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Dynamics of the universe with global rotation

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Abstract

We analyze the dynamics of the FRW models with global rotation in terms of dynamical system methods. We reduce the dynamics of these models to the FRW models with some fictitious fluid which scales like radiation matter. This fluid mimics dynamical effects of global rotation. The significance of the global rotation of the Universe for the resolution of the acceleration and horizon problems in cosmology is investigated. It is found that the dynamics of the Universe can be reduced to the two-dimensional Hamiltonian dynamical system. Then the construction of the Hamiltonian allows for full classification of evolution paths. On the phase portraits we find the domains of cosmic acceleration for the globally rotating universe as well as the trajectories for which the horizon problem is solved. We show that the FRW models with global rotation are structurally stable. This proves that the universe acceleration is due to the global rotation. It is also shown how global rotation gives a natural explanation of the empirical relation between angular momentum for clusters and superclusters of galaxies. The relation J ~ M2 is obtained as a consequence of self similarity invariance of the dynamics of the FRW model with global rotation. In derivation of this relation we use the Lie group of symmetry analysis of differential equation.

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Authors and Affiliations

  1. Astronomical Observatory, Jagiellonian University, Orla 171, 30-244, Kraków, Poland

    Marek Szydłowski & Włodzimierz Godłowski

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  1. Marek Szydłowski
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  2. Włodzimierz Godłowski
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Correspondence to Marek Szydłowski.

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Szydłowski, M., Godłowski, W. Dynamics of the universe with global rotation. Gen Relativ Gravit 37, 907–936 (2005). https://doi.org/10.1007/s10714-005-0075-2

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