S. P. Kandalkar , A. P. Wasnik, M. N.Gaikwad
Some locally rotationally symmetric (LRS) Bianchi type I cosmological model of universe filled with dark energy from a wet dark fluid in the presence and absence of magnetic field is in investigated in general theory of relativity . We assume F23 is non vanishing component of Fij. We obtain exact solutions to the field equation, where a relation between metric potential ð? = ð??ð?? is considered. The geometrical and kinematical properties of the models and the behaviours of the anisotropy of the dark energy have been carried out.