scholarly journals Inverse Compton scattering model for gamma-ray production in MeV blazars

1998 ◽  
Vol 294 (3) ◽  
pp. 439-442 ◽  
Author(s):  
W. Bednarek
Keyword(s):  
Compton Scattering ◽  
Gamma Ray ◽  
Scattering Model ◽  
Inverse Compton Scattering ◽  
Inverse Compton

scholarly journals Quiescent Magnetar Emission: Resonant Compton Upscattering

2004 ◽  
Vol 218 ◽  
pp. 267-270
Author(s):  
Matthew G. Baring
Keyword(s):  
Compton Scattering ◽  
Gamma Ray ◽  
Stellar Surface ◽  
X Rays ◽  
Polar Cap ◽  
Inverse Compton Scattering ◽  
Strong Fields ◽  
Inverse Compton ◽  
Gamma Ray Emission

A principal candidate for quiescent non-thermal gamma-ray emission from magnetars is resonant inverse Compton scattering in the strong fields of their magnetospheres. This paper outlines expectations for such emission, formed from non-thermal electrons accelerated in a pulsar-like polar cap potential upscattering thermal X-rays from the hot stellar surface. The resultant spectra are found to be strikingly flat, with fluxes and strong pulsation that could be detectable by GLAST.

scholarly journals A Simulation of Radius-frequency Mapping for PSR J1848-0123 with an Inverse Compton Scattering Model

2021 ◽  
Vol 916 (2) ◽  
pp. 62
Author(s):  
L. H. Shang ◽  
X. Xu ◽  
S. J. Dang ◽  
Q. J. Zhi ◽  
J. T. Bai ◽  
...  
Keyword(s):  
Compton Scattering ◽  
Scattering Model ◽  
Inverse Compton Scattering ◽  
Inverse Compton

scholarly journals A Joint Model for Radio and γ-ray Emission from Pulsars

2003 ◽  
Vol 214 ◽  
pp. 167-170 ◽  
Author(s):  
G. J. Qiao ◽  
K. J. Lee ◽  
H. G. Wang ◽  
R. X. Xu
Keyword(s):  
Electromagnetic Wave ◽  
Compton Scattering ◽  
Gamma Ray ◽  
Joint Model ◽  
Acceleration Process ◽  
Inverse Compton Scattering ◽  
Band Emission ◽  
Null Surface ◽  
Inverse Compton ◽  
Γ Ray

Although pulsars can radiate electromagnetic wave from radio to gamma ray bands, we still have no a united model to understand the multi-band emission. In this paper the effort for a joint model is presented. The inverse Compton scattering (ICS) and a second acceleration process near the null surface are involved to account for the radio and the gama-ray emission, respectively. Various kind of pulse profiles and other observational properties can be reproduced.

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