A New Class of Inhomogeneous String Cosmological Models in General Relativity

Abstract

A new class of solutions of Einstein field equations has been investigated for inhomogeneous cylindrically symmetric space-time with string source. To get the deterministic solution, it has been assumed that the expansion ($\theta$) in the model is proportional to the eigen value ${\sigma }_1^1$ of the shear tensor ${\sigma }_j^i$. Certain physical and geometric properties of the models are also discussed.

12 pages, no figure. Submitted to Astrophys. Space Sci. arXiv admin note: substantial text overlap with arXiv:0705.0904

References in corpus (3)

• String cosmology in Bianchi I space-time
• Bianchi Type III String Cosmological Models with Time Dependent Bulk Viscosity
• Strange Quark Matter Attached to the String Cloud in the Spherical Symmetric Space-Time Admitting Conformal Motion

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