Abstract:We have studied the spatially homogeneous and anisotropic Locally Rotationally Symmetric (LRS) Bianchi type-I universe in F(T) theory of gravity. By using a conservation equation, we have discussed some well known F(T) models. It is interesting to observe that these F(T) gravity models represent the different phases (matter, radiation and dark energy eras) of the universe. An attempt has been made to retain Sharif and Rani's [1] forms of the various quantities. Our results are analogous to the results obtained by Sharif and Rani [1].
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