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Information Missing Puzzle, Where Is Hawking's Error?

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arxiv 1804.06726 v3 pith:B6HCTROF submitted 2018-04-16 physics.gen-ph hep-th

classification physics.gen-phhep-th
keywords blackholehorizoncentralhawkinginformationmissingpuzzlequestion
verification ladder T0 review T1 audit T2 compute T3 formal
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Matters falling into and consisting of a blackhole can oscillate periodically across instead of accumulate statically on the central point and form singularities there. In quantum language, this oscillation not only resolves central singularities of the blackhole but also blurs its horizon remarkably. This blurring makes the horizon not a zero-thickness geometric surface any more, but an extended physic region whose thickness is comparable with the horizon radius itself. It is our negligence of this fact that leads to the information missing puzzle, and other related question in blackhole physics. Besides the title question and Schwarzschild singularity's resolving, the current work also provides interpretations for the origin of Bekenstein-Hawking entropy and an explicitly unitary formulation of Hawking radiations.

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Cited by 2 Pith papers

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

  1. Complementarity of Gravitation Collapse (II) XOB and the Damping Gravitational Waveform as Evidences

    gr-qc 2025-05 reject novelty 5.0 of 10

    The paper argues that binary black-hole merger waveforms damp only if black holes have extended inner structure that deforms like a banana during merger.

  2. Complementarity of Gravitational Collapse (I) Origin of the Bekenstein-Hawking Entropy

    gr-qc 2025-05 reject novelty 4.0 of 10

    The paper claims black hole entropy arises from counting quantum states of collapsing dust shells, with Schwarzschild and Lemaitre coordinates giving complementary views of the same horizonless interior.

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