scholarly journals GENERAL PROPERTIES OF THE RADIATION SPECTRA FROM RELATIVISTIC ELECTRONS MOVING IN LANGMUIR TURBULENCE

2014 ◽  
Vol 787 (1) ◽  
pp. 28 ◽  
Author(s):  
Yuto Teraki ◽  
Fumio Takahara
1992 ◽  
Vol 128 ◽  
pp. 207-208
Author(s):  
S. V. Bogovalov ◽  
YU. D. Kotov

AbstractSuper-hard γ-ray radiation spectra have been calculated. This radiation is generated near the velocity-of-light cylinder through the process of inverse-Compton scattering of relativistic electrons by thermal photons radiated by a neutron star. These calculations have been compared with observations of the Crab and Vela pulsars at 1000-GeV γ-ray energies. A correlation between γ-ray flares and those in soft (Ex ≃ lkeV) X-rays are predicted.


2018 ◽  
Vol 33 (07n08) ◽  
pp. 1850035 ◽  
Author(s):  
M. V. Bondarenco

Edge effects in spectra of non-dipole radiation from ultra-relativistic electrons passing through various finite targets are analyzed from a unified point of view. Examples include radiation in a finite magnet, bremsstrahlung at double scattering, and bremsstrahlung in an amorphous plate. A generalization of the encountered spectral decomposition property is proposed. The relevance of phenomena of jet–inter-jet radiation interference and electron time delay in the target is emphasized. Features produced by them in the radiation spectra are discussed.


1982 ◽  
Vol 62 (3-4) ◽  
pp. 167-171 ◽  
Author(s):  
V. B. Ganenko ◽  
I. I. Miroshnichenko ◽  
E. V. Pegushin ◽  
V. M. Sanin ◽  
S. V. Shalatskij

2005 ◽  
Vol 166 (3) ◽  
pp. 171-190 ◽  
Author(s):  
Guido R. Mocken ◽  
Christoph H. Keitel

1986 ◽  
Vol 91 (3-4) ◽  
pp. 313-315 ◽  
Author(s):  
V. B. Ganenko ◽  
V. I. Noga ◽  
E. V. Pegushin ◽  
V. M. Sanin ◽  
S. V. Shalatskij

2021 ◽  
pp. 19-23
Author(s):  
N.V. Maksyuta ◽  
V.I. Vysotskii ◽  
S.V. Efimenko ◽  
Yu.A. Slinchenko

The paper deals with the calculation of electron interaction potentials with the main charged [110] axes in a lithium hydride crystal at T = 300, 600, and 900 K temperatures. For relativistic electrons with Lorentz factors γ = 50, 75, 100 the energy and corresponding wave functions of transverse levels of channeling motion are found numerically. The radiation spectra of channeling electrons with (and without) accounting an angular dispersion are calculated on the basis of these data.


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