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Quantum black hole and Hawking radiation at microscopic magnifying

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arxiv gr-qc/0506006 v1 pith:K6QO5BFI submitted 2005-06-01 gr-qc astro-phhep-th

classification gr-qcastro-phhep-th
keywords blackholeradiationhawkingquantumabsorptionbehindestablish
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We establish a state of stopping the Hawking radiation by quantum Schwarzschild black hole in the framework of quasi-classical thermal quantization for particles behind the horizon. The mechanism of absorption and radiation by the black hole is presented.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Causal Space-Time Structure and non-Hausdorff Extension of Schwarzschild Black Hole Interior

    gr-qc 2026-07 conditional novelty 5.0 of 10

    Geodesic reflections fix causal cones under the horizon; the RN zero-charge limit yields an infinite band without closed cycles, plus a non-Hausdorff thermal interior extension.

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