Integrable cosmological models with an additional scalar field
Abstract We consider modified gravity cosmological models that can be transformed into two-field chiral cosmological models by the conformal metric transformation. For the $$R^2$$ R 2 gravity model with an additional scalar field and the corresponding two-field model with the cosmological constant a...
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2021
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oai:doaj.org-article:38e32076e6404e07af7e2addcf1acb4c2021-11-14T12:13:52ZIntegrable cosmological models with an additional scalar field10.1140/epjc/s10052-021-09792-41434-60441434-6052https://doaj.org/article/38e32076e6404e07af7e2addcf1acb4c2021-11-01T00:00:00Zhttps://doi.org/10.1140/epjc/s10052-021-09792-4https://doaj.org/toc/1434-6044https://doaj.org/toc/1434-6052Abstract We consider modified gravity cosmological models that can be transformed into two-field chiral cosmological models by the conformal metric transformation. For the $$R^2$$ R 2 gravity model with an additional scalar field and the corresponding two-field model with the cosmological constant and nonstandard kinetic part of the action, the general solutions have been obtained in the spatially flat FLRW metric. We analyze the correspondence of the cosmic time solutions obtained and different possible evolutions of the Hubble parameters in the Einstein and Jordan frames.Vsevolod R. IvanovSergey Yu. VernovSpringerOpenarticleAstrophysicsQB460-466Nuclear and particle physics. Atomic energy. RadioactivityQC770-798ENEuropean Physical Journal C: Particles and Fields, Vol 81, Iss 11, Pp 1-11 (2021) |
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Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 |
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Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 Vsevolod R. Ivanov Sergey Yu. Vernov Integrable cosmological models with an additional scalar field |
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Abstract We consider modified gravity cosmological models that can be transformed into two-field chiral cosmological models by the conformal metric transformation. For the $$R^2$$ R 2 gravity model with an additional scalar field and the corresponding two-field model with the cosmological constant and nonstandard kinetic part of the action, the general solutions have been obtained in the spatially flat FLRW metric. We analyze the correspondence of the cosmic time solutions obtained and different possible evolutions of the Hubble parameters in the Einstein and Jordan frames. |
format |
article |
author |
Vsevolod R. Ivanov Sergey Yu. Vernov |
author_facet |
Vsevolod R. Ivanov Sergey Yu. Vernov |
author_sort |
Vsevolod R. Ivanov |
title |
Integrable cosmological models with an additional scalar field |
title_short |
Integrable cosmological models with an additional scalar field |
title_full |
Integrable cosmological models with an additional scalar field |
title_fullStr |
Integrable cosmological models with an additional scalar field |
title_full_unstemmed |
Integrable cosmological models with an additional scalar field |
title_sort |
integrable cosmological models with an additional scalar field |
publisher |
SpringerOpen |
publishDate |
2021 |
url |
https://doaj.org/article/38e32076e6404e07af7e2addcf1acb4c |
work_keys_str_mv |
AT vsevolodrivanov integrablecosmologicalmodelswithanadditionalscalarfield AT sergeyyuvernov integrablecosmologicalmodelswithanadditionalscalarfield |
_version_ |
1718429340248571904 |