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Strong Scalar QED in Inhomogeneous Electromagnetic Fields

机译:强校标QED在不均匀的电磁场

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Strong quantum electrodynamics (QED) has attracted attention recently partly because many astrophysical phenomena have been observed to involve electromagnetic fields beyond the critical strength for electron-positron pair production and partly because terrestrial experiments will generate electromagnetic fields above or near the critical strength in the near future. In this talk, we critically review QED phenomena involving strong external electromagnetic fields. Strong QED is characterized by vacuum polarization due to quantum fluctuations and pair production due to the vacuum instability. A canonical method is elaborated for pair production at zero or finite temperature by inhomogeneous electric fields. An algorithm is advanced to calculate the pair-production rate for electric fields acting for finite periods of time, or for electric fields localized in space, or for oscillating electric fields. Finally, strong QED is discussed in astrophysics, in particular, strange stars.
机译:最近的Quantum电动动力学(QED)最近引起了关注,因为已经观察到许多天体物理现象,以涉及超出电子正电子对生产的临界强度的电磁场,部分是因为地面实验将产生上方或附近近乎临界强度的电磁场 未来。 在这次谈话中,我们批判地审查涉及强外部电磁场的QED现象。 由于真空不稳定,强度QED由于量子波动和对生产而具有真空偏振。 通过非均匀电场阐述了一种规范方法,以零或有限温度对生产。 一种算法进行了前进,以计算用于有限时间的电场的一对生产速率,或用于空间中的局部局部的电场,或用于振荡电场。 最后,在天体物理学,特别是奇怪的恒星中讨论了强的QED。

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