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Resonant Production of an Ultrarelativistic Electron–Positron Pair at the Gamma Quantum Scattering by a Field of the X-ray Pulsar

机译:通过X射线脉冲场的伽马量子散射在γ量子散射处的谐振产生

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The process of a resonant production of an ultrarelativistic electron–positron pair in the process of gamma-quantum scattering in the X-ray field of a pulsar is theoretically studied. This process has two reaction channels. Under resonant conditions, an intermediate electron (for a channel A) or a positron (for a channel B) enters the mass shell. As a result, the initial second-order process of the fine-structure constant in the X-ray field effectively splits into two first-order processes: the X-ray field-stimulated Breit–Wheeler process and the the X-ray field-stimulated Compton effect on an intermediate electron or a positron. The resonant kinematics of the process is studied in detail. It is shown that for the initial gamma quantum there is a threshold energy, which for the X-ray photon energy (1– 10 2 ) keV has the order of magnitude ( 10 3 –10) MeV. In this case, all the final particles (electron, positron, and final gamma quantum) fly in a narrow cone along the direction of the initial gamma quantum momentum. It is important to note that the energies of the electron–positron pair and the final gamma quantum depend significantly on their outgoing angles. The obtained resonant probability significantly exceeds the non-resonant one. The obtained results can be used to explain the spectrum of positrons near pulsars.
机译:在理论上研究了在脉冲脉冲X射线场中的伽马量子散射过程中谐振产生的谐振产生的过程。该过程具有两个反应通道。在共振条件下,中间电子(对于通道A)或正电子(用于通道B)进入质量壳。结果,X射线场中的微结构常数的初始二阶处理有效地分成两顺序:X射线场刺激的Breit-Wheeler过程和X射线场 - 刺激康普顿对中间电子或正电子的影响。详细研究了该方法的共振运动学。结果表明,对于初始伽马量子,存在阈值能量,其对于X射线光子能量(1-102)KeV具有幅度(10 3 -10)MeV的阶数。在这种情况下,所有最终颗粒(电子,正电子和最终伽马量子)沿初始伽马量子动量的方向沿窄锥片飞行。重要的是要注意,电子 - 正电子对的能量和最终伽马量子显着取决于它们的外向角度。获得的共振概率显着超过了非共振的概率。获得的结果可用于解释脉冲星附近的正弦光谱。

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