Geometries with integrable singularity -- black/white holes and astrogenic universes

V.N. Lukash; V.N. Strokov

Geometries with integrable singularity -- black/white holes and astrogenic universes

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arxiv 1109.2796 v1 pith:C55Z4HCH submitted 2011-09-13 astro-ph.CO gr-qchep-th

V.N. Lukash , V.N. Strokov This is my paper · ORCID

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keywords blackcosmologicalflowsgeometriesholesintegrablesingularityuniverses

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abstract

We briefly review the problem of generating cosmological flows of matter in GR (the genesis of universes), analyze models' shortcomings and their basic assumptions yet to be justified in physical cosmology. We propose a paradigm of cosmogenesis based on the class of spherically symmetric solutions with {\it integrable} singularity $r=0$. They allow for geodesically complete geometries of black/white holes, which may comprise space-time regions with properties of cosmological flows.

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Timelike convergence condition in regular black-hole spacetimes with (anti-)de Sitter core
gr-qc 2025-09 conditional novelty 6.0 of 10

In spherical symmetry the timelike convergence condition reduces to three mass-function inequalities, and the new one forces every smooth de Sitter core regular black hole to violate the TCC near the core.

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