Research
Bianchi Type-VI0 Dark Energy Cosmological Models in General Relativity
Bianchi type-VI0 cosmological models of the universe filled with dark energy with constant and time-dependent equation of state parameters are investigated in general relativity. We obtain exact solutions of EinsteinΓ’β¬β’s field equations using the condition that the shear scalar is proportional to the expansion scalar, which represent singular and non-singular cosmological models of the universe. The physical behavior of the models are discussed. We conclude that the universe models do not approach isotropy through the evolution of the universe.
