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Structurally stable approximations to Friedmann—Lemaître world models

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“Briser les contraintes de l'espace-temps, tel est le but ultime de l'homme: exploiter tous les modes d'action non locale qui peuvent être aisément contrôlés, c'est ce qu'exige l'humanité...” René Thom,Penser les mathématiques

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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