Energy and momentum of Bianchi Type VI_h Universes
arXiv:1501.04990 · doi:10.1155/2015/705262
Abstract
We obtain the energy and momentum of the Bianchi type VI_h universes using different prescriptions for the energy-momentum complexes in the framework of general relativity. The energy and momentum of the Bianchi VI_h universe are found to be zero for the parameter h = -1 of the metric. The vanishing of these results support the conjecture of Tryon that Universe must have a zero net value for all conserved quantities.This also supports the work of Nathan Rosen with the Robertson-Walker metric. Moreover, it raises an interesting question: "Why h=-1 case is so special?"
References in corpus (13)
- Planck 2013 results. XVI. Cosmological parameters
- Planck 2013 results. I. Overview of products and scientific results
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
- Planck 2013 results. XXII. Constraints on inflation
- Planck 2013 Results. XXIV. Constraints on primordial non-Gaussianity
- Relativistic images of Schwarzschild black hole lensing
- Time delay and magnification centroid due to gravitational lensing by black holes and naked singularities
- Inflationary Universe with Anisotropic Hair
- Energy-momentum complexes in f(R) theories of gravity
- Late time Acceleration and Role of Skewness in Anisotropic models
- Bergmann-Thomson energy-momentum complex for solutions more general than the Kerr-Schild class
- Energy Contents of Some Well-Known Solutions in Teleparallel Gravity
- Energy and Momentum densities of cosmological models, with equation of state , in general relativity and teleparallel gravity
Cited by in corpus (9)
- Cosmological models with a hybrid scale factor in an extended gravity theory
- Anisotropic cosmological reconstruction in gravity
- Dynamical features of an anisotropic cosmological model
- Accelerating models with a hybrid scale factor in extended gravity
- Investigating the physical and geometrical parameters of the cosmological models with anisotropic background
- Stability, dark energy parameterization and swampland aspect of Bianchi Type- cosmological models with f(R, T)-gravity
- Localization of Energy and Momentum in an Asymptotically Reissner-Nordström Non-singular Black Hole Space-time Geometry
- The energy of the universe in the Bianchi type-II cosmological model
- Cosmological models with Big rip and Pseudo rip Scenarios in extended theory of gravity