Ultra-bright, well-collimated, GeV gamma-ray production in the QED regime

2018 ◽  
Vol 25 (2) ◽  
pp. 023107 ◽  
Author(s):  
Chen Liu ◽  
Baifei Shen ◽  
Xiaomei Zhang ◽  
Liangliang Ji ◽  
Zhigang Bu ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Qed Regime

scholarly journals Generation of gamma-ray beam with orbital angular momentum in the QED regime

2016 ◽  
Vol 23 (9) ◽  
pp. 093120 ◽  
Author(s):  
Chen Liu ◽  
Baifei Shen ◽  
Xiaomei Zhang ◽  
Yin Shi ◽  
Liangliang Ji ◽  
...  
Keyword(s):  
Angular Momentum ◽  
Orbital Angular Momentum ◽  
Gamma Ray ◽  
Qed Regime

scholarly journals Brilliant GeV gamma-ray flash from inverse Compton scattering in the QED regime

2018 ◽  
Vol 60 (4) ◽  
pp. 044004 ◽  
Author(s):  
Z Gong ◽  
R H Hu ◽  
H Y Lu ◽  
J Q Yu ◽  
D H Wang ◽  
...  
Keyword(s):  
Compton Scattering ◽  
Gamma Ray ◽  
Inverse Compton Scattering ◽  
Inverse Compton ◽  
Qed Regime

On the possible gamma-ray source in Cygnus

1967 ◽  
Vol 31 ◽  
pp. 469-471
Author(s):  
J. G. Duthie ◽  
M. P. Savedoff ◽  
R. Cobb
Keyword(s):  
Gamma Rays ◽  
Gamma Ray ◽  
Right Ascension

A source of gamma rays has been found at right ascension 20h15m, declination +35°, with an uncertainty of 6° in each coordinate. Its flux is (1·5 ± 0·8) x 10-4photons cm-2sec-1at 100 MeV. Possible identifications are reviewed, but no conclusion is reached. The mechanism producing the radiation is also uncertain.

Solar Flare Energetic Neutral Emission Measurements in the Project Coronas-I

1994 ◽  
Vol 144 ◽  
pp. 635-639
Author(s):  
J. Baláž ◽  
A. V. Dmitriev ◽  
M. A. Kovalevskaya ◽  
K. Kudela ◽  
S. N. Kuznetsov ◽  
...  
Keyword(s):  
Solar Flare ◽  
Energy Range ◽  
Gamma Rays ◽  
Pulse Shape ◽  
Gamma Ray ◽  
Pulse Shape Discrimination ◽  
Shape Discrimination ◽  
Solar Neutron ◽  
Low Altitude

AbstractThe experiment SONG (SOlar Neutron and Gamma rays) for the low altitude satellite CORONAS-I is described. The instrument is capable to provide gamma-ray line and continuum detection in the energy range 0.1 – 100 MeV as well as detection of neutrons with energies above 30 MeV. As a by-product, the electrons in the range 11 – 108 MeV will be measured too. The pulse shape discrimination technique (PSD) is used.

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