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Repeated Compton scattering in a strong magnetic field

Repeated Compton scattering in a strong magnetic field
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摘要 Repeated scatterings of unpolarized photons by non-relativistic electrons in a static and uniform magnetic field are investigated by using the Boltzmann equation with quantum mechanical correction factors for the stimulated scattering effects.The resulting Kompaneets equation depends explicitly on the electron cyclotron frequency and the incidence angle of the incoming photons relative to the direction of the magnetic field.The evolutionary behavior of the photon spectrum and energy density is highly anisotropic with respect to the static external magnetic field.Possible applications of our results to the X-ray emission from compact and massive stellar objects are discussed in detail and those to the interaction of the microwave background radiation with the hot electrons in galactic clusters are discussed briefly. Repeated scatterings of unpolarized photons by non-relativistic electrons in a static and uniform magnetic field are investigated by using the Boltzmann equation with quantum mechanical correction factors for the stimulated scattering effects. The resulting Kompaneets equation depends explicitly on the electron cyclotron frequency and the incidence angle of the incoming photons relative to the direction of the magnetic field. The evolutionary behavior of the photon spectrum and energy density is highly anisotropic with respect to the static external magnetic field. Possible applications of our results to the X-ray emission from compact and massive stellar objects are discussed in detail and those to the interaction of the microwave background radiation with the hot electrons in galactic clusters are discussed briefly.
出处 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS 2012年第10期1931-1937,共7页 中国科学:物理学、力学、天文学(英文版)
基金 supported by the National Natural Science Foundation of China (Grant Nos. Y011091001,11003023 and 10833003)
关键词 electromagnetic waves: magnetospheric propagation X-ray scattering: interactions with matter neutron stars 匀强磁场 康普顿散射 玻耳兹曼方程 量子力学修正 光子散射 相对论性电子 微波背景辐射 影响因素
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