scholarly journals Design Study for Direction Variable Compton Scattering Gamma Ray

2013 ◽  
Vol 425 (19) ◽  
pp. 192020
Author(s):  
T Kii ◽  
M Omer ◽  
H Negm ◽  
Y W Choi ◽  
R Kinjo ◽  
...  
Keyword(s):  
Compton Scattering ◽  
Gamma Ray ◽  
Design Study

IACT Array Performance and Design Study for Multi-TeV Gamma-Ray Astronomy

2008 ◽  
Author(s):  
G. Rowell ◽  
V. Stamatescu ◽  
J. Denman ◽  
G. Thornton ◽  
A. Smith ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Design Study ◽  
Gamma Ray Astronomy ◽  
Array Performance

scholarly journals Design study of a “scintronic” crystal targeting tens of picoseconds time resolution for gamma ray imaging: the ClearMind detector

2020 ◽  
Vol 15 (07) ◽  
pp. P07029-P07029
Author(s):  
D. Yvon ◽  
V. Sharyy ◽  
M. Follin ◽  
J.-P. Bard ◽  
D. Breton ◽  
...  
Keyword(s):  
Time Resolution ◽  
Gamma Ray ◽  
Design Study ◽  
Gamma Ray Imaging

A design study of atmospheric Cerenkov radiation telescope for very high energy gamma-ray astronomy

1985 ◽  
Vol 115 (1) ◽  
pp. 163-183 ◽  
Author(s):  
S. K. Gupta ◽  
P. V. Ramana Murthy ◽  
S. C. Tonwar ◽  
P. R. Vishwanath
Keyword(s):  
Gamma Ray ◽  
High Energy ◽  
Cerenkov Radiation ◽  
Design Study ◽  
Gamma Ray Astronomy ◽  
High Energy Gamma ◽  
Very High Energy ◽  
Energy Gamma ◽  
Very High

Saturated Compton scattering models for the soft gamma-ray repeater bursts

1997 ◽  
Author(s):  
I. A. Smith ◽  
E. P. Liang ◽  
A. Crider ◽  
D. Lin ◽  
M. Kusunose
Keyword(s):  
Compton Scattering ◽  
Gamma Ray

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.

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