There and Back Again: Quantum Radiation from Round-trip Flying Mirrors

There and Back Again: Quantum Radiation from Round-trip Flying Mirrors

Erasing a black hole leaves spacetime flat, so light passing through the region before any star forms and after black hole's evaporation shows no time delay, just like a flying mirror that returns to its initial starting point. Quantum radiation from a round-trip flying mirror has not been solv...

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Veröffentlicht in:arXiv.org 2024-11
Hauptverfasser: Ahsan Mujtaba, Ievlev, Evgenii, Gorban, Matthew J, Good, Michael R R
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Black holes
Flight
Fourier analysis
Time dependence
Time lag
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Ievlev, Evgenii
Gorban, Matthew J
Good, Michael R R
description Erasing a black hole leaves spacetime flat, so light passing through the region before any star forms and after black hole's evaporation shows no time delay, just like a flying mirror that returns to its initial starting point. Quantum radiation from a round-trip flying mirror has not been solved despite the model's mathematical simplicity and physical clarity. Here, we solve the particle creation from worldlines that asymptotically start and stop at the same spot, resulting in interesting spectra and symmetries, including the time dependence of thermal radiance associated with Bose-Einstein and Fermi-Dirac Bogolubov coefficients. Fourier analysis, intrinsically linked to the Bogolubov mechanism, shows that a thermal Bogolubov distribution does not describe the spin statistics of the quantum field.
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subjects Black holes
Flight
Fourier analysis
Time dependence
Time lag
title There and Back Again: Quantum Radiation from Round-trip Flying Mirrors
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