磁化中子星的硬Gamma射线产生机制  

Production Mechanism of Hard Gamma Rays from Magnetized Neutron Stars

作　　者：安树元[1] 

机构地区：[1]首都师范大学物理系

出　　处：《首都师范大学学报（自然科学版）》1998年第1期27-30,共4页Journal of Capital Normal University：Natural Science Edition

摘　　要：基于对磁化中子星磁层中极相对论电子辐射机制和辐射输运性质的讨论，指出被观测到的硬γ射线可能来自于磁化中子星的逃逸同步曲率辐射光子．逃逸硬γ射线光子最有可能产生于光速柱面附近的一个区域．ased on the discussions of emission mechanisms of extreme relativistic electrons and propagation properties of radiations in the magnetosphere of magnetized neutron stars, it is indicated that some hard gamma rays detected by energetic gamma ray telescopes would be the escaped synchrotron curvature photons from the magnetized neutron stars and possibly producted in an area nere the surface of light cylinders.

关 键 词：Gamma射线 同步曲率辐射 磁对产生 中子星 非热发射源 

分 类 号：O572.12[理学—粒子物理与原子核物理]