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Friedmann Dynamics Recovered from Compactified Einstein–Gauss–Bonnet Cosmology

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Abstract

Cosmological dynamics is studied in Einstein–Gauss–Bonnet gravity with a perfect fluid source in arbitrary dimension. A systematic analysis is performed for the case that the theory does not admit maximally symmetric solutions. Considering two independent scale factors, namely, one for the 3D space and one for the extra-dimensional space, it is found that a regime exists where the scale factor of extra dimensions tends to a constant value via damped oscillations for not too negative pressure of the fluid, so that asymptotically the evolution of the (3 + 1)-dimensional Friedmann model with perfect fluid is recovered.

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Authors and Affiliations

  1. Centro de Estudios Cientificos (CECs), Casilla, 1469, Valdivia, Chile

    F. Canfora

  2. Instituto de Ciencias Físicas y Matemáticas, Universidad Austral de Chile, Valdivia, Chile

    A. Giacomini

  3. Programa de Pós-Graduaзão em Física, Universidade Federal do Maranhão (UFMA), 65085-580, São Luís, Maranhão, Brazil

    S. A. Pavluchenko

  4. Sternberg Astronomical Institute, Moscow State University, Moscow, 119991, Russia

    A. Toporensky

  5. Kazan Federal University, Kazan, 420008, Russia

    A. Toporensky

Authors
  1. F. Canfora
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  2. A. Giacomini
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  3. S. A. Pavluchenko
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  4. A. Toporensky
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Correspondence to F. Canfora.

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Canfora, F., Giacomini, A., Pavluchenko, S.A. et al. Friedmann Dynamics Recovered from Compactified Einstein–Gauss–Bonnet Cosmology. Gravit. Cosmol. 24, 28–38 (2018). https://doi.org/10.1134/S0202289318010048

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  • DOI: https://doi.org/10.1134/S0202289318010048

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