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The Mechanisms for the Generation of Pulsar Radio and High-energy Emission
George Z. Machabeli
Journal:

Publications of the Astronomical Society of Australia / Volume 18 / Issue 4 / 2001

Published online by Cambridge University Press:

05 March 2013, pp. 394-399
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The recent theory of propagation and generation of waves in a pulsar’s magnetosphere is discussed. In particular we consider models of pulsar radio emission due to plasma instabilities. Wave–particle interactions can lead to quasilinear diffusion increasing a particle’s pitch-angle. The recent model of γ-ray emission from synchrotron radiation as a result of quasilinear diffusion is discussed.