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String Theory and Black Hole Complementarity

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arxiv hep-th/9507094 v1 pith:52VCWZ72 submitted 1995-07-18 hep-th

Joseph Polchinski This is my paper · ORCID
classification hep-th
keywords blackholestringtheoryattemptclarifycomplementarityinformation
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Is string theory relevant to the black hole information problem? This is an attempt to clarify some of the issues involved. Presented at Strings '95.

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Cited by 4 Pith papers

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

  1. The Page curve of Hawking radiation from semiclassical geometry

    hep-th 2019-08 accept novelty 8.0 of 10

    Hawking radiation entropy follows the Page curve when quantum extremal surfaces are identified with RT/HRT surfaces in a higher-dimensional holographic dual, making the black hole interior part of the radiation's enta...

  2. Stringy Black Hole Interiors

    hep-th 2019-08 conditional novelty 7.0 of 10

    The paper argues that the operator F, the fusion of winding string operators W+ and W-, describes folded strings that fill the SL(2,R)/U(1) black hole and radiate at the Hawking temperature.

  3. Macroscopic Black-Hole Remnants in a Nonlocal Field Theory: Towards Hawking Radiation in SFT

    hep-th 2026-06 unverdicted novelty 6.0 of 10

    In a smeared massless scalar on dynamical black hole, outgoing particle number drops to zero after scrambling time due to SFT nonlocality, implying macroscopic remnant.

  4. UV Effects and Short-Lived Hawking Radiation: Alternative Resolution of Information Paradox

    hep-th 2024-11 unverdicted novelty 5.0 of 10

    Hawking radiation terminates around the scrambling time due to trans-Planckian stringy effects in GUP and string-field-theory-inspired toy models, yielding negligible evaporation and a mostly classical black hole.

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