Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation
Lin K.-N. Ievlev E. Good M.R.R. Chen P.
June 2024Springer Nature
European Physical Journal C
2024#84Issue 6
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.
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Department of Physics and Center for Theoretical Sciences, National Taiwan University, Taipei, 10617, Taiwan
Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei, 10617, Taiwan
William I. Fine Theoretical Physics Institute, School of Physics and Astronomy, University of Minnesota, Minneapolis, 55455, MN, United States
Physics Department and Energetic Cosmos Laboratory, Nazarbayev University, Astana, 010000, Kazakhstan
Kavli Institute for Particle Astrophysics and Cosmology, SLAC, Stanford University, Stanford, 94305, CA, United States
Department of Physics and Center for Theoretical Sciences
Leung Center for Cosmology and Particle Astrophysics
William I. Fine Theoretical Physics Institute
Physics Department and Energetic Cosmos Laboratory
Kavli Institute for Particle Astrophysics and Cosmology
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