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

Publications of the Astronomical Society of Australia

George Z. Machabeli¹ 

关键词: pulsars: general;    radiation mechanisms:;    non-thermal;   

DOI  :  10.1071/AS01045

学科分类：天文学(综合)

来源: CSIRO

【 摘 要 】

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.

【 授权许可】

Unknown