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An extended theory of gravity in a modified Riemann’s geometry

    https://doi.org/10.1142/S0219887819500671Cited by:4 (Source: Crossref)

    In this work, we study the evolution of an isotropic universe in an extended theory of gravity obtained geometrically by transforming the normal-gauge Lyra displacement vector field ϕμ as a complex vectorial function depending on a dynamical scalar field φ. By using the latest observational data, we observe that for ω0=0.98 the universe starts accelerating at the critical scale factor aac=0.626 which corresponds to a redshift of zac0.6. We also find that the dark energy fluid considered in this model is a generalized fluid with equation of state p=ρ+F(ρ,a).

    PACS: 98.80.Jk, 98.80.−k, 95.36.+x, 04.50.Kd, 02.40.Ky

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