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How Wrinkled is the Surface of a Black Hole?

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arxiv gr-qc/9701056 v1 pith:N3NQB3EU submitted 1997-01-26 gr-qc hep-th

classification gr-qchep-th
keywords blackholescalethresholdbelowfluctuationshorizonwrinkled
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We present evidence that, below a certain threshold scale, the horizon of a black hole is strongly wrinkled, with its shape manifesting a self-similar (``fractal'') spectrum of fluctuations on all scales below the threshold. This threshold scale is small compared to the radius of the black hole, but still much larger than the Planck scale. If present, such fluctuations might account for a large part of the horizon entropy.

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Cited by 1 Pith paper

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

  1. Trade-off Relation for Black Hole Entropy Fluctuations

    gr-qc 2026-05 unverdicted novelty 4.0 of 10

    Within stochastic semiclassical gravity, a trade-off exists between the stochastic variance of black hole entropy change and the number of infalling photons encoding which-path information.

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