Inadequacies in the conventional treatment of the radiation field of moving sources
Houshang Ardavan, Arzhang Ardavan, John Singleton, Joseph Fasel and, Andrea Schmidt

TL;DR
This paper reveals fundamental differences between the classical retarded potential and the wave equation solution for electromagnetic fields of moving sources, especially for superluminal patterns, explaining why conventional methods overlook certain radiation decay behaviors.
Contribution
It demonstrates that neglecting boundary terms in the wave equation solution leads to incorrect predictions for superluminal source radiation fields.
Findings
Boundary term in wave equation is larger than source term for superluminal sources.
Radiation from rotating superluminal sources decays as R^{-1/2}, not R^{-1}.
Experimental confirmation of the R^{-1/2} decay prediction.
Abstract
There is a fundamental difference between the classical expression for the retarded electromagnetic potential and the corresponding retarded solution of the wave equation that governs the electromagnetic field. While the boundary contribution to the retarded solution for the {\em potential} can always be rendered equal to zero by means of a gauge transformation that preserves the Lorenz condition, the boundary contribution to the retarded solution of the wave equation governing the {\em field} may be neglected only if it diminishes with distance faster than the contribution of the source density in the far zone. In the case of a source whose distribution pattern both rotates and travels faster than light {\em in vacuo}, as realized in recent experiments, the boundary term in the retarded solution governing the field is by a factor of the order of {\em larger} than the source…
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