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

Abstract

Abstract 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 $$n_s$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>n</mml:mi> <mml:mi>s</mml:mi> </mml:msub> </mml:math> are in good agreement with results from Planck-2018 TT+TE+EE+lowE data for the model parameter $$n &gt; 2$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>n</mml:mi> <mml:mo>&gt;</mml:mo> <mml:mn>2</mml:mn> </mml:mrow> </mml:math> .