Bianchi Type V Magnetized String Dust Bulk Viscous Fluid Cosmological Model with Variable Magnetic Permeability
- First Online:
- Cite this article as:
- Bali, R. Int J Theor Phys (2009) 48: 476. doi:10.1007/s10773-008-9823-x
- 73 Downloads
Bianchi Type V magnetized string dust bulk viscous fluid cosmological model with variable magnetic permeability, is investigated. The magnetic field is due to an electric current produced along x-axis. Thus the magnetic fields is in yz-plane and F23 is the only non-vanishing component of electromagnetic field tensor Fij. To get the deterministic model in terms of cosmic time t, we have also assumed the condition ζθ=constant where ζ the coefficient of bulk viscosity and θ the expansion in the model. The behaviour of the model in presence and absence of magnetic field and bulk viscosity and singularities in the model are also discussed.