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Dumb Holes and the Effects of High Frequencies on Black Hole Evaporation

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arxiv gr-qc/9409008 v2 pith:RCMPK2FD submitted 1994-09-06 gr-qc

classification gr-qc
keywords blackevaporationhighholeprocessdumbfrequenciesfrequency
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The naive calculation of black hole evaporation makes the thermal emission depend on the arbitrary high frequency behaviour of the theory where the theory is certainly wrong. Using the sonic analog to black holes-- dumb holes-- I show numerically that a change in the dispersion relation at high frequencies does not seem to alter the evaporation process, lending weight to the reality of the black hole evaporation process. I also suggest a reason for the insensitivity of the process to high frequency regime.

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Cited by 4 Pith papers

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  3. Simulating Hawking radiation in quantum many-body systems: deviations from the thermal spectrum

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  4. UV Effects and Short-Lived Hawking Radiation: Alternative Resolution of Information Paradox

    hep-th 2024-11 unverdicted novelty 5.0 of 10

    Hawking radiation terminates around the scrambling time due to trans-Planckian stringy effects in GUP and string-field-theory-inspired toy models, yielding negligible evaporation and a mostly classical black hole.

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