Dynamics of inhomogeneities of metric in the vicinity of a singularity in multidimensional cosmology authors
arXiv:gr-qc/9408004 · doi:10.1103/PhysRevD.52.723
Abstract
The problem of construction of a general ihomogeneous solution of -dimensional Einstein equations in the vicinity of a cosmological singularity is considered. It is shown that near the singularity a local behavior of metric functions is described by a billiard on a space of a constant negative curvature. The billiard is shown to have a finite volume and consequently to be a mixing one. Dynamics of inhomogeneities of metric is studied and it is shown that its statistical properties admit a complete description. An invariant measure describing statistics of inhomogeneities is obtained and a role of a minimally-coupled scalar field in dynamics of the inhomogeneities is also considered.
9 pages. 1 figure available by request
References in corpus (1)
Cited by in corpus (17)
- Hyperbolic Kac-Moody Algebras and Chaos in Kaluza-Klein Models
- Spacelike Singularities and Hidden Symmetries of Gravity
- Classical and Quantum Features of the Mixmaster Singularity
- Describing general cosmological singularities in Iwasawa variables
- Quasi-Isotropization of the Inhomogeneous Mixmaster Universe Induced by an Inflationary Process
- Geometric Configurations, Regular Subalgebras of E10 and M-Theory Cosmology
- Singularity-free and non-chaotic inhomogeneous Mixmaster in polymer representation for the volume of the universe
- Cosmological wormholes
- Five-dimensional Supergravity and Hyperbolic Kac-Moody Algebra G2H
- Arithmetic and Hyperbolic Structures in String Theory
- On avoiding cosmological oscillating behavior for S-brane solutions with diagonal metrics
- Billiard representation for multidimensional multi-scalar cosmological model with exponential potentials
- Kac-Moody Algebras in M-theory
- Kasner-like behaviour for subcritical Einstein-matter systems
- A Scenario for the Dimensional Compactification in Eleven-Dimensional Space-Time
- Billiard representation for pseudo-Euclidean Toda-like systems of cosmological origin
- Integrability of anisotropic and homogeneous Universes in scalar-tensor theory of gravitation