The nonlinear future stability of the FLRW family of solutions to the irrotational Euler–Einstein system with a positive cosmological constant
Journal of the European Mathematical Society, Tome 15 (2013) no. 6, pp. 2369-2462.

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In this article, we study small perturbations of the family of Friedmann-Lemaître-Robertson-Walker cosmological background solutions to the coupled Euler-Einstein system with a positive cosmological constant in 1+3 spacetime dimensions. The background solutions model an initially uniform quiet fluid of positive energy density evolving in a spacetime undergoing exponentially accelerated expansion. Our nonlinear analysis shows that under the equation of state p=c2ρ,01/3, the background metric + fluid solutions are globally future-stable under small irrotational perturbations of their initial data. In particular, we prove that the perturbed spacetime solutions, which have the topological structure [0,∞)XT3, are future causally geodesically complete. Our analysis is based on a combination of energy estimates and pointwise decay estimates for quasilinear wave equations featuring dissipative inhomogeneous terms. Our main new contribution is showing that when 01/3, exponential spacetime expansion is strong enough to suppress the formation of fluid shocks. This contrasts against a well-known result of Christodoulou, who showed that in Minkowski spacetime, the corresponding constant-state irrotational fluid solutions are unstable.
DOI : 10.4171/jems/424
Classification : 35-XX, 83-XX
Keywords: cosmological constant, energy dissipation, expanding spacetime, geodesically complete, global existence, irrotational fluid, relativistic fluid, wave coordinates
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     title = {The nonlinear future stability of the {FLRW} family of solutions to the irrotational {Euler{\textendash}Einstein} system with a positive cosmological constant},
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Igor Rodnianski; Jared Speck. The nonlinear future stability of the FLRW family of solutions to the irrotational Euler–Einstein system with a positive cosmological constant. Journal of the European Mathematical Society, Tome 15 (2013) no. 6, pp. 2369-2462. doi : 10.4171/jems/424. http://geodesic.mathdoc.fr/articles/10.4171/jems/424/

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