• SOME LRS BIANCHI TYPE II STRING COSMOLOGICAL MODELS FOR VISCOUS FLUID DISTRIBUTION IN GENERAL RELATIVITY

Abstract

Some LRS Bianchi type II string cosmological models are discussed. We have assumed the condition, here is the energy density, is the string tension density and is a constant. We have also used a condition that, The scalar expansion is proportional to the shear, to get determinate solution in terms of cosmic time t. The physical and geometrical aspects of the models are also discussed.