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Abstract
Friedmann—Lemaître cosmology is briefly reviewed in terms of dynamical systems. It is demonstrated that in certain cases bulk viscosity dissipation structurally stabilizes Friedmann—Lemaître solutions. It turns out that, for A=0, there are structurally stable solutions if ξ~ε1/2, where ξ is the bulk viscosity coefficient. For A≠0 structurally stable solutions are essentially those with ξ=const. The role of structural stability in physics and cosmology is shortly discussed.
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Golda, Z., Heller, M. & Szydlowski, M. Structurally stable approximations to Friedmann—Lemaître world models. Astrophys Space Sci 90, 313–326 (1983). https://doi.org/10.1007/BF00650065
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DOI: https://doi.org/10.1007/BF00650065