Larmor Temperature, Casimir Dynamics, and Planck's Law
arXiv:2211.00946 · doi:10.3390/physics5030050
Abstract
Classical radiation from a single relativistically accelerating electron is investigated where the temperature characterizing the system highlights the dependence on acceleration. In the context of the dynamic Casimir effect with Planck-distributed photons and thermal black hole evaporation, we demonstrate analytic consistency between the ideas of constant acceleration and equilibrium thermal radiation. For ultra-relativistic speeds, we demonstrate a long-lasting constant peel acceleration and constant power emission, which is consistent with the idea of balanced equilibrium of Planck-distributed particle radiation.
arXiv comment10 pages, 5 figures; resubmission after major revision
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