Unified solutions of energy-momentum-squared gravity
In this study, we realize a unified solution of F(R, T 2) gravity in the context of the spatially flat Friedmann-Robertson-Walker universe, where R is the Ricci curvature scalar and T2 = Tμν Tμν is the scalar constructed from the square of the energy-momentum tensor. We observe that these solutions...
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Format: | Tagungsbericht |
Sprache: | eng |
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Online-Zugang: | Volltext |
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Zusammenfassung: | In this study, we realize a unified solution of F(R, T 2) gravity in the context of the spatially flat Friedmann-Robertson-Walker universe, where R is the Ricci curvature scalar and T2 = Tμν Tμν is the scalar constructed from the square of the energy-momentum tensor. We observe that these solutions describe a transition from deceleration eras of the universe to late-time quintessential dark energy in a unified form. |
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ISSN: | 0094-243X 1551-7616 |
DOI: | 10.1063/1.5078923 |