Reconstruction of f(R) Gravity from Cosmological Unified Dark Fluid Model

In this work, we reconstruct the cosmological unified dark fluid model proposed previously by Elkhateeb (Astrophys Space Sci 363(1):7, 2018) in the framework of f ( R ) gravity. Utilizing the equivalence between the scalar-tensor theory and the f ( R ) gravity theory, the scalar field for the dark f...

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Bibliographic Details
Published in:Foundations of physics 2024-02, Vol.54 (1), Article 18
Main Author: Elkhateeb, Esraa Ali
Format: Article
Language:English
Subjects:
Classical and Quantum Gravitation
Classical Mechanics
History and Philosophical Foundations of Physics
Mathematical models
Parameters
Philosophy of Science
Physics
Physics and Astronomy
Quantum Physics
Relativity Theory
Scalars
Statistical Physics and Dynamical Systems
Tensors
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Summary:In this work, we reconstruct the cosmological unified dark fluid model proposed previously by Elkhateeb (Astrophys Space Sci 363(1):7, 2018) in the framework of f ( R ) gravity. Utilizing the equivalence between the scalar-tensor theory and the f ( R ) gravity theory, the scalar field for the dark fluid is obtained, whence the f ( R ) function is extracted and its viability is discussed. The f ( R ) functions and the scalar field potentials have then been extracted in the early and late times of asymptotically de Sitter spacetime. The ability of our function to describe early time inflation is also tested. The early time scalar field potential is used to derive the slow roll inflation parameters. Our results of the tensor-to-scalar ratio r and the scalar spectral index n s are in good agreement with results from Planck-2018 TT+TE+EE+lowE data for the model parameter n > 2 .
ISSN:0015-9018
1572-9516
DOI:10.1007/s10701-023-00751-5