Abstract
We study how the uncertainty in the cosmological parameters impacts on the detection of topological signals, focussing on three cubic torus universes and using three tests: the information content, the statistic, and the Bayesian evidence. We find, within the concordance cosmological model, that 3D torus universes with a size of or larger cannot be detected. For the toroidal models that can be detected, the detection significance is primarily influenced by , which enters both in the noise amplitude due to the Integrated Sachs-Wolfe effect and in the size of the causal horizon which limits the accessible fundamental domain. On large angular scales , only significantly alters the detection for all three estimators considered here.
2 More- Received 7 May 2007
DOI:https://doi.org/10.1103/PhysRevD.77.023525
©2008 American Physical Society