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arXiv 2403.15519hep-phastro-ph.HEhep-th
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在强X射线波场中的共振逆康普顿效应中产生超高等能伽马量子的窄束

Generation of narrow beams of super high-energy gamma quanta in the resonant inverse Compton-effect in the field of a strong x-ray wave

Sergei P. Roshchupkin, Sergey B. Makarov

AI总结:

本文理论研究强电磁波场中超相对论电子散射伽马量子的Oleinik共振,揭示散射道和湮灭道分别分裂为外场受激康普顿效应和Breit-Wheeler过程,并预言可解释中子星和磁星附近高能伽马流的窄束产生机制。

摘要:

本文对强电磁波场中超相对论电子散射伽马量子的过程中Oleinik共振进行了理论研究。研究表明,在共振条件下,该反应的散射道按照精细结构常数有效地分裂为两个一阶过程,例如外场受激康普顿效应;而该反应的湮灭道则有效地衰变为正向和反向的外场受激Breit-Wheeler过程。研究显示了末态粒子共振能量和共振截面与末态伽马量子的出射角、所吸收和发射的波光子数以及问题的特征量子参数之间的显著依赖关系。这些量子参数由初始粒子能量与康普顿效应和Breit-Wheeler过程的特征能量之比决定。得到了末态电子和伽马量子出射角之间的明确关系,这在性质上将共振过程与非共振过程区分开来。研究了初始电子能量显著超过初始伽马量子能量的情形。得到了高能初始电子能量转化为末态伽马量子能量的条件。同时,这种过程的共振微分截面显著(高出数个数量级)超过相应的非共振截面。这项理论研究预言了若干新的物理效应,这些效应可能解释在中子星和磁星附近产生的高能伽马量子流。

英文摘要:

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. It is shown that under resonant conditions, the scattering channels of the reaction effectively split into two first-order processes according to a fine structure constant such as the external field-stimulated Compton effect. And the annihilation channel of the reaction effectively decays into direct and reverse the external field-stimulated Breit-Wheeler processes. The significant dependence of the resonant energy of final particles and resonant cross sections on the outgoing angles of the final gamma quantum, the number of absorbed and emitted photons of the wave, as well as the characteristic quantum parameters of the problem is shown. These quantum parameters are determined by the ratio of the initial particle energies to the characteristic energies of the Compton effect and the Breit-Wheeler process. An unambiguous relationship between the outgoing angles of final electrons and gamma quanta has been obtained, which qualitatively distinguishes the resonant process from the non-resonant one. The cases when the energy of the initial electrons significantly exceeds the energy of the initial gamma quanta have been studied. The conditions under which the energy of high-energy initial electrons is converted into the energy of final gamma quanta are obtained. At the same time, the resonant differential cross-section of such a process significantly (by several orders of magnitude) exceeds the corresponding non-resonant cross-section. This theoretical study predicts a number of new physical effects that may explain the high-energy fluxes of gamma quanta born near neutron stars and magnetars.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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