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Snowmass White Paper: Micro- and Macro-Structure of Black Holes

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arxiv 2203.04981 v1 pith:XXROKTBE submitted 2022-03-09 hep-th

classification hep-th
keywords theoryparadoxresolvestringblackblack-holedegreesdescribe
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The black-hole information paradox provides a stringent test of would-be theories of quantum gravity. String theory has made significant progress toward a resolution of this paradox, and has led to the fuzzball and microstate geometry programs. The central thesis of these programs is that only string theory has sufficiently many degrees of freedom to resolve black-hole microstructure, and that horizons and singularities are artifacts of attempting to describe gravity using a theory that has too few degrees of freedom to resolve the physics. Fuzzballs and microstate geometries recast black holes within string theory as horizonless and singularity-free objects that not only resolve the paradox but provide new insight into the underlying microstructure. We give an overview of this approach, summarize its current status and describe future prospects and insights that are now within reach.

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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. Berry Picking: Random Wave Chaos Hierarchy for BPS Microstate Geometries

    hep-th 2026-07 conditional novelty 6.0 of 10

    Wave chaos in BPS microstate geometries strengthens toward black-hole-like throats while geodesic chaos weakens, and weak-coupling CFT Renyi entropies do not share that bulk hierarchy.

  2. Nonradial stability of topological stars

    gr-qc 2025-02 conditional novelty 6.0 of 10

    Numerical linear perturbation analysis finds no instability in nonradial Type-II modes of topological stars with zero Kaluza-Klein momentum.

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