Beijing 100871, China;2. Center for Astrophysics, Guangzhou University, Guangzhou 510400, China |
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Abstract: | The electric properties of pulsar’s inner annular gap are explored in this paper. Under two main assumptions, (1) the pulsar is alive, (2) the total charge of pulsar should not vary with time, the condition for the acceleration of negative particle in the annular region is derived. The acceleration condition is j− ? 0.5j+, i.e., the current carried by negative particles is greater than or equal to 0.5 times of the current carried by positive particles. This condition holds even when the backward flow of positive particles exists in the annular region. It is noted that the outflow of negative particles offers good opportunities to understand the current closure problem of pulsar as well as wide radiation beam of pulsar observed at high energy band. |
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Keywords: | Pulsars: general Radiation mechanisms: non-thermal |
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