Abstract
The main objective of this manuscript is to study the anisotropic universe in \(f(G)\) Gravity. For this purpose, locally rotationally symmetric Bianchi type \(I\) spacetime is considered. A viable \(f(G)\) model is used to explore the exact solutions of modified field equations. In particular, two families involving power law and exponential type solutions have been discussed. Some important cosmological parameters are calculated for the obtained solutions. Moreover, energy density and pressure of the universe is analyzed for the model under consideration.
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