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The Mechanisms for the Generation of Pulsar Radio and High-energy Emission

Published online by Cambridge University Press:  05 March 2013

George Z. Machabeli
George Z. Machabeli*
Affiliation:
Center for Plasma Astrophysics of Abastumani Astrophysical Observatory, Georgian Academy of Sciences, A. Kazbegi Avenue 2a, GE-380060 Tbilisi, Georgia
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Abstract

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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.

Keywords

pulsars: generalradiation mechanisms:non-thermal
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 18 , Issue 4 , 2001 , pp. 394 - 399
Copyright
Copyright © Astronomical Society of Australia 2001

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