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On physical foundations and observational effects of cosmic rotation

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arxiv astro-ph/0008106 v1 pith:OFDHRUV2 submitted 2000-08-07 astro-ph gr-qc

Yuri N. Obukhov This is my paper · ORCID
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keywords rotationcosmiceffectsmodelsobservationalattentioncosmologicaldescribed
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An overview of the cosmological models with expansion, shear and rotation is presented. Problems of the rotating models are discussed, their general kinematic properties and dynamical realizations are described. A particular attention is paid to the discussion of possible observational effects which could be used to estimate or to put limits on the cosmic rotation.

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Cited by 1 Pith paper

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  1. Simulating Rotating Newtonian Universes

    astro-ph.CO 2024-11 conditional novelty 6.0 of 10

    First 3D N-body simulations of a rotating, shear-free Newtonian universe show more than 1% anisotropy between polar and equatorial expansion rates at maximal allowed rotation.

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