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A Joint model for radio and gamma-ray emission from pulsars

G. J. Qiao·K. J. Lee·H. G. Wang·R. X. Xu
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Abstract

Although pulsars can radiate electromagnetic wave from radio to gamma ray bands, we still have no a united model to understand the multi-band emission. In this paper the effort for a joint model is presented. The inverse Compton scattering (ICS) and a second acceleration process near the null charge surface are involved to account for the radio and the gama-ray emission, respectively. Various kind of pulse profiles and other observational properties can be reproduced.

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G. J. Qiao, K. J. Lee, H. G. Wang, R. X. Xu. 2003-03-11. A Joint model for radio and gamma-ray emission from pulsars. https://arxiv.org/abs/astro-ph/0303231

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