Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation
arXiv:2402.16137 · doi:10.1140/epjc/s10052-024-12991-4
Abstract
We investigate the radiation from accelerating electrons with asymptotic constant velocity and their analog signatures as evaporating black holes with left-over remnants. We find high-speed electrons, while having a high temperature, correspond to low-temperature analog remnants.
arXiv comment14 pages, 12 figures
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