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Radiation reaction and renormalization for a photon-like charged particle

机译:辐射反应和光子样带电的重整化   粒子

摘要

A renormalization scheme which relies on energy-momentum and angular momentumbalance equations is applied to the derivation of effective equation of motionfor a massless point-like charge. Unlike the massive case, the rates ofradiated energy-momentum and angular momentum tend to infinity whenever thesource is accelerated. The external electromagnetic fields which do not changethe velocity of the particle admit only its presence within the interactionarea. The effective equation of motion is the equation on eigenvalues andeigenvectors of the electromagnetic tensor. The massless charges move alongbase line determined by the eigenvectors when the effective equation of motionpossesses uniform solutions. It is interesting that the same solution arises inRylov's model of magnetosphere of a rapidly rotating neutron star (pulsar).
机译:依靠能量动量和角动量平衡方程的重整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中。运动的有效方程是关于电磁张量的特征值和特征向量的方程。当有效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。

著录项

  • 作者

    Yaremko, Yurij;

  • 作者单位
  • 年度 2009
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  • 原文格式 PDF
  • 正文语种 {"code":"en","name":"English","id":9}
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