Chaos in cosmology

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Abstract

We consider open cosmological models with multiply connected spacelike slices. In these universes there is a finite, convex region in which the world lines turn chaotic. We point out some physical effects of the topology in wave fields, like particle creation-annihilation, violation of the space-reflection symmetry, and fluctuations in the temperature of the microwave background. The evolution of classical and quantum mechanical probability densities under the mixing horospherical flow is discussed.

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Tomaschitz, R. (1994). Chaos in cosmology. IFIP Transactions A: Computer Science and Technology (pp. 431–439). Publ by Elsevier Science Publishers B.V. https://doi.org/10.1007/978-94-010-0997-3_7

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