Bianchi Type V String Cosmological Models in General Relativity
arXiv:0912.0464 · doi:10.1007/s12043-011-0061-z
Abstract
Bianchi type V string cosmological models in general relativity are investigated. To get the exact solution of Einstein's field equations, we have taken some scale transformations followed by Camci (2001). It is shown that Einstein's field equations are solvable for any arbitrary cosmic scale function. Solution for particular form of cosmic scale functions are also obtained. Some physical and geometrical aspects of the models are discussed.
12 pages, Accepted version in Pramana - J. Physics
References in corpus (6)
- String cosmology in Bianchi I space-time
- Strange Quark Matter Attached to the String Cloud in the Spherical Symmetric Space-Time Admitting Conformal Motion
- Some Bianchi Type III String Cosmological Models with Bulk Viscosity
- Cylindrically Symmetric Inhomogeneous Universes with a Cloud of Strings
- Generation of Bianchi type V cosmological models with varying -term
- A New Class of Inhomogeneous String Cosmological Models in General Relativity
Cited by in corpus (5)
- Bianchi-V string cosmological model and late time acceleration
- Anisotropic String Cosmological Models in Heckmann-Suchuking Space-Time
- Anisotropic bulk viscous string cosmological models of the Universe under a time-dependent deceleration parameter
- Anisotropic massive strings in scalar-tensor theory of gravitation
- Some LRS Bianchi-I String Cosmological Models with Variable Deceleration Parameter