文摘
In this paper, based on the BSBM theory, we investigate the dynamics of a homogeneous and anisotropic Bianchi type-V (BV) cosmological model subject to variation of the fine structure constant. By performing stability analysis, the anisotropic cosmic attractors are obtained and the anisotropic parameters are studied. The outcome confirms that universe underwent both anisotropy and variation of fine structure constant in the past for an accelerating expansion. However, the result also shows that both anisotropy and fundamental constant variation exist at the present epoch and even become greater in the future. This is in contradiction with the current observational data and therefore the model is not satisfactory.