Elementary processes in strong magnetic fields

被引：0
|
作者：
Ventura, J [1 ]
机构：
[1] Univ Crete, Dept Phys, Iraklion 71003, Crete, Greece
来源：
Electromagnetic Spectrum of Neutron Stars | 2005年 / 210卷
关键词：
stars : neutron; stars : pulsars; stars : magnetic fields;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The magnetic constriction of electronic orbits in strong magnetic fields (SMF) drastically modifies the properties of electronic matter, while SW will even modify the properties of electromagnetic radiation in vacuum through such processes as polarization, pair creation, and photon splitting. We review the bulk properties of matter in SMF with emphasis on radiative opacities and transport in external magnetic fields appropriate for application to pulsars and magnetars. SMF changes in atomic matter and condensed matter at the surface layers of neutron stars are also touched upon.
引用
收藏
页码：63 / 74
页数：12
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