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arxiv: 1301.5544 · v1 · submitted 2013-01-23 · 🌀 gr-qc · astro-ph.CO· hep-th

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Space-Times with Integrable Singularity

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classification 🌀 gr-qc astro-ph.COhep-th
keywords singularityinflationintegrableuniverseallowsalreadyapproachbefore
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We use the phenomenological approach to study properties of space-time in the vicinity of the Schwarzschild black-hole singularity. Requiring finiteness of the Schwarzschild-like metrics we come to the notion of integrable singularity that is, in a sense, weaker than the conventional singularity and allows the (effective) matter to pass to the white-hole region. This leads to a possibility of generating a new universe there. Thanks to the gravitational field of the singularity, this universe is already born highly inflated ('singularity-induced inflation') before the ordinary inflation starts.

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Cited by 2 Pith papers

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

  1. On gravitational collapse and integrable singularities

    gr-qc 2026-05 unverdicted novelty 5.0

    After Minkowski breaking in the interior geometry, the quantum potential in the Raychaudhuri equation strongly resists further collapse toward the central singularity.

  2. On gravitational collapse and integrable singularities

    gr-qc 2026-05 unverdicted novelty 3.0

    After Minkowski breaking in collapsing matter, the quantum potential in the Raychaudhuri equation strongly opposes collapse to the Schwarzschild singularity.