Monotonic functions in Bianchi models: Why they exist and how to find them
arXiv:0907.0653 · doi:10.1088/0264-9381/27/1/015009
Abstract
All rigorous and detailed dynamical results in Bianchi cosmology rest upon the existence of a hierarchical structure of conserved quantities and monotonic functions. In this paper we uncover the underlying general mechanism and derive this hierarchical structure from the scale-automorphism group for an illustrative example, vacuum and diagonal class A perfect fluid models. First, kinematically, the scale-automorphism group leads to a reduced dynamical system that consists of a hierarchy of scale-automorphism invariant sets. Second, we show that, dynamically, the scale-automorphism group results in scale-automorphism invariant monotone functions and conserved quantities that restrict the flow of the reduced dynamical system.
26 pages, replaced to match published version
References in corpus (3)
Cited by in corpus (10)
- Revisiting Fractional Cosmology
- Extended phase-space analysis of the Horava-Lifshitz cosmology
- Recent developments concerning generic spacelike singularities
- Scalar field deformations of Lambda-CDM cosmology
- Time-averaging axion-like interacting scalar fields models
- Spacetime Singularities: Recent Developments
- Averaging Generalized Scalar Field Cosmologies I: Locally Rotationally Symmetric Bianchi III and open Friedmann-Lemaître-Robertson-Walker models
- Future asymptotics of tilted Bianchi type II cosmologies
- Averaging Generalized Scalar Field Cosmologies II: Locally Rotationally Symmetric Bianchi I and flat Friedmann-Lemaître-Robertson-Walker models
- Cosmological global dynamical systems analysis