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In the Quest for Cosmic Rotation

Mathematics Department, Higher Military Institute of Air Defence, Moskovsky prospect 28, 150001 Yaroslavl, Russia
Department of Theoretical Physics, Faculty of Mathematics, Physics and Informatics, Comenius University, Mlynská dolina 6280, 842 48 Bratislava, Slovakia
Nuclear Safety Institute (IBRAE), Russian Academy of Sciences, B. Tulskaya 52, 115191 Moscow, Russia
Author to whom correspondence should be addressed.
Universe 2020, 6(1), 14;
Received: 27 November 2019 / Revised: 7 January 2020 / Accepted: 8 January 2020 / Published: 15 January 2020
(This article belongs to the Special Issue Rotation Effects in Relativity)
This paper analyzes the problem of global rotation in general relativity (GR) theory. Simple cosmological models with rotation and expansion are presented, which give a natural explanation of the modern values of the acceleration parameter at different red shifts without involving the concepts of “dark energy” and “dark matter”. It is shown that due to the smallness of the cosmological rotation, for its detection one should use observations that do not depend on the magnitude of the angular velocity of the Universe. Such tests include the effects of the cosmic mirror and the cosmic lens. For the first time on the basis of modern electronic catalogs the search on the celestial sphere of images of our Galaxy and other galaxies is made. Viable candidates for both effects have been found. View Full-Text
Keywords: cosmology; cosmological effects; rotation of the Universe cosmology; cosmological effects; rotation of the Universe
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MDPI and ACS Style

Korotky, V.A.; Masár, E.; Obukhov, Y.N. In the Quest for Cosmic Rotation. Universe 2020, 6, 14.

AMA Style

Korotky VA, Masár E, Obukhov YN. In the Quest for Cosmic Rotation. Universe. 2020; 6(1):14.

Chicago/Turabian Style

Korotky, Vladimir A.; Masár, Eduard; Obukhov, Yuri N. 2020. "In the Quest for Cosmic Rotation" Universe 6, no. 1: 14.

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