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A Stringy Effect on Hawking Radiation

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arxiv 2309.12926 v2 pith:QMXWMKDC submitted 2023-09-22 hep-th

Pei-Ming Ho , Yosuke Imamura , Hikaru Kawai , Wei-Hsiang Shao This is my paper · ORCID
classification hep-th
keywords fieldhawkingradiationstringtheoriesapplicationaroundbackground
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In string theories, interactions are exponentially suppressed for trans-Planckian space-like external momenta. We study a class of quantum field theories that exhibit this feature modeled after Witten's bosonic open string field theory, and discover a Lorentz-invariant UV/IR relation that leads to the spacetime uncertainty principle proposed by Yoneya. Application to a dynamical black hole background suggests that Hawking radiation is turned off around the scrambling time.

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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. 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.

  2. The Case For Black Hole Remnants: A Review

    gr-qc 2024-11 unverdicted novelty 2.0 of 10

    A review arguing that black hole remnants remain viable and that the species and entropy objections to them are not decisive, so remnants could resolve the information paradox.

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