Abstract
We study the mixing properties of compact k = −1 FLRW models, as a function of the cosmological parameters and the topological compactification scale. We find the mixing to be less pronounced than some of the claims made previously, nevertheless in low density universes the mechanism can give rise to appreciable mixing and result in a reduction in the measured cmwbr anisotropy on a range of angular scales. These models also have other important features, namely: (i) they allow chaos to be expressed in a gauge invariant way; (ii) they are structurally stable and (iii) in low density universes they result in radically different estimates of length scales with potentially important consequences for the interpretation of the angular variation of the background radiation.
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Ellis, G., Tavakol, R. (1994). Mixing Properties of Compact K = −1 FLRW Models. In: Hobill, D., Burd, A., Coley, A. (eds) Deterministic Chaos in General Relativity. NATO ASI Series, vol 332. Springer, Boston, MA. https://doi.org/10.1007/978-1-4757-9993-4_13
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DOI: https://doi.org/10.1007/978-1-4757-9993-4_13
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