Spectra of radiation for spinless and spin relativistic particles in strong magnetic fields

被引:0
|
作者
Yuan, YF [1 ]
Zhang, JL [1 ]
机构
[1] Univ Sci & Technol China, Ctr Astrophys, Hefei 230026, Peoples R China
关键词
pulsar magnetosphere; synchro-curvature radiation; quantum radiation spectrum;
D O I
暂无
中图分类号
O29 [应用数学];
学科分类号
070104 ;
摘要
Synchro-curvature radiation put forward by Zhang and Cheng is a new and universal radiation mechanism, it describes in derail the radiation properties of a relativistic charged particle moving in a curved magnetic field. This new radiation generalizes ail the classical results of ordinary synchrotron and curvature radiations and reveals inherent linkage and unification between them. Additionly, a general, simple and unitary formula is provided for discussing the radiation problem in research of pulsars. However, the magnitude of the magnetic field of a pulsar is so strong (10(7)-10(9)T) that the quantum effects cannot be neglected. The GFWW method developed recently by Lieu and Axford is applied to generalize the results of Zhang and Cheng. The quantum limited synchro-curvature radiation spectra for spinless K-G particles and spin-1/2 Dirac particles are presented, respectively. Their radiation properties are also discussed.
引用
收藏
页码:99 / 106
页数:8
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