Cylindrically Symmetric Inhomogeneous Universes with a Cloud of Strings

Abstract

Cylindrically symmetric inhomogeneous string cosmological models are investigated in presence of string fluid as a source of matter. To get the three types of exact solutions of Einstein's field equations we assume $A=f(x)k(t)$, $B=g(x)\ell (t)$ and $C=h(x)\ell (t)$. Some physical and geometric aspects of the models are discussed.

9 pages

References in corpus (5)

• String cosmology in Bianchi I space-time
• Bianchi Type III String Cosmological Models with Time Dependent Bulk Viscosity
• Some Bianchi Type III String Cosmological Models with Bulk Viscosity
• Bianchi Type I Massive String Magnetized Barotropic Perfect Fluid Cosmological Model in General Relativity
• Higher Dimensional Strange Quark Matter Coupled to the String Cloud with Electromagnetic Field Admitting One Parameter Group of Conformal Motion

Cited by in corpus (10)

• Effects of a cloud of strings on the extended phase space of Einstein-Gauss-Bonnet AdS black holes
• The emergence of universal relations in the AdS black holes thermodynamics
• Bianchi-V string cosmological model and late time acceleration
• Invariant Bianchi type I models in $f\left(R,T\right)$ Gravity
• Anisotropic String Cosmological Models in Heckmann-Suchuking Space-Time
• Cloud of strings in f(R) gravity
• Does a Cloud of Strings Affect Shear Viscosity Bound?
• An optimal system and invariant solutions of dark energy Models in cylindrically symmetric space-time
• Some Invariant String Cosmological Models in Cylindrically Symmetric Space-time
• The Effect of Bulk Dimension in the presence of String Cloud on Viscosity Bound