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Angular distribution for the electron recoil in pair production by linearly polarized γ- rays on electrons

机译:电子上线性极化的γ射线成对产生的电子反冲的角分布

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In this work we study the angular distribution of electron recoil in pair production by linearly polarized gamma rays in the electron electric field. We also present a new algorithm for the simulation of this cross-section for the polar and azimuthal angle distributions for the recoil electron obtained from the cross section calculated using the Borsellino diagrams in the high energy limit ([1] E.A. Vinokurov, E.A. Kurae, Sov. Phys. JETP 36 (1973) 602). Although this process has a lower probability than the pair production in the nucleus field (~ 1/Z), it is nevertheless interesting since the azimuthal distribution of the recoil electron is highly sensitive to the polarization of the incoming gamma radiation. This process is also interesting for the fact that in the range of Born approximation, the distribution of the polar and azimuthal angles of the electron recoil momentum does not depend explicitly on photon energy. This is important in astrophysics since the astrophysical sources are in general non-monochromatic. We insert the algorithm into the Geant4 toolkit and made simple simulation to test the method.
机译:在这项工作中,我们研究了电子电场中线性极化伽马射线在成对生产中电子反冲的角分布。我们还提出了一种新算法,用于模拟该截面的反冲电子的极性和方位角分布,该反冲电子是根据在高能量极限下使用Borsellino图计算得出的截面得到的([1] EA Vinokurov,EA Kurae, Sov.Phys.JETP 36(1973)602)。尽管此过程的概率比在原子核场中产生原子对的概率低(约1 / Z),但由于反冲电子的方位角分布对入射的伽马射线的偏振高度敏感,因此这很有趣。这个过程也很有趣,因为在Born近似范围内,电子反冲动量的极角和方位角的分布并不明显取决于光子能量。这在天体物理学中很重要,因为天文学的来源通常是非单色的。我们将算法插入Geant4工具包中,并进行了简单的仿真以测试该方法。

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