Lyapunov function for cosmological dynamical system
We 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...
Saved in:
Published in | Demonstratio mathematica Vol. 50; no. 1; pp. 51 - 55 |
---|---|
Main Authors | , |
Format | Journal Article |
Language | English |
Published |
De Gruyter Open
01.04.2017
De Gruyter |
Subjects | |
Online Access | Get full text |
Cover
Loading…
Summary: | We 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. |
---|---|
ISSN: | 2391-4661 2391-4661 |
DOI: | 10.1515/dema-2017-0005 |