Bianchi type-V String Cosmological Model with Domain Walls in the Presence of Quark Matter

Abstract

In this paper, exact solutions of Einstein field equations of Bianchi type V string cosmological model with domain wall in the presence of quark matter have been obtained by using Ù = H² + b/R². It is interesting to note that the strings in this model do not survive. Also the model does not remain anisotropic throughout the evolution of the universe. Some physical and kinematical properties of the model are also discussed.