Dynamics of anisotropic universe in f(G) gravity

The main objective of this paper is to investigate anisotropic universe in f(G) gravity. Locally rotationally symmetric Bianchi type I cosmological model is considered for this purpose. First, some exact solutions with a well-known form of f (G) model are explored. In particular, two solutions are reported for the analysis. Secondly, we discuss the energy conditions for the model under consideration. The viability of the model is investigated via graphical analysis using the present day values of cosmological parameters. The strong energy condition is violated which shows that anisotropic universe in f (G) gravity supports the phenomenon of expansion of universe.