From the cosmological model to generation of the Hubble flow
V. N. Lukash, E. V. Mikheeva, and V. N. Strokov
TL;DR
This paper reviews various methods for explaining the observed Hubble flow, exploring early universe conditions and proposing a new cosmogenesis model based on black/white hole geometries with integrable singularities.
Contribution
It introduces a novel cosmogenesis paradigm using geodesically complete black/white hole geometries with integrable singularities.
Findings
Extrapolation of the Standard Model informs early universe properties
New paradigm links black/white hole geometries to cosmogenesis
Discussion of approaches to generate the Hubble flow
Abstract
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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