On propagation of photons in a magnetized medium

被引：1
|
作者：
Cruz Rodriguez, L. [1 ]
Perez Martinez, A. [2 ]
Perez Rojas, H. [2 ]
Rodriguez Querts, E. [2 ,3 ]
机构：
[1] Univ La Habana, Fac Fis, Vedado La Habana 10400, Cuba
[2] Inst Cibernet Matemat & Fis ICIMAF, Havana 10400, Cuba
[3] CINVESTAV, IPN, Dept Fis, Mexico City 07000, DF, Mexico
来源：
ASTRONOMISCHE NACHRICHTEN | 2015年 / 336卷 / 8-9期
关键词：
magnetic fields; radiation transfer; POLARIZATION; ELECTRON; FIELD;
D O I：
10.1002/asna.201512245
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The aim of this work is to solve the dispersion relations near the first excitation threshold of a photon propagating along a magnetic field in the strong field limit. We have calculated the time damping of the photon in two particular cases: the degenerate gas as well as the diluted gas limit, both being important from the astro-physical point of view. In particular, the diluted gas limit could describe the magnetosphere of neutron stars. The solutions have been used to obtain a finite quantum Faraday angle in both limits. A resonant behavior for the Faraday angle is also obtained. To reproduce the semi-classical result for the Faraday rotation angle, the weak field limit is considered. ((c) 2015 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)
引用
收藏
页码：895 / 899
页数：5
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