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Lyapunov function for cosmological dynamical system

Lyapunov function for cosmological dynamical system AbstractWe prove the asymptotic global stability of the de Sitter solution in the Friedmann-Robertson-Walker conservative and dissipative cosmology. In the proof we construct a Lyapunov function in an exact form and establish its relationship with the first integral of dynamical system determining evolution of the flat Universe. Our result is that de-Sitter solution is asymptotically stable solution for general form of equation of state p = (ρ, H), where dependence on the Hubble function H means that the effect of dissipation are included. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Demonstratio Mathematica de Gruyter

Lyapunov function for cosmological dynamical system

Demonstratio Mathematica , Volume 50 (1): 5 – Apr 25, 2017

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Publisher
de Gruyter
Copyright
© 2017 Marek Szydłowski and Adam Krawiec
ISSN
0420-1213
eISSN
2391-4661
DOI
10.1515/dema-2017-0005
Publisher site
See Article on Publisher Site

Abstract

AbstractWe prove the asymptotic global stability of the de Sitter solution in the Friedmann-Robertson-Walker conservative and dissipative cosmology. In the proof we construct a Lyapunov function in an exact form and establish its relationship with the first integral of dynamical system determining evolution of the flat Universe. Our result is that de-Sitter solution is asymptotically stable solution for general form of equation of state p = (ρ, H), where dependence on the Hubble function H means that the effect of dissipation are included.

Journal

Demonstratio Mathematicade Gruyter

Published: Apr 25, 2017

References