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Quantum effects across dynamical horizons

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arxiv 2003.11095 v2 pith:4DNJT2XB submitted 2020-03-24 gr-qc hep-th

classification gr-qchep-th
keywords horizonseffecthawkingtrappingdynamicaleffectsfutureinner
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We present a generalization of the Hawking effect for dynamical trapping horizons by calculating the tunneling rate in the Hamilton-Jacobi formalism. It turns out that all horizons classified by Hayward are subjected to thermal quantum effects. While the Hawking effect for future outer and past inner trapping horizons is given as a particle emission, we show that the Hawking effect for future inner and past outer trapping horizons translates to an absorption. The universality of the treatment allows a natural transfer to the static case.

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  1. Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor

    gr-qc 2025-04 conditional novelty 6.0 of 10

    A singularity-free black hole radiates more coldly and more like a perfect black body than Schwarzschild does, and, on one assumption about its parameters, it ends as a zero-temperature remnant instead of evaporating.

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