Radiative Opacities and Compton Scattering in Strong Magnetic Fields

1970 ◽  
Vol 160 ◽  
pp. L153 ◽  
Author(s):  
V. Canuto
Keyword(s):  
Magnetic Fields ◽  
Compton Scattering ◽  
Strong Magnetic Fields

Compton scattering in strong magnetic fields

1986 ◽  
Vol 309 ◽  
pp. 362 ◽  
Author(s):  
Joseph K. Daugherty ◽  
Alice K. Harding
Keyword(s):  
Magnetic Fields ◽  
Compton Scattering ◽  
Strong Magnetic Fields

scholarly journals Compton scattering in strong magnetic fields: Spin-dependent influences at the cyclotron resonance

2014 ◽  
Vol 90 (4) ◽  
Author(s):  
Peter L. Gonthier ◽  
Matthew G. Baring ◽  
Matthew T. Eiles ◽  
Zorawar Wadiasingh ◽  
Caitlin A. Taylor ◽  
...  
Keyword(s):  
Magnetic Fields ◽  
Compton Scattering ◽  
Cyclotron Resonance ◽  
Strong Magnetic Fields

One- and two-photon Compton scattering in strong magnetic fields

1986 ◽  
Vol 34 (2) ◽  
pp. 440-451 ◽  
Author(s):  
R. W. Bussard ◽  
S. B. Alexander ◽  
P. Mészáros
Keyword(s):  
Magnetic Fields ◽  
Compton Scattering ◽  
Strong Magnetic Fields ◽  
Two Photon

scholarly journals Inverse Compton Scattering in Strong Magnetic Fields: Applied to the Radiation Mechanism of PSR 0531+21

1987 ◽  
Vol 125 ◽  
pp. 453-453
Author(s):  
H. Chen ◽  
X.J. Wu ◽  
G.J. Qiao
Keyword(s):  
Magnetic Fields ◽  
Power Spectrum ◽  
Compton Scattering ◽  
Cross Section ◽  
Quantum Effect ◽  
Single Electron ◽  
Radiation Mechanism ◽  
Strong Magnetic Fields ◽  
Inverse Compton Scattering ◽  
Inverse Compton

In strong magnetic field near pulsar's surface, the quantum effect for electrons is quite complicated. The classical approximation may lose resonance feature, which gives much smaller cross-section.In this paper, we performed numerical integrations to get the total cross-section and the power spectrum of single electron. Thus considering the resonance, the inverse Compton scattering could be an efficient mechanism in strong magnetic fields. We have carefully calculated the power spectrum of single electron travelling through the isotropic thermal fields.

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