From the cosmological model to generation of the Hubble flow
classification
🌌 astro-ph.CO
hep-ph
keywords
cosmologicalflowhubblemodelapproachesblackcompleteconditions
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We review different approaches to the problem of generating the observed Hubble flow, whose discussion was pioneered by A.D. Sakharov. Extrapolating the Cosmological Standard Model to the past makes it possible to determine physical properties of and conditions in the early universe. We discuss a new cosmogenesis paradigm based on studying geodesically complete geometries of black/white holes with integrable singularities.
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