Cosmological acceleration

S.I. Blinnikov^{a, b, c, d}, A.D. Dolgov^a, b
^aNational Research Center "Kurchatov Institute", Alikhanov Institute of Theoretical and Experimental Physics, ul. B. Cheremushkinskaya 25, Moscow, 117218, Russian Federation
^bNovosibirsk State University, ul. Pirogova 2, Novosibirsk, 630090, Russian Federation
^cKavli Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwanoha 5-1-5, Kashiwa, 277-8568, Japan
^dDukhov Research Institute of Automatics, ul. Sushchevskaya 22, Moscow, 119017, Russian Federation

An overview is given of the current status of the theory and observations of the acceleration of expansion the observable part of the universe.

Keywords: accelerating expansion of universe, dark energy
PACS: 04.50.−h, 12.10.Kt, 95.36.+x, 98.80.−k (all)
DOI: 10.3367/UFNe.2018.10.038469
URL: https://ufn.ru/en/articles/2019/6/a/
Web of Science

000484015200001
Scopus

2-s2.0-85072920695
ADS NASA

2019PhyU...62..529B
Citation: Blinnikov S I, Dolgov A D "Cosmological acceleration" Phys. Usp. 62 529–567 (2019)

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Received: 21st, March 2018, revised: 27th, October 2018, accepted: 31st, October 2018

Оригинал: Блинников С И, Долгов А Д «Космологическое ускорение» УФН 189 561–602 (2019); DOI: 10.3367/UFNr.2018.10.038469

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