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Statistical Models of Light with an Example in Relativistic Dynamics

机译:光的统计模型,以相对论动力学为例

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The propagation of light is well described by Maxwell’s field equations ofelectromagnetism in relativistic space; its emission and absorption by quantum mechanics.However, some open questions remain. For example, is there a means to break gauge symmetry?Do any surprises await us at high energies or unexplored scales? Are there further interactionsbetween fundamental forces? Many authors have suggested that a deeper understanding canbe achieved through a statistical model of the continuous electromagnetic media in which lightcan propagate. In such an approach the electromagnetic fields are of the same nature as morefamiliar force fields: statistical averages of underlying physical quantities. The goals of thisapproach are not only to explain why Maxwell’s equations of propagation and the quantumtheory of emission and absorption apply, but also to explore new predictions as well. Here webriefly review the approach, and demonstrate its utility in allowing a derivation of the Lorentzboost factors of Special Relativity.
机译:麦克斯韦的相对论空间电磁场方程很好地描述了光的传播。量子力学对其的发射和吸收。然而,仍然存在一些悬而未决的问题。例如,有没有办法打破量规的对称性?在高能量或未经探索的规模下,有什么惊喜在等待着我们吗?基本力之间是否存在进一步的相互作用?许多作者建议,可以通过光可以在其中传播的连续电磁介质的统计模型来加深了解。在这种方法中,电磁场与更熟悉的力场具有相同的性质:基础物理量的统计平均值。该方法的目的不仅是解释为什么麦克斯韦的传播方程以及发射和吸收的量子理论适用,而且还探索新的预测。在这里,webriefly回顾了这种方法,并展示了其在推导狭义相对论的洛伦兹boost因子中的效用。

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