MAGNETIZED BIANCHI TYPE-III STRING COSMOLOGICAL MODEL FOR ANTI-STIFF FLUID IN GENERAL RELATIVITY

In this paper, we have explored magnetized Bianchi type-III string cosmological model for anti-stiff fluid in general relativity. Anti-stiff fluid models create more interest in the study because these models are free from initial singularity. We assume that F-12 is the only nonzero component of electromagnetic field tensor F-ij. For the complete determination of the model, we assume the expansion in the model is proportional to the shear. The general solution of the Einstein's field equations for the cosmological model have been obtained under the assumption of anti-stiff fluid i.e. p + rho = 0, where rho and p are the rest energy density and the pressure of the fluid, respectively. The physical and geometrical consequences of the model in the presence of magnetic field are discussed.