8 reveals a notable trend: The spectrum of the radiation emitted by the transluminal grating asymptotically adopts a quasi-thermal distribution, akin to e - ħ ω / k B T H with T H an equivalent Hawking temperature.
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8 reveals a notable trend: The spectrum of the radiation emitted by the transluminal grating asymptotically adopts a quasi-thermal distribution, akin to e - ħ ω / k B T H with T H an equivalent Hawking temperature.