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The final burst of the moving mirror is unrelated to the partner mode of analog Hawking radiation
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Flying mirrors with appropriate trajectories have been recognized as an analog system that mimics black hole Hawking evaporation and have been widely investigated. It has recently been suggested that the partner mode of the analog Hawking radiation emitted from a moving mirror would manifest itself through a final burst when the mirror executes a sudden stop. Here we argue the opposite via the partner formula for the moving mirror model. By expanding the theoretical foundation of the partner formula and augmenting it with numerical analysis, we demonstrate that the supposed final burst is induced by a shock that requires the input of external energy, whereas the Hawking radiation partner mode, which is associated with the zero-point vacuum fluctuations, is not responsible for the burst.
Forward citations
Cited by 2 Pith papers
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Energy Flux as an Entanglement Current in Moving-Mirror Radiation
In moving-mirror analog Hawking radiation, negative energy flux is correlated with entanglement growth between local detector modes and is interpreted as an information-return channel tied to partner-mode recovery.
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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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