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Radiation Reaction and Renormalization for a Photon-Like Charged Particle

机译:像光子一样的带电粒子的辐射反应和归一化

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A renormalization scheme which relies on energy-momentum and angularmomentum balance equations is applied to the derivation of effective equation of motionfor a massless point-like charge. Unlike the massive case, the rates of radiated energymomentum and angular momentum tend to infinity whenever the source is accelerated. Theexternal electromagnetic fields which do not change the velocity of the particle admit onlyits presence within the interaction area. The effective equation of motion is the equation oneigenvalues and eigenvectors of the electromagnetic tensor. The massless charges move alongbase line determined by the eigenvectors when the effective equation of motion possesses uniformsolutions. It is interesting that the same solution arises in Rylov’s model of magnetosphere ofa rapidly rotating neutron star (pulsar).
机译:依靠能量动量和角动量平衡方程的重归一化方案被应用于无质量点状电荷的运动有效方程的推导。与大规模情况不同,无论何时加速辐射源,辐射能量动量和角动量的速率都趋于无穷大。不会改变粒子速度的外部电磁场仅允许其存在于相互作用区域内。有效的运动方程是电磁张量的方程特征值和特征向量。当有效的运动方程具有统一解时,无质量电荷沿着由特征向量确定的基线移动。有趣的是,在快速旋转的中子星(脉冲星)的雷洛夫磁层模型中也出现了相同的解决方案。

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