Self-scattering in gamma ray sources used in compton scattering experiments

Author(s):  
A.J. Rollason ◽  
J. Felsteiner ◽  
G.E.W. Bauer ◽  
J.R. Schneider
Keyword(s):  
1997 ◽  
Author(s):  
I. A. Smith ◽  
E. P. Liang ◽  
A. Crider ◽  
D. Lin ◽  
M. Kusunose
Keyword(s):  

2004 ◽  
Vol 218 ◽  
pp. 267-270
Author(s):  
Matthew G. Baring

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.


2016 ◽  
Vol 11 (0) ◽  
pp. 3406066-3406066
Author(s):  
Takehito HAYAKAWA ◽  
Shuji MIYAMOTO ◽  
Takayasu MOCHIZUKI ◽  
Ken HORIKAWA ◽  
Sho AMANO ◽  
...  

2013 ◽  
Vol 425 (19) ◽  
pp. 192020
Author(s):  
T Kii ◽  
M Omer ◽  
H Negm ◽  
Y W Choi ◽  
R Kinjo ◽  
...  

2012 ◽  
Vol 39 (2) ◽  
pp. n/a-n/a ◽  
Author(s):  
Sebastien Celestin ◽  
Victor P. Pasko

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