KOPTĚVA, Olena, Iryna BORMOTOVA, Maria CHURILOVA and Zdeněk STUCHLÍK. Accelerated Expansion of the Universe in the Model with Nonuniform Pressure. Astrophysical Journal. Institute of Physics Publishing, 2019, vol. 887, No 1, p. "98-1"-"98-9", 9 pp. ISSN 0004-637X. Available from: https://dx.doi.org/10.3847/1538-4357/ab4f7f.
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Basic information
Original name Accelerated Expansion of the Universe in the Model with Nonuniform Pressure
Authors KOPTĚVA, Olena (804 Ukraine, guarantor, belonging to the institution), Iryna BORMOTOVA (804 Ukraine, belonging to the institution), Maria CHURILOVA (804 Ukraine, belonging to the institution) and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution).
Edition Astrophysical Journal, Institute of Physics Publishing, 2019, 0004-637X.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher United Kingdom of Great Britain and Northern Ireland
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19240/19:A0000410
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.3847/1538-4357/ab4f7f
UT WoS 000506001500098
Keywords in English cosmology; expanding universe; cosmological models; accelerating universe; Einstein field equations
Tags , GB14-37086G, RCTPA, RIVOK, SGS12-2019
Tags International impact, Reviewed
Links GB14-37086G, research and development project.
Changed by Changed by: Ing. Petra Skoumalová, učo 50554. Changed: 21/4/2020 10:26.
Abstract
We present the particular case of the Stephani solution for shear-free perfect fluid with uniform energy density and nonuniform pressure. Such models appeared as possible alternative to the consideration of the exotic forms of matter like dark energy that would cause the acceleration of universe expansion. These models are characterized by the spatial curvature, depending on time. We analyze the properties of the cosmological model obtained on the basis of exact solution of the Stephani class, and adapt it to the recent observational data. The spatial geometry of the model is investigated. We show that despite possible singularities, the model can describe the current stage of the universe's evolution.
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