Computer simulation of charge recombination in model tracks of high-energy electrons in nonpolar liquids; kinetics and escape

1997 ◽  
Vol 49 (6) ◽  
pp. 675-687 ◽  
Author(s):  
W.M. Bartczak ◽  
A. Hummel
1997 ◽  
Vol 101 (8) ◽  
pp. 1619-1627 ◽  
Author(s):  
Laurens D. A. Siebbeles ◽  
Witold M. Bartczak ◽  
Michel Terrissol ◽  
Andries Hummel

2019 ◽  
Vol 209 ◽  
pp. 01007
Author(s):  
Francesco Nozzoli

Precision measurements by AMS of the fluxes of cosmic ray positrons, electrons, antiprotons, protons as well as their rations reveal several unexpected and intriguing features. The presented measurements extend the energy range of the previous observations with much increased precision. The new results show that the behavior of positron flux at around 300 GeV is consistent with a new source that produce equal amount of high energy electrons and positrons. In addition, in the absolute rigidity range 60–500 GV, the antiproton, proton, and positron fluxes are found to have nearly identical rigidity dependence and the electron flux exhibits different rigidity dependence.


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