RELATIVISTIC ELECTRON-POSITRON PLASMA QUASI-LINEAR RELAXATION AT THE PRESENCE OF MAGNETIC BREMSSTRAHLUNG

1979 ◽  
Vol 40 (C7) ◽  
pp. C7-713-C7-714 ◽  
Author(s):  
J. G. Lominadze ◽  
G. Z. Machabeli ◽  
A. B. Mikhailovsky
2003 ◽  
Vol 67 (3) ◽  
Author(s):  
D. A. Keston ◽  
E. W. Laing ◽  
D. A. Diver

1999 ◽  
Vol 13 (26) ◽  
pp. 3133-3147 ◽  
Author(s):  
LAUREAN HOMORODEAN

The magnetic susceptibilities of the degenerate and nondegenerate relativistic electron gases, and of the nondegenerate electron–positron gas are presented.


2016 ◽  
Vol 688 ◽  
pp. 012010 ◽  
Author(s):  
Hui Chen ◽  
J. Bonlie ◽  
R. Cauble ◽  
F. Fiuza ◽  
W. Goldstein ◽  
...  

2000 ◽  
Vol 177 ◽  
pp. 371-374
Author(s):  
V.S. Beskin ◽  
R.R. Rafikov

AbstractTwo-fluid effects on the radial 2D outflow of relativistic electron–positron plasma are considered. It is shown that when the longitudinal electric current is smaller than the Goldreich–Julian one, almost all electromagnetic energy is transformed into the energy of particles in the narrow boundary layer near the light surface |E| = |B|.


1986 ◽  
Vol 41 (8) ◽  
pp. 1005-1008
Author(s):  
F. Winterberg

The prerequisite for an efficient electron-positron gamma ray laser, which is the rapid formation o f a dense electron-positron plasma in a time shorter than the time for pair annihilation, is ideally fulfilled in a relativistic electron-positron superpinch. Because the cross section for annihilation decreases quadratically with the center o f mass energy, the time requirements otherwise imposed, are greatly relaxed. A relativistic electron-positron pinch can collapse under a complete population inversion into a very dense state possessing the form o f a long filament, just as it is required for a gamma ray laser. The gamma ray energies are the total center of mass energies, which can be much larger than the electron-positron rest mass energies.


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