Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-26T04:56:49.712Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Published online by Cambridge University Press:  04 August 2017

H. Chen ,
X.J. Wu  and
G.J. Qiao
H. Chen
Affiliation:
Division of Astrophysics, Geophysics Department, Peking University, Peking, China
X.J. Wu
Affiliation:
Division of Astrophysics, Geophysics Department, Peking University, Peking, China
G.J. Qiao
Affiliation:
Division of Astrophysics, Geophysics Department, Peking University, Peking, China

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
V. Neutron Star Physics
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 453
Copyright
Copyright © Reidel 1987