Tracing the cosmic history by Gauss-Bonnet gravity
Ivan De Martino, Mariafelicia De Laurentis, Salvatore Capozzıello
Abstract
Cosmic history can be traced considering further curvature contributions inside the gravitational action. Assuming that standard general relativity can be extended by other curvature invariants, we discuss the possibility that an action containing higher-order curvature terms can fit, in principle, the whole universe evolution. In particular, a theory like $F(R,\mathcal{G})$, with $R$ the Ricci scalar and $\mathcal{G}$ the Gauss-Bonnet topological term, contains all the curvature invariants that, depending on the energy regime, can address inflation, and matter dominated and dark energy regimes. In this paper, we investigate this possibility considering how $F(R,\mathcal{G})$ models can lead gravity from ultraviolet to infrared scales. Specifically, we will take into account a cosmographic approach for this purpose.