A New Type of Exact Arbitrarily Inhomogeneous Cosmology: Evolution of Deceleration in the Flat Homogeneous-On-Average Case
arXiv:1203.3652 · doi:10.1088/1475-7516/2012/01/043
Abstract
A new method for constructing exact inhomogeneous universes is presented, that allows variation in 3 dimensions. The resulting spacetime may be statistically uniform on average, or have random, non-repeating variation. The construction utilises the Darmois junction conditions to join many different component spacetime regions. In the initial simple example given, the component parts are spatially flat and uniform, but much more general combinations should be possible. Further inhomogeneity may be added via swiss cheese vacuoles and inhomogeneous metrics. This model is used to explore the proposal, that observers are located in bound, non-expanding regions, while the universe is actually in the process of becoming void dominated, and thus its average expansion rate is increasing. The model confirms qualitatively that the faster expanding components come to dominate the average, and that inhomogeneity results in average parameters which evolve differently from those of any one component, but more realistic modelling of the effect will need this construction to be generalised.
JCAP Latex, 14pp, 2 figures(2nd with 5 plots), 4 tables
Cited by in corpus (8)
- Ricci focusing, shearing, and the expansion rate in an almost homogeneous Universe
- Observations in statistically homogeneous, locally inhomogeneous cosmological toy-models without FLRW backgrounds
- Local and non-local measures of acceleration in cosmology
- Understanding the Dyer-Roeder approximation as a consequence of local cancellations of projected shear and expansion rate fluctuations
- Relativistic cosmology number densities in void-Lemaitre-Tolman-Bondi models
- Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaitre-Tolman-Bondi model
- On the intrinsically flat cosmological models in a lattice
- An effective -Szekeres modelling of the local Universe with Cosmicflows-4