https://doi.org/10.1140/epjc/s10052-024-12991-4
Regular Article - Theoretical Physics
Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation
1
Department of Physics and Center for Theoretical Sciences, National Taiwan University, 10617, Taipei, Taiwan
2
Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, 10617, Taipei, Taiwan
3
William I. Fine Theoretical Physics Institute, School of Physics and Astronomy, University of Minnesota, 55455, Minneapolis, MN, USA
4
Physics Department and Energetic Cosmos Laboratory, Nazarbayev University, 010000, Astana, Kazakhstan
5
Kavli Institute for Particle Astrophysics and Cosmology, SLAC, Stanford University, 94305, Stanford, CA, USA
Received:
12
March
2024
Accepted:
5
June
2024
Published online:
25
June
2024
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.
© The Author(s) 2024
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