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How Many New Worlds Are Inside a Black Hole?

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arxiv hep-th/9511136 v1 pith:2EQHWSO7 submitted 1995-11-19 hep-th gr-qc

classification hep-thgr-qc
keywords blackboundariesholesitteruniversesapplicationcreationcurvature
verification ladder T0 review T1 audit T2 compute T3 formal
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We propose a possible internal structure for a Schwarzschild black hole resulting from the creation of multiple de Sitter universes with lightlike boundaries when the curvature reaches Planckian values. The intersection of the boundaries is studied and a scenario leading to disconnected de Sitter universes is proposed. The application to the information loss problem is then discussed.

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Cited by 3 Pith papers

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

  1. Charged Black Holes in Quasi-Topological Gravity Coupled to Born-Infeld Nonlinear Electrodynamics

    gr-qc 2026-04 unverdicted novelty 6.0 of 10

    Exact charged black hole solutions in quasi-topological gravity with Born-Infeld electrodynamics are constructed, revealing model-dependent interior regularity with some cases singular and others regular but with AdS cores.

  2. Charged Black Holes in Quasi-Topological Gravity Coupled to Born-Infeld Nonlinear Electrodynamics

    gr-qc 2026-04 unverdicted novelty 6.0 of 10

    Derives exact charged black hole solutions in quasi-topological gravity with Born-Infeld electrodynamics, showing model-dependent regularity with some cases having finite-radius singularities and others replacing de S...

  3. Vaidya-Type Solutions of Quasitopological Gravity Interacting with Nonlinear Electrodynamics

    gr-qc 2026-07 conditional novelty 5.0 of 10

    Radiating (Vaidya-type) charged black holes in quasitopological gravity are generated from static ones by promoting mass and charge to functions of time, with the required currents and radiation fluxes constructed explicitly.

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