Classical 5D fields generated by a uniformly accelerated point source
I. Aharonovich, L. P. Horwitz

TL;DR
This paper investigates five-dimensional gauge fields generated by a uniformly accelerated source, comparing them with Maxwell fields, and finds that non-zero modes influence test particle motion.
Contribution
It introduces a numerical method to compute 5D fields from hyperbolic motion and analyzes their differences from classical Maxwell fields.
Findings
Zero mode matches Maxwell fields
Non-zero modes affect test particle dynamics
Numerical Green-function approach developed
Abstract
Gauge fields associated with the manifestly covariant dynamics of particles in spacetime are five-dimensional. In this paper we explore the old problem of fields generated by a source undergoing hyperbolic motion in this framework. The 5D fields are computed numerically using absolute time -retarded Green-functions, and qualitatively compared with Maxwell fields generated by the same motion. We find that although the zero mode of all fields coincides with the corresponding Maxwell problem, the non-zero mode should affect, through the Lorentz force, the observed motion of test particles.
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Taxonomy
TopicsRelativity and Gravitational Theory · Black Holes and Theoretical Physics · Cosmology and Gravitation Theories
