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Gravity Induced Spontaneous Radiation

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arxiv 2207.05158 v4 pith:WJPJGBL2 submitted 2022-07-02 hep-th

classification hep-th
keywords radiationblackentropygisrgravityholesinducedmechanism
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We suggest that behind the black hole information paradox is a new and universal radiation mechanism, Gravity Induced Spontaneous Radiation, or GISR hereafter. This mechanism happens to all kinds of compositional objects and it requires only their microscopic structure as the basis. It's always accompanied with such inner structures' variation and allows for explicitly hermitian hamiltonian description. For black holes, by Wigner-Wiesskopf approximation we show that such a radiation has a thermal spectrum exactly the same as hawking radiation; while through numeric integration, we show that the variation of the radiation particles' entropy exhibits all features of Page curve as expected. We also provide exact and analytic solutions to the Einstein equation describing microscopic structures required by the GISR of black holes and show that, after quantisation the degeneracy of wave functions corresponding with those solutions are consistent with the area law formula of Bekenstein-Hawking entropy.

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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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