IR-finite thermal acceleration radiation
arXiv:2304.04412 · doi:10.1016/j.aop.2024.169593
Abstract
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.
arXiv comment10 pages, 9 figures
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Cited by in corpus (5)
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- Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation
- Electron-mirror duality and thermality
- Classical Acceleration Temperature (CAT) in a Box
- Through the Looking-Glass, and What AdS Found There: quantum particle production with a Whittaker spectrum