From the Cosmological Model to the generation of the Hubble flow

V.N. Lukash, E.V. Mikheeva, V.N. Strokov
Astro Space Centre, Lebedev Physical Institute, Russian Academy of Sciences, ul. Profsoyuznaya 84/32, Moscow, 117997, Russian Federation

This paper reviews various approaches to the question (pioneered by Sakharov) of how the observed Hubble flow forms. By extrapolating the Cosmological Standard Model to the past, the geometrical properties of and conditions in the early Universe are determined. A new cosmogenesis paradigm based on geodesically complete black/white hole geometries with an integrable singularity is discussed.

PACS: 04.70.−s, 95.36.+x, 98.80.−k (all)
DOI: 10.3367/UFNe.0182.201202k.0216
URL: https://ufn.ru/en/articles/2012/2/j/
Web of Science

000304186400009
Scopus

2-s2.0-84862070303
ADS NASA

2012PhyU...55..204L
Citation: Lukash V N, Mikheeva E V, Strokov V N "From the Cosmological Model to the generation of the Hubble flow" Phys. Usp. 55 204–209 (2012)

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Received: 28th, July 2011, accepted: 25th, May 2011

Оригинал: Лукаш В Н, Михеева Е В, Строков В Н «От космологической модели к образованию хаббловского потока» УФН 182 216–221 (2012); DOI: 10.3367/UFNr.0182.201202k.0216

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