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On the Light Curve and Spectra of X-Rays and Gamma-Rays from the Crab Pulsar |
| ZHANG Li1,2;K. S. Cheng2;ME1 Dong-Cheng1 |
| 1Yunnan Astrophysics Center, Yunnan University, Kunming 650091
2Department of Physics, University of Hong Kong, Pokfulam Road, Hong Kong
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| Cite this article: |
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ZHANG Li, K. S. Cheng, ME Dong-Cheng 2000 Chin. Phys. Lett. 17 544-546 |
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Abstract We use a three-dimensional pulsar magnetosphere model to study the light curve and spectra of x-rays and gamma-rays from the Crab pulsar. In this model, the vertical size of the outer gap is first determined by a self-consistent model in which the outer gap is limited by pair production from collisions of thermal photons produced by polar cap heating of backflow outer gap current and curvature photons emitted by gap accelerated charged particles. The transverse size of the outer gap is determined by local pair production conditions. In principle, there are two topologically disconnected outer gaps present in the magnetosphere of a pulsar, and both incoming and outgoing particle flows are allowed. However, doublepeak light curves with strong bridges are most common, Making use of the three-dimensional structure of the outer gap and its local properties, we compare the results of our model with the light curve and phase-resolved spectra of the Crab pulsar.
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| Keywords:
97.60.Gb
95.85.Nv
95.85.Pw
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Published: 01 July 2000
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