A relativistic model of the topological acceleration effect
arXiv:1109.1596 · doi:10.1088/0264-9381/29/16/165006
Abstract
It has previously been shown heuristically that the topology of the Universe affects gravity, in the sense that a test particle near a massive object in a multiply connected universe is subject to a topologically induced acceleration that opposes the local attraction to the massive object. This effect distinguishes different comoving 3-manifolds, potentially providing a theoretical justification for the Poincaré dodecahedral space observational hypothesis and a dynamical test for cosmic topology. It is necessary to check if this effect occurs in a fully relativistic solution of the Einstein equations that has a multiply connected spatial section. A Schwarzschild-like exact solution that is multiply connected in one spatial direction is checked for analytical and numerical consistency with the heuristic result. The T (slab space) heuristic result is found to be relativistically correct. For a fundamental domain size of , a slow-moving, negligible-mass test particle lying at distance along the axis from the object of mass to its nearest multiple image, where , has a residual acceleration away from the massive object of , where is Apéry's constant. For and to $20\hGpc$, this linear expression is accurate to over $3\hMpc \ltapprox x \ltapprox 2\hGpc$. Thus, at least in a simple example of a multiply connected universe, the topological acceleration effect is not an artefact of Newtonian-like reasoning, and its linear derivation is accurate over about three orders of magnitude in .
12 pages, 2 figures, 1 table; v3: N-body simulation discussion removed, references added, minor errors corrected
References in corpus (6)
- Multiscale cosmology and structure-emerging Dark Energy: A plausibility analysis
- A weak acceleration effect due to residual gravity in a multiply connected universe
- Observational constraints on modified gravity models and the Poincaré dodecahedral topology
- The size of the Universe according to the Poincare dodecahedral space hypothesis
- Cosmic Topology: a Brief Overview
- Cosmological Parameters and Cosmic Topology