On spatial volume averaging in Lema\^ıtre--Tolman--Bondi dust models. Part I: back reaction, spacial curvature and binding energy
arXiv:0807.1145
Abstract
We provide a comprehensive analytic study (rigorous and qualitative) of the conditions for the existence of a a positive kinematic back reaction term $\QQ>0$, in the context of Buchert's scalar averaging formalism applied to spherically symmetric Lemaître-Tolman-Bondi (LTB) dust solutions in which averaging domains are given as spherical comoving regions containing a symmetry center. We introduce proper volume and quasi-local average functionals and functions in order to examine the conditions for $\QQ\geq 0$, and in the process we also explore the relation between back reaction, spatial curvature and binding energy for a wide variety of LTB configurations. The back reaction term is positive for all "hyperbolic" regular domains with negative spatial curvature, either in the full radial range or in the radial asymptotic range. This result is also valid if these domains contain an inner "elliptic" region with positive curvature undergoing local collapse. For some cases in which positive spatial curvature decreases asymptotically, the conditions for a positive back reaction can still be met but seem to be more restrictive. Since $\QQ>0$ is a necessary condition for a positive "effective" acceleration that would mimic the effect of dark energy (in the context of Buchert's formalism), we examine this issue in LTB models in a follow up paper (part II).
This replacement corrects an important error of the previous version. The paper (part I) now deals only with back--reaction, spatial curvature and other issues, leaving "effective acceleration" for a follow up article (part II). No further modifications will be made. 40 pages in IOP LaTeX format
References in corpus (7)
- The effect of inhomogeneous expansion on the supernova observations
- Testing backreaction effects with observations
- Can inhomogeneties accelerate the cosmic volume expansion?
- Apparent and average acceleration of the Universe
- Accelerated expansion without dark energy
- The Accelerated Expansion of the Universe Challenged by an Effect of the Inhomogeneities. A Review
- Quasi-local variables, non-linear perturbations and back-reaction in spherically symmetric spacetimes
Cited by in corpus (14)
- Testing backreaction effects with observations
- What is dust? - Physical foundations of the averaging problem in cosmology
- A novel approach to the dynamics of Szekeres dust models
- Back-reaction and effective acceleration in generic LTB dust models
- Apparent and average acceleration of the Universe
- Gravitational entropies in LTB dust models
- Radial asymptotics of Lemaitre-Tolman-Bondi dust models
- Invariant characterization of the growing and decaying density modes in LTB dust models
- The Averaging Problem in Cosmology
- On the role of shear in cosmological averaging II: large voids, non-empty voids and a network of different voids
- Cosmic bulk viscosity through backreaction
- Averaged Lemaître-Tolman-Bondi dynamics
- Gravitational energy as dark energy: Cosmic structure and apparent acceleration
- A new approach for doing theoretical and numeric work with Lemaitre-Tolman-Bondi dust models