Generation of Narrow Beams of Super High-Energy Gamma Quanta in the Resonant Compton Effect in the Field of a Strong X-ray Wave

被引:3
|
作者
Roshchupkin, Sergei P. [1 ]
Makarov, Sergey B. [1 ]
机构
[1] Peter Great St Petersburg Polytech Univ, Inst Phys & Mech, Polytech Skaya 29, St Petersburg 195251, Russia
关键词
Oleinik resonances; Compton effect; gamma quanta; ultrarelativistic electrons; strong electromagnetic fields; EFFECTS IN-FIELD; RELATIVISTIC ELECTRONS; LASER; SCATTERING; INTENSITY; RADIATION; PHOTON; BREMSSTRAHLUNG; COLLISION; PHYSICS;
D O I
10.3390/photonics11070597
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The article presents a theoretical study of Oleinik resonances in the process of scattering a gamma quantum by an ultrarelativistic electron in the field of a strong electromagnetic wave with intensities up to 1027Wcm-2. The resonant kinematics for three possible resonant reaction channels in a strong external field have been studied in detail. It is shown that under resonant conditions, the scattering channels of the reaction effectively split into two first-order processes according to the fine structure constant, such as the external field-stimulated Compton effect. The annihilation channel of the reaction effectively decays into direct and reverse the external field-stimulated Breit-Wheeler processes. In the absence of interference from the reaction channels, a resonant differential cross-section was obtained in a strong external electromagnetic field. The cases when the energy of the initial electrons significantly exceeds the energy of the initial gamma quanta have been studied. At the same time, all particles (initial and final) fly in a narrow cone away from the direction of wave propagation. The conditions under which the energy of ultrarelativistic initial electrons is converted into the energy of a finite gamma quantum are studied. It is shown that the resonant differential cross-section of such a process significantly (by several orders of magnitude) exceeds the corresponding nonresonant cross-section. This theoretical study predicts a number of new physical effects that may explain the high-energy fluxes of gamma quanta produced near neutron stars and magnetars.
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页数:29
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