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Structural stability properties of friedman cosmology

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Abstract

A dynamical system with Robertson-Walker symmetries and the equation of the statep=γ∈, 0≤γ≤1, considered both as a conservative and nonconservative system, is studied with respect to its structural stability properties. Different cases are shown and analyzed on the phase space (x=R D, y=x).

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Authors and Affiliations

  1. Faculty of Philosophy, Vatican Astronomical Observatory, Vatican City State Pontificial Academy of Cracow, ul. Augustiańska 7, 31-064, Krakow, Poland

    Marek Szydlowski & Michael Heller

  2. N. Copernicus Astronomical Centre, Polish Academy of Sciences, ul. Orla 171, 30-244, Kraków, Poland

    Zdzislaw Golda

Authors
  1. Marek Szydlowski
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  2. Michael Heller
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  3. Zdzislaw Golda
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Szydlowski, M., Heller, M. & Golda, Z. Structural stability properties of friedman cosmology. Gen Relat Gravit 16, 877–890 (1984). https://doi.org/10.1007/BF00762940

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  • DOI: https://doi.org/10.1007/BF00762940

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