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Quantum Gravitational Corrections to Particle Creation by Black Holes

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arxiv 2303.00310 v1 pith:PNWFEVSN submitted 2023-03-01 hep-th

classification hep-th
keywords quantumblackcorrectionsholeemissionexteriorgravitationalhawking
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We calculate quantum gravitational corrections to the amplitude for the emission of a Hawking particle by a black hole. We show explicitly how the amplitudes depend on quantum corrections to the exterior metric (quantum hair). This reveals the mechanism by which information escapes the black hole. The quantum state of the black hole is reflected in the quantum state of the exterior metric, which in turn influences the emission of Hawking quanta.

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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. Spacetime-curvature induced uncertainty principle: linking the large-structure global effects to the local black hole physics

    gr-qc 2024-11 reject novelty 3.0 of 10

    The authors derive a black hole metric with a cosmological-constant-dependent effective mass and use EHT and VLBI data to put extremely weak bounds on a quantum parameter beta.

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