This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy.

Some Magnetized Bulk Viscous String Cosmological Models in Cylindrically Symmetric Inhomogeneous Universe with Variable Λ-Term

2009 Chinese Physical Society and IOP Publishing Ltd
, , Citation Anirudh Pradhan 2009 Commun. Theor. Phys. 51 367 DOI 10.1088/0253-6102/51/2/36

0253-6102/51/2/367

Abstract

Some cylindrically symmetric inhomogeneous viscous fluid string cosmological models with magnetic field and cosmological term Λ varying with time are investigated. To get the deterministic solution, it has been assumed that the expansion (θ) in the model is proportional to the eigen value σ11 of the shear tensor σji. The value of cosmological constant for the model is found to be small and positive, which is supported by the results from recent supernovae Ia observations. The effect of bulk viscosity is to produce a change in perfect fluid and hence exhibits essential influence on the character of the solution. The physical and geometric properties of the models are also discussed in presence and absence of magnetic field.

Export citation and abstract BibTeX RIS

10.1088/0253-6102/51/2/36