Accepted articles

Reviews of topical problems


Cosmological acceleration

 a, b, c,  d, a, e, f
a Novosibirsk State University, ul. Pirogova2, Novosibirsk, 630090, Russian Federation
b National Research Center "Kurchatov Institute", Alikhanov Institute of Theoretical and Experimental Physics, ul. B. Cheremushkinskaya 25, Moscow, 117218, Russian Federation
c Kavli Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwanoha 5-1-5, Kashiwa, 277-8568, Japan
d Russian Federation State Scientific Center A.I. Alikhanov Institute ofTheoretical and Experimental Physics, ul. Bolshaya Cheremushkinskaya 25, Moscow, 117259, Russian Federation
e Dipartimento di Fisica e Scienze della Terra, Università degli Studi di Ferrara Polo Scientifico e Tecnologico — Edificio C, Via Saragat 1, Ferrara, 44122, Italy
f Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Ferrara Polo Scientifico e Tecnologico — Edificio C, Via Saragat 1, Ferrara, 44122, Italy

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

Text is available here.

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
Citation: Blinnikov S I, Dolgov A D "Cosmological acceleration" Phys. Usp., accepted

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

:   ,    « » ,  ; DOI: 10.3367/UFNr.2018.10.038469

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