IR-finite thermal acceleration radiation

Fuente: arXiv
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Hauptverfasser: Ievlev, Evgenii, Good, Michael R. R., Linder, Eric V.
Format: Preprint
Veröffentlicht: 2023
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author Ievlev, Evgenii
Good, Michael R. R.
Linder, Eric V.
author_facet Ievlev, Evgenii
Good, Michael R. R.
Linder, Eric V.
contents 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.
format Preprint
id arxiv_https___arxiv_org_abs_2304_04412
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle IR-finite thermal acceleration radiation
Ievlev, Evgenii
Good, Michael R. R.
Linder, Eric V.
General Relativity and Quantum Cosmology
Quantum Physics
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.
title IR-finite thermal acceleration radiation
topic General Relativity and Quantum Cosmology
Quantum Physics
url https://arxiv.org/abs/2304.04412