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Quantum black hole and Hawking radiation at microscopic magnifying
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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
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Causal Space-Time Structure and non-Hausdorff Extension of Schwarzschild Black Hole Interior
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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