IR-finite thermal acceleration radiation
Ievlev E. Good M.R.R. Linder E.V.
February 2024Academic Press Inc.
Annals of Physics
2024#461
A charge accelerating in a straight line following the Schwarzschild–Planck moving mirror motion emits thermal radiation for a finite period. Such a mirror motion demonstrates quantum purity and serves as a direct analogy of a black hole with unitary evolution and complete evaporation. Extending the analog to classical electron motion, we derive the emission spectrum, power radiated, and finite total energy and particle count, with particular attention to the thermal radiation limit. This potentially opens the possibility of a laboratory analog of black hole evaporation.
Acceleration radiation , Beta decay , Black hole evaporation , Moving mirror
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Physics Department, Nazarbayev University, Astana, 010000, Kazakhstan
Energetic Cosmos Laboratory, Nazarbayev University, Astana, 010000, Kazakhstan
Theoretical and Nuclear Physics Department, al-Farabi Qazaq National University, Almaty, 050040, Kazakhstan
Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei, 10617, Taiwan
Berkeley Center for Cosmological Physics, United States
Berkeley Lab, University of California, Berkeley, 94720, CA, United States
Physics Department
Energetic Cosmos Laboratory
Theoretical and Nuclear Physics Department
Leung Center for Cosmology and Particle Astrophysics
Berkeley Center for Cosmological Physics
Berkeley Lab
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