Abstract
In this paper, LRS Bianchi type I string fluid cosmological model with magnetic field in bimetric theory of gravitation is investigated by assuming barotropic equation of state for pressure and density and assuming the bulk viscosity to be inversely proportional to the scalar expansion. The source of energy momentum tensor is a bulk viscous fluid containing one dimensional string with electromagnetic field. The physical and geometrical properties of the model are discussed. The bulk viscosity affected the whole properties of the model.
Recommended Citation
Borkar, M. S. and Gaikwad, N. P.
(2014).
String Fluid Cosmological Model with Magnetic Field in Bimetric Theory of Gravitation,
Applications and Applied Mathematics: An International Journal (AAM), Vol. 9,
Iss.
1, Article 15.
Available at:
https://digitalcommons.pvamu.edu/aam/vol9/iss1/15