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Infrared acceleration radiation
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We present an exactly soluble electron trajectory that permits an analysis of the soft (deep infrared) radiation emitted, the existence of which has been experimentally observed during beta decay via lowest order inner bremsstrahlung. Our treatment also predicts the time evolution and temperature of the emission, and possibly the spectrum, by analogy with the closely related phenomenon of the dynamic Casimir effect.
Forward citations
Cited by 2 Pith papers
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An advanced undergraduate derivation of acceleration thermality
An exactly solvable non-uniform electron trajectory yields classical radiation whose spectrum is precisely one-dimensional Planck, defining temperature T = ħκ/(2π k_B c).
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TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra
The manuscript is internally inconsistent: the abstract and full text describe different papers, so the stated result cannot be assessed.
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