An extended theory of gravity in a modified Riemann’s geometry
Abstract
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 as a complex vectorial function depending on a dynamical scalar field . By using the latest observational data, we observe that for the universe starts accelerating at the critical scale factor which corresponds to a redshift of . We also find that the dark energy fluid considered in this model is a generalized fluid with equation of state .
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